# List of stars in Andromeda

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 | 00$^h$ 08$^m$ 23.17$^s$ | +29° 05′ 27.0″ | 2.07 | −0.30 | 97 | B9p | Alpheratz, Sirrah; α$^2$ CVn variable, ΔV = 0.04$^m$, P = 0.966222 d; spectroscopic binary, also δ Peg |
| Mirach | β | 43 | | 6860 | 5447 | 01$^h$ 09$^m$ 43.80$^s$ | +35° 37′ 15.0″ | 2.07 | −1.86 | 199 | M0IIIvar | Mirach; variable, has a planet or brown dwarf (b) |
| γ$^1$ And | γ$^1$ | 57 | | 12533 | 9640 | 02$^h$ 03$^m$ 53.92$^s$ | +42° 19′ 47.5″ | 2.10 | −3.08 | 355 | K3IIb | Almach; quadruple star system |
| δ And | δ | 31 | | 3627 | 3092 | 00$^h$ 39$^m$ 19.60$^s$ | +30° 51′ 40.4″ | 3.27 | 0.81 | 101 | K3III... | spectroscopic binary; suspected variable |
| Andromeda Galaxy | (n) | 33 | | | | 00$^h$ 42$^m$ 44.31$^s$ | +41° 16′ 09.4″ | 3.44 (nebulous) | | 2540000 | | BD+40°148; naked eye spiral galaxy in the Local group |
| 51 And | (υ) | 51 | | 9927 | 7607 | 01$^h$ 37$^m$ 59.50$^s$ | +48° 37′ 42.6″ | 3.59 | −0.04 | 174 | K3III | Nembus; multiple star |
| ο And | ο | 1 | | 217675 | 113726 | 23$^h$ 01$^m$ 55.25$^s$ | +42° 19′ 33.5″ | 3.62 | −3.01 | 692 | B6pv SB | quadruple star system; γ Cas variable, V$_{max}$ = 3.55$^m$, V$_{min}$ = 3.78$^m$ |
| λ And | λ | 16 | | 222107 | 116584 | 23$^h$ 37$^m$ 33.71$^s$ | +46° 27′ 33.0″ | 3.81 | 1.75 | 84 | G8III-IV | RS CVn variable, V$_{max}$ = 3.65$^m$, V$_{min}$ = 4.05$^m$, P = 53.95 d |
| μ And | μ | 37 | | 5448 | 4436 | 00$^h$ 56$^m$ 45.10$^s$ | +38° 29′ 57.3″ | 3.86 | 0.75 | 136 | A5V | multiple star |
| ζ And | ζ | 34 | | 4502 | 3693 | 00$^h$ 47$^m$ 20.39$^s$ | +24° 16′ 02.6″ | 4.08 | 0.35 | 181 | K1II | β Lyr/RS CVn variable, V$_{max}$ = 3.92$^m$, V$_{min}$ = 4.14$^m$, P = 17.7696 d |
| υ And | | 50 | | 9826 | 7513 | 01$^h$ 36$^m$ 47.98$^s$ | +41° 24′ 23.0″ | 4.10 | 3.45 | 44 | F8V | Titawin, has four planets (b, c, d & e) |
| κ And | κ | 19 | | 222439 | 116805 | 23$^h$ 40$^m$ 24.44$^s$ | +44° 20′ 02.3″ | 4.15 | 0.57 | 170 | B9IVn | triple star, has a planet (b) |
| φ And | φ | 42 | | 6811 | 5434 | 01$^h$ 09$^m$ 30.12$^s$ | +47° 14′ 30.6″ | 4.26 | −2.51 | 736 | B7III | emission-line star |
| ι And | ι | 17 | | 222173 | 116631 | 23$^h$ 38$^m$ 08.18$^s$ | +43° 16′ 05.1″ | 4.29 | −1.65 | 502 | B8V | Keff al Salsalat, Manus Catenata |
| π And | π | 29 | | 3369 | 2912 | 00$^h$ 36$^m$ 52.84$^s$ | +33° 43′ 09.7″ | 4.34 | −2.18 | 656 | B5V | spectroscopic binary; suspected variable |
| ε And | ε | 30 | | 3546 | 3031 | 00$^h$ 38$^m$ 33.50$^s$ | +29° 18′ 44.5″ | 4.34 | 0.77 | 169 | G5III... | |
| η And | η | 38 | | 5516 | 4463 | 00$^h$ 57$^m$ 12.43$^s$ | +23° 25′ 03.9″ | 4.40 | 0.04 | 243 | G8III-IV | spectroscopic binary |
| σ And | σ | 25 | | 1404 | 1473 | 00$^h$ 18$^m$ 19.71$^s$ | +36° 47′ 07.2″ | 4.51 | 1.33 | 141 | A2V | suspected variable |
| ν And | ν | 35 | | 4727 | 3881 | 00$^h$ 49$^m$ 48.83$^s$ | +41° 04′ 44.2″ | 4.53 | −2.06 | 679 | B5V SB | spectroscopic binary |
| 7 And | | 7 | | 219080 | 114570 | 23$^h$ 12$^m$ 32.92$^s$ | +49° 24′ 21.5″ | 4.53 | 2.58 | 80 | F0V | |
