tag:blogger.com,1999:blog-30382784708488394862024-03-13T20:35:58.594+05:30science & educationAnonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.comBlogger77125tag:blogger.com,1999:blog-3038278470848839486.post-67047690253326118742015-03-06T18:30:00.000+05:302015-03-06T18:30:57.666+05:30for organize medical health check up camp just call @ 7838265385<div dir="ltr" style="text-align: left;" trbidi="on">
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Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-11044118565416265392014-12-05T02:44:00.000+05:302014-12-05T02:44:54.819+05:30buy gold now or start your gold business<div dir="ltr" style="text-align: left;" trbidi="on">
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Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0Southern Asia20.96143961409685 78.75-6.7374513859031495 37.441406 48.66033061409685 120.058594tag:blogger.com,1999:blog-3038278470848839486.post-32908228158094560482014-02-07T01:20:00.000+05:302014-02-07T01:20:07.674+05:30Topological insulators could exist in six new types not seen before, theorists predict<div dir="ltr" style="text-align: left;" trbidi="on">
<a href="http://phys.org/news/2014-02-topological-insulators-theorists.html" target="_blank">Topological insulators could exist in six new types not seen before, theorists predict</a><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif; font-size: 14px;">Topological insulators—materials whose surfaces can freely conduct electrons even though their interiors are electrical insulators—have been of great interest to physicists in recent years because of unusual properties that may provide insights into quantum physics. But most analysis of such materials has had to rely on highly simplified models.</span><br />
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Now, a team of researchers at MIT has performed a more detailed analysis that hints at the existence of six new kinds of topological insulators. The work also predicts the materials' physical properties in sufficient detail that it should be possible to identify them unambiguously if they are produced in the lab, the scientists say.</div>
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The new findings are reported this week in the journal <i style="margin: 0px; padding: 0px;">Science</i> by MIT professor of physics Senthil Todadri, graduate student Chong Wang, and Andrew Potter, a former MIT graduate student who is now a postdoc at the University of California at Berkeley.</div>
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"In contrast to conventional insulators, the surface of the topological insulators harbors exotic physics that are interesting both for fundamental physics, and possibly for applications," Senthil says. But attempts to study the properties of these materials have "relied on a highly simplified model in which the electrons inside the solid are treated as though they did not interact with each other." New analytical tools applied by the MIT team now reveal "that there are six, and only six, new kinds of topological insulators that require strong electron-electron interactions."</div>
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"The surface of a three-dimensional material is two-dimensional," Senthil says—which explains why the electrical behavior of the surface of a <a class="textTag" href="http://phys.org/tags/topological+insulator/" rel="tag" style="color: #313d57; outline: 0px;">topological insulator</a> is so different from that of the interior. But, he adds, "The kind of two-dimensional physics that emerges [on these surfaces] can never be in a two-dimensional material. There has to be something inside, otherwise this <a class="textTag" href="http://phys.org/tags/physics/" rel="tag" style="color: #313d57; outline: 0px;">physics</a> will never occur. That's what's exciting about these materials," which reveal processes that don't show up in other ways.</div>
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In fact, Senthil says, this new work based on analysis of such surface phenomena shows that some previous predictions of phenomena in two-dimensional <a class="textTag" href="http://phys.org/tags/materials/" rel="tag" style="color: #313d57; outline: 0px;">materials</a> "cannot be right."</div>
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Since this is a new finding, he says, it is too soon to say what applications these new topological insulators might have. But the analysis provides details on predicted properties that should allow experimentalists to begin to understand the behavior of these exotic states of matter.</div>
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"If they exist, we know how to detect them," Senthil says of these new phases. "And we know that they can exist." What this research doesn't yet show, however, is what these new topological insulators' composition might be, or how to go about creating them.</div>
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The next step, he says, is to try to predict "what compositions might lead to" these newly predicted phases of topological insulators. "It's an open question now that we need to attack."</div>
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Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-69138235556036657422013-06-06T10:58:00.001+05:302013-06-06T10:58:27.297+05:30Download our new Android App<a href="http://www.appsgeyser.com/480919">Download our new Android App</a>: Check out our new Android App science education. Get it here <a href="http://www.appsgeyser.com/480919">http://www.appsgeyser.com/480919</a>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-29623128991469195532013-06-02T23:25:00.001+05:302013-06-02T23:25:52.768+05:30Cool Captures<a href="http://www.appsbar.com/Apps/prabhupd/436833#.UauHC-F9CTo.blogger">Cool Captures</a>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-19279988378426170242013-03-16T03:30:00.002+05:302013-03-16T03:30:35.190+05:30Cool Library <span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; line-height: 18px;"><b><span style="font-size: x-large;">Cool Library </span></b></span><br />
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http://pothi.com/pothi/book/prabhakar-prasad-waqt-ne-kahaAnonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-50594104543873182922013-03-15T14:51:00.001+05:302013-03-15T14:51:18.579+05:30Some Knowledgable Facts | Pothi.com my new book<a href="http://pothi.com/pothi/book/prabhakar-prasad-some-knowledgable-facts">Some Knowledgable Facts | Pothi.com</a><br />
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Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-78214400140991799312013-03-08T23:42:00.002+05:302013-03-08T23:42:39.008+05:30My Book in Paperwork form buy it<div class="separator" style="clear: both; text-align: center;">
<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhg9rBFajicD0O5WjtY2msHdQC1jIoI3dwJei79z1scfY8qQSXx97gPX2sJko49fcDCXDeN_ri3JP9QYNwnPH_L5TS4qIUFDoitoASrXnsh7QNv5qF5szxTttHZ0TKGTMLShu9qwiM6nx4/s1600/ttt.PNG" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhg9rBFajicD0O5WjtY2msHdQC1jIoI3dwJei79z1scfY8qQSXx97gPX2sJko49fcDCXDeN_ri3JP9QYNwnPH_L5TS4qIUFDoitoASrXnsh7QNv5qF5szxTttHZ0TKGTMLShu9qwiM6nx4/s1600/ttt.PNG" /></a></div>
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this is cover pics of my paperwork format of book...</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_ndE6mA4VvpWS-CyWFb8D0_ydfHygVnbDyfFPy-9Hrszrb0l6YMqAKmr3JJs0QPAEXuR4yKBrCFl3dt09hyphenhyphenD85sBGT7dXjO-wvAP9IzjVqIVJiMQTZYlpXO5znJ7FVSu2KF2U7WfuOaA/s1600/product_thumbnail.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_ndE6mA4VvpWS-CyWFb8D0_ydfHygVnbDyfFPy-9Hrszrb0l6YMqAKmr3JJs0QPAEXuR4yKBrCFl3dt09hyphenhyphenD85sBGT7dXjO-wvAP9IzjVqIVJiMQTZYlpXO5znJ7FVSu2KF2U7WfuOaA/s1600/product_thumbnail.jpg" /></a></div>
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this is cover of my ebook.</div>
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">Khushi har pal unke pas rakhna</span></div>
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">hello friends. how are you all?</span></div>
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">read it friends. </span></div>
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">Khushi har pal unke pas rakhna</span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;" /><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">eBook (ePub)</span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;" /><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;">read it friends......</span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;" /><span class="text_exposed_show" style="background-color: white; color: #333333; display: inline; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 18px;"><br /><a href="http://www.lulu.com/shop/prabhakar-prasad/khushi-har-pal-unke-pas-rakhna/ebook/product-20737155.html" rel="nofollow nofollow" style="color: #3b5998; cursor: pointer; text-decoration: none;" target="_blank">http://www.lulu.com/shop/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>prabhakar-prasad/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>khushi-har-pal-unke-pas-rak<wbr></wbr><span class="word_break" style="display: inline-block;"></span>hna/ebook/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>product-20737155.html</a><br /><br />its paperwork format link here ----<br /><br /><a href="http://www.lulu.com/shop/prabhakar-prasad/khushi-har-pal-unke-pas-rakhna/paperback/product-20737595.html" rel="nofollow nofollow" style="color: #3b5998; cursor: pointer; text-decoration: none;" target="_blank">http://www.lulu.com/shop/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>prabhakar-prasad/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>khushi-har-pal-unke-pas-rak<wbr></wbr><span class="word_break" style="display: inline-block;"></span>hna/paperback/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>product-20737595.html</a></span></div>
Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-21652365606678371662013-03-08T20:58:00.000+05:302013-03-08T20:58:06.275+05:30My Book<div class="separator" style="clear: both; text-align: center;">
<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiyGz1SsAxidQnJBqMKhB9fet0DRTTKYKGjp0cBM86VBmXoszWlxIZkWoAhqQ4kAhK6ik8iXfBJ82RJBWv_Yf730R0aeZT8_wQdKDCjAlVt38fonEpEQQFw2lj2VWDykJUMdjTveayBRv0/s1600/product_thumbnail.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiyGz1SsAxidQnJBqMKhB9fet0DRTTKYKGjp0cBM86VBmXoszWlxIZkWoAhqQ4kAhK6ik8iXfBJ82RJBWv_Yf730R0aeZT8_wQdKDCjAlVt38fonEpEQQFw2lj2VWDykJUMdjTveayBRv0/s1600/product_thumbnail.jpg" /></a></div>
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hiii friends,<br />
how are you all?<br />
this is my 1st book...<br />
you can read it here..... this has an ebook format..<br />
i think you love it...<br />
<span aria-live="polite" class="fbPhotosPhotoCaption" data-ft="{"type":45}" id="fbPhotoSnowliftCaption" style="background-color: white; color: #333333; display: inline; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 13px; line-height: 18px; outline: none; width: auto;" tabindex="0"><span class="hasCaption">Khushi har pal unke pas rakhna<br /><br />eBook (ePub)<br /><br />read it friends......<br /><br /><a href="http://www.lulu.com/shop/prabhakar-prasad/khushi-har-pal-unke-pas-rakhna/ebook/product-20737155.html" rel="nofollow nofollow" style="color: #3b5998; cursor: pointer; text-decoration: none;" target="_blank">http://www.lulu.com/shop/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>prabhakar-prasad/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>khushi-har-pal-unke-pas-rak<wbr></wbr><span class="word_break" style="display: inline-block;"></span>hna/ebook/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>product-20737155.html</a></span></span><br />
