List of stars in Coma Berenices
# List of stars in Coma Berenices

This is the list of notable stars in the constellation Coma Berenices, sorted by decreasing brightness.

| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| - | - | - | - | - | - | - | - | - | - | - | - | - |
| β Com | β | 43 | | 114710 | 64394 | $13^h$ $11^m$ $52.92^s$ | +27° 52′ 33.7″ | 4.26 | 4.42 | 30 | G0V | suspected BY Dra variable, ΔV = $0.02^m$ |
| α Com A | α | 42 | | 114378 | 64241 | $13^h$ $09^m$ $59.55^s$ | +17° 31′ 44.8″ | 4.32 | 3.54 | 47 | F5V | Diadem, Al Dafirah; double star; suspected Algol variable, $V_{max}$ = $4.29^m,$ $V_{min}$ = $4.35^m,$ P = 9485.68 d |
| γ Com | γ | 15 | | 108381 | 60742 | $12^h$ $26^m$ $56.33^s$ | +28° 16′ 07.0″ | 4.35 | 0.76 | 170 | K2IIICN+... | |
| 11 Com | | 11 | | 107383 | 60202 | $12^h$ $20^m$ $43.09^s$ | +17° 47′ 33.6″ | 4.72 | −0.50 | 361 | G8III | |
| 36 Com | | 36 | | 112769 | 63355 | $12^h$ $58^m$ $55.47^s$ | +17° 24′ 33.7″ | 4.76 | −0.05 | 299 | M0III | suspected variable, $V_{max}$ = $4.74^m,$ $V_{min}$ = $4.82^m$ |
| 12 Com A | | 12 | | 107700 | 60351 | $12^h$ $22^m$ $30.32^s$ | +25° 50′ 46.3″ | 4.78 | 0.16 | 273 | F8:p... | double star; suspected variable, $V_{max}$ = $4.78^m,$ $V_{min}$ = $4.89^m$ |
| 23 Com | | 23 | | 109485 | 61394 | $12^h$ $34^m$ $51.12^s$ | +22° 37′ 45.1″ | 4.80 | −0.44 | 365 | A0IV | |
| 41 Com | | 41 | | 113996 | 64022 | $13^h$ $07^m$ $10.71^s$ | +27° 37′ 29.7″ | 4.80 | −0.04 | 303 | K5III | has a planet (b) |
| 35 Com | | 35 | | 112033 | 62886 | $12^h$ $53^m$ $17.77^s$ | +21° 14′ 42.1″ | 4.89 | −0.10 | 324 | G8III | |
| 37 Com | | 37 | LU | 112989 | 63462 | $13^h$ $00^m$ $16.49^s$ | +30° 47′ 06.1″ | 4.90 | −2.32 | 898 | K1IIIp | RS CVn variable, ΔV = $0.15^m$ |
| 14 Com | | 14 | | 108283 | 60697 | $12^h$ $26^m$ $24.07^s$ | +27° 16′ 05.7″ | 4.92 | 0.30 | 273 | F0p | |
| 7 Com | | 7 | | 106714 | 59847 | $12^h$ $16^m$ $20.56^s$ | +23° 56′ 43.5″ | 4.93 | 0.52 | 248 | K0III | |
| 31 Com | | 31 | LS | 111812 | 62763 | $12^h$ $51^m$ $41.93^s$ | +27° 32′ 26.6″ | 4.93 | 0.06 | 307 | G0III | Polaris Galacticum Borealis, Lángjiāng (郎將), FK Com variable, $V_{max}$ = $4.87^m,$ $V_{min}$ = $4.97^m$ |
| 16 Com | | 16 | | 108382 | 60746 | $12^h$ $26^m$ $59.30^s$ | +26° 49′ 32.6″ | 4.98 | 0.29 | 282 | A4V | |
| HD 106760 | | | | 106760 | 59856 | $12^h$ $16^m$ $30.17^s$ | +33° 03′ 42.5″ | 4.99 | 0.13 | 306 | K1III | suspected variable |
