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 | 13h 11m 52.92s | +27° 52′ 33.7″ | 4.26 | 4.42 | 30 | G0V | suspected BY Dra variable, ΔV = 0.02m | ||||
α Com A | α | 42 | 114378 | 64241 | 13h 09m 59.55s | +17° 31′ 44.8″ | 4.32 | 3.54 | 47 | F5V | Diadem, Al Dafirah; double star; suspected Algol variable, Vmax = 4.29m, Vmin = 4.35m, P = 9485.68 d | ||||
γ Com | γ | 15 | 108381 | 60742 | 12h 26m 56.33s | +28° 16′ 07.0″ | 4.35 | 0.76 | 170 | K2IIICN+... | |||||
11 Com | 11 | 107383 | 60202 | 12h 20m 43.09s | +17° 47′ 33.6″ | 4.72 | −0.50 | 361 | G8III | ||||||
36 Com | 36 | 112769 | 63355 | 12h 58m 55.47s | +17° 24′ 33.7″ | 4.76 | −0.05 | 299 | M0III | suspected variable, Vmax = 4.74m, Vmin = 4.82m | |||||
12 Com A | 12 | 107700 | 60351 | 12h 22m 30.32s | +25° 50′ 46.3″ | 4.78 | 0.16 | 273 | F8:p... | double star; suspected variable, Vmax = 4.78m, Vmin = 4.89m | |||||
23 Com | 23 | 109485 | 61394 | 12h 34m 51.12s | +22° 37′ 45.1″ | 4.80 | −0.44 | 365 | A0IV | ||||||
41 Com | 41 | 113996 | 64022 | 13h 07m 10.71s | +27° 37′ 29.7″ | 4.80 | −0.04 | 303 | K5III | has a planet (b) | |||||
35 Com | 35 | 112033 | 62886 | 12h 53m 17.77s | +21° 14′ 42.1″ | 4.89 | −0.10 | 324 | G8III | ||||||
37 Com | 37 | LU | 112989 | 63462 | 13h 00m 16.49s | +30° 47′ 06.1″ | 4.90 | −2.32 | 898 | K1IIIp | RS CVn variable, ΔV = 0.15m | ||||
14 Com | 14 | 108283 | 60697 | 12h 26m 24.07s | +27° 16′ 05.7″ | 4.92 | 0.30 | 273 | F0p | ||||||
7 Com | 7 | 106714 | 59847 | 12h 16m 20.56s | +23° 56′ 43.5″ | 4.93 | 0.52 | 248 | K0III | ||||||
31 Com | 31 | LS | 111812 | 62763 | 12h 51m 41.93s | +27° 32′ 26.6″ | 4.93 | 0.06 | 307 | G0III | Polaris Galacticum Borealis, Lángjiāng (郎將), [1] FK Com variable, Vmax = 4.87m, Vmin = 4.97m | ||||
16 Com | 16 | 108382 | 60746 | 12h 26m 59.30s | +26° 49′ 32.6″ | 4.98 | 0.29 | 282 | A4V | ||||||
HD 106760 | 106760 | 59856 | 12h 16m 30.17s | +33° 03′ 42.5″ | 4.99 | 0.13 | 306 | K1III | suspected variable | ||||||
24 Com A | 24 | 109511 | 61418 | 12h 35m 07.76s | +18° 22′ 37.2″ | 5.03 | −1.34 | 614 | K2III | double star; suspected variable, Vmax = 4.98m, Vmin = 5.06m | |||||
6 Com | 6 | 106661 | 59819 | 12h 16m 00.23s | +14° 53′ 56.9″ | 5.09 | 1.18 | 198 | A3V | ||||||
27 Com | 27 | 111067 | 62356 | 12h 46m 38.75s | +16° 34′ 39.5″ | 5.12 | 0.15 | 322 | K3III | ||||||
13 Com | 13 | GN | 107966 | 60514 | 12h 24m 18.54s | +26° 05′ 55.0″ | 5.17 | 0.47 | 284 | A3V | α² Cvn variable, Vmax = 5.15m, Vmin = 5.18m | ||||
α Com B | α | 42 | 114379 | 13h 09m 59.30s | +17° 31′ 46.0″ | 5.22 | component of the α Com system | ||||||||
