39:
2407:
46:
776:(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
749:
attempted to identify the name with particular stars, principally in the modern constellations
Centaurus and Colomba. The stars of Colomba were assigned to Canis Majoris in the
789:
1646:
801:
590:
1228:
851:
of about 18,700 K, giving it the blue-white hue of a B-type star. It is relatively young for a star, with an estimated age of 32 million years.
1048:
Evans, D. S. (June 20–24, 1966), "The
Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),
481:
1287:
Underhill, A. B.; et al. (November 1979), "Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars",
1226:
Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway
Hipparcos stars within 3 kpc from the Sun",
831:
The primary component is a large star with nearly four times the Sun's radius and almost eight times the mass of the Sun. It has a
2459:
2469:
1330:
Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants",
1718:
1472:
2429:
999:
Telting, J. H.; et al. (June 2006), "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars",
1654:
1508:
2474:
1738:
1053:
769:
2449:
2434:
773:
70:
504:
2377:
1743:
672:
745:"the solitary ones". This was an appellation early Arab poets used for a number of anonymous stars. Later
1727:
574:
2464:
2454:
843:
of hydrogen at its core. The star is emitting 3,603 times the luminosity of the Sun and is a suspected
809:
1938:
1711:
836:
668:
586:
1529:
1418:
2354:
1653:, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from
1550:
793:
1050:
Determination of Radial
Velocities and their Applications, Proceedings from IAU Symposium no. 30
808:
system, which means that the pair have not been individually resolved with a telescope, but the
2444:
2064:
1860:
1855:
1488:
832:
797:
578:
568:
358:
134:
1500:
1493:
1382:
Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), "Rotational
Velocities of B Stars",
2204:
2011:
1890:
1790:
1127:
Pourbaix, D.; et al. (2004), "SB9: The Ninth
Catalogue of Spectroscopic Binary Orbits",
848:
813:
711:
563:
489:
1150:
1012:
909:
611:
2439:
2410:
2359:
2318:
2044:
1820:
1704:
1620:
1583:
1391:
1349:
1296:
1247:
1192:
1146:
1093:
1057:
1008:
979:
954:
905:
844:
825:
805:
321:
259:
172:
1442:
8:
2144:
2103:
1880:
1870:
1815:
1805:
1785:
1780:
582:
1624:
1587:
1465:
A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their
Derivations
1395:
1353:
1300:
1251:
1196:
1097:
1061:
983:
958:
2113:
1810:
1775:
1365:
1339:
1265:
1237:
1162:
1136:
1109:
1083:
921:
895:
280:
117:
1875:
1850:
1845:
1840:
1835:
1830:
1800:
1762:
1504:
1468:
1369:
1269:
1260:
1166:
1113:
719:
559:
525:
338:
63:
925:
2001:
1996:
1991:
1986:
1981:
1976:
1971:
1966:
1961:
1928:
1923:
1918:
1913:
1908:
1903:
1898:
1865:
1825:
1628:
1591:
1399:
1357:
1304:
1255:
1200:
1154:
1101:
1026:
1016:
913:
817:
746:
632:
456:
243:
1956:
1951:
1946:
1679:
1158:
1021:
917:
696:
469:
191:
93:
20:
978:, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,
824:. The pair orbit around their common center of mass once every 675 days with an
38:
1696:
840:
821:
550:
374:
308:
251:
231:
219:
1309:
1105:
1074:
Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",
886:
van
Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",
2423:
855:
660:
208:
166:
80:
1574:
Curtis, H. D. (April 1909), "Five stars having variable radial velocities",
2193:
1361:
723:
436:
402:
1141:
664:
656:
348:
156:
145:
106:
85:
755:, leading to more recent assignment of the name for Zeta Canis Majoris.
