# List of stars in Aries

This is the list of notable stars in the constellation Aries, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| Hamal | 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; suspected variable, V$_{max}$ = 1.98$^m$, V$_{min}$ = 2.04$^m$; has a planet (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; suspected variable, 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; suspected variable, 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, Nir al Botain, Lucida Ventris, part of Al Buṭain; suspected variable, V$_{max}$ = 4.33$^m$, V$_{min}$ = 4.37$^m$ |
| HD 20644 | | | | 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 | γ$^2$ | 5 | | 11503 | | 01$^h$ 53$^m$ 31.80$^s$ | +19° 17′ 45.0″ | 4.62 | 1.11 | 164.0 | kA0hA3(IV)SiSr | Mesarthim, Mesartim; binary star; α$^2$ CVn variable, ΔV = 0.04$^m$, P = 1.6092 d |
| 35 Ari | | 35 | | 16908 | 12719 | 02$^h$ 43$^m$ 27.11$^s$ | +27° 42′ 25.8″ | 4.65 | −0.62 | 370 | B3V | |
| γ$^1$ Ari | γ$^1$ | 5 | | 11502 | 8832 | 01$^h$ 53$^m$ 31.77$^s$ | +19° 17′ 38.7″ | 4.70 | 1.19 | 164.0 | B9.5IV | component of the γ Ari system |
| λ Ari | λ | 9 | | 11973 | 9153 | 01$^h$ 57$^m$ 55.78$^s$ | +23° 35′ 45.9″ | 4.79 | 1.73 | 133 | F0V | binary star |
| ζ Ari | ζ | 58 | | 20150 | 15110 | 03$^h$ 14$^m$ 54.11$^s$ | +21° 02′ 40.7″ | 4.87 | −0.22 | 340 | A1V | part of Al Buṭain |
| 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 | spectroscopic binary |
| ι Ari | ι | 8 | | 11909 | 9110 | 01$^h$ 57$^m$ 21.03$^s$ | +17° 49′ 03.3″ | 5.09 | −1.44 | 659 | K1p... | spectroscopic binary |
| 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″ | 5.18 | 2.26 | 125 | A7III-IV | δ Sct variable, V$_{max}$ = 5.18$^m$, V$_{min}$ = 5.22$^m$, P = 0.0355 d |
| ε Ari A | ε | 48 | | 18519 | | 02$^h$ 59$^m$ 12.70$^s$ | +21° 20′ 25.0″ | 5.2 | 0.16 | 332 | A2Vs | part of Al Buṭain; binary star |
| 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 | part of Al Buṭain; spectroscopic binary |
| τ$^1$ Ari | τ$^1$ | 61 | | 20756 | 15627 | 03$^h$ 21$^m$ 13.61$^s$ | +21° 08′ 49.7″ | 5.27 | −0.49 | 462 | B5IV | triple star system; Beta Lyrae variable |
| 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 | binary star |
| ξ Ari | ξ | 24 | | 14951 | 11249 | 02$^h$ 24$^m$ 49.04$^s$ | +10° 36′ 38.2″ | 5.48 | −0.85 | 603 | B7IV | variable star, ΔV = 0.007$^m$, P = 1.73515 d |
| ε Ari B | ε | 48 | | 18519 | 13914 | 02$^h$ 59$^m$ 12.73$^s$ | +21° 20′ 25.6″ | 5.5 | 0.46 | 332 | A2Vs | component of the ε Ari system |
| 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 | part of Al Buṭain; suspected BY Dra variable |
| HD 20149 | | | | 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 | |
| HD 19270 | | | | 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 | semiregular variable, V$_{max}$ = 5.67$^m$, V$_{min}$ = 5.74$^m$, P = 5.0320 d |