17 Com | 17 | AI | 108662 | 60904 | 12h 28m 54.72s | +25° 54′ 46.4″ | 5.29 | 0.70 | 270 | A0p | α² Cvn and δ Sct variable, Vmax = 5.23m, Vmin = 5.4m, P = 5.0633 d | ||||
21 Com | 21 | UU | 108945 | 61071 | 12h 31m 00.57s | +24° 34′ 01.9″ | 5.44 | 0.57 | 311 | A2pvar | Kissīn; [2] α² CVn and δ Sct variable, Vmax = 5.41m, Vmin = 5.46m | ||||
18 Com | 18 | 108722 | 60941 | 12h 29m 27.05s | +24° 06′ 32.1″ | 5.47 | 1.36 | 216 | F5III | ||||||
26 Com | 26 | 110024 | 61724 | 12h 39m 07.36s | +21° 03′ 45.3″ | 5.49 | 0.77 | 286 | G9III | ||||||
HD 107325 | 107325 | 60170 | 12h 20m 19.72s | +26° 37′ 11.1″ | 5.52 | 2.11 | 157 | K2III-IV | suspected variable, Vmax = 5.50m, Vmin = 5.56m | ||||||
FS Com | 40 | FS | 113866 | 63950 | 13h 06m 22.58s | +22° 36′ 58.6″ | 5.53 | −0.69 | 572 | M5III | semiregular variable, Vmax = 5.3m, Vmin = 6.1m, P = 58 d | ||||
5 Com | 5 | 106057 | 59501 | 12h 12m 09.30s | +20° 32′ 31.6″ | 5.60 | −0.26 | 484 | K0II-III | ||||||
4 Com | 4 | 105981 | 59468 | 12h 11m 51.20s | +25° 52′ 13.3″ | 5.66 | −1.22 | 774 | K4III | variable star, ΔV = 0.005m, P = 6.71096 d | |||||
20 Com | 20 | 108765 | 60957 | 12h 29m 43.22s | +20° 53′ 46.3″ | 5.68 | 1.22 | 254 | A3V | ||||||
25 Com | 25 | 109742 | 61571 | 12h 36m 58.35s | +17° 05′ 22.5″ | 5.70 | −0.31 | 518 | K5III | ||||||
HD 106887 | 106887 | 59923 | 12h 17m 30.60s | +28° 56′ 13.6″ | 5.71 | 2.07 | 174 | A4m | |||||||
29 Com | 29 | 111397 | 62541 | 12h 48m 54.20s | +14° 07′ 21.5″ | 5.71 | 0.25 | 402 | A1V | 36 Virginis | |||||
HD 116706 | 116706 | 65466 | 13h 25m 06.68s | +23° 51′ 16.0″ | 5.75 | 1.29 | 254 | A3IV | suspected variable | ||||||
30 Com | 30 | 111469 | 62576 | 12h 49m 17.51s | +27° 33′ 08.4″ | 5.76 | 0.75 | 327 | A2V | ||||||
HD 109519 | 109519 | 61420 | 12h 35m 08.15s | +21° 52′ 53.2″ | 5.86 | −0.65 | 652 | K1III | |||||||
2 Com | 2 | 104827 | 58858 | 12h 04m 16.58s | +21° 27′ 33.0″ | 5.89 | 0.68 | 359 | F0IV-V | ||||||
HD 114326 | 114326 | 64226 | 13h 09m 47.89s | +16° 50′ 55.1″ | 5.91 | −0.85 | 733 | K5III | suspected variable | ||||||
38 Com | 38 | 113095 | 63533 | 13h 01m 09.62s | +17° 07′ 23.5″ | 5.97 | 0.52 | 400 | K0III | ||||||
39 Com | 39 | 113848 | 63948 | 13h 06m 21.28s | +21° 09′ 12.6″ | 6.00 | 2.51 | 163 | F4V | ||||||
HD 105805 | 105805 | 59364 | 12h 10m 46.10s | +27° 16′ 53.5″ | 6.01 | 1.14 | 308 | A4Vn | suspected variable, Vmax = 6.00m, Vmin = 6.04m | ||||||
HD 108123 | 108123 | 60599 | 12h 25m 15.07s | +23° 55′ 34.7″ | 6.03 | 0.11 | 497 | K0III | |||||||
HD 114889 | 114889 | 64496 | 13h 13m 12.54s | +18° 43′ 37.7″ | 6.10 | 1.30 | 297 | G8III | |||||||