2253:
2179:
2174:
2169:
2164:
2159:
2154:
2149:
684:
449:
416:
335:
266:
179:
1031:
945:
Cousins, A. W. J. (1972), "UBV Photometry of Some Very Bright Stars",
2385:
2136:
976:
Michigan catalogue of two-dimensional spectral types for the HD stars
680:
1286:
2390:
2338:
2333:
2328:
2323:
2284:
2279:
2232:
2227:
2222:
2217:
2212:
2087:
2082:
2077:
2072:
2054:
2049:
2039:
2034:
2029:
2024:
2019:
1632:
1596:
1404:
1205:
751:
676:
539:
1344:
1242:
1088:
998:
900:
45:
2289:
2108:
1183:
Abt, Helmut A. (August 2005), "Observed
Orbital Eccentricities",
758:
675:
in the constellation and hence readily visible to the naked eye.
73:
66:
1611:
Mitchell, S. A. (October 1909), "Seven spectroscopic binaries",
2303:
2271:
2248:
1770:
738:
688:
641:
605:
496:
429:
271:
1499:(Reprint ed.), New York: Dover Publications Inc, p.
847:. This energy is being radiated from its outer envelope at an
300:
1126:
947:
Monthly Notes of the
Astronomical Society of Southern Africa
2118:
1753:
644:
235:
223:
692:
1551:"Bulletin of the IAU Working Group on Star Names, No. 1"
1467:(2nd rev. ed.). Cambridge, Massachusetts: Sky Pub.
1225:
683:
mission yield a distance estimate of around 362
638:
1329:
788:
The binary nature of this system was first noted by
647:
635:
2376:
1492:
1120:
1289:Monthly Notices of the Royal Astronomical Society
1229:Monthly Notices of the Royal Astronomical Society
2421:
1726:
1221:
1219:
1217:
1215:
1425:, Centre de Données astronomiques de Strasbourg
1381:
1282:
1280:
1278:
1073:
1462:
1325:
1323:
1321:
1319:
1178:
1176:
994:
992:
881:
879:
877:
875:
873:
871:
1712:
1212:
940:
938:
936:
934:
800:, using radial velocity measurements made by
111:–30° 03′ 48.1202″
1604:
1375:
1275:
792:based on observations made in 1906 from the
16:Binary star in the constellation Canis Major
1651:Australia Telescope, Outreach and Education
1316:
1173:
1067:
989:
885:
868:
854:Zeta Canis Majoris is located close to the
1719:
1705:
1567:
969:
967:
931:
2135:
1595:
1481:
1456:
1403:
1343:
1308:
1259:
1241:
1204:
1140:
1087:
1030:
1020:
899:
1610:
1530:"IAU Working Group on Star Names (WGSN)"
1435:
1052:, vol. 30, University of Toronto:
1043:
1041:
964:
944:
215:
2422:
2270:
1573:
1411:
839:that is generating energy through the
796:in Chile. It was confirmed in 1909 by
1700:
1639:
1543:
1487:
1047:
695:. It is drifting further away with a
55:Location of ζ Canis Majoris (circled)
1522:
1463:Kunitzsch, Paul; Smart, Tim (2006).