| θ And | θ | 24 | | 1280 | 1366 | 00$^h$ 17$^m$ 05.54$^s$ | +38° 40′ 54.0″ | 4.61 | 0.16 | 253 | A2V | suspected variable |
| 3 And | | 3 | | 218031 | 113919 | 23$^h$ 04$^m$ 10.83$^s$ | +50° 03′ 06.1″ | 4.64 | 0.94 | 179 | K0III | |
| 65 And | | 65 | | 14872 | 11313 | 02$^h$ 25$^m$ 37.40$^s$ | +50° 16′ 43.2″ | 4.73 | −0.39 | 345 | K4III | triple star |
| 58 And | | 58 | | 13041 | 9977 | 02$^h$ 08$^m$ 29.15$^s$ | +37° 51′ 33.1″ | 4.78 | 0.86 | 198 | A5IV-V | |
| 8 And | | 8 | | 219734 | 115022 | 23$^h$ 17$^m$ 44.62$^s$ | +49° 00′ 55.0″ | 4.82 | −1.69 | 655 | M2III | suspected variable |
| ω And | ω | 48 | | 8799 | 6813 | 01$^h$ 27$^m$ 39.09$^s$ | +45° 24′ 25.0″ | 4.83 | 2.57 | 92 | F5IV | |
| γ$^2$ And | γ$^2$ | 57 | | 12534 | | 02$^h$ 03$^m$ 54.70$^s$ | +42° 19′ 51.0″ | 4.84 | -0.3 | 350 | B8V | component of the γ And system; triple star system |
| 60 And | b | 60 | | 13520 | 10340 | 02$^h$ 13$^m$ 13.34$^s$ | +44° 13′ 54.1″ | 4.84 | −1.32 | 556 | K4III | suspected variable |
| ξ And | ξ | 46 | | 8207 | 6411 | 01$^h$ 22$^m$ 20.39$^s$ | +45° 31′ 43.5″ | 4.87 | 0.98 | 195 | K0III-IV | Adhil |
| τ And | τ | 53 | | 10205 | 7818 | 01$^h$ 40$^m$ 34.80$^s$ | +40° 34′ 37.6″ | 4.96 | −1.64 | 681 | B8III | suspected variable |
| 41 H. And | υ | | | 10307 | 7918 | 01$^h$ 41$^m$ 46.52$^s$ | +42° 36′ 49.7″ | 4.96 | 4.45 | 41 | G2V | spectroscopic binary |
| ψ And | ψ | 20 | | 223047 | 117221 | 23$^h$ 46$^m$ 02.04$^s$ | +46° 25′ 13.0″ | 4.97 | −3.05 | 1309 | G5Ib | multiple star |
| 22 And | | 22 | | 571 | 841 | 00$^h$ 10$^m$ 19.24$^s$ | +46° 04′ 20.2″ | 5.01 | −2.44 | 1006 | F2II | |
| χ And | χ | 52 | | 10072 | 7719 | 01$^h$ 39$^m$ 21.02$^s$ | +44° 23′ 10.1″ | 5.01 | 0.66 | 242 | G8III... | |
| 41 And | (d) | 41 | | 6658 | 5317 | 01$^h$ 08$^m$ 00.72$^s$ | +43° 56′ 32.1″ | 5.04 | 1.14 | 196 | A3m | |
| 2 And | | 2 | | 217782 | 113788 | 23$^h$ 02$^m$ 36.34$^s$ | +42° 45′ 28.1″ | 5.09 | −0.06 | 349 | A3Vn | multiple star |
| V428 And | | | V428 | 3346 | 2900 | 00$^h$ 36$^m$ 46.47$^s$ | +44° 29′ 18.6″ | 5.14 | −1.38 | 656 | K5III | semiregular variable, ΔV = 0.06$^m$, P = 11.5 d; has a possible planetary system |
| ρ And | ρ | 27 | | 1671 | 1686 | 00$^h$ 21$^m$ 07.23$^s$ | +37° 58′ 07.3″ | 5.16 | 1.71 | 160 | F5III | |
| HD 2421 | | | | 2421 | 2225 | 00$^h$ 28$^m$ 13.59$^s$ | +44° 23′ 40.2″ | 5.18 | 0.63 | 265 | A2Vs | spectroscopic binary |
| 64 And | | 64 | | 14770 | 11220 | 02$^h$ 24$^m$ 24.89$^s$ | +50° 00′ 23.9″ | 5.19 | −0.11 | 375 | G8III | |
| GN And | | 28 | GN | 2628 | 2355 | 00$^h$ 30$^m$ 07.34$^s$ | +29° 45′ 06.1″ | 5.20 | 1.43 | 185 | A7III | low-amplitude δ Sct variable, ΔV = 0.05$^m$, P = 0.0693041 d |
| 14 And | | 14 | | 221345 | 116076 | 23$^h$ 31$^m$ 17.20$^s$ | +39° 14′ 11.0″ | 5.22 | 0.80 | 249 | K0III | Veritate, suspected variable; has a planet (b) |
| 49 And | A | 49 | | 9057 | 6999 | 01$^h$ 30$^m$ 06.10$^s$ | +47° 00′ 26.6″ | 5.27 | 0.53 | 290 | K0III | |
