29:
2991:
36:
976:
of Mu
Cassiopeiae has caused it to almost double its distance from B. There are now two other stars brighter than magnitude 10 that are closer to Mu Cassiopeiae, although they are also background objects. The companions C and D are separated from each-other by four
1612:
Boyajian, Tabetha S.; et al. (August 2008). "Angular
Diameters of the G Subdwarf μ Cassiopeiae A and the K Dwarfs σ Draconis and HR 511 from Interferometric Measurements with the CHARA Array".
949:
This is one of the first high-velocity stars to be identified. Compared to other nearby stars including the Sun, this pair are moving at a relatively high velocity of 167 km/s through the
1848:
Lippincott, S. L.; Wyckoff, S. (September 1964). "Parallax and orbital motion of the astrometric binary mu
Cassiopeiae from photographs taken with the 24-inch Sproul refractor".
2009:
1142:
Nordström, B.; et al. (May 2004). "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs".
806:
801:
571:
1015:, allowing an initial estimate of separate masses. The companion is over six magnitudes (330 times) fainter than the primary star, and it is presumed to be a
2002:
3058:
946:, or abundance of heavy elements, is about one-sixth that in the Sun. It is slightly smaller than the Sun with less mass and a lower luminosity.
1206:
Drummond, Jack D; Christou, Julian C; Fugate, Robert Q (1995). "Full
Adaptive Optics Images of ADS 9731 and MU Cassiopeiae: Orbits and Masses".
3073:
903:, and the name was from Al Marfik or Al Mirfaq (المرفق), meaning "the elbow". It is dimly visible to the naked eye as a point of light with an
1559:
992:, a star that is observed to oscillate due to the gravitational influence of an unseen companion, and that companion has now been resolved.
972:. All are distant background objects fainter than 11th magnitude. The brightest of these is catalogued as component B, but the very high
1400:
Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data
Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".
1011:. In 1966, the individual components were first resolved by the American astronomer Peter A. Wehinger using the 84-inch reflector at the
3038:
3023:
3013:
2994:
1995:
1596:
1486:
Mamajek, Eric E.; et al. (November 2008). "Improved Age
Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics".
1884:
785:
3048:
2034:
57:
3063:
1012:
969:
1308:"Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age"
623:
2961:
816:
812:
999:. Since then the orbital elements of the two stars have been fairly well established. The two stars are separated by a
2029:
820:
777:
1790:
1719:
1058:
3068:
3053:
2018:
1588:
864:
70:
3028:
3018:
2269:
1777:
1706:
1045:
904:
797:
1116:
1831:
1760:
2483:
2478:
1244:
Keenan, Philip C; McNeil, Raymond C (1989). "The
Perkins catalog of revised MK types for the cooler stars".
924:
3043:
2440:
1665:
Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001).
1539:
789:
781:
438:
121:
3033:
2779:
2377:
2367:
2191:
996:
771:
766:
739:
579:
392:
2161:
2156:
1961:
1918:
1857:
1809:
1738:
1678:
1631:
1505:
1450:
1409:
1374:
1329:
1253:
1215:
1161:
1077:
352:
249:
2131:
2081:
793:
2111:
1799:
1728:
1647:
1621:
1521:
1495:
1468:
1440:
1347:
1319:
1269:
1177:
1151:
1095:
1067:
989:
957:
270:
102:
1427:
Jao, Wei-Chun; Nelan, Edmund P.; Henry, Todd J.; Franz, Otto G.; Wasserman, Lawrence H. (2016).
2838:
1909:
Wehinger, Peter A.; Wyckoff, Susan (February 1966). "Preliminary Mass
Determination of μ Cas".
