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	<title>Science Today &#187; radiation</title>
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		<title>Black Hole Bonanza</title>
		<link>http://www.calacademy.org/sciencetoday/black-hole-bonanza/5511311/</link>
		<comments>http://www.calacademy.org/sciencetoday/black-hole-bonanza/5511311/#comments</comments>
		<pubDate>Sat, 22 Jun 2013 02:05:38 +0000</pubDate>
		<dc:creator>molly</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[Top Story]]></category>
		<category><![CDATA[andromeda]]></category>
		<category><![CDATA[black hole]]></category>
		<category><![CDATA[bonanza]]></category>
		<category><![CDATA[bulge]]></category>
		<category><![CDATA[chandra]]></category>
		<category><![CDATA[globular cluster]]></category>
		<category><![CDATA[milky way]]></category>
		<category><![CDATA[nasa]]></category>
		<category><![CDATA[observatory]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[sister galaxy]]></category>
		<category><![CDATA[x-ray]]></category>

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		<description><![CDATA[What does it mean when we confirm that Andromeda is host to a “black hole bonanza”?]]></description>
				<content:encoded><![CDATA[<p><span style="color: #888888;"><strong>By Alyssa Keimach</strong></span></p>
<p>Astronomers often describe <a href="http://www.nasa.gov/mission_pages/chandra/multimedia/bonanza_image.html">Andromeda</a> as a “sister galaxy” to our own <a href="http://www.nasa.gov/mission_pages/GLAST/science/milky_way_galaxy.html">Milky Way</a>. It is relatively nearby, similarly sized, and comparably shaped. So what does it mean when we confirm that Andromeda is host to a “black hole bonanza”?</p>
<p>A <a href="http://science.nasa.gov/astrophysics/focus-areas/black-holes/">black hole</a> is born when a massive star collapses, resulting in a high concentration of gravity, so strong that light cannot even escape its pull. By definition, we can’t observe black holes directly, but astronomers can <a href="http://www.space.com/3457-tricky-task-detecting-black-holes.html">detect them</a> if a close-orbiting star is pulled inside. Gravitational forces <a href="http://en.wikipedia.org/wiki/Accretion_disc">compress the star’s material</a>, producing high-energy radiation in the process.</p>
<p>NASA’s <a href="http://www.nasa.gov/mission_pages/chandra/main/index.html">Chandra X-ray observatory</a> followed the radiation trail to identify 26 new black hole candidates, the largest number found outside of the Milky Way to date. Follow-up observations by the European Space Agency’s <a href="http://xmm.esac.esa.int/">XMM-Newton X-ray observatory</a> gave information useful for determining the nature of these black holes.</p>
<p>The first step in classifying Chandra’s findings: confirm the black hole sizes and locations. The process relies on perspective. In the same way a tall person standing far away can appear the same size as a short person much closer, objects in space can deceive us with their apparent size, so we need to look for additional clues. In the case of black holes, researchers saw bright and fast variability of <a href="http://www.mpa-garching.mpg.de/HIGHLIGHT/2003/highlight0304_e.html">X-ray emission</a> to determine these 26 black holes are smaller “<a href="http://www.nasa.gov/mission_pages/chandra/multimedia/igr.html">stellar mass</a>” systems <i>within</i> Andromeda rather than supermassive black holes <i>behind</i> Andromeda.</p>
<p>As it turns out, <a href="http://imagine.gsfc.nasa.gov/docs/science/know_l1/pulsars.html">neutron stars</a> can look a lot like black holes from a distance, so researchers analyzed x-ray brightness and color. Neutron stars also emit x-ray radiation, but a black hole appears brighter—and a different color.</p>
<p>Eight of the black holes reside in <a href="http://hyperphysics.phy-astr.gsu.edu/hbase/astro/globular.html">globular clusters</a>, concentrations of stars spherically distributed about the center of a galaxy that exist in both the Milky Way and Andromeda. However, astronomers have not yet discovered black holes in any of the Milky Way’s globular clusters.</p>
<p>“When it comes to finding black holes in the central region of a galaxy, it is indeed the case where bigger is better,” said co-author <a href="http://hea-www.harvard.edu/~ssm/">Stephen Murray</a> of Johns Hopkins University and the Harvard-Smithsonian Center for Astrophysics (CfA). “In the case of Andromeda, we have a bigger bulge and a bigger supermassive black hole than in the Milky Way, so we expect more smaller black holes are made there as well.”</p>
<p>Perhaps the two galaxies aren’t as sisterly as we thought. The central <a href="http://en.wikipedia.org/wiki/Bulge_(astronomy)">bulge</a> of Andromeda is larger, which explains why seven of the new candidates exist within 1,000 light years of Andromeda’s core.</p>
<p>Considering that we can only detect black holes when they are producing high-energy radiation, there must be more that we have not found yet—in both galaxies. Lead author <a href="http://www.robinbarnard.com/">Robin Barnard</a> of CfA states, “While we are excited to find so many black holes in Andromeda, we think it’s just the tip of the iceberg, most black holes won’t have close companions and will be invisible to us.”</p>
