# List of stars in Lepus

This is the list of notable stars in the constellation Lepus, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Lep | α | 11 | | 36673 | 25985 | 05$^h$ 32$^m$ 43.81$^s$ | −17° 49′ 20.3″ | 2.58 | −5.40 | 1283 | F0Ib | Arneb (Elarneb), Arsh; suspected variable, V$_{max}$ = 2.56$^m$, V$_{min}$ = 2.62$^m$ |
| β Lep | β | 9 | | 36079 | 25606 | 05$^h$ 28$^m$ 14.73$^s$ | −20° 45′ 33.2″ | 2.81 | −0.63 | 159 | G5II | Nihal (Nibal) |
| ε Lep | ε | 2 | | 32887 | 23685 | 05$^h$ 05$^m$ 27.65$^s$ | −22° 22′ 15.1″ | 3.19 | −1.02 | 227 | K4III | suspected variable, V$_{max}$ = 3.12$^m$, V$_{min}$ = 3.20$^m$ |
| μ Lep | μ | 5 | | 33904 | 24305 | 05$^h$ 12$^m$ 55.87$^s$ | −16° 12′ 19.5″ | 3.29 | −0.47 | 184 | B9IV: HgMn | α$^2$ CVn variable, V$_{max}$ = 2.97$^m$, V$_{min}$ = 3.41$^m$, P = 2 d |
| ζ Lep | ζ | 14 | | 38678 | 27288 | 05$^h$ 46$^m$ 57.35$^s$ | −14° 49′ 19.0″ | 3.55 | 1.89 | 70 | A2Vann | has a possible asteroid belt |
| γ Lep | γ | 13 | | 38393 | 27072 | 05$^h$ 44$^m$ 27.97$^s$ | −22° 26′ 51.0″ | 3.59 | 3.83 | 29 | F7V | |
| η Lep | η | 16 | | 40136 | 28103 | 05$^h$ 56$^m$ 24.32$^s$ | −14° 10′ 04.9″ | 3.71 | 2.82 | 49 | F1V | |
| δ Lep | δ | 15 | | 39364 | 27654 | 05$^h$ 51$^m$ 19.15$^s$ | −20° 52′ 39.0″ | 3.76 | 1.08 | 112 | G8III/IV | |
| λ Lep | λ | 6 | | 34816 | 24845 | 05$^h$ 19$^m$ 34.53$^s$ | −13° 10′ 36.4″ | 4.29 | −3.30 | 1076 | B0.5IV | |
| κ Lep | κ | 4 | | 33949 | 24327 | 05$^h$ 13$^m$ 13.89$^s$ | −12° 56′ 28.6″ | 4.36 | −1.81 | 559 | B7V | suspected variable |
| ι Lep | ι | 3 | | 33802 | 24244 | 05$^h$ 12$^m$ 17.89$^s$ | −11° 52′ 08.9″ | 4.45 | 0.11 | 241 | B8V | |
| θ Lep | θ | 18 | | 41695 | 28910 | 06$^h$ 06$^m$ 09.33$^s$ | −14° 56′ 07.0″ | 4.67 | 1.08 | 170 | A0V | |
| HD 34968 | | | | 34968 | 24927 | 05$^h$ 20$^m$ 26.91$^s$ | −21° 14′ 23.1″ | 4.70 | −1.04 | 459 | A0V | suspected variable, V$_{max}$ = 4.67$^m$, V$_{min}$ = 4.72$^m$ |
| HD 32309 | | | | 32309 | 23362 | 05$^h$ 01$^m$ 25.56$^s$ | −20° 03′ 06.8″ | 4.91 | 0.88 | 209 | B9V | |
| 17 Lep | | 17 | SS | 41511 | 28816 | 06$^h$ 04$^m$ 59.13$^s$ | −16° 29′ 03.9″ | 4.92 | −2.66 | 1069 | Ap shell | rotating ellipsoidal and Z And variable, V$_{max}$ = 4.82$^m$, V$_{min}$ = 5.06$^m$, P = 260.34 d |
| HD 32436 | | | | 32436 | 23430 | 05$^h$ 02$^m$ 09.77$^s$ | −26° 16′ 29.4″ | 5.01 | 0.65 | 242 | K1III | aka HR 1628 |
