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	<title>Sepientia &#187; black holes</title>
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		<title>Black holes do join together</title>
		<link>http://sepientia.com/2009/07/black-holes-do-join-together/</link>
		<comments>http://sepientia.com/2009/07/black-holes-do-join-together/#comments</comments>
		<pubDate>Sat, 25 Jul 2009 15:07:14 +0000</pubDate>
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				<category><![CDATA[Science]]></category>
		<category><![CDATA[Space]]></category>
		<category><![CDATA[black holes]]></category>

		<guid isPermaLink="false">http://sepientia.com/?p=33</guid>
		<description><![CDATA[Planetary scientists have found the first solid evidence for a moderate-size black hole in a distant galaxy, backing up the idea that smaller black holes merge into huge ones.
A black hole is an object with such a powerful gravitational field that it absorbs all the light that passes near it and reflects nothing.
Until now, identified [...]]]></description>
			<content:encoded><![CDATA[<p><img class="alignleft size-thumbnail wp-image-34" title="Black_Hole_01" src="http://sepientia.com/wp-content/uploads/2009/07/Black_Hole_01-150x150.jpg" alt="Black_Hole_01" width="150" height="150" /><span style="color: #000000;">Planetary scientists have found the first solid evidence for a moderate-size black hole in a distant galaxy, backing up the idea that smaller black holes merge into huge ones.</span></p>
<p><span style="color: #000000;">A black hole is an object with such a powerful gravitational field that it absorbs all the light that passes near it and reflects nothing.</span></p>
<p><span style="color: #000000;">Until now, identified black holes have been either super-massive (several million to several billion times the mass of the Sun) in the centre of galaxies, or about the size of a typical star (between three and 20 Solar masses).</span></p>
<p><span style="color: #000000;">Now, an international team has discovered the black hole HLX-1, 290 million light years from Earth, which it is more than 500 times the mass of the Sun, using the European Space Agency&#8217;s telescope.</span></p>
<p><span style="color: #000000;"><span id="more-33"></span></span><span style="color: #000000;">Team member Dr Sean Farrell of the University of Leicester said: &#8220;While it is widely accepted that stellar mass black holes are created during death throes of massive stars, it is still unknown how super-massive black holes are formed.</span></p>
<p><span style="color: #000000;">&#8220;One theory is that super-massive black holes may be formed by the merger of a number of intermediate mass black holes. To ratify such a theory, however, you must first prove the existence of intermediate black holes.</span></p>
<p><span style="color: #000000;">&#8220;The identification of HLX-1 is therefore an important step towards a better understanding of the formation of the super-massive black holes that exist at the centre of the Milky Way and other galaxies.&#8221;</span></p>
<p><span style="color: #000000;">In fact, the HLX-1 (Hyper-Luminous X-ray source 1) lies towards the edge of the galaxy ESO 243-49. It is ultra- luminous in X-rays, with a maximum X-ray brightness of approximately 260 million times that of the Sun.</span></p>
<p><span style="color: #000000;">The X-ray signature of HLX-1 and the lack of a counterpart in optical images confirm that it is neither a foreground star nor a background galaxy, and its position indicates that it is not the central engine of that galaxy.</span></p>
<p><span style="color: #000000;">And, using XMM-Newton observations carried out on the 23rd November 2004 and the 28th November 2008, the team showed that HLX-1 displayed a variation in its X-ray signature. This indicated that it must be a single object and not a group of many fainter sources.</span></p>
<p><span style="color: #000000;">The huge radiance observed can only be explained if HLX-1 contains a black hole more than 500 times the mass of the Sun. No other physical explanation can account for the data.</span></p>
<p><span style="color: #000000;">source: </span><a href="http://www.discoveryon.info/">http://www.discoveryon.info/</a></p>
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