364:. This mechanism cannot explain b Cen (AB)b, because core accretion becomes less efficient at large distances from the star, and massive stars like b Centauri A cause the disc to dissipate much quicker. It's more probable that the planet formed directly from the circumstellar gas, through a mechanism known as gravitational instability. This process is much faster than core accretion and can act even at separations of hundreds of astronomical units. Another possibility is that the planet formed closer to the central stars and was subsequently ejected to its current orbit through interactions with another body, but this is disfavored by the lack of evidence of other planets in the system and by the low eccentricity of b Cen (AB)b.
254:
2016:
34:
430:
Janson, Markus; Squicciarini, Vito; Delorme, Philippe; Gratton, Raffaele; Bonnefoy, Mickaƫl; Reffert, Sabine; Mamajek, Eric E.; Eriksson, Simon C.; Vigan, Arthur; Langlois, Maud; Engler, Natalia; Chauvin, Gaƫl; Desidera, Silvano; Mayer, Lucio; Marleau, Gabriel-Dominique; Bohn, Alexander J.; Samland,
497:
Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaƫl; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaƫl; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini,
281:
separation that had infrared colors consistent with a massive planet. A second observation in 2021 confirmed that the object has common proper motion with b
Centauri and therefore is physically bound to the system. The authors of this study also looked for old observations of b Centauri and found
498:
Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C. (2021). "A wide-orbit giant planet in the high-mass b
Centauri binary system".
431:
Matthias; Meyer, Michael; d'Orazi, Valentina; Henning, Thomas; Quanz, Sascha; Kenworthy, Matthew; Carson, Joseph C. (2021). "BEAST begins: Sample characteristics and survey performance of the B-star
Exoplanet Abundance Study".
344:. The mass ratio between b Cen (AB)b and the central binary star is 0.10ā0.17%, which is similar to the Sun-Jupiter system and is consistent to the expectations that more massive stars tend to have more massive planets.
339:
The SPHERE images show the planet has approximately 0.01% the solar luminosity, a relic of its recent formation. From this luminosity and the age of the system, cooling models predict it has a mass of about 11 times the
328:. The three epochs of observations show evidence of the orbital motion of the planet around the central stars, but the orbit is still not well constrained. The data are consistent with an
367:
The discovery of b Cen (AB)b showed that planets can exist even around massive stars. Previous studies had shown that planet occurrence rate starts to drop for stars over 2
62:
43:
385:
can detect. The discovers of b Cen (AB)b argued that the short lifetime of the circumstellar discs around massive stars may prevent planets from
2043:
300:, b Centauri is the most massive system around which a planet has been found; previously, the most massive star with a known planet was 3
2038:
630:
269:
to search for planets around B-type stars in the
ScorpiusāCentaurus association. SPHERE is equipped with a sophisticated
1634:
559:
Shatsky, N.; Tokovinin, A. (2002). "The mass ratio distribution of B-type visual binaries in the Sco OB2 association".
57:
78:
655:
97:
352:
The formation mechanism for b Cen (AB)b is uncertain. It is believed that most giant planets are formed via
253:
1981:
1392:
650:
406:
867:
639:
1417:
357:
623:
174:
286:
in 2000, but was considered a background star at the time. With a primary star mass of 5ā6
1253:
382:
1841:
1836:
1736:
1025:
834:
353:
582:
454:
1963:
1700:
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578:
517:
450:
333:
314:
266:
114:
39:
8:
386:
321:
283:
226:
142:
521:
2019:
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1548:
1543:
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541:
507:
466:
440:
361:
809:
804:
779:
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674:
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389:
closer to their stars, but allows the existence of distant planets like b Cen (AB)b.
598:
1932:
1665:
719:
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586:
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309:
89:
462:
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749:
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341:
1950:
1629:
1442:
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1010:
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682:
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329:
274:
181:
125:
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945:
935:
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739:
724:
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608:
238:
20:
273:
that blocks out the light from a star and allows exoplanets around it to be
1927:
1907:
1675:
1576:
824:
819:
814:
799:
789:
769:
764:
729:
537:
242:
205:
356:, in which a rocky core, after growing to a critical mass, starts rapidly
332:
between 2650 and 7170 years, inclination between 128 and 157 degrees, and
257:
Artist's impression showing b
Centauri b. b Centauri is in the background.
