50:
57:
1361:
Metcalfe, Travis S.; Van Saders, Jennifer L.; Basu, Sarbani; Buzasi, Derek; Drake, Jeremy J.; Egeland, Ricky; Huber, Daniel; Saar, Steven H.; Stassun, Keivan G.; Ball, Warrick H.; Campante, Tiago L.; Finley, Adam J.; Kochukhov, Oleg; Mathur, Savita; Reinhold, Timo; See, Victor; Baliunas, Sallie;
738:
The evolution of the parent star, nearing the conclusion of its life cycle, has been regarded as a model for the potential evolution of our planetary system. This is especially relevant for predicting whether the Sun will eventually engulf the Earth at the end of its own lifecycle (cf.
1812:
Beichman, C. A.; Bryden, G.; Rieke, G. H.; Stansberry, J. A.; Trilling, D. E.; Stapelfeldt, K. R.; Werner, M. W.; Engelbracht, C. W.; et al. (2005). "Planets and
Infrared Excesses: Preliminary Results from a Spitzer MIPS Survey of Solar-Type Stars".
1937:
Marshall, J. P.; Moro-Martín, A.; Eiroa, C.; Kennedy, G.; Mora, A.; Sibthorpe, B.; Lestrade, J.-F.; Maldonado, J.; et al. (2014). "Correlations between the stellar, planetary, and debris components of exoplanet systems observed by
Herschel".
724:'s. A paper published in 2011 supported this claim using a new reduction of the astrometric data, with an updated mass value of 169.7 times Jupiter, with a 3σ confidence region 100.1 to 199.6 Jupiter masses. Such a massive body would be a dim
1628:
Reffert, S.; Quirrenbach, A. (2011). "Mass constraints on substellar companion candidates from the re-reduced
Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs".
677:
G0V. The star is thought to have 96 percent of the Sun's mass, along with 1.3 times its radius and 1.7 times its luminosity. It may only be 51 to 65 percent as enriched with elements heavier than
1327:
Fuhrmann, Klaus; Pfeiffer, Michael J.; Bernkopf, Jan (1998). "F- and G-type stars with planetary companions: Upsilon
Andromedae, rho (1) Cancri, tau Bootis, 16 Cygni and rho Coronae Borealis".
2702:
585:
581:
735:
to rule out any stellar companions to this star, in addition to detecting a second planetary companion in a 102-day orbit. Another two planets were discovered in 2023.
407:
688:
The rotation period of Rho
Coronae Borealis is approximately 20 days, even though at this age stars are hypothesized to decouple their rotational evolution and
2003:
720:
satellite data indicated that the orbital inclination of the star's companion was 0.5°, nearly face-on, implying that its mass was as much as 115 times
2102:
1089:
2132:
2662:
1866:
Bryden, G.; Beichman, C. A.; Carpenter, J. M.; Rieke, G. H.; Stapelfeldt, K. R.; Werner, M. W.; Tanner, A. M.; Lawler, S. M.; et al. (2009).
1076:
at 24- or 70-micrometre wavelengths, which would be expected if a disk were present. No evidence for a disk was detected in observations with the
2672:
573:
1101:
1095:
2127:
2677:
1908:
1744:
2122:
2022:
557:
2692:
78:
1769:
Trilling, D. E.; Brown, R. H.; Rivkin, A. S. (2000). "Circumstellar Dust Disks around Stars with Known
Planetary Companions".
2687:
764:
589:
2095:
480:
2017:
707:
An extrasolar planet in a 39.8-day orbit around Rho
Coronae Borealis was discovered in 1997 by observing the star's
2667:
2657:
2447:
2437:
1077:
711:
variations. This detection method only gives a lower limit on the true mass of the companion. In 2001, preliminary
2294:
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1517:
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2179:
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561:
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140:
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49:
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790:
256:
2347:
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2337:
2332:
2244:
2234:
2219:
1222:"EXPRES IV: Two Additional Planets Orbiting ρ Coronae Borealis Reveal Uncommon System Architecture"
795:
2042:
2327:
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2317:
2312:
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1973:
1947:
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277:
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31:
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689:
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74:
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459:
451:
375:
240:
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740:
708:
638:
388:
173:
99:
91:
1916:
1883:
1836:
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1711:
1604:
1557:
1438:
1389:
1300:
1249:
2582:
1892:
1867:
1534:
Noyes, Robert W.; et al. (1997). "A Planet
Orbiting the Star ρ Coronae Borealis".