| 24 Com A | | 24 | | 109511 | 61418 | $12^h$ $35^m$ $07.76^s$ | +18° 22′ 37.2″ | 5.03 | −1.34 | 614 | K2III | double star; suspected variable, $V_{max}$ = $4.98^m,$ $V_{min}$ = $5.06^m$ |
| 6 Com | | 6 | | 106661 | 59819 | $12^h$ $16^m$ $00.23^s$ | +14° 53′ 56.9″ | 5.09 | 1.18 | 198 | A3V | |
| 27 Com | | 27 | | 111067 | 62356 | $12^h$ $46^m$ $38.75^s$ | +16° 34′ 39.5″ | 5.12 | 0.15 | 322 | K3III | |
| 13 Com | | 13 | GN | 107966 | 60514 | $12^h$ $24^m$ $18.54^s$ | +26° 05′ 55.0″ | 5.17 | 0.47 | 284 | A3V | α² Cvn variable, $V_{max}$ = $5.15^m,$ $V_{min}$ = $5.18^m$ |
| α Com B | α | 42 | | 114379 | | $13^h$ $09^m$ $59.30^s$ | +17° 31′ 46.0″ | 5.22 | | | | component of the α Com system |
| 17 Com | | 17 | AI | 108662 | 60904 | $12^h$ $28^m$ $54.72^s$ | +25° 54′ 46.4″ | 5.29 | 0.70 | 270 | A0p | α² Cvn and δ Sct variable, $V_{max}$ = $5.23^m,$ $V_{min}$ = $5.4^m,$ P = 5.0633 d |
| 21 Com | | 21 | UU | 108945 | 61071 | $12^h$ $31^m$ $00.57^s$ | +24° 34′ 01.9″ | 5.44 | 0.57 | 311 | A2pvar | Kissīn; α² CVn and δ Sct variable, $V_{max}$ = $5.41^m,$ $V_{min}$ = $5.46^m$ |
| 18 Com | | 18 | | 108722 | 60941 | $12^h$ $29^m$ $27.05^s$ | +24° 06′ 32.1″ | 5.47 | 1.36 | 216 | F5III | |
| 26 Com | | 26 | | 110024 | 61724 | $12^h$ $39^m$ $07.36^s$ | +21° 03′ 45.3″ | 5.49 | 0.77 | 286 | G9III | |
| HD 107325 | | | | 107325 | 60170 | $12^h$ $20^m$ $19.72^s$ | +26° 37′ 11.1″ | 5.52 | 2.11 | 157 | K2III-IV | suspected variable, $V_{max}$ = $5.50^m,$ $V_{min}$ = $5.56^m$ |
| FS Com | | 40 | FS | 113866 | 63950 | $13^h$ $06^m$ $22.58^s$ | +22° 36′ 58.6″ | 5.53 | −0.69 | 572 | M5III | semiregular variable, $V_{max}$ = $5.3^m,$ $V_{min}$ = $6.1^m,$ P = 58 d |
| 5 Com | | 5 | | 106057 | 59501 | $12^h$ $12^m$ $09.30^s$ | +20° 32′ 31.6″ | 5.60 | −0.26 | 484 | K0II-III | |
| 4 Com | | 4 | | 105981 | 59468 | $12^h$ $11^m$ $51.20^s$ | +25° 52′ 13.3″ | 5.66 | −1.22 | 774 | K4III | variable star, ΔV = $0.005^m,$ P = 6.71096 d |
| 20 Com | | 20 | | 108765 | 60957 | $12^h$ $29^m$ $43.22^s$ | +20° 53′ 46.3″ | 5.68 | 1.22 | 254 | A3V | |
| 25 Com | | 25 | | 109742 | 61571 | $12^h$ $36^m$ $58.35^s$ | +17° 05′ 22.5″ | 5.70 | −0.31 | 518 | K5III | |
| HD 106887 | | | | 106887 | 59923 | $12^h$ $17^m$ $30.60^s$ | +28° 56′ 13.6″ | 5.71 | 2.07 | 174 | A4m | |
| 29 Com | | 29 | | 111397 | 62541 | $12^h$ $48^m$ $54.20^s$ | +14° 07′ 21.5″ | 5.71 | 0.25 | 402 | A1V | 36 Virginis |