1038:
973:
835:of B2.5 V, which means it is a
69:
1423:SIMBAD Astronomical Object Database
1182:
761:referred to these stars as ألأغربة
227:
13:
1495:Star Names: Their Lore and Meaning
1419:"zet CMa -- Cepheid variable Star"
816:can be discerned by shifts in the
722:assigned by the German astronomer
14:
2486:
1677:
1671:
2406:
2405:
1739:Canis Major in Chinese astronomy
1261:10.1111/j.1365-2966.2010.17434.x
1054:International Astronomical Union
770:International Astronomical Union
631:
44:
37:
2460:Henry Draper Catalogue objects
804:in 1908. It is a single-lined
671:of +3.0, making it one of the
1:
2470:Bright Star Catalogue objects
861:
820:of the primary caused by the
783:
1744:List of stars in Canis Major
1728:Constellation of Canis Major
1680:"FURUD (Zeta Canis Majoris)"
1129:Astronomy & Astrophysics
7:
1443:"IAU Catalog of Star Names"
810:gravitational perturbations
774:Working Group on Star Names
250:9.00 ± 0.13
10:
2491:
2430:B-type main-sequence stars
1159:10.1051/0004-6361:20041213
1022:10.1051/0004-6361:20054730
1001:Astronomy and Astrophysics
918:10.1051/0004-6361:20078357
888:Astronomy and Astrophysics
18:
2403:
2372:
2347:
2311:
2302:
2266:
2241:
2203:
2192:
2131:
2096:
2063:
2010:
1937:
1889:
1761:
1752:
1734:
1384:The Astrophysical Journal
1332:Astronomische Nachrichten
1185:The Astrophysical Journal
1106:10.1134/S1063773712050015
837:B-type main sequence star
669:apparent visual magnitude
598:
556:
549:
545:
396:
391:
299:
295:
185:
178:
128:
60:
31:
1686:, University of Illinois
19:Not to be confused with
2475:Stars with proper names
2355:Canis Major Overdensity
1310:10.1093/mnras/189.3.601
1151:2004A&A...424..727P
1013:2006A&A...452..945T
910:2007A&A...474..653V
794:D. O. Mills Observatory
702:
659:system in the southern
281:Absolute magnitude
118:Apparent magnitude
2450:Durchmusterung objects
2435:Spectroscopic binaries
1362:10.1002/asna.200911355
833:stellar classification
679:measurements from the
359:Argument of periastron
1647:"The Colour of Stars"
1613:Astrophysical Journal
1576:Astrophysical Journal
849:effective temperature
814:astrometric companion
729:The traditional name
667:. This system has an
974:Houk, Nancy (1979),
845:Beta Cephei variable
806:spectroscopic binary
564:1 Canis Majoris
2378:Astronomical events
2109:WASP-64 (Atakoraka)
1625:1909ApJ....30..239M
1588:1909ApJ....29..229C
1396:2002ApJ...573..359A
1354:2010AN....331..349H
1301:1979MNRAS.189..601U
1252:2011MNRAS.410..190T
1197:2005ApJ...629..507A
1098:2012AstL...38..331A
1062:1967IAUS...30...57E
984:1982mcts.book.....H
959:1972MNSSA..31...69C
747:Arabian astronomers
599:Database references
505:Rotational velocity
28:
27:Zeta Canis Majoris
716:Zeta Canis Majoris
699:of +32 km/s.
620:Zeta Canis Majoris
551:Other designations
167:Variable type
135:Spectral type
26:
2465:Hipparcos objects
2455:Flamsteed objects
2417:
2416:
2399:
2398:
2368:
2367:
2298:
2297:
2262:
2261:
2188:
2187:
2145:ν Canis Majoris b
2127:
2126:
1678:Kaler, James B.,
1474:978-1-931559-44-7
1076:Astronomy Letters
737:derives from the
720:Bayer designation
617:
616:
230: +4.03
218: +7.32
2482:
2409:
2408:
2374:
2373:
2309:
2308:
2268:
2267:
2201:
2200:
2133:
2132:
2073:43197 (Amadioha)
1759:
1758:
1721:
1714:
1707:
1698:
1697:
1693:
1692:
1691:
1665:
1664:
1663:
1662:
1643:
1637:
1636:
1608:
1602:
1601:
1599:
1571:
1565:
1564:
1562:
1560:
1555:
