2144:
837:. Even after the brown dwarf was accounted for, the star still showed a drift in the radial velocity measurements, suggesting another companion in a longer-period orbit. In 2004 after further observations, the parameters of a proposed companion was announced.
806:-rich star – what astronomers term the abundance of elements of higher atomic number than helium – which may explain the star's unusually high luminosity for its class. The star has a slightly greater mass and radius compared to the Sun.
840:
Further observation of this system revised this picture in 2017, showing that the system instead consisted of a pair of co-orbiting stars being viewed nearly face-on, with the pair being orbited in turn by a Super-Jupiter designated
1330:
Udry, S.; et al. (2002). "The CORALIE survey for southern extra-solar planets VIII. The very low-mass companions of HD 141937, HD 162020, HD 168443, HD 202206: Brown dwarfs or "superplanets"?".
712:
1307:
550:
1411:
Correia, A.; et al. (2005). "The CORALIE survey for southern extra-solar planets. XIII. A pair of planets around HD202206 or a circumbinary planet?".
2191:
1524:
2171:
2166:
1489:
1544:
2186:
31:
874:
1258:"Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs"
1389:
799:
605:
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1471:
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1025:
2196:
1413:
1332:
1852:
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1012:
784:
757:
1066:
1480:
2075:
2070:
1898:
788:
704:
385:
99:
2176:
2042:
1870:
1729:
698:
558:
336:
2181:
2147:
1510:
1432:
1351:
1269:
1219:
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1133:
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830:
296:
213:
905:
708:
1699:
1669:
1664:
1609:
1448:
1422:
1367:
1341:
1235:
1209:
1151:
1123:
1034:
234:
76:
1988:
1639:
1584:
1576:
1568:
1297:
880:
733:
633:
361:
27:
1719:
1684:
1634:
1624:
1604:
1599:
1440:
1436:
1359:
1355:
1277:
1227:
1141:
1054:
1049:
773:
597:
518:
197:
1694:
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1629:
1614:
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1589:
1493:
1486:
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818:
795:
777:
531:
276:
138:
52:
1273:
1223:
1181:
1137:
2119:
1714:
1709:
1704:
1679:
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1619:
973:
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689:
408:
262:
205:
185:
173:
1496:
by Rory Barnes & Richard
Greenberg, Lunar and Planetary Lab, University of Arizona
2160:
1842:
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1674:
1649:
1644:
1239:
1155:
749:
162:
39:
1452:
2101:
2006:
1983:
1860:
1742:
1737:
1371:
935:
792:
660:
488:
444:
1059:
1016:
1444:
1363:
1978:
1973:
1968:
1963:
918:
846:
842:
822:
803:
753:
745:
583:
375:
315:
110:
65:
44:
1502:
1146:
1111:
2019:
2014:
1231:
1200:
Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".
765:
677:
501:
458:
358:
220:
126:
1955:
1937:
1916:
1906:
1888:
1883:
1878:
1468:
850:
845:. The secondary stellar companion, now designated component B rather than '
1385:
2080:
2065:
2060:
2055:
2050:
1427:
1346:
798:. It is an estimated three billion years old and is spinning with a
647:
2096:
826:
2127:
2033:
1932:
1302:
1174:
Michigan
Catalogue of Two-dimensional Spectral Types for the HD Stars
1070:
910:
727:
575:
471:
225:
1282:
1257:
1128:
1039:
1214:
761:
254:
1559:
869:
189:
177:
1506:
1021:
Data
Release 2: Summary of the contents and survey properties"
893:
834:
769:
1110:
Benedict, G. Fritz; Harrison, Thomas E. (June 2017).
821:
measurements of the star revealed the existence of a
2118:
2089:
2041:
2032:
2005:
1954:
1925:
1897:
1869:
1851:
1728:
1567:
1558:
791:of G6V, indicating it is generating energy through
16:
1015:; et al. (Gaia collaboration) (August 2018).
