32:
2814:
798:
39:
753:(Algenib), Beta Cassiopeiae was one of three bright stars known as the "Three Guides" marking the equinoctial colure. This is an imaginary line running due south from Beta Cassiopeiae through Alpha Andromedae to the celestial equator, at a point where the Sun's path (the ecliptic) crosses it each autumn and spring equinox.
884:
shape with an equatorial bulge that is 24% larger than the polar radius. This shape is causing the polar region to have a higher temperature than the equator: the temperature difference is about 1,000 K. The axis of rotation is inclined about 20 degrees to the line of sight from the Earth.
780:
As a star in the deep northern hemisphere of the sky, Beta
Cassiopeiae is prominent to viewers in the northern hemisphere but not often seen by those in the southern hemisphere. The constellation of Cassiopeia does not rise above the horizon to viewers in
672:"the stained hand" referred to the five stars comprising the 'W' of the constellation Cassiopeia, and depicted a hand stained with henna. The term was abbreviated and somehow came to signify β Cassiopeiae alone. The old "stained hand" was part of an
826:. More than three times the size of and 28 times brighter than the Sun, Caph has an absolute magnitude of +1.3. It was once an A-type star with about double the Sun's mass. It is now in the process of cooling and expanding to become a
993:
Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Robinson, P. E. (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars
Earlier than M0 within 40 Parsecs: The Northern Sample. I".
830:. Its core is likely to have used up its hydrogen and is shrinking and heating, while its outer envelope of hydrogen is expanding and cooling. Stars do not spend much time in this state and are relatively uncommon. Caph's
661:(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
1832:
506:
486:
1489:
372:
857:. It is a monoperiodic pulsator, with a brightness that ranges from magnitude +2.25 to +2.31 with a period of 2.5 hours. This type of variable includes subgiant or
970:
Kukarkin, B. V.; et al. (1971). "General
Catalogue of Variable Stars containing information on 20437 variable stars discovered and designated till 1968".
1706:
1641:
Delta Scuti and
Related Stars, Reference Handbook and Proceedings of the 6th Vienna Workshop in Astrophysics, held in Vienna, Austria, 4–7 August 1999
1825:
1117:
Evans, D. S. (June 20–24, 1966). "The
Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick (eds.).
2871:
2866:
680:
stretching from the
Pleiades, which signified the "head" through Taurus and Perseus and into Cassiopeia, while the other "hand" was in Cetus.
1689:
1471:
1342:
1639:
Poretti, E. (2000). "The
Frequency Content of δ Scuti Stars as Determined by Photometry". In Breger, Michel; Montgomery, Michael (eds.).
2846:
2817:
1818:
1752:
1545:
1520:
1433:
1292:
2861:
654:
462:
870:
2881:
1857:
1234:
60:
2886:
2851:
880:
This star is rotating at about 92% of its critical velocity, completing 1.12 rotations every day. This is giving the star an
1486:
410:
2784:
703:
478:
1852:
658:
1140:
Jaschek, C.; Gomez, A. E. (1998). "The absolute magnitude of the early type MK standards from HIPPARCOS parallaxes".
769:) of +2.28, it is one of the five stars which make up the 'W' of Cassiopeia, adjacent to the just brighter Schedar (
2876:
2841:
1841:
588:
73:
2092:
466:
1449:
1180:
Che, X.; et al. (May 2011). "Colder and Hotter: Interferometric
Imaging of β Cassiopeiae and α Leonis".
2306:
2301:
865:
and nearing the end of their core hydrogen fusion lifetime. Their pulsations are related to the same helium
1705:
Teays, Terry J.; Schmidt, Edward G.; Pasinetti
Fracassini, Laura E.; Fracassini, Massimo (15 August 1989).
2856:
2836:
2263:
816:
766:
596:
498:
474:
122:
1797:
1082:
Daszyńska, J.; Cugier, H. (2003). "Far-Ultraviolet light curves of the δ Scuti variable: β Cassiopeiae".
2602:
2200:
2190:
2014:
1789:
1746:
470:
458:
380:
1781:
1793:
1785:
1777:
1773:
1984:
1979:
1718:
1654:
1602:
1249:
1199:
1149:
1122:
1091:
1059:
1013:
975:
936:
889:
842:
673:
577:
246:
159:
1379:
1954:
1904:
494:
1400:
1308:
777:, traditionally known as Tycho's Star, appeared about 5 degrees to the northwest of Caph in 1572.
