# List of stars in Canis Minor

This is the list of notable stars in the constellation Canis Minor, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| Procyon | α | 10 | | 61421 | 37279 | 07$^h$ 39$^m$ 18.54$^s$ | +05° 13′ 39.0″ | 0.34 | 2.65 | 11 | F5IV-V | Antecanis, Al Shira, Elgomaisa; 7th brightest star, 13th nearest star system; binary; suspected variable, V$_{max}$ = 0.34$^m$, V$_{min}$ = 0.41$^m$ |
| β CMi | β | 3 | | 58715 | 36188 | 07$^h$ 27$^m$ 09.07$^s$ | +08° 17′ 21.9″ | 2.89 | −0.70 | 170 | B8Vvar | Gomeisa; γ Cas variable, V$_{max}$ = 2.84$^m$, V$_{min}$ = 2.92$^m$ |
| γ CMi | γ | 4 | | 58972 | 36284 | 07$^h$ 28$^m$ 09.83$^s$ | +08° 55′ 31.8″ | 4.33 | −1.10 | 318 | K3III SB | semiregular variable, V$_{max}$ = 4.30$^m$, V$_{min}$ = 4.34$^m$, P = 55 d |
| HD 66141 | (λ) | (13) | | 66141 | 39311 | 08$^h$ 02$^m$ 15.95$^s$ | +02° 20′ 03.5″ | 4.39 | −0.13 | 261 | K2III | suspected variable; has a planet (b) |
| 6 CMi | | 6 | | 59294 | 36425 | 07$^h$ 29$^m$ 47.78$^s$ | +12° 00′ 23.8″ | 4.55 | −1.63 | 560 | K2III | suspected variable, V$_{max}$ = 4.48$^m$, V$_{min}$ = 4.55$^m$ |
| ε CMi | ε | 2 | | 58367 | 36041 | 07$^h$ 25$^m$ 38.90$^s$ | +09° 16′ 34.0″ | 4.99 | −2.42 | 988 | G8III | |
| ζ CMi | ζ | 13 | | 63975 | 38373 | 07$^h$ 51$^m$ 42.00$^s$ | +01° 46′ 00.8″ | 5.12 | −0.43 | 420 | B8II | |
| η CMi | η | 5 | | 58923 | 36265 | 07$^h$ 28$^m$ 02.08$^s$ | +06° 56′ 31.5″ | 5.22 | 0.06 | 351 | F0III | |
| δ$^1$ CMi | δ$^1$ | 7 | | 59881 | 36641 | 07$^h$ 32$^m$ 05.95$^s$ | +01° 54′ 52.1″ | 5.24 | −1.67 | 787 | F0III | |
| 11 CMi | | 11 | | 62832 | 37921 | 07$^h$ 46$^m$ 16.22$^s$ | +10° 46′ 05.9″ | 5.25 | 0.34 | 312 | A1Vnn | |
| 14 CMi | | 14 | | 65345 | 38962 | 07$^h$ 58$^m$ 20.75$^s$ | +02° 13′ 28.3″ | 5.30 | 0.75 | 264 | K0III | |
| HD 55751 | | | | 55751 | 34987 | 07$^h$ 14$^m$ 20.07$^s$ | +03° 06′ 41.1″ | 5.36 | −1.45 | 749 | K0III | |
| 1 CMi | | 1 | | 58187 | 35987 | 07$^h$ 24$^m$ 58.19$^s$ | +11° 40′ 10.4″ | 5.37 | 0.43 | 317 | A5IV | |
| δ$^2$ CMi | δ$^2$ | 8 | | 60111 | 36723 | 07$^h$ 33$^m$ 11.68$^s$ | +03° 17′ 25.0″ | 5.59 | 2.44 | 139 | F2V | |
| HD 65900 | | | | 65900 | 39213 | 08$^h$ 01$^m$ 13.91$^s$ | +04° 52′ 47.2″ | 5.65 | 0.52 | 346 | A1V | |
| HD 55730 | | | | 55730 | 35005 | 07$^h$ 14$^m$ 32.65$^s$ | +12° 06′ 57.1″ | 5.71 | 0.68 | 331 | G6III | |
| HD 54079 | | | | 54079 | 34387 | 07$^h$ 07$^m$ 49.48$^s$ | +07° 28′ 16.7″ | 5.74 | −0.47 | 568 | K0III: | |
| HD 56031 | | | | 56031 | 35120 | 07$^h$ 15$^m$ 39.42$^s$ | +07° 58′ 39.9″ | 5.78 | −0.56 | 604 | M4III | semiregular variable, ΔV = 0.08$^m$ |