HD 117876 | 117876 | 66086 | 13h 32m 48.17s | +24° 20′ 50.0″ | 6.11 | 0.32 | 470 | G8III | |||||||
HD 107326 | 107326 | 60168 | 12h 20m 17.84s | +26° 00′ 06.6″ | 6.16 | 2.25 | 198 | F0IV | suspected variable, Vmax = 6.12m, Vmin = 6.16m | ||||||
HD 113022 | 113022 | 63497 | 13h 00m 38.86s | +18° 22′ 22.3″ | 6.20 | 3.14 | 133 | F6Vs | |||||||
HD 114092 | 114092 | 64077 | 13h 07m 53.66s | +27° 33′ 22.0″ | 6.20 | 0.82 | 389 | K4III | |||||||
HD 107655 | 107655 | 60327 | 12h 22m 10.86s | +24° 46′ 26.0″ | 6.21 | 1.20 | 327 | A0V | |||||||
HD 107054 | 107054 | 60018 | 12h 18m 31.57s | +30° 14′ 57.6″ | 6.23 | 2.51 | 181 | A9.5III | |||||||
8 Com | 8 | 107168 | 60087 | 12h 19m 19.20s | +23° 02′ 04.9″ | 6.26 | 1.55 | 285 | A8m | ||||||
22 Com | 22 | 109307 | 61295 | 12h 33m 34.23s | +24° 16′ 58.8″ | 6.28 | 1.15 | 346 | A4V | ||||||
HD 111893 | 111893 | 62825 | 12h 52m 27.52s | +16° 07′ 21.1″ | 6.29 | 1.05 | 364 | A7V | |||||||
LW Com | LW | 111395 | 62523 | 12h 48m 47.26s | +24° 50′ 25.7″ | 6.31 | 5.12 | 56 | G7V | BY Dra variable, ΔV = 0.10m, P = 15.80 d | |||||
HD 114724 | 114724 | 64417 | 13h 12m 08.42s | +24° 15′ 29.3″ | 6.31 | 0.32 | 513 | K1III | |||||||
HD 107398 | 107398 | 60197 | 12h 20m 41.37s | +27° 03′ 17.4″ | 6.32 | 1.49 | 301 | F3V + F3V | suspected variable | ||||||
32 Com | 32 | 111862 | 62807 | 12h 52m 12.26s | +17° 04′ 26.2″ | 6.32 | −2.43 | 1831 | M0III | variable star, ΔV = 0.011m, P = 52.08333 d | |||||
HD 106926 | 106926 | 59941 | 12h 17m 44.24s | +15° 08′ 41.3″ | 6.36 | 0.30 | 532 | K4III | |||||||
9 Com | 9 | 107213 | 60098 | 12h 19m 29.66s | +28° 09′ 26.0″ | 6.38 | 2.90 | 162 | F8Vs | ||||||
HD 109996 | 109996 | 61719 | 12h 39m 02.21s | +22° 39′ 34.4″ | 6.39 | 1.15 | 364 | K1III | |||||||
3 Com | 3 | 105778 | 59352 | 12h 10m 31.64s | +16° 48′ 33.4″ | 6.40 | −0.81 | 903 | A4V | suspected variable | |||||
HD 108007 | 108007 | 60525 | 12h 24m 26.81s | +25° 34′ 56.7″ | 6.41 | 1.46 | 319 | F0V | |||||||
HD 112060 | 112060 | 62904 | 12h 53m 32.20s | +19° 28′ 53.4″ | 6.42 | 3.20 | 144 | G5IV | |||||||
HD 111591 | 111591 | 62653 | 12h 50m 17.23s | +22° 51′ 48.8″ | 6.43 | 0.80 | 435 | K0III | has a planet (b) | ||||||
HD 115365 | 115365 | 64779 | 13h 16m 32.33s | +19° 47′ 06.8″ | 6.43 | 1.76 | 280 | F0V | |||||||
FM Com | FM | 107131 | 60066 | 12h 19m 02.03s | +26° 00′ 30.1″ | 6.44 | 2.03 | 248 | Am | δ Sct variable, Vmax = 6.4m, Vmin = 6.48m, P = 0.0551 d | |||||
HD 115319 | 115319 | 64751 | 13h 16m 14.35s | +19° 03′ 06.2″ | 6.46 | 1.59 | 307 | G8III | |||||||
HD 106022 | 106022 | 59489 | 12h 12m 00.97s | +28° 32′ 11.3″ | 6.47 | 1.94 | 263 | F5V | |||||||