1934:
1734:
1644:
1618:
1592:
1215:
1189:
1029:
1003:
952:
926:
762:
723:
600:
267:
105:
1561:
1119:
Determination of Radial
Velocities and their Applications, Proceedings from IAU Symposium no. 30
2661:
1681:
31:
2004:
1969:
1929:
1919:
1899:
1894:
1884:
1876:
1685:
1541:
1516:
1467:
1429:
1338:
1288:
866:
770:
684:
615:
431:
56:
1235:"Ca II HK emission in rapidly rotating stars. Evidence for an onset of the solar-type dynamo"
527:
2332:
2170:
2165:
2160:
2155:
2145:
2140:
1924:
1909:
1726:
1673:
1610:
1257:
1253:
1207:
1153:
1099:
1021:
944:
940:
746:
719:
715:
711:
707:
556:
402:
347:
230:
38:
1358:
1999:
1994:
1989:
1974:
1964:
1914:
1805:
1493:
881:
360:
178:
81:
877:. Delta Scuti stars are located at the intersection of the strip with the main sequence.
1722:
1658:
1606:
1335:
A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations
1203:
1126:
1095:
1063:
1017:
979:
2322:
2135:
2130:
2125:
2120:
2115:
2110:
2082:
2077:
2072:
2067:
2062:
2057:
2052:
2047:
1959:
1949:
1944:
1939:
831:
502:
449:
238:
218:
206:
1103:
2830:
2726:
2337:
2105:
2100:
2042:
2037:
2032:
2027:
2022:
1738:
1674:
1211:
1121:. Vol. 30. University of Toronto: International Astronomical Union. p. 57.
1033:
892:
with a faint companion in a 27-day orbit, but it is now thought to be a single star.
858:
838:
584:
195:
154:
68:
1622:
1219:
956:
2671:
2641:
2636:
2451:
750:
327:
297:
1801:
1262:
2352:
948:
2746:
2741:
2464:
2433:
2428:
2423:
2418:
2413:
2408:
2403:
2398:
802:
797:
395:
144:
133:
94:
1050:
Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars".
2579:
2459:
2393:
1810:
917:
van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction".
862:
592:
340:
307:
253:
166:
2388:
2380:
2327:
2296:
2291:
2253:
2248:
2243:
2185:
2150:
827:
2766:
2761:
2666:
2615:
2574:
2569:
2564:
2286:
2281:
2238:
2233:
2175:
1649:
1597:
1583:
Buzasi, D. L.; et al. (2005). "Altair: The Brightest δ Scuti Star".
1008:
846:
782:
438:
1233:
Schröder, C.; Reiners, Ansgar; Schmitt, Jürgen H. M. M. (January 2009),
2797:
2792:
2710:
2705:
2700:
2651:
2610:
2559:
2554:
2549:
2544:
2539:
2534:
2529:
2524:
2519:
2514:
2509:
2504:
2499:
2494:
2489:
2484:
2479:
2474:
2469:
2347:
2276:
2271:
2213:
2208:
1769:
874:
774:
2685:
2656:
2646:
2593:
2228:
2223:
2218:
2180:
854:
822:
786:
521:
387:
320:
258:
1730:
1614:
1025:
2756:
2736:
2731:
2631:
2342:
1194:
931:
796:
2751:
2362:
2357:
1867:
850:
807:
580:
482:
222:
210:
1814:
861:
stars of spectral classes F5–A0, having masses between 1.5–2.5
845:; in fact, the fourth brightest of such stars in the sky after
490:
1496:, Hong Kong Space Museum. Accessed on line November 23, 2010.
603:(+2.28 mag, variable) has an absolute magnitude of +1.3 mag.
565:
1562:"MAST: Barbara A. Mikulski Archive for Space Telescopes"
1401:"Bulletin of the IAU Working Group on Star Names, No. 1"
1337:(2nd rev. ed.). Cambridge, Massachusetts: Sky Pub.
706:, refers to an asterism consisting of β Cassiopeiae,
568:
562:
457:
Caph, Chaph, Kaff, Al Sanam al Nakah,
1643:. ASP Conference Series. Vol. 210. p. 45.
1052:
Communications of the Lunar and Planetary Laboratory
631:
2783:
2719:
2693:
2684:
2624:
2601:
2592:
2450:
2379:
2315:
2262:
2199:
2091:
2013:
1875:
1866:
559:
1466:, written by 陳久金. Published by 台灣書房出版有限公司, 2005,
1287:. New York, NY: Dover Publications. p. 146.
