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 | 05h 32m 43.81s | −17° 49′ 20.3″ | 2.58 | −5.40 | 1283 | F0Ib | Arneb (Elarneb), Arsh; suspected variable, Vmax = 2.56m, Vmin = 2.62m | ||||
| β Lep | β | 9 | 36079 | 25606 | 05h 28m 14.73s | −20° 45′ 33.2″ | 2.81 | −0.63 | 159 | G5II | Nihal (Nibal) | ||||
| ε Lep | ε | 2 | 32887 | 23685 | 05h 05m 27.65s | −22° 22′ 15.1″ | 3.19 | −1.02 | 227 | K4III | suspected variable, Vmax = 3.12m, Vmin = 3.20m | ||||
| μ Lep | μ | 5 | 33904 | 24305 | 05h 12m 55.87s | −16° 12′ 19.5″ | 3.29 | −0.47 | 184 | B9IV: HgMn | α2 CVn variable, Vmax = 2.97m, Vmin = 3.41m, P = 2 d | ||||
| ζ Lep | ζ | 14 | 38678 | 27288 | 05h 46m 57.35s | −14° 49′ 19.0″ | 3.55 | 1.89 | 70 | A2Vann | has a possible asteroid belt | ||||
| γ Lep | γ | 13 | 38393 | 27072 | 05h 44m 27.97s | −22° 26′ 51.0″ | 3.59 | 3.83 | 29 | F7V | |||||
| η Lep | η | 16 | 40136 | 28103 | 05h 56m 24.32s | −14° 10′ 04.9″ | 3.71 | 2.82 | 49 | F1V | |||||
| δ Lep | δ | 15 | 39364 | 27654 | 05h 51m 19.15s | −20° 52′ 39.0″ | 3.76 | 1.08 | 112 | G8III/IV | |||||
| λ Lep | λ | 6 | 34816 | 24845 | 05h 19m 34.53s | −13° 10′ 36.4″ | 4.29 | −3.30 | 1076 | B0.5IV | |||||
| κ Lep | κ | 4 | 33949 | 24327 | 05h 13m 13.89s | −12° 56′ 28.6″ | 4.36 | −1.81 | 559 | B7V | suspected variable | ||||
| ι Lep | ι | 3 | 33802 | 24244 | 05h 12m 17.89s | −11° 52′ 08.9″ | 4.45 | 0.11 | 241 | B8V | |||||
| θ Lep | θ | 18 | 41695 | 28910 | 06h 06m 09.33s | −14° 56′ 07.0″ | 4.67 | 1.08 | 170 | A0V | |||||
| HD 34968 | 34968 | 24927 | 05h 20m 26.91s | −21° 14′ 23.1″ | 4.70 | −1.04 | 459 | A0V | suspected variable, Vmax = 4.67m, Vmin = 4.72m | ||||||
| HD 32309 | 32309 | 23362 | 05h 01m 25.56s | −20° 03′ 06.8″ | 4.91 | 0.88 | 209 | B9V | |||||||
| 17 Lep | 17 | SS | 41511 | 28816 | 06h 04m 59.13s | −16° 29′ 03.9″ | 4.92 | −2.66 | 1069 | Ap shell | rotating ellipsoidal and Z And variable, Vmax = 4.82m, Vmin = 5.06m, P = 260.34 d | ||||
| HD 32436 | 32436 | 23430 | 05h 02m 09.77s | −26° 16′ 29.4″ | 5.01 | 0.65 | 242 | K1III | aka HR 1628 | ||||||
| HD 41312 | 41312 | 28675 | 06h 03m 15.56s | −26° 17′ 05.1″ | 5.03 | −0.35 | 388 | K3II/IIICNv | |||||||
| HD 34310 | 34310 | 24505 | 05h 15m 24.37s | −26° 56′ 36.4″ | 5.06 | 0.45 | 272 | B9V | |||||||
| HD 35162 | 35162 | 25045 | 05h 21m 46.27s | −24° 46′ 22.6″ | 5.06 | 0.28 | 294 | A2/A3 | |||||||
| 8 Lep | 8 | 35337 | 25202 | 05h 23m 30.16s | −13° 55′ 38.5″ | 5.25 | −3.47 | 1811 | B2IV | ||||||
| 19 Lep | 19 | 42042 | 29048 | 06h 07m 41.63s | −19° 09′ 57.6″ | 5.28 | −1.41 | 710 | M1III | semiregular variable | |||||
| ν Lep | ν | 7 | 34863 | 24873 | 05h 19m 59.03s | −12° 18′ 56.2″ | 5.29 | 0.25 | 332 | B7/B8V | |||||
| HD 41841 | 41841 | 28943 | 06h 06m 32.10s | −23° 06′ 38.8″ | 5.46 | −0.36 | 475 | A2V | |||||||
