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Mimosa (star)

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979: 32: 2522: 1052: 39: 1113:, which might occur in roughly 6 million years. The high temperature of the star's outer envelope is what gives the star the blue-white hue that is characteristic of B-type stars. It is generating a strong stellar wind and is losing about 10  913:(WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included 1141:, are likely optical companions that are not physically associated with the system. The β Crucis system may be a member of the Lower Centaurus–Crux sub-group of the 1036:. However, the orbital plane of the pair is only about 10°, which probably means the inclination of the star's pole is also likely to be low. This suggests that the 1794: 1934: 1129:
The secondary, β Crucis B, may be a main sequence star with a stellar class of B2. In 2007, a third companion was announced, which may be a low mass, pre-
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Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick (eds.).
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is used to export live cattle from Australia to customers in Asia. An episode dedicated to the vessel features in the television documentary series
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Rizzuto, Aaron; Ireland, Michael; Robertson, J. G. (October 2011), "Multidimensional Bayesian membership analysis of the Sco OB2 moving group",
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Cohen, David H.; et al. (June 2008), "Chandra spectroscopy of the hot star βCrucis and the discovery of a pre-main-sequence companion",
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Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007–2013)".
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star fusing hydrogen into helium in its core. At more than ten times the mass of the Sun, Mimosa has sufficient mass to explode as a
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that have exhausted the supply of hydrogen at their cores, Mimosa's temperature and luminosity imply that it is more likely to be a
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Aerts, C.; et al. (January 1998), "Evidence for binarity and multiperiodicity in the beta Cephei star beta Crucis",
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Kilian, J. (February 1994), "Chemical abundances in early B-type stars. 5: Metal abundances and LTE/NLTE comparison",
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Kaltcheva, N. T.; Golev, V. K.; Moran, K. (2014), "Massive stellar content of the Galactic supershell GSH 305+01−24",
1942: 2602: 906: 688: 2587: 2562: 910: 60: 2557: 2100: 2567: 2057: 611: 694: 1085:. The periods of all three modes are in the range of 4.03–4.59 hours. Owing to the first application of 2597: 2222: 2125: 1134: 706: 80: 1721: 1695: 1126:
every 100 million years. The wind is leaving the system with a velocity of 2,000 km s or more.
1017:. The pair orbit each other every 5 years with an estimated separation that varies from 5.4 to 12.0 2454: 2387: 1170: 1941:, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from 1742: 837: 755: 1837: 1510:
Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30
2577: 2552: 2353: 1182: 1094: 698: 447: 177: 1181:, along with 26 other stars, each of which represents a state. Mimosa represents the State of 731: 2320: 2120: 1670: 1639: 1074: 770: 565: 1600: 1558: 1495: 1270: 2109: 1981: 1820: 1621: 1596: 1554: 1517: 1491: 1438: 1339: 1313: 1266: 1070: 1010: 786: 402: 301: 1217: 8: 2343: 1162: 1146: 1006: 702: 1985: 1824: 1625: 1521: 1442: 1343: 1317: 2093: 1999: 1971: 1890: 1872: 1570: 1544: 1456: 1428: 1282: 1256: 322: 145: 1861:"Polarimetric detection of non-radial oscillation modes in the β Cephei star β Crucis" 1081:
where such stars are found. It has three different pulsation modes, none of which are
2500: 2449: 2144: 2051: 1994: 1894: 1860: 1772: 1676: 1516:. Vol. 30. University of Toronto: International Astronomical Union. p. 57. 1451: 1158: 1082: 1078: 1018: 817: 763: 683: 632: 423: 165: 56: 2003: 1574: 1286: 2073: 1989: 1882: 1562: 1460: 1446: 1368: 1274: 1098: 1090: 1029: 921: 857: 599: 591: 528: 285: 87: 1910: 1566: 2505: 2495: 1798: 1332:
VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S
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Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",
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Heintz, W. D. (October 1957), "The radial velocity variation of beta Crucis",
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van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",
2572: 2541: 2525: 2202: 2192: 2187: 2086: 1166: 1130: 1106: 743: 250: 209: 170: 68: 2441: 2382: 2167: 2017: 1194: 1048:, this would mean the star has a rotational period of only about 3.6 days. 1045: 951: 947: 833: 655: 508: 477: 2423: 2418: 2197: 2177: 1086: 1056: 821: 798: 794: 584: 214: 199: 188: 134: 38: 31: 2078: 1859:
Cotton, D. V.; Buzasi, D. B; Aerts, C.; Bailey, J.; et al. (2021),
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Hoffleit, Dorrit; Jaschek, Carlos (1991). "The Bright star catalogue".
