# Liste d'étoiles du Bélier

Cet article recense les étoiles situées dans la constellation du Bélier, classées par magnitude apparente décroissante.

## Liste

| Dés. | B | F | Var | HD | HIP | α | δ | Mag. app. | Mag. abs. | Dist. (al) | Type | Notes |
| α Ari | α | 13 | | 12929 | 9884 | 02$^h$ 07$^m$ 10,29$^s$ | +23° 27′ 46,0″ | 2,01 | 0,48 | 66 | K2III | Hamal, Hemal, Hamul, Ras Hammel, El Nath, Arietis ; variable suspectée, V$_{max}$ = 1,98$^m$, V$_{min}$ = 2,04$^m$ ; possède une exoplanète (b) |
| β Ari | β | 6 | | 11636 | 8903 | 01$^h$ 54$^m$ 38,35$^s$ | +20° 48′ 29,9″ | 2,64 | 1,33 | 60 | A5V... | Sheratan, Sharatan, Al Sharatain ; variable suspectée, V$_{max}$ = 2,56$^m$, V$_{min}$ = 2,70$^m$ |
| 41 Ari | c | 41 | | 17573 | 13209 | 02$^h$ 49$^m$ 58,99$^s$ | +27° 15′ 38,8″ | 3,61 | 0,16 | 159 | B8Vn | Bharani ; variable suspectée, V$_{max}$ = 3,60$^m$, V$_{min}$ = 3,64$^m$ |
| δ Ari | δ | 57 | | 19787 | 14838 | 03$^h$ 11$^m$ 37,67$^s$ | +19° 43′ 36,1″ | 4,35 | 0,79 | 168 | K2IIIvar | Botein ; variable suspectée, V$_{max}$ = 4,33$^m$, V$_{min}$ = 4,37$^m$ |
| HR 999 | | | | 20644 | 15549 | 03$^h$ 20$^m$ 20,37$^s$ | +29° 02′ 54,6″ | 4,47 | −2,00 | 640 | K2II-III | |
| 39 Ari | | 39 | | 17361 | 13061 | 02$^h$ 47$^m$ 54,44$^s$ | +29° 14′ 50,7″ | 4,52 | 0,80 | 181 | K1III | Lilii Borea |
| γ$^2$ Ari | γ² | 5 | | 11503 | | 01$^h$ 53$^m$ 31,80$^s$ | +19° 17′ 45,0″ | 4,62 | | 204 | kA0hA3 (IV)SiSr | Mesarthim, Mesartim ; étoile binaire ; variable de type α$^2$ CVn, ΔV = 0,04 mag, P = 1,6092 j |
| 35 Ari | | 35 | | 16908 | 12719 | 02$^h$ 43$^m$ 27,11$^s$ | +27° 42′ 25,8″ | 4,65 | −0,62 | 370 | B3V | Binaire spectroscopique |
| γ$^1$ Ari | γ$^1$ | 5 | | 11502 | 8832 | 01$^h$ 53$^m$ 31,77$^s$ | +19° 17′ 38,7″ | 4,70 | −0,10 | 204 | B9,5IV | Composante du système γ Ari |
| λ Ari | λ | 9 | | 11973 | 9153 | 01$^h$ 57$^m$ 55,78$^s$ | +23° 35′ 45,9″ | 4,79 | 1,73 | 133 | F0V | Étoile binaire |
| ζ Ari | ζ | 58 | | 20150 | 15110 | 03$^h$ 14$^m$ 54,11$^s$ | +21° 02′ 40,7″ | 4,87 | −0,22 | 340 | A1V | |
| 14 Ari | | 14 | | 13174 | 10053 | 02$^h$ 09$^m$ 25,29$^s$ | +25° 56′ 23,9″ | 4,98 | 0,02 | 320 | F2III | |
| κ Ari | κ | 12 | | 12869 | 9836 | 02$^h$ 06$^m$ 33,91$^s$ | +22° 38′ 54,3″ | 5,03 | 1,23 | 187 | A2m | Binaire spectroscopique |