1105:
1103:
1101:
1099:
1195:
1193:
1191:
1112:"HD 202206: A Circumbinary Brown Dwarf System"
1097:
1095:
1093:
1091:
1089:
1087:
1085:
1083:
1081:
1079:
760:of +8.1, it is too faint to be visible to the
1518:
1308:Centre de données astronomiques de Strasbourg
825:companion with at least 17 times the mass of
764:eye. It is located at a distance of 150
70:−20° 47′ 21.1624″
8:
1256:Valenti, Jeff A.; Fischer, Debra A. (2005).
1262:The Astrophysical Journal Supplement Series
30:J2000.0
2115:
2038:
2002:
1951:
1564:
1525:
1511:
1503:
1167:
1165:
1426:
1345:
1281:
1251:
1249:
1213:
1145:
1127:
1058:
1048:
1038:
1007:
1005:
1003:
1001:
999:
997:
995:
993:
855:
989:
853:star with 8.9% of the mass of the Sun.
169:
1325:
1323:
776:, and is drifting further away with a
18:
7:
1388:(Press release). Garching, Germany:
181:
1172:Houk, N.; Smith-Moore, M. (1988).
833:orbit with a period of around 256
14:
2143:
2142:
1545:Capricornus in Chinese astronomy
1481:Extrasolar Planets Encyclopaedia
204:21.7264 ± 0.0651
1067:Gaia DR2 record for this source
857:The HD 202206 planetary system
2192:Henry Draper Catalogue objects
1487:Extrasolar Planet Interactions
1:
1390:European Southern Observatory
800:projected rotational velocity
1550:List of stars in Capricornus
1534:Constellation of Capricornus
1026:Astronomy & Astrophysics
909:
904:
899:
886:
873:
868:
861:
1060:10.1051/0004-6361/201833051
783:The primary component is a
2213:
2172:M-type main-sequence stars
2167:G-type main-sequence stars
1445:10.1051/0004-6361:20042376
1414:Astronomy and Astrophysics
1364:10.1051/0004-6361:20020685
1333:Astronomy and Astrophysics
802:of 2.3 km/s. It is a
2140:
2114:
2001:
1950:
1540:
1232:10.1134/S1063773712050015
785:G-type main-sequence star
758:apparent visual magnitude
720:
695:
688:
653:
437:
432:
253:
249:
132:
125:
93:
24:
1147:10.3847/1538-3881/aa6d59
1116:The Astronomical Journal
1437:2005A&A...440..751C
1356:2002A&A...390..267U
1050:2018A&A...616A...1G
748:system in the southern
235:Absolute magnitude
77:Apparent magnitude
2187:Durchmusterung objects
829:around the star in an
789:stellar classification
386:Argument of periastron
817:In 2000, analysis of
337:Longitude of the node
1386:"Exoplanets Galore!"
865:(in order from star)
780:of +14.7 km/s.
184: −119.999
1274:2005ApJS..159..141V
1224:2012AstL...38..331A
1182:1988mcts.book.....H
1138:2017AJ....153..258B
858:
721:Database references
606:Rotational velocity
172: −39.079
21:
1492:2016-05-05 at the
1474:2012-05-27 at the
856:
690:Other designations
100:Spectral type
19:
2197:Hipparcos objects
2154:
2153:
2136:
2135:
2110:
2109:
2028:
2027:
1997:
1996:
1946:
1945:
1202:Astronomy Letters
982:
981:
897:
884:
866:
739:
738:
224:(46.0 ± 0.1
219:150.1 ± 0.4
2204:
2146:
2145:
2116:
2039:
2003:
1952:
1605:δ (Deneb Algedi)
1565:
1527:
1520:
1513:
1504:
1457:
1456:
1430:
1428:astro-ph/0411512
1408:
1402:
1401:
1399:
1397:
1392:. April 15, 2000
1382:
1376:
1375:
1349:
1347:astro-ph/0202458
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269:256.33 days
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94:Characteristics
89:
87:
80:
60:
55:
25:Observation data
22:
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2207:
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2201:
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2120:Galaxy clusters
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1993:
1942:
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1494:Wayback Machine
1476:Wayback Machine
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1199:
1198:
1189:
1176:. Vol. 4.
