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	<title>Supernova Women &#8211; Suitto Eyewear</title>
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		<title>WEI</title>
		<link>https://suittoeyewear.com/en/modelo/wei/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:30:49 +0000</pubDate>
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					<description><![CDATA[In 393 during the reign of Tai-Yuan, Chinese astronomers observed a new star visible for more than 200 days. This timing rules out the hypothesis that this event corresponded to a comet. The supernova appeared in the asterism of Wěi, located in the constellation Scorpius, located at the tail of the said scorpion.]]></description>
		
		
		
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		<title>TAR</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:24:31 +0000</pubDate>
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					<description><![CDATA[TAR: On February 23, 1987, astrophysicists Ian Shelton and Oscar Duhalde discovered the supernova SN 1987A. Located within the Large Magellanic Cloud about 168,000 light-years from Earth, the progenitor star of SN 1987A was about 20 times the mass of the Sun, with a diameter about 40 times that of the Sun.]]></description>
		
		
		
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		<title>MET</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:15:49 +0000</pubDate>
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					<description><![CDATA[The supernova SN 2017 egm was discovered on May 23, 2017 by astronomers at the University of Cambridge. It is located in a spiral galaxy about 420 million light-years away, has a high concentration of elements heavier than hydrogen and helium. It is the first evidence of the appearance of a superluminous supernova in metal [&#8230;]]]></description>
		
		
		
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		<title>MAH</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:13:43 +0000</pubDate>
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					<description><![CDATA[MAH: The supernova SN 2017 egm was discovered on May 23, 2017 by astronomers at the University of Cambridge. It is located in a spiral galaxy about 420 million light-years away, has a high concentration of elements heavier than hydrogen and helium. It is the first evidence of the appearance of a superluminous supernova in [&#8230;]]]></description>
		
		
		
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		<title>CAS</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 22:57:55 +0000</pubDate>
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					<description><![CDATA[Japanese and Chinese astronomers recorded in eight different writings the appearance of supernova SN 1181 between August 4 and 6, 1181. It is one of the eight supernovae belonging to the Milky Way observable with the naked eye, which appeared in the constellation Cassiopeia and was visible in the night sky for about 185 days.]]></description>
		
		
		
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		<title>CAN</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 22:56:59 +0000</pubDate>
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					<description><![CDATA[On July 4, 1054, Chinese astronomers observed the supernova SN 1054 appear in the constellation Taurus. The Anasazi Indians of present-day Arizona in the USA also observed it and depicted it in a petroglyph in Chaco Canyon. The Crab Nebula is its remnant and currently has 75,000 times more energy than the sun.]]></description>
		
		
		
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		<title>AND</title>
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		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 22:50:42 +0000</pubDate>
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					<description><![CDATA[AND: Supernova SN 1885A, also known as supernova Andromedae, was discovered on August 19, 1885 by Irish astronomer Isaac Ward and one day later by Estonian astronomer Ernst Hartwing. It is the only recorded supernova in the Andromeda galaxy.]]></description>
		
		
		
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