815:Beta Cassiopeiae is a yellow-white hued giant of
1315:. Centre de Données astronomiques de Strasbourg
1634:
1632:
1448:Wang Liang was a famous charioteer during the
912:
910:
908:
906:
904:
1826:
1428:. Cambridge, MA: Sky Publishing. p. 26.
888:Beta Cassiopeiae was once considered to be a
733:
727:
695:
688:
99:+59° 08′ 59.2120″
8:
1506:
1504:
1502:
1309:"V* bet Cas—Variable Star of delta Sct type"
624:
2780:
2690:
2598:
2447:
2376:
1872:
1833:
1819:
1811:
1515:. New York: Copernicus Books. p. 27.
1175:
1173:
1171:
1169:
1167:
1165:
1163:
1648:
1596:
1261:
1193:
1077:
1075:
1073:
1007:
930:
819:F2 III with a surface temperature around
59:J2000
1380:"IAU Working Group on Star Names (WGSN)"
1278:
1276:
1274:
1272:
668:Originally, the pre-Islamic Arabic term
1680:. Cambridge University Press. pp.
1045:
1043:
900:
202:
1744:
1707:"The chromosphere of Beta Cassiopeiae"
18:
618:. It also bore the traditional names
7:
1424:Kunitzsch, Paul; Smart, Tim (2006).
1333:Kunitzsch, Paul; Smart, Tim (2006).
16:Star in the constellation Cassiopeia
1564:. Space Telescope Science Institute
972:General Catalogue of Variable Stars
805:for Beta Cassiopeiae, plotted from
625:
214:
48:Location of β Cassiopeiae (circled)
14:
1283:Allen, Richard Hinckley (1963) .
653:"the Camel's Hump". In 2016, the
2813:
2812:
655:International Astronomical Union
555:
37:
30:
1858:Cassiopeia in Chinese astronomy
1540:. Jacaranda Press. p. 84.
1426:Dictionary of Modern Star Names
2872:Henry Draper Catalogue objects
785:, and only low if one were in
1:
2867:Bright Star Catalogue objects
1751:: CS1 maint: date and year (
1285:Star-names and their meanings
1104:10.1016/S0273-1177(02)00630-0
641:reaching from the Pleiades),
1676:Understanding variable stars
740:the First Star of Wang Liang
726:for β Cassiopeiae itself is
704:Legs (Chinese constellation)
237:59.58 ± 0.38
1853:List of stars in Cassiopeia
1842:Constellation of Cassiopeia
1359:"IAU Catalog of Star Names"
1263:10.1051/0004-6361:200810377
871:Hertzsprung–Russell diagram
734:
696:
659:Working Group on Star Names
632:
2903:
2847:Cassiopeia (constellation)
1513:The Hundred Greatest Stars
1242:Astronomy and Astrophysics
1212:10.1088/0004-637X/732/2/68
1142:Astronomy and Astrophysics
1084:Advances in Space Research
949:10.1051/0004-6361:20078357
919:Astronomy and Astrophysics
2810:
2779:
2446:
2375:
1848:
1585:The Astrophysical Journal
1182:The Astrophysical Journal
739:
728:
689:
514:
455:
448:
444:
291:
286:
282:
172:
165:
116:
53:
24:
1511:Kaler, James B. (2002).
1450:Spring and Autumn period
996:The Astronomical Journal
2862:Stars with proper names
1672:Percy, John R. (2007).
1254:2009A&A...493.1099S
1154:1998A&A...330..619J
941:2007A&A...474..653V
268:Absolute magnitude
106:Apparent magnitude
20:Caph, Beta Cassiopeiae
2882:Durchmusterung objects
1536:Newell, W. J. (1965).
1487:香港太空館 - 研究資源 - 亮星中英對照表
837:Beta Cassiopeiae is a
812:
622:(from the Arabic word
2887:Gliese and GJ objects
2852:Delta Scuti variables
1711:Astrophysical Journal
873:as that of classical
800:
1768:Beta Cassiopeiae on
890:spectroscopic binary
722:. Consequently, the
599:. The white star of
578:Delta Scuti variable
550:), officially named
2785:Astronomical events
1806:Articles and images
1723:1989ApJ...343..916T
1659:2000ASPC..210...45P
1607:2005ApJ...619.1072B
1204:2011ApJ...732...68C
1127:1967IAUS...30...57E
1096:2003AdSpR..31..381D
1064:1966CoLPL...4...99J
1018:2003AJ....126.2048G
980:1971GCVS3.C......0K
834:is unusually weak.