777:
732:
549:
533:
248:
228:
212:
17:
2641:
1798:
1720:
1683:
1573:
1511:
1407:
1275:"Stellar diameters and temperatures - V. 11 newly characterized exoplanet host stars"
1180:
674:
670:
634:
197:
86:
1729:
1668:
2080:
1977:
1852:
884:
348:
307:
1969:
1868:"Planets and Debris Disks: Results from a Spitzer/MIPS Search for Infrared Excess"
1660:
1502:
1463:
1171:
1132:
2283:
717:
437:
151:
112:
2060:
1398:
1363:
1258:
1221:
2617:
2612:
2607:
2602:
2597:
2391:
1995:
1012:
945:
823:
696:
654:
626:
361:
321:
263:
161:
1589:"Preliminary Astrometric Masses for Proposed Extrasolar Planetary Companions"
685:) and is likely somewhat older than the Sun at around ten billion years old.
2483:
2420:
2370:
2365:
1364:"Magnetic and Rotational Evolution of ρ CrB from Asteroseismology with TESS"
1309:
1274:
725:
713:
658:
565:
2027:
2542:
2537:
2532:
2527:
2522:
2401:
2386:
1827:
1548:
678:
522:
56:
2568:
2563:
2396:
721:
2505:
1521:
1190:
800:
650:
630:
604:
429:
334:
268:
1844:
1790:
1702:
1613:
1588:
1565:
1484:
1447:
1422:
1380:
1240:
1153:
2491:
1952:
1643:
1291:
545:
695:
Multiple star catalogs list a 10th-magnitude companion about two
2406:
2142:
759:
682:
646:
232:
216:
2084:
783:
642:
471:
1468:
Data
Release 3. Summary of the content and survey properties"
1137:
Data
Release 3. Summary of the content and survey properties"
1745:"New Clues for What Will Happen When the Sun Eats the Earth"
1220:
Brewer, John M.; Zhao, Lily L.; et al. (June 2023).
1462:
Vallenari, A.; et al. (Gaia collaboration) (2023).
1131:
Vallenari, A.; et al. (Gaia collaboration) (2023).
1587:
Han, Inwoo; Black, David C.; Gatewood, George (2001).
2590:
2581:
2551:
2513:
2504:
2476:
2428:
2419:
2379:
2356:
2293:
2273:
2150:
2141:
1104:- Rho Coronae Borealis d and Rho Coronae Borealis e
731:In 2016, however, a paper was published that used
1996:"A Planet Orbiting the Star rho Coronae Borealis"
1682:Fulton, Benjamin J.; et al. (October 2016).
1279:Monthly Notices of the Royal Astronomical Society
1068:around the star. Follow-up observations with the
1909:"Catalog of withdrawn or refuted resolved Disks"
1684:"Three Temperate Neptunes Orbiting Nearby Stars"
699:away, but it is an unrelated background object.
2703:Planetary systems with four confirmed planets
2096:
117:+33° 18′ 12.6395″
8:
1215:
1213:
1211:
1209:
1207:
1205:
1203:
1201:
1199:
2004:Harvard-Smithsonian Center for Astrophysics
1423:"The Washington Visual Double Star Catalog"
641:. The star is thought to be similar to the
77:J2000.0
2587:
2510:
2425:
2147:
2103:
2089:
2081:
1356:
1354:
1352:
1350:
1322:
1320:
747:The Rho Coronae Borealis planetary system
1951:
1891:
1826:
1719:
1701:
1642:
1612:
1547:
1501:
1483:
1446:
1397:
1379:
1308:
1290:
1257:
1239:
1170:
1152:
1090:List of exoplanets discovered before 2000
27:Star in the constellation Corona Borealis
745:
66:Location of ρ Coronae Borealis (circled)
1913:Catalog of Resolved Circumstellar Disks
1273:von Braun, Kaspar; et al. (2014).
1114:
204:
36:
1126:
1124:
1122:
1120:
1118:
1102:List of exoplanets discovered in 2023
1096:List of exoplanets discovered in 2016
7:
2128:Corona Borealis in Chinese astronomy
1060:In October 1999, astronomers at the
2133:Hercules–Corona Borealis Great Wall
2000:Advanced Fiber Optic Echelle (AFOE)
220:
1421:Mason, B. D.; et al. (2014).
