List of stars in Canis Major
This is the list of notable stars in the constellation Canis Major, sorted by decreasing brightness.
List
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. | Sp. class | Notes |
| Sirius A, B | α | 9 | 48915 | 32349 | −1.46 | 1.42 | 8.6 | A0m... | Alhabor, Aschere, Canicula, the Dog Star; brightest star, 5th nearest star system; binary | |||
| ε CMa | ε | 21 | 52089 | 33579 | 1.50 | −4.10 | 431 | B2II | Adhara, Aoul al Adzari, Prima Virginum part of Al ʽAdhārā or Al Adzari | |||
| δ CMa | δ | 25 | 54605 | 34444 | 1.83 | −6.87 | 1791 | F8Ia | Wezen, Thalath al Adzari, Tertia Virginum, part of Al ʽAdhārā or Al Adzari; variable star, | |||
| β CMa | β | 2 | 44743 | 30324 | 1.98 | −3.95 | 499 | B1II/III | Mirzam ; β Cep variable, | |||
| η CMa | η | 31 | 58350 | 35904 | 2.45 | −7.51 | 3196 | B5Ia | Aludra, part of Al ʽAdhārā or Al Adzari; α Cyg variable | |||
| ζ CMa | ζ | 1 | 44402 | 30122 | 3.02 | −2.05 | 336 | B2.5V | Furud; spectroscopic binary; suspected variable | |||
| ο2 CMa | ο2 | 24 | 53138 | 33977 | 3.02 | −6.46 | 2567 | B3Ia | Thanih al Adzari, Secunda Virginum, part of Al ʽAdhārā or Al Adzari; α Cyg variable | |||
| σ CMa | σ | 22 | 52877 | 33856 | 3.49 | −4.37 | 1216 | K4III | Unurgunite, irregular variable, | |||
| κ CMa | κ | 13 | 50013 | 32759 | 3.50 | −3.42 | 789 | B1.5IVne | γ Cas variable, | |||
| ο1 CMa | ο1 | 16 | 50877 | 33152 | 3.89 | −5.02 | 1976 | K3Iab | irregular variable, | |||
| ν2 CMa | ν2 | 7 | 47205 | 31592 | 3.95 | 2.46 | 65 | K1III+... | Yějī, has a planet ; suspected variable, | |||
| ω CMa | ω | 28 | 56139 | 35037 | 4.01 | −3.25 | 924 | B2IV/Ve | γ Cas variable, | |||
| θ CMa | θ | 14 | 50778 | 33160 | 4.08 | −0.36 | 252 | K4III | ||||
| γ CMa | γ | 23 | 53244 | 34045 | 4.12 | −1.34 | 402 | B8II | Muliphein; suspected variable | |||
| ξ1 CMa | ξ1 | 4 | 46328 | 31125 | 4.34 | −4.65 | 2050 | B1III | β Cep variable, | |||
| ι CMa | ι | 20 | 51309 | 33347 | 4.36 | −5.51 | 3075 | B3Ib/II | β Cep variable, | |||
| τ CMa | τ | 30 | 57061 | 35415 | 4.37 | −5.59 | 3196 | O9Ib | member of the NGC 2362 star cluster; β Lyr variable | |||
| ν3 CMa | ν3 | 8 | 47442 | 31700 | 4.42 | −1.35 | 464 | K0II/III | ||||
| 27 CMa | 27 | EW | 56014 | 34981 | 4.42 | −4.00 | 1575 | B3IIIe | binary, component A spectroscopic binary, component B γ Cas variable, | |||
| λ CMa | λ | 45813 | 30788 | 4.47 | −1.01 | 406 | B4V | |||||
| ξ2 CMa | ξ2 | 5 | 46933 | 31416 | 4.54 | −0.97 | 412 | A0III | ||||
| π CMa | π | 19 | 51199 | 33302 | 4.66 | 2.33 | 95 | F2IV/V | variable star, | |||
| HD 56618 | 56618 | 35205 | 4.66 | −1.05 | 453 | M2III | suspected variable | |||||
| HD 47667 | 47667 | 31827 | 4.82 | −3.60 | 1575 | K2III | ||||||
| 15 CMa | π1 | 15 | EY | 50707 | 33092 | 4.82 | −3.65 | 1614 | B1IV | β Cep variable, | ||