| HD 34538 | 34538 | 24679 | 05h 17m 40.25s | −13° 31′ 10.9″ | 5.48 | 2.06 | 158 | G8IV | suspected variable, Vmax = 5.38m, Vmin = 5.50m | ||||||
| HD 39070 | 39070 | 27517 | 05h 49m 36.55s | −14° 29′ 00.8″ | 5.49 | 0.60 | 310 | G8III | |||||||
| HD 42301 | 42301 | 29150 | 06h 08m 57.87s | −22° 25′ 38.2″ | 5.49 | 1.02 | 255 | A0V | |||||||
| 10 Lep | 10 | 36473 | 25853 | 05h 31m 07.62s | −20° 51′ 48.8″ | 5.53 | 0.93 | 272 | A0V | ||||||
| HD 42341 | 42341 | 29205 | 06h 09m 34.53s | −14° 35′ 04.9″ | 5.56 | 1.49 | 212 | K2III | |||||||
| RX Lep | RX | 33664 | 24169 | 05h 11m 22.85s | −11° 50′ 57.2″ | 5.60 | −0.08 | 447 | M6.2III | semiregular variable, Vmax = 5.12m, Vmin = 6.65m, P = 79.54 d | |||||
| HD 32667 | 32667 | 23554 | 05h 03m 53.26s | −24° 23′ 17.0″ | 5.61 | 1.72 | 196 | A2IV | triple star system, aka HR 1645 | ||||||
| HD 39853 | 39853 | 27938 | 05h 54m 43.59s | −11° 46′ 27.3″ | 5.62 | −1.18 | 746 | K3 comp | suspected variable | ||||||
| HD 35505 | 35505 | 25280 | 05h 24m 28.47s | −16° 58′ 32.7″ | 5.64 | 1.50 | 220 | A0V | |||||||
| HD 31925 | 31925 | 23166 | 04h 59m 01.44s | −16° 22′ 34.8″ | 5.65 | 2.47 | 141 | F5V | suspected variable, Vmax = 5.62m, Vmin = 5.69m | ||||||
| HD 32890 | 32890 | 23668 | 05h 05m 16.19s | −26° 09′ 08.1″ | 5.71 | 1.37 | 240 | K2III | |||||||
| HD 42443 | 42443 | 29234 | 06h 09m 47.91s | −22° 46′ 28.2″ | 5.71 | 2.04 | 176 | F5V | |||||||
| HD 42621 | 42621 | 29294 | 06h 10m 34.69s | −27° 09′ 15.1″ | 5.72 | 0.68 | 331 | K1III | |||||||
| HD 38206 | 38206 | 26966 | 05h 43m 21.66s | −18° 33′ 26.8″ | 5.73 | 1.53 | 226 | A0V | |||||||
| 1 Lep | 1 | 32503 | 23474 | 05h 02m 44.94s | −22° 47′ 42.3″ | 5.74 | −0.29 | 524 | K1IV | ||||||
| YY Lep | YY | 41933 | 28984 | 06h 06m 57.52s | −21° 48′ 44.2″ | 5.74 | −1.54 | 931 | M3II/III | semiregular variable | |||||
| HD 35736 | 35736 | 25397 | 05h 25m 59.82s | −19° 41′ 43.3″ | 5.78 | 2.61 | 140 | F5V | |||||||
| HD 39190 | 39190 | 27533 | 05h 49m 53.51s | −22° 58′ 18.9″ | 5.87 | −0.49 | 610 | A1V | |||||||
| 12 Lep | 12 | 38090 | 26865 | 05h 42m 13.96s | −22° 22′ 25.5″ | 5.88 | −0.97 | 765 | A2/A3V | ||||||
| HD 40151 | 40151 | 28085 | 05h 56m 14.20s | −22° 50′ 24.2″ | 5.95 | 1.19 | 292 | K0/K1III | |||||||
| HD 34721 | 34721 | 24786 | 05h 18m 50.24s | −18° 07′ 48.7″ | 5.96 | 3.98 | 81 | G0V | |||||||
| HD 33093 | 33093 | 23831 | 05h 07m 24.88s | −12° 29′ 27.6″ | 5.97 | 3.17 | 118 | G2V | suspected variable | ||||||
| HD 32996 | 32996 | 23777 | 05h 06m 36.73s | −13° 07′ 21.6″ | 6.04 | 0.81 | 363 | B9.5/A0IV | |||||||
| HD 40972 | 40972 | 28520 | 06h 01m 13.11s | −25° 25′ 03.8″ | 6.04 | 0.81 | 363 | A0V | |||||||
| HD 35991 | 35991 | 25532 | 05h 27m 36.49s | −21° 22′ 32.8″ | 6.08 | 0.75 | 380 | K0III | |||||||
| HD 42729 | 42729 | 29347 | 06h 11m 13.66s | −26° 28′ 55.6″ | 6.08 | −0.50 | 675 | B9.5IV/V | |||||||
