title: Liste d'étoiles du Corbeau
text: # Liste d'étoiles du Corbeau
  
  Cet article recense les étoiles situées dans la constellation du Corbeau, classées par magnitude apparente décroissante.
  
  ## Liste
  
  | Dés. | B | F | Var | HD | HIP | α | δ | Mag. app. | Mag. abs. | Dist. (al) | Type | Notes |
  | - | - | - | - | - | - | - | - | - | - | - | - | - |
  | γ Crv | γ | 4 | | 106625 | 59803 | $12^h$ $15^m$ $48,47^s$ | −17° 32′ 31,1″ | 2,58 | −0,94 | 165 | B8III | Gienah Corvi, Gienah, Gienah Ghurab ; probablement variable |
  | β Crv | β | 9 | | 109379 | 61359 | $12^h$ $34^m$ $23,23^s$ | −23° 23′ 47,8″ | 2,65 | −0,51 | 140 | G5II | Kraz, Tso Hea ; probablement variable |
  | δ Crv | δ | 7 | | 108767 | 60965 | $12^h$ $29^m$ $51,98^s$ | −16° 30′ 54,3″ | 2,94 | 0,79 | 88 | B9,5V | Algorab, Algoral, Algorel, Algores ; étoile double ; probablement variable |
  | ε Crv | ε | 2 | | 105707 | 59316 | $12^h$ $10^m$ $07,53^s$ | −22° 37′ 11,3″ | 3,02 | −1,82 | 303 | K2III | Minkar ; probablement variable |
  | α Crv | α | 1 | | 105452 | 59199 | $12^h$ $08^m$ $24,75^s$ | −24° 43′ 43,6″ | 4,02 | 3,17 | 48 | F1V | Al Chiba, Al Minliar al Ghurab, Alchiba, Alchita, Alkhiba ; possible variable de type γ Dor |
  | η Crv | η | 8 | | 109085 | 61174 | $12^h$ $32^m$ $04,48^s$ | −16° 11′ 45,1″ | 4,30 | 3,00 | 59 | F2V | Probablement variable |
  | HR 4699 | | | | 107418 | 60221 | $12^h$ $20^m$ $55,72^s$ | −13° 33′ 56,7″ | 5,14 | 1,24 | 196 | K0III | Variable |
  | VV Crv | | | VV | 110317 | 61910 | $12^h$ $41^m$ $16,02^s$ | −13° 00′ 50,1″ | 5,17 | 0,51 | 278 | F3IV | Système quadruple ; variable de type Algol, $V_{max}$ = +5,19, $V_{min}$ = +5,34 |
  | ζ Crv | ζ | 5 | | 107348 | 60189 | $12^h$ $20^m$ $33,71^s$ | −22° 12′ 57,0″ | 5,20 | −0,16 | 385 | B8V | Étoile Be ; étoile double ; probablement variable |
  | 31 Crt | | (31) | TY | 104337 | 58587 | $12^h$ $00^m$ $51,17^s$ | −19° 39′ 32,4″ | 5,28 | −3,37 | 1753 | B2IV | TY Crv ; binaire spectroscopique ; variable ellipsoïdale, $V_{max}$ = +5,19, $V_{min}$ = +5,23 |
  | 3 Crv | | 3 | | 105850 | 59394 | $12^h$ $11^m$ $03,88^s$ | −23° 36′ 08,5″ | 5,45 | 1,70 | 183 | A1V | |
  | | | | | 109272 | 61296 | $12^h$ $33^m$ $34,27^s$ | −12° 49′ 49,2″ | 5,58 | 2,15 | 158 | G8III/IV | |
  | | | | | 108821 | 61015 | $12^h$ $30^m$ $17,46^s$ | −23° 41′ 47,1″ | 5,63 | −1,57 | 898 | M0III | Probablement variable |
  | 6 Crv | | 6 | | 107815 | 60425 | $12^h$ $23^m$ $21,60^s$ | −24° 50′ 26,2″ | 5,66 | 0,73 | 316 | K1III | |
  | | | | | 109141 | 61212 | $12^h$ $32^m$ $36,09^s$ | −13° 51′ 32,3″ | 5,74 | 2,90 | 120 | F3IV/V | |
  | | | | | 106485 | 59728 | $12^h$ $14^m$ $59,58^s$ | −20° 50′ 39,2″ | 5,82 | 0,65 | 353 | K0IIICN... | |
  | | | | | 107295 | 60157 | $12^h$ $20^m$ $10,83^s$ | −22° 10′ 32,3″ | 5,94 | 0,13 | 474 | K0III+... | Étoile double |
  | | | | | 109931 | 61688 | $12^h$ $38^m$ $44,69^s$ | −18° 15′ 00,6″ | 6,00 | 2,03 | 203 | F0V | |
