This is the list of notable stars in the constellation Andromeda, sorted by decreasing brightness.
Name B F Var HD HIP RA Dec vis.mag. abs.mag. Dist. (ly) Sp. class Notes Alpheratz α, (δ) 21 358 677 2.07 −0.30 97 B9p Alpheratz, Sirrah; α2 CVn variable, ; spectroscopic binary, also δ Peg Mirach β 43 6860 5447 2.07 −1.86 199 M0IIIvar Mirach; variable, has a planet or brown dwarf (b) γ1 And γ1 57 12533 9640 2.10 −3.08 355 K3IIb Almach; quadruple star system δ And δ 31 3627 3092 3.27 0.81 101 K3III... spectroscopic binary; suspected variable 51 And (υ) 51 9927 7607 3.59 −0.04 174 K3III Nembus; multiple star ο And ο 1 217675 113726 3.62 −3.01 692 B6pv SB AlfarasalkamilIAU-Catalog of Star Names quadruple star system; γ Cas variable, λ And λ 16 222107 116584 3.81 1.75 84 G8III-IV Udkadua, RS CVn variable, μ And μ 37 5448 4436 3.86 0.75 136 A5V multiple star ζ And ζ 34 4502 3693 4.08 0.35 181 K1II Shimu, β Lyr/RS CVn variable, υ And υ 50 9826 7513 4.10 3.45 44 F8V Titawin,Final Results of NameExoWorlds Public Vote Released has four planets (b, c, d & e) κ And κ 19 222439 116805 4.15 0.57 170 B9IVn Kaffalmusalsala, triple star, has a planet (b) φ And φ 42 6811 5434 4.26 −2.51 736 B7III Junnanmen, emission-line star ι And ι 17 222173 116631 4.29 −1.65 502 B8V Rasalnaqa, Keff al Salsalat, Manus CatenataE.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket π And π 29 3369 2912 4.34 −2.18 656 B5V spectroscopic binary; suspected variable ε And ε 30 3546 3031 4.34 0.77 169 G5III... η And η 38 5516 4463 4.40 0.04 243 G8III-IV Kui, spectroscopic binary σ And σ 25 1404 1473 4.51 1.33 141 A2V suspected variable ν And ν 35 4727 3881 4.53 −2.06 679 B5V SB spectroscopic binary 7 And 7 219080 114570 4.53 2.58 80 F0V Honores θ And θ 24 1280 1366 4.61 0.16 253 A2V suspected variable 3 And 3 218031 113919 4.64 0.94 179 K0III 65 And 65 14872 11313 4.73 −0.39 345 K4III triple star 58 And 58 13041 9977 4.78 0.86 198 A5IV-V 8 And 8 219734 115022 4.82 −1.69 655 M2III suspected variable ω And ω 48 8799 6813 4.83 2.57 92 F5IV γ2 And γ2 57 12534 4.84 -0.3 350 B8V component of the γ And system; triple star system 60 And b 60 13520 10340 4.84 −1.32 556 K4III suspected variable ξ And ξ 46 8207 6411 4.87 0.98 195 K0III-IV Adhil τ And τ 53 10205 7818 4.96 −1.64 681 B8III suspected variable 41 H. And υ 10307 7918 4.96 4.45 41 G2V spectroscopic binary ψ And ψ 20 223047 117221 4.97 −3.05 1309 G5Ib multiple star 22 And 22 571 841 5.01 −2.44 1006 F2II χ And χ 52 10072 7719 5.01 0.66 242 G8III... 41 And (d) 41 6658 5317 5.04 1.14 196 A3m 2 And 2 217782 113788 5.09 −0.06 349 A3Vn multiple star V428 And V428 3346 2900 5.14 −1.38 656 K5III semiregular variable, ; has a possible planetary system ρ And ρ 27 1671 1686 5.16 1.71 160 F5III HD 2421 2421 2225 5.18 0.63 265 A2Vs spectroscopic binary 64 And 64 14770 11220 5.19 −0.11 375 G8III GN And 28 GN 2628 2355 5.20 1.43 185 A7III low-amplitude δ Sct variable, 14 And 14 221345 116076 5.22 0.80 249 K0III Veritate, suspected variable; has a planet (b) 49 And A 49 9057 6999 5.27 0.53 290 K0III 32 And 32 3817 3231 5.30 0.18 344 G8III 4 And 4 218452 114200 5.30 0.20 342 K5III double star 6 Per (h) (6)Persei, on the constellation boundary between Andromeda with Perseus 13530 10366 5.31 1.38 199 G8III:var spectroscopic binary; suspected variable 62 And c 62 14212 10819 5.31 0.84 