List of stars in Canes Venatici
# List of stars in Canes Venatici

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

| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| - | - | - | - | - | - | - | - | - | - | - | - | - |
| Cor Caroli | $α^2$ | 12 | | 112413 | 63125 | $12^h$ $56^m$ $01.84^s$ | +38° 19′ 05.7″ | 2.89 | 0.25 | 114 | A0spe... | prototype α² CVn variable, $V_{max}$ = $2.86^m,$ $V_{min}$ = $2.93^m,$ P = 5.46939 d; binary star with $α^1$ CVn |
| β CVn | β | 8 | | 109358 | 61317 | $12^h$ $33^m$ $45.09^s$ | +41° 21′ 24.4″ | 4.24 | 4.63 | 27 | G0V | Chara, Asterion; solar analog; suspected variable, $V_{max}$ = $4.24^m,$ $V_{min}$ = $4.29^m$ |
| 24 CVn | | 24 | | 118232 | 66234 | $13^h$ $34^m$ $27.37^s$ | +49° 00′ 57.3″ | 4.68 | 0.85 | 190 | A5V | suspected variable, $V_{max}$ = $4.60^m,$ $V_{min}$ = $4.70^m$ |
| 20 CVn | | 20 | AO | 115604 | 64844 | $13^h$ $17^m$ $32.64^s$ | +40° 34′ 21.2″ | 4.72 | 0.00 | 286 | F3III | δ Sct variable, $V_{max}$ = $4.7^m,$ $V_{min}$ = $4.75^m,$ P = 0.12168 d |
| AW CVn | | | AW | 120933 | 67665 | $13^h$ $51^m$ $47.49^s$ | +34° 26′ 39.5″ | 4.76 | −1.58 | 604 | K5III | semiregular variable, $V_{max}$ = $4.72^m,$ $V_{min}$ = $4.81^m$ |
| 5 CVn | | 5 | | 107950 | 60485 | $12^h$ $24^m$ $01.48^s$ | +51° 33′ 44.0″ | 4.77 | −0.64 | 393 | G7III | Xiāng (相); suspected eclipsing binary, ΔV = $0.07^m$ |
| 25 CVn | | 25 | | 118623 | 66458 | $13^h$ $37^m$ $27.70^s$ | +36° 17′ 41.4″ | 4.82 | 0.97 | 192 | A7III | binary star |
| HR 5110 | | | BH | 118216 | 66257 | $13^h$ $34^m$ $47.75^s$ | +37° 10′ 56.8″ | 4.91 | 1.67 | 145 | F2IV SB | RS CVn variable, ΔV = $0.07^m,$ P = 2.61317 d |
| HD 115004 | | | | 115004 | 64540 | $13^h$ $13^m$ $42.98^s$ | +40° 09′ 10.3″ | 4.94 | −1.08 | 522 | K0III | |
| 6 CVn | | 6 | | 108225 | 60646 | $12^h$ $25^m$ $51.00^s$ | +39° 01′ 07.3″ | 5.01 | 0.79 | 227 | G8III-IV | variable star, ΔV = $0.006^m,$ P = 157.23270 d |
| 21 CVn | | 21 | BK | 115735 | 64906 | $13^h$ $18^m$ $14.54^s$ | +49° 40′ 55.3″ | 5.13 | 0.51 | 275 | A0V | α² CVn variable, ΔV = $0.04^m$ |
| 14 CVn | | 14 | | 113797 | 63901 | $13^h$ $05^m$ $44.46^s$ | +35° 47′ 55.9″ | 5.20 | 0.51 | 282 | B9V | suspected variable, $V_{max}$ = $5.10^m,$ $V_{min}$ = $5.29^m$ |
| 3 CVn | | 3 | | 107274 | 60122 | $12^h$ $19^m$ $48.72^s$ | +48° 59′ 02.9″ | 5.28 | −0.72 | 517 | M0III | suspected variable |
| HD 109317 | | | | 109317 | 61309 | $12^h$ $33^m$ $38.90^s$ | +33° 14′ 51.6″ | 5.42 | 0.86 | 266 | K0IIICN... | |
