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IDCS J1426.5+3508

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This core, while still extremely hot, contains cooler gas than its surroundings. This is the most distant galaxy cluster where such a “cool core” of gas has been observed. These cool cores are important in understanding how quickly hot gas cools off in clusters, influencing the rate of stars at which
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in the center of the cluster. Apart from the cool core, the hot gas in the cluster is remarkably symmetrical and smooth. This is another piece of evidence that IDCS 1426 formed very rapidly and quickly in the early Universe. Despite the high mass and rapid evolution of this cluster, its existence
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emission near the middle of the cluster, but not exactly at the center. The location of this “core” of gas suggests that the cluster had a collision or interaction with another massive system of galaxies, perhaps within about the last 500 million years. This would cause the core to become offset.
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IDCS 1426 is being observed from when the Universe was only 3.8 billion years old. For an enormous structure to form rapidly, mergers with smaller clusters would likely play a role in a large cluster’s growth.
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to determine its distance. About 90% of the mass of the cluster is in the form of dark matter, the substance that has been detected only through its gravitational pull on normal matter composed of atoms.
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Brodwin, Mark; McDonald, Michael; Gonzalez, Anthony H.; Stanford, S. A.; Eisenhardt, Peter R.; Stern, Daniel; Zeimann, Gregory R. (2015-04-06).
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have observed IDCS 1426 when the universe was less than a third of its current age.
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stars are born. This cooling rate can be slowed by outbursts from a
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This rare galaxy cluster, which is located 10 billion
983: 922: 889: 769: 515: 424: 406: 349: 78:in 2012, IDCS 1426 was then observed using the 59:from Earth, has a mass of almost 500 trillion 303: 8: 378:(asteroid sample-return mission; Sep 2016) 310: 296: 288: 34:Galaxy Cluster IDCS J1426.5+3508 from the 236: 218: 48:for short) is an extremely massive young 116: 7: 25: 1050: 1049: 1038: 924: 519: 397: 391: 385: 353: 104:does not pose a threat to the 1: 366:(X-ray observatory; Feb 2016) 149:Mohon, Lee (6 January 2016). 124:Mohon, Lee (6 January 2016). 1065:Category:2017 in outer space 1060:Category:2016 in outer space 1055:Category:2015 in outer space 90:There is a region of bright 975:45P/Honda–Mrkos–Pajdušáková 534:atmospheric composition of 238:10.3847/0004-637X/817/2/122 106:standard model of cosmology 57:light travel distance years 1107: 755:2MASS J11193254–1137466 AB 126:"Galaxy Cluster IDCS 1426" 1033: 435:Asteroid close approaches 383: 370:ExoMars Trace Gas Orbiter 323: 207:The Astrophysical Journal 876:WISE J080822.18-644357.3 372:(Mars orbiter; Mar 2016) 74:First discovered by the 18:Galaxy Cluster IDCS 1426 1026:(Mars lander; Oct 2016) 101:supermassive black hole 76:Spitzer Space Telescope 1045:Outer space portal 688:OGLE-2007-BLG-349(AB)b 80:Hubble Space Telescope 38: 36:Hubble Space Telescope 950:C/2016 R2 (PANSTARRS) 33: 693:OGLE-2012-BLG-0950Lb 351:Space probe launches 1013:(end of mission to 970:43P/Wolf–Harrington 559:(retracted in 2022) 229:2016ApJ...817..122B 179:chandra.harvard.edu 945:53P/Van Biesbroeck 698:Proxima Centauri b 489:469219 KamoĘ»oalewa 39: 1073: 1072: 984:Space exploration 42:IDCS J1426.5+3508 16:(Redirected from 1098: 1053: 1052: 1043: 1042: 1041: 999:orbit; Jul 2016) 928: 872: 869: 867: 866: 857: 854: 852: 851: 847:(471325) 2011 KT 832: 829: 827: 826: 817: 794: 781: 760:2MASS J2126–8140 560: 523: 508: 506: 505: 501:(164121) 2003 YT 491: 484: 482: 481: 472: 470: 469: 460: 458: 457: 448: 446: 445: 401: 395: 389: 357: 340: 333: 312: 305: 298: 289: 283: 282: 280: 279: 265: 259: 258: 240: 222: 204: 195: 189: 188: 186: 185: 171: 165: 164: 