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Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-80824165670670070562013-02-13T02:13:00.003+05:302013-02-13T02:13:40.914+05:30Michael Kors<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; line-height: 18px;"><b><span style="font-size: x-large;">Michael Kors</span></b></span><br />
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: large; line-height: 18px;">Michael Kors is on track to be fashion's newest billionaire </span><a href="http://bit.ly/Y7fsFV" rel="nofollow nofollow" style="background-color: white; color: #3b5998; cursor: pointer; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; line-height: 18px; text-decoration: initial;" target="_blank">http://bit.ly/Y7fsFV</a><br />
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<span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; line-height: 18px;"><span style="font-size: large;">The fashion icon is fast approaching billionaire status as the stock of his company surged today after forecasting profits for fiscal 2013, more than double those from last year. If Kors doesn't sell any more company stock, he'd join the 10-figure club when it breaks $70 a share. Based on recent growth, that may not be far away.</span></span>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-65098944012373257322012-09-11T00:46:00.000+05:302012-09-11T00:46:19.569+05:30FREE Invitation to Join Zurker India<div dir="ltr" style="text-align: left;" trbidi="on">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh4GL0PJs553EJr32xKcK8tt5I_HguGaCCgGBiA8WvyDX4Gv-eqbeXfMpwQdyOX07DE1ps6atZq4ja_q8AnSdyRLYt1WOKCabatGLhZ4sEY7S9v1I8rjo1XCBHGJfOB0jszitO49qTf2xo/s1600/Capture.PNG" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="192" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh4GL0PJs553EJr32xKcK8tt5I_HguGaCCgGBiA8WvyDX4Gv-eqbeXfMpwQdyOX07DE1ps6atZq4ja_q8AnSdyRLYt1WOKCabatGLhZ4sEY7S9v1I8rjo1XCBHGJfOB0jszitO49qTf2xo/s320/Capture.PNG" width="320" /></a></div>
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<b><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;">this is zurker global membership countrywise ...</span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;">India has 269,958 members. but zurker India wants 1,000,000 members. when zurker India acheived these no. of members. then its going to public. now it is in beta phase.</span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;">so now zurker India wants 730,042 members of same value of vShares.. </span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;">so who want to catch up these vShares, and earn alots of money... </span><br style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;" /><span style="background-color: white; color: #333333; font-family: 'lucida grande', tahoma, verdana, arial, sans-serif; font-size: 12.800000190734863px; line-height: 13.600000381469727px;">and become an owner of zurker India. </span></b><br />
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<b>Zurker is a new visionary social networking website that is currently storming the web. You will become the owner of one social websites and also earn from it. Zurker is in beta and BY INVITE ONLY:<br />Well, here is your opportunity! Don't miss out!<br />so join here<br />Note that don't forget to confirm your email id.</b><br /><a href="http://www.facebook.com/l.php?u=http%3A%2F%2Fow.ly%2FdA46b&h=_AQEAYs2vAQGLj2No9c6FMNd9olXpLocGkutKO1rURJVq5w&s=1" rel="nofollow nofollow" style="color: #3b5998; cursor: pointer; text-decoration: none;" target="_blank">http://ow.ly/dA46b</a></div>
<br />
<br />
facebook : - http://facebook.com/prabhupd<br />
facebook group : - <a href="https://www.facebook.com/groups/489918284354041/">https://www.facebook.com/groups/489918284354041/</a><br />
<br />
have any question ask me?</div>
Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-82697080958266343752012-08-21T00:38:00.001+05:302012-08-21T00:38:45.936+05:30prelaunchX Invitation<a href="http://prelaunchx.com/x/prabhupd#.UDKLIj3Rh_I.blogger">prelaunchX Invitation</a>: You're invited to join prelaunchXAnonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com2tag:blogger.com,1999:blog-3038278470848839486.post-67058747134291107632012-06-27T03:39:00.000+05:302012-06-27T03:39:09.838+05:30OBESITY<div dir="ltr" style="text-align: left;" trbidi="on">
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<b><i><span style="color: blue;">OBESITY : -</span></i></b></div>
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Obesity is a growing global health problem. Obesity is when someone is so overweight that it is a threat to their health.</div>
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Obesity typically results from over-eating (especially an unhealthy diet) and lack of enough exercise.</div>
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In our modern world with increasingly cheap, high calorie food (example, fast food — or “junk food”), prepared foods that are high in things like salt, sugars or fat, combined with our increasingly sedentary lifestyles, increasing urbanization and changing modes of transportation, it is no wonder that obesity has rapidly increased in the last few decades, around the world.</div>
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<strong>For the first time in human history, the number of overweight people rivals the number of underweight people</strong>.… While the world’s underfed population has declined slightly since 1980 to 1.1 billion, the number of overweight people has surged to 1.1 billion.</div>
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<span style="color: #6e7173;">In the United States, 55 percent of adults are overweight by international standards. A whopping 23 percent of American adults are considered obese. And the trend is spreading to children as well, with one in five American kids now classified as overweight.… </span><i><u><span style="color: orange;">[O]besity cost the United States 12 percent of the national health care budget in the late 1990s, $118 billion, more than double the $47 billion attributable to smoking.</span></u></i></div>
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Overweight and obesity are advancing rapidly in the developing world as well … [while] 80 percent of the world’s hungry children live in countries with food surpluses.</div>
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technofixes like liposuction or olestra attract more attention than the behavioral patterns like poor eating habits and sedentary lifestyles that underlie obesity. Liposuction is now the leading form of cosmetic surgery in the United States, for example, at 400,000 operations per year. While billions are spent on gimmicky diets and food advertising, far too little money is spent on nutrition education.</div>
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The BBC revealed that <a href="http://www.bbc.co.uk/radio4/science/costingtheearth_20050414.shtml" id="id163311" style="color: #6e7173;" title="External Link: 'The best meal you'll never have!' Costing the Earth, BBC Radio 4, April 14, 2005">food wastage is enormous</a>. In the United Kingdom, some astonishing 30-40% of all food is never eaten, while in the US, some 40-50% of all food ready for harvest never gets eaten. UK alone sees some £20 billion ($38 billion US dollars) worth of food thrown away each year.</div>
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Nursing Schools lists <a href="http://www.nursingschools.net/blog/2010/05/12-startling-stats-on-americas-food-supply/" style="color: #6e7173;" title="External Link: '12 Startling Stats On Americas Food Supply', Nursing Schools, May 25, 2010">a number of concerning facts about food in the US</a>:</div>
<ul>
<li>40-50% of all food ready for harvest never gets eaten.</li>
<li>Every year, over 25% of Americans get sick from what they eat.</li>
<li>As few as 13 major corporations control nearly all of the slaughterhouses in the U.S.</li>
<li>Americans eat 31% more packaged food than fresh food.</li>
<li>The FDA tests only about 1% of food imports. (The US imports about 15% of what they eat.)</li>
<li>A simple frozen dinner can contains ingredients from over 500 different suppliers so you have to trust all of those hundreds of companies along the way stuck to regulations about food safety.</li>
<li>50% of tested samples of high fructose corn syrup tested for mercury.</li>
<li>Americans eat about six to nine pounds of chemical food additives per year.</li>
<li>Food intolerance is on the rise, with as many as 30 million people in the U.S. showing symptoms.</li>
<li>Fewer than 27% of Americans eat the correct ratio of meats to vegetables.</li>
<li>80% of the food supply is the responsibility of the FDA yet the number of inspections has decreased while the number of producers has increased.</li>
<li>Keeping fields contamination-free can cost well over $250,000–a discouraging sum to smaller farmers.</li>
</ul>
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The World Health Organization (WHO) provides a number of <a href="http://www.who.int/mediacentre/factsheets/fs311/en/index.html" style="color: #6e7173;" title="External Link: 'Obesity and overweight', Fact sheet No. 311, WHO, September 2006">facts on obesity</a>, including that globally in 2005:</div>
<ul>
<li>Approximately 1.6 billion adults (age 15+) were overweight</li>
<li>At least 400 million adults were obese</li>
<li>At least 20 million children under the age of 5 years are overweight globally in 2005.</li>
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The WHO also projected that by 2015, approximately 2.3 billion adults will be overweight and more than 700 million will be obese.</div>
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Globally, in 2010 the number of overweight children under the age of five, is estimated to be over 42 million. Close to 35 million of these are living in developing countries.</div>
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Overweight and obese children are likely to stay obese into adulthood and more likely to develop noncommunicable diseases like diabetes and cardiovascular diseases at a younger age.</div>
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The WHO that <a href="http://www.who.int/mediacentre/factsheets/fs311/en/index.html" style="color: #6e7173;" title="External Link: 'Obesity and overweight', Fact sheet No. 311, WHO, September 2006">many low- and middle-income countries are now facing a “double burdern” of disease</a>:</div>
<ul>
<li>While they continue to deal with the problems of infectious disease and under-nutrition, at the same time they are experiencing a rapid upsurge in chronic disease risk factors such as obesity and overweight, particularly in urban settings.</li>
<li>It is not uncommon to find under-nutrition and obesity existing side-by-side within the same country, the same community and even within the same household.</li>
<li>This double burden is caused by inadequate pre-natal, infant and young child nutrition followed by exposure to high-fat, energy-dense, micronutrient-poor foods and lack of physical activity.</li>
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With obesity comes increasing risks of</div>
<ul>
<li>Cardiovascular disease (mainly heart disease and stroke) — already the world’s number one cause of death, killing 17 million people each year.</li>
<li>Diabetes (type 2) — which has rapidly become a global epidemic.</li>