| δ$^3$ CMi | δ$^3$ | 9 | | 60357 | 36812 | 07$^h$ 34$^m$ 15.89$^s$ | +03° 22′ 18.3″ | 5.83 | −0.75 | 676 | A0Vnn | |
| HD 64685 | | | | 64685 | 38712 | 07$^h$ 55$^m$ 31.44$^s$ | +08° 51′ 47.0″ | 5.86 | 2.95 | 124 | F2IV | |
| HD 60803 | | | | 60803 | 37031 | 07$^h$ 36$^m$ 34.77$^s$ | +05° 51′ 43.6″ | 5.89 | 2.69 | 142 | G0V | binary |
| HD 56989 | | | | 56989 | 35476 | 07$^h$ 19$^m$ 22.37$^s$ | +02° 44′ 26.6″ | 5.90 | −0.11 | 520 | G9III | |
| HD 57006 | | | | 57006 | 35509 | 07$^h$ 19$^m$ 47.61$^s$ | +07° 08′ 35.1″ | 5.91 | 2.04 | 193 | F8IV | |
| HD 61887 | | | | 61887 | 37478 | 07$^h$ 41$^m$ 35.16$^s$ | +03° 37′ 29.4″ | 5.95 | 0.00 | 504 | A0V | |
| HD 57608 | | | | 57608 | 35712 | 07$^h$ 22$^m$ 03.48$^s$ | +00° 10′ 37.7″ | 5.99 | −5.08 | 5344 | B8III | |
| HD 61563 | | | | 61563 | | 07$^h$ 40$^m$ 06.99$^s$ | +05° 13′ 52.2″ | 6.07 | -0.26 | 670 | A0IV+A0IV | binary |
| HD 65066 | | | | 65066 | 38868 | 07$^h$ 57$^m$ 15.88$^s$ | +08° 38′ 28.6″ | 6.03 | 1.25 | 294 | K0III | |
| HD 55111 | | | | 55111 | 34768 | 07$^h$ 11$^m$ 51.39$^s$ | +05° 39′ 17.0″ | 6.07 | −0.83 | 782 | A1V | |
| HD 55184 | | | | 55184 | 34789 | 07$^h$ 12$^m$ 07.50$^s$ | +05° 28′ 27.7″ | 6.15 | −0.67 | 753 | K0III | |
| HD 64938 | | | | 64938 | 38794 | 07$^h$ 56$^m$ 23.91$^s$ | +04° 29′ 08.1″ | 6.16 | −0.91 | 845 | G8III | |
| HD 62264 | | | | 62264 | 37614 | 07$^h$ 43$^m$ 05.42$^s$ | +00° 11′ 21.7″ | 6.17 | 0.46 | 453 | K0III | |
| HD 63799 | | | | 63799 | 38300 | 07$^h$ 50$^m$ 47.36$^s$ | +03° 16′ 38.4″ | 6.17 | 0.81 | 384 | K1III | |
| HD 66011 | | | | 66011 | 39271 | 08$^h$ 01$^m$ 50.73$^s$ | +08° 54′ 50.2″ | 6.22 | 2.34 | 194 | G0IV | |
| HD 60275 | | | | 60275 | 36796 | 07$^h$ 34$^m$ 04.98$^s$ | +10° 34′ 05.2″ | 6.28 | 0.73 | 420 | A1V | |
| BC CMi | | | BC | 64052 | 38406 | 07$^h$ 52$^m$ 07.16$^s$ | +03° 16′ 39.1″ | 6.30 | 0.75 | 420 | M5 | semiregular variable, V$_{max}$ = 6.14$^m$, V$_{min}$ = 6.42$^m$, P = 35 d |
| HD 65123 | | | | 65123 | 38870 | 07$^h$ 57$^m$ 16.39$^s$ | +01° 07′ 37.3″ | 6.35 | 2.51 | 191 | F6V | |
| HD 58552 | | | | 58552 | 36123 | 07$^h$ 26$^m$ 27.81$^s$ | +10° 36′ 29.0″ | 6.38 | 1.45 | 316 | A2IV | |
| HD 59603 | | | | 59603 | 36553 | 07$^h$ 31$^m$ 08.79$^s$ | +11° 12′ 10.8″ | 6.38 | −0.32 | 712 | K0 | |
| HD 63838 | | | | 63838 | 38306 | 07$^h$ 50$^m$ 53.42$^s$ | +00° 04′ 46.4″ | 6.38 | 0.86 | 414 | K2III | |
| HD 58599 | | | | 58599 | 36141 | 07$^h$ 26$^m$ 41.22$^s$ | +11° 00′ 31.9″ | 6.39 | −1.55 | 1264 | B7II-III | |