| HD 41312 | | | | 41312 | 28675 | 06$^h$ 03$^m$ 15.56$^s$ | −26° 17′ 05.1″ | 5.03 | −0.35 | 388 | K3II/IIICNv | |
| HD 34310 | | | | 34310 | 24505 | 05$^h$ 15$^m$ 24.37$^s$ | −26° 56′ 36.4″ | 5.06 | 0.45 | 272 | B9V | |
| HD 35162 | | | | 35162 | 25045 | 05$^h$ 21$^m$ 46.27$^s$ | −24° 46′ 22.6″ | 5.06 | 0.28 | 294 | A2/A3 | |
| 8 Lep | | 8 | | 35337 | 25202 | 05$^h$ 23$^m$ 30.16$^s$ | −13° 55′ 38.5″ | 5.25 | −3.47 | 1811 | B2IV | |
| 19 Lep | | 19 | | 42042 | 29048 | 06$^h$ 07$^m$ 41.63$^s$ | −19° 09′ 57.6″ | 5.28 | −1.41 | 710 | M1III | semiregular variable |
| ν Lep | ν | 7 | | 34863 | 24873 | 05$^h$ 19$^m$ 59.03$^s$ | −12° 18′ 56.2″ | 5.29 | 0.25 | 332 | B7/B8V | |
| HD 41841 | | | | 41841 | 28943 | 06$^h$ 06$^m$ 32.10$^s$ | −23° 06′ 38.8″ | 5.46 | −0.36 | 475 | A2V | |
| HD 34538 | | | | 34538 | 24679 | 05$^h$ 17$^m$ 40.25$^s$ | −13° 31′ 10.9″ | 5.48 | 2.06 | 158 | G8IV | suspected variable, V$_{max}$ = 5.38$^m$, V$_{min}$ = 5.50$^m$ |
| HD 39070 | | | | 39070 | 27517 | 05$^h$ 49$^m$ 36.55$^s$ | −14° 29′ 00.8″ | 5.49 | 0.60 | 310 | G8III | |
| HD 42301 | | | | 42301 | 29150 | 06$^h$ 08$^m$ 57.87$^s$ | −22° 25′ 38.2″ | 5.49 | 1.02 | 255 | A0V | |
| 10 Lep | | 10 | | 36473 | 25853 | 05$^h$ 31$^m$ 07.62$^s$ | −20° 51′ 48.8″ | 5.53 | 0.93 | 272 | A0V | |
| HD 42341 | | | | 42341 | 29205 | 06$^h$ 09$^m$ 34.53$^s$ | −14° 35′ 04.9″ | 5.56 | 1.49 | 212 | K2III | |
| RX Lep | | | RX | 33664 | 24169 | 05$^h$ 11$^m$ 22.85$^s$ | −11° 50′ 57.2″ | 5.60 | −0.08 | 447 | M6.2III | semiregular variable, V$_{max}$ = 5.12$^m$, V$_{min}$ = 6.65$^m$, P = 79.54 d |
| HD 32667 | | | | 32667 | 23554 | 05$^h$ 03$^m$ 53.26$^s$ | −24° 23′ 17.0″ | 5.61 | 1.72 | 196 | A2IV | triple star system, aka HR 1645 |
| HD 39853 | | | | 39853 | 27938 | 05$^h$ 54$^m$ 43.59$^s$ | −11° 46′ 27.3″ | 5.62 | −1.18 | 746 | K3 comp | suspected variable |
| HD 35505 | | | | 35505 | 25280 | 05$^h$ 24$^m$ 28.47$^s$ | −16° 58′ 32.7″ | 5.64 | 1.50 | 220 | A0V | |
| HD 31925 | | | | 31925 | 23166 | 04$^h$ 59$^m$ 01.44$^s$ | −16° 22′ 34.8″ | 5.65 | 2.47 | 141 | F5V | suspected variable, V$_{max}$ = 5.62$^m$, V$_{min}$ = 5.69$^m$ |
| HD 32890 | | | | 32890 | 23668 | 05$^h$ 05$^m$ 16.19$^s$ | −26° 09′ 08.1″ | 5.71 | 1.37 | 240 | K2III | |
| HD 42443 | | | | 42443 | 29234 | 06$^h$ 09$^m$ 47.91$^s$ | −22° 46′ 28.2″ | 5.71 | 2.04 | 176 | F5V | |
| HD 42621 | | | | 42621 | 29294 | 06$^h$ 10$^m$ 34.69$^s$ | −27° 09′ 15.1″ | 5.72 | 0.68 | 331 | K1III | |