<li>Musculoskeletal disorders — especially osteoarthritis.</li>
<li>Some cancers (endometrial, breast, and colon).</li>
</ul>
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In Europe, for example, the <a href="http://www.euro.who.int/obesity" style="color: #6e7173;" title="External Link: 'Obesity in Europe', WHO Regional Office for Europe, May 26, 2008">WHO’s European regional body</a> says that “obesity is already responsible for 2-8% of health costs and 10-13% of deaths in different parts of the Region.”</div>
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The report further highlights that the costs of coronary heart disease alone are around £10 billion a year (approximately 14 billion in U.S. dollars). These costs are made up of</div>
<ul>
<li>£1.6 billion in direct costs (primarily to the tax payer through the costs of treatment by the British National Health Service) and</li>
<li>£8.4 billion in indirect costs (to industry and to society as a whole, though loss of productivity due to death and disability).</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
Other issues and problems they point out include:</div>
<ul>
<li>Encouraging/advertising unhealthy diets and foods (especially to children);</li>
<li>Generally putting low priority on health;</li>
<li>Industry-dominated food policy at the expense of local grocery stores;</li>
<li>Deteriorating health of children in poverty;</li>
<li>and so on.</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
Food systems causes of obesity</div>
<div style="margin-top: 10px; padding: 0px;">
The main problem has been the increased availability of high energy food, because of:</div>
<ul>
<li>Liberalized international food markets</li>
<li>Food subsidies that “have arguably distorted the food supply in favour of less healthy foodstuffs”</li>
<li>“Transnational food companies [that] have flooded the global market with cheap to produce, energy dense, nutrient empty foods”</li>
<li>“Supermarkets and food service chains [that are] encouraging bulk purchases, convenience foods, and supersized portions”</li>
<li>Healthy eating often being more expensive than less healthy options, (despite global food prices having dropped on average).</li>
<li>Marketing, especially “food advertising through television [which] aims to persuade individuals—particularly children—that they desire foods high in saturated fats, sugars, and salt.”</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
The local environment and obesity</div>
<div style="margin-top: 10px; padding: 0px;">
How people live, what factors make them active or sedentary are also a factor. For exapmle,</div>
<ul>
<li>“Research, mainly in high income countries, indicates that local urban planning and design can influence weight in several ways.”</li>
<li>For example, levels of physical activity are affected by<ul>
<li>Connected streets and the ability to walk from place to place</li>
<li>Provision of and access to local public facilities and spaces for recreation and play</li>
</ul>
</li>
<li>The increasing reliance on cars leads to physical inactivity, and while a long-time problem in rich countries, is a growing problem in developing countries.</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
<ins>Social conditions and obesity</ins></div>
<div style="margin-top: 10px; padding: 0px;">
Examples of issues the BMJ noted here include</div>
<ul>
<li>“Working and living conditions, such as having enough money for a healthy standard of living, underpin compliance with national health guidelines”</li>
<li>“Increasingly less job control, security, flexibility of working hours, and access to paid family leave … undermining the material and psychosocial resources necessary for empowering individuals and communities to make healthy living choices.”</li>
<li>Inequality, which can lead to different groups being disadvantaged and having less access to needed resources and healthier foods</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
</div>
<div style="margin-top: 10px; padding: 0px;">
Addressing obesity at the global level</div>
<div style="margin-top: 10px; padding: 0px;">
This involves international institutions, agreements, trade and other policies. For example,</div>
<ul>
<li>The World Health Organization (WHO) is a key institution at this level. It’s global strategy in this area focuses on developing food and agricultural policies that are aligned to promoting public health and multisectorial policies that promote physical activity, as well as generally being an information provider.</li>
<li>A joint program of the United Nations Food and Agriculture Organization and the World Health Organization, the experience of the <a href="http://www.codexalimentarius.net/" style="color: #6e7173;">Codex Alimentarius Commission</a> highlights the challenges at international level. The Commission was set up to help governments protect the health of consumers and ensure fair trade practices in the food trade.</li>
<li>But challenges and obstacles persist. For example, “industry representatives hugely outnumber representatives from public interest groups, resulting in an imbalance between the goals of trade and consumer protection.”</li>
</ul>
<div style="margin-top: 10px; padding: 0px;">
Obesity is a complex condition, one with serious social and psychological dimensions, that affects virtually all age and socioeconomic groups and threatens to overwhelm both developed and developing countries. In 1995, there were an estimated 200 million obese adults worldwide and another 18 million under-five children classified as overweight. As of 2000, the number of obese adults has increased to over 300 million. Contrary to conventional wisdom, the obesity epidemic is not restricted to industrialized societies; in developing countries, it is estimated that over 115 million people suffer from obesity-related problems.</div>
<div style="margin-top: 10px; padding: 0px;">
Generally, although men may have higher rates of overweight, women have higher rates of obesity. For both, obesity poses a major risk for serious diet-related noncommunicable diseases, including diabetes mellitus, cardiovascular disease, hypertension and stroke, and certain forms of cancer. Its health consequences range from increased risk of premature death to serious chronic conditions that reduce the overall quality of life.</div>
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</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-25609059411262106232012-05-30T04:35:00.000+05:302012-05-30T04:35:13.028+05:30Important Dates & Discoveries<div dir="ltr" style="text-align: left;" trbidi="on">
<b><u><span style="color: blue;">Important Dates & Discoveries : -</span></u></b><br />
A brief <span style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small; text-align: -webkit-auto;">chronological listing of some of the most important discoveries in cosmology, astronomy and physics, from ancient Babylon, India and Greece, right up to the 20th Century. Learn how some of the essential concepts and laws of modern physics which are mentioned in this website (and the earlier ideas out of which they grew) developed in a historical context.</span><span style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small; text-align: -webkit-auto;"> </span><br />
<span style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small; text-align: -webkit-auto;"><br /></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small; text-align: -webkit-auto;">Its sections : -</span><br />
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<ul style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: small; text-align: -webkit-auto;">
<li>Ancient World (20th Century B.C. - 4th Century A.D.)</li>
<li>Medieval & Renaissance World (5th Century A.D. - 16th Century)</li>
<li>Early Modern World (17th Century - 19th Century)</li>
<li>Modern World (20th Century )</li>
</ul>
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<span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">1) <b><i><span style="color: yellow;">Ancient World : -</span></i></b></span></div>
<div style="text-align: -webkit-auto;">
<ul style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: small;">
<li>20th -16th Century B.C. - Ancient Babylonian tablets show knowledge of the distinction between the moving planets and the “fixed” stars, and the recognition that the movement of planets are regular and periodic.</li>
<li>15th - 12th Century B.C. - The Hindu Rigveda of ancient India describes the origin of the universe in which a “cosmic egg” or Brahmanda, containing the Sun, Moon, planets and the whole universe, expands out of a single concentrated point before subsequently collapsing again, reminiscent of the much later Big Bang and oscillating universe theories.</li>
<li>5th Century B.C. - The Greek philosopher Anaxagoras becomes arguably the first to formulate a kind of molecular theory of matter, and to regard the physical universe as subject to the rule of rationality or reason.</li>
<li>5th Century B.C. - The Greek philosophers Leucippus and Democritus found the school of Atomism, which holds that the universe is composed of very small, indivisible and indestructible building blocks known as atoms, which then form different combinations and shapes in an infinite void.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Geocentric universe of Aristotle and Ptolemy - click for larger version" border="0" height="200" src="http://www.physicsoftheuniverse.com/images/cosmologies_aristotelian.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Geocentric universe of Aristotle and Ptolemy</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>4th Century B.C. - The Greek philosopher Aristotle describes a geocentric universe in which the fixed, spherical Earth is at the centre, surrounded by concentric celestial spheres of planets and stars. Although he portrays the universe as finite in size, he stresses that it exists unchanged and static throughout eternity.</li>
<li>4th Century B.C. - The Greek philosopher Heraclides proposes that the apparent daily motion of the stars is created by the rotation of the Earth on its axis once a day, and that the Sun annually circles a central Earth, while the other planets orbit the Sun (a geocentric model with heliocentric aspects).</li>
<li>3rd Century B.C. - The Stoic philosophers of ancient Greece assert a kind of “island universe” in which a finite cosmos is surrounded by an infinite void (similar in principle to a galaxy).</li>
<li>3rd Century B.C. - The Greek mathematician and geographer Eratosthenes proved that the Earth was round, and made a remarkably accurate calculation of its circumference and its tilt (as well as devising a system of latitude and longitude, and, possibly, estimating the distance of the Earth from the Sun).</li>
<li>3rd Century B.C. - The Greek astronomer and mathematician Aristarchus of Samos is the first to present an explicit argument for a heliocentric model of the Solar System, placing the Sun, not the Earth, at the center of the known universe. He describes the Earth as rotating daily on its axis and revolving annually about the Sun in a circular orbit, along with a sphere of fixed stars.</li>
<li>2nd Century B.C. - The Greek astronomer Hipparchus of Nicea makes the first measurement of the precession of the equinoxes, and compiles the first star catalogue (in which he proposes our modern system of apparent magnitudes). He also improves on the Solar System model of Apollonius of Perga, in which an eccentric circle carries around a smaller circle (an epicycle), which in turn carries around a planet.</li>