| 32 And | | 32 | | 3817 | 3231 | 00$^h$ 41$^m$ 07.20$^s$ | +39° 27′ 31.2″ | 5.30 | 0.18 | 344 | G8III | |
| 4 And | | 4 | | 218452 | 114200 | 23$^h$ 07$^m$ 39.28$^s$ | +46° 23′ 14.3″ | 5.30 | 0.20 | 342 | K5III | double star |
| 6 Per | | (6) | | 13530 | 10366 | 02$^h$ 13$^m$ 36.02$^s$ | +51° 03′ 58.4″ | 5.31 | 1.38 | 199 | G8III:var | spectroscopic binary; suspected variable |
| 62 And | c | 62 | | 14212 | 10819 | 02$^h$ 19$^m$ 16.85$^s$ | +47° 22′ 48.0″ | 5.31 | 0.84 | 255 | A1V | |
| 18 And | | 18 | | 222304 | 116709 | 23$^h$ 39$^m$ 08.35$^s$ | +50° 28′ 18.3″ | 5.35 | −0.04 | 390 | B9V | |
| 55 And | | 55 | | 11428 | 8814 | 01$^h$ 53$^m$ 17.35$^s$ | +40° 43′ 47.3″ | 5.42 | −0.67 | 540 | K1III | double star |
| 11 And | | 11 | | 219945 | 115152 | 23$^h$ 19$^m$ 29.79$^s$ | +48° 37′ 30.7″ | 5.44 | 0.43 | 328 | K0III | |
| | | | | 3421 | 2942 | 00$^h$ 37$^m$ 21.23$^s$ | +35° 23′ 58.2″ | 5.45 | −2.03 | 1022 | G5III | |
| 36 And | | 36 | | 5286 | 4288 | 00$^h$ 54$^m$ 58.02$^s$ | +23° 37′ 42.4″ | 5.46 | 2.51 | 127 | K1IV | suspected variable |
| V340 And | | 15 | V340 | 221756 | 116354 | 23$^h$ 34$^m$ 37.55$^s$ | +40° 14′ 11.6″ | 5.55 | 1.28 | 233 | A1III | low-amplitude δ Sct variable, ΔV = 0.007$^m$ |
| PZ And | | 63 | PZ | 14392 | 10944 | 02$^h$ 20$^m$ 58.17$^s$ | +50° 09′ 05.5″ | 5.57 | 0.38 | 356 | B9p Si | α$^2$ CVn variable, ΔV = 0.05$^m$, P = 4.189 d |
| 47 And | | 47 | | 8374 | 6514 | 01$^h$ 23$^m$ 40.56$^s$ | +37° 42′ 54.0″ | 5.60 | 1.54 | 211 | A1m | |
| | | | | 10204 | 7825 | 01$^h$ 40$^m$ 39.56$^s$ | +43° 17′ 51.9″ | 5.63 | 1.05 | 268 | A9IV: | |
| 44 And | | 44 | | 6920 | 5493 | 01$^h$ 10$^m$ 18.85$^s$ | +42° 04′ 53.7″ | 5.67 | 2.06 | 172 | F8V | |
| 5 And | | 5 | | 218470 | 114210 | 23$^h$ 07$^m$ 45.25$^s$ | +49° 17′ 43.6″ | 5.68 | 3.02 | 111 | F5V | |
| HD 5788 | | | | 5788 | 4675 | 01$^h$ 00$^m$ 03.55$^s$ | +44° 42′ 47.9″ | 5.69 | 0.14 | 420 | A2Vn | binary star with HD 5789 |
| 56 And | | 56 | | 11749 | 9021 | 01$^h$ 56$^m$ 09.23$^s$ | +37° 15′ 06.5″ | 5.69 | 0.73 | 320 | G8III... | multiple star |
| 23 And | | 23 | | 905 | 1086 | 00$^h$ 13$^m$ 30.94$^s$ | +41° 02′ 08.6″ | 5.71 | 2.99 | 114 | F0IV | |
| HD 16028 | | | | 16028 | 12072 | 02$^h$ 35$^m$ 38.74$^s$ | +37° 18′ 44.2″ | 5.72 | −0.86 | 676 | K4III | triple star |
| V388 And | | 13 | V388 | 220885 | 115755 | 23$^h$ 27$^m$ 07.33$^s$ | +42° 54′ 43.1″ | 5.75 | 0.97 | 294 | B9III | α$^2$ CVn variable, V$_{max}$ = 5.73$^m$, V$_{min}$ = 5.77$^m$, P = 1.47931 d |
| 12 And | | 12 | | 220117 | 115280 | 23$^h$ 20$^m$ 53.17$^s$ | +38° 10′ 56.9″ | 5.77 | 2.63 | 138 | F5V | triple star |
| | | | | 1632 | 1657 | 00$^h$ 20$^m$ 45.54$^s$ | +32° 54′ 40.4″ | 5.79 | −0.69 | 646 | K5III | |
| 45 And | | 45 | | 7019 | 5550 | 01$^h$ 11$^m$ 10.29$^s$ | +37° 43′ 26.9″ | 5.80 | −1.44 | 916 | B7III-IV | double star |
| HD 14622 | | | | 14622 | 11090 | 02$^h$ 22$^m$ 50.36$^s$ | +41° 23′ 47.5″ | 5.81 | 2.44 | 154 | F0III-IV | has two optical companions |
| 10 And | | 10 | | 219981 | 115191 | 23$^h$ 19$^m$ 52.38$^s$ | +42° 04′ 40.9″ | 5.81 | −0.30 | 542 | M0III | |