| HD 38206 | | | | 38206 | 26966 | 05$^h$ 43$^m$ 21.66$^s$ | −18° 33′ 26.8″ | 5.73 | 1.53 | 226 | A0V | |
| 1 Lep | | 1 | | 32503 | 23474 | 05$^h$ 02$^m$ 44.94$^s$ | −22° 47′ 42.3″ | 5.74 | −0.29 | 524 | K1IV | |
| YY Lep | | | YY | 41933 | 28984 | 06$^h$ 06$^m$ 57.52$^s$ | −21° 48′ 44.2″ | 5.74 | −1.54 | 931 | M3II/III | semiregular variable |
| HD 35736 | | | | 35736 | 25397 | 05$^h$ 25$^m$ 59.82$^s$ | −19° 41′ 43.3″ | 5.78 | 2.61 | 140 | F5V | |
| HD 39190 | | | | 39190 | 27533 | 05$^h$ 49$^m$ 53.51$^s$ | −22° 58′ 18.9″ | 5.87 | −0.49 | 610 | A1V | |
| 12 Lep | | 12 | | 38090 | 26865 | 05$^h$ 42$^m$ 13.96$^s$ | −22° 22′ 25.5″ | 5.88 | −0.97 | 765 | A2/A3V | |
| HD 40151 | | | | 40151 | 28085 | 05$^h$ 56$^m$ 14.20$^s$ | −22° 50′ 24.2″ | 5.95 | 1.19 | 292 | K0/K1III | |
| HD 34721 | | | | 34721 | 24786 | 05$^h$ 18$^m$ 50.24$^s$ | −18° 07′ 48.7″ | 5.96 | 3.98 | 81 | G0V | |
| HD 33093 | | | | 33093 | 23831 | 05$^h$ 07$^m$ 24.88$^s$ | −12° 29′ 27.6″ | 5.97 | 3.17 | 118 | G2V | suspected variable |
| HD 32996 | | | | 32996 | 23777 | 05$^h$ 06$^m$ 36.73$^s$ | −13° 07′ 21.6″ | 6.04 | 0.81 | 363 | B9.5/A0IV | |
| HD 40972 | | | | 40972 | 28520 | 06$^h$ 01$^m$ 13.11$^s$ | −25° 25′ 03.8″ | 6.04 | 0.81 | 363 | A0V | |
| HD 35991 | | | | 35991 | 25532 | 05$^h$ 27$^m$ 36.49$^s$ | −21° 22′ 32.8″ | 6.08 | 0.75 | 380 | K0III | |
| HD 42729 | | | | 42729 | 29347 | 06$^h$ 11$^m$ 13.66$^s$ | −26° 28′ 55.6″ | 6.08 | −0.50 | 675 | B9.5IV/V | |
| HD 37306 | | | | 37306 | 26395 | 05$^h$ 37$^m$ 08.76$^s$ | −11° 46′ 31.7″ | 6.10 | 2.00 | 215 | A2V | |
| HD 38054 | | | | 38054 | 26866 | 05$^h$ 42$^m$ 14.49$^s$ | −17° 31′ 49.4″ | 6.15 | −0.16 | 597 | K3III | |
| HD 38392 | | | AK | 38392 | | 05$^h$ 44$^m$ 26.50$^s$ | −22° 25′ 18.0″ | 6.15 | | | K2V | common proper motion with γ Lep; BY Draconis variable, ΔV = 0.06$^m$, P = 21.4 d |
| HD 39385 | | | | 39385 | 27670 | 05$^h$ 51$^m$ 28.62$^s$ | −22° 55′ 36.6″ | 6.16 | 0.49 | 443 | K0IIICN... | |
| HD 38713 | | | | 38713 | 27308 | 05$^h$ 47$^m$ 07.81$^s$ | −16° 14′ 17.0″ | 6.18 | −0.36 | 664 | G8III | |
| HD 41125 | | | | 41125 | 28622 | 06$^h$ 02$^m$ 33.81$^s$ | −14° 29′ 49.9″ | 6.20 | 0.58 | 434 | K0III | |
| HD 40745 | | | AC | 40745 | 28434 | 06$^h$ 00$^m$ 17.66$^s$ | −12° 53′ 59.7″ | 6.21 | 2.32 | 195 | F2IV | γ Doradus variable |
| HD 34045 | | | | 34045 | 24394 | 05$^h$ 13$^m$ 59.94$^s$ | −14° 36′ 24.7″ | 6.22 | 1.84 | 245 | A9II/III | |