1856:
1538:
1533:
1528:
1523:
1518:
1513:
1508:
1503:
1498:
1493:
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1478:
1098:
1088:
1043:
920:
915:
910:
905:
900:
784:
759:
754:
573:
307:. The discovery was published in December 2021 on the scientific journal
270:
1958:
1917:
1912:
1902:
1198:
1188:
1183:
1173:
1163:
1103:
1083:
1078:
1073:
1000:
895:
890:
885:
880:
875:
857:
852:
847:
842:
261:
The b
Centauri system was included in the BEAST survey, which uses the
277:. The first observation of the system in 2019 revealed an object at a
1824:
1764:
1670:
1460:
1376:
1371:
1366:
1361:
1356:
1351:
1346:
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1208:
1203:
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1178:
1168:
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1143:
1138:
1133:
1128:
1123:
1118:
1108:
1093:
1068:
1063:
1058:
1053:
1048:
1038:
1033:
995:
990:
985:
940:
381:
stars, but this result is valid only for close in planets, which the
234:
230:
161:
1999:
1994:
1886:
1881:
1876:
1871:
1866:
1861:
1851:
1846:
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1809:
1804:
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1789:
1784:
1779:
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1759:
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1685:
1639:
1624:
1619:
1614:
1609:
1604:
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1402:
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445:
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1584:
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1407:
1113:
950:
429:
1989:
1727:
1713:
1705:
1695:
1657:
1412:
1397:
1005:
320:
Named b
Centauri (AB)b (shortened as 'b Cen (AB)b'), this is a
262:
411:
Exoplanet
Exploration: Planets Beyond our Solar System (NASA)
665:
193:
33:
324:
that orbits the stellar pair at a projected separation of
19:
This article is about b
Centauri b. For Ī² Centauri B, see
496:
46:. The planet b Centauri b is indicated by an arrow.
1980:
2030:
558:
1949:
638:
423:
624:
1575:
492:
490:
488:
486:
484:
482:
480:
631:
617:
552:
1459:
572:
511:
477:
444:
16:Long-period exoplanet orbiting b Centauri
252:
233:, located in the southern constellation
282:that the planet had been imaged by the
2031:
1656:
2044:Exoplanets detected by direct imaging
612:
293:and a total system mass of 6ā10
225:(sometimes b Centauri (AB) b) is a
13:
14:
2055:
2015:
2014:
229:orbiting the binary star system
32:
1635:ScorpiusāCentaurus association
656:Centaurus in Chinese astronomy
399:
374:and reaches almost zero for 3
1:
2039:Exoplanets discovered in 2021
392:
347:
248:
7:
463:10.1051/0004-6361/202039683
360:the surrounding gas of the
10:
2060:
651:List of stars in Centaurus
640:Constellation of Centaurus
591:10.1051/0004-6361:20011542
561:Astronomy and Astrophysics
530:10.1038/s41586-021-04124-8
433:Astronomy and Astrophysics
317:astronomer Markus Janson.
18:
2012:
1976:
1945:
1895:
1735:
1726:
1652:
1571:
1455:
1385:
1252:
1024:
866:
833:
673:
664:
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241:, with a mass 10.9 times
216:
192:
172:
167:
157:
141:
126:Orbital period (sidereal)
123:
113:
95:
88:
76:
68:
56:
51:
31:
971:V816 (Przybylski's Star)
168:Physical characteristics
583:2002A&A...382...92S
455:2021A&A...646A.164J
90:Orbital characteristics
383:radial velocity method
258:
256:
38:b Centauri imaged by
1964:Shapley Supercluster
1701:Southern Crab Nebula
1418:PSR B1259ā63/LS 2883
698:C (Proxima Centauri)
315:Stockholm University
267:Very Large Telescope
1982:Astronomical events
688:A (Rigil Kentaurus)
522:2021Natur.600..231J
407:"Exoplanet-catalog"
322:circumbinary planet
284:ESO 3.6 m Telescope
279:5.3 arcseconds
227:circumbinary planet
69:Discovery date
28:
1857:5128 (Centaurus A)
1544:Proxima Centauri b
362:circumstellar disc
336:smaller than 0.4.
265:instrument at the
259:
237:. The planet is a
58:Discovered by
26:
2026:
2025:
2008:
2007:
1972:
1971:
1941:
1940:
1722:
1721:
1710:
1648:
1647:
1567:
1566:
1451:
1450:
1428:WASP-15 (Nyamien)
506:(7888): 231ā234.