255 A1V 18 And 18 222304 116709 5.35 −0.04 390 B9V 55 And 55 11428 8814 5.42 −0.67 540 K1III double star 11 And 11 219945 115152 5.44 0.43 328 K0III 3421 2942 5.45 −2.03 1022 G5III 36 And 36 5286 4288 5.46 2.51 127 K1IV suspected variable V340 And 15 V340 221756 116354 5.55 1.28 233 A1III low-amplitude δ Sct variable, PZ And 63 PZ 14392 10944 5.57 0.38 356 B9p Si α2 CVn variable, 47 And 47 8374 6514 5.60 1.54 211 A1m 10204 7825 5.63 1.05 268 A9IV: 44 And 44 6920 5493 5.67 2.06 172 F8V 5 And 5 218470 114210 5.68 3.02 111 F5V HD 5788 5788 4675 5.69 0.14 420 A2Vn binary star with HD 5789 56 And 56 11749 9021 5.69 0.73 320 G8III... multiple star 23 And 23 905 1086 5.71 2.99 114 F0IV HD 16028 16028 12072 5.72 −0.86 676 K4III triple star V388 And 13 V388 220885 115755 5.75 0.97 294 B9III α2 CVn variable, 12 And 12 220117 115280 5.77 2.63 138 F5V triple star 1632 1657 5.79 −0.69 646 K5III 45 And 45 7019 5550 5.80 −1.44 916 B7III-IV double star HD 14622 14622 11090 5.81 2.44 154 F0III-IV has two optical companions 10 And 10 219981 115191 5.81 −0.30 542 M0III HD 222109 222109 116582 5.81 −1.20 823 B8V double star HD 224635 224635 118281 5.81 3.50 95 F8 multiple star OU And OU 223460 117503 5.86 0.21 440 G1IIIe FK Com variable, 1439 1493 5.88 −0.23 543 A0IV HD 2767 2767 2475 5.88 0.10 467 K1III... binary star HD 1606 1606 1630 5.89 −0.37 582 B7V suspected variable 11727 9001 5.89 −1.52 991 K5III optical component of 56 And KK And KK 9531 7321 5.90 0.50 392 B8Vp(Si) α2 CVn variable, 16176 12181 5.91 2.24 177 F5V 6 And 6 218804 114430 5.91 3.65 112 F5V Astrometric binary 10975 8423 5.94 1.06 308 K0III 39 And 39 6116 4903 5.95 0.84 344 A5m double star 8671 6711 5.98 2.90 135 F7V AN And 9 AN 219815 115065 5.98 0.17 472 A7m β Lyr variable, HD 5608 5608 4552 5.99 2.17 190 K0 has a planet (b) 224165 117956 6.01 −2.46 1614 G8Ib 224342 118071 6.01 −2.22 1442 F8III 4335 3604 6.03 0.32 452 B9.5IIIMNp. 13594 10403 6.05 2.96 135 F5V HD 3883 3883 3269 6.06 0.30 462 A7m suspected variable V439 And V439 166 544 6.07 5.39 45 K0V BY Draconis variable, 5118 4185 6.07 0.77 374 K3III: 221293 116030 6.07 −0.33 621 G9III HD 223229 223229 117340 6.08 −1.96 1320 B3IV suspected variable 225239 394 6.09 3.26 120 G2V 59 And A 59 13294 10176 6.09 1.56 263 B9V binary star 26 And 26 1438 1501 6.10 −0.53 692 B8V double star 5526 4501 6.10 0.45 439 K2III HD 225218 225218 365 6.11 −2.45 1680 B9III double star 7647 5993 6.11 −0.18 590 K5 HD 1185 1185 1302 6.12 1.28 303 A2V double star 218416 114162 6.12 0.55 423 K0III GO And GO 4778 3919 6.13 1.34 296 A0p... α2 CVn variable, 7158 5650 6.13 −0.52 698 M1III 66 And 66 15138 11465 6.16 2.54 173 F4V spectroscopic binary 14372 10924 6.17 −0.87 836 B5V 743 967 6.18 0.05 550 K4III 3411 2926 6.18 1.13 334 K2III HD 221776 221776 116365 6.18 −0.41 678 K5 double star 16327 12287 6.19 1.60 270 F6III triple star HD 221246 221246 115996 6.19 −0.91 856 K5III member of the NGC 7686 star cluster OP And OP 9746 7493 6.20 0.65 420 K1III: BY Dra variable, 400 699 6.21 3.61 108 F8IV 14213 10814 6.21 0.50 452 A4V 952 1123 6.22 1.45 293 A1V HD 895 895 1076 6.24 0.78 403 G0III triple star 222451 116824 6.24 3.01 144 F1V 224906 137 6.25 −1.80 1331 B9IIIp Mn 11613 8922 6.25 1.13 345 K2 HD 220105 220105 115261 6.25 1.73 261 A5Vn double star 221661 116292 6.25 0.12 548 G8II HD 2942 2942 2583 6.26 0.47 