| La Superba | | | Y | 110914 | 62223 | $12^h$ $45^m$ $07.83^s$ | +45° 26′ 24.8″ | 5.42 | −1.27 | 710 | C7Iab | semiregular variable, $V_{max}$ = $4.86^m,$ $V_{min}$ = $5.88^m,$ P = 267.8 d |
| HD 120164 | | | | 120164 | 67250 | $13^h$ $46^m$ $59.87^s$ | +38° 32′ 33.9″ | 5.51 | 0.67 | 304 | K0III+... | |
| 23 CVn | | 23 | | 116010 | 65072 | $13^h$ $20^m$ $19.00^s$ | +40° 09′ 02.0″ | 5.60 | −0.91 | 655 | K1III | |
| $α^1$ CVn | $α^1$ | 12 | | 112412 | 63121 | $12^h$ $56^m$ $00.60^s$ | +38° 18′ 52.9″ | 5.61 | 2.78 | 120.2 | F0V | component of the Cor Caroli system |
| HD 120420 | | | | 120420 | 67384 | $13^h$ $48^m$ $38.74^s$ | +31° 11′ 24.4″ | 5.61 | 0.71 | 311 | K0III | |
| HD 113847 | | | | 113847 | 63916 | $13^h$ $05^m$ $52.28^s$ | +45° 16′ 06.6″ | 5.64 | −0.21 | 483 | K1III | suspected variable, $V_{max}$ = $5.64^m,$ $V_{min}$ = $5.84^m$ |
| 2 CVn | | 2 | | 106690 | 59831 | $12^h$ $16^m$ $07.54^s$ | +40° 39′ 36.9″ | 5.69 | −1.35 | 834 | M1III | |
| TU CVn | | | TU | 112264 | 63024 | $12^h$ $54^m$ $56.54^s$ | +47° 11′ 48.3″ | 5.75 | −0.92 | 704 | M5III | semiregular variable, $V_{max}$ = $5.50^m,$ $V_{min}$ = $6.2^m,$ P = 44.2 d |
| 19 CVn | | 19 | | 115271 | 64692 | $13^h$ $15^m$ $32.05^s$ | +40° 51′ 18.6″ | 5.77 | 1.39 | 245 | A7V | |
| HD 115723 | | | | 115723 | 64927 | $13^h$ $18^m$ $27.71^s$ | +34° 05′ 53.9″ | 5.81 | −0.14 | 504 | K4.5III | |
| HD 111604 | | | DT | 111604 | 62641 | $12^h$ $50^m$ $10.81^s$ | +37° 31′ 00.8″ | 5.87 | 0.50 | 387 | A3V | δ Sct variable |
| HD 116957 | | | | 116957 | 65550 | $13^h$ $26^m$ $16.58^s$ | +46° 01′ 41.2″ | 5.88 | 0.68 | 357 | K0III: | |
| HD 120047 | | | | 120047 | 67194 | $13^h$ $46^m$ $13.63^s$ | +41° 05′ 19.9″ | 5.88 | 2.33 | 167 | A5V | |
| HD 120819 | | | | 120819 | 67605 | $13^h$ $51^m$ $09.21^s$ | +34° 39′ 52.3″ | 5.89 | −0.69 | 676 | M2III | variable star, ΔV = $0.010^m,$ P = 7.94786 d |
| 17 CVn | | 17 | | 114447 | 64246 | $13^h$ $10^m$ $03.27^s$ | +38° 29′ 55.9″ | 5.91 | 1.95 | 202 | A9III-IV | γ Dor variable, ΔV = $0.008^m,$ P = 0.69004 d |
| HD 121164 | | | | 121164 | 67782 | $13^h$ $53^m$ $10.36^s$ | +28° 38′ 53.0″ | 5.91 | 1.86 | 211 | A7V | |
| HD 120048 | | | | 120048 | 67210 | $13^h$ $46^m$ $19.10^s$ | +38° 30′ 13.2″ | 5.92 | 0.46 | 403 | G9III | |
| 10 CVn | | 10 | | 110897 | 62207 | $12^h$ $44^m$ $59.68^s$ | +39° 16′ 42.9″ | 5.95 | 4.75 | 57 | G0V | |
| HD 119458 | | | | 119458 | 66907 | $13^h$ $42^m$ $43.42^s$ | +34° 59′ 20.4″ | 5.98 | 0.11 | 486 | G5III | |