1547:
1541:
1540:
1538:
1536:
1526:
1520:
1519:
1518:
1517:
1498:
1485:
1479:
1478:
1460:
1454:
1453:
1451:
1449:
1439:
1433:
1432:
1431:
1430:
1415:
1409:
1408:
1407:
1379:
1373:
1372:
1347:
1327:
1314:
1313:
1312:
1284:
1273:
1272:
1263:
1245:
1223:
1210:
1209:
1208:
1180:
1171:
1170:
1144:
1142:astro-ph/0406573
1124:
1118:
1117:
1091:
1071:
1065:
1064:
1045:
1036:
1035:
1034:
1024:
996:
987:
986:
971:
962:
961:
942:
929:
928:
903:
883:
718:, is the star's
654:
653:
650:
649:
646:
643:
640:
637:
572:
537:
535:
414:
412:
363:
351:
343:
229:
217:
129:Characteristics
121:
101:
96:
61:Observation data
48:
41:
29:
25:
2490:
2489:
2485:
2484:
2483:
2481:
2480:
2479:
2420:
2419:
2418:
2413:
2395:
2364:
2343:
2294:
2258:
2237:
2195:
2184:
2123:
2104:RX J0720.4−3125
2092:
2059:
2006:
1933:
1885:
1748:
1730:
1725:
1689:
1687:
1674:
1669:
1668:
1660:
1658:
1645:
1644:
1640:
1609:
1605:
1572:
1568:
1558:
1556:
1553:
1549:
1548:
1544:
1534:
1532:
1528:
1527:
1523:
1515:
1513:
1511:
1486:
1482:
1475:
1461:
1457:
1447:
1445:
1441:
1440:
1436:
1428:
1426:
1417:
1416:
1412:
1380:
1376:
1328:
1317:
1285:
1276:
1224:
1213:
1181:
1174:
1125:
1121:
1072:
1068:
1046:
1039:
997:
990:
972:
965:
943:
932:
884:
869:
864:
786:
780:for this star.
708:ζ Canis Majoris
705:
697:radial velocity
634:
630:
624:ζ Canis Majoris
594:
567:
560:ζ CMa, Zeta CMa
558:Furud, Phurud,
533:
531:
511: sin
470:Surface gravity
462:
459:
442:
439:
422:
419:
410:
408:
383:
381:
364:
356:
347:2,416,508
346:
333:
286:
269:
226:
202:+32.2 km/s
197:
192:Radial velocity
116:
99:
94:Right ascension
92:
62:
56:
54:
53:
52:
51:
50:
49:
24:
21:Z Canis Majoris
17:
12:
11:
5:
2488:
2478:
2477:
2472:
2467:
2462:
2457:
2452:
2447:
2442:
2437:
2432:
2415:
2414:
2404:
2401:
2400:
2397:
2396:
2394:
2393:
2388:
2382:
2380:
2370:
2369:
2366:
2365:
2363:
2362:
2357:
2351:
2349:
2345:
2344:
2342:
2341:
2336:
2331:
2326:
2321:
2315:
2313:
2306:
2300:
2299:
2296:
2295:
2293:
2292:
2287:
2282:
2276:
2274:
2264:
2263:
2260:
2259:
2257:
2256:
2251:
2245:
2243:
2239:
2238:
2236:
2235:
2230:
2225:
2220:
2215:
2209:
2207:
2198:
2190:
2189:
2186:
2185:
2183:
2182:
2177:
2172:
2167:
2162:
2157:
2152:
2147:
2141:
2139:
2129:
2128:
2125:
2124:
2122:
2121:
2116:
2114:WISE 0713−2917
2111:
2106:
2100:
2098:
2094:
2093:
2091:
2090:
2085:
2080:
2075:
2069:
2067:
2061:
2060:
2058:
2057:
2052:
2047:
2042:
2037:
2032:
2027:
2022:
2016:
2014:
2008:
2007:
2005:
2004:
1999:
1994:
1989:
1984:
1979:
1974:
1969:
1964:
1959:
1954:
1949:
1943:
1941:
1935:
1934:
1932:
1931:
1926:
1921:
1916:
1911:
1906:
1901:
1895:
1893:
1887:
1886:
1884:
1883:
1878:
1873:
1871:σ (Unurgunite)
1868:
1863:
1858:
1853:
1848:
1843:
1838:
1833:
1828:
1823:
1818:
1813:
1808:
1803:
1798:
1793:
1788:
1783:
1778:
1773:
1767:
1765:
1756:
1750:
1749:
1747:
1746:
1741:
1735:
1732:
1731:
1724:
1723:
1716:
1709:
1701:
1695:
1694:
1673:
1672:External links
1670:
1667:
1666:
1638:
1633:10.1086/141699
1603:
1597:10.1086/141645
1566:
1542:
1521:
1509:
1480:
1473:
1455:
1434:
1410:
1405:10.1086/340590
1390:(1): 359–365,
1374:
1338:(4): 349–360,
1315:
1295:(3): 601–605,
1274:
1236:(1): 190–200,
1211:
1206:10.1086/431207
1191:(1): 507–511,
1172:
1119:
1066:
1056:, p. 57,
1037:
1007:(3): 945–953,
988:
963:
930:
894:(2): 653–664,
866:
865:
863:
860:
841:nuclear fusion
822:Doppler effect
798:S. A. Mitchell
785:
782:
765:"the ravens".