| 19 Ari | | 19 | | 13596 | 10328 | 02$^h$ 13$^m$ 03.25$^s$ | +15° 16′ 47.7″ | 5.72 | −0.38 | 541 | M0III | suspected variable, 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 | not variable |
| 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 | semiregular variable, 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 SX Ari variable, V$_{max}$ = 5.75$^m$, V$_{min}$ = 5.81$^m$, P = 0.727902 d |
| 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 | suspected variable |
| 1 Ari A | | 1 | | 11154 | 8544 | 01$^h$ 50$^m$ 08.58$^s$ | +22° 16′ 31.3″ | 5.83 | −0.40 | 574 | K1III+... | binary star |
| 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 | |
| HD 15524 | | | | 15524 | 11670 | 02$^h$ 30$^m$ 32.31$^s$ | +25° 14′ 06.8″ | 5.88 | 2.34 | 166 | F6IV | |
| HD 12139 | | | | 12139 | 9307 | 01$^h$ 59$^m$ 35.60$^s$ | +21° 03′ 31.0″ | 5.89 | 0.45 | 399 | K0III-IV | |
| HR 830 | | (16) | VZ | 17471 | 13121 | 02$^h$ 48$^m$ 45.87$^s$ | +25° 11′ 17.1″ | 5.89 | 0.14 | 460 | A0V | 16 Trianguli; Alpha² CVn variable, 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 | | | | component of the 1 Ari system |
| 49 Ari | | 49 | | 18769 | 14109 | 03$^h$ 01$^m$ 54.15$^s$ | +26° 27′ 44.4″ | 5.91 | 1.82 | 214 | A3m | suspected variable, 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″ | 5.93 | 2.77 | 139 | F2Vw | suspected variable, V$_{max}$ = 5.93$^m$, V$_{min}$ = 5.97$^m$ |
| HD 18700 | | | | 18700 | 14036 | 03$^h$ 00$^m$ 44.09$^s$ | +10° 52′ 13.7″ | 5.93 | 0.27 | 441 | K6 | |
| HD 13522 | | | | 13522 | 10296 | 02$^h$ 12$^m$ 37.51$^s$ | +24° 10′ 04.1″ | 5.96 | −0.23 | 565 | K0 | |
| HD 12479 | | | | 12479 | 9533 | 02$^h$ 02$^m$ 35.08$^s$ | +13° 28′ 36.2″ | 5.97 | −1.10 | 845 | M2III | suspected variable |
| HD 19698 | | | | 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 | |
| HD 19637 | | | | 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 | |
| HD 12140 | | | | 12140 | 9295 | 01$^h$ 59$^m$ 25.88$^s$ | +12° 17′ 41.8″ | 6.09 | 1.51 | 269 | A6V | |
| HD 19789 | | | | 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 | not variable; runaway star |
| HD 15152 | | | | 15152 | 11415 | 02$^h$ 27$^m$ 07.26$^s$ | +27° 00′ 45.3″ | 6.14 | 0.37 | 464 | K5III | suspected variable |
| 26 Ari | | 26 | UU | 15550 | 11678 | 02$^h$ 30$^m$ 38.37$^s$ | +19° 51′ 19.4″ | 6.14 | 1.94 | 226 | A9V | δ Sct variable, V$_{max}$ = 6.10$^m$, V$_{min}$ = 6.15$^m$, P = 0.0676 d |
| 60 Ari | | 60 | | 20663 | 15557 | 03$^h$ 20$^m$ 25.57$^s$ | +25° 39′ 46.7″ | 6.14 | 1.40 | 289 | K3III: | |
| HD 15385 | | | | 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 | |
| HD 12594 | | | | 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″ | 6.25 | 0.03 | 570 | M0III | semiregular variable, V$_{max}$ = 6.25$^m$, V$_{min}$ = 6.28$^m$ |