HD 107415 | 107415 | 60210 | 12h 20m 48.75s | +15° 32′ 27.5″ | 6.47 | 0.64 | 479 | K0 | |||||||
28 Com | 28 | 111308 | 62478 | 12h 48m 14.36s | +13° 33′ 11.2″ | 6.47 | 0.99 | 407 | A1V | ||||||
HD 115404 | 115404 | 64797 | 13h 16m 50.67s | +17° 01′ 04.1″ | 6.49 | 6.24 | 37 | K2V | |||||||
1 Com | 1 | 104452 | 58661 | 12h 01m 44.30s | +22° 05′ 39.6″ | 6.57 | 0.61 | 507 | G0II | ||||||
24 Com B | 24 | 109510 | 61415 | 12h 35m 06.35s | +18° 22′ 37.3″ | 6.57 | −2.96 | 2629 | A7m | component of the 24 Com system; suspected variable, Vmax = 6.55m, Vmin = 6.59m | |||||
17 Com | 17 | 108651 | 60891 | 12h 28m 44.58s | +25° 53′ 57.7″ | 6.63 | 2.14 | 258 | A0p | ||||||
10 Com | 10 | 107276 | 60123 | 12h 19m 50.63s | +28° 27′ 51.8″ | 6.64 | 1.85 | 296 | Am | ||||||
HD 112127 | 112127 | 62944 | 12h 53m 55.75s | +26° 46′ 48.0″ | 6.88 | 345 | K3III | carbon star | |||||||
33 Com | 33 | 111892 | 62819 | 12h 52m 22.83s | +17° 06′ 30.5″ | 6.93 | 1.50 | 397 | F8 | ||||||
HD 114762 | 114762 | 64426 | 13h 12m 19.74s | +17° 31′ 01.6″ | 7.30 | 4.27 | 132 | F9V | has a planet (b) | ||||||
HD 107146 | 107146 | 60074 | 12h 19m 06.50s | +16° 32′ 53.9″ | 7.07 | 93 | G2V | has a debris disk | |||||||
KR Com | KR | 115955 | 65069 | 13h 20m 15.78s | +17° 45′ 57.0″ | 7.26 | 273.7 | F5 | W UMa variable, Vmax = 7.26m, Vmin = 7.32m, P = 0.40797003 d | ||||||
HD 115708 | HH | 115708 | 64936 | 13h 18m 37.25s | +26° 21′ 56.8″ | 7.83 | 377 | A2p | α2 CVn variable, Vmax = 7.77m, Vmin = 7.85m, P = 5.07 d | ||||||
HD 108863 | 108863 | 61020 | 12h 30m 20s | +21° 56′ 54″ | 7.89 | 453 | K0 | has a planet (b) | |||||||
HD 116029 | 116029 | 65117 | 13h 20m 40s | +24° 38′ 55″ | 8.04 | 402 | K1III | has a planet (b) | |||||||
HD 106103 | GM | 106103 | 59527 | 12h 12m 24.90s | +27° 22′ 48.3″ | 8.09 | 277.2 | F5V | δ Sct variable, Vmax = 8.06m, Vmin = 8.14m, P = 0.208 d | ||||||
IL Com | IL | 108102 | 60582 | 12h 25m 02.26s | +25° 33′ 38.4″ | 8.14 | 310.2 | F8 | RS CVn variable, ΔV = 0.04m | ||||||
FK Com | FK | 117555 | 65915 | 13h 30m 46.80s | +24° 13′ 57.75″ | 8.17 | 1.2 | 800 | G5II | prototype FK Com variable, Vmax = 8.03m, Vmin = 8.43m, P = 2.4015 d | |||||
12 Com B | 12 | 107701 | 12h 22m 32.30s | +25° 51′ 06.0″ | 8.60 | component of the 12 Com system | |||||||||
IN Com | IN | 112313 | 63087 | 12h 55m 33.75s | +25° 53′ 30.6″ | 8.70 | 2690 | G5III-IV | central star of planetary nebula LoTr 5; ΔV = 0.07m | ||||||
HD 108874 | 108874 | 61028 | 12h 30m 26.88s | +25° 52′ 47.4″ | 8.76 | 4.58 | 224 | G5 | has two planets (b & c) | ||||||
BD +25 2511 | HZ | 12h 29m 40.92s | +24° 31′ 14.7″ | 9.76 | G8:V... | RS CVn variable, Vmax = 9.71m, Vmin = 9.81m | |||||||||
