603:
27:
2627:
591:
653:
Chauvin, G.; Desidera, S.; Lagrange, A. -M.; Vigan, A.; Gratton, R.; Langlois, M.; Bonnefoy, M.; Beuzit, J. -L.; Feldt, M.; Mouillet, D.; Meyer, M.; Cheetham, A.; Biller, B.; Boccaletti, A.; d'Orazi, V.; Galicher, R.; Hagelberg, J.; Maire, A. -L.; Mesa, D.; Olofsson, J.; Samland, M.; Schmidt, T. O.
837:
Petrus, S.; Bonnefoy, M.; Chauvin, G.; Charnay, B.; Marleau, G.-D.; Gratton, R.; Lagrange, A.-M.; Rameau, J.; Mordasini, C.; Nowak, M.; Delorme, P.; Boccaletti, A.; Carlotti, A.; Houllé, M.; Vigan, A.; Allard, F.; Desidera, S.; d'Orazi, V.; Hoeijmakers, H. J.; Wyttenbach, A.; Lavie, B. (2021),
782:
Carter, Aarynn L.; Hinkley, Sasha; Kammerer, Jens; Skemer, Andrew; Biller, Beth A.; Leisenring, Jarron M.; Millar-Blanchaer, Maxwell A.; Petrus, Simon; Stone, Jordan M.; Ward-Duong, Kimberly; Wang, Jason J.; Girard, Julien H.; Hines, Dean C.; Perrin, Marshall D.; Pueyo, Laurent (2023-07-06).
535:
HIP 65426 b is the first exoplanet to be imaged by JWST and the first exoplanet to be detected beyond 5 μm. The observations demonstrate that the James Webb Space
Telescope will exceed its nominal predicted performance by a factor of 10 and that it will be able to image 0.3
511:
654:
B.; Sissa, E.; Bonavita, M.; Charnay, B.; Cudel, M.; Daemgen, S.; Delorme, P.; Janin-Potiron, P.; et al. (2017). "Discovery of a warm, dusty giant planet around HIP 65426".
309:
31:
HIP 65426 b is on the lower left of the image, with the circle representing what
Neptune's orbit would look like around the star HIP 65426, represented by a small cross.
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785:"The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High Contrast Imaging of the Exoplanet HIP 65426 b from 2-16 μm"
1112:
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374:. The planet is around 14 million years old. However, it is not associated with a debris disk, despite its young age, causing it to not fit
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520:. The atmospheric fitting of both temperature and radius are in disagreement with evolutionary models. The team also constrained the
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of the planet, but the new JWST astrometry of the planet did not significantly improve the orbit of the planet, especially the
428:(JWST) observations was published. The JWST direct imaging observations between 2-16 μm of HIP 65426 b tightly constrained its
69:
63:
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The spectrum taken in 2020 has indicated that HIP 65426 b is carbon-poor and oxygen-rich compared to Solar System gas giants.
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Spectral analysis of data from the James Webb Space
Telescope revealed strong evidence of silicate clouds containing
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The exoplanet HIP 65426 b orbits its host star HIP 65426, an A2V star with apparent magnitude 7.01 and a mass of
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47:
1049:"Odd planetary system around fast-spinning star doesn't quite fit existing models of planet formation"
708:"Odd planetary system around fast-spinning star doesn't quite fit existing models of planet formation"
328:
In August 2022, this planet and its host star were included among 20 systems to be named by the third
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891:"Scientists have found a planet that means everything they thought about planets isn't true"
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919:"Astronomers Directly Image Super-Jupiter around HIP 65426 | Astronomy | Sci-News.com"
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In
September 2022, HIP 65426 b became the first exoplanet directly observed by the
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HIP 65426. It was discovered on 6 July 2017 by the SPHERE consortium using the
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1142:"Spectral Retrieval with JWST Photometric data: a Case Study for HIP 65426 b"
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from Earth. It is the first planet discovered by ESO's SPHERE instrument.