28:
2181:
2146:
2106:
2096:
2076:
2071:
2061:
2053:
1592:
1555:
1551:
1544:
1008:
1004:
900:
762:
644:
417:
53:
2509:
2347:
2342:
2337:
2332:
2322:
2317:
2101:
2086:
2066:
1969:
1926:
1865:
1819:
1814:
1748:
1743:
1686:
1639:
1513:
1458:
1382:
1337:
1261:
1223:
1169:
1165:
1106:
1085:
1081:
995:
In 1961, the close binary nature of this system was discovered by
Nicholas E. Wagman at the
916:
873:
726:
615:
539:
233:
841:
2176:
2171:
2166:
2151:
2141:
2091:
920:
552:
331:
181:
78:
1667:"The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog"
1965:
1922:
1861:
1682:
1635:
1509:
1454:
1413:
1378:
1333:
1257:
1219:
2499:
2312:
2307:
2302:
2297:
2292:
2287:
2259:
2254:
2249:
2244:
2239:
2234:
2229:
2224:
2136:
2126:
2121:
1000:
931:
753:
308:
241:
221:
209:
1463:
1428:
3007:
2903:
2514:
2282:
2277:
2219:
2214:
2209:
2204:
2199:
1351:
1273:
1099:
973:
939:
861:
198:
159:
65:
1525:
1472:
1365:
Carney, B. W. (October 1979). "Subdwarf ultraviolet excesses and metal abundances".
1181:
2848:
2818:
2813:
2628:
1888:
1651:
1110:
708:
674:
512:
471:
1824:
1781:
1753:
1710:
1429:"Cool Subdwarf Investigations. III. Dynamical Masses of Low-metallicity Subdwarfs"
1090:
1049:
2529:
1582:
1402:
VizieR On-line Data
Catalog: B/GCVS. Originally Published in: 2009yCat....102025S
1173:
2923:
2918:
2641:
2610:
2605:
2600:
2595:
2590:
2585:
2580:
2575:
943:
857:
601:
371:
143:
132:
91:
1982:
1342:
1307:
960:
stars that are thought to have formed before the galactic disk first appeared.
2756:
2636:
2570:
1987:
984:
978:
908:
688:
525:
485:
414:
256:
169:
2565:
2557:
2504:
2473:
2468:
2430:
2425:
2420:
2362:
2327:
1016:
950:
2943:
2938:
2843:
2792:
2751:
2746:
2741:
2463:
2458:
2415:
2410:
2352:
1156:
935:
661:
35:
2974:
2969:
2887:
2882:
2877:
2828:
2787:
2736:
2731:
2726:
2721:
2716:
2711:
2706:
2701:
2696:
2691:
2686:
2681:
2676:
2671:
2666:
2661:
2656:
2651:
2646:
2524:
2453:
2448:
2390:
2385:
2862:
2833:
2823:
2770:
2405:
2400:
2395:
2357:
1835:
1764:
1120:
953:
835:
746:
701:
593:
498:
261:
1054:
Early Data Release 3: Summary of the contents and survey properties"
1974:
1949:
1930:
1869:
1804:
1733:
1691:
1666:
1643:
1517:
1445:
1386:
1324:
1265:
1227:
1072:
2933:
2913:
2908:
2808:
2519:
1626:
1500:
968:
There are five visible companions to Mu Cassiopeiae listed in the
290:
2928:
2539:
2534:
2044:
322:
225:
213:
1991:
1786:
Data Release 2: Summary of the contents and survey properties"
1715:
Data Release 2: Summary of the contents and survey properties"
1550:(Reprint ed.). New York: Dover Publications Inc. p.
912:
923:
of −98 km/s. This star will move into the constellation
882:
938:, meaning it has a luminosity below that expected for a G5
888:
907:
of 5.16. The system is located at a distance of 25
1954:
Publications of the Astronomical Society of the Pacific
891:
885:
2960:
2896:
2870:
2861:
2801:
2778:
2769:
2627:
2556:
2492:
2439:
2376:
2268:
2190:
2052:
2043:
930:Mu Cassiopeiae is given as a standard star for the
879:
876:
1780:; et al. (Gaia collaboration) (August 2018).
1709:; et al. (Gaia collaboration) (August 2018).
1543:
1301:
1299:
1297:
1295:
1293:
1291:
1289:
1287:
1285:
1283:
934:G5Vb, although it is frequently described as a
1306:Bond, Howard E.; et al. (December 2020).
2003:
96:+54° 55′ 12.5612″
8:
1137:
1135:
1133:
1131:
1129:
1019:, a class M main sequence or subdwarf star.
988:away. Mu Cassiopeiae itself is known as an
1950:"An astrometric study of four binary stars"
1048:; et al. (Gaia collaboration) (2021).
2957:
2867:
2775:
2624:
2553:
2049:
2010:
1996:
1988:
1201:
1199:
1197:
1195:
1193:
1191:
1973:
1823:
1813:
1803:
1752:
1742:
1732:
1690:
1625:
1499:
1462:
1444:
1341:
1323:
1239:
1237:
1155:
1089:
1071:
56:J2000
1246:Astrophysical Journal Supplement Series
1028:
205:
1584:Patrick Moore's Data Book of Astronomy
15:
1948:Heintz, W. D.; Cantor, B. A. (1994).