515:Database references
411:Rotational velocity
217: −179.77
205: +523.50
21:
1538:The Australian Sky
1492:2009-09-29 at the
813:
763:apparent magnitude
509: J00092+5909
450:Other designations
155:Variable type
123:Spectral type
112:+2.28 (2.25–2.31)
19:
2877:Hipparcos objects
2842:Flamsteed objects
2824:
2823:
2806:
2805:
2775:
2774:
2680:
2679:
2588:
2587:
2442:
2441:
2371:
2370:
1691:978-0-521-23253-1
1472:978-986-7332-25-7
1344:978-1-931559-44-7
867:instability strip
771:Alpha Cassiopeiae
670:al-Kaff al-Khadib
651:al-Sanam al-Nakah
616:Bayer designation
597:spectral class F2
595:belonging to the
533:
532:
257:(16.8 ± 0.1
2894:
2816:
2815:
2781:
2691:
2662:LBN 114.55+00.22
2599:
2448:
2377:
2287:17156 (Nushagak)
1873:
1835:
1828:
1821:
1812:
1757:
1756:
1750:
1742:
1702:
1696:
1695:
1679:
1669:
1663:
1662:
1652:
1650:astro-ph/0002304
1636:
1627:
1626:
1600:
1598:astro-ph/0405127
1580:
1574:
1573:
1571:
1569:
1558:
1552:
1551:
1533:
1527:
1526:
1508:
1497:
1485:
1481:
1475:
1462:
1458:
1452:
1446:
1440:
1439:
1421:
1415:
1414:
1412:
1410:
1405:
1397:
1391:
1390:
1388:
1386:
1376:
1370:
1369:
1367:
1365:
1355:
1349:
1348:
1330:
1324:
1323:
1321:
1320:
1305:
1299:
1298:
1280:
1267:
1266:
1265:
1248:(3): 1099–1107,
1239:
1230:
1224:
1223:
1197:
1177:
1158:
1157:
1137:
1131:
1130:
1114:
1108:
1107:
1079:
1068:
1067:
1047:
1038:
1037:
1011:
1009:astro-ph/0308182
990:
984:
983:
974:(3rd ed.).
967:
961:
960:
934:
914:
843:Delta Scuti type
825:
749:(Alpheratz) and
747:Alpha Andromedae
741:
737:
731:
730:
699:
692:
691:
635:
628:
627:
612:Beta Cassiopeiae
601:second magnitude
575:
574:
571:
570:
567:
564:
561:
536:Beta Cassiopeiae
305:
252:54.7 ± 0.3
216:
204:
117:Characteristics
109:
89:
84:
54:Observation data
41:
34:
22:
2902:
2901:
2897:
2896:
2895:
2893:
2892:
2891:
2827:
2826:
2825:
2820:
2802:
2771:
2715:
2676:
2620:
2584:
2438:
2367:
2333:IRAS 23304+6147
2311:
2258:
2195:
2087:
2009:
1862:
1844:
1839:
1765:
1760:
1743:
1704:
1703:
1699:
1692:
1684:–144, 182–187.
1671:
1670:
1666:
1638:
1637:
1630:
1582:
1581:
1577:
1567:
1565:
1560:
1559:
1555:
1548:
1535:
1534:
1530:
1523:
1510:
1509:
1500:
1494:Wayback Machine
1483:
1482:
1478:
1460:
1459:
1455:
1447:
1443:
1436:
1423:
1422:
1418:
1408:
1406:
1403:
1399:
1398:
1394:
1384:
1382:
1378:
1377:
1373:
1363:
1361:
1357:
1356:
1352:
1345:
1332:
1331:
1327:
1318:
1316:
1307:
1306:
1302:
1295:
1282:
1281:
1270:
1237:
1232:
1231:
1227:
1179:
1178:
1161:
1139:
1138:
1134:
1116:
1115:
1111:
1081:
1080:
1071:
1049:
1048:
1041:
992:
991:
987:
969:
968:
964:
916:
915:
902:
898:
882:oblate spheroid
820:
795:
759:
665:for this star.
