List of stars in Camelopardalis explained

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

NameBFVarHDHIPRADecvis.
mag.
abs.
mag.
Dist. (ly)Sp. classNotes
β 10 31910 23522 4.03 −3.40 997 G0Ib
CS 21291 16228 4.21 −6.39 4289 B9Ia α Cyg variable,
α 9 30614 22783 4.26 −7.38 6936 O9.5Ia SB: Shǎowèi (少衛)[1]
BE 23475 17884 4.39 −2.97 964 M1III irregular variable,
7 31278 23040 4.43 −0.88 376 A1V
CE 21389 16281 4.55 −4.85 2470 A0Ia SB: α Cyg variable,
49878 33694 4.55 0.76 187 K4III
γ 23401 17959 4.59 −0.47 335 A2IVn
BK 20336 15520 4.74 −2.21 801 B2.5Vne γ Cas variable,
42818 29997 4.76 1.10 176 A0Vn
23089 17587 4.78 −2.17 799 A3V...
VZ 55966 36547 4.92 −0.89 473 M4IIIa semiregular variable,
24479 18505 4.95 −0.13 338 B9.5V
24480 18488 4.99 −3.78 1852 K3I-II
25291 19018 5.00 −3.63 1734 F0II
BD 22649 17296 5.06 −0.95 520 S5.3 SB: a symbiotic star; irregular variable,
3 29317 21727 5.07 −0.84 495 K0III SB
33564 25110 5.08 3.47 68 F6V has a planet (b)
21447 16292 5.09 1.25 191 A1V
43 49340 33104 5.11 −2.32 1000 B7III
CQ 20797 15890 5.13 −2.79 1249 M0II irregular variable,
42 48879 32864 5.14 −1.98 867 B4IV
106112 59504 5.14 2.50 110 A5m rotating ellipsoidal variable,
26764 19949 5.20 0.03 353 A2Vn
31 TU 39220 27971 5.20 −0.27 405 A2V TU Cam; eclipsing spectroscopic binary
11 BV 32343 23734 5.22 −1.35 671 B2.5Ve BV Cam; γ Cas variable, ; double star with 12 Cam
16 34787 25197 5.24 0.15 340 A0Vn
90089 51502 5.25 3.59 70 F2V
27022 20266 5.26 0.22 333 G5III
4 30121 22287 5.29 1.81 162 A3m
37 41597 29246 5.35 0.20 349 G8III
2 29316 21730 5.36 0.71 277 A8V multiple star
36 41927 29490 5.36 −1.11 642 K2II-III
40 42633 29730 5.37 −0.55 498 K3III
64307 39117 5.37 −1.29 700 K3III
Σ 1694 A 112028 62572 5.38 0.54 303 A1IIIsh
64486 39538 5.39 0.36 330 B9IVs
23277 17854 5.40 0.40 325 A2m
27245 20376 5.40 −0.18 427 M0III
17 35583 25769 5.43 −1.85 931 M1III
BN 32650 24254 5.44 0.14 374 B9p Si α2 CVn variable,
46588 32439 5.44 4.18 58 F7V
30442 22626 5.47 −0.46 499 M2III
5 30958 22854 5.52 −1.02 661 B9.5V
89571 51384 5.52 2.47 133 F0IV
68375 40793 5.55 0.79 292 G8III
37289 26882 5.62 0.96 279 K5III
58425 36528 5.63 −0.08 453 K2III
34255 24914 5.64 −3.27 1976 K4Iab:
26670 19968 5.69 0.20 409 B5Vn
50885 33827 5.69 −0.04 457 K4III
26755 19983 5.72 1.18 263 K1III
22764 17342 5.74 −3.41 2203 K3.5IIIb + K3V
117566 65595 5.74 0.98 292 G2.5IIIb
31134 22936 5.75 −0.08 478 A2Vs
45866 31940 5.75 −0.50 579 K5III
1 DL 28446 21148 5.78 B0III SB β Cep variable,
104985 58952 5.78 0.74 333 G9III Tonatiuh,[2] has a planet (b)
23005 17585 5.79 2.07 181 F0IV
24141 18217 5.80 2.21 170 A5m
33541 24732 5.81 0.60 359 A0V
23523 17891 5.82 1.57 231 A5Vn
25274 19129 5.88 −0.53 623 K2III
46509 31946 5.88 −0.66 663 K0III
27322 20380 5.91 1.02 310 A3V
28780 21452 5.91 0.24 443 A1V
Σ 1694 B 112014 62561 5.92 1.75 222 A0V spectroscopic binary
120565 66878 5.92 0.68 364 G9III
26 38091 27249 5.93 2.07 193 A4Vn
51 62066 37949 5.93 0.89 332 K2III:
28204 21247 5.94 0.65 373 A8m
29678 22361 5.96 2.66 149 A9IV
21819 16599 5.98 1.82 222 A3V
32356 23766 6.00 −0.19 563 K5II
105943 59384 6.00 −1.64 1101 K5III:
53 AX 65339 39261 6.02 1.05 321 A3Vp... AX Cam; α2 CVn variable, ; spectroscopic binary
31662 23380 6.03 3.19 120 F4V + M0V
44472 30794 6.03 −0.12 553 A4V + G1V
26076 19730 6.05 0.80 365 K1III
31312 23442 6.05 −0.37 628 K5III
24 37601 26942 6.05 2.11 200 K0III
26553 19823 6.06 −1.96 1309 G2-3II
12 BM 32357 23743 6.08 −0.33 625 K0III BM Cam; RS CVn variable, ; double star with 11 Cam