1040:
1038:
1036:
1034:
1032:
7:
919:, and is moving closer with a high
217:
45:Location of μ Cassiopeiae (circled)
1581:Patrick Moore; Robin Rees (2011).
1546:Star Names: Their Lore and Meaning
14:
240:130.2881 ± 0.4348
2990:
2989:
1117:Gaia EDR3 record for this source
1007:with distance range of 3.3-11.9
872:
34:
27:
2035:Cassiopeia in Chinese astronomy
1832:Gaia DR2 record for this source
1761:Gaia DR2 record for this source
981:and form a binary system about
3059:Henry Draper Catalogue objects
1013:Kitt Peak National Observatory
970:Washington Double Star Catalog
867:. This system shares the name
1:
3074:Bright Star Catalogue objects
1367:Astrophysical Journal, Part 1
1791:Astronomy & Astrophysics
1720:Astronomy & Astrophysics
1111:10.1051/0004-6361/202039657e
1059:Astronomy & Astrophysics
2030:List of stars in Cassiopeia
2019:Constellation of Cassiopeia
1825:10.1051/0004-6361/201833051
1754:10.1051/0004-6361/201833051
1464:10.3847/0004-6256/152/6/153
1091:10.1051/0004-6361/202039657
3090:
3039:Cassiopeia (constellation)
3024:M-type main-sequence stars
3014:G-type main-sequence stars
1589:Cambridge University Press
1174:10.1051/0004-6361:20035959
1144:Astronomy and Astrophysics
2987:
2956:
2623:
2552:
2025:
1614:The Astrophysical Journal
1488:The Astrophysical Journal
1312:The Astrophysical Journal
905:apparent visual magnitude
828:
759:
752:
667:
464:
459:
289:
285:
175:
168:
115:
50:
21:
1671:The Astronomical Journal
1433:The Astronomical Journal
1343:10.3847/1538-4357/abc172
1815:2018A&A...616A...1G
1744:2018A&A...616A...1G
1166:2004A&A...418..989N
1082:2021A&A...649A...1G
271:Absolute magnitude
103:Apparent magnitude
3049:Durchmusterung objects
956:. They are low metal,
439:Argument of periastron
220: −1,564.844
208: +3,468.251
3064:Gliese and GJ objects
1883:Professor Jim Kaler.
1208:Astrophysical Journal
997:Allegheny Observatory
393:Longitude of the node
1911:Astronomical Journal
1850:Astronomical Journal
2962:Astronomical events
1966:1994PASP..106..363H
1923:1966AJ.....71Q.185W
1862:1964AJ.....69..471L
1683:2001AJ....122.3466M
1636:2008ApJ...683..424B
1510:2008ApJ...687.1264M
1455:2016AJ....152..153J
1414:2009yCat....102025S
1379:1979ApJ...233..211C
1334:2020ApJ...904..112B
1258:1989ApJS...71..245K
1220:1995ApJ...450..380D
829:Database references
767:30 Cassiopeiae
624:Rotational velocity
18:
990:astrometric binary
754:Other designations
260:(7.68 ± 0.03
255:25.03 ± 0.08
160:Variable type
122:Spectral type
16:
3069:Hipparcos objects
3054:Flamsteed objects
3001:
3000:
2983:
2982:
2952:
2951:
2857:
2856:
2765:
2764:
2619:
2618:
2548:
2547:
1561:978-0-486-21079-7
901:Theta Cassiopeiae
852:, Latinized from
847:
846:
3081:
3029:Solar-type stars
3019:G-type subdwarfs
2993:
2992:
2958:
2868:
2839:LBN 114.55+00.22
2776:
2625:
2554:
2464:17156 (Nushagak)
2050:
2012:
2005:
1998:
1989:
1983:SolStation entry
1979:
1977:
1935:
1934:
1906:
1900:
1899:
1897:
1896:
1887:. Archived from
1885:"Mu Cassiopeiae"
1880:
1874:
1873:
1845:
1839:
1829:
1827:
1817:
1807:
1774:
1768:
1758:
1756:
1746:
1736:
1703:
1697:
1696:
1694:
1662:
1656:
1655:
1629:
1609:
1603:
1602:
1578:
1572:
1571:
1569:
1568:
1549:
1536:
1530:
1529:
1503:
1494:(2): 1264–1293.