609:
558:
554:
510:
437:1.09–1.18
417: sin
361:Surface gravity
353:
350:
333:
330:
326:3.43–3.69
313:
310:
303:
273:
256:
213:
184:
179:Radial velocity
104:
87:
82:Right ascension
80:
55:
49:
47:
46:
45:
44:
43:
42:
17:
12:
11:
5:
2900:
2898:
2890:
2889:
2884:
2879:
2874:
2869:
2864:
2859:
2854:
2849:
2844:
2839:
2829:
2828:
2822:
2821:
2811:
2808:
2807:
2804:
2803:
2801:
2800:
2795:
2789:
2787:
2777:
2776:
2773:
2772:
2770:
2769:
2764:
2759:
2754:
2749:
2744:
2739:
2734:
2729:
2723:
2721:
2717:
2716:
2714:
2713:
2708:
2703:
2697:
2695:
2688:
2682:
2681:
2678:
2677:
2675:
2674:
2669:
2664:
2659:
2654:
2649:
2644:
2639:
2634:
2628:
2626:
2622:
2621:
2619:
2618:
2613:
2607:
2605:
2596:
2590:
2589:
2586:
2585:
2583:
2582:
2577:
2572:
2567:
2562:
2557:
2552:
2547:
2542:
2537:
2532:
2527:
2522:
2517:
2512:
2507:
2502:
2497:
2492:
2487:
2482:
2477:
2472:
2467:
2462:
2456:
2454:
2444:
2443:
2440:
2439:
2437:
2436:
2431:
2426:
2421:
2416:
2411:
2406:
2401:
2396:
2391:
2385:
2383:
2373:
2372:
2369:
2368:
2366:
2365:
2360:
2355:
2350:
2345:
2343:PSR J0205+6449
2340:
2335:
2330:
2325:
2319:
2317:
2313:
2312:
2310:
2309:
2304:
2299:
2294:
2289:
2284:
2279:
2274:
2268:
2266:
2260:
2259:
2257:
2256:
2251:
2246:
2241:
2236:
2231:
2226:
2221:
2216:
2211:
2205:
2203:
2197:
2196:
2194:
2193:
2188:
2183:
2178:
2173:
2168:
2163:
2158:
2153:
2148:
2143:
2138:
2133:
2128:
2123:
2118:
2113:
2108:
2103:
2097:
2095:
2089:
2088:
2086:
2085:
2080:
2075:
2070:
2065:
2060:
2055:
2050:
2045:
2040:
2035:
2030:
2025:
2019:
2017:
2011:
2010:
2008:
2007:
2002:
1997:
1992:
1987:
1982:
1977:
1972:
1967:
1962:
1957:
1952:
1947:
1942:
1937:
1932:
1927:
1922:
1917:
1912:
1907:
1902:
1897:
1892:
1887:
1881:
1879:
1870:
1864:
1863:
1861:
1860:
1855:
1849:
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1838:
1837:
1830:
1823:
1815:
1809:
1808:
1764:
1763:External links
1761:
1759:
1758:
1731:10.1086/167761
1697:
1690:
1664:
1628:
1615:10.1086/426704
1591:(2): 1072–76.
1575:
1553:
1546:
1528:
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1498:
1476:
1453:
1441:
1434:
1416:
1392:
1371:
1350:
1343:
1325:
1300:
1293:
1268:
1225:
1159:
1132:
1109:
1090:(2): 381–386.
1069:
1039:
1026:10.1086/378365
985:
962:
925:(2): 653–664.