| HD 222109 | | | | 222109 | 116582 | 23$^h$ 37$^m$ 32.03$^s$ | +44° 25′ 44.5″ | 5.81 | −1.20 | 823 | B8V | double star |
| HD 224635 | | | | 224635 | 118281 | 23$^h$ 59$^m$ 29.33$^s$ | +33° 43′ 26.9″ | 5.81 | 3.50 | 95 | F8 | multiple star |
| OU And | | | OU | 223460 | 117503 | 23$^h$ 49$^m$ 40.96$^s$ | +36° 25′ 31.4″ | 5.86 | 0.21 | 440 | G1IIIe | FK Com variable, ΔV = 0.07$^m$, P = 24.2 d |
| | | | | 1439 | 1493 | 00$^h$ 18$^m$ 38.22$^s$ | +31° 31′ 02.0″ | 5.88 | −0.23 | 543 | A0IV | |
| HD 2767 | | | | 2767 | 2475 | 00$^h$ 31$^m$ 25.61$^s$ | +33° 34′ 54.1″ | 5.88 | 0.10 | 467 | K1III... | binary star |
| HD 1606 | | | | 1606 | 1630 | 00$^h$ 20$^m$ 24.39$^s$ | +30° 56′ 08.2″ | 5.89 | −0.37 | 582 | B7V | suspected variable |
| | | | | 11727 | 9001 | 01$^h$ 55$^m$ 54.47$^s$ | +37° 16′ 40.1″ | 5.89 | −1.52 | 991 | K5III | optical component of 56 And |
| KK And | | | KK | 9531 | 7321 | 01$^h$ 34$^m$ 16.60$^s$ | +37° 14′ 13.9″ | 5.90 | 0.50 | 392 | B8Vp(Si) | α$^2$ CVn variable, ΔV = 0.012$^m$, P = 0.6684 d |
| | | | | 16176 | 12181 | 02$^h$ 36$^m$ 57.08$^s$ | +38° 44′ 02.3″ | 5.91 | 2.24 | 177 | F5V | |
| 6 And | | 6 | | 218804 | 114430 | 23$^h$ 10$^m$ 27.36$^s$ | +43° 32′ 41.1″ | 5.91 | 3.65 | 112 | F5V | Astrometric binary |
| | | | | 10975 | 8423 | 01$^h$ 48$^m$ 38.84$^s$ | +37° 57′ 10.6″ | 5.94 | 1.06 | 308 | K0III | |
| 39 And | | 39 | | 6116 | 4903 | 01$^h$ 02$^m$ 54.28$^s$ | +41° 20′ 42.7″ | 5.95 | 0.84 | 344 | A5m | double star |
| | | | | 8671 | 6711 | 01$^h$ 26$^m$ 18.60$^s$ | +43° 27′ 28.4″ | 5.98 | 2.90 | 135 | F7V | |
| AN And | | 9 | AN | 219815 | 115065 | 23$^h$ 18$^m$ 23.33$^s$ | +41° 46′ 25.3″ | 5.98 | 0.17 | 472 | A7m | β Lyr variable, V$_{max}$ = 5.96$^m$, V$_{min}$ = 6.11$^m$, P = 3.21952 d |
| HD 5608 | | | | 5608 | 4552 | 00$^h$ 58$^m$ 14.19$^s$ | +33° 57′ 03.8″ | 5.99 | 2.17 | 190 | K0 | has a transiting planet (b) |
| | | | | 224165 | 117956 | 23$^h$ 55$^m$ 33.48$^s$ | +47° 21′ 21.0″ | 6.01 | −2.46 | 1614 | G8Ib | |
| | | | | 224342 | 118071 | 23$^h$ 57$^m$ 03.63$^s$ | +42° 39′ 29.7″ | 6.01 | −2.22 | 1442 | F8III | |
| | | | | 4335 | 3604 | 00$^h$ 46$^m$ 10.80$^s$ | +44° 51′ 41.4″ | 6.03 | 0.32 | 452 | B9.5IIIMNp. | |
| | | | | 13594 | 10403 | 02$^h$ 14$^m$ 02.53$^s$ | +47° 29′ 03.8″ | 6.05 | 2.96 | 135 | F5V | |
| HD 3883 | | | | 3883 | 3269 | 00$^h$ 41$^m$ 35.98$^s$ | +24° 37′ 44.6″ | 6.06 | 0.30 | 462 | A7m | suspected variable |
| V439 And | | | V439 | 166 | 544 | 00$^h$ 06$^m$ 36.53$^s$ | +29° 01′ 19.0″ | 6.07 | 5.39 | 45 | K0V | BY Draconis variable, ΔV = 0.04$^m$, P = 6.23 d |
| | | | | 5118 | 4185 | 00$^h$ 53$^m$ 28.22$^s$ | +37° 25′ 05.9″ | 6.07 | 0.77 | 374 | K3III: | |
| | | | | 221293 | 116030 | 23$^h$ 30$^m$ 39.54$^s$ | +38° 39′ 44.0″ | 6.07 | −0.33 | 621 | G9III | |
| HD 223229 | | | | 223229 | 117340 | 23$^h$ 47$^m$ 33.05$^s$ | +46° 49′ 57.3″ | 6.08 | −1.96 | 1320 | B3IV | suspected variable |
| | | | | 225239 | 394 | 00$^h$ 04$^m$ 53.21$^s$ | +34° 39′ 34.4″ | 6.09 | 3.26 | 120 | G2V | |