1171:
1170:
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1109:
1108:
1077:
1013:Brown, A. G. A.
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863:
819:radial velocity
815:
809:
796:hydrogen fusion
778:radial velocity
716:
697:
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671:
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641:
639:
622:
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612: sin
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532:Surface gravity
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277:Semi-major axis
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139:Radial velocity
117:
115:
85:
83:
75:
58:
53:Right ascension
51:
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5:
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1463:External links
1461:
1459:
1458:
1421:(2): 751–758.
1403:
1377:
1340:(1): 267–279.
1319:
1289:
1283:10.1086/430500
1268:(1): 141–166.
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2007:Star clusters
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40:Constellation
38:
37:
33:
29:
23:
2177:Brown dwarfs
2102:PKS 2126-158
1984:HD 202772 Ab
1911:
1578:
1499:
1479:
1418:
1412:
1406:
1396:December 30,
1394:. Retrieved
1380:
1337:
1331:
1311:. Retrieved
1301:
1292:
1265:
1261:
1205:
1201:
1173:
1119:
1115:
1030:
1024:
1018:
917:
901:Eccentricity
839:
816:
808:
782:
741:
740:
726:
659:
632:
613:
609:
604:
582:
557:
535:
530:
500:
470:
443:
407:
384:
370:2,452,176.14
357:
335:
314:
297:Eccentricity
295:
275:
261:
233:
212:
196:
161:
137:
2182:Capricornus
1979:HD 204313 b
1974:HD 202206 c
1964:HD 192310 b
1600:γ (Nashira)
1298:"HD 202206"
906:Inclination
843:HD 202206 c
823:brown dwarf
766:light years
754:Capricornus
746:binary star
584:Metallicity
559:Temperature
392:(secondary)
316:Inclination
111:color index
66:Declination
45:Capricornus
2161:Categories
2020:Palomar 12
2015:Messier 30
1956:Exoplanets
1650:ν (Alshat)
1585:α (Algedi)
1313:2020-07-05
1208:(5): 331.
1129:1705.00659
1040:1804.09365
985:References
813:Companions
756:. With an
627: km/s
534:(log
502:Luminosity
374:0.12
359:Periastron
156: km/s
127:Astrometry
104:G6V + M8V
20:HD 202206
1938:LP 816-60
1730:Flamsteed
1590:β (Dabih)
1469:HD 202206
1240:119257644
1215:1108.4971
1156:119105717
1122:(6): 12.
862:Companion
851:red dwarf
831:eccentric
772:based on
768:from the
742:HD 202206
701:−21° 5972
418:(primary)
79: (V)
2148:Category
2034:Galaxies
1853:Variable
1490:Archived
1472:Archived
1453:16175663
849:', is a
774:parallax
682:☉
523:☉
493:☉
463:☉
237: (M
214:Distance
198:Parallax
34:J2000.0
2097:IC 1337
1433:Bibcode
1372:9389274
1352:Bibcode
1270:Bibcode
1220:Bibcode
1178:Bibcode
1134:Bibcode
1045:Bibcode
827:Jupiter
787:with a
433:Details
32:Equinox
2128:HCG 87
1933:HATS-3
1917:204313
1912:202206
1907:197027
1838:47 (c)
1833:46 (c)
1803:36 (b)
1768:24 (A)
1451:
1370:
1303:SIMBAD
1238:
1158:. 258.
1154:
1071:VizieR
1033:. A1.
