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	<title>The World's Greatest Japanese &#187; astronomy</title>
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	<link>http://www.japanese-greatest.com</link>
	<description>The wonderful things in which Japan is number one in the world.</description>
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		<title>A planetarium that can project the most stars &#8211; MEGASTAR by Takayuki Ohira</title>
		<link>http://www.japanese-greatest.com/astronomy/megastar.html</link>
		<comments>http://www.japanese-greatest.com/astronomy/megastar.html#comments</comments>
		<pubDate>Mon, 19 May 2008 14:44:36 +0000</pubDate>
		<dc:creator>nolitenn</dc:creator>
				<category><![CDATA[astronomy]]></category>

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		<description><![CDATA[In July 2004, Takayuki Ohira's "MEGASTAR" was established permanently in the National Museum of Emerging Science and Innovation. It can project a total of five million stars that would otherwise be too far to see, at a magnitude of up to 12.5 times their size.]]></description>
			<content:encoded><![CDATA[<p>In July 2004, Takayuki Ohira&#8217;s &#8220;MEGASTAR&#8221; was established permanently in the National Museum of Emerging Science and Innovation. It can project a total of five million stars that would otherwise be too far to see, at a magnitude of up to 12.5 times their size.<span id="more-110"></span></p>
<p>In 1998, another &#8220;MEGASTAR&#8221;, a lens-type planetarium, opened to the public in London. It projected 1.7 million stars. That record has, of course, been broken.</p>
<p>In 2005, &#8220;HOMESTAR&#8221; was developed in cooperation with SEGA TOYS for the first time in the world, and uses a domestic optical system. It can project 10,000 stars (of which 8,600 are invisible to the naked eye) up to 6.5 times their size.</p>
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		<title>Subaru: The largest optical telescope in the world, owned by the National Astronomical Observatory</title>
		<link>http://www.japanese-greatest.com/astronomy/telescope-subaru.html</link>
		<comments>http://www.japanese-greatest.com/astronomy/telescope-subaru.html#comments</comments>
		<pubDate>Sun, 18 May 2008 13:02:33 +0000</pubDate>
		<dc:creator>nolitenn</dc:creator>
				<category><![CDATA[astronomy]]></category>

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		<description><![CDATA[In 1998, a large scale, optical infrared telescope, named "Subaru", was established at the top of Mt. Mauna Kea in Hawaii Island by the National Astronomical Observatory.]]></description>
			<content:encoded><![CDATA[<p>In 1998, a large scale, optical infrared telescope, named &#8220;Subaru&#8221;, was established at the top of Mt. Mauna Kea in Hawaii Island by the National Astronomical Observatory.<span id="more-109"></span></p>
<p>Its diameter is 8.3m and, being a one-piece mirror, is the largest in the world; so big, in fact, that it takes 7 years to polish. Subaru&#8217;s average margin of error is 12mm. Its accuracy is so good that it can be used to see a ball at the top of Mt. Fuji from the center of Tokyo. Subaru has 261 actuators on the back side of the reflector to control movement.</p>
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		<title>Discovery of a primitive galaxy almost as large as the Milky Way Galaxy</title>
		<link>http://www.japanese-greatest.com/astronomy/primitive-galaxy.html</link>
		<comments>http://www.japanese-greatest.com/astronomy/primitive-galaxy.html#comments</comments>
		<pubDate>Fri, 25 Apr 2008 14:28:50 +0000</pubDate>
		<dc:creator>nolitenn</dc:creator>
				<category><![CDATA[astronomy]]></category>

