SpARCS1049+56
Galaxy cluster
From Wikipedia, the free encyclopedia
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.
| SpARCSJ1049+56 | |
|---|---|
Image, using data from Spitzer and the Hubble Space Telescope | |
| Observation data (Epoch J2000) | |
| Right ascension | 10h 49m 22.6s |
| Declination | +56° 40′ 33″ |
| Redshift | 1.7 |
| Binding mass | (3.5±1.2)×1014 M☉ |