# List of stars in Libra

This is the list of notable stars in the constellation Libra, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| β Lib | β | 27 | | 135742 | 74785 | 15$^h$ 17$^m$ 00.47$^s$ | −09° 22′ 58.3″ | 2.61 | −0.84 | 160 | B8V | Zubeneschamali; suspected variable |
| α$^2$ Lib | α$^2$ | 9 | | 130841 | 72622 | 14$^h$ 50$^m$ 52.78$^s$ | −16° 02′ 29.8″ | 2.75 | 0.88 | 77 | A3IV | Zubenelgenubi; spectroscopic binary; suspected variable; member of the α Lib system |
| σ Lib | σ | 20 | | 133216 | 73714 | 15$^h$ 04$^m$ 04.26$^s$ | −25° 16′ 54.7″ | 3.25 | −1.51 | 292 | M3/M4III | previously γ Scorpii, Brachium; semiregular variable, V$_{max}$ = 3.2$^m$, V$_{min}$ = 3.46$^m$, P = 20 d |
| υ Lib | υ | 39 | | 139063 | 76470 | 15$^h$ 37$^m$ 01.46$^s$ | −28° 08′ 06.3″ | 3.60 | −0.28 | 195 | K3III | previously o Scorpii |
| τ Lib | τ | 40 | | 139365 | 76600 | 15$^h$ 38$^m$ 39.38$^s$ | −29° 46′ 39.7″ | 3.66 | −2.01 | 445 | B2.5V | |
| γ Lib | γ | 38 | | 138905 | 76333 | 15$^h$ 35$^m$ 31.54$^s$ | −14° 47′ 22.4″ | 3.91 | 0.56 | 152 | K0III | Zubenelhakrabi, has two planets |
| θ Lib | θ | 46 | | 142198 | 77853 | 15$^h$ 53$^m$ 49.48$^s$ | −16° 43′ 46.6″ | 4.13 | 0.64 | 163 | K0III | |
| 16 Lib | | 16 | | 132052 | 73165 | 14$^h$ 57$^m$ 11.06$^s$ | −04° 20′ 45.9″ | 4.47 | 2.24 | 91 | F0V | |
| ι$^1$ Lib | ι$^1$ | 24 | | 134759 | 74392 | 15$^h$ 12$^m$ 13.31$^s$ | −19° 47′ 29.9″ | 4.54 | −0.77 | 376 | Asp... | α$^2$ CVn variable, V$_{max}$ = 4.53$^m$, V$_{min}$ = 4.56$^m$, P = 3.10 d |
| 37 Lib | | 37 | | 138716 | 76219 | 15$^h$ 34$^m$ 10.52$^s$ | −10° 03′ 50.3″ | 4.61 | 2.30 | 94 | K1IV | |
| κ Lib | κ | 43 | | 139997 | 76880 | 15$^h$ 41$^m$ 56.82$^s$ | −19° 40′ 42.9″ | 4.75 | −0.69 | 400 | K5III | Rì (日), suspected variable |
| δ Lib | δ | 19 | | 132742 | 73473 | 15$^h$ 00$^m$ 58.39$^s$ | −08° 31′ 08.2″ | 4.91 | 0.06 | 304 | B9.5V | Zuben Elakribi or Mululizu; Algol variable, V$_{max}$ = 4.91$^m$, V$_{min}$ = 5.9$^m$, P = 2.33 d |
| ε Lib | ε | 31 | | 137052 | 75379 | 15$^h$ 24$^m$ 11.93$^s$ | −10° 19′ 18.8″ | 4.92 | 2.37 | 106 | F5IV | |
| 11 Lib | | 11 | | 130952 | 72631 | 14$^h$ 51$^m$ 01.02$^s$ | −02° 17′ 55.9″ | 4.93 | 0.82 | 216 | G8... | RS CVn variable, V$_{max}$ = 4.91$^m$, V$_{min}$ = 4.95$^m$, P = 60.55 d |
