List of stars in Coma Berenices

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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 β431147106439413h 11m 52.92s+27° 52 33.74.264.4230G0Vsuspected BY Dra variable, ΔV = 0.02m
α Com A α421143786424113h 09m 59.55s+17° 31 44.84.323.5447F5VDiadem, Al Dafirah; double star; suspected Algol variable, Vmax = 4.29m, Vmin = 4.35m, P = 9485.68 d
γ Com γ151083816074212h 26m 56.33s+28° 16 07.04.350.76170K2IIICN+...
11 Com 111073836020212h 20m 43.09s+17° 47 33.64.72−0.50361G8III
36 Com 361127696335512h 58m 55.47s+17° 24 33.74.76−0.05299M0IIIsuspected variable, Vmax = 4.74m, Vmin = 4.82m
12 Com A 121077006035112h 22m 30.32s+25° 50 46.34.780.16273F8:p...double star; suspected variable, Vmax = 4.78m, Vmin = 4.89m
23 Com 231094856139412h 34m 51.12s+22° 37 45.14.80−0.44365A0IV
41 Com 411139966402213h 07m 10.71s+27° 37 29.74.80−0.04303K5IIIhas a planet (b)
35 Com 351120336288612h 53m 17.77s+21° 14 42.14.89−0.10324G8III
37 Com 37LU1129896346213h 00m 16.49s+30° 47 06.14.90−2.32898K1IIIp RS CVn variable, ΔV = 0.15m
14 Com 141082836069712h 26m 24.07s+27° 16 05.74.920.30273F0p
7 Com 71067145984712h 16m 20.56s+23° 56 43.54.930.52248K0III
31 Com 31LS1118126276312h 51m 41.93s+27° 32 26.64.930.06307G0IIIPolaris Galacticum Borealis, Lángjiāng (郎將), [1] FK Com variable, Vmax = 4.87m, Vmin = 4.97m
16 Com 161083826074612h 26m 59.30s+26° 49 32.64.980.29282A4V
HD 106760 1067605985612h 16m 30.17s+33° 03 42.54.990.13306K1IIIsuspected variable
24 Com A 241095116141812h 35m 07.76s+18° 22 37.25.03−1.34614K2IIIdouble star; suspected variable, Vmax = 4.98m, Vmin = 5.06m
6 Com 61066615981912h 16m 00.23s+14° 53 56.95.091.18198A3V
27 Com 271110676235612h 46m 38.75s+16° 34 39.55.120.15322K3III
13 Com 13GN1079666051412h 24m 18.54s+26° 05 55.05.170.47284A3V α² Cvn variable, Vmax = 5.15m, Vmin = 5.18m
α Com B α4211437913h 09m 59.30s+17° 31 46.05.22component of the α Com system
17 Com 17AI1086626090412h 28m 54.72s+25° 54 46.45.290.70270A0pα² Cvn and δ Sct variable, Vmax = 5.23m, Vmin = 5.4m, P = 5.0633 d
21 Com 21UU1089456107112h 31m 00.57s+24° 34 01.95.440.57311A2pvarKissīn; [2] α² CVn and δ Sct variable, Vmax = 5.41m, Vmin = 5.46m
18 Com 181087226094112h 29m 27.05s+24° 06 32.15.471.36216F5III
26 Com 261100246172412h 39m 07.36s+21° 03 45.35.490.77286G9III
HD 107325 1073256017012h 20m 19.72s+26° 37 11.15.522.11157K2III-IVsuspected variable, Vmax = 5.50m, Vmin = 5.56m
FS Com 40FS1138666395013h 06m 22.58s+22° 36 58.65.53−0.69572M5III semiregular variable, Vmax = 5.3m, Vmin = 6.1m, P = 58 d
5 Com 51060575950112h 12m 09.30s+20° 32 31.65.60−0.26484K0II-III
4 Com 41059815946812h 11m 51.20s+25° 52 13.35.66−1.22774K4IIIvariable star, ΔV = 0.005m, P = 6.71096 d
20 Com 201087656095712h 29m 43.22s+20° 53 46.35.681.22254A3V
25 Com 251097426157112h 36m 58.35s+17° 05 22.55.70−0.31518K5III
HD 106887 1068875992312h 17m 30.60s+28° 56 13.65.712.07174A4m
29 Com 291113976254112h 48m 54.20s+14° 07 21.55.710.25402A1V36 Virginis
HD 116706 1167066546613h 25m 06.68s+23° 51 16.05.751.29254A3IVsuspected variable
30 Com 301114696257612h 49m 17.51s+27° 33 08.45.760.75327A2V
HD 109519 1095196142012h 35m 08.15s+21° 52 53.25.86−0.65652K1III
