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Rho Coronae Borealis

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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;
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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.
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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".
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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".
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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
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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".
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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.
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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
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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
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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).
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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
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Trilling, D. E.; Brown, R. H.; Rivkin, A. S. (2000). "Circumstellar Dust Disks around Stars with Known Planetary Companions".
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An extrasolar planet in a 39.8-day orbit around Rho Coronae Borealis was discovered in 1997 by observing the star's
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variations. This detection method only gives a lower limit on the true mass of the companion. In 2001, preliminary
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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
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Data Release 3. Summary of the content and survey properties"
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Data Release 3. Summary of the content and survey properties"
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Brewer, John M.; Zhao, Lily L.; et al. (June 2023).
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Vallenari, A.; et al. (Gaia collaboration) (2023).
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Vallenari, A.; et al. (Gaia collaboration) (2023).
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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: 1015: 1010: 1008: 988: 987: 986: 976: 975: 974: 964: 963: 962: 948: 943: 941: 921: 919: 912: 910: 903: 902: 901: 887: 882: 880: 860: 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: 2059: 2051: 2049: 2041: 2033: 2031: 2016: 2008: 2006: 1994: 1991: 1986: 1985: 1936: 1935: 1931: 1922: 1920: 1906: 1905: 1901: 1865: 1864: 1860: 1811: 1810: 1806: 1768: 1767: 1763: 1753: 1751: 1742: 1741: 1737: 1681: 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: 908: 906: 899: 897: 896: 894: 890: 885: 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: 2716: 2714: 2706: 2705: 2700: 2695: 2690: 2685: 2680: 2675: 2670: 2665: 2660: 2655: 2650: 2640: 2639: 2633: 2632: 2629: 2628: 2626: 2625: 2620: 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: 2340: 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733:interferometry 704: 701: 666: 663: 633:) away in the 614: 613: 608: 600: 599: 595: 594: 564: 143761, 540: 537: 536: 530: 529: 526: 525: 512: 504: 503: 493: 476: 475: 463: 455: 454: 441: 433: 432: 419: 411: 410: 397: 384: 383: 379: 376: 365: 357: 356: 352: 349: 338: 330: 329: 325: 322: 311: 303: 302: 299: 298: 294: 293: 290: 289: 286: 281: 273: 272: 260: 252: 251: 245: 236: 235: 202: 193: 192: 182: 177: 169: 168: 165: 164: 158: 157: 154: 147: 146: 143: 137: 136: 132: 131: 128: 119: 118: 115: 109: 108: 106:16 01 02.66049 103: 95: 94: 89: 83: 82: 69: 68: 54: 53: 47: 46: 45: 44: 43: 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 2715: 2704: 2701: 2699: 2698:2MASS objects 2696: 2694: 2691: 2689: 2686: 2684: 2683:Solar analogs 2681: 2679: 2676: 2674: 2671: 2669: 2666: 2664: 2661: 2659: 2656: 2654: 2651: 2649: 2648:Bayer objects 2646: 2645: 2643: 2624: 2621: 2619: 2616: 2614: 2611: 2609: 2606: 2604: 2601: 2599: 2596: 2595: 2593: 2589: 2586: 2584: 2580: 2570: 2567: 2565: 2562: 2560: 2557: 2556: 2554: 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567: 563: 559: 556: 21527, 555: 551: 547: 543: 538: 535: 531: 527: 524: 513: 511: 510: 506: 505: 494: 492: 490: 486: 482: 478: 477: 473: 464: 462: 461: 457: 456: 453: 442: 440: 439: 435: 434: 431: 420: 418: 417: 413: 412: 409: 398: 396: 394: 390: 386: 385: 382: 366: 364: 363: 359: 358: 355: 339: 337: 336: 332: 331: 328: 312: 310: 309: 305: 304: 300: 295: 291: 287: 285: 279: 275: 274: 270: 265: 261: 259: 258: 254: 253: 250: 246: 244: 242: 238: 237: 234: 230: 218: 214: 203: 201: 199: 198:Proper motion 195: 194: 183: 181: 175: 171: 170: 166: 163: 159: 155: 153: 149: 148: 144: 142: 139: 138: 133: 129: 125: 121: 120: 116: 114: 111: 110: 104: 101: 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: 1693: 1687: 1677: 1634: 1630: 1623: 1596: 1592: 1582: 1539: 1535: 1529: 1475: 1471: 1465: 1457: 1430: 1426: 1416: 1371: 1367: 1332: 1328: 1282: 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 2063:. 2045:. 2020:. 2002:. 1998:. 1972:. 1964:. 1956:. 1942:. 1911:. 1886:. 1874:. 1870:. 1847:. 1839:. 1831:. 1817:. 1793:. 1785:. 1773:. 1747:. 1724:. 1714:. 1706:. 1692:. 1686:. 1663:. 1655:. 1647:. 1633:. 1607:. 1595:. 1591:. 1568:. 1560:. 1552:. 1538:. 1506:. 1496:. 1488:. 1474:. 1470:. 1441:. 1429:. 1425:. 1402:. 1392:. 1384:. 1370:. 1366:. 1349:^ 1331:. 1319:^ 1303:. 1295:. 1281:. 1277:. 1252:. 1244:. 1230:. 1224:. 1198:^ 1175:. 1165:. 1157:. 1143:. 1139:. 1117:^ 1049:— 1046:— 1017:🜨 994:— 991:— 950:🜨 927:— 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 2200:θ 2195:η 2190:ζ 2185:ζ 2180:ε 2175:δ 2170:γ 2104:e 2097:t 2090:v 2073:. 2055:. 2037:. 2012:. 1980:. 1968:: 1960:: 1950:: 1926:. 1896:. 1890:: 1882:: 1855:. 1843:: 1835:: 1825:: 1801:. 1789:: 1781:: 1758:. 1732:. 1718:: 1710:: 1700:: 1671:. 1659:: 1651:: 1641:: 1617:. 1611:: 1603:: 1576:. 1564:: 1556:: 1546:: 1524:. 1514:. 1500:: 1492:: 1482:: 1464:" 1451:. 1445:: 1437:: 1410:. 1396:: 1388:: 1378:: 1343:. 1339:: 1313:. 1307:: 1299:: 1289:: 1262:. 1256:: 1248:: 1238:: 1193:. 1183:. 1169:: 1161:: 1151:: 1133:" 1025:± 1014:M 1007:± 1000:d 947:M 940:± 933:c 918:± 909:± 889:J 886:M 879:± 872:b 845:± 836:± 825:M 808:e 786:) 782:( 773:) 769:( 517:± 498:± 491:) 489:i 485:v 483:( 472:d 468:± 446:± 430:K 424:± 402:± 395:) 393:g 377:L 370:± 350:R 343:± 323:M 316:± 284:) 282:V 271:) 231:/ 215:/ 187:± 180:) 178:v 34:. 20:)

Index

Rho Coronae Borealis c
R Coronae Borealis


Epoch
Equinox
Constellation
Corona Borealis
Right ascension
Declination
Apparent magnitude
Spectral type
color index
Astrometry
Radial velocity
Proper motion
mas
yr
mas
yr
Parallax
mas
Distance
ly
pc
Absolute magnitude
Mass
M
Radius
R

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