| HD 37971 | | | | 37971 | 26821 | 05$^h$ 41$^m$ 41.51$^s$ | −16° 43′ 33.0″ | 6.22 | −1.65 | 1221 | B4/B5III | |
| HD 42486 | | | | 42486 | 29233 | 06$^h$ 09$^m$ 47.16$^s$ | −26° 42′ 04.0″ | 6.27 | 0.64 | 435 | G8/K0III | |
| HD 35850 | | | AF | 35850 | 25486 | 05$^h$ 27$^m$ 04.75$^s$ | −11° 54′ 03.0″ | 6.30 | 4.16 | 87 | F7V: | RS CVn variable, V$_{max}$ = 6.26$^m$, V$_{min}$ = 6.35$^m$, P = 1 d |
| HD 33162 | | | | 33162 | 23874 | 05$^h$ 07$^m$ 49.82$^s$ | −12° 35′ 32.8″ | 6.33 | −0.52 | 763 | M1III | semiregular variable, V$_{max}$ = 6.28$^m$, V$_{min}$ = 6.40$^m$, P = 16.62 d |
| HD 38382 | | | | 38382 | 27075 | 05$^h$ 44$^m$ 28.41$^s$ | −20° 07′ 36.0″ | 6.34 | 4.30 | 83 | F8/G0V | |
| HD 42327 | | | | 42327 | 29178 | 06$^h$ 09$^m$ 20.20$^s$ | −18° 07′ 34.8″ | 6.36 | 0.86 | 410 | B9Vn... | |
| HD 34798 | | | YZ | 34798 | 24825 | 05$^h$ 19$^m$ 17.44$^s$ | −18° 31′ 11.8″ | 6.37 | −0.56 | 791 | B5IV/V | 53 Per variable |
| HD 40235 | | | | 40235 | 28118 | 05$^h$ 56$^m$ 34.43$^s$ | −23° 12′ 55.4″ | 6.37 | 0.44 | 499 | K0III | |
| HD 33238 | | | | 33238 | 23908 | 05$^h$ 08$^m$ 13.26$^s$ | −15° 05′ 43.3″ | 6.38 | −0.31 | 710 | K1III + F/G | |
| HD 33667 | | | | 33667 | 24114 | 05$^h$ 10$^m$ 44.59$^s$ | −25° 54′ 37.9″ | 6.40 | −0.33 | 724 | K1III/IV | |
| HD 37643 | | | | 37643 | 26602 | 05$^h$ 39$^m$ 16.23$^s$ | −17° 50′ 57.9″ | 6.40 | −1.61 | 1304 | B4 | |
| HD 32612 | | | | 32612 | 23551 | 05$^h$ 03$^m$ 52.12$^s$ | −14° 22′ 12.9″ | 6.42 | −1.62 | 1320 | B2IV | |
| HD 34318 | | | | 34318 | 24560 | 05$^h$ 16$^m$ 10.56$^s$ | −11° 21′ 09.2″ | 6.45 | −0.60 | 838 | G0 | |
| HD 33095 | | | | 33095 | 23818 | 05$^h$ 07$^m$ 09.78$^s$ | −19° 23′ 33.1″ | 6.47 | 3.58 | 123 | G2V | |
| HD 35137 | | | | 35137 | 25059 | 05$^h$ 21$^m$ 55.31$^s$ | −17° 36′ 13.1″ | 6.47 | 0.72 | 461 | K0III | |
| HD 35386 | | | | 35386 | 25180 | 05$^h$ 23$^m$ 11.98$^s$ | −26° 42′ 19.8″ | 6.49 | 2.89 | 171 | F6V | |
| HD 34797 | | | TX | 34797 | 24827 | 05$^h$ 19$^m$ 18.31$^s$ | −18° 30′ 34.4″ | 6.54 | | 799 | B7Vp | α$^2$ CVn variable, ΔV = 0.04$^m$, P = 2.28715 d |
| S Lep | | | S | 41698 | 28874 | 06$^h$ 05$^m$ 45.54$^s$ | −24° 11′ 43.9″ | 6.74 | −0.46 | 898 | M5III | semiregular variable, V$_{max}$ = 6$^m$, V$_{min}$ = 7.58$^m$, P = 97.3 d |
| HD 42659 | | | UV | 42659 | 29365 | 06$^h$ 11$^m$ 21.75$^s$ | −15° 47′ 35.0″ | 6.77 | | 429 | Ap... | rapidly oscillating Ap star |