| HD 37306 | 37306 | 26395 | 05h 37m 08.76s | −11° 46′ 31.7″ | 6.10 | 2.00 | 215 | A2V | |||||||
| HD 38054 | 38054 | 26866 | 05h 42m 14.49s | −17° 31′ 49.4″ | 6.15 | −0.16 | 597 | K3III | |||||||
| HD 38392 | AK | 38392 | 05h 44m 26.50s | −22° 25′ 18.0″ | 6.15 | K2V | common proper motion with γ Lep; BY Draconis variable, ΔV = 0.06m, P = 21.4 d | ||||||||
| HD 39385 | 39385 | 27670 | 05h 51m 28.62s | −22° 55′ 36.6″ | 6.16 | 0.49 | 443 | K0IIICN... | |||||||
| HD 38713 | 38713 | 27308 | 05h 47m 07.81s | −16° 14′ 17.0″ | 6.18 | −0.36 | 664 | G8III | |||||||
| HD 41125 | 41125 | 28622 | 06h 02m 33.81s | −14° 29′ 49.9″ | 6.20 | 0.58 | 434 | K0III | |||||||
| HD 40745 | AC | 40745 | 28434 | 06h 00m 17.66s | −12° 53′ 59.7″ | 6.21 | 2.32 | 195 | F2IV | γ Doradus variable | |||||
| HD 34045 | 34045 | 24394 | 05h 13m 59.94s | −14° 36′ 24.7″ | 6.22 | 1.84 | 245 | A9II/III | |||||||
| HD 37971 | 37971 | 26821 | 05h 41m 41.51s | −16° 43′ 33.0″ | 6.22 | −1.65 | 1221 | B4/B5III | |||||||
| HD 42486 | 42486 | 29233 | 06h 09m 47.16s | −26° 42′ 04.0″ | 6.27 | 0.64 | 435 | G8/K0III | |||||||
| HD 35850 | AF | 35850 | 25486 | 05h 27m 04.75s | −11° 54′ 03.0″ | 6.30 | 4.16 | 87 | F7V: | RS CVn variable, Vmax = 6.26m, Vmin = 6.35m, P = 1 d | |||||
| HD 33162 | 33162 | 23874 | 05h 07m 49.82s | −12° 35′ 32.8″ | 6.33 | −0.52 | 763 | M1III | semiregular variable, Vmax = 6.28m, Vmin = 6.40m, P = 16.62 d | ||||||
| HD 38382 | 38382 | 27075 | 05h 44m 28.41s | −20° 07′ 36.0″ | 6.34 | 4.30 | 83 | F8/G0V | |||||||
| HD 42327 | 42327 | 29178 | 06h 09m 20.20s | −18° 07′ 34.8″ | 6.36 | 0.86 | 410 | B9Vn... | |||||||
| HD 34798 | YZ | 34798 | 24825 | 05h 19m 17.44s | −18° 31′ 11.8″ | 6.37 | −0.56 | 791 | B5IV/V | 53 Per variable | |||||
| HD 40235 | 40235 | 28118 | 05h 56m 34.43s | −23° 12′ 55.4″ | 6.37 | 0.44 | 499 | K0III | |||||||
| HD 33238 | 33238 | 23908 | 05h 08m 13.26s | −15° 05′ 43.3″ | 6.38 | −0.31 | 710 | K1III + F/G | |||||||
| HD 33667 | 33667 | 24114 | 05h 10m 44.59s | −25° 54′ 37.9″ | 6.40 | −0.33 | 724 | K1III/IV | |||||||
| HD 37643 | 37643 | 26602 | 05h 39m 16.23s | −17° 50′ 57.9″ | 6.40 | −1.61 | 1304 | B4 | |||||||
| HD 32612 | 32612 | 23551 | 05h 03m 52.12s | −14° 22′ 12.9″ | 6.42 | −1.62 | 1320 | B2IV | |||||||
| HD 34318 | 34318 | 24560 | 05h 16m 10.56s | −11° 21′ 09.2″ | 6.45 | −0.60 | 838 | G0 | |||||||
| HD 33095 | 33095 | 23818 | 05h 07m 09.78s | −19° 23′ 33.1″ | 6.47 | 3.58 | 123 | G2V | |||||||
| HD 35137 | 35137 | 25059 | 05h 21m 55.31s | −17° 36′ 13.1″ | 6.47 | 0.72 | 461 | K0III | |||||||
| HD 35386 | 35386 | 25180 | 05h 23m 11.98s | −26° 42′ 19.8″ | 6.49 | 2.89 | 171 | F6V | |||||||
| HD 34797 | TX | 34797 | 24827 | 05h 19m 18.31s | −18° 30′ 34.4″ | 6.54 | 799 | B7Vp | α2 CVn variable, ΔV = 0.04m, P = 2.28715 d | ||||||