| HD 17918 | | | | 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 | suspected variable, V$_{max}$ = 6.28$^m$, V$_{min}$ = 6.34$^m$ |
| HD 16955 | | | | 16955 | 12744 | 02$^h$ 43$^m$ 51.25$^s$ | +25° 38′ 18.0″ | 6.35 | 1.19 | 352 | A3V | |
| HD 19080 | | | | 19080 | 14318 | 03$^h$ 04$^m$ 40.65$^s$ | +15° 51′ 22.5″ | 6.37 | −0.06 | 631 | K3III | |
| HD 18928 | | | | 18928 | 14232 | 03$^h$ 03$^m$ 30.11$^s$ | +28° 16′ 11.8″ | 6.38 | 2.89 | 163 | F0V | |
| HD 13201 | | | | 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$^m$ 40.0468$^s$ | +31° 07′ 37.9″ | 6.40 | 4.23 | 88 | G0V | has a planet (b) |
| HD 19549 | | | | 19549 | 14649 | 03$^h$ 09$^m$ 20.10$^s$ | +20° 45′ 40.1″ | 6.41 | 0.45 | 506 | K2 | |
| HD 19600 | | | | 19600 | 14719 | 03$^h$ 10$^m$ 08.83$^s$ | +27° 49′ 11.6″ | 6.42 | 0.09 | 601 | A0V | |
| HD 14262 | | | | 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 | suspected variable, ΔV = 0.07$^m$ |
| UX Ari | | | UX | 21242 | 16042 | 03$^h$ 26$^m$ 35.36$^s$ | +28° 42′ 55.2″ | 6.47 | 2.97 | 164 | G5IV | RS CVn variable, V$_{max}$ = 6.35$^m$, V$_{min}$ = 6.71$^m$, P = 6.388 d |
| 30 Ari A | | 30 | | 16246 | 12189 | 02$^h$ 37$^m$ 00.44$^s$ | +24° 38′ 50.1″ | 6.48 | 3.46 | 131 | F6III | binary star |
| HD 14067 | | | | 14067 | 10657 | 02$^h$ 17$^m$ 10.4$^s$ | +23° 46′ 04″ | 6.51 | 0.44 | 533 | G9 III | has a planet (b) |
| 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 | δ Sct variable, V$_{max}$ = 6.64$^m$, V$_{min}$ = 6.76$^m$, P = 0.1606 d |
| AF Ari | | | AF | 14595 | 11035 | 02$^h$ 22$^m$ 06.62$^s$ | +22° 52′ 24.9″ | 6.71 | 0.50 | 615 | G3III | Algol type variable, V$_{max}$ = 6.30$^m$, V$_{min}$ = 7.10$^m$, P = 153 d |
| VY Ari | | | VY | 17433 | 13118 | 02$^h$ 48$^m$ 43.72$^s$ | +31° 06′ 54.7″ | 6.76 | 3.65 | 136.5 | K0 | RS CVn variable, V$_{max}$ = 6.68$^m$, V$_{min}$ = 7.15$^m$, P = 16.1996 d |
| 50 Ari | | 50 | | 18654 | 14021 | 03$^h$ 00$^m$ 31.50536$^s$ | +18° 00′ 17.9143″ | 6.80 | | | A0V | |
| 23 Ari | | 23 | | 14305 | 10810 | 02$^h$ 19$^m$ 08.72041$^s$ | +19° 41′ 15.7463″ | 6.83 | | | F8V | |
| 52 Ari B | | 52 | | 19135 | | 03$^h$ 05$^m$ 26.70$^s$ | +25° 15′ 19.0″ | 7.00 | | | | component of the 52 Ari system |
| 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″ | 7.09 | 4.11 | 129 | F6V | component of the 30 Ari system; has a planet (b) |
| R Ari | | | R | 13913 | 10576 | 02$^h$ 16$^m$ 07.11$^s$ | +25° 03′ 23.7″ | 7.40 | -2.99 | 3900 | M3-6e | Mira variable, V$_{max}$ = 7.1$^m$, V$_{min}$ = 14.3$^m$, P = 185.67 d |
| HD 12661 | | | | 12661 | 9683 | 02$^h$ 04$^m$ 34.29$^s$ | +25° 24′ 51.5″ | 7.44 | 4.59 | 121 | K0V | has two planets (b & c) |
| HD 17674 | | | | 17674 | 13291 | 02$^h$ 51$^m$ 04.3$^s$ | +30° 17′ 12″ | 7.56 | | 145 | G0V | has two planets (b) |