<p><span style="color: #888888;"><strong>Alyssa Keimach is an astronomy and astrophysics student at the University of Michigan and interns </strong><strong>for the </strong></span><a href="http://www.calacademy.org/academy/exhibits/planetarium/"><strong>Morrison Planetarium</strong></a><strong>.</strong></p>
<p><em>Image: NASA/JPL-Caltech/UCLA</em></p>
<img width="110" height="62" src="http://www.calacademy.org/sciencetoday/wp-content/uploads/2013/06/427006main_pia12832-c516-110x62.jpg" class="attachment-110x62 wp-post-image" alt="andromeda, sister galaxy, milky way, black hole, bonanza, chandra, x-ray, nasa, observatory, radiation, globular cluster, bulge" />]]></content:encoded>
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		<title>Japanese Heroes</title>
		<link>http://www.calacademy.org/sciencetoday/japanese-heroes/554089/</link>
		<comments>http://www.calacademy.org/sciencetoday/japanese-heroes/554089/#comments</comments>
		<pubDate>Tue, 22 Mar 2011 23:18:24 +0000</pubDate>
		<dc:creator>molly</dc:creator>
				<category><![CDATA[Life]]></category>
		<category><![CDATA[Technology]]></category>
		<category><![CDATA[Top Story]]></category>
		<category><![CDATA[earthquake]]></category>
		<category><![CDATA[fukushima]]></category>
		<category><![CDATA[Japan]]></category>
		<category><![CDATA[nuclear energy]]></category>
		<category><![CDATA[radiation]]></category>

		<guid isPermaLink="false">http://www.calacademy.org/sciencetoday/?p=4089</guid>
		<description><![CDATA[The workers at the Fukushima plant are risking their own lives saving others.]]></description>
				<content:encoded><![CDATA[<p>As reports from <a href="http://blogs.nature.com/news/thegreatbeyond/2011/03/first_estimates_of_radioactive.html"><em>Nature</em></a>, <a href="http://www.npr.org/2011/03/22/134755614/Japan-Nuclear-Power-Development">NPR</a> and <a href="http://www.scientificamerican.com/article.cfm?id=radiation-risks-unknown">others</a> surface today about lower radiation risks from the crippled Fukushima Daiichi nuclear plant in Japan, the long-term effects, especially for those who work at the plant, are unknown. But it’s these workers who are responsible for keeping this disaster under control.</p>
<p>According to <a href="http://news.nationalgeographic.com/news/2011/03/110317-japan-reactor-fukushima-nuclear-power-plant-radiation-exposure/"><em>National Geographic</em></a>, as of last week there were about 330 workers at the plant, working in fifteen-minute shifts to keep from getting sick. <a href="http://www.npr.org/2011/03/18/134665531/nuclear-workers-take-risks-for-the-public-good">NPR</a> reports that:</p>
<p style="padding-left: 30px;">So far, at least 15 of these workers have been injured by explosions. An additional 17 have suffered what the Japanese government called &#8220;deposition of radioactive material&#8221; to their faces. Two are missing.</p>
<p>How much radiation are they being exposed to? It’s hard to say. But an article in <a href="http://www.nature.com/news/2011/110322/full/471419a.html"><em>Nature News</em></a><em> </em>identifies that:</p>
<p style="padding-left: 30px;">The [Japanese] government has increased the allowable dose for workers from 100 milli­sieverts per year to 250 millisieverts per year — five times the annual allowable dose for US radiation workers — to allow emergency operations to continue. This dose is considered by the US National Institutes of Health as the lower limit for the first symptoms of radiation sickness.</p>
<p>Millisieverts are the standard by which radiation is measured. For reference, <a href="http://news.nationalgeographic.com/news/2011/03/110317-japan-reactor-fukushima-nuclear-power-plant-radiation-exposure/"><em>National Geographic</em></a><em> </em>shares that:</p>
<p style="padding-left: 30px;">…the average person receives about one to two millisieverts a year from natural sources in their environments, and one chest x-ray yields about 0.2 millisievert.</p>
<p>As the viral, must-see <a href="http://www.youtube.com/watch?v=5sakN2hSVxA">Nuclear Boy</a>, states on YouTube, these workers are really “stepping up to the plate.” (The YouTube video explains the disaster very clearly through a stinky metaphor, in which the Fukushima workers are doctors taking turns caring for Nuclear Boy. Watch it, if you haven’t.)<em> </em></p>
<p>Not only are they risking their lives, in the process, they are making excellent, life-saving decisions. From <a href="http://www.nature.com/news/2011/110322/full/471417a.html"><em>Nature News</em></a><em>:</em></p>
<p style="padding-left: 30px;">And already it is clear that decisions made in the initial 24 hours by the handful of operators in the control room probably averted a much greater nuclear catastrophe than the one that now faces Japan.</p>
<p style="padding-left: 30px;">
<p><em>Fukushima Unit I Visualization by <a title="User:Nesnad" href="http://commons.wikimedia.org/wiki/User:Nesnad">Nesnad</a><span style="color: #ffffff;">/Wikimedia</span></em></p>
<img width="110" height="62" src="http://www.calacademy.org/sciencetoday/wp-content/uploads/2011/03/Hydrogen_explosion_Fukushima_Unit_1_cg_visualization-110x62.jpg" class="attachment-110x62 wp-post-image" alt="Hydrogen_explosion_Fukushima_Unit_1_cg_visualization" />]]></content:encoded>
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