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to be the most striking concentration of galaxies. He found it particularly interesting because of its "great linear dimension, the numerous population and distinctly elongated form". This can be identified with what we now know as the core of the
Shapley
183:
in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the
Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies.
247:
231:, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. Around the same time, Roberto Scaramella and co-workers had also noticed the Shapley Supercluster in the
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may be anotherâand has led to a surge of interest in this supercluster. It has been found that the Great
Attractor and all the galaxies in our region of the universe (including our galaxy, the
208:, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo.
139:
interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the
290:. This approach enables new ways of understanding and modelling variations in galactic movements. The nearest large underdense area has been labelled the
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Part of Abell 3558, the galaxy cluster at the center of the
Shapley Supercluster, the largest mass concentration in the observable Universe
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267:(CMB) frame of reference. This has led many to speculate that the Shapley Supercluster may be one of the major causes of our galaxy's
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364:; Carrasco, Eleazar R.; Reisenegger, Andreas; Slezak, Eric; Muriel, HernĂĄn; DĂźnner, Rolando; SodrĂŠ, Laerte Jr.;
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in the supercluster creates a relative movement away from underdense areas, that may be visualized as a virtual
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In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the
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started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch
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Scaramella, R.; Baiesi-Pillastrini, G.; Chincarini, G.; Vettolani, G.; Zamorani, G. (April 1989).
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495:"A marked concentration of galaxy clusters: is this the origin of large-scale motions?"
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306: â A possible non-random component of the peculiar velocity of galaxy clusters
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374:"The Shapley supercluster: the largest matter concentration in the local Universe"
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204:. Shapley estimated the distance to this cloud to be 14 times that to the
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440:"The distribution of galaxies in the direction of the 'Great Attractor'"
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312: â Region of overdensity of galaxies within the local supercluster
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The
Shapley Supercluster lies very close to the direction in which the
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In 2017 it was proposed that the movement towards attractors like the
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670:"A Complete CEnsus of Star formation in the Shapley supercluster"
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of galaxies (including our galaxy) is moving with respect to the
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336: â Large group of smaller galaxy clusters or galaxy groups
324: â All of space observable from the Earth at the present
227:
in
England. In this paper, the supercluster was named after
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In recent times, the
Shapley Supercluster was named by
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Largest concentration of galaxies in our local universe
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387:(124). European Southern Observatory (ESO): 30â31.
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330: â Galaxy cluster in the constellation Norma
318: â Closest neighboring galaxy supercluster
195:), but found a 'cloud' in the constellation of
279:) are moving toward the Shapley Supercluster.
754:
655:"X-rays Reveal What Makes the Milky Way Move"
8:
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676:. Osservatorio Astronomico di Capodimonte.
570:(30 January 2017). "The dipole repeller".
27:
702:
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638:Consiglio Nazionale delle Ricerche (CNR)
221:Automated Plate Measuring Facility (APM)
2165:
346:
18:
640:. Istituto di Radioastronomia (IRA).
438:Raychaudhury, Somak (November 1989).
322:Large-scale structure of the universe
81:â30° 0′ 0″
7:
644:from the original on March 26, 2007.
33:Galaxies in the Shapley Supercluster
689:(Jan 30, 2017). "Dipole Repeller".
649:Harvard College Observatory (HCO)
372:; Ragone, Cinthia J. (June 2006).
127:) is the largest concentration of
14:
674:Istituto Nazionale di Astrofisica
250:A map of the Shapley Supercluster
215:, from a survey of galaxies from
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2192:
2180:
2168:
2145:
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1765:ScorpiusâCentaurus association
786:Centaurus in Chinese astronomy
549:"What is the Great Attractor?"
109:Shapley Concentration, SCl 124
1:
219:Sky survey plates, using the
316:HydraâCentaurus Supercluster
634:"The Shapley Concentration"
265:cosmic microwave background
169:Harvard College Observatory
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781:List of stars in Centaurus
770:Constellation of Centaurus
419:www.atlasoftheuniverse.com
415:"The Shapley Supercluster"
167:and his colleagues at the
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661:. IFA. January 11, 2006.