| HD 14787 | | | | 14787 | 11130 | 02$^h$ 50$^m$ 53.0$^s$ | +29° 01′ 21″ | 7.63 | | 390 | G5 | has a planet (b) |
| HIP 14810 | | | | | 14810 | 03$^h$ 11$^m$ 14.23$^s$ | +21° 05′ 50.5″ | 8.52 | 4.90 | 172 | G5V | has three planets (b, c & d) |
| BD +20°307 | | | | | 8920 | 01$^h$ 54$^m$ 50.79$^s$ | +21° 18′ 22.5″ | 9.01 | 4.19 | 300 | G0V | has a circumstellar disk |
| X Ari | | | X | 19510 | 14601 | 03$^h$ 08$^m$ 30.89$^s$ | +10° 26′ 45.2″ | 9.04 | -1.23 | 3700 | F0.5 | RR Lyr variable, V$_{max}$ = 9.036$^m$, V$_{min}$ = 9.966$^m$, P = 0.6511796 d |
| RX Ari | | | RX | | | 02$^h$ 15$^m$ 20.78$^s$ | +22° 34′ 11.1″ | 9.41 | | | F2V | Algol variable, V$_{max}$ = 9.40$^m$, V$_{min}$ = 10.1$^m$, P = 1.029626 d |
| HAT-P-47 | | | | | | 02$^h$ 33$^m$ 14.0$^s$ | +30° 21′ 38″ | 10.6 | | 874 | | has a transiting planet (b) |
| SS Ari | | | SS | | | 02$^h$ 04$^m$ 18.41$^s$ | +24° 00′ 02.2″ | 10.15 | 3.52 | 692 | G0 | W UMa variable, V$_{max}$ = 10.10$^m$, V$_{min}$ = 10.63$^m$, P = 0.40598257 d |
| TT Ari | | | TT | | | 02$^h$ 06$^m$ 53.08$^s$ | +15° 17′ 41.8″ | 10.2 | | | Bep: | VY Scl star, V$_{max}$ = 10.2$^m$, V$_{min}$ = 16.5$^m$, P = 0.137551 d |
| RV Ari | | | RV | | | 02$^h$ 15$^m$ 07.50$^s$ | +18° 04′ 27.9″ | 11.61 | | | A0 | double-mode δ Sct variable, V$_{max}$ = 11.61$^m$, V$_{min}$ = 12.30$^m$, P = 0.0931281 d |
| WASP-11/HAT-P-10 | | | | | | 03$^h$ 09$^m$ 28.55$^s$ | +30° 40′ 24.9″ | 11.89 | 6.41 | 408 | K3V | has a transiting planet (b) |
| HAT-P-48 | | | | | | 02$^h$ 57$^m$ 53.0$^s$ | +30° 37′ 33″ | 12.16 | | 995 | | has a transiting planet (b) |
| L 1159-16 | | | TZ | | | 02$^h$ 00$^m$ 12.79$^s$ | +13° 03′ 11.2″ | 12.26 | 13.99 | 14.5 | M4.5 | flare star and BY Dra variable |
| LkHα 264 | | | WY | | | 02$^h$ 56$^m$ 37.56$^s$ | +20° 05′ 37.1″ | 12.46 | | | K5/6e | T Tau star, 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 | RR Lyr variable, V$_{max}$ = 12.12$^m$, V$_{min}$ = 12.60$^m$, P = 0.3543006 d |
| HAT-P-25 | | | | | | 03$^h$ 13$^m$ 45$^s$ | +25° 11′ 51″ | 13.19 | 5.83 | 969 | G5 | has a transiting planet (b) |
| HAT-P-52 | | | | | | 02$^h$ 50$^m$ 53.0$^s$ | +29° 01′ 21″ | 14.07 | 6.14 | 1256 | | has a transiting planet (b) |
| WX Ari | | | WX | | | 02$^h$ 47$^m$ 36.22$^s$ | +10° 35′ 37.7″ | 15.3 | | | CV | VY Scl star and eclipsing binary, V$_{max}$ = 14.5$^m$, V$_{min}$ = <16.7$^m$, P = 0.1393512 d |
| Teegarden's star | | | | | | 02$^h$ 53$^m$ 00.89$^s$ | +16° 52′ 52.7″ | 15.40 | 17.47 | 12.6 | M7.5 | |
| XY Ari | | | XY | | | 02$^h$ 56$^m$ 08.19$^s$ | +19° 26′ 34.1″ | | | | WD+M0V | DQ Her variable and eclipsing binary |
| PSR B0301+19 | | | | | | 03$^h$ 04$^m$ 33.12$^s$ | +19° 32′ 51.4″ | | | | | pulsar |
| 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.] |||||||||||||