1138: 1123: 1114: 1102: 1025: 994: 662: 521: 484: 420: 308: 221: 840:, and these civilizations regarded it as part of the constellation of 2410: 2366: 2361: 2333: 2310: 2305: 2300: 2295: 2290: 2285: 2280: 2275: 2270: 2265: 2260: 2212: 2207: 1110: 1014: 841: 759: 1051: 2469: 2464: 2459: 2255: 2250: 2245: 2240: 2235: 2230: 2038:. CTV Global Media. Archived from the original on 15 September 2008 1877: 1024:
The primary, β Crucis A, is a massive star with about 16 times the
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Mimosa: The Life and Times of the Ship That Sailed to Patagonia
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star. The X-ray emission from this star was detected using the
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is a modern contraction of the Bayer designation. In 2016, the
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with components that are too close together to resolve with a
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measurements, Mimosa is located at a distance of 280 
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Determination of Radial Velocities and Their Applications
875: 437: 93: 1838:"MAST: Barbara A. Mikulski Archive for Space Telescopes" 1743:"Bulletin of the IAU Working Group on Star Names, No. 1" 1481: 1961: 1858: 881: 878: 869: 105: 1416: 1306:
Communications of the Lunar and Planetary Laboratory
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of about 27,000 K it is at the hot edge of the
872: 863: 2024: 1534: 860: 99: 96: 90: 1412: 1410: 1408: 1406: 1404: 1089:it is the heaviest star with an age determined by 1964:Monthly Notices of the Royal Astronomical Society 1771:, written by 陳久金. Published by 台灣書房出版有限公司, 2005, 1420:Monthly Notices of the Royal Astronomical Society 1402: 1400: 1398: 1396: 1394: 1392: 1390: 1388: 1386: 1384: 2539: 2074:http://jumk.de/astronomie/big-stars/becrux.shtml 1021:. The system is only 8 to 11 million years old. 1615: 742:is the second-brightest object in the southern 1381: 1329: 1242: 1240: 1238: 1236: 1234: 2094: 1955: 1662: 1650:Centre de données astronomiques de Strasbourg 961: 955: 931: 925: 139:−59° 41′ 19.5792″ 2440: 1782: 1580: 1528: 1477: 1475: 1473: 1471: 1469: 1040:rotational velocity is quite high, at about 2010: 1939:Australia Telescope, Outreach and Education 1688: 1246: 1231: 820:. Although Mimosa is at roughly −60° 2101: 2087: 1852: 1299: 1297: 1295: 954:. Consequently, Mimosa itself is known as 2409: 2108: 1993: 1975: 1876: 1804: 1668: 1548: 1466: 1450: 1432: 1260: 1212: 1210: 824:, and therefore not visible north of 30° 59:J2000       1722:"IAU Working Group on Star Names (WGSN)" 1367:, university of Illinois, archived from 1050: 977: 1355: 1353: 1292: 1044:. With a radius of about 8.4 times the 836:it was visible north of 40° due to the 257: 2540: 2486: 1810: 1632: 1586: 1207: 1157:Mimosa is represented in the flags of 942:, refers to an asterism consisting of 2082: 1927: 1905: 1903: 1735: 1611: 1609: 1507: 1177:. It is also featured in the flag of 1149:of stars that share a common origin. 