704:
701:
673:brighter stars
615:
614:
609:
601:
600:
596:
595:
571:−30°3038
557:
554:
553:
547:
546:
543:
542:
529:
521:
520:
517:
500:
499:
493:
485:
484:
478:
465:
464:
460:
457:
453:
445:
444:
440:
437:
433:
425:
424:
420:
417:
406:
398:
397:
394:
393:
389:
388:
385:
379:
375:Semi-amplitude
370:
369:
366:
353:
352:
344:
330:
329:
326:
317:
316:
313:
304:
303:
297:
296:
293:
292:
289:
284:
276:
275:
270:(111 ± 2
263:
255:
254:
248:
239:
238:
213:
204:
203:
200:
195:
187:
186:
183:
182:
176:
175:
169:
163:
162:
159:
152:
151:
148:
141:
140:
137:
131:
130:
126:
125:
122:
113:
112:
109:
103:
102:
100:06 20 18.79204
97:
89:
88:
83:
77:
76:
58:
57:
43:
42:
36:
35:
34:
33:
32:
15:
9:
6:
4:
3:
2:
2487:
2476:
2473:
2471:
2468:
2466:
2463:
2461:
2458:
2456:
2453:
2451:
2448:
2446:
2445:Bayer objects
2443:
2441:
2438:
2436:
2433:
2431:
2428:
2427:
2425:
2412:
2402:
2392:
2389:
2387:
2384:
2383:
2381:
2379:
2375:
2371:
2361:
2358:
2356:
2353:
2352:
2350:
2346:
2340:
2337:
2335:
2332:
2330:
2327:
2325:
2322:
2320:
2317:
2316:
2314:
2310:
2307:
2305:
2301:
2291:
2288:
2286:
2283:
2281:
2278:
2277:
2275:
2273:
2269:
2265:
2255:
2252:
2250:
2247:
2246:
2244:
2240:
2234:
2231:
2229:
2226:
2224:
2221:
2219:
2216:
2214:
2211:
2210:
2208:
2206:
2202:
2199:
2197:
2191:
2181:
2178:
2176:
2173:
2171:
2168:
2166:
2163:
2161:
2158:
2156:
2153:
2151:
2148:
2146:
2143:
2142:
2140:
2138:
2134:
2130:
2120:
2117:
2115:
2112:
2110:
2107:
2105:
2102:
2101:
2099:
2095:
2089:
2086:
2084:
2081:
2079:
2076:
2074:
2071:
2070:
2068:
2066:
2062:
2056:
2053:
2051:
2048:
2046:
2043:
2041:
2038:
2036:
2033:
2031:
2028:
2026:
2023:
2021:
2018:
2017:
2015:
2013:
2009:
2003:
2000:
1998:
1995:
1993:
1990:
1988:
1985:
1983:
1980:
1978:
1975:
1973:
1970:
1968:
1965:
1963:
1960:
1958:
1955:
1953:
1950:
1948:
1945:
1944:
1942:
1940:
1936:
1930:
1927:
1925:
1922:
1920:
1917:
1915:
1912:
1910:
1907:
1905:
1902:
1900:
1897:
1896:
1894:
1892:
1888:
1882:
1879:
1877:
1874:
1872:
1869:
1867:
1864:
1862:
1859:
1857:
1854:
1852:
1849:
1847:
1844:
1842:
1839:
1837:
1834:
1832:
1829:
1827:
1824:
1822:
1819:
1817:
1814:
1812:
1809:
1807:
1804:
1802:
1799:
1797:
1794:
1792:
1789:
1787:
1784:
1782:
1781:γ (Muliphein)
1779:
1777:
1774:
1772:
1769:
1768:
1766:
1764:
1760:
1757:
1755:
1751:
1745:
1742:
1740:
1737:
1736:
1733:
1729:
1722:
1717:
1715:
1710:
1708:
1703:
1702:
1699:
1685:
1681:
1676:
1675:
1657:on 2013-12-03
1656:
1652:
1648:
1642:
1634:
1630:
1626:
1622:
1618:
1614:
1607:
1598:
1593:
1589:
1585:
1581:
1577:
1570:
1552:
1546:
1531:
1525:
1512:
1510:0-486-21079-0
1506:
1502:
1497:
1496:
1490:
1484:
1476:
1470:
1466:
1459:
1444:
1438:
1424:
1420:
1414:
1406:
1401:
1397:
1393:
1389:
1385:
1378:
1371:
1367:
1363:
1359:
1355:
1351:
1346:
1341:
1337:
1333:
1326:
1324:
1322:
1320:
1311:
1306:
1302:
1298:
1294:
1290:
1283:
1281:
1279:
1271:
1267:
1262:
1257:
1253:
1249:
1244:
1239:
1235:
1231:
1230:
1222:
1220:
1218:
1216:
1207:
1202:
1198:
1194:
1190:
1186:
1179:
1177:
1168:
1164:
1160:
1156:
1152:
1148:
1143:
1138:
1134:
1130:
1123:
1115:
1111:
1107:
1103:
1099:
1095:
1090:
1085:
1081:
1077:
1070:
1063:
1059:
1055:
1051:
1044:
1042:
1033:
1028:
1023:
1018:
1014:
1010:
1006:
1002:
995:
993:
985:
981:
977:
970:
968:
960:
956:
952:
948:
941:
939:
937:
935:
927:
923:
919:
915:
911:
907:
902:
897:
893:
889:
882:
880:
878:
876:
874:
872:
867:
859:
857:
856:solar antapex
852:
850:
846:
842:
838:
834:
829:
827:
823:
819:
815:
812:of an unseen
811:
807:
803:
802:F. E. Harpham
799:
795:
791:
790:G. E. Paddock
781:
779:
775:
771:
768:In 2016, the
766:
764:
760:
756:
754:
753:
748:
744:
740:
736:
732:
727:
725:
721:
717:
713:
709:
700:
698:
694:
690:
686:
682:
678:
674:
670:
666:
662:
661:constellation
658:
652:
629:
626:, also named
625:
621:
613:
610:
608:
607:
603:
602:
597:
593: 196698
592:
588:
585: 30122,
584:
581: 44402,
580:
576:
570:
565:
561:
555:
552:
548:
544:
541:
530:
528:
527:
523:
522:
518:
516:
514:
510:
506:
502:
501:
498:
494:
492:
491:
487:
486:
483:
479:
477:
475:
471:
467:
466:
463:
454:
452:
451:
447:
446:
443:
434:
432:
431:
427:
426:
423:
407:
405:
404:
400:
399:
395:
390:
386:
377:
376:
372:
371:
367:
362:
360:
355:
354:
350:
345:
342:
340:
337:
332:
331:
327:
325:
323:
319:
318:
315:675 days
314:
312:
310:
306:
305:
302:
298:
294:
290:
288:
282:
278:
277:
273:
268:
265:362 ± 5
264:
262:
261:
257:
256:
253:
249:
247:
245:
241:
240:
237:
233:
225:
221:
214:
212:
210:
209:Proper motion
206:
205:
201:
199:
193:
189:
188:
184:
181:
177:
174:
170:
168:
165:
164:
160:
158:
154:
153:
149:
147:
143:
142:
138:
136:
133:
132:
127:
123:
119:
115:
114:
110:
108:
105:
104:
98:
95:
91:
90:
87:
84:
82:
81:Constellation
79:
78:
75:
72:
68:
65:
59:
47:
40:
30:
22:
1795:
1688:, retrieved
1683:
1659:, retrieved
1655:the original
1650:
1641:
1616:
1612:
1606:
1579:
1575:
1569:
1557:. Retrieved
1545:
1533:. Retrieved
1524:
1514:, retrieved
1494:
1489:Allen, R. H.