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2013:
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2018:
1724:
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1200:"James Webb Discovery - First Direct Image of Exoplanet - HIP 65426 b"
386:. It was discovered as part of the SHINE program, which aimed to find
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2023:
2008:
1616:
566:
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333:
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1158:
852:
801:
668:
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1120:
1113:"NASA's Webb Takes Its First-Ever Direct Image of Distant World"
305:
193:
1223:
838:"Medium-resolution spectrum of the exoplanet HIP 65426 B",
370:. This planetary system is located in the constellation
950:
513:, which provides a robust mass constraint of 7.1±1.1
438:
332:
project. The approved names, proposed by a team from
310:
Spectro-Polarimetric High-Contrast
Exoplanet Research
336:, were announced in June 2023. HIP 65426 b is named
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2506:
2346:
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2186:
2070:
1996:
1863:
1635:
1477:
1444:
1284:
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1025:"The Extrasolar Planet Encyclopaedia — HIP 65426 b"
506:{\displaystyle \log(L_{bol}/L_{sun})=-4.23\pm 0.02}
233:
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150:
145:
123:
101:
94:
82:
75:
61:
53:
41:
36:
1072:Johnson-Groh, Mara; July 12, 2017 (12 July 2017).
946:"Holiday Special: Eight nights of Exoplanet Light"
505:
777:
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773:
771:
769:
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648:
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8:
832:
830:
573:JWST might be able to push the limit to a 5
382:from its parent star, with a possible dusty
19:
1096:: CS1 maint: numeric names: authors list (
1074:"New exoplanet challenges formation models"
2588:
2557:
2343:
2264:
2183:
2067:
1281:
1242:
1228:
1220:
971:"ESO's SPHERE Unveils its First Exoplanet"
25:
1175:
1157:
913:
911:
851:
818:
800:
731:
729:
727:
667:
569:-mass objects at 10 au for M-dwarfs. For
473:
464:
452:
437:
412:with no evidence of a dusty atmosphere.
16:Hot Jupiter exoplanet orbiting HIP 65426
642:
416:James Webb Space Telescope observations
1089:
940:
938:
376:current models for planetary formation
18:
2650:Exoplanets detected by direct imaging
631:List of exoplanets discovered in 2017
348:words for "Mother Earth" and "star".
312:(SPHERE) instrument belonging to the
7:
923:Breaking Science News | Sci-News.com
14:
789:The Astrophysical Journal Letters
2626:
2625:
1030:Extrasolar Planets Encyclopaedia
601:
589:
561:-mass objects at 100-200 au for
2246:Scorpius–Centaurus association
1267:Centaurus in Chinese astronomy
485:
445:
1:
2655:Exoplanets discovered in 2017
314:European Southern Observatory
2670:Exoplanets with proper names
1111:Fisher, Alise (2022-09-01).
840:Astronomy & Astrophysics
1140:Wang 王, Ji 吉 (2023-11-01).
870:10.1051/0004-6361/202038914
686:10.1051/0004-6361/201731152
340:and its host star is named
2686:
1262:List of stars in Centaurus
1251:Constellation of Centaurus
1204:www.jameswebbdiscovery.com
656:Astronomy and Astrophysics
610:James Webb Space Telescope
608:HIP 65426 b viewed by the
426:James Webb Space Telescope
395:James Webb Space Telescope
2623:
2587:
2556:
2263:
2182:
2066:
1257:
582:planet at 0.5 to 2.5 au.
284:
24:
20:HIP 65426 b / Najsakopajk
1582:V816 (Przybylski's Star)
1177:10.3847/1538-3881/acfca0
1146:The Astronomical Journal
995:"List of ExoWorlds 2022"
820:10.3847/2041-8213/acd93e
146:Physical characteristics
862:2021A&A...648A..59P
678:2017A&A...605L...9C
532:remains unconstrained.
96:Orbital characteristics
507:
390:around 600 new stars.