| 48 Lib | | 48 | FX | 142983 | 78207 | 15$^h$ 58$^m$ 11.38$^s$ | −14° 16′ 45.5″ | 4.95 | −1.03 | 513 | B8Ia/Iab | γ Cas variable, V$_{max}$ = 4.74$^m$, V$_{min}$ = 4.96$^m$ |
| 42 Lib | | 42 | | 139663 | 76742 | 15$^h$ 40$^m$ 16.91$^s$ | −23° 49′ 05.0″ | 4.97 | −0.37 | 381 | K3III | suspected variable |
| λ Lib | λ | 45 | | 142096 | 77811 | 15$^h$ 53$^m$ 20.06$^s$ | −20° 10′ 01.2″ | 5.03 | −0.16 | 356 | B3V | α$^2$ CVn variable, ΔV = 0.02$^m$, P = 3.31 d |
| 36 Lib | | 36 | | 138688 | 76259 | 15$^h$ 34$^m$ 37.31$^s$ | −28° 02′ 48.9″ | 5.13 | −0.14 | 369 | K2/K3III | |
| α$^1$ Lib | α$^1$ | 8 | | 130819 | 72603 | 14$^h$ 50$^m$ 41.26$^s$ | −15° 59′ 49.5″ | 5.15 | 3.28 | 77 | F3V | spectroscopic binary; member of the α Lib system |
| HR 5780 | | | IU | 138764 | 76243 | 15$^h$ 34$^m$ 26.53$^s$ | −09° 11′ 00.1″ | 5.16 | 0.00 | 351 | B6IV | slowly pulsating B star, V$_{max}$ = 5.14$^m$, V$_{min}$ = 5.19$^m$, P = 1.26 d |
| ν Lib | ν | 21 | | 133774 | 73945 | 15$^h$ 06$^m$ 37.62$^s$ | −16° 15′ 24.3″ | 5.19 | −1.66 | 765 | K5III | Zuben Hakrabim |
| 12 Lib | | 12 | | 131430 | 72929 | 14$^h$ 54$^m$ 20.14$^s$ | −24° 38′ 31.7″ | 5.27 | −0.09 | 384 | K2/K3III | |
| μ Lib | μ | 7 | | 130559 | 72489 | 14$^h$ 49$^m$ 19.09$^s$ | −14° 08′ 56.3″ | 5.32 | 1.03 | 235 | Ap | α$^2$ CVn variable |
| HD 126218 | | | | 126218 | 70469 | 14$^h$ 24$^m$ 48.66$^s$ | −24° 48′ 22.6″ | 5.34 | −0.10 | 400 | K0III | |
| 41 Lib | | 41 | | 139446 | 76628 | 15$^h$ 38$^m$ 54.51$^s$ | −19° 18′ 06.2″ | 5.36 | 0.27 | 340 | G8III/IV | |
| η Lib | η | 44 | | 140417 | 77060 | 15$^h$ 44$^m$ 04.42$^s$ | −15° 40′ 21.6″ | 5.41 | 2.14 | 147 | A6IV | Zuben Hakrabi |
| 49 Lib | | 49 | | 143333 | 78400 | 16$^h$ 00$^m$ 19.98$^s$ | −16° 31′ 56.6″ | 5.47 | 2.89 | 107 | F7V | variable star, ΔV = 0.004$^m$, P = 0.45 d |
| ξ$^2$ Lib | ξ$^2$ | 15 | | 131918 | 73133 | 14$^h$ 56$^m$ 46.11$^s$ | −11° 24′ 35.0″ | 5.48 | −0.61 | 538 | K4III | |
| HD 138413 | | | | 138413 | 76106 | 15$^h$ 32$^m$ 36.71$^s$ | −19° 40′ 13.3″ | 5.50 | 1.29 | 227 | A2IV | |
| HD 132833 | | | | 132833 | 73497 | 15$^h$ 01$^m$ 19.81$^s$ | −02° 45′ 17.5″ | 5.52 | −0.67 | 564 | M0III | suspected variable |
| HD 135534 | | | | 135534 | 74732 | 15$^h$ 16$^m$ 23.03$^s$ | −22° 23′ 57.9″ | 5.52 | −0.41 | 500 | K2III | |