785:. Mimosa forms part of the prominent 1830: 1714: 1501: 1350: 1840:. Space Telescope Science Institute 1323: 1173:as one of five stars making up the 1122:per year, or the equivalent of the 269: 13: 2020:. FOTW Flags Of The World website. 1900: 1759: 1702:. Simulation Curriculum Corp. 2009 1606: 14: 2614: 2067: 2018:"Astronomy of the Brazilian Flag" 973: 2521: 2520: 1995:10.1111/j.1365-2966.2011.19256.x 1452:10.1111/j.1365-2966.2008.13176.x 907:International Astronomical Union 856: 86: 37: 30: 804: 2593:Henry Draper Catalogue objects 1143:Scorpius–Centaurus association 1059:for Beta Crucis, plotted from 847:It bore the traditional names 16:Star in the constellation Crux 1: 2583:Bright Star Catalogue objects 1201: 1152: 1101:is typically associated with 1030:projected rotational velocity 1005:. In 1957, German astronomer 1537:Astronomy & Astrophysics 1097:of B0.5 III. While the 893:, which is derived from the 292:11.71 ± 0.98  48:Location of Mimosa (circled) 7: 1696:"Audio Pronunciation Guide" 1675:, Y Lolfa, pp. 56–57, 1567:10.1051/0004-6361/201321454 1218:"IAU Catalog of Star Names" 962: 932: 911:Working Group on Star Names 899:the flower of the same name 897:for 'actor', may come from 10: 2619: 2548:B-type main-sequence stars 1887:10.1038/s41550-021-01531-9 1589:Astronomy and Astrophysics 1484:Astronomy and Astrophysics 1279:10.1051/0004-6361:20078357 1249:Astronomy and Astrophysics 2518: 2482: 2436: 2405: 2375: 2352: 2319: 2221: 2143: 2134: 2126:Crux in Chinese astronomy 2116: 2056:: CS1 maint: unfit URL ( 1669:Wilkinson, Susan (2007), 1135:Chandra X-ray Observatory 967: 956: 926: 718: 680: 673: 648: 470: 465: 341: 337: 227: 220: 159: 53: 24: 1915:stars.astro.illinois.edu 1009:discovered that it is a 851:and the historical name 2603:Stars with proper names 1601:1994A&A...282..867K 1559:2014A&A...562A..69K 1496:1998A&A...329..137A 1271:2007A&A...474..653V 968:the Third Star of Cross 838:precession of equinoxes 323:Absolute magnitude 166:Evolutionary stage 146:Apparent magnitude 2588:Durchmusterung objects 2563:Spectroscopic binaries 1792:香港太空館 - 研究資源 - 亮星中英對照表 1700:Starry Night Education 1361:"MIMOSA (Beta Crucis)" 1095:stellar classification 1069:β Crucis A is a known 1066: 1032:of this star is about 986: 448:Argument of periastron 2558:Beta Cephei variables 2121:List of stars in Crux 2110:Constellation of Crux 1935:"The Colour of Stars" 1075:effective temperature 1054: 981: 828:, in the time of the 797:or a possible triple 2568:Lower Centaurus Crux 2388:PSR B1259−63/LS 2883 1011:spectroscopic binary 182:B0.5 III / B2V 1986:2011MNRAS.416.3108R 1825:1957Obs....77..200H 1626:1991bsc..book.....H 1522:1967IAUS...30...57E 1443:2008MNRAS.386.1855C 1344:2009yCat....102025S 1318:1966CoLPL...4...99J 1147:stellar association 1073:, although with an 1007:Wulff-Dieter Heintz 756:20th-brightest