220:
219:
2051:
2018:
2017:
1978:
1977:
1947:
1946:
1733:
1732:
1708:
1666:Boomerang Nebula
1654:
1653:
1573:
1572:
1457:
1456:
1443:WASP-167/KELT-13
1393:2MASS J1126ā5003
671:
670:
633:
626:
619:
610:
609:
603:
602:
576:
574:astro-ph/0109456
556:
550:
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417:
403:
327:
280:
204:
202:
153:
151:
137:
135:
109:
107:
79:Detection method
36:
29:
25:
2059:
2058:
2054:
2053:
2052:
2050:
2049:
2048:
2029:
2028:
2027:
2022:
2004:
1968:
1951:Galaxy clusters
1937:
1923:IRAS 13224-3809
1891:
1718:
1644:
1563:
1447:
1381:
1347:117618 (Dofida)
1248:
1020:
862:
829:
660:
642:
637:
607:
606:
557:
553:
495:
478:
428:
424:
415:
413:
405:
404:
400:
395:
380:
377:
373:
370:
350:
342:mass of Jupiter
325:
313:and was led by
306:
303:
299:
296:
292:
289:
278:
275:directly imaged
251:
243:that of Jupiter
211:
208:
200:
198:
187:
184:
177:
149:
147:
133:
131:
128:
105:
103:
100:
98:Semi-major axis
81:
47:
24:
17:
12:
11:
5:
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2041:
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2023:
2013:
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2002:
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1463:
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1445:
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1430:
1425:
1423:PSR J1311ā3430
1420:
1415:
1410:
1405:
1400:
1395:
1389:
1387:
1383:
1382:
1380:
1379:
1374:
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1334:
1329:
1324:
1319:
1314:
1309:
1304:
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1289:
1284:
1282:102117 (Uklun)
1279:
1274:
1269:
1264:
1258:
1256:
1250:
1249:
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1241:
1236:
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628:
621:
613:
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476:
422:
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394:
391:
378:
375:
371:
368:
354:core accretion
349:
346:
330:orbital period
304:
301:
297:
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290:
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250:
247:
218:
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96:
93:
92:
86:
85:
84:Direct imaging
82:
77:
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73:
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66:
65:
60:
54:
53:
49:
48:
37:
15:
9:
6:
4:
3:
2:
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2011:
2001:
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1911:
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1578:
1577:Star clusters
1574:
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1207:
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1202:
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1197:
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1190:
1187:
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1177:
1175:
1172:
1170:
1167:
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1160:
1157:
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1130:
1127:
1125:
1122:
1120:
1117:
1115:
1112:
1110:
1107:
1105:
1102:
1100:
1097:
1095:
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1087:
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1077:
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1072:
1070:
1067:
1065:
1062:
1060:
1057:
1055:
1052:
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738:
736:
733:
731:
728:
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723:
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710:Ī³ (Muhlifain)
708:
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239:super-Jupiter
236:
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35:
30:
22:
21:Beta Centauri
1933:PKS 1353ā341
1928:PKS 1144-379
1908:ESO 325-G004
1474:b Centauri b
1473:
564:
560:
554:
503:
499:
436:
432:
425:
414:. Retrieved
410:
401:
366:
351:
338:
334:eccentricity
319:
308:
260:
223:b Centauri b
222:
221:
115:Eccentricity
27:b Centauri b
1539:HIP 67522 b
1534:HIP 65426 b
1529:HD 121504 b
1524:HD 117618 b
1519:HD 117207 b
1514:HD 114729 b
1509:HD 114386 b
1499:HD 113538 b
1494:HD 101930 b
1489:HD 109749 b
1484:HD 103197 b
1479:HD 102117 b
735:Īø (Menkent)
693:B (Toliman)
326:560 AU
271:coronagraph
175:Mean radius
143:Inclination
2033:Categories
1959:Abell S740
1918:ESO 444-46
1913:ESO 383-76
1903:ESO 269-57
1676:G292.0+1.8
1461:Exoplanets
725:Ī¶ (Alnair)
513:2112.04833
446:2101.02043
416:2023-10-24
393:References
231:b Centauri
162:b Centauri
1671:Fleming 1
835:Flamsteed
705:Ī² (Hadar)
546:245005994
471:230770142
387:migrating
358:accreting
348:Formation
249:Discovery
235:Centaurus
52:Discovery
2020:Category
2000:SN 1986G
1995:SN 1895B
1728:Galaxies
1709:(RCW 86)
1691:NGC 5307
1686:NGC 3918
1640:Stock 16
1625:NGC 5662
1620:NGC 5617
1615:NGC 5460
1610:NGC 5316
1605:NGC 5281
1600:NGC 5286
1595:NGC 4230
1590:NGC 3766
1559:WASP-15b
1403:Gaia BH2
1244:5489 (c)
1239:5485 (c)
1234:5471 (b)
1224:5358 (v)
1204:5222 (y)
1199:5207 (N)
1194:5174 (z)
1189:5172 (M)
1184:5141 (Q)
1179:5089 (d)
1174:5071 (K)
1169:5041 (m)
1164:5035 (J)
1159:5006 (r)
1144:4940 (f)
1139:4889 (n)
1134:4888 (e)
1129:4874 (p)
1124:4831 (w)
1119:4817 (l)
1109:4748 (u)
1104:4732 (G)
1099:4724 (x)
1089:4712 (x)
1084:4682 (F)
1079:4652 (D)
1074:4620 (E)
1069:4546 (B)
1064:4537 (j)
1044:4476 (C)
1039:4466 (C)
1034:4460 (A)
1001:V945 (H)
946:V763 (C)
941:V761 (a)
868:Variable
599:16697655
538:34880428
439:: A164.