| S Lep | S | 41698 | 28874 | 06h 05m 45.54s | −24° 11′ 43.9″ | 6.74 | −0.46 | 898 | M5III | semiregular variable, Vmax = 6m, Vmin = 7.58m, P = 97.3 d | |||||
| HD 42659 | UV | 42659 | 29365 | 06h 11m 21.75s | −15° 47′ 35.0″ | 6.77 | 429 | Ap... | rapidly oscillating Ap star | ||||||
| 4 Mon | (4) | 42116 | 29118 | 06h 08m 25.39s | −11° 08′ 46.6″ | 6.90 | 1.80 | 342 | A2 | ||||||
| HD 37847 | TW | 37847 | 26714 | 05h 40m 39.72s | −20° 17′ 55.6″ | 7.00 | 720 | K0IV | RS CVn variable, ΔV = 0.32m, P = 28.84338 d | ||||||
| HD 33844 | 33844 | 24275 | 05h 12m 36.08s | −14° 57′ 04.27″ | 7.30 | 329 | has two planets (b and c) | ||||||||
| T Lep | T | 32803 | 23636 | 05h 04m 50.85s | −21° 54′ 16.5″ | 7.40 | 2670 | M6ev | Mira variable, Vmax = 7.4m, Vmin = 14.3m, P = 372 d | ||||||
| HD 31527 | 31527 | 22905 | 04h 55m 38s | −23° 14′ 31″ | 7.48 | 126 | G0V | has three planets (b, c and d) | |||||||
| R Lep | R | 31996 | 23203 | 04h 59m 36.50s | −14° 48′ 21.0″ | 7.71 | 1350 | C7,6e | Hind's Crimson Star; Mira variable, Vmax = 5.5m, Vmin = 11.7m, P = 445 d | ||||||
| HD 33283 | 33283 | 23889 | 05h 08m 01.01s | −26° 47′ 50.9″ | 8.05 | 3.36 | 282 | G4V | has a planet (b) | ||||||
| HD 33142 | 33142 | 23844 | 05h 07m 36s | −13° 59′ 11″ | 8.13 | 411 | K0III | has a planet (b) | |||||||
| Gliese 229 | 42581 | 29295 | 06h 10m 34.62s | −21° 51′ 52.7″ | 8.14 | 9.33 | 19 | M1/M2V | suspected flare star; has a brown dwarf companion | ||||||
| RY Lep | RY | 38882 | 27400 | 05h 48m 10.25s | −20° 01′ 25.0″ | 8.25 | 647 | A9V | δ Sct variable, Vmax = 8.05m, Vmin = 8.46m, P = 0.2251475 d | ||||||
| HD 32450 | 32450 | 23452 | 05h 02m 28.42s | −21° 15′ 23.9″ | 8.32 | 27.961 | M0V | ||||||||
| RS Lep | RS | 40640 | 05h 59m 18.42s | −20° 13′ 25.1″ | 9.88 | A0V | Algol variable, Vmax = 9.91m, Vmin = 10.38m, P = 1.2885439 d | ||||||||
| TOI-421 | 05h 27m 24.83s | −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 | 04h 56m 17.99s | −21° 13′ 02.0″ | 10.52 | 1910 | A9/F0Iab: | RR Lyr variable, Vmax = 9.890m, Vmin = 11.093m, P = 0.5814789 d | ||||||
| WASP-61 | 05h 01m 12.0s | −26° 03′ 15″ | 12.5 | 1566 | F7 | has a transiting planet (b) | |||||||||
| WASP-49 | 06h 04m 21.47s | −16° 57′ 55″ | 11.35 | 638 | G6 | has a transiting planet (b) | |||||||||
Table legend:
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References
- ESA (1997). "The Hipparcos and Tycho Catalogues". Retrieved 2006-12-26.
- Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26.
- Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 2006-12-26.
- "SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. Retrieved 2007-01-04.
- Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 2012-02-27. Retrieved 2010-07-16.
- "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