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26:
1101:V816 (Przybylski's Star)
629:at Atlas of the Universe
239:: they had named it the
721:10.1038/s41550-016-0036
602:10.1038/s41550-016-0036
225:University of Cambridge
366:Drinkwater, Michael J.
251:
249:
121:Shapley Concentration
2254:Galaxy superclusters
2239:Shapley Supercluster
2094:Shapley Supercluster
1831:Southern Crab Nebula
1548:PSR B1259â63/LS 2883
828:C (Proxima Centauri)
659:University of Hawaii
627:Shapley Supercluster
237:clusters of galaxies
217:UK Schmidt Telescope
147:. It is 650 million
117:Shapley Supercluster
22:Shapley Supercluster
2112:Astronomical events
818:A (Rigil Kentaurus)
713:2017NatAs...1E..36H
687:Courtois, HÊlène M.
685:; Tully, R. Brent;
594:2017NatAs...1E..36H
568:Courtois, HÊlène M.
566:; Tully, R. Brent;
511:1989Natur.338..562S
456:1989Natur.342..251R
393:2006Msngr.124...30P
241:Alpha concentration
1987:5128 (Centaurus A)
1674:Proxima Centauri b
370:Parker, Quentin A.
252:
213:Somak Raychaudhury
193:Virgo Supercluster
181:apparent magnitude
104:Other designations
39:Observation data (
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681:Hoffman, Yehuda;
562:Hoffman, Yehuda;
505:(6216): 562â564.
450:(6247): 251â255.
358:Proust, Dominique
284:Shapley Attractor
189:Coma Supercluster
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683:Pomarède, Daniel
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255:Current interest
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551:. 14 July 2014.
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273:Great Attractor
269:peculiar motion
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233:Abell catalogue
173:Bruce telescope
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137:gravitationally
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840:Îł (Muhlifain)
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381:The Messenger
375:
371:
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363:
359:
353:
351:
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332:
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328:Norma Cluster
326:
323:
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49:
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37:
30:
25:
20:
2223:Solar System
2093:
2063:PKS 1353â341
2058:PKS 1144-379
2038:ESO 325-G004
1604:b Centauri b
735:
697:(36): 0036.
694:
690:
673:
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637:
575:
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543:
502:
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447:
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422:. Retrieved
418:
409:
384:
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334:Supercluster
287:
281:
258:
240:
210:
202:Supercluster
186:
177:Bloemfontein
162:
124:
120:
116:
114:
2211:Outer space
2199:Spaceflight
1669:HIP 67522 b
1664:HIP 65426 b
1659:HD 121504 b
1654:HD 117618 b
1649:HD 117207 b
1644:HD 114729 b
1639:HD 114386 b
1629:HD 113538 b
1624:HD 101930 b
1619:HD 109749 b
1614:HD 103197 b
1609:HD 102117 b
865:θ (Menkent)
823:B (Toliman)
578:(2): 0036.
261:Local Group
149:light-years
77:Declination
2233:Categories
2089:Abell S740
2048:ESO 444-46
2043:ESO 383-76
2033:ESO 269-57
1806:G292.0+1.8
1591:Exoplanets
855:Îś (Alnair)
704:1702.02483
585:1702.02483
424:2020-09-23
341:References
95:(652