2 Com 21048275885812h 04m 16.58s+21° 27 33.05.890.68359F0IV-V
HD 114326 1143266422613h 09m 47.89s+16° 50 55.15.91−0.85733K5IIIsuspected variable
38 Com 381130956353313h 01m 09.62s+17° 07 23.55.970.52400K0III
39 Com 391138486394813h 06m 21.28s+21° 09 12.66.002.51163F4V
HD 105805 1058055936412h 10m 46.10s+27° 16 53.56.011.14308A4Vnsuspected variable, Vmax = 6.00m, Vmin = 6.04m
HD 108123 1081236059912h 25m 15.07s+23° 55 34.76.030.11497K0III
HD 114889 1148896449613h 13m 12.54s+18° 43 37.76.101.30297G8III
HD 117876 1178766608613h 32m 48.17s+24° 20 50.06.110.32470G8III
HD 107326 1073266016812h 20m 17.84s+26° 00 06.66.162.25198F0IVsuspected variable, Vmax = 6.12m, Vmin = 6.16m
HD 113022 1130226349713h 00m 38.86s+18° 22 22.36.203.14133F6Vs
HD 114092 1140926407713h 07m 53.66s+27° 33 22.06.200.82389K4III
HD 107655 1076556032712h 22m 10.86s+24° 46 26.06.211.20327A0V
HD 107054 1070546001812h 18m 31.57s+30° 14 57.66.232.51181A9.5III
8 Com 81071686008712h 19m 19.20s+23° 02 04.96.261.55285A8m
22 Com 221093076129512h 33m 34.23s+24° 16 58.86.281.15346A4V
HD 111893 1118936282512h 52m 27.52s+16° 07 21.16.291.05364A7V
LW Com LW1113956252312h 48m 47.26s+24° 50 25.76.315.1256G7VBY Dra variable, ΔV = 0.10m, P = 15.80 d
HD 114724 1147246441713h 12m 08.42s+24° 15 29.36.310.32513K1III
HD 107398 1073986019712h 20m 41.37s+27° 03 17.46.321.49301F3V + F3Vsuspected variable
32 Com 321118626280712h 52m 12.26s+17° 04 26.26.32−2.431831M0IIIvariable star, ΔV = 0.011m, P = 52.08333 d
HD 106926 1069265994112h 17m 44.24s+15° 08 41.36.360.30532K4III
9 Com 91072136009812h 19m 29.66s+28° 09 26.06.382.90162F8Vs
HD 109996 1099966171912h 39m 02.21s+22° 39 34.46.391.15364K1III
3 Com 31057785935212h 10m 31.64s+16° 48 33.46.40−0.81903A4Vsuspected variable
HD 108007 1080076052512h 24m 26.81s+25° 34 56.76.411.46319F0V
HD 112060 1120606290412h 53m 32.20s+19° 28 53.46.423.20144G5IV
HD 111591 1115916265312h 50m 17.23s+22° 51 48.86.430.80435K0IIIhas a planet (b)
HD 115365 1153656477913h 16m 32.33s+19° 47 06.86.431.76280F0V
FM Com FM1071316006612h 19m 02.03s+26° 00 30.16.442.03248Amδ Sct variable, Vmax = 6.4m, Vmin = 6.48m, P = 0.0551 d
HD 115319 1153196475113h 16m 14.35s+19° 03 06.26.461.59307G8III
HD 106022 1060225948912h 12m 00.97s+28° 32 11.36.471.94263F5V
HD 107415 1074156021012h 20m 48.75s+15° 32 27.56.470.64479K0
28 Com 281113086247812h 48m 14.36s+13° 33 11.26.470.99407A1V
HD 115404 1154046479713h 16m 50.67s+17° 01 04.16.496.2437K2V
1 Com 11044525866112h 01m 44.30s+22° 05 39.66.570.61507G0II
24 Com B 241095106141512h 35m 06.35s+18° 22 37.36.57−2.962629A7mcomponent of the 24 Com system; suspected variable, Vmax = 6.55m, Vmin = 6.59m
17 Com 171086516089112h 28m 44.58s+25° 53 57.76.632.14258A0p
10 Com 101072766012312h 19m 50.63s+28° 27 51.86.641.85296Am
HD 112127 1121276294412h 53m 55.75s+26° 46 48.06.88345K3III carbon star
33 Com 331118926281912h 52m 22.83s+17° 06 30.56.931.50397F8
HD 114762 1147626442613h 12m 19.74s+17° 31 01.67.304.27132F9Vhas a planet (b)
HD 107146 1071466007412h 19m 06.50s+16° 32 53.97.0793G2Vhas a debris disk
KR Com KR1159556506913h 20m 15.78s+17° 45 57.07.26273.7F5 W UMa variable, Vmax = 7.26m, Vmin = 7.32m, P = 0.40797003 d