379:☉
372:☉
305:☉
298:☉
291:☉
1681:IC 2944
1658:Nebulae
1585:IC 2944
1469:2M1207b
1438:WASP-42
1433:WASP-41
1408:GJ 3737
579:Bibcode
518:Bibcode
451:Bibcode
1990:SN 185
1714:SuWt 2
1706:SN 185
1696:RCW 79
1413:J1407b
1398:2M1207
1377:131399
1372:125595
1367:125072
1362:124448
1357:121504
1352:121228
1342:117207
1337:116434
1332:115600
1327:114729
1322:114386
1317:113766
1312:113538
1307:110113
1302:109749
1297:108236
1292:107914
1287:103197
1277:101930
1272:100453
597:
567:: 92.
544:
536:
500:Nature
469:
310:Nature
263:SPHERE
63:SPHERE
44:SPHERE
1896:Other
1765:4650A
1386:Other
1267:98176
1262:97413
1016:V1400
1011:V1369
1006:V1032
858:4 (h)
853:3 (k)
848:2 (g)
843:1 (i)
675:Bayer
666:Stars
595:S2CID
569:arXiv
542:S2CID
508:arXiv
467:S2CID
441:arXiv
180:1.11
1887:5419
1882:5408
1877:5398
1872:5291
1867:5253
1862:5161
1852:5114
1847:5102
1842:5091
1837:5090
1832:5026
1820:5011
1815:4976
1810:4945
1805:4744
1800:4743
1795:4730
1790:4729
1785:4709
1780:4706
1775:4696
1770:4683
1760:4622
1755:4603
1750:4444
1745:3783
1229:5371
1219:5297
1214:5241
1209:5224
1154:4989
1149:4979
1114:4796
1094:4721
1059:4523
1054:4522
1049:4499
996:V863
991:V886
986:V885
981:V842
976:V831
966:V810
961:V803
956:V779
951:V766
936:V752
931:V744
926:V346
534:PMID
199:10.9
194:Mass
158:Star
136:2650
132:7170
72:2021
1737:NGC
587:doi
565:382
526:doi
504:600
459:doi
437:646
203:1.6
152:128
148:157
119:0.4
104:556
40:VLT
2035::
1254:HD
1026:HR
921:DY
916:BV
911:SX
906:SV
901:RR
593:.
585:.
577:.
563:.
540:.
532:.
524:.
516:.
502:.
479:^
465:.
457:.
449:.
435:.
409:.
245:.
108:17
1825:A
1630:Ļ
1554:d
1549:c
1504:c
896:Y
891:V
886:U
881:T
876:R
825:Ļ
820:Ļ
815:Ļ
810:Ļ
805:Ļ
800:Ļ
795:Ļ
790:Ļ
785:Ļ
780:Īæ
775:Īæ
770:Ī¾
765:Ī¾
760:Ī½
755:Ī¼
750:Ī»
745:Īŗ
740:Ī¹
730:Ī·
720:Īµ
715:Ī“
683:Ī±
632:e
625:t
618:v
601:.
589::
581::
571::
548:.
528::
520::
510::
473:.
461::
453::
443::
419:.
376:M
369:M
302:M
295:M
288:M
210:J
207:M
201:Ā±
186:J
183:R
150:Ā±
134:Ā±
106:Ā±
42:/
23:.
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