| ζ$^4$ Lib | ζ$^4$ | 35 | | 138485 | 76126 | 15$^h$ 32$^m$ 55.23$^s$ | −16° 51′ 10.1″ | 5.53 | −1.33 | 769 | B3V | suspected variable |
| 30 Ser | | (30) | | 141378 | 77464 | 15$^h$ 48$^m$ 56.81$^s$ | −03° 49′ 06.7″ | 5.53 | 2.07 | 160 | A5IV | |
| 50 Lib | | 50 | | 143459 | 78436 | 16$^h$ 00$^m$ 47.64$^s$ | −08° 24′ 40.8″ | 5.53 | −0.21 | 459 | A0Vs | |
| HD 136479 | | | | 136479 | 75127 | 15$^h$ 21$^m$ 07.64$^s$ | −05° 49′ 29.4″ | 5.54 | 0.96 | 269 | K1III | |
| ζ$^1$ Lib | ζ$^1$ | 32 | | 137744 | 75730 | 15$^h$ 28$^m$ 15.40$^s$ | −16° 42′ 59.1″ | 5.64 | −1.58 | 908 | K4III | On 24 December 2031 it will be occulted by Venus over the North Pacific, Alaska, Northern Canada.$^{:165}$ |
| HD 130529 | | | | 130529 | 72488 | 14$^h$ 49$^m$ 18.76$^s$ | −24° 15′ 05.3″ | 5.68 | −1.99 | 1113 | K3III+... | |
| 4 Lib | | 4 | | 129433 | 71974 | 14$^h$ 43$^m$ 13.57$^s$ | −24° 59′ 51.8″ | 5.70 | 0.21 | 409 | B9.5V | 53 Hydrae |
| Gliese 570 | | | KX | 131977 | 73184 | 14$^h$ 57$^m$ 27.35$^s$ | −21° 24′ 55.7″ | 5.72 | 6.86 | 19 | K4V | BY Dra variable, ΔV = 0.04$^m$ |
| HD 136956 | | | | 136956 | 75352 | 15$^h$ 23$^m$ 52.26$^s$ | −12° 22′ 09.9″ | 5.72 | −0.61 | 603 | G8III | |
| HD 134373 | | | | 134373 | 74239 | 15$^h$ 10$^m$ 18.65$^s$ | −26° 19′ 57.4″ | 5.75 | 0.05 | 450 | K0III | |
| ξ$^1$ Lib | ξ$^1$ | 13 | | 131530 | 72934 | 14$^h$ 54$^m$ 22.91$^s$ | −11° 53′ 54.0″ | 5.78 | 0.54 | 365 | G7III | |
| HD 139254 | | | | 139254 | 76532 | 15$^h$ 37$^m$ 48.06$^s$ | −23° 08′ 29.5″ | 5.79 | 1.18 | 272 | K0III | |
| HD 129944 | | | | 129944 | 72210 | 14$^h$ 46$^m$ 06.75$^s$ | −23° 09′ 10.3″ | 5.80 | 0.55 | 366 | K0III | |
| ζ$^3$ Lib | ζ$^3$ | 34 | | 138137 | 75944 | 15$^h$ 30$^m$ 40.39$^s$ | −16° 36′ 34.0″ | 5.82 | −0.37 | 564 | K0III | |
| HD 139329 | | | | 139329 | 76569 | 15$^h$ 38$^m$ 16.24$^s$ | −21° 00′ 58.2″ | 5.82 | 1.06 | 292 | K0III | |
| HD 135051 | | | | 135051 | 74539 | 15$^h$ 13$^m$ 53.32$^s$ | −26° 11′ 36.8″ | 5.84 | −1.41 | 918 | G8/K0II | |
| 18 Lib | | 18 | | 132345 | 73310 | 14$^h$ 58$^m$ 53.64$^s$ | −11° 08′ 37.9″ | 5.88 | 0.95 | 316 | K3III-IV | |
| 47 Lib | | 47 | | 142378 | 77939 | 15$^h$ 55$^m$ 00.37$^s$ | −19° 22′ 58.4″ | 5.95 | −0.46 | 623 | B2/B3V | suspected variable |