<li>2nd Century B.C. - The Hellenistic astronomer and philosopher Seleucus of Seleucia supports Aristarchus’ heliocentric theory, and links the tides to the influence of the Moon.</li>
<li>2nd Century A.D. - The Roman-Egyptian mathematician and astronomer Ptolemy (Claudius Ptolemaeus) describes a geocentric model, largely based on Aristotelian ideas, in which the planets and the rest of the universe orbit about a stationary Earth in circular epicycles, which becomes the scientific orthodoxy for nearly two millennia (essentially until Copernicus in the 16th Century). He also details the complex motions of the stars and planetary paths using equants, allowing astronomers to predict the positions of the planets.</li>
</ul>
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<span style="color: #741b47; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;"><b>2) MEDIEVAL & RENAISSANCE WORLD : -</b></span></div>
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<span style="color: #741b47; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;"><b><br /></b></span></div>
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<ul style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: small;">
<li>5th Century A.D. - The Indian astonomer and mathematician Aryabhata proposes that the Earth turns on its own axis, and describes elliptical orbits around the Sun, which some have interpreted as heliocentrism.</li>
<li>6th Century A.D. - The Christian philosopher John Philoponus of Alexandria argues against the ancient Greek notion of an infinite past, and is perhaps the first commentator to argue that the universe is finite in time and therefore had a beginning.</li>
<li>7th Century - The Indian astronomer Brahmagupta, a follower of the heliocentric theory of the Solar System earlier developed by Aryabhata, recognizes gravity as a force of attraction in his "The Opening of the Universe" of 628, in which he describes a force of attraction between the Sun and the Earth.</li>
<li>9th Century - The Muslim astronomer Ja'far ibn Muhammad Abu Ma'shar al-Balkhi developes a planetary model which some have interpreted as heliocentric model.</li>
<li>9th - 11th Century - Early Muslim and Jewish theologians such as Al-Kindi, Saadia Gaon and Al-Ghazali offer logical arguments supporting a finite universe.</li>
<li>11th Century - The Arab polymath Alhazen (also known as Ibn al-Haytham) becomes the first to apply the scientific method to astronomy.</li>
<li>11th Century - The Persian astronomer Abu al-Rayhan al-Biruni describes the Earth's gravitation as the attraction of all things towards the centre of the Earth, and hypothesizes that the Earth turns daily on its axis and annually around the Sun.</li>
<li>11th Century - The Persian polymath Omar Khayyam demonstrates that the universe is not moving around Earth, but that the Earth revolves on its axis, bringing into view different star constellations throughout the night and day. He also calculated the <b><i><u><span style="color: red;">solar year as 365.24219858156 days</span></u></i></b> (correct to six decimal places).</li>
<li>14th Century - The Arab astronomer and engineer Ibn al-Shatir (of the Iranian Maragha school of astronomy) refines and improves the accuracy of the geocentric Ptolemaic model and develops the first accurate model of lunar motion.</li>
<li>15th Century - The Persian astronomer and mathematician Ali Qushji rejects the Aristotelian notion of a stationary Earth in favour of a rotating Earth.</li>
<li>15th Century - Somayaji Nilakantha of the Kerala school of astronomy and mathematics in southern India develops a computational system for a partially heliocentric planetary model in which Mercury, Venus, Mars, Jupiter and Saturn orbit the Sun, which in turn orbits the Earth.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Heliocentric universe of Copernicus" border="0" height="200" src="http://www.physicsoftheuniverse.com/images/cosmologies_copernican.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Heliocentric universe of Copernicus</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1543 - The Polish astronomer and polymath Nicolaus Copernicus (adapting the geocentric Maragha model of Ibn al-Shatir to meet the requirements of the ancient heliocentric universe of Aristarchus), proposes that the Earth rotates on its axis once daily and travels around the Sun once a year, and demonstrates that the motions of celestial objects can be explained without putting the Earth at rest in the centre of the universe. His Copernican Principle (that the Earth is not in a central, specially favoured position) and its implications (that celestial bodies obey physical laws identical to those on Earth) first establishes cosmology as a science rather than a branch of metaphysics, and marks a shift away from anthropocentrism.</li>
<li>1576 - The English astronomer Thomas Digges popularizes Copernicus’ ideas and also extends them by positing the existence of a multitude of stars extending to infinity, rather than Copernicus’ narrow band of fixed stars.</li>
<li>1584 - The Italian philosopher Giordano Bruno takes the Copernican Principle a stage further by suggesting that even the Solar System is not the centre of the universe, but rather a relatively insignificant star system among an infinite multitude of others.</li>
<li>1587 - The Danish nobleman and astronomer Tycho Brahe develops a kind of hybrid of the Ptolemaic and Copernican models, a geo-heliocentric system similar to that of Somayaji Nilakantha, now known as the Tychonic system. This involves a static Earth at the centre of the universe, around which revolve the Sun and the Moon, with the other five planets revolving around the Sun.</li>
</ul>
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<span style="color: orange; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;"><b>3) EARLY MODERN WORLD : -</b></span></div>
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<ul style="background-color: white; font-family: Arial, Helvetica, 'Sans Serif'; font-size: small;">
<li>1605 - The German mathematician and astronomer Johannes Kepler establishes his three Laws of Planetary Motion, mathematical laws that describe the motion of planets in the Solar System, including the ground-breaking idea that the planets follow elliptical, not circular, paths around the Sun. Newton later used them to deduce his own Laws of Motion and his Law of Universal Gravitation.</li>
<li>1610 - The Italian mathematician and physicist Galileo Galilei develops an astronomical telescope powerful enough to indentify moons orbiting Jupiter, sunspots on the Sun and the different phases of Mercury, all of which are instrumental in convincing the scientific community of the day that the heliocentric Copernican model of the Solar System is superior to the geocentric Ptolemiac model.</li>
<li>1632 - Galileo Galilei first describes the Principle of Relativity, the idea that the fundamental laws of physics are the same in all inertial frames and that, purely by observing the outcome of mechanical experiments, one cannot distinguish a state of rest from a state of constant velocity.</li>
<li>1633 - The French philosopher René Descartes outlines a model of a static, infinite universe made up of tiny “corpuscles” of matter, a viewpoint not dissimilar to ancient Greek atomism. Descartes’ universe shares many elements of Sir Isaac Newton’s later model, although Descartes’ vacuum of space is not empty but composed of huge swirling whirlpools of ethereal or fine matter, producing what would later be called gravitational effects.</li>
<li>1638 - Galileo Galilei demonstrates that unequal weights would fall with the same finite speed in a vacuum, and that their time of descent is independent of their mass. Thus, freely falling bodies, heavy or light, have the same constant acceleration, due to the force of gravity.</li>
<li>1675 - The English physicist Sir Isaac Newton argues that light is composed of particles, which are refracted by acceleration toward a denser medium, and posits the existence of “aether” to transmit forces between the particles.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Newton's Law of Universal Gravitation - click for larger version" border="0" height="126" src="http://www.physicsoftheuniverse.com/images/relativity_gravity.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Newton's Law of Universal Gravitation</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1687 - Sir Isaac Newton publishes his “Principia”, which describes an infinite, steady state, static, universe, in which matter on the large scale is uniformly distributed. In the work, he establishes the three Laws of Motion (“a body persists its state of rest or of uniform motion unless acted upon by an external unbalanced force”; “force equals mass times acceleration”; and “to every action there is an equal and opposite reaction”) and the Law of Universal Gravitation (that every particle in the universe attracts every other particle according to an inverse-square formula) that were not to be improved upon for more than two hundred years. He is credited with introducing the idea that the motion of objects in the heavens (such as planets, the Sun and the Moon) can be described by the same set of physical laws as the motion of objects on the ground (like cannon balls and falling apples).</li>
<li>1734 - The Swedish scientist and philosopher Emanuel Swedenborg proposes a hierarchical universe, still generally based on a Newtonian static universe, but with matter clustered on ever larger scales of hierarchy, endlessly being recycled. This idea of a hierarchical universe and the “nebular hypothesis” were developed further (independently) by Thomas Wright (1750) and Immanuel Kant (1775).</li>
<li>1761 - The Swiss physicist Johann Heinrich Lambert supports Wright and Kant’s hierarchical universe and nebular hypothesis, and also hypothesizes that the stars near the Sun are part of a group which travel together through the Milky Way, and that there are many such groupings or star systems throughout the galaxy.</li>
<li>1783 - The amateur British astronomer John Michell proposes the theoretical idea of an object massive enough that its gravity would prevent even light from escaping (which has since become known as a black hole). He realizes that such an object would not be directly visible, but could be identified by the motions of a companion star if it was part of a binary system. A similar idea was independently proposed by the Frenchman Pierre-Simon Laplace in 1795.</li>
<li>1789 - The French chemist Antoine-Laurent de Lavoisier definitively states the Law of Conservation of Mass (although others had previously expressed similar ideas, including the ancient Greek Epicurus, the medieval Persian Nasir al-Din al-Tusi and the 18th Century scientists Mikhail Lomonosov, Joseph Black, Henry Cavendish and Jean Rey), and identifies (albeit slightly incorrectly) 23 elements which he claims can not be broken down into simpler substances.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Wave interference in Thomas Young's double-slit experiment - click for larger version" border="0" height="170" src="http://www.physicsoftheuniverse.com/images/quantum_double_slit.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Wave interference in Thomas Young's double-slit experiment</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1803 - The English scientist Thomas Young demonstrates, in his famous double-slit experiment, the interference of light and concludes that light is a wave, not a particle as Sir Isaac Newton had ruled.</li>