| HD 114357 | | | | 114357 | 64212 | $13^h$ $09^m$ $38.72^s$ | +37° 25′ 23.3″ | 6.01 | 1.20 | 299 | K3III | |
| HD 115810 | | | | 115810 | 64979 | $13^h$ $19^m$ $04.27^s$ | +35° 07′ 40.6″ | 6.01 | 1.94 | 213 | F0IV | |
| 4 CVn | | 4 | AI | 107904 | 60467 | $12^h$ $23^m$ $47.08^s$ | +42° 32′ 33.8″ | 6.03 | 0.98 | 334 | F3IV | δ Sct variable, $V_{max}$ = $5.89^m,$ $V_{min}$ = $6.15^m,$ P = 0.2085 d |
| HD 117710 | | | | 117710 | 65951 | $13^h$ $31^m$ $15.84^s$ | +42° 06′ 21.9″ | 6.07 | 1.53 | 263 | K2III | |
| CL CVn | | | CL | 116581 | 65376 | $13^h$ $23^m$ $53.92^s$ | +37° 02′ 02.2″ | 6.10 | −1.74 | 1207 | M3III | slow irregular variable, ΔV = $~0.10^m$ |
| HD 112570 | | | | 112570 | 63211 | $12^h$ $57^m$ $07.80^s$ | +46° 10′ 36.9″ | 6.12 | 0.99 | 344 | K0III-IV | suspected variable, $V_{max}$ = $6.12^m,$ $V_{min}$ = $6.5^m$ |
| 7 CVn | | 7 | | 108845 | 60988 | $12^h$ $30^m$ $03.10^s$ | +51° 32′ 08.1″ | 6.21 | 2.94 | 147 | F7V | |
| HD 119035 | | | | 119035 | 66690 | $13^h$ $40^m$ $15.63^s$ | +31° 00′ 42.5″ | 6.21 | 0.12 | 540 | G5II: | |
| HD 119081 | | | | 119081 | 66725 | $13^h$ $40^m$ $39.12^s$ | +28° 03′ 54.5″ | 6.22 | 0.88 | 382 | K3III | |
| HD 109345 | | | | 109345 | 61320 | $12^h$ $33^m$ $47.41^s$ | +33° 23′ 04.9″ | 6.24 | 0.94 | 374 | K0III | |
| 11 CVn | | 11 | | 111421 | 62516 | $12^h$ $48^m$ $41.86^s$ | +48° 28′ 00.5″ | 6.25 | 0.49 | 463 | A6m | |
| HD 112171 | | | | 112171 | 62972 | $12^h$ $54^m$ $13.15^s$ | +33° 32′ 03.9″ | 6.25 | 1.89 | 243 | A7IV | |
| 15 CVn | | 15 | | 114376 | 64217 | $13^h$ $09^m$ $42.04^s$ | +38° 32′ 01.9″ | 6.25 | −1.48 | 1144 | B7III | |
| HD 122675 | | | | 122675 | 68567 | $14^h$ $02^m$ $12.17^s$ | +45° 45′ 13.1″ | 6.28 | 0.17 | 544 | K2III | |
| HD 119445 | | | | 119445 | 66892 | $13^h$ $42^m$ $28.87^s$ | +41° 40′ 27.3″ | 6.30 | −1.00 | 942 | G6III | |
| HD 121682 | | | | 121682 | 68065 | $13^h$ $56^m$ $10.54^s$ | +32° 01′ 56.9″ | 6.31 | 2.01 | 236 | F4IV-V | |
| HD 107610 | | | | 107610 | 60305 | $12^h$ $21^m$ $56.30^s$ | +47° 10′ 56.1″ | 6.33 | 1.46 | 307 | K2III | |
| HD 110834 | | | | 110834 | 62172 | $12^h$ $44^m$ $27.12^s$ | +44° 06′ 10.8″ | 6.34 | 1.54 | 298 | F6IV | |
| HD 116303 | | | | 116303 | 65230 | $13^h$ $22^m$ $03.97^s$ | +43° 54′ 12.0″ | 6.34 | 0.60 | 458 | A7m | suspected variable, $V_{max}$ = $6.34^m,$ $V_{min}$ = $6.37^m$ |
| 9 CVn | | 9 | | 109980 | 61692 | $12^h$ $38^m$ $46.30^s$ | +40° 52′ 28.9″ | 6.35 | 2.27 | 213 | A7Vn | suspected variable |