| HD 130157 | | | | 130157 | 72310 | 14$^h$ 47$^m$ 13.66$^s$ | −21° 19′ 29.6″ | 6.05 | −2.73 | 1863 | K4/K5III | |
| ι$^2$ Lib | ι$^2$ | 25 | | 134967 | 74493 | 15$^h$ 13$^m$ 19.22$^s$ | −19° 38′ 50.8″ | 6.07 | 1.93 | 219 | A2V | |
| HD 132375 | | | | 132375 | 73309 | 14$^h$ 58$^m$ 52.99$^s$ | −04° 59′ 20.4″ | 6.08 | 3.37 | 114 | F8V | |
| HD 142703 | | | HR | 142703 | 78078 | 15$^h$ 56$^m$ 33.33$^s$ | −14° 49′ 45.7″ | 6.12 | 2.48 | 173 | A2Ib/II | δ Sct variable, ΔV = 0.02$^m$, P = 0.06 d |
| HD 133670 | | | | 133670 | 73927 | 15$^h$ 06$^m$ 27.10$^s$ | −22° 01′ 54.1″ | 6.13 | 2.24 | 195 | K0III | suspected variable |
| ο Lib | ο | 29 | | 136407 | 75118 | 15$^h$ 21$^m$ 01.36$^s$ | −15° 32′ 54.2″ | 6.14 | 2.45 | 178 | F2V | |
| HD 130557 | | | | 130557 | 72449 | 14$^h$ 48$^m$ 54.10$^s$ | −00° 50′ 51.7″ | 6.15 | 0.98 | 353 | B9Vsvar... | |
| 28 Lib | | 28 | | 136366 | 75110 | 15$^h$ 20$^m$ 53.68$^s$ | −18° 09′ 30.6″ | 6.16 | −0.27 | 631 | G8II/III | |
| 26 Lib | | 26 | | 135230 | 74600 | 15$^h$ 14$^m$ 33.77$^s$ | −17° 46′ 06.7″ | 6.18 | −1.80 | 1283 | B9III | |
| HD 139160 | | | | 139160 | 76503 | 15$^h$ 37$^m$ 28.51$^s$ | −26° 16′ 47.3″ | 6.19 | −0.14 | 600 | B9IV | |
| HD 128429 | | | | 128429 | 71469 | 14$^h$ 36$^m$ 59.80$^s$ | −12° 18′ 19.1″ | 6.20 | 3.66 | 88 | F6V + WD | Blue straggler |
| HD 138105 | | | | 138105 | 75939 | 15$^h$ 30$^m$ 36.25$^s$ | −20° 43′ 42.5″ | 6.20 | 1.92 | 234 | A3V | suspected variable |
| HD 141853 | | | | 141853 | 77689 | 15$^h$ 51$^m$ 38.41$^s$ | −14° 08′ 00.8″ | 6.20 | −0.43 | 692 | G8III | |
| 2 Lib | | 2 | | 126035 | 70336 | 14$^h$ 23$^m$ 25.63$^s$ | −11° 42′ 50.0″ | 6.22 | 1.19 | 330 | G7III | |
| HD 140986 | | | | 140986 | 77287 | 15$^h$ 46$^m$ 45.43$^s$ | −06° 07′ 13.3″ | 6.24 | −1.05 | 937 | K0III | |
| HD 138488 | | | | 138488 | 76143 | 15$^h$ 33$^m$ 09.53$^s$ | −24° 29′ 25.2″ | 6.26 | 1.22 | 331 | A3/5V +A9/F2 | |
| 10 Lib | | 10 | | 131027 | 72702 | 14$^h$ 51$^m$ 51.31$^s$ | −18° 21′ 19.2″ | 6.27 | −0.97 | 913 | K0II/III | |
| HD 135367 | | | | 135367 | 74623 | 15$^h$ 14$^m$ 50.61$^s$ | −05° 30′ 09.3″ | 6.28 | −0.95 | 911 | K3III | |
| HD 138268 | | | | 138268 | 76033 | 15$^h$ 31$^m$ 43.45$^s$ | −20° 09′ 53.4″ | 6.28 | 1.96 | 239 | A5V | |
| HD 140301 | | | | 140301 | 77007 | 15$^h$ 43$^m$ 24.86$^s$ | −15° 02′ 34.8″ | 6.30 | 0.80 | 411 | K0III | |