| 145 G. CMa | 56577 | 35210 | 4.83 | −6.59 | 6269 | K4III | Double star; suspected variable, | |||||
| UW CMa | 29 | UW | 57060 | 35412 | 4.88 | −4.93 | 2991 | O7Ia:fp | β Lyr variable, | |||
| HD 57821 | 57821 | 35727 | 4.94 | −1.06 | 517 | B5II/III | ||||||
| HD 43445 | 43445 | 29735 | 5.00 | −0.30 | 375 | B9V | ||||||
| μ CMa | μ | 18 | 51250 | 33345 | 5.00 | −2.22 | 908 | B9.5V | Isis | |||
| HD 43827 | χ | 43827 | 29895 | 5.15 | −1.05 | 567 | K1III | |||||
| HD 46184 | 46184 | 31084 | 5.16 | 0.05 | 343 | K1III | ||||||
| HD 58343 | FW | 58343 | 35951 | 5.18 | −2.13 | 945 | B2Vne | γ Cas variable, | ||||
| HD 44951 | 44951 | 30457 | 5.21 | −0.34 | 420 | K3III | ||||||
| 10 CMa | 10 | FT | 48917 | 32292 | 5.23 | −4.29 | 2608 | B2V | γ Cas variable, | |||
| HD 47536 | 47536 | 31688 | 5.25 | −0.17 | 396 | K1III | has two planets | |||||
| 11 CMa | ψ | 11 | 49229 | 32492 | 5.28 | −1.19 | 642 | B8/B9III | ||||
| HD 51283 | 51283 | 33316 | 5.28 | −3.82 | 2159 | B2/B3III | suspected variable | |||||
| HD 57146 | 57146 | 35427 | 5.29 | −2.80 | 1353 | G2II | suspected variable | |||||
| HD 49048 | ψ | 49048 | 32411 | 5.30 | −0.13 | 398 | A1IV/V | |||||
| HD 58535 | 58535 | 35957 | 5.35 | −0.79 | 552 | K1III | suspected variable, | |||||
| HD 56342 | 56342 | 35083 | 5.36 | −1.12 | 646 | B2V | suspected variable, | |||||
| HD 58215 | 58215 | 35848 | 5.37 | −0.76 | 549 | K4III | variable star, | |||||
| HD 49662 | 49662 | 32677 | 5.39 | −0.96 | 607 | B7IV | variable star, | |||||
| NO CMa | NO | 58155 | 35795 | 5.40 | −2.81 | 1430 | B3V | Be star | ||||
| FN CMa | FN | 53974 | 34301 | 5.41 | −4.29 | 2835 | B0.5IV | β Cep variable, | ||||
| HD 58286 | 58286 | 35855 | 5.41 | −2.34 | 1156 | B2/B3II/III | ||||||
| HD 51733 | 51733 | 33478 | 5.45 | 2.52 | 126 | F3V | ||||||
| HD 55070 | 55070 | 34624 | 5.46 | −1.01 | 643 | G8III | ||||||
| HD 56405 | 56405 | 35180 | 5.46 | 0.82 | 277 | A1V | suspected variable | |||||
| FR CMa | FR | 44458 | 30214 | 5.48 | −3.07 | 1672 | B1Vpe SB | γ Cas variable, | ||||
| HD 43955 | φ | 43955 | 29941 | 5.51 | −1.91 | 994 | B2/B3V | |||||
| HD 56160 | 56160 | 35044 | 5.58 | 0.97 | 273 | K3III | variable star, | |||||
| HD 52018 | 52018 | 33575 | 5.59 | −1.93 | 1042 | B2V | ||||||
| HD 57478 | 57478 | 35615 | 5.59 | −0.57 | 556 | G8/K0III | ||||||
| NR CMa | NR | 58954 | 36186 | 5.60 | 0.93 | 280 | F2V | δ Sct variable | ||||
| HD 45018 | 45018 | 30436 | 5.61 | −1.04 | 697 | K5III | suspected variable | |||||
| HD 46936 | 46936 | 31362 | 5.62 | −0.25 | 487 | B9V | ||||||
| HR 2501 | HP | 49131 | 32385 | 5.62 | −2.81 | 1583 | B+... | γ Cas and λ Eri variable, | ||||
| LS CMa | LS | 52670 | 33804 | 5.64 | −1.85 | 1028 | B2/B3III/IV | eclipsing binary | ||||
| HD 50644 | 50644 | 33077 | 5.65 | 0.63 | 329 | A9/F0III | ||||||