<li>1805 - The English chemist John Dalton develops his atomic theory, proposing that each chemical element is composed of atoms of a single unique type, and that, though they are both immutable and indestructible, they can combine to form more complex structures.</li>
<li>1839 - The English scientist Michael Faraday concludes from his work on electromagnetism that, contrary to scientific opinion of the time, the divisions between the various kinds of electricity are illusory. He also establishes that magnetism can affect rays of light, and that there is an underlying relationship between the two phenomena.</li>
<li>1861 - The French scientist Louis Pasteur’s experiments show that organisms such as bacteria and fungi do not appear of their own accord in sterile nutrient-rich media, suggesting that the long-held acceptance of the spontaneous generation of life from non-living matter may be incorrect.</li>
<li>1864 - The Scottish physicist James Clerk Maxwell demonstrates that electric and magnetic fields travel through space in the form of waves at the constant speed of light and that electricity, magnetism and even light are all manifestations of electromagnetism. He collected together laws originally derived by Carl Friedrich Gauss, Michael Faraday and André-Marie Ampère into a unified and consistent theory (often known as Maxwell’s Equations).</li>
<li>1896 - The French physicist Henri Becquerel discovers that certain kinds of matter emit radiation of their own accord (Radioactivity).</li>
<li>1897 - The British physicist J. J. Thomson discovers the electron, the first known sub-atomic particle.</li>
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<span style="color: blue; font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;"><b><i>4) MODERN WORLD : -</i></b></span></div>
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<span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;"><ul>
<li>1900 - The German physicist Max Planck suggests, while describing his law of black body radiation, that light may be emitted in discrete frequencies or “quanta”, and establishes the value of the Planck Constant to describe the sizes of these quanta. This is often regarded as marking the birth of quantum physics.</li>
<li>1905 - The German physicist Albert Einstein shows how the Photoelectric Effect is caused by absorption of quanta of light (or photons), an important step in understanding the quantum nature of light and electrons, and a strong influence on the formation of the concept of wave-particle duality in quantum theory.</li>
<li>1905 - Albert Einstein publishes his Special Theory of Relativity, in which he generalizes Galileo's Principle of Relativity (that all uniform motion is relative, and that there is no absolute and well-defined state of rest) from mechanics to all the laws of physics, and incorporates the principle that the speed of light is the same for all inertial observers regardless of the state of motion of the source.</li>
<li>1905 - In a separate paper, Albert Einstein derives the concept of mass-energy equavalance (that any mass has an associated energy) and his famous <b><i><u><span style="color: blue;">E = mc<sup>2</sup> </span></u></i></b>equation.</li>
<li>1907 - The German mathematician Hermann Minkowski realizes that Einstein's Special Theory of Relativity can be best understood in a four-dimensional space, which he calls “space-time” and in which time and space are not separate entities but intermingled in a four-dimensional space.</li>
<li>1911 - The New Zealand chemist Ernest Rutherford interprets the 1909 experiments of Hans Geiger and Ernest Marsden, establishing for the first time the “planetary model” of the atom, where a central nucleus is circled by a number of tiny electrons like planets around a Sun.</li>
<li>1915 - The German physicist Karl Schwarzschild provides the first exact solution to Einstein’s field equations of general relativity (even before Einstein publishes the theory) for the limited case of a single spherical non-rotating mass, which leads to the “Schwarzschild radius” which defines the size of the event horizon of a non-rotating black hole.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="General relativity predicts the gravitational bending of light by massive bodies - click for larger version" border="0" height="200" src="http://www.physicsoftheuniverse.com/images/relativity_light_bending.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">General relativity predicts the gravitational bending of light by massive bodies</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1916 - Albert Einstein publishes his General Theory of Relativity, in which he unifies special relativity and Newton's Law of Universal Gravitation, and describes gravity as a property of the curvature of four-dimensional space-time. Objects (including planets, like the Earth, for instance) fly freely under their own inertia through warped space-time, following curved paths because this is the shortest possible path in warped space.</li>
<li>1916 - The Austrian physicist Ludwig Flamm examinesSchwarzschild’s solution to Einstein’s field equations and points out that the equations theoretically allow for some kind of invisible connection between two distinct regions of space-time (later to become known as a “wormhole”).</li>
<li>1917 - Albert Einstein publishes a paper introducing the “cosmological constant” into the General Theory of Relativity in an attempt to model the behaviour of the entire universe, an idea he later called his “greatest blunder” but which, in the light of recent discoveries, is beginning to look remarkably prescient.</li>
<li>1919 - Ernest Rutherford is credited with the discovery of the proton when he notices the signatures of hydrogen nuclei when alpha-particles are shot into nitrogen gas. In these experiments, he also became the first person to transmute one element into another (nitrogen into oxygen) through a deliberate man-made nuclear reaction.</li>
<li>1919 - The English astrophysicist Arthur Eddington uses his measurements of an eclipse to confirm the deflection of starlight by the gravity of the Sun as predicted in Einstein’s General Theory of Relativity.</li>
<li>1919 - The German mathematician Theodor Kaluza proposes the addition of a fifth dimension to the General Theory of Relativity, a precursor to much later superstring theory attempts to combine general relativity and quantum theory. The Swedish physicist Oskar Klein independently proposes a similar idea in 1926.</li>
<li>1922 - The Russian biochemist Alexander Oparin hypothesizes that life on Earth began in a “primeval soup” of matter and water between 3.9 and 3.5 billion years ago, as chemical reactions produced small organic molecules from substances present in the atmosphere, which were then organized by chance into the more complex organic molecules that are the basis of<a class="sticky" href="http://www.physicsoftheuniverse.com/dates.html" style="color: #006600;">life</a>.</li>
<li>1922 - The Russian cosmologist and mathematician Alexander Friedmann discovers the expanding universe solution to Einstein’s general relativity field equations. The solution for a universe with positive curvature (spherical space) results in the universe expanding for a time and then contracting due to the pull of its gravity, in a perpetual cycle of Big Bang followed by Big Crunch now known as the oscillating universe theory.</li>
<li>1925 - The American astronomer Edwin Hubble proves conclusively that nebulae such as the Andromeda Nebula are much too distant to be part of the Milky Way and are in fact entire galaxies outside our own, thus settling the “Great Debate” about the nature of spiral nebulae and the size of the universe.</li>
<li>1925 - The Austrian theoretical physicist Wolfgang Pauli establishes an important quantum mechanical principle known as the Pauli exclusion principle, which states that no two identical fermions (such as electrons) may occupy the same quantum state simultaneously.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Heisenberg's microscope thought experiment to illustrate the effects of the uncertainty principle - click for larger version" border="0" height="318" src="http://www.physicsoftheuniverse.com/images/quantum_microscope.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Heisenberg's microscope thought experiment to illustrate the effects of the uncertainty principle</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1926 - The German physicist Werner Heisenberg formulates his uncertainity principle, that the values of certain pairs of variables cannot both be known exactly (i.e. the more precisely one variable is known, the less precisely the other can be known), a central concept in quantum physics.</li>
<li>1926 - The Austrian physicist Erbin
Schrödinger publishes what is now known as the Schrödinger Equation, a central and revolutionary achievement in quantum physics. Later, in 1935, he proposes the famous “Schrödinger's Cat” thought experiment or paradox concerning quantum superposition, decoherence and entanglement.</li>
<li>1927 - The Belgian Roman Catholic priest and physicist Georges Lemaitre proposes (even before Hubble’s corroborating evidence) that the universe is expanding, followed in 1931 by the first definitive version of what has become known as the Big Bang theory of the origin of the universe.</li>
<li>1928 - The British physicist Paul Dirac provides a description of the “spin” of elementry particles such as electrons which is consistent with both the principles of quantum mechanics and the Special Theory of Relativity, and predicts the existence of antimatter.</li>
<li>1929 - Edwin Hubble definitively shows that all the galaxies in the universe are moving away from us, according to a formula which has become known as Hubble's Law, showing that the universe is not in fact static, but expanding.</li>
<li>1932 - The English physicist James Chadwick discovers the neutron; the American physicist Carl Anderson identifies the positron (the anti-electron which had been predicted by Paul Dirac a few years earlier); and the British physicist John Cockcroft and the Irish physicist Ernest Walton succeed in transmuting lithium into helium and other chemical elements using high energy protons, popularly referred to as “splitting the atom”.</li>
<li>1934 - The Swiss-American astronomer Fritz Zwicky and the German-American Walter Baade coin the term “supernova” and hypothesize (correctly) that they are the transition of normal stars into neutron stars, as well as the origin of cosmic rays. Zwicky also uses the virial theorem to deduce the existence of unseen matter (what is now called dark matter) in the universe, as well as the effect of gravitational lensing.</li>
<li>1935 - Albert Einstein and the Israeli physicist Nathan Rosen achieve a solution to Einstein’s field equations known as an Einstein-Rosen bridge (also known as a Lorentzian wormhole or a Schwarzschild wormhole).</li>
<li>1935 - The Indian-American astrophysicist Subrahmanyan Chandrasekhar establishes the “Chandrasekhar limit” of about 1.4 solar masses, above which a star must continue to collapse into a neutron star rather than settling down into a white dwarf.</li>
<li>1939 - The discovery of nuclear fission results from the Berlin experiments of Otto Hahn, Lise Meitner, Fritz Strassmann and Otto Frisch.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="In a steady state universe, overall density remains constant - click for larger version" border="0" height="200" src="http://www.physicsoftheuniverse.com/images/glossary_steady_state.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">In a steady state universe, overall density remains constant</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1948 - The English astronomer Fred Hoyle and the Austrians Thomas Gold and Hermann Bondi propose a non-standard cosmology (i.e. one opposed to the standard Big Bang model) known as the steady state universe. This theory describes a universe that has no beginning and no end, and that expands continuously, but in which new matter is constantly created and inserted as it expands in order to maintain a constant density, so that its overall look does not change over time.</li>