| ι Ari | ι | 8 | | 11909 | 9110 | 01$^h$ 57$^m$ 21,03$^s$ | +17° 49′ 03,3″ | 5,09 | −1,44 | 659 | K1p... | Binaire spectroscopique |
| τ$^2$ Ari | τ$^2$ | 63 | | 20893 | 15737 | 03$^h$ 22$^m$ 45,27$^s$ | +20° 44′ 31,6″ | 5,10 | 0,15 | 319 | K3III | |
| 38 Ari | | 38 | UV | 17093 | 12832 | 02$^h$ 44$^m$ 57,51$^s$ | +12° 26′ 45,5″ | 5,17 | 2,26 | 125 | A7III-IV | Variable de type δ Sct, V$_{max}$ = 5,18$^m$, V$_{min}$ = 5,22$^m$, P = 0,0355 j |
| ε Ari A | ε | 48 | | 18519 | 13914 | 02$^h$ 59$^m$ 12,73$^s$ | +21° 20′ 25,6″ | 5,2 | −0,13 | 292 | A2Vs | Étoile binaire |
| η Ari | η | 17 | | 13555 | 10306 | 02$^h$ 12$^m$ 47,98$^s$ | +21° 12′ 39,5″ | 5,23 | 2,84 | 98 | F5V | |
| π Ari | π | 42 | | 17543 | 13165 | 02$^h$ 49$^m$ 17,56$^s$ | +17° 27′ 51,6″ | 5,26 | −1,07 | 603 | B6V | Binaire spectroscopique |
| τ$^1$ Ari | τ$^1$ | 61 | | 20756 | 15627 | 03$^h$ 21$^m$ 13,61$^s$ | +21° 08′ 49,7″ | 5,27 (5,26–5,32) | −0,49 | 462 | B5IV | Système triple à éclipses ; variable de type β Lyr |
| 33 Ari | | 33 | | 16628 | 12489 | 02$^h$ 40$^m$ 41,03$^s$ | +27° 03′ 39,6″ | 5,30 | 1,03 | 233 | A3V | |
| ν Ari | ν | 32 | | 16432 | 12332 | 02$^h$ 38$^m$ 49,00$^s$ | +21° 57′ 41,2″ | 5,45 | 0,32 | 346 | A7V | |
| 52 Ari A | | 52 | | 19134 | 14376 | 03$^h$ 05$^m$ 26,69$^s$ | +25° 15′ 18,7″ | 5,45 | 0,00 | 402 | B7Vn | Étoile binaire |
| ξ Ari | ξ | 24 | | 14951 | 11249 | 02$^h$ 24$^m$ 49,04$^s$ | +10° 36′ 38,2″ | 5,48 | −0,85 | 603 | B7IV | Étoile variable |
| ε Ari B | ε | 48 | | 18520 | | 02$^h$ 59$^m$ 12,70$^s$ | +21° 20′ 25,0″ | 5,5 | | | | Composante du système ε Ari |
| 64 Ari | | 64 | | 21017 | 15861 | 03$^h$ 24$^m$ 18,46$^s$ | +24° 43′ 27,1″ | 5,50 | 1,26 | 230 | K4III | |
| σ Ari | σ | 43 | | 17769 | 13327 | 02$^h$ 51$^m$ 29,57$^s$ | +15° 04′ 55,7″ | 5,52 | −0,32 | 479 | B7V | |
| 62 Ari | | 62 | | 20825 | 15696 | 03$^h$ 22$^m$ 11,89$^s$ | +27° 36′ 27,3″ | 5,55 | −1,82 | 973 | G5III | |
| 21 Ari | | 21 | | 13872 | 10535 | 02$^h$ 15$^m$ 42,83$^s$ | +25° 02′ 35,7″ | 5,57 | 2,16 | 157 | F6V | |
| θ Ari | θ | 22 | | 14191 | 10732 | 02$^h$ 18$^m$ 07,55$^s$ | +19° 54′ 04,2″ | 5,58 | 0,21 | 387 | A1Vn | |
| ρ$^3$ Ari | ρ$^3$ | 46 | | 18256 | 13702 | 02$^h$ 56$^m$ 25,98$^s$ | +18° 01′ 25,1″ | 5,58 | 2,83 | 115 | F6V | Variable de type BY Dra suspectée |
| | | | | 20149 | 15154 | 03$^h$ 15$^m$ 20,45$^s$ | +30° 33′ 24,0″ | 5,61 | −0,01 | 434 | A1Vs | |