1483:
1464:
1458:
1446:. Retrieved
1437:
1427:, retrieved
1422:
1413:
1387:
1383:
1377:
1335:
1331:
1292:
1288:
1233:
1227:
1188:
1184:
1132:
1128:
1122:
1079:
1075:
1069:
1049:
1004:
1000:
975:
950:
946:
891:
887:
853:
830:
826:eccentricity
787:
777:
772:organized a
767:
763:al-ʼaghribah
762:
757:
750:
742:
734:
730:
728:
724:Johann Bayer
715:
707:
706:
627:
623:
619:
618:
604:
589: 2282,
524:
519:25 km/s
512:
508:
503:
495:18,700
488:
473:
468:
448:
428:
401:
373:
357:
334:
322:Eccentricity
320:
307:
279:
258:
242:
207:
190:
139:B2.5 V
2440:Canis Major
1619:: 239–242,
1582:: 229–231,
1135:: 727–732,
691:) from the
665:Canis Major
657:binary star
577: 240,
490:Temperature
455:3,603
365:(secondary)
157:color index
146:color index
107:Declination
86:Canis Major
2424:Categories
2254:Messier 41
2180:HD 43197 b
2170:HD 45364 b
2160:HD 47186 b
2150:HD 47536 b
2137:Exoplanets
1801:η (Aludra)
1791:ε (Adhara)
1776:β (Mirzam)
1771:α (Sirius)
1690:2012-02-16
1661:2012-01-16
1516:2010-12-12
1429:2012-02-15
1082:(5): 331,
1032:2066/36162
862:References
784:Properties
726:in 1603.
687:(111
472:(log
450:Luminosity
336:Periastron
180:Astrometry
171:Suspected
2386:SN 1999ec
1891:Flamsteed
1796:ζ (Furud)
1786:δ (Wezen)
1370:111387483
1345:1003.2335
1270:118629873
1243:1007.4883
1167:119387088
1114:119257644
1089:1108.4971
901:0708.1752
828:of 0.57.
712:Latinized
681:Hipparcos
480:4.0
435:3.9
387:13.5 km/s
384:(primary)
368:207°
120: (V)
2411:Category
2391:SN 2003H
2304:Galaxies
2285:NGC 2361
2280:NGC 2359
2233:NGC 2374
2228:NGC 2362
2223:NGC 2360
2218:NGC 2354
2213:NGC 2204
2196:clusters
1939:Variable
1491:(1963),
926:18759600
818:spectrum
752:Almagest
743:al-furūd
677:Parallax
461:☉
441:☉
421:☉
283: (M
260:Distance
244:Parallax
2360:IC 2163
2290:Sh2-297
2272:Nebulae
1962:UW (29)
1621:Bibcode
1584:Bibcode
1559:28 July
1448:28 July
1392:Bibcode
1350:Bibcode
1297:Bibcode
1248:Bibcode
1193:Bibcode
1147:Bibcode
1094:Bibcode
1058:Bibcode
1009:Bibcode
980:Bibcode
955:Bibcode
906:Bibcode
759:Al Sufi
741:ألفرود
655:, is a
392:Details
161:–0.195
124:+3.025
74:J2000.0
71:Equinox
67:J2000.0
2249:Gaia 1
1535:22 May
1507:
1471:
1368:
1268:
1165:
1112:
953:: 69,
924:
739:Arabic
735:Phurud
606:SIMBAD
538:
430:Radius
415:
309:Period