UX Com | UX | 63561 | 13h 01m 33.02s | +28° 37′ 54.1″ | 10.01 | 592 | G7III: | RS CVn variable, Vmax = 9.96m, Vmin = 10.52m, P = 3.642583 d | |||||||
KELT-6 | 13h 03m 55.65s | +30° 38′ 24.28″ | 10.38 | 3.46 | 791 | F8IV | Has two planets (b & c) | ||||||||
RZ Com | RZ | 61414 | 12h 35m 05.06s | +23° 20′ 14.0″ | 10.57 | 614 | G0Vn | W UMa variable, Vmax = 10.42m, Vmin = 11.13m, P = 0.33850604 d | |||||||
Feige 66 | 61602 | 12h 37m 23.52s | +25° 03′ 59.9″ | 10.59 | 530 | Op | subdwarf | ||||||||
SS Com | SS | 12h 49m 39.08s | +18° 42′ 11.9″ | 11.00 | F5 | W UMa variable, Vmax = 10.75m, Vmin = 11.31m, P = 0.412822 d | |||||||||
RW Com | RW | 61243 | 12h 33m 00.28s | +26° 42′ 58.8″ | 11.25 | 278.4 | G2+G2 | W UMa variable, Vmax = 11m, Vmin = 11.7m, P = 0.237346 d | |||||||
CC Com | CC | 12h 12m 06.03s | +22° 31′ 58.7″ | 11.61 | 261.0 | K4/5V | W UMa variable, Vmax = 11.61m, Vmin = 12.20m, P = 0.2206864 d | ||||||||
U Com | U | 61809 | 12h 40m 03.20s | +27° 29′ 56.1″ | 11.76 | 929 | A9 | RR Lyr variable, Vmax = 11.5m, Vmin = 11.97m, P = 0.2927382 d | |||||||
ST Com | ST | 64875 | 13h 17m 51.34s | +20° 46′ 50.8″ | 11.92 | F5 | RR Lyr variable, Vmax = 11.017m, Vmin = 11.823m, P = 0.5989210 d | ||||||||
EK Com | EK | 12h 51m 21.45s | +27° 13′ 47.0″ | 12.02 | K0V | W UMa variable | |||||||||
HZ 43 | 64766 | 13h 16m 21.85s | +29° 05′ 55.4″ | 12.66 | 125.6 | DA.9 + M3Ve | white dwarf/red dwarf binary system | ||||||||
GD 153 | 12h 57m 02.34s | +22° 01′ 52.7″ | 13.35 | DA1.2 | white dwarf | ||||||||||
HZ 21 | 12h 13m 56.25s | +32° 56′ 31.4″ | 14.69 | DA: | white dwarf | ||||||||||
GP Com | GP | 13h 05m 42.43s | +18° 01′ 04.0″ | 15.69 | DBe | interacting binary white dwarf, ΔV = 0.6m, has a planet (b) | |||||||||
LM Com | LM | 12h 26m 30.90s | +30° 38′ 52.7″ | 16.15 | DA1.7 | re-radiating binary system | |||||||||
AL Com | AL | 12h 32m 25.80s | +14° 20′ 42.2″ | 16.2 | WZ Sge variable | ||||||||||
RBS 1223 | 13h 08m 48.7s | +21° 27′ 08″ | 28.6 | neutron star | |||||||||||
GO Com | GO | 12h 56m 37.10s | +26° 36′ 43.7″ | SU UMa variable | |||||||||||
PSR B1237+25 | 12h 39m 40.39s | +24° 53′ 49.9″ | pulsar | ||||||||||||
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Canes Venatici is one of the 88 constellations designated by the International Astronomical Union (IAU). It is a small northern constellation that was created by Johannes Hevelius in the 17th century. Its name is Latin for 'hunting dogs', and the constellation is often depicted in illustrations as representing the dogs of Boötes the Herdsman, a neighboring constellation.