| 10 Ari | | 10 | | 12558 | 9621 | 02$^h$ 03$^m$ 39,26$^s$ | +25° 56′ 07,6″ | 5,64 | 2,02 | 172 | F8IV | |
| 31 Ari | | 31 | | 16234 | 12153 | 02$^h$ 36$^m$ 37,75$^s$ | +12° 26′ 52,2″ | 5,64 | 2,91 | 115 | F7V | |
| | | | | 19270 | 14439 | 03$^h$ 06$^m$ 23,69$^s$ | +13° 11′ 14,6″ | 5,64 | 0,69 | 319 | K3III | |
| 15 Ari | | 15 | AV | 13325 | 10155 | 02$^h$ 10$^m$ 37,54$^s$ | +19° 30′ 01,5″ | 5,68 | −0,87 | 665 | M3III | Variable semi-régulière, V$_{max}$ = 5,67$^m$, V$_{min}$ = 5,74$^m$, P = 5,0320 j |
| 19 Ari | | 19 | | 13596 | 10328 | 02$^h$ 13$^m$ 03,25$^s$ | +15° 16′ 47,7″ | 5,72 | −0,38 | 541 | M0III | Variable suspectée, V$_{max}$ = 5,68$^m$, V$_{min}$ = 5,76$^m$ |
| μ Ari | μ | 34 | | 16811 | 12640 | 02$^h$ 42$^m$ 21,92$^s$ | +20° 00′ 41,7″ | 5,74 | 0,66 | 338 | A0V | |
| 55 Ari | | 55 | | 19548 | 14677 | 03$^h$ 09$^m$ 36,73$^s$ | +29° 04′ 37,6″ | 5,74 | −1,96 | 1128 | B8III | |
| 7 Ari | | 7 | RR | 11763 | 8993 | 01$^h$ 55$^m$ 51,03$^s$ | +23° 34′ 38,4″ | 5,76 | −0,26 | 522 | K1III | Non-variable (malgré sa désignation RR Ari) |
| ρ$^2$ Ari | ρ$^2$ | 45 | RZ | 18191 | 13654 | 02$^h$ 55$^m$ 48,50$^s$ | +18° 19′ 54,0″ | 5,76 | 0,30 | 403 | M6IIIvar | Variable semi-régulière, V$_{max}$ = 5,45$^m$, V$_{min}$ = 6,01$^m$ |
| ο Ari | ο | 37 | | 17036 | 12803 | 02$^h$ 44$^m$ 32,97$^s$ | +15° 18′ 42,8″ | 5,78 | −0,07 | 482 | B9Vn | |
| 56 Ari | | 56 | SX | 19832 | 14893 | 03$^h$ 12$^m$ 14,24$^s$ | +27° 15′ 25,2″ | 5,78 | 0,50 | 371 | B9p Si | Prototype des variables de type SX Ari, V$_{max}$ = 5,75$^m$, V$_{min}$ = 5,81$^m$, P = 0,727902 j |
| 20 Ari | | 20 | | 13871 | 10540 | 02$^h$ 15$^m$ 45,94$^s$ | +25° 46′ 59,2″ | 5,79 | 2,77 | 131 | F6IV-V | |
| 47 Ari | | 47 | | 18404 | 13834 | 02$^h$ 58$^m$ 05,08$^s$ | +20° 40′ 07,7″ | 5,80 | 3,29 | 104 | F5IV | Variable suspectée |
| 1 Ari A | | 1 | | 11154 | 8544 | 01$^h$ 50$^m$ 08,58$^s$ | +22° 16′ 31,3″ | 5,83 | −0,40 | 574 | K1III+... | Étoile binaire |
| 40 Ari | | 40 | | 17459 | 13108 | 02$^h$ 48$^m$ 32,06$^s$ | +18° 17′ 01,9″ | 5,83 | −0,11 | 502 | K1III | |
| 4 Ari | | 4 | | 10982 | 8387 | 01$^h$ 48$^m$ 10,90$^s$ | +16° 57′ 20,3″ | 5,86 | 1,14 | 287 | B9,5V | |
| | | | | 15524 | 11670 | 02$^h$ 30$^m$ 32,31$^s$ | +25° 14′ 06,8″ | 5,88 | 2,34 | 166 | F6IV | |
| | | | | 12139 | 9307 | 01$^h$ 59$^m$ 35,60$^s$ | +21° 03′ 31,0″ | 5,89 | 0,45 | 399 | K0III-IV | |