HD 115708 HH1157086493613h 18m 37.25s+26° 21 56.87.83377A2pα2 CVn variable, Vmax = 7.77m, Vmin = 7.85m, P = 5.07 d
HD 108863 1088636102012h 30m 20s+21° 56 547.89453K0has a planet (b)
HD 116029 1160296511713h 20m 40s+24° 38 558.04402K1IIIhas a planet (b)
HD 106103 GM1061035952712h 12m 24.90s+27° 22 48.38.09277.2F5Vδ Sct variable, Vmax = 8.06m, Vmin = 8.14m, P = 0.208 d
IL Com IL1081026058212h 25m 02.26s+25° 33 38.48.14310.2F8RS CVn variable, ΔV = 0.04m
FK Com FK1175556591513h 30m 46.80s+24° 13 57.758.171.2800G5IIprototype FK Com variable, Vmax = 8.03m, Vmin = 8.43m, P = 2.4015 d
12 Com B 1210770112h 22m 32.30s+25° 51 06.08.60component of the 12 Com system
IN Com IN1123136308712h 55m 33.75s+25° 53 30.68.702690G5III-IVcentral star of planetary nebula LoTr 5; ΔV = 0.07m
HD 108874 1088746102812h 30m 26.88s+25° 52 47.48.764.58224G5has two planets (b & c)
BD +25 2511 HZ12h 29m 40.92s+24° 31 14.79.76G8:V...RS CVn variable, Vmax = 9.71m, Vmin = 9.81m
UX Com UX6356113h 01m 33.02s+28° 37 54.110.01592G7III:RS CVn variable, Vmax = 9.96m, Vmin = 10.52m, P = 3.642583 d
KELT-6 13h 03m 55.65s+30° 38 24.2810.383.46791F8IVHas two planets (b & c)
RZ Com RZ6141412h 35m 05.06s+23° 20 14.010.57614G0VnW UMa variable, Vmax = 10.42m, Vmin = 11.13m, P = 0.33850604 d
Feige 66 6160212h 37m 23.52s+25° 03 59.910.59530Op subdwarf
SS Com SS12h 49m 39.08s+18° 42 11.911.00F5W UMa variable, Vmax = 10.75m, Vmin = 11.31m, P = 0.412822 d
RW Com RW6124312h 33m 00.28s+26° 42 58.811.25278.4G2+G2W UMa variable, Vmax = 11m, Vmin = 11.7m, P = 0.237346 d
CC Com CC12h 12m 06.03s+22° 31 58.711.61261.0K4/5VW UMa variable, Vmax = 11.61m, Vmin = 12.20m, P = 0.2206864 d
U Com U6180912h 40m 03.20s+27° 29 56.111.76929A9 RR Lyr variable, Vmax = 11.5m, Vmin = 11.97m, P = 0.2927382 d
ST Com ST6487513h 17m 51.34s+20° 46 50.811.92F5RR Lyr variable, Vmax = 11.017m, Vmin = 11.823m, P = 0.5989210 d
EK Com EK12h 51m 21.45s+27° 13 47.012.02K0VW UMa variable
HZ 43 6476613h 16m 21.85s+29° 05 55.412.66125.6DA.9 + M3Vewhite dwarf/red dwarf binary system
GD 153 12h 57m 02.34s+22° 01 52.713.35DA1.2 white dwarf
HZ 21 12h 13m 56.25s+32° 56 31.414.69DA:white dwarf
GP Com GP13h 05m 42.43s+18° 01 04.015.69DBe interacting binary white dwarf, ΔV = 0.6m, has a planet (b)
LM Com LM12h 26m 30.90s+30° 38 52.716.15DA1.7re-radiating binary system
AL Com AL12h 32m 25.80s+14° 20 42.216.2 WZ Sge variable
RBS 1223 13h 08m 48.7s+21° 27 0828.6 neutron star
GO Com GO12h 56m 37.10s+26° 36 43.7 SU UMa variable
PSR B1237+25 12h 39m 40.39s+24° 53 49.9 pulsar
Table legend:

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Coma Berenices Constellation in the northern hemisphere

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 Star in the constellation Coma Berenices

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 Flocculent unbarred spiral galaxy in the constellation Coma Berenices

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 Star in the constellation Coma Berenices

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 Star in the constellation Coma Berenices

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.

References