| HD 116706 | | | | 116706 | 65466 | $13^h$ $25^m$ $06.68^s$ | +23° 51′ 16.0″ | 5.75 | 1.29 | 254 | A3IV | suspected variable |
| 30 Com | | 30 | | 111469 | 62576 | $12^h$ $49^m$ $17.51^s$ | +27° 33′ 08.4″ | 5.76 | 0.75 | 327 | A2V | |
| HD 109519 | | | | 109519 | 61420 | $12^h$ $35^m$ $08.15^s$ | +21° 52′ 53.2″ | 5.86 | −0.65 | 652 | K1III | |
| 2 Com | | 2 | | 104827 | 58858 | $12^h$ $04^m$ $16.58^s$ | +21° 27′ 33.0″ | 5.89 | 0.68 | 359 | F0IV-V | |
| HD 114326 | | | | 114326 | 64226 | $13^h$ $09^m$ $47.89^s$ | +16° 50′ 55.1″ | 5.91 | −0.85 | 733 | K5III | suspected variable |
| 38 Com | | 38 | | 113095 | 63533 | $13^h$ $01^m$ $09.62^s$ | +17° 07′ 23.5″ | 5.97 | 0.52 | 400 | K0III | |
| 39 Com | | 39 | | 113848 | 63948 | $13^h$ $06^m$ $21.28^s$ | +21° 09′ 12.6″ | 6.00 | 2.51 | 163 | F4V | |
| HD 105805 | | | | 105805 | 59364 | $12^h$ $10^m$ $46.10^s$ | +27° 16′ 53.5″ | 6.01 | 1.14 | 308 | A4Vn | suspected variable, $V_{max}$ = $6.00^m,$ $V_{min}$ = $6.04^m$ |
| HD 108123 | | | | 108123 | 60599 | $12^h$ $25^m$ $15.07^s$ | +23° 55′ 34.7″ | 6.03 | 0.11 | 497 | K0III | |
| HD 114889 | | | | 114889 | 64496 | $13^h$ $13^m$ $12.54^s$ | +18° 43′ 37.7″ | 6.10 | 1.30 | 297 | G8III | |
| HD 117876 | | | | 117876 | 66086 | $13^h$ $32^m$ $48.17^s$ | +24° 20′ 50.0″ | 6.11 | 0.32 | 470 | G8III | |
| HD 107326 | | | | 107326 | 60168 | $12^h$ $20^m$ $17.84^s$ | +26° 00′ 06.6″ | 6.16 | 2.25 | 198 | F0IV | suspected variable, $V_{max}$ = $6.12^m,$ $V_{min}$ = $6.16^m$ |
| HD 113022 | | | | 113022 | 63497 | $13^h$ $00^m$ $38.86^s$ | +18° 22′ 22.3″ | 6.20 | 3.14 | 133 | F6Vs | |
| HD 114092 | | | | 114092 | 64077 | $13^h$ $07^m$ $53.66^s$ | +27° 33′ 22.0″ | 6.20 | 0.82 | 389 | K4III | |
| HD 107655 | | | | 107655 | 60327 | $12^h$ $22^m$ $10.86^s$ | +24° 46′ 26.0″ | 6.21 | 1.20 | 327 | A0V | |
| HD 107054 | | | | 107054 | 60018 | $12^h$ $18^m$ $31.57^s$ | +30° 14′ 57.6″ | 6.23 | 2.51 | 181 | A9.5III | |
| 8 Com | | 8 | | 107168 | 60087 | $12^h$ $19^m$ $19.20^s$ | +23° 02′ 04.9″ | 6.26 | 1.55 | 285 | A8m | |
| 22 Com | | 22 | | 109307 | 61295 | $12^h$ $33^m$ $34.23^s$ | +24° 16′ 58.8″ | 6.28 | 1.15 | 346 | A4V | |
| HD 111893 | | | | 111893 | 62825 | $12^h$ $52^m$ $27.52^s$ | +16° 07′ 21.1″ | 6.29 | 1.05 | 364 | A7V | |
| LW Com | | | LW | 111395 | 62523 | $12^h$ $48^m$ $47.26^s$ | +24° 50′ 25.7″ | 6.31 | 5.12 | 56 | G7V | BY Dra variable, ΔV = $0.10^m,$ P = 15.80 d |