1483:
1477:
1476:
1466:
1448:
1424:
1418:
1417:
1397:
1391:
1390:
1362:
1356:
1355:
1345:
1327:
1303:
1278:
1277:
1241:
1232:
1231:
1203:
1186:
1185:
1159:
1157:astro-ph/0405198
1139:
1124:
1114:
1103:
1093:
1075:
1042:
987:
927:around 5200 AD.
898:
897:
894:
893:
890:
887:
884:
881:
878:
810:
775:
686:
684:
656:
654:
613:
611:
591:
589:
569:
567:
537:
535:
510:
508:
483:
481:
454:
452:
443:
431:
429:
422:
406:
404:
397:
384:
382:
365:
363:
345:
343:
336:
321:
319:
219:
207:
154:
152:
116:Characteristics
106:
86:
81:
51:Observation data
38:
31:
19:
3089:
3088:
3084:
3083:
3082:
3080:
3079:
3078:
3004:
3003:
3002:
2997:
2979:
2948:
2892:
2853:
2797:
2761:
2615:
2544:
2510:IRAS 23304+6147
2488:
2435:
2372:
2264:
2186:
2039:
2021:
2016:
1947:
1944:
1939:
1938:
1908:
1907:
1903:
1894:
1892:
1882:
1881:
1877:
1847:
1846:
1842:
1778:Brown, A. G. A.
1776:
1775:
1771:
1707:Brown, A. G. A.
1705:
1704:
1700:
1664:
1663:
1659:
1611:
1610:
1606:
1599:
1591:. p. 296.
1580:
1579:
1575:
1566:
1564:
1562:
1538:
1537:
1533:
1485:
1484:
1480:
1426:
1425:
1421:
1399:
1398:
1394:
1364:
1363:
1359:
1305:
1304:
1281:
1243:
1242:
1235:
1205:
1204:
1189:
1150:(3): 989–1019.
1141:
1140:
1127:
1105:(Erratum:
1104:
1046:Brown, A. G. A.
1044:
1043:
1030:
1025:
982:
966:
921:radial velocity
875:
871:
824:
805:
770:
732:
729:
714:
711:
694:
691:
682:
680:
659:
657:
652:
650:
630: sin
609:
607:
587:
585:
565:
563:
553:Surface gravity
545:
542:
533:
531:
518:
515:
506:
504:
491:
488:
479:
477:
450:
448:
444:
436:
427:
425:
412:
402:
400:
390:
380:
378:
361:
359:
341:
339:
332:Semi-major axis
329:
317:
315:
276:
259:
216:
192:−98.3 km/s
187:
182:Radial velocity
150:
148:
110:
101:
84:
79:Right ascension
77:
52:
46:
44:
43:
42:
41:
40:
39:
12:
11:
5:
3087:
3085:
3077:
3076:
3071:
3066:
3061:
3056:
3051:
3046:
3041:
3036:
3031:
3026:
3021:
3016:
3006:
3005:
2999:
2998:
2988:
2985:
2984:
2981:
2980:
2978:
2977:
2972:
2966:
2964:
2954:
2953:
2950:
2949:
2947:
2946:
2941:
2936:
2931:
2926:
2921:
2916:
2911:
2906:
2900:
2898:
2894:
2893:
2891:
2890:
2885:
2880:
2874:
2872:
2865:
2859:
2858:
2855:
2854:
2852:
2851:
2846:
2841:
2836:
2831:
2826:
2821:
2816:
2811:
2805:
2803:
2799:
2798:
2796:
2795:
2790:
2784:
2782:
2773:
2767:
2766:
2763:
2762:
2760:
2759:
2754:
2749:
2744:
2739:
2734:
2729:
2724:
2719:
2714:
2709:
2704:
2699:
2694:
2689:
2684:
2679:
2674:
2669:
2664:
2659:
2654:
2649:
2644:
2639:
2633:
2631:
2621:
2620:
2617:
2616:
2614:
2613:
2608:
2603:
2598:
2593:
2588:
2583:
2578:
2573:
2568:
2562:
2560:
2550:
2549:
2546:
2545:
2543:
2542:
2537:
2532:
2527:
2522:
2520:PSR J0205+6449
2517:
2512:
2507:
2502:
2496:
2494:
2490:
2489:
2487:
2486:
2481:
2476:
2471:
2466:
2461:
2456:
2451:
2445:
2443:
2437:
2436:
2434:
2433:
2428:
2423:
2418:
2413:
2408:
2403:
2398:
2393:
2388:
2382:
2380:
2374:
2373:
2371:
2370:
2365:
2360:
2355:
2350:
2345:
2340:
2335:
2330:
2325:
2320:
2315:
2310:
2305:
2300:
2295:
2290:
2285:
2280:
2274:
2272:
2266:
2265:
2263:
2262:
2257:
2252:
2247:
2242:
2237:
2232:
2227:
2222:
2217:
2212:
2207:
2202:
2196:
2194:
2188:
2187:
2185:
2184:
2179:
2174:
2169:
2164:
2159:
2154:
2149:
2144:
2139:
2134:
2129:
2124:
2119:
2114:
2109:
2104:
2099:
2094:
2089:
2084:
2079:
2074:
2069:
2064:
2058:
2056:
2047:
2041:
2040:
2038:
2037:
2032:
2026:
2023:
2022:
2017:
2015:
2014:
2007:
2000:
1992:
1986:
1985:
1980:
1975:10.1086/133386
1943:
1942:External links
1940:
1937:
1936:
1931:10.1086/110028
1901:
1875:
1870:10.1086/109301
1840:
1769:
1698:
1692:10.1086/323920
1657:
1644:10.1086/589554
1620:(1): 424–432.
1604:
1597:
1573:
1560:
1531:
1518:10.1086/591785
1478:
1419:
1392:
1387:10.1086/157383
1357:
1279:
1266:10.1086/191373
1233:
1228:10.1086/176148
1187:
1125:
1027:
1026:
1024:
1021:
1001:semimajor axis
965:
962:
932:spectral class
860:system in the
850:Mu Cassiopeiae
845:
844:
839:
831:
830:
826:
825:
760:
757:
756:
750:
749:
743:
735:
734:
730:
727:
723:
717:
716:
712:
709:
705:
697:
696:
692:
689:
678:
670:
669:
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664:
648:
640:
639:
636:
619:
618:
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583:
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128:
127:
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118:
117:
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107:
98:
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94:
88:
87:
85:01 08 16.30295
82:
74:
73:
68:
62:
61:
48:
47:
33:
32:
26:
25:
24:
23:
22:
17:μ Cassiopeiae
13:
10:
9:
6:
4:
3:
2:
3086:
3075:
3072:
3070:
3067:
3065:
3062:
3060:
3057:
3055:
3052:
3050:
3047:
3045:
3044:Bayer objects
3042:
3040:
3037:
3035:
3032:
3030:
3027:
3025:
3022:
3020:
3017:
3015:
3012:
3011:
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2930:
2927:
2925:
2922:
2920:
2917:
2915:
2912:
2910:
2907:
2905:
2904:Andromeda VII
2902:
2901:
2899:
2895:
2889:
2886:
2884:
2881:
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2817:
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2648:
2645:
2643:
2640:
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2634:
2632:
2630:
2629:Star clusters
2626:
2622:
2612:
2609:
2607:
2604:
2602:
2599:
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2100:
2098:
2095:
2093:
2090:
2088:
2085:
2083:
2080:
2078:
2075:
2073:
2072:γ (Navi/Tsih)
2070:
2068:
2065:
2063:
2060:
2059:
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2055:
2051:
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2046:
2042:
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2028:
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2024:
2020:
2013:
2008:
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1994:
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1990:
1984:
1981:
1976:
1971:
1967:
1963:
1959:
1955:
1951:
1946:
1945:
1941:
1932:
1928:
1924:
1920:
1916:
1912:
1905:
1902:
1891:on 2006-08-24
1890:
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1002:
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993:
991:
986:
980:
975:
974:proper motion
971:
963:
961:
959:
958:Population II
955:
952:
947:
945:
941:
940:main sequence
937:
933:
928:
926:
922:
918:
914:
910:
906:
902:
896:
870:
866:
863:
862:constellation
859:
855:
854:μ Cassiopeiae
851:
843:
840:
838:
837:
833:
832:
827:
822:
818:
814:
808:
804: 22024,
803:
799:
795:
791:
787:
783:
779:
773:
768:
764:
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698:
695:
679:
677:
676:
672:
671:
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649:
647:
646:
642:
641:
638:2.4 km/s
637:
635:
633:
629:
625:
621:
620:
617:
606:
604:
603:
599:
598:
595:
584:
582:
581:
577:
576:
573:
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560:
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328:
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324:
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288:
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258:
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247:
246:
243:
239:
237:
235:
231:
230:
227:
223:
215:
211:
204:
202:
200:
199:Proper motion
196:
195:
191:
189:
183:
179:
178:
174:
171:
167:
163:
161:
158:
157:
147:
145:
141:
140:
136:
134:
130:
129:
125:
123:
120:
119:
114:
111:(5.14/11.45)
108:
104:
100:
99:
95:
93:
90:
89:
83:
80:
76:
75:
72:
69:
67:
66:Constellation
64:
63:
59:
55:
49:
37:
30:
20:
3034:Binary stars
2849:Westerhout 5
2819:Heart Nebula
2814:Cassiopeia A
2515:LS I +61 303
2116:
1957:
1953:
1914:
1910:
1904:
1893:. Retrieved
1889:the original
1878:
1853:
1849:
1843:
1795:
1789:
1783:
1772:
1724:
1718:
1712:
1701:
1674:
1670:
1660:
1617:
1613:
1607:
1583:
1576:
1565:. Retrieved
1545:
1540:Allen, R. H.
1534:
1491:
1487:
1481:
1436:
1432:
1422:
1405:
1401:
1395:
1370:
1366:
1360:
1315:
1311:
1249:
1245:
1211:
1207:
1147:
1143:
1063:
1057:
1051:
994:
967:
948:
929:
868:
853:
849:
848:
834:
823: 10460
796: 5336,
792: 6582,
784: 1360,
780: 1030,
738:
725:0.0062
720:
700:
673:
643:
631:
627:
622:
600:
578:
556:
551:
524:
497:
470:
437:
413:
391:
370:
353:Eccentricity
351:
330:
307:
297:
269:
248:
232:
197:
180:
2975:SN 1572 (B)
2924:Dwingeloo 2
2919:Dwingeloo 1
2642:Messier 103
2611:HD 240237 b
2606:HD 240210 b
2576:HD 219134 b
2162:υ (Castula)
2077:δ (Ruchbah)
2062:α (Schedar)
1960:: 363–364.
1856:: 471–474.
1677:(6): 3466.
1373:: 211–225.
983:4,000
979:arc seconds
944:metallicity
909:light years
858:binary star
815: 107,
809:J01080+5455
800: 321,
745:3,025
740:Temperature
602:Metallicity
580:Temperature
445:(secondary)
372:Inclination
144:color index
133:color index
126:G5Vb + M4V
92:Declination
3008:Categories
2757:Trumpler 3
2637:Messier 52
2571:HD 17156 b
2558:Exoplanets
2530:4U 0142+61
2500:BD+60°2522
2097:θ (Marfak)
2092:η (Achird)
1895:2019-02-13
1805:1804.09365
1734:1804.09365
1567:2010-12-12
1446:1607.01304
1439:(6): 153.
1325:2010.06609
1073:2012.01533
1023:References
964:Companions
942:star. The
865:Cassiopeia
788: 53,
721:Luminosity
707:0.29
555:(log
526:Luminosity
426:1,997.2235
415:Periastron
170:Astrometry
164:Suspected
71:Cassiopeia
2566:HD 7924 b
2505:Gliese 49
2192:Flamsteed
2082:ε (Segin)
1627:0804.2719
1501:0807.1686
1352:222341862
1318:(2): 19.
1274:123149047
1100:227254300
1017:red dwarf
951:Milky Way
915:based on
911:from the
819: 8,
660:5.9
298:Companion
281:5.78/11.6
105: (V)
2995:Category
2944:Maffei 2
2939:Maffei 1
2863:Galaxies
2844:Sh 2-185
2752:NGC 7790
2747:NGC 7789
2742:NGC 1027
2270:Variable
2087:ζ (Fulu)
2067:β (Caph)
1542:(1963).