25:
1907:Caer McCabe & Carlotta Pham.
669:Rho Coronae Borealis is a yellow
621:(ρ CrB, ρ Coronae Borealis) is a
2123:List of stars in Corona Borealis
2112:Constellation of Corona Borealis
2023:Extrasolar Planets Encyclopaedia
247:57.1076 ± 0.0508
55:
48:
1518:Gaia DR3 record for this source
1187:Gaia DR3 record for this source
2663:Henry Draper Catalogue objects
657:. It is orbited by four known
1:
2673:Bright Star Catalogue objects
1064:announced the existence of a
1940:Astronomy & Astrophysics
1893:10.1088/0004-637X/705/2/1226
1631:Astronomy & Astrophysics
799:
794:
789:
776:
763:
758:
751:
1970:10.1051/0004-6361/201323058
1661:10.1051/0004-6361/201015861
1503:10.1051/0004-6361/202243940
1172:10.1051/0004-6361/202243940
681:(based on its abundance of
2719:
2678:G-type main-sequence stars
1721:10.3847/0004-637X/830/1/46
1472:Astronomy and Astrophysics
1329:Astronomy and Astrophysics
1141:Astronomy and Astrophysics
1078:Herschel Space Observatory
29:
2118:
1872:The Astrophysical Journal
1815:The Astrophysical Journal
1771:The Astrophysical Journal
1689:The Astrophysical Journal
1593:The Astrophysical Journal
1368:The Astrophysical Journal
597:
548: J16010264+3318124,
539:
532:
528:
301:
296:
292:
167:
160:
134:
71:
42:
2018:"Notes for star rho CrB"
1427:The Astronomical Journal
1399:10.3847/1538-4357/ac1f19
1259:10.3847/1538-3881/acdd6f
1227:The Astronomical Journal
1098:- Rho Coronae Borealis c
1092:- Rho Coronae Borealis b
30:Not to be confused with
1962:2014A&A...565A..15M
1743:O'Callaghan, Jonathan.
1653:2011A&A...527A.140R
1494:2023A&A...674A...1G
1341:1998A&A...336..942F
1163:2023A&A...674A...1G
1070:Spitzer Space Telescope
278:Absolute magnitude
124:Apparent magnitude
2693:Durchmusterung objects
2061:"Rho Coronae Borealis"
2043:"Rho Coronae Borealis"
1749:www.quantamagazine.org
1056:Circumstellar material
18:Rho Coronae Borealis c
2688:Gliese and GJ objects
1536:Astrophysical Journal
1362:Soon, Willie (2021).
1310:10.1093/mnras/stt2360
1072:failed to detect any
1062:University of Arizona
645:with nearly the same
2453:ρ Coronae Borealis b
2448:ο Coronae Borealis b
2443:κ Coronae Borealis b
2438:ε Coronae Borealis b
755:(in order from star)
728:star, not a planet.
619:Rho Coronae Borealis
588: J16011+3318A,
2030:on November 6, 2007
1884:2009ApJ...705.1226B
1837:2005ApJ...622.1160B
1783:2000ApJ...529..499T
1712:2016ApJ...830...46F
1605:2001ApJ...548L..57H
1558:1997ApJ...483L.111N
1439:2001AJ....122.3466M
1390:2021ApJ...921..122M
1301:2014MNRAS.438.2413V
1250:2023AJ....166...46B
748:
598:Database references
592: J16010+3318A
481:Rotational velocity
267:(17.51 ± 0.02
39:
38:ρ Coronae Borealis
1066:circumstellar disk
746:
665:Stellar properties
534:Other designations
262:57.11 ± 0.05
141:Spectral type
37:
32:R Coronae Borealis
2668:Hipparcos objects
2658:Flamsteed objects
2635:
2634:
2631:
2630:
2577:
2576:
2500:
2499:
2415:
2414:
2407:XO-1 (Moldoveanu)
1053:
1052:
787:
774:
756:
690:magnetic activity
623:yellow dwarf star
616:
615:
16:(Redirected from
2710:
2588:
2511:
2426:
2148:
2105:
2098:
2091:
2082:
2074:
2072:
2071:
2056:
2054:
2053:
2038:
2036:
2035:
2026:. Archived from
2013:
2011:
2010:
1982:
1981:
1955:
1934:
1928:
1927:
1925:
1924:
1915:. Archived from
1904:
1898:
1897:
1895:
1878:(2): 1226–1236.
