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SpARCS1049+56

Galaxy cluster From Wikipedia, the free encyclopedia

SpARCS1049+56
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SpARCS1049+56 is a galaxy cluster whose heart is bursting with new stars and located at a distance of about 9.8 billion light-years away from Earth. It was discovered by NASA's Hubble and Spitzer space telescopes on 2015.[1] The galaxy cluster has a redshift of 1.7[2] and a mass of (3.5±1.2)×1014 M [3] estimated from weak gravitational lensing.

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This image, using data from Spitzer and the Hubble Space Telescope, shows the galaxy cluster SpARCS1049.
Quick facts SpARCSJ1049+56, Observation data (Epoch J2000) ...
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