23383 17707 6.09 0.48 431 B9Vnn
8 31579 23216 6.09 −0.77 767 K4III
65448 39340 6.09 0.07 522 G1III Spectroscopic binary
31590 23617 6.10 0.02 537 A1V
99945 56253 6.12 2.24 195 A2m suspected variable
15 DV 34233 24836 6.13 −1.02 879 B5V DV Cam; Algol variable,
21427 16303 6.14 1.07 337 A0V + A2V
25425 19177 6.14 0.41 457 A4Vm
30 38831 27731 6.14 0.02 545 A0Vs
33618 24479 6.15 1.28 307 K2III-IV
19 Cam 19 36570 26408 6.15 0.86 372 A0V
72582 42484 6.16 0.97 355 G7III
33266 24313 6.17 0.34 477 A2III
23 37638 27046 6.17 1.23 318 G5III:
27402 20456 6.18 0.86 378 A4V + F6V
38284 27472 6.18 0.67 412 A4V
36384 26638 6.19 −0.06 579 M0III
31675 23484 6.20 3.97 91 F6V:
31563 23582 6.21 −1.84 1331 M0III
FR 104216 58545 6.21 −0.79 819 M2III irregular variable,
38645 27795 6.22 0.70 415 G9III
39429 28205 6.24 0.66 427 K3III
25948 19400 6.25 2.87 155 F5V
115337 64437 6.25 −0.37 686 K0Ib
36496 26410 6.26 1.76 259 A8Vn Double star
45947 31703 6.26 3.51 116 F4V
104904 58874 6.27 1.86 249 F9III
27855 20772 6.28 −0.54 755 A0III + A9V?
40055 28831 6.28 −0.44 720 K4III
67934 41208 6.28 −0.31 679 A2Vn
KZ 22316 16974 6.29 0.13 557 B9p HR 1094; α² CVn variable,
25877 19412 6.29 −1.30 1072 G8II
55075 36019 6.30 −0.73 832 A0III
76990 45421 6.30 1.53 294 F0IV
23662 18067 6.31 −0.70 821 B9IVp
24164 18438 6.31 2.42 196 A5Vm
25602 19172 6.31 1.36 319 K0III-IV
71973 42249 6.31 1.69 273 A5IV-V + G6V double star
86321 49688 6.31 −0.85 883 K5III
30144 22300 6.32 2.78 166 F2V
40827 28829 6.32 0.52 471 K0+IIICN1-
26101 19673 6.33 0.96 387 K1III
111112 62170 6.33 0.57 462 A5m
30085 22508 6.36 −0.13 647 B9III
32781 24440 6.36 0.81 421 A0III:
54070 34956 6.36 0.94 396 K0.5III
47 56820 35735 6.36 2.13 229 A8Vm
21794 16602 6.37 2.09 234 F7V double star
32715 24017 6.37 3.38 129 F3V:
77246 45097 6.37 1.93 252 F2IV
34200 24955 6.39 1.04 384 G6III
30752 22720 6.40 0.37 523 A2V
69054 41011 6.40 0.63 466 K0III + G2V
20104 15309 6.41 0.10 596 A2V + A4V Double star
40956 28951 6.42 0.90 414 G9III has a planet (b)
79517 45764 6.42 1.14 370 G8III
21903 16712 6.43 2.69 183 F3V
32518 24003 6.44 1.09 383 K1III Mago,[3] has a planet (b)
18 36066 25973 6.44 3.23 143 F8V
21769 16587 6.45 −0.40 763 A4III
65299 40559 6.45 0.24 568 A3IV
23594 17858 6.46 0.40 531 B9V
29329 22152 6.46 3.92 105 F7V
118686 66251 6.46 −1.03 1025 K5III:
57742 36211 6.47 −0.72 893 B9V
34450 25322 6.48 −1.45 1254 M0.5IIIbBa0.5
39 41782 29348 6.48 −1.47 1268 M2III
21203 16177 6.49 −0.61 858 B9V + A1
25225 19222 6.49 1.00 409 G8III
14 33296 24348 6.49 1.91 268 A7Vn
38058 27346 6.49 0.64 482 G9III
52030 34238 6.49 −0.58 847 K5III has an unconfirmed planet (b)
40568 28656 6.50 0.31 565 G7-8III
49 BC 62140 37934 6.50 1.95 265 F0p SrEu BC Cam; α2 CVn variable,
29 38618 27592 6.53 0.88 441 A4IV-V
HD 44385 44385 31231 6.60 698 K3III has a planet (b)
6 31189 22994 6.63 0.39 874 K4III
24064 18451 6.75 -0.36 862 K4III has a planet (b)
28 38129 27283 6.79 0.39 622 A7V
22 37070 26587 7.03 3.14 196 F5
20 36770 26426 7.45 1.37 1,163 G8II-III [4]
35759 25883 7.74 3.44 236 F9/G0V has a planet (b)
29021 21571 7.76 100 G5V has a planet (b)
10.8 17.6

See also

Sources

Notes and References

  1. AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 11 日
  2. http://www.iau.org/news/pressreleases/detail/iau1514/ Final Results of NameExoWorlds Public Vote Released
  3. Web site: Germany. NameExoWorlds. en. 2019-12-23.
  4. SIMBAD, 20 Camelopardalis (accessed 29 July 2012)