1863:
1857:
1856:
1830:
1828:astro-ph/0412265
1821:(2): 1160–1170.
1809:
1803:
1802:
1766:
1760:
1759:
1757:
1755:
1740:
1734:
1733:
1723:
1705:
1679:
1673:
1672:
1646:
1625:
1619:
1618:
1616:
1584:
1578:
1577:
1551:
1549:astro-ph/9704248
1542:(2): L111–L114.
1531:
1525:
1515:
1505:
1487:
1459:
1453:
1452:
1450:
1418:
1412:
1411:
1401:
1383:
1358:
1345:
1344:
1324:
1315:
1314:
1312:
1294:
1285:(3): 2413–2425.
1270:
1264:
1263:
1261:
1243:
1217:
1194:
1184:
1174:
1156:
1128:
1040:
1039:
1038:
1028:
1026:
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1008:
988:
987:
986:
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974:
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962:
948:
943:
941:
921:
919:
912:
910:
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902:
901:
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882:
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859:
858:
848:
846:
839:
837:
826:
821:
820:
819:
781:
768:
754:
749:
703:Planetary system
520:
518:
501:
499:
474:
469:
449:
447:
427:
425:
405:
403:
373:
371:
346:
344:
319:
317:
226:
222:
210:
206:
190:
188:
135:Characteristics
127:
107:
102:
72:Observation data
59:
52:
40:
21:
2718:
2717:
2713:
2712:
2711:
2709:
2708:
2707:
2653:Corona Borealis
2638:
2637:
2636:
2627:
2623:RX J1532.9+3021
2583:Galaxy clusters
2573:
2547:
2496:
2472:
2411:
2375:
2352:
2289:
2269:
2137:
2114:
2109:
2078:
2069:
2067:
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2051:
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2016:
2008:
2006:
1994:
1991:
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1935:
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1901:
1865:
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1810:
1806:
1768:
1767:
1763:
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1751:
1742:
1741:
1737:
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1680:
1676:
1627:
1626:
1622:
1586:
1585:
1581:
1533:
1532:
1528:
1461:
1460:
1456:
1420:
1419:
1415:
1360:
1359:
1348:
1326:
1325:
1318:
1272:
1271:
1267:
1219:
1218:
1197:
1130:
1129:
1116:
1111:
1086:
1074:infrared excess
1058:
1036:
1034:
1033:
1031:
1024:
1022:
1018:
1013:
1006:
1004:
984:
982:
981:
979:
972:
970:
969:
967:
960:
958:
957:
955:
951:
946:
939:
937:
917:
915:
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906:
899:
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894:
890:
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878:
876:
856:
854:
853:
851:
844:
842:
835:
833:
829:
824:
817:
815:
814:
812:
780:
767:
753:
741:Future of Earth
709:radial velocity
705:
667:
639:Corona Borealis
593:
516:
514:
497:
495:
487: sin
467:
465:
445:
443:
423:
421:
401:
399:
389:Surface gravity
381:
378:
369:
367:
354:
351:
342:
340:
327:
324:
315:
313:
283:
266:
224:
219:
208:
186:
184:
179:
174:Radial velocity
122:
105:
100:Right ascension
98:
92:Corona Borealis
73:
67:
65:
64:
63:
62:
61:
60:
35:
28:
23:
22:
15:
12:
11:
5:
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2695:
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2675:
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2615:
2610:
2605:
2600:
2594:
2592:
2585:
2579:
2578:
2575:
2574:
2572:
2571:
2566:
2561:
2559:FSC 15307+3253
2555:
2553:
2549:
2548:
2546:
2545:
2540:
2535:
2530:
2525:
2519:
2517:
2508:
2502:
2501:
2498:
2497:
2495:
2494:
2492:XO-1b (Negoiu)
2489:
2486:
2480:
2478:
2474:
2473:
2471:
2470:
2465:
2460:
2455:
2450:
2445:
2440:
2434:
2432:
2423:
2417:
2416:
2413:
2412:
2410:
2409:
2404:
2399:
2394:
2389:
2383:
2381:
2377:
2376:
2374:
2373:
2371:145457 (Kamuy)
2368:
2362:
2360:
2354:
2353:
2351:
2350:
2345:
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2212:
2207:
2202:
2197:
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2177:
2172:
2167:
2162:
2156:
2154:
2145:
2139:
2138:
2136:
2135:
2130:
2125:
2119:
2116:
2115:
2110:
2108:
2107:
2100:
2093:
2085:
2076:
2075:
2057:
2039:
2014:
1990:
1989:External links
1987:
1984:
1983:
1929:
1899:
1858:
1845:10.1086/428115
1804:
1791:10.1086/308280
1777:(1): 499–505.
