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ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin
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di pårtaedjî – di rcopyî, di rispåde eyet di rdiner cisse ouve ci
di rdjårber – di candjî ciste ouve
Avou les condicions ki shuvèt :
atribucion – Vos dvoz dner les racsegnes so l’ oteur ki vont bén, diner on loyén eviè l’ licince eyet mete si des candjmints ont stî fwaits. Vos ploz fé çoula di tote sôre di manires, mins nén tot djant ki l’ oteur vs aspale udonbén asprouve l’ uzaedje ki vos nd e fjhoz.
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Ci fitchî cial a des infôrmåcions di rawete, motoit bén radjoutêyes pa l’ aparey foto limerike ou l’ sicanrece eployeye po fé l’ imådje.
Si l’ imådje a stî candjeye dispoy adon, i s’ pout ki sacwants detays ni corespondexhe pus totafwait.
Date ey eure ki les dnêyes ont stî fwaites
28 d' awousse 2013 a 15:30
Crédit ou fournisseur
ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin
Source
European Southern Observatory
Titre court
Image of HIP 102152
Tite di l' imådje
This image shows solar twin HIP 102152, a star located 250 light-years from Earth in the constellation of Capricornus (The Sea Goat). HIP 102152 is more like the Sun than any other solar twin — apart from the fact that it is nearly four billion years older, giving us an unprecedented chance to study how the Sun will look when it ages. It is the oldest solar twin identified to date, and was studied by an international team using ESO’s Very Large Telescope, led by astronomers in Brazil. The different colours of the star are caused by the star moving slightly between the two exposures, many years apart.