star 719:Database references 612:Rotational velocity 21: 1797:2011-01-30 at the 1067: 1019:Astronomical Units 987: 982:The constellation 816:) is the system's 675:Other designations 272: −16.18  260: −42.97  210:Variable type 178:Spectral type 19: 2598:Hipparcos objects 2532: 2531: 2514: 2513: 2501:Dragonfish Nebula 2478: 2477: 2450:Dragonfish Nebula 2432: 2431: 2401: 2400: 1777:978-986-7332-25-7 1682:978-0-86243-952-1 1093:. The star has a 1079:instability strip 1071:β Cephei variable 1046:radius of the Sun 818:Bayer designation 764:Bayer designation 737: 736: 2610: 2524: 2523: 2484: 2483: 2438: 2437: 2407: 2406: 2141: 2140: 2103: 2096: 2089: 2080: 2079: 2062: 2061: 2055: 2047: 2045: 2043: 2028: 2022: 2021: 2014: 2008: 2007: 1997: 1979: 1970:(4): 3108–3117, 1959: 1953: 1952: 1951: 1950: 1931: 1925: 1924: 1922: 1921: 1907: 1898: 1897: 1880: 1865:Nature Astronomy 1856: 1850: 1849: 1847: 1845: 1834: 1828: 1827: 1808: 1802: 1790: 1786: 1780: 1767: 1763: 1757: 1756: 1754: 1752: 1747: 1739: 1733: 1732: 1730: 1728: 1718: 1712: 1711: 1709: 1707: 1692: 1686: 1685: 1666: 1660: 1659: 1657: 1656: 1636: 1630: 1629: 1613: 1604: 1603: 1584: 1578: 1577: 1552: 1532: 1526: 1525: 1505: 1499: 1498: 1479: 1464: 1463: 1454: 1436: 1427:(4): 1855–1871, 1414: 1379: 1378: 1377: 1376: 1357: 1348: 1347: 1327: 1321: 1320: 1301: 1290: 1289: 1264: 1244: 1229: 1228: 1226: 1224: 1214: 1171:Papua New Guinea 1099:luminosity class 1091:asteroseismology 1043: 1035: 969: 965: 959: 958: 935: 929: 928: 888: 887: 884: 883: 880: 877: 874: 871: 868: 865: 862: 777:and abbreviated 692: 682:Mimosa Becrux,, 640: 574: 555: 506: 460: 452: 440: 435: 428: 412: 393: 380: 271: 259: 160:Characteristics 155: 149: 129: 124: 115: 114: 111: 110: 107: 104: 101: 98: 95: 92: 54:Observation data 41: 34: 22: 18: 2618: 2617: 2613: 2612: 2611: 2609: 2608: 2607: 2538: 2537: 2535: 2533: 2528: 2510: 2506:IRAS 12063-6259 2496:Coalsack Nebula 2474: 2428: 2397: 2371: 2348: 2315: 2217: 2130: 2112: 2107: 2070: 2065: 2049: 2048: 2041: 2039: 2030: 2029: 2025: 2016: 2015: 2011: 1960: 1956: 1948: 1946: 1933: 1932: 1928: 1919: 1917: 1909: 1908: 1901: 1857: 1853: 1843: 1841: 1836: 1835: 1831: 1813:The Observatory 1809: 1805: 1799:Wayback Machine 1788: 1787: 1783: 1765: 1764: 1760: 1750: 1748: 1745: 1741: 1740: 1736: 1726: 1724: 1720: 1719: 1715: 1705: 1703: 1694: 1693: 1689: 1683: 1667: 1663: 1654: 1652: 1638: 1637: 1633: 1614: 1607: 1585: 1581: 1533: 1529: 1506: 1502: 1480: 1467: 1415: 1382: 1374: 1372: 1359: 1358: 1351: 1328: 1324: 1302: 1293: 1245: 1232: 1222: 1220: 1216: 1215: 1208: 1204: 1188:A vessel named 1155: 1124:mass of the Sun 1120: 1117: 1041: 1033: 976: 917:for this star. 859: 855: 807: 714: 687: 668: 665: 638: 618: sin  572: 553: 542:Surface gravity 534: 531: 514: 511: 504: 490: 487: 458: 453: 445: 433: 431: 418: 410: 389:Semi-major axis 386: 378: 328: 311: 268: 244:+15.6 km/s 239: 234:Radial velocity 153: 144: 127: 122:Right ascension 120: 89: 85: 55: 49: 47: 46: 