| VZ Ari | | (16) | VZ | 17471 | 13121 | 02$^h$ 48$^m$ 45,87$^s$ | +25° 11′ 17,1″ | 5,89 | 0,14 | 460 | A0V | 16 Trianguli ; variable de type α$^2$ CVn, V$_{max}$ = 5,82$^m$, V$_{min}$ = 5,89$^m$ |
| 1 Ari B | | 1 | | 11155 | | 01$^h$ 50$^m$ 08,50$^s$ | +22° 16′ 33,0″ | 5,90 | | | | Composante du système 1 Ari |
| 49 Ari | | 49 | | 18769 | 14109 | 03$^h$ 01$^m$ 54,15$^s$ | +26° 27′ 44,4″ | 5,91 | 1,82 | 214 | A3m | Variable suspectée, V$_{max}$ = 5,90$^m$, V$_{min}$ = 5,94$^m$ |
| 59 Ari | | 59 | | 20618 | 15514 | 03$^h$ 19$^m$ 55,81$^s$ | +27° 04′ 16,7″ | 5,91 | 1,91 | 205 | G8IV | |
| 54 Cet | | (54) | | 11257 | 8588 | 01$^h$ 50$^m$ 52,01$^s$ | +11° 02′ 36,4″ | 5,92 | 2,77 | 139 | F2Vw | Variable suspectée, V$_{max}$ = 5,93$^m$, V$_{min}$ = 5,97$^m$ |
| | | | | 18700 | 14036 | 03$^h$ 00$^m$ 44,09$^s$ | +10° 52′ 13,7″ | 5,93 | 0,27 | 441 | K6 | |
| | | | | 13522 | 10296 | 02$^h$ 12$^m$ 37,51$^s$ | +24° 10′ 04,1″ | 5,96 | −0,23 | 565 | K0 | |
| | | | | 12479 | 9533 | 02$^h$ 02$^m$ 35,08$^s$ | +13° 28′ 36,2″ | 5,97 | −1,10 | 845 | M2III | Variable suspectée |
| | | | | 19698 | 14764 | 03$^h$ 10$^m$ 38,78$^s$ | +11° 52′ 21,7″ | 5,97 | −0,05 | 522 | B8V | |
| 29 Ari | | 29 | | 15814 | 11843 | 02$^h$ 32$^m$ 54,15$^s$ | +15° 02′ 04,1″ | 6,00 | 3,71 | 94 | F8V | |
| 11 Ari | | 11 | | 12885 | 9859 | 02$^h$ 06$^m$ 49,22$^s$ | +25° 42′ 16,5″ | 6,01 | −1,75 | 1160 | B9IV-Vn | |
| 16 Ari | | 16 | | 13363 | 10203 | 02$^h$ 11$^m$ 12,06$^s$ | +25° 56′ 13,0″ | 6,01 | −0,94 | 801 | K4III | |
| | | | | 19637 | 14748 | 03$^h$ 10$^m$ 27,04$^s$ | +26° 53′ 45,9″ | 6,02 | 0,54 | 406 | K3III | |
| 66 Ari | | 66 | | 21467 | 16181 | 03$^h$ 28$^m$ 26,57$^s$ | +22° 48′ 15,4″ | 6,03 | 1,83 | 226 | K0IV | |
| 65 Ari | | 65 | | 21050 | 15870 | 03$^h$ 24$^m$ 26,11$^s$ | +20° 48′ 12,6″ | 6,07 | 1,23 | 303 | A1V | |
| | | | | 12140 | 9295 | 01$^h$ 59$^m$ 25,88$^s$ | +12° 17′ 41,8″ | 6,09 | 1,51 | 269 | A6V | |
| | | | | 19789 | 14821 | 03$^h$ 11$^m$ 21,93$^s$ | +13° 02′ 52,1″ | 6,11 | 0,99 | 344 | K0IIIp | |
| 53 Ari | | 53 | UW | 19374 | 14514 | 03$^h$ 07$^m$ 25,69$^s$ | +17° 52′ 47,9″ | 6,13 | −0,69 | 755 | B1,5V | Étoile en fuite ; non-variable (malgré sa désignation UW Ari) |
| | | | | 15152 | 11415 | 02$^h$ 27$^m$ 07,26$^s$ | +27° 00′ 45,3″ | 6,14 | 0,37 | 464 | K5III | Variable suspectée |