1526:27151456
1473:15983830
1182:11027621
1003:of 7.61
936:subdwarf
917:parallax
761:Marfak,
731:☉
713:☉
693:☉
544:☉
517:☉
490:☉
273: (M
250:Distance
234:Parallax
2970:SN 1181
2829:IC 1805
2771:Nebulae
2737:NGC 663
2732:NGC 659
2727:NGC 654
2722:NGC 637
2717:NGC 559
2712:NGC 457
2707:NGC 436
2702:NGC 433
2697:NGC 381
2692:NGC 366
2687:NGC 358
2682:NGC 225
2677:NGC 189
2672:NGC 146
2667:NGC 136
2662:NGC 133
2657:NGC 129
2652:NGC 110
2647:NGC 103
2525:Tycho G
2298:YZ (21)
1962:Bibcode
1919:Bibcode
1917:: 185.
1858:Bibcode
1810:Bibcode
1739:Bibcode
1679:Bibcode
1652:8886682
1632:Bibcode
1506:Bibcode
1451:Bibcode
1410:Bibcode
1375:Bibcode
1330:Bibcode
1254:Bibcode
1252:: 245.
1216:Bibcode
1214:: 380.
1162:Bibcode
1115:.
1078:Bibcode
925:Perseus
856:, is a
774:+54°223
460:Details
401:223.868
379:110.671
302:μ Cas B
58:Equinox
2834:KjPn 8
2824:IC 289
2484:240430
2479:240429
2474:240237
2469:240210
2245:48 (A)
1836:VizieR
1798:. A1.
1765:VizieR
1727:. A1.
1650:
1595:
1558:
1524:
1471:
1354:. 112.
1350:
1272:
1180:
1121:VizieR
1098:
1066:: A1.
954:galaxy
869:Marfak
836:SIMBAD
702:Radius
687:
685:0.0035
681:0.1728
614:
592:
570:
538:
511:
499:Radius
484:
482:0.0122
478:0.7440
455:°
449:330.37
430:0.0067
407:°
385:°
364:0.0011
360:0.5885
344:0.0013
340:0.9985
316:21.568
309:Period
137:+0.10
60:J2000
2934:IC 10
2914:3C 35
2909:3C 20
2897:Other
2809:3C 58
2802:Other
2591:e (h)
2493:Other
2459:15558
2368:V1405
2363:V1022
2054:Bayer
2045:Stars
1830:
1800:arXiv
1759:
1729:arXiv
1648:S2CID
1622:arXiv
1522:S2CID
1496:arXiv
1469:S2CID
1441:arXiv
1348:S2CID
1320:arXiv
1270:S2CID
1178:S2CID
1152:arXiv
1096:S2CID
1068:arXiv
899:with
763:μ Cas
608:−0.81
586:5,306
568:0.011
564:4.515
536:0.005
532:0.445
509:0.008
505:0.789
418:epoch
405:0.064
383:0.064
320:0.015
291:Orbit
218:Dec.:
153:0.006
149:0.695
109:5.159
54:Epoch
2929:MB 3
2793:7635
2540:WR 3
2535:WR 2
2454:7977
2449:7924
2431:8881
2426:8853
2421:8832
2358:V987
2353:V773
2348:V863
2343:V762
2338:V705
2333:V669
2328:V547
2323:V509
2318:V373
1784:Gaia
1713:Gaia
1593:ISBN
1556:ISBN
1052:Gaia
842:data
807:CCDM
675:Mass
651:12.7
612:0.03
472:Mass
453:0.18
142:B−V
131:U−B
2888:278
2883:185
2878:147
2871:NGC
2788:281
2780:NGC
2416:932
2411:743
2406:297
2401:273
2396:244
2391:196
2386:144
1970:doi
1958:106
1927:doi
1866:doi
1834:at
1820:doi
1796:616
1763:at
1749:doi
1725:616
1687:doi
1675:122
1640:doi
1618:683
1552:148
1514:doi
1492:687
1459:doi
1437:152
1383:doi
1371:233
1338:doi
1316:904
1262:doi
1224:doi
1212:450
1170:doi
1148:418
1119:at
1107:doi
1086:doi
1064:649
1009:AUs
1005:AUs
913:Sun
883:ɑːr
821:LTT
817:LHS
813:LFT
802:SAO
794:HIP
778:FK5
662:Gyr
658:3.1
655:2.7
645:Age
616:dex
572:cgs
441:(ω)
420:(T)
395:(Ω)
374:(i)
355:(e)
334:(a)
311:(P)
242:mas
236:(π)
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