45: 44: 43: 42: 17: 12: 11: 5: 2616: 2606: 2605: 2600: 2595: 2590: 2585: 2580: 2575: 2570: 2565: 2560: 2555: 2550: 2530: 2529: 2519: 2516: 2515: 2512: 2511: 2509: 2508: 2503: 2498: 2492: 2490: 2480: 2479: 2476: 2475: 2473: 2472: 2467: 2462: 2457: 2452: 2446: 2444: 2434: 2433: 2430: 2429: 2427: 2426: 2421: 2415: 2413: 2403: 2402: 2399: 2398: 2396: 2395: 2390: 2385: 2379: 2377: 2373: 2372: 2370: 2369: 2364: 2358: 2356: 2350: 2349: 2347: 2346: 2341: 2336: 2331: 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2443: 2442:Star clusters 2439: 2435: 2425: 2422: 2420: 2417: 2416: 2414: 2412: 2408: 2404: 2394: 2391: 2389: 2386: 2384: 2381: 2380: 2378: 2374: 2368: 2367:108147 (Tupã) 2365: 2363: 2360: 2359: 2357: 2355: 2351: 2345: 2342: 2340: 2337: 2335: 2332: 2330: 2327: 2326: 2324: 2322: 2318: 2312: 2309: 2307: 2304: 2302: 2299: 2297: 2294: 2292: 2289: 2287: 2284: 2282: 2279: 2277: 2274: 2272: 2269: 2267: 2264: 2262: 2259: 2257: 2254: 2252: 2249: 2247: 2244: 2242: 2239: 2237: 2234: 2232: 2229: 2228: 2226: 2224: 2220: 2214: 2211: 2209: 2206: 2204: 2201: 2199: 2196: 2194: 2191: 2189: 2186: 2184: 2181: 2179: 2176: 2174: 2171: 2169: 2166: 2164: 2161: 2159: 2156: 2154: 2151: 2150: 2148: 2146: 2142: 2139: 2137: 2133: 2127: 2124: 2122: 2119: 2118: 2115: 2111: 2104: 2099: 2097: 2092: 2090: 2085: 2084: 2081: 2075: 2072: 2071: 2059: 2053: 2037: 2033: 2027: 2019: 2013: 2005: 2001: 1996: 1991: 1987: 1983: 1978: 1973: 1969: 1965: 1958: 1945:on 2012-03-18 1944: 1940: 1936: 1930: 1916: 1912: 1906: 1904: 1896: 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1108: 1107:main sequence 1104: 1100: 1096: 1092: 1088: 1084: 1080: 1076: 1072: 1064: 1063: 1058: 1053: 1049: 1047: 1039: 1031: 1027: 1022: 1020: 1016: 1012: 1008: 1004: 1000: 996: 992: 985: 980: 971: 964: 953: 949: 945: 941: 940: 934: 923: 918: 916: 912: 908: 904: 900: 896: 892: 886: 854: 850: 845: 843: 839: 835: 831: 827: 823: 819: 815: 811: 802: 800: 796: 792: 788: 784: 780: 776: 772: 768: 765: 762:. It has the 761: 757: 753: 749: 745: 744:constellation 741: 733: 730: 728: 727: 723: 722: 717: 713: 240259 712: 708: 705: 62434, 704: 700: 696: 690: 685: 684:β Crucis 679: 676: 672: 669: 660: 658: 657: 653: 652: 647: 644: 637: 635: 634: 630: 629: 625: 623: 621: 617: 613: 609: 608: 604: 602: 601: 597: 596: 593: 589: 587: 586: 582: 581: 578: 570: 568: 567: 563: 562: 559: 551: 549: 547: 543: 539: 538: 535: 526: 524: 523: 519: 518: 515: 502: 500: 499: 495: 494: 491: 482: 480: 479: 475: 474: 469: 464: 456: 451: 449: 444: 443: 439: 430: 427: 425: 422: 417: 416: 408: 406: 404: 400: 399: 395: 392: 390: 385: 384: 376: 374: 372: 368: 367: 363: 361: 358: 357: 353: 351: 348: 347: 344: 340: 336: 332: 330: 324: 320: 319: 315: 312:(85 ± 7  310: 306: 304: 303: 299: 298: 295: 291: 289: 287: 283: 282: 279: 275: 267: 263: 256: 254: 252: 251:Proper motion 248: 247: 243: 241: 235: 231: 230: 226: 223: 219: 216: 213: 211: 208: 207: 203: 201: 197: 196: 192: 190: 186: 185: 181: 179: 176: 175: 