| FY CMa | FY | 58978 | 36168 | 5.65 | −2.54 | 1417 | B1II | γ Cas variable, | ||||
| LZ CMa | LZ | 54912 | 34579 | 5.69 | −3.06 | 1831 | B2V | β Lyr variable, | ||||
| HD 47946 | 47946 | 31870 | 5.70 | 1.36 | 241 | K1III | ||||||
| R CMa | R | 57167 | 35487 | 5.70 | 2.48 | 144 | F2III/IV | Algol variable, | ||||
| ν1 CMa | ν1 | 6 | 47138 | 31564 | 5.71 | 1.07 | 277 | G8III/F3V... | ||||
| HD 46547 | 46547 | 31190 | 5.73 | −1.32 | 838 | B2V | suspected variable, | |||||
| IY CMa | IY | 45871 | 30840 | 5.74 | −1.27 | 823 | B5IV | Be star; eclipsing binary | ||||
| HD 50123 | HZ | 50123 | 32810 | 5.74 | −0.97 | 718 | B3V | rotating ellipsoidal variable, | ||||
| FV CMa | FV | 54309 | 34360 | 5.75 | −4.04 | 2964 | B2V:nn | γ Cas variable, | ||||
| HD 45765 | 45765 | 30836 | 5.76 | 0.19 | 424 | K0III | ||||||
| HD 49980 | 49980 | 32809 | 5.77 | −2.62 | 1552 | K3III | ||||||
| HD 55589 | 55589 | 34888 | 5.77 | −0.77 | 661 | K0 | ||||||
| HD 44081 | 44081 | 30011 | 5.79 | −2.97 | 1842 | B3II/III | suspected β Cep variable | |||||
| HD 58461 | 58461 | 35998 | 5.79 | 3.08 | 114 | F3V | ||||||
| HD 58612 | 58612 | 36024 | 5.79 | −4.19 | 3228 | B5III | ||||||
| HD 59067 | 59067 | 36251 | 5.79 | −1.66 | 1009 | B8Vv comp VB | γ Cas variable, | |||||
| 17 CMa | π2 | 17 | 51055 | 33248 | 5.80 | −0.54 | 605 | A2V | ||||
| HD 55344 | 55344 | 34758 | 5.84 | −0.04 | 489 | A0IV/V | ||||||
| MZ CMa | MZ | 57615 | 35626 | 5.87 | −0.86 | 723 | M3III | semiregular variable | ||||
| HD 43396 | 43396 | 29679 | 5.88 | −1.39 | 929 | K2III | variable star, | |||||
| 26 CMa | 26 | MM | 55522 | 34798 | 5.91 | −0.80 | 718 | B2IV/V | 53 Per variable | |||
| HD 46189 | 46189 | 31037 | 5.92 | −1.78 | 1128 | B3IV/V | variable star, | |||||
| HD 49095 | 49095 | 32366 | 5.92 | 3.99 | 79 | F7V | ||||||
| HD 47182 | 47182 | 31599 | 5.95 | −0.91 | 769 | K4/K5III | ||||||
| HD 55762 | 55762 | 34914 | 5.96 | −0.90 | 780 | K4III | suspected variable, | |||||
| HD 43544 | 43544 | 29771 | 5.97 | −1.07 | 836 | B2/B3V | suspected variable, | |||||
| HD 43429 | 43429 | 29692 | 5.99 | 1.96 | 208 | K1III | ||||||
| OS CMa | OS | 54764 | 34561 | 6.00 | B1Ib/II | α Cyg variable | ||||||
| HR 2800 | HQ | 57593 | 35611 | 6.00 | −2.71 | 1801 | B3V | Algol variable, | ||||
| HD 47561 | 47561 | 31758 | 6.01 | 0.26 | 460 | A0IV | ||||||
| HD 56578 | 56578 | 35213 | 6.02 | 1.53 | 258 | A5m... | ||||||
| HD 44021 | 44021 | 29993 | 6.04 | −0.73 | 738 | M1III: | suspected variable, | |||||
| HD 49001 | 49001 | 32368 | 6.04 | 0.15 | 492 | K2III | ||||||
| HD 58585 | 58585 | 36017 | 6.04 | −3.90 | 3165 | A6II | ||||||
| HD 43745 | 43745 | 29843 | 6.05 | 3.04 | 130 | F8/G0V | ||||||
| HD 45588 | 45588 | 30711 | 6.05 | 3.67 | 97 | F8/G0V | ||||||
| HD 47827 | 47827 | 31859 | 6.05 | −0.32 | 614 | A0V | ||||||