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		<description><![CDATA[The National Astronomical Observatory of Japan and others (Koji Ohta and others of Kyoto University, Tohoku University and the University of Tokyo) discovered a primitive galaxy almost as large as the Milky Way Galaxy, and announced it in Nature Magazine, Aug. 1. 1996. Ohta, K., Yamada, T., Nakanishi, K., Kohno, K., Akiyama, M. and Kawabe, R., "Detection of Molecular Gas in the Quasar BR1202 - 0725 at Redshift z = 4.69" , Nature 382 (1996) 426]]></description>
			<content:encoded><![CDATA[<p>The <span class="vcard"><a target="_blank" href="http://www.nao.ac.jp/E/" title="National Astronomical Observatory of Japan" class="url fn org">National Astronomical Observatory of Japan</a></span> (<span class="vcard"><a target="_blank" href="http://www.nao.ac.jp/" title="国立天文台" class="url fn org">国立天文台</a></span>) and others (<span class="vcard"><cite class="fn n"><span class="given-name">Koji</span> <span class="family-name">Ohta</span></cite></span> and others of <span class="vcard"><a target="_blank" href="http://www.kyoto-u.ac.jp/" title="Kyoto University" class="url fn org">Kyoto University</a></span>, <span class="vcard"><a target="_blank" href="http://www.tohoku.ac.jp/" title="Tohoku University" class="url fn org">Tohoku University</a></span> and <span class="vcard"><a target="_blank" href="http://www.u-tokyo.ac.jp/" title="the University of Tokyo" class="url fn org">the University of Tokyo</a></span>) discovered a primitive galaxy almost as large as the Milky Way Galaxy, and announced it in Nature Magazine, Aug. 1. 1996. Ohta, K., Yamada, T., Nakanishi, K., Kohno, K., Akiyama, M. and Kawabe, R., &#8220;Detection of Molecular Gas in the Quasar BR1202 &#8211; 0725 at Redshift z = 4.69&#8243; , Nature 382 (1996) 426<span id="more-86"></span></p>
<p>One of the farthest heavenly bodies (z=4.7*), quasar BR1202-0725 was observed with the Nobeyama Millimeter Array at NRO Cosmic Radio Facilities, a division of the National Astronomical Observatory of Japan. It was confirmed to contain a large quantity of carbon monoxide molecules.</p>
<p>At quasar BR1202-0725, at a distance of 14 billion light-years, or one billion years after the Big Bang 15 billion years ago, hydrogen molecular gas and carbon monoxide molecule were found. Their mass is 100 billion times that of as the sun, and equal to the total mass of our Galaxy.</p>
<p>This discovery brought epoch-making progress to research into the process from our galaxies formative period to its maturity. For example, we now know that there was carbon and hydrogen made in a star, in a young (one billion years old) galaxy.</p>
<p>Thin interstellar gas and interstellar matter form a thick area and this forms an interstellar molecular cloud**, then a star results from gravitational contraction.</p>
<p>A supernova is the final stage of a star that reduces the component atoms to an interstellar gas and interstellar dust.  The next circulation of a star&#8217;s formation begins.</p>
<p>In order of quantity, there are hydrogen, helium, oxygen, and carbon in space. We know that carbon, the main component of known life, exists as a carbon ion in interstellar gas, and as carbon monoxide in an interstellar molecular cloud.</p>
<p>* Z is a sign to represent the amount of redshift: the degree of how long a wavelength of light gets longer by Doppler shift while heavenly bodies recede from our position.</p>
<p>** interstellar molecular cloud: very thin gas, about 10 hydrogen atoms per 1 cm3, extends between stars in the Galaxy.  There are high-density areas (100-10000 hydrogen atoms per 1cm3) here and there, which seem like clouds. These are called interstellar molecular clouds. They measure several, or dozens of parsecs, with an absolute temperature of about 10 Kelvin. Their mass is typically hundreds or tens of thousands of times that of the sun. An interstellar molecular cloud whose mass is more than hundreds of thousands of times that of the sun is considered an especially huge molecular cloud. Stars are formed in a particularly high-density part of an interstellar molecular cloud by gravitational contraction. The main ingredient of an interstellar molecular cloud is mostly the hydrogen molecule (H2), secondly the helium atom (He), then the carbon monoxide molecule (CO). The ratio of hydrogen molecules to carbon monoxide molecules is about 10000:1.</p>
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		<title>Discovery of the Visible Light Flare by Tomonori Totani</title>
		<link>http://www.japanese-greatest.com/astronomy/visible-light-flare.html</link>
		<comments>http://www.japanese-greatest.com/astronomy/visible-light-flare.html#comments</comments>
		<pubDate>Tue, 19 Feb 2008 16:08:24 +0000</pubDate>
		<dc:creator>tsukimidango</dc:creator>
				<category><![CDATA[astronomy]]></category>

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		<description><![CDATA[By Tomonori Totani: Assistant Professor(presently Associate Professor) at Department of Astronomy, Kyoto University , April 1, 2005

By a large scale search of the universe, a phenomenon that light flares will increase greatly in only several days has been discovered emanating from the center of a seemingly usual galaxy that exists at a distance of about four billion light years from the earth.]]></description>
			<content:encoded><![CDATA[<p>By Tomonori Totani: Assistant Professor(presently Associate Professor) at Department of Astronomy, Kyoto University , April 1, 2005</p>
<p>By a large scale search of the universe, a phenomenon that light flares will increase greatly in only several days has been discovered emanating from the center of a seemingly usual galaxy that exists at a distance of about four billion light years from the earth.<span id="more-16"></span></p>
<p>This radiation has come out from a gas disk that rotates around a huge black hole with a mass 100 million times larger than our sun. The gas disk is probably located 1 billion kilometers away from this massive black hole and rotates at a speed close to the speed of light.</p>
<p>This black hole is significantly larger than the black hole that is at the center of our galaxy and the black hole at the centre of our galaxy has a mass 3 million times larger than the mass of our sun.</p>
<p>This is the first time that the intense activity of the visible light region has been discovered from such a black hole.</p>
<p>The thought that there is a large black hole at the core of all galaxies in the universe is becoming the mainstream now, and the result of this discovery mentioned above supports this thought.</p>
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