172: 171:Main sequence 169: 167: 164: 163: 158: 154:(1.23 - 1.31) 151: 147: 143: 142: 138: 136: 133: 132: 126: 123: 119: 118: 113: 84: 82: 81:Pronunciation 79: 78: 75: 72: 70: 69:Constellation 67: 66: 62: 58: 52: 40: 33: 23: 2534: 2383:NGC 4349-127 2157: 2040:. Retrieved 2035: 2026: 2012: 1967: 1963: 1957: 1947:, retrieved 1943:the original 1938: 1929: 1918:. Retrieved 1914: 1868: 1864: 1854: 1842:. Retrieved 1832: 1816: 1812: 1806: 1789:(in Chinese) 1784: 1768: 1766:(in Chinese) 1761: 1749:. Retrieved 1737: 1725:. Retrieved 1716: 1704:. Retrieved 1699: 1690: 1671: 1664: 1653:, retrieved 1643: 1634: 1617: 1592: 1588: 1582: 1540: 1536: 1530: 1513: 1509: 1503: 1487: 1483: 1424: 1418: 1373:, retrieved 1369:the original 1364: 1335: 1331: 1325: 1309: 1305: 1252: 1248: 1221:. Retrieved 1195:Mighty Ships 1193: 1189: 1187: 1156: 1145:. This is a 1128: 1068: 1060: 1023: 988: 952:Delta Crucis 948:Gamma Crucis 937: 919: 914: 909:organized a 902: 890: 852: 848: 846: 813: 809: 808: 805:Nomenclature 782: 778: 774: 766: 739: 738: 724: 709: 4853, 654: 631: 626:35 km/s 619: 615: 610: 598: 583: 564: 545: 540: 527:34,000  520: 496: 476: 446: 419: 403:Eccentricity 401: 387: 369: 359: 349: 321: 300: 284: 249: 232: 2424:HD 108147 b 2419:HD 106906 b 2042:25 November 1490:: 137–146, 1163:New Zealand 1103:giant stars 1087:polarimetry 1057:light curve 1001:) from the 966:, English: 936:), meaning 822:declination 814:Beta Crucis 799:star system 795:binary star 789:called the 775:Beta Crucis 769:, which is 754:), and the 697: 481, 590:−0.08  585:Metallicity 575:1,000  566:Temperature 454:(secondary) 396:8.7 AU 200:color index 189:color index 135:Declination 2542:Categories 2411:Exoplanets 2163:γ (Gacrux) 2158:β (Mimosa) 1949:2012-01-16 1920:2024-08-15 1878:2205.11679 1844:8 December 1655:2022-05-07 1640:"HD 93521" 1375:2011-12-30 1312:(99): 99, 1202:References 1153:In culture 1139:arcseconds 1026:Sun's mass 946:, Mimosa, 933:Shí Zì Jià 793:. It is a 544:(log  522:Luminosity 421:Periastron 364:β Crucis B 354:β Crucis A 222:Astrometry 2173:ε (Ginan) 2153:α (Acrux) 1977:1106.2857 1895:244953278 1618:New Haven 1550:1312.5592 1434:0802.4084 1338:: 02025. 1262:0708.1752 1190:MV Becrux 1159:Australia 1111:supernova 1038:azimuthal 1015:telescope 997:(86  989:Based on 842:Centaurus 771:Latinised 760:night sky 556:0.1  507:0.6  432:2,449,879 360:Companion 148: (V) 2526:Category 2470:NGC 4609 2465:NGC 4349 2460:NGC 4103 2223:Variable 2168:δ (Imai) 2052:cite web 2004:54510608 1911:"Mimosa" 1795:Archived 1575:54222753 1287:18759600 1119:☉ 1042:120 km s 991:parallax 826:latitude 810:β Crucis 787:asterism 779:Beta Cru 767:β Crucis 667:☉ 661:10  605:3.6 days 600:Rotation 533:☉ 513:☉ 489:☉ 483:16  436:38  381:2.5 days 325: (M 302:Distance 286:Parallax 2488:Nebulae 1982:Bibcode 1821:Bibcode 1819:: 200, 1751:28 July 1622:Bibcode 1597:Bibcode 1555:Bibcode 1543:: A69, 1518:Bibcode 1492:Bibcode 1461:2924933 1439:Bibcode 1340:Bibcode 1314:Bibcode 