| 59 And A | | 59 | | 13294 | 10176 | 02$^h$ 10$^m$ 52.83$^s$ | +39° 02′ 22.5″ | 6.09 | 1.56 | 263 | B9V | binary star |
| 26 And | | 26 | | 1438 | 1501 | 00$^h$ 18$^m$ 42.15$^s$ | +43° 47′ 28.1″ | 6.10 | −0.53 | 692 | B8V | double star |
| | | | | 5526 | 4501 | 00$^h$ 57$^m$ 39.64$^s$ | +45° 50′ 21.8″ | 6.10 | 0.45 | 439 | K2III | |
| HD 225218 | | | | 225218 | 365 | 00$^h$ 04$^m$ 36.60$^s$ | +42° 05′ 33.2″ | 6.11 | −2.45 | 1680 | B9III | double star |
| | | | | 7647 | 5993 | 01$^h$ 17$^m$ 05.05$^s$ | +44° 54′ 07.5″ | 6.11 | −0.18 | 590 | K5 | |
| HD 1185 | | | | 1185 | 1302 | 00$^h$ 16$^m$ 21.50$^s$ | +43° 35′ 42.4″ | 6.12 | 1.28 | 303 | A2V | double star |
| | | | | 218416 | 114162 | 23$^h$ 07$^m$ 10.05$^s$ | +52° 48′ 59.6″ | 6.12 | 0.55 | 423 | K0III | |
| GO And | | | GO | 4778 | 3919 | 00$^h$ 50$^m$ 18.21$^s$ | +45° 00′ 08.1″ | 6.13 | 1.34 | 296 | A0p... | α$^2$ CVn variable, ΔV = 0.04$^m$, P = 2.5481 d |
| | | | | 7158 | 5650 | 01$^h$ 12$^m$ 34.06$^s$ | +45° 20′ 14.9″ | 6.13 | −0.52 | 698 | M1III | |
| 66 And | | 66 | | 15138 | 11465 | 02$^h$ 27$^m$ 51.75$^s$ | +50° 34′ 12.7″ | 6.16 | 2.54 | 173 | F4V | spectroscopic binary |
| | | | | 14372 | 10924 | 02$^h$ 20$^m$ 41.50$^s$ | +47° 18′ 39.0″ | 6.17 | −0.87 | 836 | B5V | |
| | | | | 743 | 967 | 00$^h$ 11$^m$ 59.03$^s$ | +48° 09′ 08.5″ | 6.18 | 0.05 | 550 | K4III | |
| | | | | 3411 | 2926 | 00$^h$ 37$^m$ 07.20$^s$ | +24° 00′ 51.3″ | 6.18 | 1.13 | 334 | K2III | |
| HD 221776 | | | | 221776 | 116365 | 23$^h$ 34$^m$ 46.73$^s$ | +38° 01′ 26.3″ | 6.18 | −0.41 | 678 | K5 | double star |
| | | | | 16327 | 12287 | 02$^h$ 38$^m$ 17.86$^s$ | +37° 43′ 36.6″ | 6.19 | 1.60 | 270 | F6III | triple star |
| HD 221246 | | | | 221246 | 115996 | 23$^h$ 30$^m$ 07.39$^s$ | +49° 07′ 59.3″ | 6.19 | −0.91 | 856 | K5III | member of the NGC 7686 star cluster |
| OP And | | | OP | 9746 | 7493 | 01$^h$ 36$^m$ 27.21$^s$ | +48° 43′ 22.2″ | 6.20 | 0.65 | 420 | K1III: | BY Dra variable, ΔV = 0.09$^m$ |
| | | | | 400 | 699 | 00$^h$ 08$^m$ 41.02$^s$ | +36° 37′ 38.7″ | 6.21 | 3.61 | 108 | F8IV | |
| | | | | 14213 | 10814 | 02$^h$ 19$^m$ 10.84$^s$ | +46° 28′ 20.2″ | 6.21 | 0.50 | 452 | A4V | |
| | | | | 952 | 1123 | 00$^h$ 14$^m$ 02.29$^s$ | +33° 12′ 21.9″ | 6.22 | 1.45 | 293 | A1V | |
| HD 895 | | | | 895 | 1076 | 00$^h$ 13$^m$ 23.93$^s$ | +26° 59′ 15.4″ | 6.24 | 0.78 | 403 | G0III | triple star |
| | | | | 222451 | 116824 | 23$^h$ 40$^m$ 40.47$^s$ | +36° 43′ 14.6″ | 6.24 | 3.01 | 144 | F1V | |
| | | | | 224906 | 137 | 00$^h$ 01$^m$ 43.85$^s$ | +42° 22′ 01.7″ | 6.25 | −1.80 | 1331 | B9IIIp Mn | |
| | | | | 11613 | 8922 | 01$^h$ 54$^m$ 53.75$^s$ | +40° 42′ 07.9″ | 6.25 | 1.13 | 345 | K2 | |
| HD 220105 | | | | 220105 | 115261 | 23$^h$ 20$^m$ 44.11$^s$ | +44° 06′ 58.5″ | 6.25 | 1.73 | 261 | A5Vn | double star |
| | | | | 221661 | 116292 | 23$^h$ 33$^m$ 42.99$^s$ | +45° 03′ 29.1″ | 6.25 | 0.12 | 548 | G8II | |
| HD 2942 | | | | 2942 | 2583 | 00$^h$ 32$^m$ 49.09$^s$ | +28° 16′ 48.8″ | 6.26 | 0.47 | 469 | G8II | triple star |
