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A Step in the Right Direction
Solar Child
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10-12-2007 11:04 AM
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cosmi rays
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rxj1713.7-3946
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<div style="margin: 12px 0px; font-family: arial; color: #333333; background: #ffffff; border: solid 4px #e5e5e5; width: 100%; clear: left;"><div class="CM_CTB_Content_Wrap" style="margin: 0px; padding: 0px;background-color: #ffffff;"><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://www.clipmarks.com/images/source-bg.gif); background-repeat: repeat-x; height: 24px; line-height: 24px; vertical-align: middle; padding-bottom: 4px; color: #666666; font-size: 10px;" ><a href="http://clipmarks.com/clip-to-blog/" title="see clips that are hot right now"><img src="http://content.clipmarks.com/blog_embed/959d40a2-6238-4939-8a60-a177f4d7d73e/BFF61DBE-8ACD-495F-89E5-346111190CAF/" alt="" width="19" height="19" border="0" style="vertical-align: middle; margin: 0px 4px; display: inline; border: none; float:none;" /></a>clipped from <a title="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html" href="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html" style="font-size: 11px;">www.space.com</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html"><B>Origin of Cosmic Rays Confirmed </B></blockquote><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://www.clipmarks.com/images/source-bg.gif); background-repeat: repeat-x; height: 24px; line-height: 24px; vertical-align: middle; padding-bottom: 4px; color: #666666; font-size: 10px;" ><a href="http://clipmarks.com/clip-to-blog/" title="see clips that are hot right now"><img src="http://content8.clipmarks.com/images/clip-icon.gif" alt="" width="19" height="19" border="0" style="vertical-align: middle; margin: 0px 4px; display: inline; border: none; float:none;" /></a>clipped from <a title="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-x-ray-02.jpg&cap=NASA%27s+Chandra+X-ray+Observatory+image+shows+the+edge+of+RXJ1713.7-3946%2C+a+supernova+remnant.+On+the+right%2C+X-ray+hot+spots+are+appearing+and+disappearing.+The+rapid+rise+and+fall+of+the+spots+indicate+that+electrons+are+being+accelerated+to+near-light+speed+in+the+presence+of+strong+magnetic+fields.+Credit%3A+CXC%2FYasunobu+Uchiyama%2FHESS%2FNature" href="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-x-ray-02.jpg&cap=NASA%27s+Chandra+X-ray+Observatory+image+shows+the+edge+of+RXJ1713.7-3946%2C+a+supernova+remnant.+On+the+right%2C+X-ray+hot+spots+are+appearing+and+disappearing.+The+rapid+rise+and+fall+of+the+spots+indicate+that+electrons+are+being+accelerated+to+near-light+speed+in+the+presence+of+strong+magnetic+fields.+Credit%3A+CXC%2FYasunobu+Uchiyama%2FHESS%2FNature" style="font-size: 11px;">www.space.com</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-x-ray-02.jpg&cap=NASA%27s+Chandra+X-ray+Observatory+image+shows+the+edge+of+RXJ1713.7-3946%2C+a+supernova+remnant.+On+the+right%2C+X-ray+hot+spots+are+appearing+and+disappearing.+The+rapid+rise+and+fall+of+the+spots+indicate+that+electrons+are+being+accelerated+to+near-light+speed+in+the+presence+of+strong+magnetic+fields.+Credit%3A+CXC%2FYasunobu+Uchiyama%2FHESS%2FNature"><div align="center"><img src="http://content9.clipmarks.com/blog_cache/www.space.com/img/4785056F-B6BC-468F-98B7-43815ECEC437" alt="" /></div></blockquote><div style="height: 2px; font-size: 2px; background: #dcdcdc; border-bottom: solid 1px #f5f5f5; margin: 2px 4px;"></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-x-ray-02.jpg&cap=NASA%27s+Chandra+X-ray+Observatory+image+shows+the+edge+of+RXJ1713.7-3946%2C+a+supernova+remnant.+On+the+right%2C+X-ray+hot+spots+are+appearing+and+disappearing.+The+rapid+rise+and+fall+of+the+spots+indicate+that+electrons+are+being+accelerated+to+near-light+speed+in+the+presence+of+strong+magnetic+fields.+Credit%3A+CXC%2FYasunobu+Uchiyama%2FHESS%2FNature"><FONT size="2" face="arial" color="#000000">NASA's Chandra X-ray Observatory image shows the edge of RXJ1713.7-3946, a supernova remnant. On the right, X-ray hot spots are appearing and disappearing. The rapid rise and fall of the spots indicate that electrons are being accelerated to near-light speed in the presence of strong magnetic fields. Credit: CXC/Yasunobu Uchiyama/HESS/Nature</FONT></blockquote><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://www.clipmarks.com/images/source-bg.gif); background-repeat: repeat-x; height: 24px; line-height: 24px; vertical-align: middle; padding-bottom: 4px; color: #666666; font-size: 10px;" ><a href="http://clipmarks.com/clip-to-blog/" title="see clips that are hot right now"><img src="http://content6.clipmarks.com/images/clip-icon.gif" alt="" width="19" height="19" border="0" style="vertical-align: middle; margin: 0px 4px; display: inline; border: none; float:none;" /></a>clipped from <a title="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-supernova-02.jpg&cap=An+image+from+Japan%27s+Suzaku+X-ray+observatory+shows+RXJ1713.7-3946%2C+which+is+a+supernova+remnant%E2%80%94the+gaseous+remnant+of+a+massive+star+that+exploded.