1761:
1735:
1674:
1620:
1614:10.1086/318927
1599:(1): L57–L60.
1579:
1566:10.1086/310754
1526:
1454:
1448:10.1086/323920
1413:
1346:
1316:
1265:
1195:
1113:
1112:
1110:
1107:
1106:
1105:
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1029:
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1016:
1002:
996:
995:
992:
989:
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868:
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861:
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827:
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804:
803:
798:
793:
788:
778:Orbital period
775:
765:Semimajor axis
762:
757:
733:interferometry
704:
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663:
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2698:2MASS objects
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2683:Solar analogs
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1919:on 2009-01-05
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675:spectral type
672:
671:main-sequence
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635:constellation
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584: 65024,
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198:Proper motion
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97:
96:
93:
90:
88:
87:Constellation
85:
84:
80:
76:
70:
58:
51:
41:
33:
19:
2282:
2249:
2160:α (Alphecca)
2077:
2068:. Retrieved
2064:
2050:. Retrieved
2046:
2032:. Retrieved
2028:the original
2021:
2007:. Retrieved
1999:
1943:
1939:
1932:
1921:. Retrieved
1917:the original
1912:
1902:
1875:
1871:
1861:
1818:
1814:
1807:
1774:
1770:
1764:
1752:. Retrieved
1748:
1738:
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1367:
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1278:
1268:
1231:
1225:
1144:
1140:
1134:
1059:
999:
932:
871:
807:
791:Eccentricity
737:
730:
712:
706:
694:
687:
673:star of the
668:
618:
617:
603:
572: 5968,
560: 9537,
507:
488:
484:
479:
458:
436:
414:
392:
387:
360:
333:
306:
276:
255:
239:
225:−772.245(53)
209:−198.278(43)
196:
172:
2165:β (Nusakan)
1754:30 December
1637:. id.A140.
1433:(6): 3466.
796:Inclination
718:astrometric
697:arc-minutes
627:light-years
542:15 CrB
438:Metallicity
416:Temperature
152:color index
113:Declination
2642:Categories
2421:Exoplanets
2392:Gliese 611
2070:2008-07-03
2065:SolStation
2052:2008-07-03
2034:2008-07-03
2009:2008-07-03
1946:. id.A15.
1923:2010-04-03
1703:1607.00007
1485:2208.00211
1381:2108.01088
1374:(2): 122.
1241:2306.06888
1154:2208.00211
1109:References
659:exoplanets
655:luminosity
552:+33°2663,
502: km/s
391:(log
362:Luminosity
191: km/s
162:Astrometry
2484:GJ 3929 b
2275:Flamsteed
1953:1403.6186
1799:121999545
1696:(1): 46.
1644:1101.2227
1574:115606006
1512:244398875
1408:236881312
1292:1312.1792
1234:(2): 46.
1181:244398875
752:Companion
726:red dwarf
714:Hipparcos
470:1.8
126: (V)
2506:Galaxies
2402:NGC 6002
2387:ADS 9731
2295:Variable
1730:36666883
1669:54986291
1084:See also
1080:either.
679:hydrogen
460:Rotation
380:☉
353:☉
326:☉
280: (M
257:Distance
241:Parallax
81:J2000.0
2569:IC 4539
2564:IC 1166
2397:GJ 3929
2047:Jumk.de
1978:2804652
1958:Bibcode
1880:Bibcode
1853:6633656
1833:Bibcode
1779:Bibcode
1708:Bibcode
1649:Bibcode
1601:Bibcode
1554:Bibcode
1490:Bibcode
1435:Bibcode
1386:Bibcode
1337:Bibcode
1335:: 942.