934:
911:Radius
728:SIMBAD
676:
672:−0.006
670:+0.007
646:
596:
574:
549:
517:
513:−0.005
511:+0.004
487:
472:Radius
457:
402:°
351:°
329:°
263:Period
150:+14.68
2090:Other
2076:7035A
1926:Other
1569:Bayer
1560:Stars
1449:S2CID
1423:arXiv
1368:S2CID
1342:arXiv
1236:S2CID
1210:arXiv
1152:S2CID
1124:arXiv
1065:
1035:arXiv
949:1,260
945:2.41
804:metal
762:naked
744:is a
667:0.089
565:5,735
508:1.084
483:−0.03
481:+0.02
426:0.001
422:0.567
396:161.9
362:epoch
308:0.001
304:0.432
255:Orbit
245:+4.80
182:Dec.:
120:0.012
116:0.714
84:+8.07
28:Epoch
2081:7073
2071:7035
2066:7030
2061:7019
2056:7016
2051:6907
1889:7898
1884:7845
1879:7722
1398:2012
1019:Gaia
962:0.03
958:0.22
930:−1.8
928:+2.9
925:17.9
894:days
870:Mass
835:days
793:core
734:data
661:Mass
594:0.01
590:0.29
478:1.05
455:0.08
451:1.07
445:Mass
428:km/s
323:10.9
285:1.40
154:0.23
109:B−V
88:0.01
2043:NGC
1478:on
1441:doi
1419:440
1360:doi
1338:390
1278:doi
1266:159
1228:doi
1142:doi
1120:153
1069:at
1055:doi
1031:616
971:1.1
967:7.7
770:Sun
752:of
713:SAO
709:HIP
648:Gyr
644:1.0
640:2.9
634:Age
625:0.5
621:2.3
598:dex
570:−74
568:+76
551:cgs
547:0.1
543:4.5
400:0.2
388:(ω)
364:(T)
345:121
339:(Ω)
327:0.8
318:(i)
299:(e)
279:(a)
265:(P)
206:mas
200:(π)
186:mas
174:mas
170:RA:
165:(μ)
2163::
1899:HD
1871:HR
1843:50
1828:45
1823:44
1818:42
1813:41
1808:37
1798:35
1793:33
1788:31
1783:30
1778:29
1773:27
1763:21
1758:20
1753:19
1748:17
1577:α
1447:.
1439:.
1431:.
1417:.
1366:.
1358:.
1350:.
1336:.
1322:^
1306:.
1300:.
1276:.
1264:.
1260:.
1248:^
1234:.
1226:.
1218:.
1206:38
1204:.
1190:^
1164:^
1150:.
1140:.
1132:.
1118:.
1114:.
1078:^
1053:.
1043:.
1029:.
1023:.
992:^
978:—
953:11
881:AU
705:HD
703:,
699:BD
412:(K
376:JD
226:pc
221:ly
190:yr
178:yr
141:(R
1969:c
1861:R
1743:4
1738:3
1720:ω
1715:ψ
1710:χ
1705:φ
1700:υ
1695:τ
1690:τ
1685:σ
1680:ρ
1675:π
1670:ο
1665:ο
1660:ξ
1655:ξ
1645:μ
1640:λ
1635:κ
1630:ι
1625:θ
1620:η
1615:ζ
1610:ε
1595:β
1526:e
1519:t
1512:v
1455:.
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1435::
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1374:.
1362::
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1344::
1316:.
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1280::
1272::
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1222::
1212::
1184:.
1180::
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1136::
1126::
1073:.
1063:.
1057::
1047::
1037::
1017:"
974:°
969:±
960:±
951:±
940:J
937:M
919:c
896:)
892:(
883:)
879:(
847:b
679:M
654:B
642:±
623:±
616:)
614:i
610:v
608:(
592:±
576:K
545:±
538:)
536:g
520:L
490:R
460:M
453:±
438:A
424:±
416:)
414:1
398:±
372:±
349:4
347:±
325:±
306:±
287:±
241:)
239:V
228:)
188:/
176:/
152:±
145:)
143:v
118:±
86:±
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