899:
897:
894:
794:
791:
758:
755:
745:Together with
614:is the star's
608:
605:
542:, abbreviated
531:
530:
525:
517:
516:
512:
511:
456:
453:
452:
446:
445:
442:
441:
435:
427:
426:
425:71.0 km/s
423:
406:
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391:
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384:
376:
375:
369:
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271:
263:
262:
250:
242:
241:
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200:
191:
190:
189:11.3 km/s
187:
182:
174:
173:
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162:
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88:00 09 10.68518
85:
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36:
35:
29:
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25:
15:
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10:
9:
6:
4:
3:
2:
2899:
2888:
2885:
2883:
2880:
2878:
2875:
2873:
2870:
2868:
2865:
2863:
2860:
2858:
2857:F-type giants
2855:
2853:
2850:
2848:
2845:
2843:
2840:
2838:
2837:Bayer objects
2835:
2834:
2832:
2819:
2809:
2799:
2796:
2794:
2791:
2790:
2788:
2786:
2782:
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2755:
2753:
2750:
2748:
2745:
2743:
2740:
2738:
2735:
2733:
2730:
2728:
2727:Andromeda VII
2725:
2724:
2722:
2718:
2712:
2709:
2707:
2704:
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2476:
2473:
2471:
2468:
2466:
2463:
2461:
2458:
2457:
2455:
2453:
2452:Star clusters
2449:
2445:
2435:
2432:
2430:
2427:
2425:
2422:
2420:
2417:
2415:
2412:
2410:
2407:
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2400:
2397:
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2278:
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2255:
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2250:
2247:
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2242:
2240:
2237:
2235:
2232:
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2227:
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2222:
2220:
2217:
2215:
2212:
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2204:
2202:
2198:
2192:
2189:
2187:
2184:
2182:
2179:
2177:
2174:
2172:
2169:
2167:
2164:
2162:
2159:
2157:
2154:
2152:
2149:
2147:
2144:
2142:
2139:
2137:
2134:
2132:
2129:
2127:
2124:
2122:
2119:
2117:
2114:
2112:
2109:
2107:
2104:
2102:
2099:
2098:
2096:
2094:
2090:
2084:
2081:
2079:
2076:
2074:
2071:
2069:
2066:
2064:
2061:
2059:
2056:
2054:
2051:
2049:
2046:
2044:
2041:
2039:
2036:
2034:
2031:
2029:
2026:
2024:
2021:
2020:
2018:
2016:
2012:
2006:
2003:
2001:
1998:
1996:
1993:
1991:
1988:
1986:
1983:
1981:
1978:
1976:
1973:
1971:
1968:
1966:
1963:
1961:
1958:
1956:
1953:
1951:
1948:
1946:
1943:
1941:
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1931:
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1926:
1923:
1921:
1918:
1916:
1913:
1911:
1908:
1906:
1903:
1901:
1898:
1896:
1895:γ (Navi/Tsih)
1893:
1891:
1888:
1886:
1883:
1882:
1880:
1878:
1874:
1871:
1869:
1865:
1859:
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1836:
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1817:
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1698:
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1668:
1665:
1660:
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1629:
1624:
1620:
1616:
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1608:
1604:
1599:
1594:
1590:
1586:
1579:
1576:
1563:
1557:
1554:
1549:
1547:0-7016-0037-3
1543:
1539:
1532:
1529:
1524:
1522:0-387-95436-8
1518:
1514:
1507:
1505:
1503:
1499:
1495:
1491:
1488:
1480:
1477:
1473:
1469:
1465:
1457:
1454:
1451:
1445:
1442:
1437:
1435:1-931559-44-9
1431:
1427:
1420:
1417:
1402:
1396:
1393:
1381:
1375:
1372:
1360:
1354:
1351:
1346:
1340:
1336:
1329:
1326:
1314:
1310:
1304:
1301:
1296:
1294:1-931559-44-9
1290:
1286:
1279:
1277:
1275:
1273:
1269:
1264:
1259:
1255:
1251:
1247:
1243:
1236:
1229:
1226:
1221:
1217:
1213:
1209:
1205:
1201:
1196:
1191:
1187:
1183:
1176:
1174:
1172:
1170:
1168:
1166:
1164:
1160:
1155:
1151:
1147:
1143:
1136:
1133:
1128:
1124:
1120:
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1110:
1105:
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986:
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950:
946:
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920:
913:
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909:
907:
905:
901:
895:
893:
891:
886:
883:
878:
876:
872:
868:
864:
860:
859:main-sequence
856:
852:
848:
844:
840:
839:variable star
835:
833:
829:
824:
818:
817:stellar class
810:
809:
804:
799:
792:
790:
788:
784:
778:
776:
772:
768:
764:
756:
754:
752:
748:
743:
736:
735:Wáng Liáng yī
725:
721:
720:λ Cassiopeiae
717:
716:α Cassiopeiae
713:
712:η Cassiopeiae
709:
708:κ Cassiopeiae
705:
701:
698:
686:
681:
679:
675:
671:
666:
664:
660:
656:
652:
649:, as well as
648:
644:
640:
636:
634:
629:
621:
617:
613:
606:
604:
602:
598:
594:
590:
586:
585:constellation
582:
579:
573:
553:
549:
545:
541:
540:β Cassiopeiae
537:
529:
526:
524:
523:
519:
518:
513:
508:
504:
500:
496:
492:
489: 21133,
488:
485: 16.00,
484:
480:
476:
472:
468:
464:
460:
454:
451:
447:
443:
440:
436:
434:
433:
429:
428:
424:
422:
420:
416:
412:
408:
407:
404:
400:
398:
397:
393:
392:
389:
385:
383:
382:
378:
377:
374:
370:
368:
366:
362:
358:
357:
354:
345:
343:
342:
338:
337:
334:
325:
323:
322:
318:
317:
314:
302:
300:
299:
295:
294:
290:
285:
281:
277:
275:
269:
265:
264:
260:
255:
251:
249:
248:
244:
243:
240:
236:
234:
232:
228:
227:
224:
220:
212:
208:
201:
199:
197:
196:Proper motion
193:
192:
188:
186:
180:
176:
175:
171:
168:
164:
161:
158:
156:
153:
152:
148:
146:
142:
141:
137:
135:
131:
130:
126:
124:
121:
120:
115:
111:
107:
103:
102:
98:
96:
93:
92:
86:
83:
79:
78:
75:
72:
70:
69:Constellation
67:
66:
62:
58:
52:
40:
33:
23:
2672:Westerhout 5
2642:Heart Nebula
2637:Cassiopeia A
2338:LS I +61 303
1889:
1747:cite journal
1714:
1710:
1700:
1675:
1667:
1640:
1588:
1584:
1578:
1566:. Retrieved
1556:
1537:
1531:
1512:
1484:(in Chinese)
1479:
1463:
1461:(in Chinese)
1456:
1444:
1425:
1419:
1407:. Retrieved
1395:
1383:. Retrieved
1374:
1362:. Retrieved
1353:
1334:
1328:
1317:. Retrieved
1312:
1303:
1284:
1245:
1241:
1228:
1185:
1181:
1145:
1141:
1135:
1118:
1112:
1087:
1083:
1055:
1051:
999:
995:
988:
971:
965:
922:
918:
887:
879:
863:solar masses
836:
814:
806:
779:
761:With a mean
760:
751:Gamma Pegasi
744:
724:Chinese name
693:
682:
677:
669:
667:
662:
657:organized a
650:
646:
642:
638:
630:
623:
619:
611:
610:
607:Nomenclature
551:
547:
543:
539:
535:
534:
520:
481: 1027,
430:
418:
414:
409:
394:
379:
364:
359:
339:
319:
296:
266:
245:
229:
194:
177:
2798:SN 1572 (B)
2747:Dwingeloo 2
2742:Dwingeloo 1
2465:Messier 103
2434:HD 240237 b
2429:HD 240210 b
2399:HD 219134 b
1985:υ (Castula)
1900:δ (Ruchbah)
1885:α (Schedar)
1002:(4): 2048.
821:7,000
803:light curve
738:, English:
637:, "palm" –
505: 107,
501: 147,
497: 746,
477: 432,
396:Metallicity
386:7,079
381:Temperature
304:1.91 ± 0.02
145:color index
134:color index
95:Declination
2831:Categories
2580:Trumpler 3
2460:Messier 52
2394:HD 17156 b
2381:Exoplanets
2353:4U 0142+61
2323:BD+60°2522
1920:θ (Marfak)
1915:η (Achird)
1798:Astrophoto
1790:Hydrogen α
1568:8 December
1319:2011-12-16
1058:(99): 99.
896:References
757:Visibility
697:Wáng Liáng
593:giant star
591:. It is a
589:Cassiopeia
469: 21,
401:0.03
371:3.40
363:(log
346:27.3
341:Luminosity
167:Astrometry
74:Cassiopeia
2389:HD 7924 b
2328:Gliese 49
2015:Flamsteed
1905:ε (Segin)
1739:121071246
1195:1105.0740
1188:(2): 68.