| HD 139290 | | | | 139290 | 76567 | 15$^h$ 38$^m$ 15.80$^s$ | −28° 12′ 23.8″ | 6.32 | 0.14 | 562 | K1III | |
| HD 142640 | | | | 142640 | 78059 | 15$^h$ 56$^m$ 14.41$^s$ | −14° 23′ 57.2″ | 6.32 | 2.29 | 208 | F6V | |
| 5 Lib | | 5 | | 129978 | 72194 | 14$^h$ 45$^m$ 57.78$^s$ | −15° 27′ 34.4″ | 6.33 | −1.33 | 1109 | K2III | |
| HD 139518 | | | | 139518 | 76666 | 15$^h$ 39$^m$ 21.39$^s$ | −23° 09′ 00.6″ | 6.33 | 1.47 | 306 | B9.5V | |
| HD 130325 | | | | 130325 | 72373 | 14$^h$ 47$^m$ 54.92$^s$ | −12° 50′ 23.2″ | 6.34 | 1.12 | 361 | K0III | |
| HD 132953 | | | | 132953 | 73571 | 15$^h$ 02$^m$ 08.59$^s$ | −07° 34′ 31.1″ | 6.38 | 0.13 | 580 | A5V | |
| 22 Lib | | 22 | | 133800 | 73953 | 15$^h$ 06$^m$ 49.10$^s$ | −16° 29′ 03.6″ | 6.41 | 0.90 | 413 | A1V | |
| HD 129980 | | | | 129980 | 72217 | 14$^h$ 46$^m$ 10.92$^s$ | −21° 10′ 32.6″ | 6.43 | 3.30 | 138 | G2V | |
| HD 137798 | | | | 137798 | 75790 | 15$^h$ 28$^m$ 58.69$^s$ | −28° 52′ 00.5″ | 6.43 | 2.51 | 198 | G0V | |
| 23 Lib | | 23 | | 134987 | 74500 | 15$^h$ 13$^m$ 28.93$^s$ | −25° 18′ 33.0″ | 6.45 | 4.40 | 84 | G5V | has two planets (b & c) |
| HD 139461 | | | | 139461 | 76603 | 15$^h$ 38$^m$ 40.07$^s$ | −08° 47′ 29.1″ | 6.45 | 4.47 | 81 | F6V | |
| 30 Lib | | 30 | | 136801 | 75294 | 15$^h$ 23$^m$ 01.78$^s$ | −15° 08′ 02.7″ | 6.46 | −0.43 | 780 | K4III | suspected variable |
| HD 134946 | | | | 134946 | 74490 | 15$^h$ 13$^m$ 17.43$^s$ | −24° 00′ 29.8″ | 6.47 | 0.96 | 412 | B8III | |
| HD 126251 | | | | 126251 | 70452 | 14$^h$ 24$^m$ 40.90$^s$ | −11° 40′ 10.7″ | 6.49 | 1.72 | 293 | F4III | |
| HD 126363 | | | | 126363 | 70501 | 14$^h$ 25$^m$ 17.63$^s$ | −13° 21′ 11.4″ | 6.49 | 0.48 | 520 | K2III | |
| HD 127964 | | | | 127964 | 71295 | 14$^h$ 34$^m$ 50.72$^s$ | −20° 26′ 21.8″ | 6.49 | 0.12 | 613 | A3V | |
| HD 134758 | | | | 134758 | 74391 | 15$^h$ 12$^m$ 12.04$^s$ | −19° 06′ 23.1″ | 6.49 | 0.33 | 555 | K4III | |
| HD 140722 | | | | 140722 | 77235 | 15$^h$ 46$^m$ 12.89$^s$ | −28° 03′ 41.1″ | 6.49 | 2.33 | 222 | F0V | |
| HD 136646 | | | | 136646 | 75272 | 15$^h$ 22$^m$ 45.19$^s$ | −29° 20′ 30.9″ | 6.50 | 0.83 | 443 | K0III | |
| HD 133112 | | | | 133112 | 73608 | 15$^h$ 02$^m$ 44.9$^s$ | −03° 01′ 53″ | 6.60 | | 323 | A6IV-V | WASP-189, has a planet (b) |