| | | | | 8774 | 6776 | 01$^h$ 27$^m$ 06.21$^s$ | +34° 22′ 39.3″ | 6.27 | 3.12 | 139 | F7IVsvar | |
| | | | | 2507 | 2270 | 00$^h$ 28$^m$ 56.67$^s$ | +36° 53′ 58.9″ | 6.28 | 0.51 | 464 | G5III | |
| | | | | 8375 | 6512 | 01$^h$ 23$^m$ 37.31$^s$ | +34° 14′ 44.2″ | 6.28 | 2.43 | 192 | G8IV | |
| | | | | 11624 | 8930 | 01$^h$ 54$^m$ 57.63$^s$ | +37° 07′ 42.0″ | 6.28 | 0.25 | 525 | K0 | |
| | | | | 7758 | 6087 | 01$^h$ 18$^m$ 10.14$^s$ | +47° 25′ 11.0″ | 6.29 | −2.07 | 1531 | K0 | |
| | | | | 16350 | 12305 | 02$^h$ 38$^m$ 27.94$^s$ | +38° 05′ 21.0″ | 6.29 | −0.47 | 734 | B9.5V | |
| | | | | 219962 | 115171 | 23$^h$ 19$^m$ 41.37$^s$ | +48° 22′ 51.1″ | 6.29 | 0.47 | 475 | K1III | |
| | | | | 217314 | 113501 | 22$^h$ 59$^m$ 10.37$^s$ | +52° 39′ 16.0″ | 6.31 | −0.26 | 672 | K2 | |
| | | | | 10597 | 8127 | 01$^h$ 44$^m$ 26.53$^s$ | +46° 08′ 23.2″ | 6.32 | 0.23 | 540 | K5III | |
| | | | | 219290 | 114714 | 23$^h$ 14$^m$ 14.34$^s$ | +50° 37′ 04.5″ | 6.32 | 0.82 | 411 | A0V | |
| | | | | 10486 | 8044 | 01$^h$ 43$^m$ 16.39$^s$ | +45° 19′ 21.5″ | 6.33 | 2.61 | 181 | K2IV | |
| | | | | 10874 | 8370 | 01$^h$ 47$^m$ 48.00$^s$ | +46° 13′ 47.6″ | 6.33 | 2.50 | 190 | F6V | |
| | | | | 1075 | 1208 | 00$^h$ 15$^m$ 06.93$^s$ | +31° 32′ 08.7″ | 6.34 | −1.70 | 1320 | K5 | |
| HD 8673 | | | | 8673 | 6702 | 01$^h$ 26$^m$ 08.62$^s$ | +34° 34′ 47.7″ | 6.34 | 3.43 | 125 | F7V | has a planet (b) |
| | | | | 1083 | 1215 | 00$^h$ 15$^m$ 10.55$^s$ | +27° 17′ 00.5″ | 6.35 | 0.84 | 412 | A1Vn | double star |
| | | | | 1527 | 1575 | 00$^h$ 19$^m$ 41.58$^s$ | +40° 43′ 46.2″ | 6.35 | 0.25 | 541 | K1III | |
| | | | | 221970 | 116505 | 23$^h$ 36$^m$ 30.52$^s$ | +32° 54′ 15.1″ | 6.35 | 1.92 | 251 | F6V | |
| CG And | | | CG | 224801 | 63 | 00$^h$ 00$^m$ 43.62$^s$ | +45° 15′ 12.0″ | 6.36 | −0.23 | 678 | B9p SiEu | α$^2$ CVn variable, V$_{max}$ = 6.32$^m$, V$_{min}$ = 6.42$^m$, P = 3.73975 d |
| HD 16004 | | | | 16004 | 12057 | 02$^h$ 35$^m$ 27.89$^s$ | +39° 39′ 52.1″ | 6.36 | 0.11 | 580 | B9MNp... | triple star |
| | | | | 13818 | 10562 | 02$^h$ 15$^m$ 57.69$^s$ | +47° 48′ 43.4″ | 6.37 | 0.61 | 462 | G9III-IV | |
| LN And | | | LN | 217811 | 113802 | 23$^h$ 02$^m$ 45.15$^s$ | +44° 03′ 31.6″ | 6.37 | −1.42 | 1177 | B2V | double star; not variable despite designation |
| V385 And | | | V385 | 220524 | 115530 | 23$^h$ 24$^m$ 08.88$^s$ | +41° 36′ 46.3″ | 6.37 | −1.55 | 1249 | M0 | irregular variable, V$_{max}$ = 6.36$^m$, V$_{min}$ = 6.47$^m$ |
| GY And | | | GY | 9996 | 7651 | 01$^h$ 38$^m$ 31.84$^s$ | +45° 23′ 58.9″ | 6.38 | 0.66 | 455 | B9Vp (Cr-Eu) | Promethium lines; α$^2$ CVn variable, V$_{max}$ = 6.27$^m$, V$_{min}$ = 6.44$^m$, P = 8000 d |
| | | | | 13013 | 9983 | 02$^h$ 08$^m$ 33.55$^s$ | +44° 27′ 34.4″ | 6.38 | 0.78 | 430 | G8III | |
| | | | | 218365 | 114152 | 23$^h$ 07$^m$ 04.99$^s$ | +35° 38′ 11.3″ | 6.38 | −0.08 | 638 | K0 | |
| | | | | 9712 | 7444 | 01$^h$ 35$^m$ 52.46$^s$ | +41° 04′ 35.1″ | 6.39 | 1.01 | 388 | K1III | |
