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	<title>Sun &#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>VEL</title>
		<link>https://suittoeyewear.com/en/modelo/vel/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:29:09 +0000</pubDate>
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					<description><![CDATA[Vela Junior is one of the few supernova remnants analyzed in its entire electromagnetic spectrum, from radio frequencies to very high energy gamma rays. The relative proximity of this supernova remnant, its large size and its strong non-thermal emission make this remnant one of the main sources used to study the mechanisms of acceleration and [&#8230;]]]></description>
		
		
		
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		<title>TYC</title>
		<link>https://suittoeyewear.com/en/modelo/tyc/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:27:42 +0000</pubDate>
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					<description><![CDATA[In 1572 the Danish astronomer Tycho Brahe, observed a strange event in the constellation Cassiopeia, a new star had appeared that shone brighter than Jupiter and was visible for eighteen months. The discovery of the supernova SN 1572 or Nova Tycho described it in a book entitled De nova stella, in which the word nova [&#8230;]]]></description>
		
		
		
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		<title>TAR</title>
		<link>https://suittoeyewear.com/en/modelo/tar/</link>
		
		<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>NOR</title>
		<link>https://suittoeyewear.com/en/modelo/nor/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:17:03 +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>MET</title>
		<link>https://suittoeyewear.com/en/modelo/met/</link>
		
		<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>
		<link>https://suittoeyewear.com/en/modelo/mah/</link>
		
		<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>LUP</title>
		<link>https://suittoeyewear.com/en/modelo/lup/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:13:17 +0000</pubDate>
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					<description><![CDATA[In the constellation of Lupus, in the spring of 1006 the supernova SN 1006 appeared, Chinese and Arab astronomers described its size equivalent to a half moon, it was the brightest stellar event in recorded history and was visible for more than a year.]]></description>
		
		
		
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		<title>HOU</title>
		<link>https://suittoeyewear.com/en/modelo/hou/</link>
		
		<dc:creator><![CDATA[Ricard Puig]]></dc:creator>
		<pubDate>Sat, 10 May 2025 23:10:50 +0000</pubDate>
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					<description><![CDATA[In the book Hou Hanshu by the Chinese historian Fan Ye, where he describes the history of the Han Dynasty between 25 and 220 AD, there is the first historical record of a supernova, SN 185 observed on December 7, 185 located near Alpha Centauri between the constellations Circinus and Centaurus.]]></description>
		
		
		
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		<title>CAS</title>
		<link>https://suittoeyewear.com/en/modelo/cas/</link>
		
		<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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