| 4 Mon | | (4) | | 42116 | 29118 | 06$^h$ 08$^m$ 25.39$^s$ | −11° 08′ 46.6″ | 6.90 | 1.80 | 342 | A2 | |
| HD 37847 | | | TW | 37847 | 26714 | 05$^h$ 40$^m$ 39.72$^s$ | −20° 17′ 55.6″ | 7.00 | | 720 | K0IV | RS CVn variable, ΔV = 0.32$^m$, P = 28.84338 d |
| HD 33844 | | | | 33844 | 24275 | 05$^h$ 12$^m$ 36.08$^s$ | −14° 57′ 04.27″ | 7.30 | | 329 | | has two planets (b and c) |
| T Lep | | | T | 32803 | 23636 | 05$^h$ 04$^m$ 50.85$^s$ | −21° 54′ 16.5″ | 7.40 | | 2670 | M6ev | Mira variable, V$_{max}$ = 7.4$^m$, V$_{min}$ = 14.3$^m$, P = 372 d |
| HD 31527 | | | | 31527 | 22905 | 04$^h$ 55$^m$ 38$^s$ | −23° 14′ 31″ | 7.48 | | 126 | G0V | has three planets (b, c and d) |
| R Lep | | | R | 31996 | 23203 | 04$^h$ 59$^m$ 36.50$^s$ | −14° 48′ 21.0″ | 7.71 | | 1350 | C7,6e | Hind's Crimson Star; Mira variable, V$_{max}$ = 5.5$^m$, V$_{min}$ = 11.7$^m$, P = 445 d |
| HD 33283 | | | | 33283 | 23889 | 05$^h$ 08$^m$ 01.01$^s$ | −26° 47′ 50.9″ | 8.05 | 3.36 | 282 | G4V | has a planet (b) |
| HD 33142 | | | | 33142 | 23844 | 05$^h$ 07$^m$ 36$^s$ | −13° 59′ 11″ | 8.13 | | 411 | K0III | has a planet (b) |
| Gliese 229 | | | | 42581 | 29295 | 06$^h$ 10$^m$ 34.62$^s$ | −21° 51′ 52.7″ | 8.14 | 9.33 | 19 | M1/M2V | suspected flare star; has a brown dwarf companion |
| RY Lep | | | RY | 38882 | 27400 | 05$^h$ 48$^m$ 10.25$^s$ | −20° 01′ 25.0″ | 8.25 | | 647 | A9V | δ Sct variable, V$_{max}$ = 8.05$^m$, V$_{min}$ = 8.46$^m$, P = 0.2251475 d |
| HD 32450 | | | | 32450 | 23452 | 05$^h$ 02$^m$ 28.42$^s$ | −21° 15′ 23.9″ | 8.32 | | 27.961 | M0V | |
| RS Lep | | | RS | 40640 | | 05$^h$ 59$^m$ 18.42$^s$ | −20° 13′ 25.1″ | 9.88 | | | A0V | Algol variable, V$_{max}$ = 9.91$^m$, V$_{min}$ = 10.38$^m$, P = 1.2885439 d |
| TOI-421 | | | | | | 05$^h$ 27$^m$ 24.83$^s$ | −14° 16′ 37.0″ | 9.93 | | 245 | G9V | has a red dwarf visual binary; has two transiting planets (b, c) |
| U Lep | | | U | 31599 | 22952 | 04$^h$ 56$^m$ 17.99$^s$ | −21° 13′ 02.0″ | 10.52 | | 1910 | A9/F0Iab: | RR Lyr variable, V$_{max}$ = 9.890$^m$, V$_{min}$ = 11.093$^m$, P = 0.5814789 d |
| WASP-61 | | | | | | 05$^h$ 01$^m$ 12.0$^s$ | −26° 03′ 15″ | 12.5 | | 1566 | F7 | has a transiting planet (b) |
| WASP-49 | | | | | | 06$^h$ 04$^m$ 21.47$^s$ | −16° 57′ 55″ | 11.35 | | 638 | G6 | has a transiting planet (b) |
| 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.] |||||||||||||