2249:Centaurus
2175:Astronomy
1801:Fleming 1
965:Flamsteed
835:β (Hadar)
527:1476-4687
472:1476-4687
401:992894162
304:Dark flow
277:Milky Way
197:Centaurus
163:In 1930,
145:Centaurus
91:200
58:Centaurus
2150:Category
2130:SN 1986G
2125:SN 1895B
1858:Galaxies
1839:(RCW 86)
1821:NGC 5307
1816:NGC 3918
1770:Stock 16
1755:NGC 5662
1750:NGC 5617
1745:NGC 5460
1740:NGC 5316
1735:NGC 5281
1730:NGC 5286
1725:NGC 4230
1720:NGC 3766
1689:WASP-15b
1533:Gaia BH2
1374:5489 (c)
1369:5485 (c)
1364:5471 (b)
1354:5358 (v)
1334:5222 (y)
1329:5207 (N)
1324:5174 (z)
1319:5172 (M)
1314:5141 (Q)
1309:5089 (d)
1304:5071 (K)
1299:5041 (m)
1294:5035 (J)
1289:5006 (r)
1274:4940 (f)
1269:4889 (n)
1264:4888 (e)
1259:4874 (p)
1254:4831 (w)
1249:4817 (l)
1239:4748 (u)
1234:4732 (G)
1229:4724 (x)
1219:4712 (x)
1214:4682 (F)
1209:4652 (D)
1204:4620 (E)
1199:4546 (B)
1194:4537 (j)
1174:4476 (C)
1169:4466 (C)
1164:4460 (A)
1131:V945 (H)
1076:V763 (C)
1071:V761 (a)
998:Variable
642:Archived
298:See also
288:repeller
191:and the
133:universe
129:galaxies
87:Distance
2161:Portals
1811:IC 2944
1788:Nebulae
1715:IC 2944
1599:2M1207b
1568:WASP-42
1563:WASP-41
1538:GJ 3737
729:7537393
709:Bibcode
610:7537393
590:Bibcode
535:4336689
507:Bibcode
480:4354365
452:Bibcode
389:Bibcode
223:at the
159:History
153:z=0.046
125:SCl 124
2120:SN 185
1844:SuWt 2
1836:SN 185
1826:RCW 79
1543:J1407b
1528:2M1207
1507:131399
1502:125595
1497:125072
1492:124448
1487:121504
1482:121228
1472:117207
1467:116434
1462:115600
1457:114729
1452:114386
1447:113766
1442:113538
1437:110113
1432:109749
1427:108236
1422:107914
1417:103197
1407:101930
1402:100453
727:
608:
533:
525:
499:Nature
478:
470:
444:Nature
399:
151:away (
70:13 25
2187:Stars
2026:Other
1895:4650A
1516:Other
1397:98176
1392:97413
1146:V1400
1141:V1369
1136:V1032
988:4 (h)
983:3 (k)
978:2 (g)
973:1 (i)
805:Bayer
796:Stars
725:S2CID
699:arXiv
606:S2CID
580:arXiv
531:S2CID
476:S2CID
377:(PDF)
271:âthe
44:J2000
41:Epoch
2017:5419
2012:5408
2007:5398
2002:5291
1997:5253
1992:5161
1982:5114
1977:5102
1972:5091
1967:5090
1962:5026
1950:5011
1945:4976
1940:4945
1935:4744
1930:4743
1925:4730
1920:4729
1915:4709
1910:4706
1905:4696
1900:4683
1890:4622
1885:4603
1880:4444
1875:3783
1359:5371
1349:5297
1344:5241
1339:5224
1284:4989
1279:4979
1244:4796
1224:4721
1189:4523
1184:4522
1179:4499
1126:V863
1121:V886
1116:V885
1111:V842
1106:V831
1096:V810
1091:V803
1086:V779
1081:V766
1066:V752
1061:V744
1056:V346
523:ISSN
468:ISSN
397:OCLC
115:The
1867:NGC
717:doi
598:doi
515:doi
503:338
460:doi
448:342
385:124
235:of
175:at
155:).
143:of
119:or
97:Mly
93:Mpc
54:(s)
2235::
1384:HD
1156:HR
1051:DY
1046:BV
1041:SX
1036:SV
1031:RR
723:.
715:.
707:.
693:.
672:.
657:.
636:.
604:.
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588:.
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458:.
446:.
442:.
417:.
395:.
383:.
379:.
368:;
360:;
349:^
294:.
243:.
2163::
1955:A
1760:Ď
1684:d
1679:c
1634:c
1026:Y
1021:V
1016:U
1011:T
1006:R
955:Ď
950:Ď
945:Ď
940:Ď
935:Ď
930:Ď
925:Ď
920:Ď
915:Ď
910:Îż
905:Îż
900:Ξ
895:Ξ
890:ν
885:Îź
880:Îť
875:Îş
870:Κ
860:Ρ
850:Îľ
845:δ
813:Îą
762:e
755:t
748:v
731:.
719::
711::
701::
695:1
612:.
600::
592::
582::
576:1
537:.
517::
509::
482:.
462::
454::
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403:.
391::
123:(
99:)
46:)
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