| 17 Lib | | 17 | | 132230 | 73249 | 14$^h$ 58$^m$ 13.42$^s$ | −11° 09′ 17.1″ | 6.61 | 1.30 | 376 | A1V | |
| 33 Lib | ζ$^2$ | 33 | GZ | 137949 | 75848 | 15$^h$ 29$^m$ 34.78$^s$ | −17° 26′ 27.4″ | 6.69 | 1.94 | 291 | Ap | rapidly oscillating Ap star, V$_{max}$ = 6.66$^m$, V$_{min}$ = 6.71$^m$, P = 4.85 d |
| HD 141569 | | | | 141569 | 77542 | 15$^h$ 49$^m$ 57.75$^s$ | −03° 55′ 16.3″ | 7.12 | | 379 | A0Ve | has a protoplanetary disk |
| 3 Lib | | 3 | | 128756 | 71652 | 14$^h$ 39$^m$ 22.01$^s$ | −25° 01′ 43.0″ | 7.20 | | 663 | K0III | |
| HD 140283 | | | | 140283 | 76976 | 15$^h$ 43$^m$ 03.10$^s$ | −10° 56′ 00.6″ | 7.21 | | 190 | sdF3 | one of the oldest stars known; suspected variable |
| FY Lib | | | FY | 132112 | 73213 | 14$^h$ 57$^m$ 46.55$^s$ | −12° 26′ 15.3″ | 7.23 | | 1310 | M5III | semiregular variable, V$_{max}$ = 6.5$^m$, V$_{min}$ = 7.78$^m$, P = 179.7 d |
| KU Lib | | | KU | 128987 | 71743 | 14$^h$ 40$^m$ 31.11$^s$ | −16° 12′ 33.4″ | 7.23 | | 77 | G8V | BY Dra variable; member of the α Lib system |
| ES Lib | | | ES | 135681 | 74765 | 15$^h$ 16$^m$ 48.61$^s$ | −13° 02′ 21.1″ | 7.25 | | 378 | A3III | β Lyr variable, V$_{max}$ = 7.1$^m$, V$_{min}$ = 7.57$^m$, P = 0.88 d |
| HD 141937 | | | | 141937 | 77740 | 15$^h$ 52$^m$ 17.55$^s$ | −18° 26′ 09.8″ | 7.25 | 4.63 | 109 | G2/G3V | has a planet (b) |
| HD 134796 | | | | 134796 | 74401 | 15$^h$ 12$^m$ 20.95$^s$ | −16° 24′ 39.86″ | 7.28 | 7.26 | | B9V | |
| HD 136905 | | | GX | 136905 | 75325 | 15$^h$ 23$^m$ 26.06$^s$ | −06° 36′ 37.8″ | 7.31 | | 378 | G8IVp | RS CVn variable, ΔV = 0.08$^m$, P = 11.13 d |
| HD 134214 | | | HI | 134214 | 74145 | 15$^h$ 09$^m$ 02.41$^s$ | −13° 59′ 58.7″ | 7.48 | | 335 | Ap... | rapidly oscillating Ap star, ΔV = 0.007$^m$ |
| HM Lib | | | HM | 137613 | 75694 | 15$^h$ 27$^m$ 48.32$^s$ | −25° 10′ 10.1″ | 7.54 | | 1940 | C | PV Tel variable, V$_{max}$ = 7.42$^m$, V$_{min}$ = 7.63$^m$ |
| HD 134701 | | | | 134701 | | 15$^h$ 11$^m$ 51.55$^s$ | −16° 36′ 40.16″ | 7.70 | 8.20 | | F5V | |
| HD 133803 | | | | 133803 | 73990 | 15$^h$ 07$^m$ 15.0$^s$ | −29° 30′ 16″ | 8.12 | | 408 | A9V | has two planets |
| HD 133131 A | | | | 133131 | 73674 | 15$^h$ 03$^m$ 35.8$^s$ | −27° 50′ 28″ | 8.4 | | | G2V | has two planets |