| V529 And | | | V529 | 8801 | 6794 | 01$^h$ 27$^m$ 26.67$^s$ | +41° 06′ 04.0″ | 6.42 | 2.69 | 182 | Am... | δ Scuti variable, ΔV = 0.03$^m$, P = 0.40331 d |
| | | | | 217731 | 113750 | 23$^h$ 02$^m$ 11.32$^s$ | +44° 34′ 22.4″ | 6.43 | 1.22 | 359 | K0 | |
| HD 222641 | | | | 222641 | 116941 | 23$^h$ 42$^m$ 14.68$^s$ | +44° 59′ 30.3″ | 6.43 | −0.48 | 786 | K5III | suspected variable |
| HD 7853 | | | | 7853 | 6140 | 01$^h$ 18$^m$ 47.02$^s$ | +37° 23′ 10.7″ | 6.44 | 0.71 | 456 | A5m | double star |
| | | | | 14221 | 10830 | 02$^h$ 19$^m$ 22.77$^s$ | +48° 57′ 19.0″ | 6.44 | 2.39 | 210 | F4V | |
| | | | | 219668 | 114981 | 23$^h$ 17$^m$ 16.59$^s$ | +45° 09′ 51.5″ | 6.44 | 2.10 | 241 | K0IV | |
| HD 6114 | | | | 6114 | 4911 | 01$^h$ 03$^m$ 01.47$^s$ | +47° 22′ 34.3″ | 6.46 | 1.39 | 337 | A9V | double star |
| | | | | 11884 | 9163 | 01$^h$ 57$^m$ 59.23$^s$ | +47° 05′ 43.9″ | 6.48 | −1.24 | 1140 | K0 | |
| ET And | | | ET | 219749 | 115036 | 23$^h$ 17$^m$ 55.99$^s$ | +45° 29′ 20.2″ | 6.48 | 0.36 | 545 | B9Vp(Si) | α$^2$ CVn variable, ΔV = 0.03$^m$, P = 1.61888 d |
| HD 222399 | | | | 222399 | 116781 | 23$^h$ 40$^m$ 02.82$^s$ | +37° 39′ 10.2″ | 6.49 | 1.74 | 291 | F2IV | double star |
| PY And | | | PY | 3322 | 2865 | 00$^h$ 36$^m$ 20.00$^s$ | +27° 15′ 17″ | 6.50 | -0.16 | 701 | B8IIImnp... | α$^2$ CVn variable, ΔV = ~0.03$^m$ |
| | | | | 800 | 1009 | 00$^h$ 12$^m$ 34.08$^s$ | +44° 42′ 26.1″ | 6.50 | 0.50 | 517 | K0 | |
| 59 And B | | 59 | | 13295 | 10180 | 02$^h$ 10$^m$ 53.67$^s$ | +39° 02′ 36.0″ | 6.82 | −1.76 | 1698 | A1Vn | component of the 59 And system |
| HD 222155 | | | | 222155 | 116616 | 23$^h$ 38$^m$ 00$^s$ | +48° 59′ 47″ | 7.1 | 3.65 | 160 | G2V | has a planet (b) |
| HD 16175 | | | | 16175 | 12191 | 02$^h$ 37$^m$ 01.91$^s$ | +42° 03′ 45.5″ | 7.28 | 3.40 | 195 | G0 | Buna; has a planet (b) |
| R And | | | R | 1967 | 1901 | 00$^h$ 24$^m$ 01.95$^s$ | +38° 34′ 37.3″ | 7.39 | -5.19 | 790 | S6.5IIIeZr6Ti2 | Mira variable, V$_{max}$ = 5.8$^m$, V$_{min}$ = 15.2$^m$, P = 409.2 d |
| HD 1605 | | | | 1605 | 1640 | 00$^h$ 20$^m$ 32.0$^s$ | +30° 58′ 29″ | 7.52 | 2.88 | 276 | K1IV | has two planets (b & c) |
| HD 13931 | | | | 13931 | 10626 | 02$^h$ 16$^m$ 47.38$^s$ | +43° 46′ 22.8″ | 7.52 | 4.3 | 144 | G0 | has a planet (b) |
| HD 5583 | | | | 5583 | | 00$^h$ 57$^m$ 57.0$^s$ | +34° 59′ 08″ | 7.6 | 0.88 | 721 | K0 | has a planet (b) |
| RW And | | | RW | 4489 | | 00$^h$ 47$^m$ 18.92$^s$ | +32° 41′ 08.6″ | 7.9 | -0.52 | 1375 | M5e-M10e(S6,2e) | Mira variable, V$_{max}$ = 7.9$^m$, V$_{min}$ = 15.7$^m$, P = 430 d |
| Groombridge 34 | | | | 1326 | 1475 | 00$^h$ 18$^m$ 22.9$^s$ | +44° 01′ 22″ | 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 | 02$^h$ 26$^m$ 51.06$^s$ | +37° 33′ 01.7″ | 8.3 | 3.0 | 377 | A5 | has a transiting planet WASP-33b |
| RU And | | | RU | | | 01$^h$ 38$^m$ 37$^s$ | 38° 40′ 12″ | 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. |
| Y And | | | | 10112 | | 01$^h$ 39$^m$ 36.89$^s$ | +39° 20′ 35″ | 10.39 | | 8,000 | M3-4.5e | Mira Cet variable |