1034:119417105
932:0708.1752
828:red giant
702:, in the
493: 2,
465: 8,
108: (V)
2818:Category
2767:Maffei 2
2762:Maffei 1
2686:Galaxies
2667:Sh 2-185
2575:NGC 7790
2570:NGC 7789
2565:NGC 1027
2093:Variable
1910:ζ (Fulu)
1890:β (Caph)
1623:16524681
1490:Archived
1409:9 August
1364:9 August
1220:14330106
957:18759600
875:Cepheids
847:Denebola
783:Tasmania
674:asterism
544:Beta Cas
352:☉
332:☉
312:☉
270: (M
247:Distance
231:Parallax
2793:SN 1181
2652:IC 1805
2594:Nebulae
2560:NGC 663
2555:NGC 659
2550:NGC 654
2545:NGC 637
2540:NGC 559
2535:NGC 457
2530:NGC 436
2525:NGC 433
2520:NGC 381
2515:NGC 366
2510:NGC 358
2505:NGC 225
2500:NGC 189
2495:NGC 146
2490:NGC 136
2485:NGC 133
2480:NGC 129
2475:NGC 110
2470:NGC 103
2348:Tycho G
2121:YZ (21)
1802:Sky Map
1770:WikiSky
1719:Bibcode
1717:: 916.
1655:Bibcode
1603:Bibcode
1250:Bibcode
1200:Bibcode
1150:Bibcode
1148:: 619.
1123:Bibcode
1092:Bibcode
1060:Bibcode
1014:Bibcode
976:Bibcode
937:Bibcode
869:on the
841:of the
775:SN 1572
685:Chinese
678:Thuraya
676:called
583:in the
576:, is a
473:+58°3,
287:Details
127:F2 III
61:Equinox
2657:KjPn 8
2647:IC 289
2307:240430
2302:240429
2297:240237
2292:240210
2068:48 (A)
1737:
1688:
1621:
1544:
1519:
1470:
1464:中國星座神話
1432:
1385:22 May
1341:
1313:SIMBAD
1291:
1218:
1032:
955:
855:Altair
832:corona
793:System
787:Cairns
767:V-band
522:SIMBAD
321:Radius
306:
63:J2000
2757:IC 10
2737:3C 35
2732:3C 20
2720:Other
2632:3C 58
2625:Other
2414:e (h)
2316:Other
2282:15558
2191:V1405
2186:V1022
1877:Bayer
1868:Stars
1794:X-Ray
1782:GALEX
1735:S2CID
1645:arXiv
1619:S2CID
1593:arXiv
1404:(PDF)
1238:(PDF)
1216:S2CID
1190:arXiv
1030:S2CID
1004:arXiv
953:S2CID
927:arXiv
643:Chaph
548:β Cas
461:Cas,
215:Dec.:
160:δ Sct
149:0.34
138:0.11
57:Epoch
2752:MB 3
2616:7635
2363:WR 3
2358:WR 2
2277:7977
2272:7924
2254:8881
2249:8853
2244:8832
2181:V987
2176:V773
2171:V863
2166:V762
2161:V705
2156:V669
2151:V547
2146:V509
2141:V373
1786:IRAS
1778:SDSS
1774:DSS2
1753:link
1686:ISBN
1570:2021
1542:ISBN
1517:ISBN
1468:ISBN
1430:ISBN
1411:2023
1387:2016
1366:2023
1339:ISBN
1289:ISBN
853:and
851:Vega
811:data
808:TESS
718:and
663:Caph
647:Kaff
645:and
639:i.e.
620:Caph
581:star
552:Caph
528:data
507:CCDM
483:GCTP
298:Mass
278:+1.3
143:B−V
132:U−B
2711:278
2706:185
2701:147
2694:NGC
2611:281
2603:NGC
2239:932
2234:743
2229:297
2224:273
2219:244
2214:196
2209:144
1727:doi
1715:343
1682:139
1611:doi
1589:619
1258:doi
1246:493
1208:doi
1186:732
1146:330
1100:doi
1022:doi
1000:126
945:doi
923:474
773:).
742:.)
729:王良一
683:In
633:kaf
587:of
546:or
503:ADS
495:HIP
491:FK5
487:SAO
479:LHS
439:Gyr
432:Age
403:dex
373:cgs
239:mas
233:(π)
219:mas
207:mas
203:RA:
198:(μ)
2833::
2264:HD
2201:HR
2136:PZ
2131:AR
2126:AO
2116:WZ
2111:TZ
2083:54
2078:50
2073:49
2063:47
2058:42
2053:12
2048:10
1804:,
1800:,
1796:,
1792:,
1788:,
1784:,
1780:,
1776:,
1772::
1749:}}
1745:{{
1733:.
1725:.
1713:.
1709:.
1653:.
1631:^
1617:.
1609:.
1601:.
1587:.
1501:^
1311:.
1271:^
1256:,
1244:,
1240:,
1214:.
1206:.
1198:.
1184:.
1162:^
1144:.
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