1297:Bibcode
1246:Bibcode
1159:Bibcode
961:−0.0045
959:+0.0044
907:39.8438
900:−0.0024
898:+0.0023
722:Jupiter
631:parsecs
297:Details
79:Equinox
2366:140913
2284:23 Her
1976:
1851:
1797:
1728:
1667:
1572:
1522:VizieR
1510:
1478:: A1.
1406:
1191:VizieR
1179:
1147:: A1.
1011:
985:−0.054
983:+0.053
968:102.19
956:0.4206
944:
920:0.0025
911:0.0027
895:0.2245
883:
877:≥1.093
857:−0.078
855:+0.054
843:12.949
838:0.0011
834:0.1061
822:
801:Radius
653:, and
651:radius
629:(17.5
605:SIMBAD
521:
450:
428:
406:
374:
347:
335:Radius
320:
227:
223:
211:
207:
2591:Abell
2552:Other
2477:Other
2430:Bayer
2380:Other
2152:Bayer
2143:Stars
1974:S2CID
1948:arXiv
1849:S2CID
1823:arXiv
1795:S2CID
1726:S2CID
1698:arXiv
1665:S2CID
1639:arXiv
1570:S2CID
1544:arXiv
1516:
1508:S2CID
1480:arXiv
1404:S2CID
1376:arXiv
1287:arXiv
1236:arXiv
1185:
1177:S2CID
1149:arXiv
1032:282.2
1027:0.011
1023:0.827
1005:≥21.6
980:0.096
973:−0.22
971:+0.27
938:≥28.2
916:0.038
881:0.023
852:0.126
847:0.014
818:−0.54
816:+0.53
813:≥3.79
625:57.1
578:ρ CrB
546:2MASS
444:−0.24
372:0.040
368:1.749
345:0.012
341:1.304
288:+4.21
221:Dec.:
185:17.88
156:0.61
130:5.39
75:Epoch
2618:2162
2613:2142
2608:2067
2603:2065
2598:2061
2543:6122
2538:6120
2533:6104
2528:6086
2523:6085
1756:2023
1466:Gaia
1135:Gaia
1043:0.0
1037:−3.7
1035:+2.2
784:days
760:Mass
683:iron
647:mass
611:data
586:CCDM
515:10.2
466:20.3
448:0.08
422:5817
404:0.05
400:4.25
318:0.01
314:0.95
308:Mass
189:0.12
150:B−V
145:G0V
2515:NGC
1966:doi
1944:565
1888:doi
1876:705
1841:doi
1819:622
1787:doi
1775:529
1716:doi
1694:830
1657:doi
1635:527
1609:doi
1597:548
1562:doi
1540:483
1520:at
1498:doi
1476:674
1443:doi
1431:122
1394:doi
1372:921
1333:336
1305:doi
1283:438
1254:doi
1232:166
1189:at
1167:doi
1145:674
1009:2.5
942:1.5
743:).
643:Sun
637:of
590:WDS
582:SAO
574:LTT
566:HIP
523:Gyr
519:0.5
509:Age
500:0.3
496:0.8
452:dex
408:cgs
249:mas
243:(π)
229:mas
213:mas
205:RA:
200:(μ)
2644::
2358:HD
2348:UW
2343:TY
2338:RS
2333:RR
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2045:.
2020:.
2002:.
1998:.
1972:.
1964:.
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950:🜨
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924:—
866:—
863:—
828:🜨
771:AU
692:.
661:.
649:,
580:,
570:HR
562:HD
558:GJ
554:GC
550:BD
544:,
426:24
269:pc
264:ly
233:yr
217:yr
176:(R
2488:c
2468:e
2463:d
2458:c
2328:W
2323:V
2318:U
2313:T
2308:S
2303:R
2265:υ
2260:τ
2255:σ
2250:ρ
2245:π
2240:ο
2235:ξ
2230:ν
2225:ν
2220:μ
2215:λ
2210:κ
2205:ι
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2195:η
2190:ζ
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2180:ε
2175:δ
2170:γ
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1014:M
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1000:d
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940:±
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918:±
909:±
889:J
886:M
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782:(
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430:K
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393:g
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350:R
343:±
323:M
316:±
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282:V
271:)
231:/
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187:±
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178:v
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