| HD 50806 | 50806 | 33094 | 6.05 | 3.99 | 84 | G3/G5V | ||||||
| HD 57118 | 57118 | 35442 | 6.11 | F2Ia | suspected variable, | |||||||
| 12 CMa | 12 | HK | 49333 | 32504 | 6.07 | −0.49 | 668 | B7II/III | α2 CVn variable | |||
| HD 53629 | 53629 | 34142 | 6.09 | 1.07 | 330 | K2IIICN... | ||||||
| HD 54173 | 54173 | 34318 | 6.09 | −1.28 | 970 | K2III | variable star, | |||||
| HD 55568 | 55568 | 34782 | 6.10 | 2.71 | 155 | A8III/IV | ||||||
| HD 47366 | 47366 | 31674 | 6.11 | 1.46 | 277 | K1III: | has two planets | |||||
| HD 44996 | 44996 | 30468 | 6.12 | −2.73 | 1918 | B4V | suspected variable | |||||
| GY CMa | GY | 55857 | 34924 | 6.12 | −4.88 | 5175 | B2II | β Cep variable, | ||||
| HD 50643 | 50643 | 33079 | 6.13 | 0.39 | 458 | A3III | ||||||
| HD 46064 | 46064 | 31024 | 6.16 | −1.57 | 1148 | B2III | suspected variable | |||||
| HD 58346 | 58346 | 35920 | 6.20 | −0.31 | 652 | B8/B9V | ||||||
| HD 51823 | 51823 | 33492 | 6.22 | −1.25 | 1019 | B2/B3V | suspected variable | |||||
| HD 50853 | 50853 | 33126 | 6.23 | 0.43 | 472 | A0V | ||||||
| HD 54958 | 54958 | 34617 | 6.23 | 2.74 | 162 | F3V | ||||||
| HD 58439 | 58439 | 35975 | 6.24 | −2.45 | 1781 | A2Ib/II | suspected variable | |||||
| HD 48501 | V350 | 48501 | 32144 | 6.26 | 2.81 | 159 | F2V | γ Dor variable, | ||||
| HD 52273 | 52273 | 33666 | 6.26 | −1.90 | 1399 | B2III | ||||||
| HD 44891 | 44891 | 30420 | 6.27 | −2.15 | 1575 | K2/K3III | ||||||
| HD 52619 | 52619 | 33760 | 6.28 | 2.11 | 222 | F3/F5V | ||||||
| HD 44225 | 44225 | 30062 | 6.29 | −0.61 | 784 | K3III | suspected variable | |||||
| HD 46407 | HR | 46407 | 31205 | 6.30 | 0.88 | 395 | K0III:... | Algol variable, | ||||
| HD 56731 | 56731 | 35241 | 6.30 | 0.46 | 481 | A9II | ||||||
| HD 44956 | 44956 | 30376 | 6.31 | 1.27 | 332 | G8III | ||||||
| KM CMa | KM | 46347 | 31086 | 6.31 | −1.10 | 988 | M4III | semiregular variable | ||||
| HD 49891 | 49891 | 32744 | 6.31 | 0.04 | 584 | A0/A1V | ||||||
| HD 44394 | 44394 | 30190 | 6.32 | −1.70 | 1309 | K5 | ||||||
| HD 45420 | 45420 | 30669 | 6.32 | 0.14 | 560 | K0/K1III | ||||||
| HD 47012 | 47012 | 31469 | 6.32 | 0.33 | 513 | K0III | ||||||
| HD 50093 | 50093 | 32827 | 6.32 | −1.52 | 1203 | B2III/IV | ||||||
| HD 52348 | 52348 | 33703 | 6.32 | −1.50 | 1194 | B3V | ||||||
| HD 55985 | 55985 | 34954 | 6.32 | −1.92 | 1449 | B2III | suspected variable | |||||
| HD 58766 | 58766 | 36045 | 6.32 | −1.09 | 988 | B2/B3III | suspected variable | |||||
| KX CMa | KX | 50648 | 33040 | 6.33 | −0.70 | 830 | M6III | semiregular variable | ||||
| HR 2680 | IL | 54031 | 34248 | 6.34 | −0.69 | 830 | B3V | Algol and 53 Per variable, | ||||
| HD 55856 | 55856 | 34940 | 6.34 | −2.08 | 1575 | B2IV | suspected variable | |||||
| HD 56341 | 56341 | 35132 | 6.34 | −0.89 | 911 | A0V | ||||||
| V415 CMa | V415 | 47247 | 31593 | 6.35 | −0.46 | 751 | B3V | Algol variable, | ||||