<li>1953 - The experiments of the American biochemists Stanley Miller and Harold Urey (known as the Miller-Urey experiments) demonstrate the feasibility of producing basic organic monomers such as amino acids from a highly reduced mixture of gases, in an attempt to back up Alexander Oparin’s hypotheses on the origins of life on Earth.</li>
<li>1963 - The New Zealand mathematician Roy Kerr discovers a solution to Einstein’s general relativity field equations which describes a spinning black hole, and argues that these are likely to be common objects throughout the universe.</li>
<li>1965 - The American astronomers Arno Penzias and Robert Wilson discover the existence of cosmic microwave background radiation, considered by most to be the best evidence for the Big Bang model of the universe (and effectively disproving Hoyle et al’s steady state universe theory).</li>
<li>1966 - The Russian physicist Andrei Sakharov outlines the three conditions necessary for the observed matter-antimatter imbalance in the universe to be possible, and hypothesizes about singularities linking parallel universe.</li>
<li>1969 - The Murchison meteorite falls on Australia, revealing significant quantities of organic compounds and amino acids (the basis of early life on Earth) which originated in outer space.</li>
<li>1970 - The English physicist Stephen Hawking provides, along with Roger Penrose, theorems regarding singularities in space-time, indicating that singularities and black holes are actually a fairly generic feature of general relativity. He also predicts that black holes should in theory emit radiation (known today as Hawking Radiation) until they eventually exhaust their energy and evaporate.</li>
<li>1980 - The American physicist Alan Guth proposes a model of the universe based on the Big Bang, but incorporating a short, early period of exponential cosmic inflation in order to solve the horizon and flatness problems of the standard Big Bang model.</li>
<li>1980 - The invention of the Scanning Tunnelling Microscope, by the German Gerd Binnig and the Swiss Heinrich Rohrer, shows visually for the first time that matter is composed of spherical atoms stacked row on row.</li>
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<tr><td align="CENTER" bgcolor="#EEEEEE" valign="TOP"><a href="http://www.physicsoftheuniverse.com/dates.html" style="color: #0000c6;"><img alt="Artist's impression of parallel universes making up the multiverse - click for larger version" border="0" height="266" src="http://www.physicsoftheuniverse.com/images/bigbang_multiverse.jpg" width="200" /></a><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: x-small;">Artist's impression of parallel universes making up the multiverse</span><span style="font-family: Arial, Helvetica, 'Sans Serif'; font-size: xx-small;"><br /></span></td></tr>
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<li>1983 - The Russian-American physicist Andrei Linde develops Guth’s cosmic inflation idea further with his chaotic inflation (or eternal inflation) theory, which sees our universe as just one of many “bubble universe” that have developed as part of a multiverse.</li>
<li>1984-6 - A series of important discoveries in string theory leads to the “first superstring revolution”, and it is first realized that string theory might be capable of describing all elemantry particles as well as the interactions between them.</li>
<li>1995 - The American theoretical physicist Edward Witten and others develop M-theory, and spark a flurry of new research in string theory, sometimes called the “second superstring revolution”.</li>
<li>1998 - Observations of distant Type 1a supernovas, both by the American astrophysicist Saul Perlmutter and by the Australians Nick Suntzeff and Brian Schmidt, indicate that they are actually further away from the Earth than expected, suggesting an accelerating expansion of the universe.</li>
<li>2002 - The American physicist Paul Steinhardt and South African-British physicist Neil Turok propose another variation of the inflating universe known as the cyclic model, developed using state-of-the-art M-theory,superstring theory and brane cosmology, which involves an inflating universe expanding and contracting in cycles.</li>
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<br /></div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-21704976109650884042012-04-18T01:47:00.001+05:302012-04-18T01:47:28.602+05:30Minerva Rewards<a href="http://prabhupd.minervarewards.com/#.T43Ppok15IQ.blogger">Minerva Rewards</a>: It's about time somebody came up with something like this! Brilliant idea. Totally awesome.<br />
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</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-20867526307695937192012-04-17T02:56:00.002+05:302012-04-17T02:56:37.693+05:30are your child's milk teeth break?<div dir="ltr" style="text-align: left;" trbidi="on">
<span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="नई दिल्ली।।">New Delhi .. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="क्या आपके बच्चे के दूध के दांत टूटने वाले हैं ?">What are your child's milk teeth break? </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="तो उन्हें फेंकने की बजाए आप उन्हें डेंटल स्टेम सेल बैंक में भविष्य में इस्तेमाल के लिए सहेज कर रख सकते हैं।">As opposed to throwing them in the dental stem cell bank can be saved for future use. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="बच्चे के आगे के जीवन में गम्भीर बीमारियों की दशा में ये दांत स्टेम कोशिकाओं के निर्माण में इस्तेमाल हो सकते हैं।">In the case of serious illnesses in the life of the child's tooth stem cells can be used in the construction.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="भारत में डेंटल स्टेम सेल बैंकिंग नई है, लेकिन फिर भी इसे अम्बलीकल कॉर्ड ब्लड बैंकिंग की अपेक्षा अधिक कारगर विकल्प माना जा रहा है।">Dental stem cell banking in India is new, but it Amblikl cord blood banking is believed to be a more effective alternative. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="स्टेम सेल थेरेपी में मरीज के शरीर के क्षतिग्रस्त ऊतकों में या घाव में स्वस्थ व नई कोशिकाएं स्थापित की जाती हैं।">Stem cell therapy in damaged tissue or lesion in the patient's body in a healthy and new cells are installed.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="स्टेमेड बायोटेक के संस्थापक व प्रबंध निदेशक शैलेष गडरे ने कहा, 'अम्बलीकल कॉर्ड रक्त सम्बंधी कोशिकाओं की अच्छी स्रोत है।">Founder and Managing Director Shailesh Gdere Stemed Biotech, said: "Amblikl good source of cord blood-related cells. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="खून सम्बंधी बीमारियों जैसे रक्त कैंसर में इनका इस्तेमाल किया जा सकता है।">Related illnesses such as blood can be used to treat blood cancer. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="वैसे कहा जाता है कि सभी बीमारियों में रक्त सम्बंधी बीमारियां केवल चार प्रतिशत ही होती हैं।'">It is said that only four percent of all illnesses are blood-related diseases. "<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="उन्होंने कहा, 'बची हुई 96 प्रतिशत ऊतक सम्बंधी बीमारियों के लिए ऊतक सम्बंधी स्टेम कोशिकाएं हासिल करने को दांत एक अच्छा स्रोत हो सकते हैं।">"The remaining 96 percent tissue-related diseases related to tissue stem cells may be a good source to extract the tooth. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="ये कोशिकाएं शरीर के सभी प्रकार के ऊतकों में प्रयुक्त हो सकती हैं।">These cells can be used in all kinds of body tissue. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="उदाहरण के तौर पर अल्जाइमर बीमारी की स्थिति में मस्तिष्क में, पार्किंसंस बीमारी होने पर आंख में, सिरोसिस होने पर लीवर में, मधुमेह होने पर अग्नाशय में व फ्रैक्चर की दशा में हड्डियों के अलावा त्वचा में भी इनका इस्तेमाल हो सकता है।'">For instance, in the brain in Alzheimer's disease, Parkinson's disease in the eye, cirrhosis of the liver, diabetes, the pancreas and in the case of fracture of the bones in the skin can also use them. "<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="ऊतक सम्बंधी कोशिकाओं का दिल की कोशिकाओं के पुनर्निर्माण में भी इस्तेमाल हो सकता है।">Related tissue cells can be used in the reconstruction of the heart cells.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="बच्चों के दांत सम्बंधी रोगों की विशेषज्ञ सविता मेनन कहती हैं कि पांच से 12 साल उम्र के बच्चों के दूध के दांतों से स्टेम कोशिकाएं आसानी से निकाली जा सकती हैं।">Children's teeth related diseases expert Savita Menon says that five to 12 years of age, children's milk teeth stem cells can be easily removed. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इसके लिए जब बच्चे का कोई दांत हिलने लगे तब उसे निकालकर उससे बिना किसी शल्यक्रिया के स्टेम कोशिकाएं इकट्ठी की जा सकती हैं।">When the baby began to move a tooth taken out from the stem cells without any surgery can be collected.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="भारत में डेंटल स्टेम सेल बैंकिंग की सुविधा देने वाली कम्पनियों की संख्या अभी बहुत कम हैं।">Dental stem cell banking facility in India that the number of companies are still very low. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इनमें स्टेमेड व स्टोर योर सेल्स जैसी कम्पनियां शामिल हैं।">These include companies such as Stemed and Store Your Sales. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="स्टेम कोशिकाओं को 21 साल की अवधि तक संरक्षित रखने पर करीब 100,000 रुपये का खर्च आ सकता है।">Stem cells to preserve the 21-year period may cost around Rs 100,000.</span>
</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-76172668479512893232012-04-17T02:50:00.001+05:302012-04-17T02:50:17.414+05:30Scientists are busy now in making of Human Brain<div dir="ltr" style="text-align: left;" trbidi="on">
<span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="लंदन : वैज्ञानिक अब मनुष्य का दिमाग बनाने में लग गए हैं।">London: Scientists are now looking into making the human mind. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इसके लिए वे दुनिया के सबसे ताकतवर कंप्यूटर का सहारा ले रहे हैं।">For this, the world's most powerful computers are taking. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="वे ब्रेन के पूरे स्ट्रक्चर और उसके काम करने के सिस्टम की नकल करने जा रहे हैं।">The structure of the brain and are going to copy the system to work. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="वे थ्रीडी इमेज का इस्तेमाल करेंगे और इसके जरिये यह समझने की कोशिश करेंगे कि दिमाग कैसे काम करता है।">They will use image Threedi through it will try to understand how the brain works.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="एक इंटरनैशनल टीम इस प्रोजेक्ट में लगी हुई है।">An international team is engaged in the project. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इसकी अगुवाई स्विट्जरलैंड के प्रफेसर हेनरी मार्करैम कर रहे हैं।">Prof Henry Markram of the Swiss are headed. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इस प्रोजेक्ट के 12 साल में पूरा होने की उम्मीद है।">The project is expected to be completed in 12 years.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="वैज्ञानिकों का कहना है कि आदमी के दिमाग में 100 अरब न्यूरॉन हैं।">The scientists say that man's mind has 100 billion neurons. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="हरेक न्यूरॉन हर सेकंड अरबों गणनाएं करता है।">The billions of calculations every second, each neuron. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="इसलिए सुपर कंप्यूटर को अरबों - अरब गणनाएं एकसाथ करने की जरूरत पड़ेगी।">So the supercomputer billion - billion calculations need to be together. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="एक परमाणु बिजली केंद्र के समान उसे नतीजे देने पड़ेंगे।">Similar to a nuclear power center will deliver the results.<br /></span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="प्रफेसर मार्करैम का कहना है कि अगर यह स्टडी कामयाब रहती है तो इससे सालाना उन दो अरब लोगों को लाभ होगा जो अल्जाइमर और पार्किंसन जैसी दिमागी बीमारियों से ग्रस्त हो जाते हैं।">Prof Markram says that if this study is successful, it will benefit the annual two billion people who suffer from Alzheimer's and Parkinson's like mental illnesses are. </span><span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="हमें यह समझने की जरूरत है कि क्या चीज आदमी को बनाती है।">We need to understand what makes a man.</span>