| HD 62407 | | | | 62407 | 37723 | 07$^h$ 44$^m$ 14.07$^s$ | +12° 51′ 36.4″ | 6.40 | −0.75 | 876 | K0 | |
| HD 63475 | | | | 63475 | 38196 | 07$^h$ 49$^m$ 32.32$^s$ | +12° 48′ 51.5″ | 6.42 | 0.44 | 511 | K0 | |
| BU CMi | | | BU | 65241 | 38945 | 07$^h$ 58$^m$ 05.90$^s$ | +07° 12′ 48.8″ | 6.42 | −0.64 | 842 | A0V | Algol variable |
| HD 57707 | | | | 57707 | 35751 | 07$^h$ 22$^m$ 28.30$^s$ | +00° 42′ 03.4″ | 6.43 | 2.24 | 225 | G5 | |
| AZ CMi | | | AZ | 62437 | 37705 | 07$^h$ 44$^m$ 07.64$^s$ | +02° 24′ 19.6″ | 6.46 | 0.84 | 433 | A5IV | δ Sct variable, V$_{max}$ = 6.44$^m$, V$_{min}$ = 6.51$^m$, P = 0.09526 d |
| HD 63798 | | | | 63798 | 38303 | 07$^h$ 50$^m$ 51.11$^s$ | +04° 27′ 33.8″ | 6.49 | 1.12 | 387 | G5 | |
| HD 62286 | | | | 62286 | 37634 | 07$^h$ 43$^m$ 21.21$^s$ | +04° 56′ 44.9″ | 6.50 | 0.03 | 643 | K0 | |
| S CMi | | | S | 59950 | 36675 | 07$^h$ 32$^m$ 43.07$^s$ | +08° 19′ 05.2″ | 6.60 | | 2450 | M7-8e | Mira variable, V$_{max}$ = 6.6$^m$, V$_{min}$ = 13.2$^m$, P = 332.94 d |
| AI CMi | | | AI | | | 07$^h$ 35$^m$ 41.15$^s$ | +00° 14′ 58.0″ | 8.31 | | | G5Iab | slow irregular variable, V$_{max}$ = 7.77$^m$, V$_{min}$ = 9.53$^m$ |
| HD 56126 | | | CY | 56126 | | 07$^h$ 16$^m$ 10.6$^s$ | +09° 59′ 48.0″ | 8.32 | | | F5Iab | post-AGB star, ΔV = 0.18$^m$, P = 39 d |
| YY CMi | | | YY | 67110 | | 08$^h$ 06$^m$ 38.56$^s$ | +01° 55′ 46.5″ | 8.70 | | | F7V | β Lyr variable, V$_{max}$ = 8.33$^m$, V$_{min}$ = 9.13$^m$, P = 1.0940197 d |
| AD CMi | | | AD | 64191 | 38473 | 07$^h$ 52$^m$ 47.18$^s$ | +01° 35′ 50.5″ | 9.38 | | 528 | F2:III | δ Sct variable, V$_{max}$ = 9.21$^m$, V$_{min}$ = 9.51$^m$, P = 0.12297443 d |
| Luyten's star | | | | | 36208 | 07$^h$ 27$^m$ 24.91$^s$ | +05° 13′ 32.8″ | 9.87 | 11.94 | 12.37 | M3.5V | |
| XZ CMi | | | XZ | | | 07$^h$ 54$^m$ 07.06$^s$ | +03° 39′ 20.4″ | 10.25 | | | F0 | Algol variable, V$_{max}$ = 9.7$^m$, V$_{min}$ = 10.42$^m$, P = 0.5780095 d |
| AK CMi | | | AK | | | 07$^h$ 40$^m$ 15.60$^s$ | +03° 57′ 09.5″ | 10.73 | | | A-F | Algol variable |
| YZ CMi | | | YZ | | | 07$^h$ 44$^m$ 40.17$^s$ | +03° 33′ 08.8″ | 11.23 | | 19.419 | M4.5V | BY Dra and UV Cet variable |
| HAT-P-50 | | | | | | 07$^h$ 52$^m$ 15.0$^s$ | +12° 08′ 22″ | 11.76 | | 1947 | | has a transiting planet (b) |
| BG CMi | | | BG | | | 07$^h$ 31$^m$ 29.01$^s$ | +09° 56′ 23.1″ | 14.5 | | | | DQ Her variable, V$_{max}$ = 13.9$^m$, V$_{min}$ = 15.6$^m$, P = 0.13475 d |
| 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.] |||||||||||||