  | | | | | 110385 | 61951 | $12^h$ $41^m$ $49,51^s$ | −19° 45′ 32,9″ | 6,02 | 1,91 | 216 | F2V | |
  | | | | | 106819 | 59895 | $12^h$ $17^m$ $03,36^s$ | −16° 41′ 37,5″ | 6,05 | −0,04 | 540 | A2V | |
  | | | | | 112304 | 63109 | $12^h$ $55^m$ $53,25^s$ | −15° 19′ 37,3″ | 6,18 | −0,38 | 669 | A0V | |
  | TU Crv | | | TU | 109585 | 61496 | $12^h$ $35^m$ $58,77^s$ | −20° 31′ 38,5″ | 6,20 | 1,77 | 251 | F0III | Variable de type δ Sct de faible amplitude |
  | | | | | 109238 | 61270 | $12^h$ $33^m$ $22,27^s$ | −19° 47′ 32,9″ | 6,26 | 0,65 | 432 | F0IV/V | |
  | | | | | 104307 | 58574 | $12^h$ $00^m$ $42,23^s$ | −21° 50′ 14,9″ | 6,28 | 0,22 | 532 | K2III | Étoile double |
  | | | | | 108477 | 60809 | $12^h$ $27^m$ $49,45^s$ | −16° 37′ 54,7″ | 6,30 | −1,67 | 1278 | G5II | |
  | | | | | 108799 | 60994 | $12^h$ $30^m$ $04,93^s$ | −13° 23′ 35,0″ | 6,37 | 4,38 | 81 | G1/G2V | Étoile multiple |
  | | | | | 109132 | 61208 | $12^h$ $32^m$ $32,89^s$ | −21° 12′ 43,2″ | 6,41 | 0,86 | 419 | K0III | |
  | TT Crv | | | TT | 107814 | 60421 | $12^h$ $23^m$ $18,90^s$ | −11° 48′ 43,5″ | 6,48 | −0,68 | 881 | M3III | Variable semi-régulière, $V_{max}$ = +6,47, $V_{min}$ = +6,57, P = 11,5 j |
  | R Crv | | | R | 107199 | 60106 | $12^h$ $19^m$ $37,87^s$ | −19° 15′ 21,8″ | 9,25 | | | M6e | Variable de type Mira, $V_{max}$ = +6,7, $V_{min}$ = +14,4, P = 317,03 j |
  | HD 111031 | | | | 111031 | 62345 | $12^h$ $46^m$ $30,85^s$ | -11° 48′ 44,8″ | 6,88 | 4,45 | 99 | G5V | Possède une exoplanète à confirmer (b) |
  | HD 103774 | | | | 103774 | 58263 | $11^h$ $56^m$ $56,0^s$ | -12° 06′ 28″ | 7,12 | | 179 | F5V | Possède une exoplanète (b) |
  | HD 104067 | | | | 104067 | 58451 | $11^h$ $59^m$ $10,01^s$ | −20° 21′ 13,6″ | 7,93 | 6,34 | 68 | K2V | Possède une exoplanète (b) |
  | HD 111980 | | | | 111980 | 62882 | $12^h$ $53^m$ $15,05^s$ | −18° 31′ 20,0″ | 8,38 | | 310,5 | F7V | Étoile à grande vitesse |
  | RV Crv | | | RV | 109796 | 61620 | $12^h$ $37^m$ $40,71^s$ | −19° 34′ 40,1″ | 8,76 | | 656 | F0V | Variable de type β Lyr |
  | SX Crv | | | SX | 110139 | 61825 | $12^h$ $40^m$ $15,04^s$ | −18° 48′ 00,9″ | 9,11 | | 298,0 | F7V | Variable de type W UMa |
  | W Crv | | | W | | | $12^h$ $07^m$ $37,36^s$ | −13° 08′ 59,0″ | 11,28 | | | G2Iab | Variable de type β Lyr |
  | LHS 2520 | | | | | | $12^h$ $10^m$ $05,60^s$ | -15° 04′ 17,0″ | 12,08 | | 40 | M3,5V | |
  | TV Crv | | | TV | | | $12^h$ $20^m$ $24,15^s$ | -18° 27′ 02,0″ | 12,2 | | | | Étoile de Tombaugh |
  | WASP-83 | | | | | | $12^h$ $40^m$ $37,0^s$ | -19° 17′ 03″ | 12,9 | | 978 | G8 | Possède une exoplanète qui transite (b) |
  | VHS J1256-1257 | | | | | | $12^h$ $56^m$ $02,15^s$ | −12° 57′ 21,7″ | 17,76 | | 41,4 | M7,5 | Naine brune qui possède une exoplanète massive (b) |
  | DENIS-P J1228.2-1547 | | | | | | $12^h$ $28^m$ $15,23^s$ | −15° 47′ 34,2″ | | | 66,0 | L5V | Naine brune binaire |
  