150:–0.71
2348:Other
2242:Other
2097:Other
2088:47186
2083:45364
2078:45184
1763:Bayer
1754:Stars
1684:Stars
1554:(PDF)
1366:S2CID
1340:arXiv
1266:S2CID
1238:arXiv
1163:S2CID
1137:arXiv
1110:S2CID
1084:arXiv
922:S2CID
896:arXiv
778:Furud
731:Furud
714:from
628:Furud
622:, or
339:epoch
301:Orbit
291:−2.21
228:Dec.:
173:β Cep
64:Epoch
2339:2283
2334:2280
2329:2227
2324:2217
2319:2207
2194:Star
2119:WR 7
2055:2812
2050:2766
2045:2764
2040:2758
2035:2450
2030:2447
2025:2437
2020:2318
1561:2016
1537:2016
1505:ISBN
1469:ISBN
1450:2016
703:Name
642:jʊər
612:data
532:32.0
403:Mass
328:0.57
155:B−V
144:U−B
2312:NGC
2205:NGC
1629:doi
1592:doi
1501:130
1400:doi
1388:573
1358:doi
1336:331
1305:doi
1293:189
1256:doi
1234:410
1201:doi
1189:629
1155:doi
1133:424
1102:doi
1027:hdl
1017:doi
1005:452
914:doi
892:474
733:or
693:Sun
663:of
591:SAO
583:HIP
575:FK5
540:Myr
536:0.4
526:Age
482:cgs
413:0.2
409:7.7
361:(ω)
341:(T)
324:(e)
311:(P)
252:mas
246:(π)
232:mas
220:mas
216:RA:
211:(μ)
2426::
2065:HD
2012:HR
2002:NR
1997:LS
1992:FY
1987:FS
1982:FN
1977:EZ
1972:CX
1967:VY
1929:27
1924:26
1919:17
1914:15
1909:12
1904:11
1899:10
1682:,
1649:,
1627:,
1617:30
1615:,
1590:,
1580:29
1578:,
1503:,
1421:,
1398:,
1386:,
1364:,
1356:,
1348:,
1334:,
1318:^
1303:,
1291:,
1277:^
1264:,
1254:,
1246:,
1232:,
1214:^
1199:,
1187:,
1175:^
1161:,
1153:,
1145:,
1131:,
1108:,
1100:,
1092:,
1080:38
1078:,
1040:^
1025:,
1015:,
1003:,
991:^
966:^
951:31
949:,
933:^
920:,
912:,
904:,
890:,
870:^
858:.
710:,
689:pc
685:ly
587:HR
579:HD
573:,
569:CD
566:,
562:,
378:(K
349:JD
272:pc
267:ly
236:yr
224:yr
194:(R
2175:c
2165:c
2155:c
1957:Z
1952:W
1947:R
1881:ω
1876:τ
1866:π
1861:ο
1856:ο
1851:ξ
1846:ξ
1841:ν
1836:ν
1831:ν
1826:μ
1821:λ
1816:κ
1811:ι
1806:θ
1720:e
1713:t
1706:v
1635:.
1631::
1623::
1600:.
1594::
1586::
1563:.
1539:.
1477:.
1452:.
1402::
1394::
1360::
1352::
1342::
1307::
1299::
1258::
1250::
1240::
1203::
1195::
1169:.
1157::
1149::
1139::
1116:.
1104::
1096::
1086::
1060::
1029::
1019::
1011::
982::
957::
916::
908::
898::
651:/
648:d
645:ə
639:f
636:ˈ
633:/
534:±
515:)
513:i
509:v
507:(
497:K
476:)
474:g
458:L
438:R
418:M
411:±
382:)
380:1
287:)
285:V
274:)
234:/
222:/
198:)
196:v
23:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