| HD 133131 B | | | | 133131 | 73674 | 15$^h$ 03$^m$ 35.8$^s$ | −27° 50′ 28″ | 8.42 | | | G2 | has a planet |
| HD 128598 | | | | 128598 | 71567 | 14$^h$ 38$^m$ 11.78$^s$ | −14° 57′ 17.2″ | 8.76 | | 3080 | K1IV/V | used to discover Uranus's rings |
| UZ Lib | | | UZ | | 76086 | 15$^h$ 32$^m$ 23.21$^s$ | −08° 32′ 00.9″ | 9.12 | | 525 | K0III | RS CVn variable, V$_{max}$ = 8.85$^m$, V$_{min}$ = 9.62$^m$, P = 4.77 d |
| HD 134440 | | | | 134440 | 74234 | 15$^h$ 10$^m$ 12.97$^s$ | −16° 27′ 47.5″ | 9.43 | | 93 | K2V | peculiar metal abundance; suspected variable |
| EH Lib | | | EH | | 73315 | 14$^h$ 58$^m$ 55.92$^s$ | −00° 56′ 53.1″ | 9.83 | 2.00 | 1,197 | A5V | δ Sct variable, V$_{max}$ = 9.35$^m$, V$_{min}$ = 10.08$^m$, P = 0.09 d |
| HD 139139 | | | | 139139 | | 15$^h$ 37$^m$ 06.21$^s$ | −19° 08′ 33.1″ | 9.84 | | 351 | G3/5V | has unusual dimming periods |
| VZ Lib | | | VZ | | 76050 | 15$^h$ 31$^m$ 51.76$^s$ | −15° 41′ 10.2″ | 10.27 | | 667 | F5 | W UMa variable, V$_{max}$ = 10.13$^m$, V$_{min}$ = 10.63$^m$, P = 0.36 d |
| Gliese 581 | | | HO | | 74995 | 15$^h$ 19$^m$ 26.82$^s$ | −07° 43′ 20.2″ | 10.55 | 11.57 | 20 | M3 | BY Dra variable, V$_{max}$ = 10.56$^m$, V$_{min}$ = 10.58$^m$; has 3 planets (b, c, e) |
| WASP-109 | | | | | | 15$^h$ 28$^m$ 13.0$^s$ | −16° 24′ 39″ | 11.4 | 3.81 | 1076 | F4V | has a transiting planets |
| HE 1523-0901 | | | | | | 15$^h$ 26$^m$ 01.07$^s$ | −09° 11′ 38.9″ | 11.50 | | | | one of the oldest stars known |
| HP Lib | | | HP | | | 15$^h$ 35$^m$ 53.08$^s$ | −14° 13′ 12.2″ | 13.65 | | | Bpec | AM CVn star and V777 Her variable, V$_{max}$ = 13.65$^m$, V$_{min}$ = 13.8$^m$, P = 0.013 d |
| K2-315 | | | | | | 15$^h$ 12$^m$ 5.06$^s$ | −20° 06′ 29.39″ | 17.67 | 13.89 | 185.3 | M3.5V | has a transiting planet (b) |
| 2MASS 1507-1627 | | | | | | 15$^h$ 07$^m$ 47.69$^s$ | −16° 27′ 38.6″ | 22.14 | | 23.9 | L5.5 | brown dwarf |
| GW Lib | | | GW | | | 15$^h$ 19$^m$ 55.35$^s$ | −25° 00′ 24.5″ | | | | | WZ Sge variable |
| WISE 1541-2250 | | | | | | 15$^h$ 41$^m$ 51.66$^s$ | −22° 50′ 25.0″ | | | 18.6 | Y0 | brown dwarf |
| IC 1059 | | | | | | 14$^h$ 50$^m$ 42.54$^s$ | −00° 52′ 33.1″ | | | | | a galaxy discovered in 1893 by Stephane Javelle |
| 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.] |||||||||||||