| Z And | | | Z | 221650 | 116287 | 23$^h$ 33$^m$ 39.95$^s$ | +48° 49′ 05.9″ | 10.53 | 2.38 | 1393 | M2III + B1eq | prototype of Z And variables, V$_{max}$ = 7.7$^m$, V$_{min}$ = 11.3$^m$ |
| HAT-P-6 | | | | | | 23$^h$ 39$^m$ 05.81$^s$ | +42° 27′ 57.5″ | 10.54 | 4.03 | 650 | F | Sterrennacht; has a transiting planet (b) |
| HAT-P-16 | | | | | | 00$^h$ 38$^m$ 17.56$^s$ | +42° 27′ 47.2″ | 10.8 | 3.9 | 766 | F8 | has a transiting planet (b) |
| HAT-P-32 | | | | | | 02$^h$ 01$^m$ 10$^s$ | +46° 41′ 16″ | 11.29 | 3.76 | 1044 | F/G | has a transiting planet (b) |
| WASP-1 | | | | | | 00$^h$ 20$^m$ 40.08$^s$ | +31° 59′ 23.8″ | 11.79 | 3.89 | 1239 | F7V | has a transiting planet (b) |
| Ross 248 | | | | | | 23$^h$ 41$^m$ 54.99$^s$ | +44° 10′ 40.8″ | 12.29 | 14.79 | 10.32 | M6e | HH And; 8th closest star system, flare star |
| HAT-P-19 | | | | | | 00$^h$ 38$^m$ 04$^s$ | +34° 42′ 42″ | 12.9 | 6.24 | 701 | K | has a transiting planet (b) |
| HAT-P-28 | | | | | | 00$^h$ 52$^m$ 00$^s$ | +34° 43′ 42″ | 13.03 | 5.05 | 1288 | G3 | has a transiting planet (b) |
| HAT-P-53 | | | | | | 01$^h$ 27$^m$ 29.0$^s$ | +38° 58′ 05″ | 13.73 | 4.45 | 2345 | | has a transiting planet (b) |
| S And | | | S | | | 00$^h$ 42$^m$ 43.11$^s$ | +41° 16′ 04.2″ | | | 2600000 | Ia | SN 1885A; BD+40°147a; type Ia supernova in the Andromeda Galaxy, V$_{max}$ = 5.8$^m$, V$_{min}$ = < 16$^m$ |
| Table legend:  • Name = Proper name  • B = Bayer designation  • F or/and G. = Flamsteed designation or Gould designation  • Var = Variable star designation  • HD = Henry Draper Catalogue designation number  • HIP = Hipparcos Catalogue designation number  • RA = Right ascension for the Epoch/Equinox J2000.0  • Dec = Declination for the Epoch/Equinox J2000.0  • vis. mag. = visual magnitude (m or m$_v$), also known as apparent magnitude  • abs. mag. = absolute magnitude (M$_v$)  • Dist. (ly) = Distance in light-years from Earth  • Sp. class = Spectral class of the star in the stellar classification system  • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] |||||||||||||

## Notes

* ↑ It was commonly with δ Peg by Bayer.
* ↑ Flamsteed lettered it as n.
* ↑ Armando Gil de Paz et al., "The GALEX Ultraviolet Atlas of Nearby Galaxies," The Astrophysical Journal Supplement Series (ApJS), American Astronomical Society, 2007, 173 185–255.
* ↑ Bayer designated it as υ Per.
* ↑ Bode lettered it as 2.υ, in his "Verzeichniss".
* ↑ Flamsteed lettered it as υ.
* ↑ Bode lettered it as 1.υ in his "Verzeichniss".
* 1 2 Final Results of NameExoWorlds Public Vote Released
* ↑ E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
* 1 2 Flamsteed unlettered it in his catalogue and atlas.
* ↑ Bayer originally lettered it as υ.
* ↑ Flamsteed lettered it as λ.
* ↑ Flamsteed lettered it as d.
* ↑ Flamsteed lettered it as ξ.
* ↑ Flamsteed lettered it as h Per.
* ↑ Persei, on the constellation boundary between Andromeda with Perseus
* ↑ 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.
* ↑ V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.