<br />
<span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="हमें यह समझने की जरूरत है कि क्या चीज आदमी को बनाती है।"><br /></span><br />
<span style="background-color: whitesmoke; color: #333333; font-family: arial, sans-serif; font-size: 16px; text-align: -webkit-auto;" title="हमें यह समझने की जरूरत है कि क्या चीज आदमी को बनाती है।"><br /></span></div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-59115163064681747292012-04-17T02:18:00.002+05:302012-04-17T02:18:49.311+05:30THE ORIGIN AND FATE OF THE UNIVERSE<div dir="ltr" style="text-align: left;" trbidi="on">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqrrfwpeoiMpZGIuqbSu7X4ul_-F3qBPddbrvXr3ISiLhxIwmto7O7h_007E7k6jCI4uTXgs-z8duiND4Q9v7ym61_v-lY4bpXzk7u7JokOlxtVLVKQx6r6spDfMtfR71AmGwhRvawwlo/s1600/black-holes-hold-universe_18665_600x450.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="266" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqrrfwpeoiMpZGIuqbSu7X4ul_-F3qBPddbrvXr3ISiLhxIwmto7O7h_007E7k6jCI4uTXgs-z8duiND4Q9v7ym61_v-lY4bpXzk7u7JokOlxtVLVKQx6r6spDfMtfR71AmGwhRvawwlo/s320/black-holes-hold-universe_18665_600x450.jpg" width="320" /></a></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">1)From<span style="background-color: yellow;"> <b><span style="color: blue;">Einstein’s general theory of
relativity</span></b></span>, predicted that space-time began at the big bang singularity and<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">would come to an end either at the big
crunch singularity (if the whole universe recollapsed), or at a singularity
inside<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">a black hole (if a local region, such
as a star, were to collapse). Any matter that fell into the hole would be
destroyed<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">at the singularity, and only the
gravitational effect of its mass would continue to be felt outside.<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;"><br /></span></div>
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</div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">2) when quantum effects were taken
into account, it seemed that the mass or energy of the matter would eventually be<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">returned to the rest of the universe,
and that the black hole, along with any singularity inside it, would evaporate<o:p></o:p></span></div>
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt; mso-ansi-language: EN-US; mso-bidi-language: AR-SA; mso-fareast-font-family: Calibri; mso-fareast-language: EN-US; mso-fareast-theme-font: minor-latin;">away and finally disappear.</span><br />
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt; mso-ansi-language: EN-US; mso-bidi-language: AR-SA; mso-fareast-font-family: Calibri; mso-fareast-language: EN-US; mso-fareast-theme-font: minor-latin;"><br /></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt; mso-ansi-language: EN-US; mso-bidi-language: AR-SA; mso-fareast-font-family: Calibri; mso-fareast-language: EN-US; mso-fareast-theme-font: minor-latin;"> </span><span style="font-family: Arial, sans-serif; font-size: 11.5pt;">Could quantum mechanics have an
equally dramatic effect on the big bang and big</span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">crunch singularities? What really
happens during the very early or late stages of the universe, when
gravitational<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">fields are so strong that quantum
effects cannot be ignored? Does the universe in fact have a beginning or an
end?<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">And if so, what are they like? </span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">According to “Hot big bang model”, This
assumes that the universe is described by a Friedmann model,<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">right back to the big bang. In such
models one finds that as the universe expands, any matter or radiation in it
gets<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">cooler. (When the universe doubles in
size, its temperature falls by half.) Since temperature is simply a measure of<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">the average energy – or speed – of the
particles, this cooling of the universe would have a major effect on the matter<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">in it. At very high temperatures,
particles would be moving around so fast that they could escape any attraction<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">toward each other due to nuclear or
electromagnetic forces, but as they cooled off one would expect particles that<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">attract each other to start to clump
together. Moreover, even the types of particles that exist in the universe
would<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">depend on the temperature. At high
enough temperatures, particles have so much energy that whenever they collide<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">many different particle/antiparticle
pairs would be produced – and although some of these particles would annihilate<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">on hitting antiparticles, they would
be produced more rap-idly than they could annihilate. At lower temperatures,<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">however, when colliding particles have
less energy, particle/antiparticle pairs would be produced less quickly – and<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">annihilation
would become faster than production.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">At the big bang itself the universe is thought to have had zero size, and so to have been infinitely hot. But as the</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">universe expanded, the temperature of the radiation decreased. One second after the big bang, it would have fallen</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">to about ten thousand million degrees. This is about a thousand times the temperature at the center of the sun, but</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">temperatures as high as this are reached in H-bomb explosions. At this time the universe would have contained</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">mostly photons, electrons, and neutrinos (extremely light particles that are affected only by the weak force and</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">gravity) and their antiparticles, together with some protons and neutrons. As the universe continued to expand and</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">the temperature to drop, the rate at which electron/antielectron pairs were being produced in collisions would have</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">fallen below the rate at which they were being destroyed by annihilation. So most of the electrons and antielectrons</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">would have annihilated with each other to produce more photons, leaving only a few electrons left over. The</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">neutrinos and antineutrinos, however, would not have annihilated with each other, because these particles interact</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">with themselves and with other particles only very weakly. So they should still be around today. If we could observe</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">them, it would provide a good test of this picture of a very hot early stage of the universe. Unfortunately, their</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;">energies nowadays would be too low for us to observe them directly.</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhntHpnGfy7A4rVnLTCCWpRgXvfc0PCbtMqbz7NuOsEnyWGR8WQ2yPrQqdLM0BSk7PfDwqShaknlXoSPlppOim_Hg7__ClLtpZXSBbs43M1h2cFxOYjffRo_yPbAileQBeo3pB73BBnV7I/s1600/images+(3).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhntHpnGfy7A4rVnLTCCWpRgXvfc0PCbtMqbz7NuOsEnyWGR8WQ2yPrQqdLM0BSk7PfDwqShaknlXoSPlppOim_Hg7__ClLtpZXSBbs43M1h2cFxOYjffRo_yPbAileQBeo3pB73BBnV7I/s1600/images+(3).jpg" /></a></div>
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<span style="font-family: Arial, sans-serif;"><span style="font-size: 15px;"><br /></span></span></div>
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</div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">If neutrinos are not massless, but<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">have a small mass of their own, as
suggested by some recent experiments, we might be able to detect them<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">indirectly: they could be a form of “dark
matter,” like that mentioned earlier, with sufficient gravitational attraction
to<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">stop
the expansion of the universe and cause it to collapse again.<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;"><br /></span></div>
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</div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">Within only a few hours of the big
bang, the production of helium and other elements would have stopped. And after<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">that, for the next million years or
so, the universe would have just continued expanding, without anything much<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">happening. Eventually, once the
temperature had dropped to a few thousand degrees, and electrons and nuclei no<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">longer had enough energy to overcome
the electromagnetic attraction between them, they would have started<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">combining to form atoms. The universe
as a whole would have continued expanding and cooling, but in regions that<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">were slightly denser than average, the
expansion would have been slowed down by the extra gravitational attraction.<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">This would eventually stop expansion
in some regions and cause them to start to recollapse. As they were<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">collapsing, the gravitational pull of
matter outside these regions might start them rotating slightly. As the
collapsing<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">region got smaller, it would spin
faster – just as skaters spinning on ice spin faster as they draw in their
arms.<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">Eventually, when the region got small