| 26 Ari | | 26 | UU | 15550 | 11678 | 02$^h$ 30$^m$ 38,37$^s$ | +19° 51′ 19,4″ | 6,14 | 1,94 | 226 | A9V | Variable de type δ Sct, V$_{max}$ = 6,10$^m$, V$_{min}$ = 6,15$^m$, P = 0,0676 j |
| 60 Ari | | 60 | | 20663 | 15557 | 03$^h$ 20$^m$ 25,57$^s$ | +25° 39′ 46,7″ | 6,14 | 1,40 | 289 | K3III: | |
| | | | | 15385 | 11578 | 02$^h$ 29$^m$ 13,63$^s$ | +23° 28′ 08,7″ | 6,20 | 1,65 | 264 | A5m | |
| 27 Ari | | 27 | | 15596 | 11698 | 02$^h$ 30$^m$ 54,38$^s$ | +17° 42′ 14,6″ | 6,21 | 1,30 | 313 | G5III-IV | |
| | | | | 12594 | 9627 | 02$^h$ 03$^m$ 42,61$^s$ | +18° 15′ 11,8″ | 6,24 | −1,83 | 1342 | K4III | |
| 54 Ari | | 54 | | 19460 | 14586 | 03$^h$ 08$^m$ 21,09$^s$ | +18° 47′ 42,3″ | 6,24 | 0,03 | 570 | M0III | Variable semi-régulière, V$_{max}$ = 6,25$^m$, V$_{min}$ = 6,28$^m$ |
| | | | | 17918 | 13448 | 02$^h$ 53$^m$ 11,66$^s$ | +16° 29′ 01,0″ | 6,30 | 1,14 | 352 | F5III | |
| 85 Cet | | (85) | | 16861 | 12647 | 02$^h$ 42$^m$ 28,95$^s$ | +10° 44′ 30,4″ | 6,32 | 0,74 | 426 | A2V | Variable suspectée, V$_{max}$ = 6,28$^m$, V$_{min}$ = 6,34$^m$ |
| | | | | 16955 | 12744 | 02$^h$ 43$^m$ 51,25$^s$ | +25° 38′ 18,0″ | 6,35 | 1,19 | 352 | A3V | |
| | | | | 19080 | 14318 | 03$^h$ 04$^m$ 40,65$^s$ | +15° 51′ 22,5″ | 6,37 | −0,06 | 631 | K3III | |
| | | | | 18928 | 14232 | 03$^h$ 03$^m$ 30,11$^s$ | +28° 16′ 11,8″ | 6,38 | 2,89 | 163 | F0V | |
| | | | | 13201 | 10050 | 02$^h$ 09$^m$ 23,03$^s$ | +17° 13′ 28,7″ | 6,40 | 3,43 | 128 | F5V | |
| HD 20367 | | | | 20367 | 15323 | 03$^h$ 17$^m$ 40,12$^s$ | +31° 07′ 37,9″ | 6,40 | 4,23 | 88 | G0 | Possède une exoplanète (b) |
| | | | | 19549 | 14649 | 03$^h$ 09$^m$ 20,10$^s$ | +20° 45′ 40,1″ | 6,41 | 0,45 | 506 | K2 | |
| | | | | 19600 | 14719 | 03$^h$ 10$^m$ 08,83$^s$ | +27° 49′ 11,6″ | 6,42 | 0,09 | 601 | A0V | |
| | | | | 14262 | 10795 | 02$^h$ 18$^m$ 57,96$^s$ | +23° 10′ 04,2″ | 6,45 | 1,34 | 343 | A7V | |
| 36 Ari | | 36 | | 17017 | 12784 | 02$^h$ 44$^m$ 19,09$^s$ | +17° 45′ 50,5″ | 6,46 | 0,89 | 413 | K2III | Variable suspectée, ΔV = 0,07 mag |
| UX Ari | | | UX | 21242 | 16042 | 03$^h$ 26$^m$ 35,36$^s$ | +28° 42′ 55,2″ | 6,47 | 2,97 | 164 | G5IV | Variable de type RS CVn, V$_{max}$ = 6,35$^m$, V$_{min}$ = 6,71$^m$ P = 6,388 j |
| 30 Ari A | | 30 | | 16246 | 12189 | 02$^h$ 37$^m$ 00,44$^s$ | +24° 38′ 50,1″ | 6,48 | 3,46 | 131 | F6III | Étoile binaire |