| HD 114724 | | | | 114724 | 64417 | $13^h$ $12^m$ $08.42^s$ | +24° 15′ 29.3″ | 6.31 | 0.32 | 513 | K1III | |
| HD 107398 | | | | 107398 | 60197 | $12^h$ $20^m$ $41.37^s$ | +27° 03′ 17.4″ | 6.32 | 1.49 | 301 | F3V + F3V | suspected variable |
| 32 Com | | 32 | | 111862 | 62807 | $12^h$ $52^m$ $12.26^s$ | +17° 04′ 26.2″ | 6.32 | −2.43 | 1831 | M0III | variable star, ΔV = $0.011^m,$ P = 52.08333 d |
| HD 106926 | | | | 106926 | 59941 | $12^h$ $17^m$ $44.24^s$ | +15° 08′ 41.3″ | 6.36 | 0.30 | 532 | K4III | |
| 9 Com | | 9 | | 107213 | 60098 | $12^h$ $19^m$ $29.66^s$ | +28° 09′ 26.0″ | 6.38 | 2.90 | 162 | F8Vs | |
| HD 109996 | | | | 109996 | 61719 | $12^h$ $39^m$ $02.21^s$ | +22° 39′ 34.4″ | 6.39 | 1.15 | 364 | K1III | |
| 3 Com | | 3 | | 105778 | 59352 | $12^h$ $10^m$ $31.64^s$ | +16° 48′ 33.4″ | 6.40 | −0.81 | 903 | A4V | suspected variable |
| HD 108007 | | | | 108007 | 60525 | $12^h$ $24^m$ $26.81^s$ | +25° 34′ 56.7″ | 6.41 | 1.46 | 319 | F0V | |
| HD 112060 | | | | 112060 | 62904 | $12^h$ $53^m$ $32.20^s$ | +19° 28′ 53.4″ | 6.42 | 3.20 | 144 | G5IV | |
| HD 111591 | | | | 111591 | 62653 | $12^h$ $50^m$ $17.23^s$ | +22° 51′ 48.8″ | 6.43 | 0.80 | 435 | K0III | has a planet (b) |
| HD 115365 | | | | 115365 | 64779 | $13^h$ $16^m$ $32.33^s$ | +19° 47′ 06.8″ | 6.43 | 1.76 | 280 | F0V | |
| FM Com | | | FM | 107131 | 60066 | $12^h$ $19^m$ $02.03^s$ | +26° 00′ 30.1″ | 6.44 | 2.03 | 248 | Am | δ Sct variable, $V_{max}$ = $6.4^m,$ $V_{min}$ = $6.48^m,$ P = 0.0551 d |
| HD 115319 | | | | 115319 | 64751 | $13^h$ $16^m$ $14.35^s$ | +19° 03′ 06.2″ | 6.46 | 1.59 | 307 | G8III | |
| HD 106022 | | | | 106022 | 59489 | $12^h$ $12^m$ $00.97^s$ | +28° 32′ 11.3″ | 6.47 | 1.94 | 263 | F5V | |
| HD 107415 | | | | 107415 | 60210 | $12^h$ $20^m$ $48.75^s$ | +15° 32′ 27.5″ | 6.47 | 0.64 | 479 | K0 | |
| 28 Com | | 28 | | 111308 | 62478 | $12^h$ $48^m$ $14.36^s$ | +13° 33′ 11.2″ | 6.47 | 0.99 | 407 | A1V | |
| HD 115404 | | | | 115404 | 64797 | $13^h$ $16^m$ $50.67^s$ | +17° 01′ 04.1″ | 6.49 | 6.24 | 37 | K2V | |
| 1 Com | | 1 | | 104452 | 58661 | $12^h$ $01^m$ $44.30^s$ | +22° 05′ 39.6″ | 6.57 | 0.61 | 507 | G0II | |
| 24 Com B | | 24 | | 109510 | 61415 | $12^h$ $35^m$ $06.35^s$ | +18° 22′ 37.3″ | 6.57 | −2.96 | 2629 | A7m | component of the 24 Com system; suspected variable, $V_{max}$ = $6.55^m,$ $V_{min}$ = $6.59^m$ |
| 17 Com | | 17 | | 108651 | 60891 | $12^h$ $28^m$ $44.58^s$ | +25° 53′ 57.7″ | 6.63 | 2.14 | 258 | A0p | |