999:nameexoworlds.iau.org
741:nameexoworlds.iau.org
737:"2022 Approved Names"
508:
430:bolometric luminosity
2575:Shapley Supercluster
2312:Southern Crab Nebula
2029:PSR B1259−63/LS 2883
1309:C (Proxima Centauri)
436:
401:Planetary atmosphere
2593:Astronomical events
1299:A (Rigil Kentaurus)
1168:2023AJ....166..203W
811:2023ApJ...951L..20C
626:Lists of exoplanets
551:main-sequence stars
266:Evolutionary model:
174:Evolutionary model:
54:Discovery date
21:
2468:5128 (Centaurus A)
2155:Proxima Centauri b
712:www.sphere.osug.fr
596:HIP 65426 star map
503:
420:In August 2022, a
378:. It is around 92
239:Atmospheric model:
158:Atmospheric model:
43:Discovered by
2637:
2636:
2619:
2618:
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2582:
2552:
2551:
2333:
2332:
2321:
2259:
2258:
2178:
2177:
2062:
2061:
2039:WASP-15 (Nyamien)
1035:Paris Observatory
388:planetary systems
316:(ESO). It is 385
293:, formally named
288:
287:
85:Alternative names
48:SPHERE consortium
2677:
2629:
2628:
2589:
2558:
2344:
2319:
2277:Boomerang Nebula
2265:
2184:
2068:
2054:WASP-167/KELT-13
2004:2MASS J1126−5003
1282:
1244:
1237:
1230:
1221:
1214:
1213:
1211:
1210:
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1190:
1189:
1179:
1161:
1137:
1131:
1130:
1128:
1127:
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1101:
1095:
1087:
1085:
1084:
1069:
1063:
1062:
1060:
1059:
1045:
1039:
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1021:
1015:
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991:
985:
984:
982:
981:
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960:
958:
957:
942:
933:
932:
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929:
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906:
905:
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902:
887:
881:
880:
855:
834:
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824:
822:
804:
779:
756:
755:
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733:
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721:
719:
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698:
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650:
605:
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369:
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228:
226:
204:
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182:
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166:
164:
138:
137:
136:
118:
117:
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64:Detection method
29:
22:
2685:
2684:
2680:
2679:
2678:
2676:
2675:
2674:
2640:
2639:
2638:
2633:
2615:
2579:
2562:Galaxy clusters
2548:
2534:IRAS 13224-3809
2502:
2329:
2255:
2174:
2058:
1992:
1958:117618 (Dofida)
1859:
1631:
1473:
1440:
1271:
1253:
1248:
1218:
1217:
1208:
1206:
1198:
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1139:
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1125:
1123:
1110:
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1088:
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1080:
1071:
1070:
1066:
1057:
1055:
1047:
1046:
1042:
1023:
1022:
1018:
1008:
1006:
1005:. 8 August 2022
993:
992:
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979:
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968:
964:
955:
953:
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943:
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895:The Independent
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622:
617:
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613:
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598:
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594:
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545:planets at 100
543:
540:
522:semi-major axis
519:
516:
469:
448:
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418:
403:
368:
359:
357:
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326:
273:
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264:
257:
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217:Surface gravity
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134:
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104:Semi-major axis
87:
66:
32:
17:
12:
11:
5:
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2074:
2064:
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2046:
2041:
2036:
2034:PSR J1311–3430
2031:
2026:
2021:
2016:
2011:
2006:
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1893:102117 (Uklun)
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1016:
986:
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826:
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723:
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641:
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621:
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541:
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73:
72:
70:Direct imaging
67:
62:
59:
58:
55:
51:
50:
45:
39:
38:
34:
33:
30:
15:
13:
10:
9:
6:
4:
3:
2:
2682:
2671:
2668:
2666:
2663:
2661:
2660:Giant planets
2658:
2656:
2653:
2651:
2648:
2647:
2645:
2632:
2622:
2612:
2609:
2607:
2604:
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2599:
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2239:
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2227:
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2222:
2219:
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2214:
2212:
2209:
2207:
2204:
2202:
2199:
2197:
2194:
2193:
2191:
2189:
2188:Star clusters
2185:
2181:
2171:
2168:
2166:
2163:
2161:
2158:
2156:
2153:
2151:
2148:
2146:
2143:
2141:
2138:
2136:
2133:
2131:
2128:
2126:
2123:
2121:
2118:
2116:
2113:
2111:
2108:
2106:
2103:
2101:
2098:
2096:
2093:
2091:
2088:
2086:
2083:
2081:
2078:
2077:
2075:
2073:
2069:
2065:
2055:
2052:
2050:
2047:
2045:
2042:
2040:
2037:
2035:
2032:
2030:
2027:
2025:
2022:
2020:
2017:
2015:
2012:
2010:
2007:
2005:
2002:
2001:
1999:
1995:
1989:
1986:
1984:
1981:
1979:
1976:
1974:
1971:
1969:
1966:
1964:
1961:
1959:
1956:
1954:
1951:
1949:
1946:
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1941:
1939:
1936:
1934:
1931:
1929:
1926:
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1921:
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1916:
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1911:
1909:
1906:
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1901:
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1879:
1876:
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1813:
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1808:
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1803:
1801:
1798:
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1600:
1598:
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1570:
1568:
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1359:
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1354:
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1349:
1347:
1344:
1342:
1339:
1337:
1334:
1332:
1329:
1327:
1324:
1322:
1321:γ (Muhlifain)
1319:
1317:
1314:
1310:
1307:
1305:
1302:
1300:
1297:
1296:
1295:
1292:
1291:
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1287:
1283:
1280:
1278:
1274:
1268:
1265:
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1226:
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1205:
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1192:
1187:
1183:
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1169:
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1133:
1122:
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1114:
1107:
1104:
1099:
1093:
1079:
1078:Astronomy.com
1075:
1068:
1065:
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1044:
1041:
1036:
1032:
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1026:
1020:
1017:
1004:
1000:
996:
990:
987:
976:
972:
966:
963:
951:
947:
941:
939:
935:
924:
920:
914:
912:
908:
896:
892:
886:
883:
879:
875:
871:
867:
863:
859:
854:
849:
845:
841:
833:
831:
827:
821:
816:
812:
808:
803:
798:
794:
790:
786:
778:
776:
774:
772:
770:
768:
766:
764:
762:
758:
746:
742:
738:
732:
730:
728:
724:
713:
709:
703:
700:
695:
691:
687:
683:
679:
675:
670:
665:
661:
657:
649:
647:
643:
636:
632:
629:
627:
624:
623:
619:
612:(August 2022)
611:
604:
592:
583:
581:
572:
568:
564:
560:
556:
552:
548:
544:
533:
531:
527:
523:
500:
497:
494:
491:
488:
480:
477:
474:
470:
465:
459:
456:
453:
449:
442:
439:
431:
427:
423:
415:
413:
411:
406:
400:
398:
396:
391:
389:
385:
381:
377:
373:
365:
351:
349:
347:
343:
339:
335:
331:
330:NameExoWorlds
323:
321:
319:
315:
311:
307:
304:orbiting the
303:
300:
299:super-Jupiter
296:
292:
283:
280:
265:
263:
253:
238:
236:
232:
221:
218:
213:
210:
197:
195:
191:
188:
172:
157:
154:
149:
144:
141:
128:
126:
122:
108:
105:
100:
97:
93:
89:
86:
81:
78:
74:
71:
68:
65:
60:
56:
52:
49:
46:
44:
40:
35:
28:
23:
2544:PKS 1353−341
2539:PKS 1144-379
2519:ESO 325-G004
2144:
2085:b Centauri b
1207:. Retrieved
1203:
1194:
1149:
1145:
1135:
1124:. Retrieved
1116:
1106:
1081:. Retrieved
1077:
1067:
1056:. Retrieved
1052:
1043:
1028:
1019:
1007:. Retrieved
998:
989:
978:. Retrieved
974:
965:
954:. Retrieved
949:
926:. Retrieved
922:
899:. Retrieved
897:. 2017-07-08
894:
885:
843:
839:
792:
788:
748:. Retrieved
740:
715:. Retrieved
711:
702:
659:
655:
534:
530:eccentricity
419:
407:
404:
392:
363:
355:
341:
337:
327:
324:Nomenclature
294:
290:
289:
255:
77:Designations
2150:HIP 67522 b
2145:HIP 65426 b
2140:HD 121504 b
2135:HD 117618 b
2130:HD 117207 b
2125:HD 114729 b
2120:HD 114386 b
2110:HD 113538 b
2105:HD 101930 b
2100:HD 109749 b
2095:HD 103197 b
2090:HD 102117 b
1346:θ (Menkent)
1304:B (Toliman)
975:www.eso.org
526:inclination
338:Najsakopajk
318:light-years
295:Najsakopajk
291:HIP 65426 b
235:Temperature
153:Mean radius
125:Inclination
90:Najsakopajk
57:6 July 2017
2644:Categories
2570:Abell S740
2529:ESO 444-46
2524:ESO 383-76
2514:ESO 269-57
2287:G292.0+1.8
2072:Exoplanets
1336:ζ (Alnair)
1209:2024-02-20
1159:2310.00089
1152:(5): 203.
1126:2022-09-01
1117:NASA Blogs
1083:2019-08-03
1058:2019-08-03
980:2017-07-07
956:2019-08-03
928:2019-08-02
901:2019-08-02
853:2012.02798
802:2208.14990
795:(1): L20.