Coma Berenices is an ancient asterism in the northern sky, which has been defined as one of the 88 modern constellations. It is in the direction of the fourth galactic quadrant, between Leo and Boötes, and it is visible in both hemispheres. Its name means "Berenice's Hair" in Latin and refers to Queen Berenice II of Egypt, who sacrificed her long hair as a votive offering. It was introduced to Western astronomy during the third century BC by Conon of Samos and was further corroborated as a constellation by Gerardus Mercator and Tycho Brahe. It is the only modern constellation named for a historic person.
Alpha Comae Berenices is a binary star in the constellation of Coma Berenices, 17.8 parsecs (58 ly) away. It consists of two main sequence stars, each a little hotter and more luminous than the Sun.
NGC 4414 is an unbarred spiral galaxy about 62 million light-years away in the constellation Coma Berenices. It is a flocculent spiral galaxy, with short segments of spiral structure but without the dramatic well-defined spiral arms of a grand design spiral. In 1974 a supernova, SN 1974G, was observed and was the only supernova in this galaxy to be recorded until 7 June 2013 when SN 2013df was discovered at magnitude 14 and 1 January 2021 when SN 2021J was discovered at magnitude 12.
31 Comae Berenices is a yellow giant star in the constellation Coma Berenices. Its apparent magnitude is about 4.9 and slightly variable. It is a rare FK Comae Berenices variable, a variable star that spins rapidly and has large starspots on its surface. It is currently in the Hertzsprung gap and its outer envelope has just begun convection. In 1989 it was given as a spectral standard for the class G0IIIp.
13 Comae Berenices is a probable binary star system in the northern constellation of Coma Berenices. It has an apparent visual magnitude of 5.17, which is bright enough to be faintly visible to the naked eye. With an annual parallax shift of 12.33 mas, it is located around 260 light years from the Sun. It is member of the nearby Coma Star Cluster.
21 Comae Berenices is a variable star in the northern constellation of Coma Berenices. It has the variable star designation UU Comae Berenices, while 21 Comae Berenices is the Flamsteed designation. According to R. H. Allen, English orientalist Thomas Hyde attributed the ancient title Kissīn to this star, a name that comes from a climbing plant – either bindweed or dog rose. This star has a white hue and is just visible to the naked eye with an apparent visual magnitude that fluctuates around 5.47. Based upon parallax measurements, it is located at a distance of approximately 270 light years away from the Sun. It is a single star but is a confirmed physical member of the Melotte 111 open cluster.
17 Comae Berenices is a multiple star system in the northern constellation of Coma Berenices. The brighter component, 17 Com A, is a naked eye star with an apparent visual magnitude of 5.2. It has a faint companion of magnitude 6.6, 17 Com B, positioned at an angular separation of 146.4″ along a position angle of 251°, as of 2018. They are located at a distance of approximately 240 light years from the Sun based on parallax measurements.