1267:Bibcode 1223:28 July 1034:35 km s 922:Chinese 758:in the 750:(after 639:8 to 11 466:Details 461:9° 350:Primary 61:Equinox 20:Mimosa 2362:106906 2002:  1893:  1775:  1769:中國星座神話 1727:22 May 1706:26 Apr 1679:  1645:SIMBAD 1573:  1459:  1285:  1179:Brazil 1083:radial 1028:. The 950:, and 915:Mimosa 903:Becrux 891:Mimosa 853:Becrux 849:Mimosa 834:Romans 740:Mimosa 726:SIMBAD 641:  571:27,000 498:Radius 377:1828.0 371:Period 204:−0.23 193:−0.98 63:J2000 2393:WR 46 2376:Other 2145:Bayer 2136:Stars 2000:S2CID 1972:arXiv 1891:S2CID 1873:arXiv 1746:(PDF) 1571:S2CID 1545:arXiv 1457:S2CID 1429:arXiv 1365:Stars 1283:S2CID 1257:arXiv 1167:Samoa 1003:Earth 944:Acrux 939:Cross 895:Latin 783:β Cru 752:Acrux 424:epoch 343:Orbit 333:−3.92 270:Dec.: 215:β Cep 152:1.25 57:Epoch 2573:Crux 2344:4890 2339:4887 2334:4848 2329:4729 2058:link 2044:2013 1846:2021 1773:ISBN 1753:2016 1729:2016 1708:2019 1677:ISBN 1225:2016 1169:and 1065:data 1062:TESS 984:Crux 970:.). 957:十字架三 832:and 748:Crux 732:data 656:Mass 478:Mass 413:0.09 409:0.38 198:B−V 187:U−B 74:Crux 1990:doi 1968:416 1883:doi 1593:282 1563:doi 1541:562 1488:329 1447:doi 1425:386 1275:doi 1253:474 927:十字架 920:In 781:or 773:to 746:of 711:SAO 703:HIP 695:FK5 689:CPD 643:Myr 633:Age 592:dex 558:cgs 552:3.6 503:8.4 457:293 450:(ω) 438:HJD 426:(T) 405:(e) 391:(a) 373:(P) 294:mas 288:(π) 274:mas 262:mas 258:RA: 253:(μ) 2544:: 2354:HD 2321:HR 2311:DU 2306:DS 2301:DL 2296:CH 2291:CD 2286:BZ 2281:BU 2276:BP 2271:BL 2266:BH 2261:BG 2054:}} 2050:{{ 2034:. 1998:, 1988:, 1980:, 1966:, 1937:, 1913:. 1902:^ 1889:, 1881:, 1867:, 1863:, 1817:77 1815:, 1698:. 1648:, 1642:, 1620:. 1608:^ 1591:, 1569:, 1561:, 1553:, 1539:, 1512:. 1486:, 1468:^ 1455:, 1445:, 1437:, 1423:, 1383:^ 1363:, 1352:^ 1334:. 1308:, 1294:^ 1281:, 1273:, 1265:, 1251:, 1233:^ 1209:^ 1198:. 1185:. 1165:, 1161:, 1055:A 999:pc 995:ly 924:, 901:. 889:. 867:eɪ 844:. 801:. 707:HR 699:HD 693:, 686:, 314:pc 309:ly 278:yr 266:yr 236:(R 103:oʊ 2256:X 2251:W 2246:V 2241:T 2236:S 2231:R 2213:μ 2208:μ 2203:λ 2198:ι 2193:θ 2188:θ 2183:η 2178:ζ 2102:e 2095:t 2088:v 2060:) 2046:. 2006:. 1992:: 1984:: 1974:: 1923:. 1885:: 1875:: 1869:6 1848:. 1823:: 1779:. 1755:. 1731:. 1710:. 1658:. 1628:. 1624:: 1599:: 1565:: 1557:: 1547:: 1524:. 1520:: 1494:: 1449:: 1441:: 1431:: 1346:. 1342:: 1336:1 1316:: 1310:4 1277:: 1269:: 1259:: 1227:. 1116:M 960:( 930:( 885:/ 882:s 879:k 876:ʌ 873:r 870:k 864:b 861:ˈ 858:/ 664:M 649:B 622:) 620:i 616:v 614:( 577:K 573:± 554:± 548:) 546:g 530:L 510:R 505:± 486:M 471:A 459:± 434:± 411:± 379:± 329:) 327:V 316:) 276:/ 264:/ 240:) 238:v 112:/ 109:ə 106:s 100:m 97:ˈ 94:ɪ 91:m 88:/

Index



Epoch
Equinox
Constellation
Crux
Pronunciation
/mɪˈmsə/
Right ascension
Declination
Apparent magnitude
Evolutionary stage
Main sequence
Spectral type
color index
color index
Variable type
β Cep
Astrometry
Radial velocity
Proper motion
mas
yr
mas
yr
Parallax
mas
Distance
ly
pc

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