enough, it would be spinning fast enough to balance the attraction of gravity,<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">and in this way disklike rotating
galaxies were born. Other regions, which did not happen to pick up a rotation,
would<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">become oval-shaped objects called
elliptical galaxies. In these, the region would stop collapsing because
individual<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">parts
of the galaxy would be orbiting stably round its center, but the galaxy would
have no overall rotation.<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;"><br /></span></div>
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</div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">the hydrogen and helium gas in the
galaxies would break up into smaller clouds that would collapse<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">under their own gravity. As these
contracted, and the atoms within them collided with one another, the
temperature<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">of the gas would increase, until
eventually it became hot enough to start nuclear fusion reactions. These would<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">convert the hydrogen into more helium,
and the heat given off would raise the pressure, and so stop the clouds from<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">contracting any further. They would
remain stable in this state for a long time as stars like our sun, burning
hydrogen<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">into helium and radiating the resulting
energy as heat and light. More massive stars would need to be hotter to<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">balance their stronger gravitational
attraction, making the nuclear fusion reactions proceed so much more rapidly
that<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">they would use up their hydrogen in as
little as a hundred million years. They would then contract slightly, and as<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">they
heated up further, would start to convert helium into heavier elements like
carbon or oxygen.<o:p></o:p></span></div>
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<br /></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; margin-left: 0in; margin-right: 0in; margin-top: 12pt;">
</div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">The outer regions of the star may
sometimes get blown off in a<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">tremendous explosion called a
supernova, which would outshine all the other stars in its galaxy. Some of the
heavier<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">elements produced near the end of the
star’s life would be flung back into the gas in the galaxy, and would provide<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">some of the raw material for the next
generation of stars. Our own sun contains about 2 percent of these heavier<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">elements, because it is a second- or
third-generation star, formed some five thousand million years ago out of a<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">cloud of rotating gas containing the
debris of earlier supernovas. Most of the gas in that cloud went to form the
sun or<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">got blown away, but a small amount of
the heavier elements collected together to form the bodies that now orbit the<o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;">sun
as planets like the earth.<o:p></o:p></span></div>
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<br /></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 11.5pt;"> (from :- </span><span style="font-family: Arial, sans-serif; font-size: 9pt; line-height: 115%;">A Brief History of Time - Stephen Hawking )</span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 9.0pt; line-height: 115%;"><o:p></o:p></span></div>
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<span style="font-family: "Arial","sans-serif"; font-size: 9.0pt; line-height: 115%;"><o:p></o:p></span></div>
</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-48392772986543755582012-03-24T03:51:00.000+05:302012-03-24T03:51:10.887+05:30Happy Navratri<div dir="ltr" style="text-align: left;" trbidi="on">
<br />
<div class="MsoNormal">
N : nav chetna</div>
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A : akhand jyoti</div>
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</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-33842558960938022582012-01-11T00:47:00.000+05:302012-01-11T00:47:15.502+05:30Farthest Developing Galaxy Cluster Ever Found<div dir="ltr" style="text-align: left;" trbidi="on">
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"> Using NASA's Hubble Space Telescope, astronomers have uncovered a cluster of galaxies in the initial stages of development. It is the most distant such grouping ever observed in the early universe.</span>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><br /></span><br />
<a href="http://www.sciencedaily.com/images/2012/01/120110114332-large.jpg" rel="thumbnail" style="background-color: white; color: #000099; font-family: Arial, Helvetica, sans-serif; font-size: 13px; line-height: 15px; text-decoration: none;"><img alt="" border="0" height="212" src="http://www.sciencedaily.com/images/2012/01/120110114332.jpg" width="300" /></a><br />
<div id="caption" style="background-color: white; font-family: Arial, Helvetica, sans-serif; font-size: 13px; line-height: 15px; padding-bottom: 10px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
<em>he composite image at left, taken in visible and near-infrared light, reveals the location of five tiny galaxies clustered together 13.1 billion light-years away. The circles pinpoint the galaxies. The sharp-eyed Wide Field Camera 3 aboard NASA's Hubble Space Telescope spied the galaxies in a random sky survey. The developing cluster is the most distant ever observed. The young galaxies lived just 600 million years after the universe's birth in the big bang. (Credit: NASA, ESA, M. Trenti (University of Colorado, Boulder, and Institute of Astronomy, University of Cambridge, UK), L. Bradley (STScI), and the BoRG team)</em></div>
<div id="caption" style="background-color: white; font-family: Arial, Helvetica, sans-serif; font-size: 13px; line-height: 15px; padding-bottom: 10px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
<em><br /></em></div>
<div id="caption" style="background-color: white; font-family: Arial, Helvetica, sans-serif; font-size: 13px; line-height: 15px; padding-bottom: 10px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
In a random sky survey made in near-infrared light, Hubble found five tiny galaxies clustered together 13.1 billion light-years away. They are among the brightest galaxies at that epoch and very young — existing just 600 million years after the big bang.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
Galaxy clusters are the largest structures in the universe, comprising hundreds to thousands of galaxies bound together by gravity. The developing cluster, or protocluster, is seen as it looked 13 billion years ago. Presumably, it has grown into one of today's massive galactic cities, comparable to the nearby Virgo cluster of more than 2,000 galaxies.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
"These galaxies formed during the earliest stages of galaxy assembly, when galaxies had just started to cluster together," said Michele Trenti of the University of Colorado at Boulder and the Institute of Astronomy at the University of Cambridge in the United Kingdom. "The result confirms our theoretical understanding of the buildup of galaxy clusters. And, Hubble is just powerful enough to find the first examples of them at this distance."</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
Trenti presented the results today at the American Astronomical Society meeting in Austin, Texas. The study will be published in an upcoming issue of <i>The Astrophysical Journal</i>.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
Most galaxies in the universe reside in groups and clusters, and astronomers have probed many mature galactic cities in detail as far as 11 billion light-years away. Finding clusters in the early phases of construction has been challenging because they are rare, dim and widely scattered across the sky.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
"We need to look in many different areas because the odds of finding something this rare are very small," said Trenti, who used Hubble's sharp-eyed Wide Field Camera 3 (WFC3) to pinpoint the cluster galaxies. "It's like playing a game of Battleship: the search is hit and miss. Typically, a region has nothing, but if we hit the right spot, we can find multiple galaxies."</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
Because the distant, fledgling clusters are so dim, the team hunted for the systems' brightest galaxies. These galaxies act as billboards, advertising cluster construction zones. From simulations, the astronomers expect galaxies at early epochs to be clustered together. Because brightness correlates with mass, the most luminous galaxies pinpoint the location of developing clusters. These powerful light beacons live in deep wells of dark matter, an invisible form of matter that makes up the underlying gravitational scaffolding for construction. The team expects many fainter galaxies that were not seen in these observations to inhabit the same neighborhood.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
The five bright galaxies spotted by Hubble are about one-half to one-tenth the size of our Milky Way, yet are comparable in brightness. The galaxies are bright and massive because they are being fed large amounts of gas through mergers with other galaxies. The team's simulations show that the galaxies will eventually merge and form the brightest central galaxy in the cluster, a giant elliptical similar to the Virgo Cluster's M87.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
These observations demonstrate the progressive buildup of galaxies. They also provide further support for the hierarchical model of galaxy assembly, in which small objects accrete mass, or merge, to form bigger objects over a smooth and steady but dramatic process of collision and collection.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
The observations are part of the Brightest of Reionizing Galaxies survey, which uses Hubble's WFC3 to search for the brightest galaxies around 13 billion years ago, when light from the first stars burned off a fog of cold hydrogen in a process called reionization.</div>
<div style="padding-bottom: 5px; padding-left: 0px; padding-right: 0px; padding-top: 5px;">
The team estimated the distance to the newly found galaxies based on their colors, but the astronomers plan to follow up with spectroscopic observations, which measure the expansion of space. Those observations will help the astronomers precisely calculate the cluster's distance and also will yield the velocities of the galaxies, which will show whether they are gravitationally bound to each other.</div>
</div>
</div>Anonymoushttp://www.blogger.com/profile/02607626611741180436noreply@blogger.com0tag:blogger.com,1999:blog-3038278470848839486.post-40982166541807032412012-01-11T00:30:00.001+05:302012-01-11T00:30:20.669+05:30LOSE/GAIN WEIGHT<div dir="ltr" style="text-align: left;" trbidi="on">
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