| 51 Ari | | 51 | | 18803 | 14150 | 03$^h$ 02$^m$ 25,87$^s$ | +26° 36′ 34,7″ | 6,62 | 4,99 | 69 | G8V | |
| VW Ari | | | VW | 15165 | 11390 | 02$^h$ 26$^m$ 45,65$^s$ | +10° 33′ 55,1″ | 6,69 | 1,16 | 416 | F0IV | Variable de type δ Sct, V$_{max}$ = 6,64$^m$, V$_{min}$ = 6,76$^m$, P = 0,1606 j |
| AF Ari | | | AF | 14595 | 11035 | 02$^h$ 22$^m$ 06,62$^s$ | +22° 52′ 24,9″ | 6,71 | 0,50 | 615 | G3III | Variable de type Algol, V$_{max}$ = 6,30$^m$, V$_{min}$ = 7,10$^m$, P = 153 j |
| VY Ari | | | VY | 17433 | 13118 | 02$^h$ 48$^m$ 43,72$^s$ | +31° 06′ 54,7″ | 6,76 | 3,65 | 136,5 | K0 | Variable de type RS CVn, V$_{max}$ = 6,68$^m$, V$_{min}$ = 7,15$^m$, P = 16,1996 j |
| 50 Ari | | 50 | | 18654 | 14021 | 03$^h$ 00$^m$ 31,51$^s$ | +18° 00′ 17,9″ | 6,80 | | | A0V | |
| 23 Ari | | 23 | | 14305 | 10810 | 02$^h$ 19$^m$ 08,72$^s$ | +19° 41′ 15,7″ | 6,83 | | 106 | F8V | |
| 52 Ari B | | 52 | | 19135 | | 03$^h$ 05$^m$ 26,70$^s$ | +25° 15′ 19,0″ | 7,00 | | | | Composante du système 52 Ari |
| ρ$^1$ Ari | ρ$^1$ | 44 | | 18091 | 13579 | 02$^h$ 54$^m$ 55,17$^s$ | +17° 44′ 05,3″ | 7,01 | 2,10 | 313 | A3 | |
| 30 Ari B | | 30 | | 16232 | 12184 | 02$^h$ 36$^m$ 57,64$^s$ | +24° 38′ 53,1″ | 7,10 | 4,12 | 129 | F4V | Composante du système 30 Ari ; possède une planète (b) |
| R Ari | | | R | 13913 | 10576 | 02$^h$ 16$^m$ 07,11$^s$ | +25° 03′ 23,7″ | 7,40 | -2,99 | 3900 | M3-6e | Variable de type Mira, V$_{max}$ = 7,1$^m$, V$_{min}$ = 14,3$^m$, P = 185,67 j |
| HD 12661 | | | | 12661 | | 02$^h$ 04$^m$ 34,29$^s$ | +25° 24′ 51,5″ | 7,44 | | 121 | | Possède deux planètes (b et c) |
| HD 17674 | | | | 17674 | 13291 | 02$^h$ 51$^m$ 04,3$^s$ | +30° 17′ 12″ | 7,56 | | 145 | G0V | Possède deux planètes (b et c) |
| HD 14787 | | | | 14787 | 11130 | 02$^h$ 50$^m$ 53,0$^s$ | +29° 01′ 21″ | 7,63 | | 390 | G5 | Possède une planète (b) |
| HIP 14810 | | | | | 14810 | 03$^h$ 11$^m$ 14,23$^s$ | +21° 05′ 50,5″ | 8,52 | 4,90 | 172 | G5V | Possède trois planètes (b, c et d) |
| BD+20 307 | | | | | 8920 | 01$^h$ 54$^m$ 50,79$^s$ | +21° 18′ 22,5″ | 9,01 | | 300 | | Possède un disque protoplanétaire |
| X Ari | | | X | 19510 | 14601 | 03$^h$ 08$^m$ 30,89$^s$ | +10° 26′ 45,2″ | 9,04 | -1,23 | 3700 | F0,5 | Variable de type RR Lyr, V$_{max}$ = 9,036$^m$, V$_{min}$ = 9,966$^m$, P = 0,6511796 j |