| HD 118156 | | | | 118156 | 66223 | $13^h$ $34^m$ $21.85^s$ | +38° 47′ 21.2″ | 6.37 | 2.20 | 223 | F0IV | |
| HD 110066 | | | AX | 110066 | 61748 | $12^h$ $39^m$ $16.85^s$ | +35° 57′ 07.1″ | 6.39 | 0.44 | 505 | A0p SrCrEu | α² CVn variable, $V_{max}$ = $6.32^m,$ $V_{min}$ = $6.55^m,$ P = 4900 d |
| HD 117361 | | | | 117361 | 65754 | $13^h$ $28^m$ $45.80^s$ | +50° 43′ 07.5″ | 6.42 | 1.97 | 253 | F0IV | |
| HD 120600 | | | | 120600 | 67483 | $13^h$ $49^m$ $44.98^s$ | +36° 37′ 58.0″ | 6.43 | 2.37 | 212 | A7IV-V | |
| HD 121197 | | | | 121197 | 67778 | $13^h$ $53^m$ $08.44^s$ | +40° 20′ 16.8″ | 6.48 | −1.64 | 1370 | K5 | |
| HD 117261 | | | | 117261 | 65723 | $13^h$ $28^m$ $26.23^s$ | +40° 43′ 47.2″ | 6.49 | 0.88 | 432 | G8III | |
| HD 111572 | | | | 111572 | 62600 | $12^h$ $49^m$ $38.05^s$ | +48° 44′ 24.2″ | 6.50 | 0.58 | 497 | K1III | suspected variable, $V_{max}$ = $6.47^m,$ $V_{min}$ = $6.53^m$ |
| HD 114975 | | | | 114975 | 64530 | $13^h$ $13^m$ $35.94^s$ | +36° 53′ 15.3″ | 6.50 | −1.58 | 1347 | M0 | |
| V CVn | | | V | 115898 | 65006 | $13^h$ $19^m$ $27.77^s$ | +45° 31′ 37.7″ | 6.74 | -2.46 | 2260 | M6IIIa | semiregular variable, $V_{max}$ = $6.52^m,$ $V_{min}$ = $8.56^m,$ P = 191.89 d |
| HD 108100 | | | DD | 108100 | 60571 | $12^h$ $24^m$ $13.93^s$ | +42° 51′ 17.0″ | 7.15 | 2.58 | 267.4 | F2V | γ Dor variable, ΔV = $0.04^m,$ P = 0.754307 d |
| BM CVn | | | BM | 116204 | 65187 | $13^h$ $21^m$ $32.26^s$ | +38° 52′ 49.5″ | 7.21 | 1.94 | 368 | K2III | RS CVn variable, ΔV = $0.06^m,$ P = 21.7 d |
| R CVn | | | R | 120499 | 67410 | $13^h$ $48^m$ $57.20^s$ | +39° 32′ 34.0″ | 7.40 | -2.51 | 3130 | M6IIIe | Mira variable, $V_{max}$ = $6.5^m,$ $V_{min}$ = $12.9^m,$ P = 328.53 d |
| HD 109995 | | | | 109995 | 61696 | $12^h$ $38^m$ $47.60^s$ | +39° 18′ 31.6″ | 7.64 | 0.46 | 891 | A0p | horizontal-branch star |
| HD 115781 | | | BL | 115781 | 64956 | $13^h$ $18^m$ $51.94^s$ | +33° 26′ 19.3″ | 8.13 | 1.5 | 691 | K1III | rotating ellipsoidal variable, ΔV = $0.24^m,$ P = 18.692 d |
| RS CVn | | | RS | 114519 | 64293 | $13^h$ $10^m$ $36.91^s$ | +35° 56′ 05.6″ | 8.23 | 3.06 | 352 | F4V+... | prototype RS CVn variable, $V_{max}$ = $7.93^m,$ $V_{min}$ = $9.14^m,$ P = 4.797887 d |
| TT CVn | | | TT | 112869 | 63389 | $12^h$ $59^m$ $22.64^s$ | +37° 49′ 03.7″ | 8.91 | | | Rp... | semiregular variable |
| HD 115444 | | | | 115444 | 64786 | $13^h$ $16^m$ $42.46^s$ | +36° 22′ 52.7″ | 8.97 | 1.72 | 918 | G9V | barium star |