469 G8II triple star 8774 6776 6.27 3.12 139 F7IVsvar 2507 2270 6.28 0.51 464 G5III 8375 6512 6.28 2.43 192 G8IV 11624 8930 6.28 0.25 525 K0 7758 6087 6.29 −2.07 1531 K0 16350 12305 6.29 −0.47 734 B9.5V 219962 115171 6.29 0.47 475 K1III 217314 113501 6.31 −0.26 672 K2 10597 8127 6.32 0.23 540 K5III 219290 114714 6.32 0.82 411 A0V 10486 8044 6.33 2.61 181 K2IV 10874 8370 6.33 2.50 190 F6V 1075 1208 6.34 −1.70 1320 K5 HD 8673 8673 6702 6.34 3.43 125 F7V has a planet (b) 1083 1215 6.35 0.84 412 A1Vn double star 1527 1575 6.35 0.25 541 K1III 221970 116505 6.35 1.92 251 F6V CG And CG 224801 63 6.36 −0.23 678 B9p SiEu α2 CVn variable, HD 16004 16004 12057 6.36 0.11 580 B9MNp... triple star 13818 10562 6.37 0.61 462 G9III-IV LN And LN 217811 113802 6.37 −1.42 1177 B2V double star; not variable despite designation V385 And V385 220524 115530 6.37 −1.55 1249 M0 irregular variable, GY And GY 9996 7651 6.38 0.66 455 B9Vp (Cr-Eu) Promethium lines; α2 CVn variable, 13013 9983 6.38 0.78 430 G8III 218365 114152 6.38 −0.08 638 K0 9712 7444 6.39 1.01 388 K1III V529 And V529 8801 6794 6.42 2.69 182 Am... δ Scuti variable, 217731 113750 6.43 1.22 359 K0 HD 222641 222641 116941 6.43 −0.48 786 K5III suspected variable HD 7853 7853 6140 6.44 0.71 456 A5m double star 14221 10830 6.44 2.39 210 F4V 219668 114981 6.44 2.10 241 K0IV HD 6114 6114 4911 6.46 1.39 337 A9V double star 11884 9163 6.48 −1.24 1140 K0 ET And ET 219749 115036 6.48 0.36 545 B9Vp(Si) α2 CVn variable, HD 222399 222399 116781 6.49 1.74 291 F2IV double star PY And PY 3322 2865 6.50 -0.16 701 B8IIImnp... α2 CVn variable, 800 1009 6.50 0.50 517 K0 59 And B 59 13295 10180 6.82 −1.76 1698 A1Vn component of the 59 And system HD 222155 222155 116616 7.1 3.65 160 G2V has a planet (b) HD 16175 16175 12191 7.28 3.40 195 G0 Buna; has a planet (b) R And R 1967 1901 7.39 -5.19 790 S6.5IIIeZr6Ti2 Mira variable, HD 1605 1605 1640 7.52 2.88 276 K1IV has two planets (b & c) HD 13931 13931 10626 7.52 4.3 144 G0 has a planet (b) HD 5583 5583 7.6 0.88 721 K0 has a planet (b) RW And RW 4489 7.9 -0.52 1375 M5e-M10e(S6,2e) Mira variable, Groombridge 34 1326 1475 8.01 10.25 11.62 M6Ve + M1Ve 16th closest star system, binary; both components GQ and GX And flare stars HD 15082 15082 11397 8.3 3.0 377 A5 has a transiting planet WASP-33b RU And RU 9.9 M5e-M6e a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 14.5 at minimum brightness to a magnitude of 9.9 at maximum brightness, with a period of approximately 238.3 days.RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30., database entry, SIMBAD. Accessed on line 2009-06-30. Y And 10112 10.39 8,000 M3-4.5e Mira Cet variable Z And Z 221650 116287 10.53 2.38 1393 M2III + B1eq prototype of Z And variables, HAT-P-6 10.54 4.03 650 F Sterrennacht; has a transiting planet (b) HAT-P-16 10.8 3.9 766 F8 has a transiting planet (b) HAT-P-32 11.29 3.76 1044 F/G has a transiting planet (b) WASP-1 11.79 3.89 1239 F7V has a transiting planet (b) Ross 248 12.29 14.79 10.32 M6e HH And; 8th closest star system, flare star HAT-P-19 12.9 6.24 701 K has a transiting planet (b) HAT-P-28 13.03 5.05 1288 G3 has a transiting planet (b) HAT-P-53 13.73 4.45 2345 has a transiting planet (b) S And S 2600000 Ia SN 1885A; BD+40°147a; type Ia supernova in the Andromeda Galaxy,
Notes
See also List of stars by constellation
References