+The+remnant+is+about+1%2C600+years+old.+The+contour+lines+show+where+gamma-ray+intensity+is+highest%2C+as+measured+by+the+High+Energy+Stereoscopic+System+%28HESS%29+in+Namibia.+Credit%3A+JAXA%2FTakaaki+Tanaka%2FHESS" href="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-supernova-02.jpg&cap=An+image+from+Japan%27s+Suzaku+X-ray+observatory+shows+RXJ1713.7-3946%2C+which+is+a+supernova+remnant%E2%80%94the+gaseous+remnant+of+a+massive+star+that+exploded.+The+remnant+is+about+1%2C600+years+old.+The+contour+lines+show+where+gamma-ray+intensity+is+highest%2C+as+measured+by+the+High+Energy+Stereoscopic+System+%28HESS%29+in+Namibia.+Credit%3A+JAXA%2FTakaaki+Tanaka%2FHESS" style="font-size: 11px;">www.space.com</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-supernova-02.jpg&cap=An+image+from+Japan%27s+Suzaku+X-ray+observatory+shows+RXJ1713.7-3946%2C+which+is+a+supernova+remnant%E2%80%94the+gaseous+remnant+of+a+massive+star+that+exploded.+The+remnant+is+about+1%2C600+years+old.+The+contour+lines+show+where+gamma-ray+intensity+is+highest%2C+as+measured+by+the+High+Energy+Stereoscopic+System+%28HESS%29+in+Namibia.+Credit%3A+JAXA%2FTakaaki+Tanaka%2FHESS"><div align="center"><img src="http://content7.clipmarks.com/blog_cache/www.space.com/img/2C28B1B9-C9BC-400C-AFC5-0FD7629EFB80" alt="" /></div></blockquote><div style="height: 2px; font-size: 2px; background: #dcdcdc; border-bottom: solid 1px #f5f5f5; margin: 2px 4px;"></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=071010-chandra-supernova-02.jpg&cap=An+image+from+Japan%27s+Suzaku+X-ray+observatory+shows+RXJ1713.7-3946%2C+which+is+a+supernova+remnant%E2%80%94the+gaseous+remnant+of+a+massive+star+that+exploded.+The+remnant+is+about+1%2C600+years+old.+The+contour+lines+show+where+gamma-ray+intensity+is+highest%2C+as+measured+by+the+High+Energy+Stereoscopic+System+%28HESS%29+in+Namibia.+Credit%3A+JAXA%2FTakaaki+Tanaka%2FHESS"><FONT size="2" face="arial" color="#000000">An image from Japan's Suzaku X-ray observatory shows RXJ1713.7-3946, which is a supernova remnant—the gaseous remnant of a massive star that exploded. The remnant is about 1,600 years old. The contour lines show where gamma-ray intensity is highest, as measured by the High Energy Stereoscopic System (HESS) in Namibia. Credit: JAXA/Takaaki Tanaka/HESS</FONT></blockquote><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://www.clipmarks.com/images/source-bg.gif); background-repeat: repeat-x; height: 24px; line-height: 24px; vertical-align: middle; padding-bottom: 4px; color: #666666; font-size: 10px;" ><a href="http://clipmarks.com/clip-to-blog/" title="see clips that are hot right now"><img src="http://content8.clipmarks.com/images/clip-icon.gif" alt="" width="19" height="19" border="0" style="vertical-align: middle; margin: 0px 4px; display: inline; border: none; float:none;" /></a>clipped from <a title="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html" href="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html" style="font-size: 11px;">www.space.com</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/scienceastronomy/071010-cosmic-ray-origin.html"><SPAN>To make the discovery, Uchiyama and his team focused NASA's <A href="http://www.space.com/php/multimedia/imagegallery/igviewer.php?imgid=3088&gid=232">Chandra telescope</A> on X-ray hot spots in a supernova remnant called RXJ1713.7-3946, located a few thousand light-years from Earth in the constellation Scorpius.</SPAN></blockquote></div><div style="margin: 0px 6px 6px 4px;"><table style="font-size: 11px;border-spacing: 0px;padding: 0px;" cellpadding="0" cellspacing="0" width="100%"><tr><td style="background:transparent;border-width:0px;padding:0px;"> </td><td align="right" style="background:transparent;border-width:0px;padding:0px;width:107px" width="107"><a href="http://clipmarks.com/share/BFF61DBE-8ACD-495F-89E5-346111190CAF/blog/" title="blog or email this clip"><img src="http://content9.clipmarks.com/images/c2b-foot.png" border="0" alt="blog it" width="107" height="17" style="border-width:0px;padding:0px;margin:0px;" /></a></td></tr></table></div></div>
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