| TX CVn | | | TX | | | $12^h$ $44^m$ $22.07^s$ | +36° 45′ 50.7″ | 9.34 | | | B1-B9Veq + K0III-M4 | Z And and rotating ellipsoidal variable, $V_{max}$ = $9.34^m,$ $V_{min}$ = $10.28^m,$ P = 199.75 d |
| VZ CVn | | | VZ | 117777 | 66017 | $13^h$ $32^m$ $03.39^s$ | +28° 35′ 04.9″ | 9.35 | 1.1 | 1460 | F3V + F6V | Algol and γ Dor variable, $V_{max}$ = $9.17^m,$ $V_{min}$ = $9.72^m,$ P = 0.84246163 d |
| HIP 65407 | | | | | 65407 | $13^h$ $24^m$ $21.0^s$ | +48° 53′ 06″ | 9.42 | 8.29 | 55 | K0 | has two planets (b & c) |
| Gliese 521 | | | | | 66625 | $13^h$ $39^m$ $24.10^s$ | +46° 11′ 11.4″ | 10.26 | 9.69 | 42.41 | M2.0V | possibly has a planet |
| BI CVn | | | BI | | 63701 | $13^h$ $03^m$ $16.41^s$ | +36° 37′ 00.6″ | 10.31 | 3.41 | 782 | F9V | W UMa variable, $V_{max}$ = $10.26^m,$ $V_{min}$ = $10.71^m,$ P = 0.38416 d |
| W CVn | | | W | | 68908 | $14^h$ $06^m$ $27.98^s$ | +37° 49′ 41.5″ | 10.49 | -0.39 | 4900 | F2III | RR Lyr variable, $V_{max}$ = $10.03^m,$ $V_{min}$ = $10.96^m,$ P = 0.5517588 d |
| Gliese 490 | | | BF | | 63253 | $12^h$ $57^m$ $40.26^s$ | +35° 13′ 30.0″ | 10.52 | 9.1 | 62.78 | M0.0V | binary star; BY Dra variable and flare star, $V_{max}$ = $10.5^m,$ $V_{min}$ = $10.6^m,$ P = 3.17 d |
| ST CVn | | | ST | | 68188 | $13^h$ $57^m$ $34.06^s$ | +29° 51′ 28.7″ | 11.21 | | | A1 | RR Lyr variable, $V_{max}$ = $11.04^m,$ $V_{min}$ = $11.6^m,$ P = 0.329045 d |
| UZ CVn | | | UZ | | 61029 | $12^h$ $30^m$ $27.70^s$ | +40° 30′ 32.0″ | 12.11 | 4.76 | 964 | A8 | RR Lyr variable |
| Z CVn | | | Z | | | $12^h$ $49^m$ $45.37^s$ | +43° 46′ 25.1″ | 12.12 | | | A5 | RR Lyr variable, $V_{max}$ = $11.46^m,$ $V_{min}$ = $12.36^m,$ P = 0.653819 d |
| DG CVn | | | DG | | | $13^h$ $31^m$ $46.62^s$ | +29° 16′ 36.7″ | 12.19 | 12.69 | 25.9 | M4.0V | flare star and BY Dra variable |
| HAT-P-36 | | | | | | $12^h$ $33^m$ $03^s$ | +44° 54′ 55″ | 12.26 | 4.75 | 1034 | | Tuiren; has a transiting planet (Bran) |
| UX CVn | | | UX | | | $12^h$ $14^m$ $48.54^s$ | +36° 38′ 49.3″ | | | | B2 | rotating ellipsoidal variable and eclipsing binary |
| HAT-P-12 | | | | | | $13^h$ $57^m$ $33.48^s$ | +43° 29′ 36.7″ | 12.84 | | | K5 | has a transiting planet |
| AM CVn | | | AM | | | $12^h$ $34^m$ $54.60^s$ | +37° 37′ 44.1″ | 14.18 | 9.15 | 330 | DBp | prototype AM CVn star |
| GD 154 | | | BG | | | $13^h$ $09^m$ $57.69^s$ | +35° 09′ 47.1″ | 15.33 | | | DA4.4 | ZZ Cet variable, ΔV = $0.09^m,$ P = 0.013727 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.] |||||||||||||