| 10 Com | | 10 | | 107276 | 60123 | $12^h$ $19^m$ $50.63^s$ | +28° 27′ 51.8″ | 6.64 | 1.85 | 296 | Am | |
| HD 112127 | | | | 112127 | 62944 | $12^h$ $53^m$ $55.75^s$ | +26° 46′ 48.0″ | 6.88 | | 345 | K3III | carbon star |
| 33 Com | | 33 | | 111892 | 62819 | $12^h$ $52^m$ $22.83^s$ | +17° 06′ 30.5″ | 6.93 | 1.50 | 397 | F8 | |
| HD 114762 | | | | 114762 | 64426 | $13^h$ $12^m$ $19.74^s$ | +17° 31′ 01.6″ | 7.30 | 4.27 | 132 | F9V | has a planet (b) |
| HD 107146 | | | | 107146 | 60074 | $12^h$ $19^m$ $06.50^s$ | +16° 32′ 53.9″ | 7.07 | | 93 | G2V | has a debris disk |
| KR Com | | | KR | 115955 | 65069 | $13^h$ $20^m$ $15.78^s$ | +17° 45′ 57.0″ | 7.26 | | 273.7 | F5 | W UMa variable, $V_{max}$ = $7.26^m,$ $V_{min}$ = $7.32^m,$ P = 0.40797003 d |
| HD 115708 | | | HH | 115708 | 64936 | $13^h$ $18^m$ $37.25^s$ | +26° 21′ 56.8″ | 7.83 | | 377 | A2p | $α^2$ CVn variable, $V_{max}$ = $7.77^m,$ $V_{min}$ = $7.85^m,$ P = 5.07 d |
| HD 108863 | | | | 108863 | 61020 | $12^h$ $30^m$ $20^s$ | +21° 56′ 54″ | 7.89 | | 453 | K0 | has a planet (b) |
| HD 116029 | | | | 116029 | 65117 | $13^h$ $20^m$ $40^s$ | +24° 38′ 55″ | 8.04 | | 402 | K1III | has a planet (b) |
| HD 106103 | | | GM | 106103 | 59527 | $12^h$ $12^m$ $24.90^s$ | +27° 22′ 48.3″ | 8.09 | | 277.2 | F5V | δ Sct variable, $V_{max}$ = $8.06^m,$ $V_{min}$ = $8.14^m,$ P = 0.208 d |
| IL Com | | | IL | 108102 | 60582 | $12^h$ $25^m$ $02.26^s$ | +25° 33′ 38.4″ | 8.14 | | 310.2 | F8 | RS CVn variable, ΔV = $0.04^m$ |
| FK Com | | | FK | 117555 | 65915 | $13^h$ $30^m$ $46.80^s$ | +24° 13′ 57.75″ | 8.17 | 1.2 | 800 | G5II | prototype FK Com variable, $V_{max}$ = $8.03^m,$ $V_{min}$ = $8.43^m,$ P = 2.4015 d |
| 12 Com B | | 12 | | 107701 | | $12^h$ $22^m$ $32.30^s$ | +25° 51′ 06.0″ | 8.60 | | | | component of the 12 Com system |
| IN Com | | | IN | 112313 | 63087 | $12^h$ $55^m$ $33.75^s$ | +25° 53′ 30.6″ | 8.70 | | 2690 | G5III-IV | central star of planetary nebula LoTr 5; ΔV = $0.07^m$ |
| HD 108874 | | | | 108874 | 61028 | $12^h$ $30^m$ $26.88^s$ | +25° 52′ 47.4″ | 8.76 | 4.58 | 224 | G5 | has two planets (b & c) |
| BD +25 2511 | | | HZ | | | $12^h$ $29^m$ $40.92^s$ | +24° 31′ 14.7″ | 9.76 | | | G8:V... | RS CVn variable, $V_{max}$ = $9.71^m,$ $V_{min}$ = $9.81^m$ |
| UX Com | | | UX | | 63561 | $13^h$ $01^m$ $33.02^s$ | +28° 37′ 54.1″ | 10.01 | | 592 | G7III: | RS CVn variable, $V_{max}$ = $9.96^m,$ $V_{min}$ = $10.52^m,$ P = 3.642583 d |