| RX Ari | | | RX | | | 02$^h$ 15$^m$ 20,78$^s$ | +22° 34′ 11,1″ | 9,41 | | | F2V | Variable de type Algol, V$_{max}$ = 9,40$^m$, V$_{min}$ = 10,1$^m$, P = 1,029626 j |
| HAT-P-47 | | | | | | 02$^h$ 33$^m$ 14,0$^s$ | +30° 21′ 38″ | 10,6 | | 874 | | Possède une planète qui transite (b) |
| SS Ari | | | SS | | | 02$^h$ 04$^m$ 18,41$^s$ | +24° 00′ 02,2″ | 10,15 | 3,52 | 692 | G0 | Variable de type W UMa, V$_{max}$ = 10,10$^m$, V$_{min}$ = 10,63$^m$, P = 0,40598257 j |
| TT Ari | | | TT | | | 02$^h$ 06$^m$ 53,08$^s$ | +15° 17′ 41,8″ | 10,2 | | | Bep: | Variable de type VY Scl, V$_{max}$ = 10,2$^m$, V$_{min}$ = 16,5$^m$, P = 0,137551 j |
| RV Ari | | | RV | | | 02$^h$ 15$^m$ 07,50$^s$ | +18° 04′ 27,9″ | 11,61 | | | A0 | Variable de type δ Sct à double mode, V$_{max}$ = 11,61$^m$, V$_{min}$ = 12,30$^m$ |
| WASP-11 | | | | | | 03$^h$ 09$^m$ 28,55$^s$ | +30° 40′ 24,9″ | 11,89 | 6,41 | 408 | K3V | HAT-P-10; Possède une planète qui transite (b) |
| HAT-P-48 | | | | | | 02$^h$ 57$^m$ 53,0$^s$ | +30° 37′ 33″ | 12,16 | | 995 | | Possède une planète qui transite (b) |
| TZ Arietis | | | TZ | | | 02$^h$ 00$^m$ 13,2$^s$ | +13° 03′ 08″ | 12,26 | 13,99 | 14,5 | | 34e système stellaire le plus proche ; étoile éruptive et variable de type BY Dra |
| LkHα 264 | | | WY | | | 02$^h$ 56$^m$ 37,56$^s$ | +20° 05′ 37,1″ | 12,46 | | | K5/6e | Étoile T Tau, V$_{max}$ = 12,25$^m$, V$_{min}$ = 12,88$^m$ |
| RW Ari | | | RW | | | 02$^h$ 16$^m$ 03,72$^s$ | +17° 31′ 59,0″ | 12,51 | | | B8 | Variable de type RR Lyr, V$_{max}$ = 12,12$^m$, V$_{min}$ = 12,60$^m$, P = 0,3543006 j |
| HAT-P-25 | | | | | | 03$^h$ 13$^m$ 45$^s$ | +25° 11′ 51″ | 13,19 | 5,83 | 969 | G5 | Possède une planète qui transite (b) |
| HAT-P-52 | | | | | | 02$^h$ 50$^m$ 53,0$^s$ | +29° 01′ 21″ | 14,07 | 6,14 | 1256 | | Possède une planète qui transite (b) |
| WX Ari | | | WX | | | 02$^h$ 47$^m$ 36,22$^s$ | +10° 35′ 37,7″ | 15,3 | | | CV | Variable de type VY Scl et binaire à éclipses, V$_{max}$ = 14,5$^m$, V$_{min}$ = < 16,7$^m$, P = 0,1393512 j |
| Étoile de Teegarden | | | | | | 02$^h$ 53$^m$ 00,9$^s$ | +16° 52′ 53″ | 15,40 | 17,47 | 12,6 | M7,5 | Naine brune ; 23e système stellaire le plus proche |
| XY Ari | | | XY | | | 02$^h$ 56$^m$ 08,19$^s$ | +19° 26′ 34,1″ | | | | WD+M0V | Variable de type DQ Her et binaire à éclipses |
| PSR B0301+19 | | | | | | 03$^h$ 04$^m$ 33,12$^s$ | +19° 32′ 51,4″ | | | | | Pulsar |