717:2017-07-06
669:1707.01413
637:References
384:atmosphere
362:0.04
2665:Centaurus
2282:Fleming 1
1446:Flamsteed
1316:β (Hadar)
1186:0004-6256
1009:27 August
878:227347064
694:102344893
498:±
492:−
443:
422:pre-print
410:enstatite
372:Centaurus
302:exoplanet
37:Discovery
2631:Category
2611:SN 1986G
2606:SN 1895B
2339:Galaxies
2320:(RCW 86)
2302:NGC 5307
2297:NGC 3918
2251:Stock 16
2236:NGC 5662
2231:NGC 5617
2226:NGC 5460
2221:NGC 5316
2216:NGC 5281
2211:NGC 5286
2206:NGC 4230
2201:NGC 3766
2170:WASP-15b
2014:Gaia BH2
1855:5489 (c)
1850:5485 (c)
1845:5471 (b)
1835:5358 (v)
1815:5222 (y)
1810:5207 (N)
1805:5174 (z)
1800:5172 (M)
1795:5141 (Q)
1790:5089 (d)
1785:5071 (K)
1780:5041 (m)
1775:5035 (J)
1770:5006 (r)
1755:4940 (f)
1750:4889 (n)
1745:4888 (e)
1740:4874 (p)
1735:4831 (w)
1730:4817 (l)
1720:4748 (u)
1715:4732 (G)
1710:4724 (x)
1700:4712 (x)
1695:4682 (F)
1690:4652 (D)
1685:4620 (E)
1680:4546 (B)
1675:4537 (j)
1655:4476 (C)
1650:4466 (C)
1645:4460 (A)
1612:V945 (H)
1557:V763 (C)
1552:V761 (a)
1479:Variable
1092:cite web
1053:phys.org
620:See also
563:M-dwarfs
524:and the
367:☉
352:Overview
344:, after
2292:IC 2944
2269:Nebulae
2196:IC 2944
2080:2M1207b
2049:WASP-42
2044:WASP-41
2019:GJ 3737
1164:Bibcode
858:Bibcode
846:: A59,
807:Bibcode
674:Bibcode
571:α Cen A
555:Neptune
424:of the
297:, is a
2601:SN 185
2325:SuWt 2
2317:SN 185
2307:RCW 79
2024:J1407b
2009:2M1207
1988:131399
1983:125595
1978:125072
1973:124448
1968:121504
1963:121228
1953:117207
1948:116434
1943:115600
1938:114729
1933:114386
1928:113766
1923:113538
1918:110113
1913:109749
1908:108236
1903:107914
1898:103197
1888:101930
1883:100453
1184:
952:. NASA
876:
750:7 June
692:
662:: L9.
567:Saturn
559:Uranus
334:Mexico
2507:Other
2376:4650A
1997:Other
1878:98176
1873:97413
1627:V1400
1622:V1369
1617:V1032
1469:4 (h)
1464:3 (k)
1459:2 (g)
1454:1 (i)
1286:Bayer
1277:Stars
1154:arXiv
874:S2CID
848:arXiv
797:arXiv
690:S2CID
664:arXiv
346:Zoque
342:Matza
2498:5419
2493:5408
2488:5398
2483:5291
2478:5253
2473:5161
2463:5114
2458:5102
2453:5091
2448:5090
2443:5026
2431:5011
2426:4976
2421:4945
2416:4744
2411:4743
2406:4730
2401:4729
2396:4709
2391:4706
2386:4696
2381:4683
2371:4622
2366:4603
2361:4444
2356:3783
1840:5371
1830:5297
1825:5241
1820:5224
1765:4989
1760:4979
1725:4796
1705:4721
1670:4523
1665:4522
1660:4499
1607:V863
1602:V886
1597:V885
1592:V842
1587:V831
1577:V810
1572:V803
1567:V779
1562:V766
1547:V752
1542:V744
1537:V346
1182:ISSN
1121:NASA
1098:link
1011:2022
752:2023
565:and
557:and
549:for
501:0.02
495:4.23
358:1.96
306:star
269:1282
260:100
256:1560
242:1667
227:0.19
223:4.07
194:Mass
181:0.03
177:1.45
165:0.04
161:0.92
113:+108
2348:NGC
1172:doi
1150:166
1003:IAU
866:doi
844:648
815:doi
793:951
745:IAU
682:doi
660:605
440:log
432:to
274:−31
272:+26
247:−24
245:+25
229:dex
203:1.1
199:7.1
140:deg
133:+15
130:100
115:−31
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1865:HD
1637:HR
1532:DY
1527:BV
1522:SX
1517:SV
1512:RR
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168:R
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