162: 161: 146: 140: 139: 137: 136: 121: 84:Keck Observatory 21: 1106: 1105: 1101: 1100: 1099: 1097: 1096: 1095: 1086:Galaxy clusters 1076: 1075: 1074: 1069: 1039: 1037: 1029: 979: 918: 885: 870: 864: 863: 860: 855: 849: 848: 845: 836:BOSS Great Wall 830: 824: 823: 820: 815: 803:SDSS J1240+6710 792: 779: 765: 558: 511: 503: 502: 499: 487: 479: 478: 475: 467: 466: 463: 455: 454: 451: 443: 442: 441:(85990) 1999 JV 439: 420: 402: 396: 390: 381: 345: 342: 336: 334: 329: 319: 316: 286: 277: 275: 267: 266: 262: 202: 197: 196: 192: 183: 181: 173: 172: 168: 159: 157: 148: 147: 143: 134: 132: 123: 122: 118: 114: 28: 23: 22: 15: 12: 11: 5: 1104: 1102: 1094: 1093: 1088: 1078: 1077: 1071: 1070: 1068: 1067: 1047: 1034: 1031: 1030: 1028: 1027: 1018: 1000: 987: 985: 981: 980: 978: 977: 972: 967: 962: 957: 952: 947: 942: 940:460P/PanSTARRS 937: 931: 929: 920: 919: 917: 916: 911: 906: 901: 895: 893: 887: 886: 884: 883: 878: 873: 858: 843: 838: 833: 818: 810: 805: 800: 795: 793:(hypothesized) 787: 782: 773: 771: 767: 766: 764: 763: 757: 752: 747: 742: 741: 740: 735: 730: 720: 715: 710: 705: 700: 695: 690: 685: 680: 675: 670: 665: 660: 655: 650: 645: 640: 635: 634: 633: 628: 623: 618: 608: 603: 598: 597: 596: 591: 586: 581: 576: 566: 561: 553: 548: 543: 538: 532: 526: 524: 513: 512: 510: 509: 497: 492: 485: 473: 461: 449: 437: 431: 429: 422: 421: 419: 418: 412: 410: 404: 403: 384: 382: 380: 379: 373: 367: 360: 358: 347: 346: 344: 343: 335: 327: 324: 321: 320: 317: 315: 314: 307: 300: 292: 285: 284: 273:hubblesite.org 260: 190: 166: 141: 115: 113: 110: 50:galaxy cluster 27:Galaxy cluster 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 1103: 1092: 1089: 1087: 1084: 1083: 1081: 1066: 1062: 1061: 1056: 1048: 1046: 1036: 1035: 1032: 1025: 1023: 1019: 1016: 1012: 1011: 1006: 1005: 1001: 998: 994: 993: 989: 988: 986: 982: 976: 973: 971: 968: 966: 963: 961: 958: 956: 953: 951: 948: 946: 943: 941: 938: 936: 933: 932: 930: 927: 921: 915: 912: 910: 907: 905: 902: 900: 897: 896: 894: 892: 888: 882: 879: 877: 874: 868: 859: 853: 844: 842: 839: 837: 834: 828: 819: 814: 811: 809: 806: 804: 801: 799: 796: 791: 788: 786: 783: 778: 775: 774: 772: 768: 761: 758: 756: 753: 751: 748: 746: 743: 739: 736: 734: 731: 729: 726: 725: 724: 721: 719: 716: 714: 711: 709: 706: 704: 701: 699: 696: 694: 691: 689: 686: 684: 681: 679: 676: 674: 671: 669: 666: 664: 661: 659: 656: 654: 651: 649: 646: 644: 641: 639: 636: 632: 629: 627: 624: 622: 619: 617: 614: 613: 612: 609: 607: 604: 602: 599: 595: 592: 590: 587: 585: 582: 580: 577: 575: 572: 571: 570: 567: 565: 562: 557: 554: 552: 549: 547: 544: 542: 539: 537: 533: 531: 530:38 Virginis b 528: 527: 525: 522: 518: 514: 507: 498: 496: 493: 490: 486: 483: 474: 471: 462: 459: 450: 447: 438: 436: 433: 432: 430: 428: 423: 417: 414: 413: 411: 409: 408:Impact events 405: 400: 394: 388: 377: 374: 371: 368: 365: 362: 361: 359: 356: 352: 348: 339: 332: 326: 325: 322: 318:2016 in space 313: 308: 306: 301: 299: 294: 293: 290: 274: 270: 264: 261: 256: 252: 248: 247:1721.1/102642 244: 239: 234: 230: 226: 221: 216: 212: 208: 201: 194: 191: 180: 176: 170: 167: 156: 152: 145: 142: 131: 127: 120: 117: 111: 109: 107: 102: 96: 93: 88: 85: 81: 77: 72: 70: 66: 62: 58: 53: 51: 47: 43: 37: 32: 19: 1058: 1022:Schiaparelli 1021: 1008: 1002: 990: 965:144P/Kushida 750:V830 Tauri b 683:Kepler-1647b 678:Kepler-1638b 673:Kepler-1625b 668:Kepler-1520b 663:Kepler-1229b 556:HD 131399 Ab 546:Gliese 536 b 276:. 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Index

Galaxy Cluster IDCS 1426

Hubble Space Telescope
galaxy cluster
light travel distance years
Suns
Universe
Astronomers
Spitzer Space Telescope
Hubble Space Telescope
Keck Observatory
X-ray
supermassive black hole
standard model of cosmology
"Galaxy Cluster IDCS 1426"
"NASA's Great Observatories Weigh Massive Young Galaxy Cluster"
"Chandra :: Photo Album :: IDCS J1426.5+3508 :: January 7, 2016"
"IDCS J1426.5+3508: The Most Massive Galaxy Cluster at $ z > 1.5$ "
arXiv
1504.01397
Bibcode
2016ApJ...817..122B
doi
10.3847/0004-637X/817/2/122
hdl
1721.1/102642
S2CID
85451444
"HubbleSite - NewsCenter - NASA's Hubble Spots Rare Gravitational Arc from Distant, Hefty Galaxy Cluster (06/26/2012) - The Full Story"
v

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