| KELT-6 | | | | | | $13^h$ $03^m$ $55.65^s$ | +30° 38′ 24.28″ | 10.38 | 3.46 | 791 | F8IV | Has two planets (b & c) |
| RZ Com | | | RZ | | 61414 | $12^h$ $35^m$ $05.06^s$ | +23° 20′ 14.0″ | 10.57 | | 614 | G0Vn | W UMa variable, $V_{max}$ = $10.42^m,$ $V_{min}$ = $11.13^m,$ P = 0.33850604 d |
| Feige 66 | | | | | 61602 | $12^h$ $37^m$ $23.52^s$ | +25° 03′ 59.9″ | 10.59 | | 530 | Op | subdwarf |
| SS Com | | | SS | | | $12^h$ $49^m$ $39.08^s$ | +18° 42′ 11.9″ | 11.00 | | | F5 | W UMa variable, $V_{max}$ = $10.75^m,$ $V_{min}$ = $11.31^m,$ P = 0.412822 d |
| RW Com | | | RW | | 61243 | $12^h$ $33^m$ $00.28^s$ | +26° 42′ 58.8″ | 11.25 | | 278.4 | G2+G2 | W UMa variable, $V_{max}$ = $11^m,$ $V_{min}$ = $11.7^m,$ P = 0.237346 d |
| CC Com | | | CC | | | $12^h$ $12^m$ $06.03^s$ | +22° 31′ 58.7″ | 11.61 | | 261.0 | K4/5V | W UMa variable, $V_{max}$ = $11.61^m,$ $V_{min}$ = $12.20^m,$ P = 0.2206864 d |
| U Com | | | U | | 61809 | $12^h$ $40^m$ $03.20^s$ | +27° 29′ 56.1″ | 11.76 | | 929 | A9 | RR Lyr variable, $V_{max}$ = $11.5^m,$ $V_{min}$ = $11.97^m,$ P = 0.2927382 d |
| ST Com | | | ST | | 64875 | $13^h$ $17^m$ $51.34^s$ | +20° 46′ 50.8″ | 11.92 | | | F5 | RR Lyr variable, $V_{max}$ = $11.017^m,$ $V_{min}$ = $11.823^m,$ P = 0.5989210 d |
| EK Com | | | EK | | | $12^h$ $51^m$ $21.45^s$ | +27° 13′ 47.0″ | 12.02 | | | K0V | W UMa variable |
| HZ 43 | | | | | 64766 | $13^h$ $16^m$ $21.85^s$ | +29° 05′ 55.4″ | 12.66 | | 125.6 | DA.9 + M3Ve | white dwarf/red dwarf binary system |
| GD 153 | | | | | | $12^h$ $57^m$ $02.34^s$ | +22° 01′ 52.7″ | 13.35 | | | DA1.2 | white dwarf |
| HZ 21 | | | | | | $12^h$ $13^m$ $56.25^s$ | +32° 56′ 31.4″ | 14.69 | | | DA: | white dwarf |
| GP Com | | | GP | | | $13^h$ $05^m$ $42.43^s$ | +18° 01′ 04.0″ | 15.69 | | | DBe | interacting binary white dwarf, ΔV = $0.6^m,$ has a planet (b) |
| LM Com | | | LM | | | $12^h$ $26^m$ $30.90^s$ | +30° 38′ 52.7″ | 16.15 | | | DA1.7 | re-radiating binary system |
| AL Com | | | AL | | | $12^h$ $32^m$ $25.80^s$ | +14° 20′ 42.2″ | 16.2 | | | | WZ Sge variable |
| RBS 1223 | | | | | | $13^h$ $08^m$ $48.7^s$ | +21° 27′ 08″ | 28.6 | | | | neutron star |
| GO Com | | | GO | | | $12^h$ $56^m$ $37.10^s$ | +26° 36′ 43.7″ | | | | | SU UMa variable |
| PSR B1237+25 | | | | | | $12^h$ $39^m$ $40.39^s$ | +24° 53′ 49.9″ | | | | | pulsar |
| 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.] |||||||||||||
