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2XMM J083026+524133 (2XMM J0830) is a very large galaxy cluster that lies 7.7 billion light-years away. It was discovered by chance by ESA's XMM Newton and the Large Binocular Telescope (LBT) in Arizona in 2008 while it was looking at the quasar APM 08279+5255. As of 2008, it was the largest known galaxy cluster at red shift z ≧ 1, weighing in at an estimated 1015 solar masses. However, galaxy cluster XMMXCS 2215-1738 is several billion light years farther away.

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  • 2XMM J083026+524133 (en)
  • 2XMM J083026+524133 (in)
  • 2XMM J083026+524133 (it)
  • 2XMM J083026+524133 (pl)
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  • 2XMM J083026+524133 (2XMM J0830) is a very large galaxy cluster that lies 7.7 billion light-years away. It was discovered by chance by ESA's XMM Newton and the Large Binocular Telescope (LBT) in Arizona in 2008 while it was looking at the quasar APM 08279+5255. As of 2008, it was the largest known galaxy cluster at red shift z ≧ 1, weighing in at an estimated 1015 solar masses. However, galaxy cluster XMMXCS 2215-1738 is several billion light years farther away. (en)
  • 2XMM J083026+524133 (2XMM J0830) adalah gugus galaksi sangat besar yang terletak 7.7 miliar tahun cahaya dari Bumi. Gugus galaksi ini ditemukan oleh XMM-Newton dan Teleskop Binokular Besar di Arizona pada tahun 2008. Pada tahun 2008, merupakan gugus galaksi terbesar dengan pergeseran merah z ≧ 1, massanya diperkirakan 1015 massa matahari. Akan tetapi, gugus galaksi terletak beberapa miliar tahun cahaya lebih jauh. (in)
  • 2XMM J083026+524133 (2XMM J0830) è un ammasso di galassie massivo distante 7.7 miliardi di anni luce. È stato scoperto nel 2008 tramite il telescopio XMM-Newton dell'ESA e il Large Binocular Telescope (LBT) in Arizona. A partire dalla sua scoperta nel 2008, risulta essere il più vasto ammasso di galassie conosciuto con red shift di z ≧ 1, di massa stimata in 1015 masse solari. Comunque, l'ammasso di galassie XMMXCS 2215-1738 risulta essere ancora più lontano, circa 10 miliardi di anni luce. (it)
  • 2XMM J083026+524133 (2XMM J0830) – bardzo duża gromada galaktyk w gwiazdozbiorze Rysia, oddalona o około 7,7 miliardów lat świetlnych od Ziemi. Została odkryta w 2008 roku przez satelitę XMM-Newton i teleskop Large Binocular Telescope. Od 2008 roku jest to największa znana gromada galaktyk spośród tych najbardziej odległych (współczynnik przesunięcia ku czerwieni z≥1), wcześniej największą była odkryta w 2006 roku gromada XMMXCS 2215-1738. (pl)
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  • X-CLASS 1649 (en)
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  • distant (en)
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  • 2XMM J083026+524133 (2XMM J0830) is a very large galaxy cluster that lies 7.7 billion light-years away. It was discovered by chance by ESA's XMM Newton and the Large Binocular Telescope (LBT) in Arizona in 2008 while it was looking at the quasar APM 08279+5255. As of 2008, it was the largest known galaxy cluster at red shift z ≧ 1, weighing in at an estimated 1015 solar masses. However, galaxy cluster XMMXCS 2215-1738 is several billion light years farther away. (en)
  • 2XMM J083026+524133 (2XMM J0830) adalah gugus galaksi sangat besar yang terletak 7.7 miliar tahun cahaya dari Bumi. Gugus galaksi ini ditemukan oleh XMM-Newton dan Teleskop Binokular Besar di Arizona pada tahun 2008. Pada tahun 2008, merupakan gugus galaksi terbesar dengan pergeseran merah z ≧ 1, massanya diperkirakan 1015 massa matahari. Akan tetapi, gugus galaksi terletak beberapa miliar tahun cahaya lebih jauh. (in)
  • 2XMM J083026+524133 (2XMM J0830) è un ammasso di galassie massivo distante 7.7 miliardi di anni luce. È stato scoperto nel 2008 tramite il telescopio XMM-Newton dell'ESA e il Large Binocular Telescope (LBT) in Arizona. A partire dalla sua scoperta nel 2008, risulta essere il più vasto ammasso di galassie conosciuto con red shift di z ≧ 1, di massa stimata in 1015 masse solari. Comunque, l'ammasso di galassie XMMXCS 2215-1738 risulta essere ancora più lontano, circa 10 miliardi di anni luce. (it)
  • 2XMM J083026+524133 (2XMM J0830) – bardzo duża gromada galaktyk w gwiazdozbiorze Rysia, oddalona o około 7,7 miliardów lat świetlnych od Ziemi. Została odkryta w 2008 roku przez satelitę XMM-Newton i teleskop Large Binocular Telescope. Od 2008 roku jest to największa znana gromada galaktyk spośród tych najbardziej odległych (współczynnik przesunięcia ku czerwieni z≥1), wcześniej największą była odkryta w 2006 roku gromada XMMXCS 2215-1738. (pl)
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