| HD 51411 | 51411 | 33330 | 6.36 | −1.83 | 1417 | B3V | Be star, | |||||
| HD 51925 | 51925 | 33532 | 6.36 | −1.89 | 1455 | B2V | suspected variable | |||||
| V352 CMa | V352 | 43162 | 29568 | 6.37 | 5.26 | 54 | G5V | BY Dra variable, | ||||
| HD 45184 | 45184 | 30503 | 6.37 | 4.65 | 72 | G2V | has a planet | |||||
| HD 46602 | 46602 | 31266 | 6.39 | 1.12 | 368 | K0III+... | ||||||
| HD 52140 | 52140 | 33591 | 6.41 | −0.46 | 771 | B3V | ||||||
| HD 48938 | 48938 | 32322 | 6.43 | 4.31 | 87 | F7V | ||||||
| HD 46037 | 46037 | 30988 | 6.44 | −1.49 | 1259 | M0/M1III | suspected variable | |||||
| HD 56876 | 56876 | 35326 | 6.45 | −0.80 | 921 | B5Vn | ||||||
| HD 47579 | 47579 | 31736 | 6.48 | −0.07 | 667 | A2V | ||||||
| HD 53975 | 53975 | 34297 | 6.48 | −4.42 | 4939 | B7Iab... | ||||||
| HD 44379 | 44379 | 30141 | 6.49 | 0.03 | 639 | K0III | ||||||
| HD 42927 | IP | 42927 | 29488 | 6.49 | 908 | B5II/III | rotating ellipsoidal variable, | |||||
| FU CMa | FU | 52437 | 33721 | 6.51 | 2100 | B3Vnn | γ Cas variable, | |||||
| W CMa | W | 54361 | 34413 | 6.56 | 8400 | C | semiregular variable, | |||||
| GU CMa | GU | 52721 | 33868 | 6.59 | 1450 | B2Vne | β Lyr variable, | |||||
| HR 2724 | HN | 55595 | 34814 | 6.61 | 805 | A5IV-V | δ Sct variable, | |||||
| EZ CMa | EZ | 50896 | 33165 | 6.91 | 4500 | WN4-s | Wolf–Rayet star, | |||||
| HD 47186 | 47186 | 31540 | 7.8 | 4.9 | 123 | G6V | has two planets | |||||
| VY CMa | VY | 58061 | 35793 | 7.95 | −9.4 | 3900 | M2.5–M5e Ia | One of the largest known stars; semiregular variable or irregular variable, | ||||
| GZ CMa | GZ | 56429 | 35187 | 7.97 | 1290 | A0III/IV | Algol variable, | |||||
| HD 45364 | 45364 | 30579 | 8.07 | 5.50 | 106 | G8V | has two planets | |||||
| FZ CMa | FZ | 52942 | 33953 | 8.14 | 1350 | B2IVn | Algol variable, | |||||
| HD 45677 | FS | 45677 | 30800 | 8.50 | 908 | Bpshe | prototype FS CMa variable, | |||||
| Z CMa | Z | 53179 | 34042 | 8.80 | 2630 | Bpe | EXor and FU Ori variable, | |||||
| HD 43197 | 43197 | 29550 | 8.95 | 5.25 | 179 | G9IV-V | Amadioha, has a planet | |||||
| SW CMa | SW | 54520 | 34431 | 9.16 | 2230 | A3IV | Algol variable, | |||||
| WASP-101 | 10.3 | F6 | has a transiting planet | |||||||||
| HD 56925 | 56925 | 35378 | 11.40 | 3700 | WN4-s | Wolf–Rayet star at center of NGC 2359 | ||||||
| DZ CMa | DZ | 11.6 | G0 | double-mode Cepheid variable, | ||||||||
| HATS-4 | 13.5 | 1370 | has a planet | |||||||||
| EUVE J0720-317 | IN | 14.64 | DA.9 | re-radiating binary system, | ||||||||
| RX J0720.4-3125 | 26.6 | 1174 | one of the nearest neutron stars | |||||||||
| PSR B0628-28 | pulsar | |||||||||||
| CX CMa | 9.6 | 6000-7000 | B5V | eclipsing binary, | ||||||||
| NN CMa | NN | 58011 | 35769 | 7.19 | -12.85 | 3397 | B1/B2Ib/IIn |
; Notes