{{Short description|None}} This is the list of notable [[star]]s in the [[constellation]] [[Libra (constellation)|Libra]], sorted by decreasing brightness.

{{Sticky header}} {| class="wikitable sortable sticky-header" |- ! width="70" | [[Proper names (astronomy)|Name]] ! [[Bayer designation|B]] ! [[Flamsteed designation|F]] ! [[Variable star designation|Var]] ! [[Henry Draper Catalogue|HD]] ! [[Hipparcos Catalogue|HIP]] ! [[Right ascension|RA]] ! [[Declination|Dec]] ! [[apparent magnitude|vis.<br />mag.]] ! [[absolute magnitude|abs.<br />mag.]] ! [[Stellar distance|Dist.]] ([[light year|ly]]) ! [[stellar classification|Sp. class]] ! Notes |- | {{nsl|Beta Librae|β Lib}} || β || 27 || || 135742 || 74785 || {{RA|15|17|00.47}} || {{DEC|−09|22|58.3}} || 2.61 || −0.84 || 160 || B8V || style="text-align:left;" | {{nsl|Zubeneschamali}}; suspected {{nsl|variable star|variable}} |- | {{nsl|Alpha Librae|α<sup>2</sup> Lib}} || α<sup>2</sup> || 9 || || 130841 || 72622 || {{RA|14|50|52.78}} || {{DEC|−16|02|29.8}} || 2.75 || 0.88 || 77 || A3IV || style="text-align:left;" | {{nsl|Zubenelgenubi}}; spectroscopic binary; suspected variable; member of the α Lib system |- | {{nsl|Sigma Librae|σ Lib}} || σ || 20 || || 133216 || 73714 || {{RA|15|04|04.26}} || {{DEC|−25|16|54.7}} || 3.25 || −1.51 || 292 || M3/M4III || style="text-align:left;" | previously {{nsl|Scorpius|γ Scorpii}}, Brachium; {{nsl|semiregular variable}}, {{Variable star|3.2|3.46|20}} |- | {{nsl|Upsilon Librae|υ Lib}} || υ || 39 || || 139063 || 76470 || {{RA|15|37|01.46}} || {{DEC|−28|08|06.3}} || 3.60 || −0.28 || 195 || K3III || style="text-align:left;" | previously {{nsl|Scorpius|o Scorpii}} |- | {{nsl|Tau Librae|τ Lib}} || τ || 40 || || 139365 || 76600 || {{RA|15|38|39.38}} || {{DEC|−29|46|39.7}} || 3.66 || −2.01 || 445 || B2.5V || style="text-align:left;" | |- | {{nsl|Gamma Librae|γ Lib}} || γ || 38 || || 138905 || 76333 || {{RA|15|35|31.54}} || {{DEC|−14|47|22.4}} || 3.91 || 0.56 || 152 || K0III || style="text-align:left;" | {{nsl|Zubenelhakrabi}}, has two planets |- | {{nsl|Theta Librae|θ Lib}} || θ || 46 || || 142198 || 77853 || {{RA|15|53|49.48}} || {{DEC|−16|43|46.6}} || 4.13 || 0.64 || 163 || K0III || |- | {{nsl|16 Librae|16 Lib}} || || 16 || || 132052 || 73165 || {{RA|14|57|11.06}} || {{DEC|−04|20|45.9}} || 4.47 || 2.24 || 91 || F0V || |- | {{nsl|Iota1 Librae|ι<sup>1</sup> Lib}} || ι<sup>1</sup> || 24 || || 134759 || 74392 || {{RA|15|12|13.31}} || {{DEC|−19|47|29.9}} || 4.54 || −0.77 || 376 || Asp... || {{nsl|Alpha2 Canum Venaticorum variable|α<sup>2</sup> CVn variable}}, {{Variable star|4.53|4.56|3.10}} |- | {{nsl|37 Librae|37 Lib}} || || 37 || || 138716 || 76219 || {{RA|15|34|10.52}} || {{DEC|−10|03|50.3}} || 4.61 || 2.30 || 94 || K1IV || |- | {{nsl|Kappa Librae|κ Lib}} || κ || 43 || || 139997 || 76880 || {{RA|15|41|56.82}} || {{DEC|−19|40|42.9}} || 4.75 || −0.69 || 400 || K5III || Rì (日),<ref name="ridpathlibra">[http://www.ianridpath.com/startales/libra.htm Ian Ridpath's Startales - Libra the Scales]</ref> suspected variable |- | {{nsl|Delta Librae|δ Lib}} || δ || 19 || || 132742 || 73473 || {{RA|15|00|58.39}} || {{DEC|−08|31|08.2}} || 4.91 || 0.06 || 304 || B9.5V || style="text-align:left;" | Zuben Elakribi or Mululizu; {{nsl|Algol variable}}, {{Variable star|4.91|5.9|2.33}} |- | {{nsl|Epsilon Librae|ε Lib}} || ε || 31 || || 137052 || 75379 || {{RA|15|24|11.93}} || {{DEC|−10|19|18.8}} || 4.92 || 2.37 || 106 || F5IV || |- | {{nsl|11 Librae|11 Lib}} || || 11 || || 130952 || 72631 || {{RA|14|51|01.02}} || {{DEC|−02|17|55.9}} || 4.93 || 0.82 || 216 || G8... || {{nsl|RS Canum Venaticorum variable|RS CVn variable}}, {{Variable star|4.91|4.95|60.55}} |- | {{nsl|48 Librae|48 Lib}} || || 48 || FX || 142983 || 78207 || {{RA|15|58|11.38}} || {{DEC|−14|16|45.5}} || 4.95 || −1.03 || 513 || B8Ia/Iab ||style="text-align:left;" | {{nsl|Gamma Cassiopeiae variable|γ Cas variable}}, {{Variable star|4.74|4.96}} |- | {{nsl|42 Librae|42 Lib}} || χ<ref>Labelled '''Chi Librae''' (χ Lib/χ Librae) by Bode in his Uranographia</ref> || 42 || || 139663 || 76742 || {{RA|15|40|16.91}} || {{DEC|−23|49|05.0}} || 4.97 || −0.37 || 381 || K3III || suspected variable |- | {{nsl|Lambda Librae|λ Lib}} || λ || 45 || || 142096 || 77811 || {{RA|15|53|20.06}} || {{DEC|−20|10|01.2}} || 5.03 || −0.16 || 356 || B3V || α<sup>2</sup> CVn variable, {{VSA|0.02|3.31}}{{Dubious|reason=Hoffleit (1996) lists it as an ellipsoidal variable|date=January 2017}} |- | 36 Lib || || 36 || || 138688 || 76259 || {{RA|15|34|37.31}} || {{DEC|−28|02|48.9}} || 5.13 || −0.14 || 369 || K2/K3III || |- | {{nsl|Alpha Librae|α<sup>1</sup> Lib}} || α<sup>1</sup> || 8 || || 130819 || 72603 || {{RA|14|50|41.26}} || {{DEC|−15|59|49.5}} || 5.15 || 3.28 || 77 || F3V || style="text-align:left;" | spectroscopic binary; member of the α Lib system |- | HR 5780 || || || IU || 138764 || 76243 || {{RA|15|34|26.53}} || {{DEC|−09|11|00.1}} || 5.16 || 0.00 || 351 || B6IV || {{nsl|slowly pulsating B star}}, {{Variable star|5.14|5.19|1.26}} |- | ν Lib || ν || 21 || || 133774 || 73945 || {{RA|15|06|37.62}} || {{DEC|−16|15|24.3}} || 5.19 || −1.66 || 765 || K5III || style="text-align:left;" |Zuben Hakrabim |- | 12 Lib || || 12 || || 131430 || 72929 || {{RA|14|54|20.14}} || {{DEC|−24|38|31.7}} || 5.27 || −0.09 || 384 || K2/K3III || |- | {{nsl|Mu Librae|μ Lib}} || μ || 7 || || 130559 || 72489 || {{RA|14|49|19.09}} || {{DEC|−14|08|56.3}} || 5.32 || 1.03 || 235 || Ap || α<sup>2</sup> CVn variable |- | HD 126218 || || || || 126218 || 70469 || {{RA|14|24|48.66}} || {{DEC|−24|48|22.6}} || 5.34 || −0.10 || 400 || K0III || |- | 41 Lib || φ<ref>Labelled '''Phi Librae''' (φ Lib/φ Librae) by Bode in his Uranographia</ref> || 41 || || 139446 || 76628 || {{RA|15|38|54.51}} || {{DEC|−19|18|06.2}} || 5.36 || 0.27 || 340 || G8III/IV || |- | η Lib || η || 44 || || 140417 || 77060 || {{RA|15|44|04.42}} || {{DEC|−15|40|21.6}} || 5.41 || 2.14 || 147 || A6IV || style="text-align:left;" |Zuben Hakrabi |- | {{nsl|49 Librae|49 Lib}} || (φ)<ref>Labelled as '''Phi Scorpii''' (φ Sco/φ Scorpii) in Bode’s Uranographia</ref> || 49 || || 143333 || 78400 || {{RA|16|00|19.98}} || {{DEC|−16|31|56.6}} || 5.47 || 2.89 || 107 || F7V || variable star, {{VSA|0.004|0.45}} |- | ξ<sup>2</sup> Lib || ξ<sup>2</sup> || 15 || || 131918 || 73133 || {{RA|14|56|46.11}} || {{DEC|−11|24|35.0}} || 5.48 || −0.61 || 538 || K4III || |- | HD 138413 || || || || 138413 || 76106 || {{RA|15|32|36.71}} || {{DEC|−19|40|13.3}} || 5.50 || 1.29 || 227 || A2IV || |- | HD 132833 || || || || 132833 || 73497 || {{RA|15|01|19.81}} || {{DEC|−02|45|17.5}} || 5.52 || −0.67 || 564 || M0III || suspected variable |- | HD 135534 || || || || 135534 || 74732 || {{RA|15|16|23.03}} || {{DEC|−22|23|57.9}} || 5.52 || −0.41 || 500 || K2III || |- | ζ<sup>4</sup> Lib || ζ<sup>4</sup> || 35 || || 138485 || 76126 || {{RA|15|32|55.23}} || {{DEC|−16|51|10.1}} || 5.53 || −1.33 || 769 || B3V || suspected variable |- | 30 Ser || || (30) || || 141378 || 77464 || {{RA|15|48|56.81}} || {{DEC|−03|49|06.7}} || 5.53 || 2.07 || 160 || A5IV || |- | 50 Lib || ψ<ref>Labelled '''Psi Librae''' (ψ Lib/ψ Librae) by Bode in his Uranographia</ref> || 50 || || 143459 || 78436 || {{RA|16|00|47.64}} || {{DEC|−08|24|40.8}} || 5.53 || −0.21 || 459 || A0Vs || |- | HD 136479 || || || || 136479 || 75127 || {{RA|15|21|07.64}} || {{DEC|−05|49|29.4}} || 5.54 || 0.96 || 269 || K1III || |- | ζ<sup>1</sup> Lib || ζ<sup>1</sup> || 32 || || 137744 || 75730 || {{RA|15|28|15.40}} || {{DEC|−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]].<ref name="Mus2002">{{cite book |date=2002 |first=Jan |last=Meeus |chapter=Mutual occultations of planets |pages=174–185 |title=More Mathematical Astronomy Morsels |isbn=0943396743 |url=https://falakmu.id/khgt/dokumen/More%20mathematical%20astronomy%20morsels%20(Jean%20Meeus)%20(Z-Library).pdf}}</ref>{{rp|165}} |- | HD 130529 || || || || 130529 || 72488 || {{RA|14|49|18.76}} || {{DEC|−24|15|05.3}} || 5.68 || −1.99 || 1113 || K3III+... || |- | 4 Lib || || 4 || || 129433 || 71974 || {{RA|14|43|13.57}} || {{DEC|−24|59|51.8}} || 5.70 || 0.21 || 409 || B9.5V || 53 Hydrae |- | {{nsl|Gliese 570}} || || || KX || 131977 || 73184 || {{RA|14|57|27.35}} || {{DEC|−21|24|55.7}} || 5.72 || 6.86 || 19 || K4V ||style="text-align:left;" | {{nsl|BY Draconis variable|BY Dra variable}}, {{VSA|0.04}} |- | HD 136956 || || || || 136956 || 75352 || {{RA|15|23|52.26}} || {{DEC|−12|22|09.9}} || 5.72 || −0.61 || 603 || G8III || |- | HD 134373 || || || || 134373 || 74239 || {{RA|15|10|18.65}} || {{DEC|−26|19|57.4}} || 5.75 || 0.05 || 450 || K0III || |- | ξ<sup>1</sup> Lib || ξ<sup>1</sup> || 13 || || 131530 || 72934 || {{RA|14|54|22.91}} || {{DEC|−11|53|54.0}} || 5.78 || 0.54 || 365 || G7III || |- | HD 139254 || || || || 139254 || 76532 || {{RA|15|37|48.06}} || {{DEC|−23|08|29.5}} || 5.79 || 1.18 || 272 || K0III || |- | HD 129944 || || || || 129944 || 72210 || {{RA|14|46|06.75}} || {{DEC|−23|09|10.3}} || 5.80 || 0.55 || 366 || K0III || |- | ζ<sup>3</sup> Lib || ζ<sup>3</sup> || 34 || || 138137 || 75944 || {{RA|15|30|40.39}} || {{DEC|−16|36|34.0}} || 5.82 || −0.37 || 564 || K0III || |- | HD 139329 || || || || 139329 || 76569 || {{RA|15|38|16.24}} || {{DEC|−21|00|58.2}} || 5.82 || 1.06 || 292 || K0III || |- | HD 135051 || || || || 135051 || 74539 || {{RA|15|13|53.32}} || {{DEC|−26|11|36.8}} || 5.84 || −1.41 || 918 || G8/K0II || |- | 18 Lib || || 18 || || 132345 || 73310 || {{RA|14|58|53.64}} || {{DEC|−11|08|37.9}} || 5.88 || 0.95 || 316 || K3III-IV || |- | 47 Lib || || 47 || || 142378 || 77939 || {{RA|15|55|00.37}} || {{DEC|−19|22|58.4}} || 5.95 || −0.46 || 623 || B2/B3V || suspected variable |- | HD 130157 || || || || 130157 || 72310 || {{RA|14|47|13.66}} || {{DEC|−21|19|29.6}} || 6.05 || −2.73 || 1863 || K4/K5III || |- | ι<sup>2</sup> Lib || ι<sup>2</sup> || 25 || || 134967 || 74493 || {{RA|15|13|19.22}} || {{DEC|−19|38|50.8}} || 6.07 || 1.93 || 219 || A2V || |- | HD 132375 || || || || 132375 || 73309 || {{RA|14|58|52.99}} || {{DEC|−04|59|20.4}} || 6.08 || 3.37 || 114 || F8V || |- | HD 142703 || || || HR || 142703 || 78078 || {{RA|15|56|33.33}} || {{DEC|−14|49|45.7}} || 6.12 || 2.48 || 173 || A2Ib/II ||style="text-align:left;" | {{nsl|Delta Scuti variable|δ Sct variable}}, {{VSA|0.02|0.06}} |- | HD 133670 || || || || 133670 || 73927 || {{RA|15|06|27.10}} || {{DEC|−22|01|54.1}} || 6.13 || 2.24 || 195 || K0III || suspected variable |- | ο Lib || ο || 29 || || 136407 || 75118 || {{RA|15|21|01.36}} || {{DEC|−15|32|54.2}} || 6.14 || 2.45 || 178 || F2V || |- | HD 130557 || || || || 130557 || 72449 || {{RA|14|48|54.10}} || {{DEC|−00|50|51.7}} || 6.15 || 0.98 || 353 || B9Vsvar... || |- | 28 Lib || || 28 || || 136366 || 75110 || {{RA|15|20|53.68}} || {{DEC|−18|09|30.6}} || 6.16 || −0.27 || 631 || G8II/III || |- | 26 Lib || || 26 || || 135230 || 74600 || {{RA|15|14|33.77}} || {{DEC|−17|46|06.7}} || 6.18 || −1.80 || 1283 || B9III || |- | HD 139160 || || || || 139160 || 76503 || {{RA|15|37|28.51}} || {{DEC|−26|16|47.3}} || 6.19 || −0.14 || 600 || B9IV || |- | {{nsl|HD 128429}} || || || || 128429 || 71469 || {{RA|14|36|59.80}} || {{DEC|−12|18|19.1}} || 6.20 || 3.66 || 88 || F6V + WD || Blue straggler |- | HD 138105 || || || || 138105 || 75939 || {{RA|15|30|36.25}} || {{DEC|−20|43|42.5}} || 6.20 || 1.92 || 234 || A3V || suspected variable |- | HD 141853 || || || || 141853 || 77689 || {{RA|15|51|38.41}} || {{DEC|−14|08|00.8}} || 6.20 || −0.43 || 692 || G8III || |- | 2 Lib || || 2 || || 126035 || 70336 || {{RA|14|23|25.63}} || {{DEC|−11|42|50.0}} || 6.22 || 1.19 || 330 || G7III || |- | HD 140986 || || || || 140986 || 77287 || {{RA|15|46|45.43}} || {{DEC|−06|07|13.3}} || 6.24 || −1.05 || 937 || K0III || |- | HD 138488 || || || || 138488 || 76143 || {{RA|15|33|09.53}} || {{DEC|−24|29|25.2}} || 6.26 || 1.22 || 331 || A3/5V +A9/F2 || |- | 10 Lib || || 10 || || 131027 || 72702 || {{RA|14|51|51.31}} || {{DEC|−18|21|19.2}} || 6.27 || −0.97 || 913 || K0II/III || |- | HD 135367 || || || || 135367 || 74623 || {{RA|15|14|50.61}} || {{DEC|−05|30|09.3}} || 6.28 || −0.95 || 911 || K3III || |- | HD 138268 || || || || 138268 || 76033 || {{RA|15|31|43.45}} || {{DEC|−20|09|53.4}} || 6.28 || 1.96 || 239 || A5V || |- | HD 140301 || || || || 140301 || 77007 || {{RA|15|43|24.86}} || {{DEC|−15|02|34.8}} || 6.30 || 0.80 || 411 || K0III || |- | HD 139290 || || || || 139290 || 76567 || {{RA|15|38|15.80}} || {{DEC|−28|12|23.8}} || 6.32 || 0.14 || 562 || K1III || |- | HD 142640 || || || || 142640 || 78059 || {{RA|15|56|14.41}} || {{DEC|−14|23|57.2}} || 6.32 || 2.29 || 208 || F6V || |- | 5 Lib || || 5 || || 129978 || 72194 || {{RA|14|45|57.78}} || {{DEC|−15|27|34.4}} || 6.33 || −1.33 || 1109 || K2III || |- | HD 139518 || || || || 139518 || 76666 || {{RA|15|39|21.39}} || {{DEC|−23|09|00.6}} || 6.33 || 1.47 || 306 || B9.5V || |- | HD 130325 || || || || 130325 || 72373 || {{RA|14|47|54.92}} || {{DEC|−12|50|23.2}} || 6.34 || 1.12 || 361 || K0III || |- | HD 132953 || || || || 132953 || 73571 || {{RA|15|02|08.59}} || {{DEC|−07|34|31.1}} || 6.38 || 0.13 || 580 || A5V || |- | 22 Lib || || 22 || || 133800 || 73953 || {{RA|15|06|49.10}} || {{DEC|−16|29|03.6}} || 6.41 || 0.90 || 413 || A1V || |- | HD 129980 || || || || 129980 || 72217 || {{RA|14|46|10.92}} || {{DEC|−21|10|32.6}} || 6.43 || 3.30 || 138 || G2V || |- | HD 137798 || || || || 137798 || 75790 || {{RA|15|28|58.69}} || {{DEC|−28|52|00.5}} || 6.43 || 2.51 || 198 || G0V || |- | {{nsl|23 Librae|23 Lib}} || || 23 || || 134987 || 74500 || {{RA|15|13|28.93}} || {{DEC|−25|18|33.0}} || 6.45 || 4.40 || 84 || G5V || style="text-align:left;" | has two {{nsl|extrasolar planet|planets}} ({{nsl|23 Librae b|b}} & {{nsl|23 Librae c|c}}) |- | HD 139461 || || || || 139461 || 76603 || {{RA|15|38|40.07}} || {{DEC|−08|47|29.1}} || 6.45 || 4.47 || 81 || F6V || |- | 30 Lib || || 30 || || 136801 || 75294 || {{RA|15|23|01.78}} || {{DEC|−15|08|02.7}} || 6.46 || −0.43 || 780 || K4III || suspected variable |- | HD 134946 || || || || 134946 || 74490 || {{RA|15|13|17.43}} || {{DEC|−24|00|29.8}} || 6.47 || 0.96 || 412 || B8III || |- | HD 126251 || || || || 126251 || 70452 || {{RA|14|24|40.90}} || {{DEC|−11|40|10.7}} || 6.49 || 1.72 || 293 || F4III || |- | HD 126363 || || || || 126363 || 70501 || {{RA|14|25|17.63}} || {{DEC|−13|21|11.4}} || 6.49 || 0.48 || 520 || K2III || |- | HD 127964 || || || || 127964 || 71295 || {{RA|14|34|50.72}} || {{DEC|−20|26|21.8}} || 6.49 || 0.12 || 613 || A3V || |- | HD 134758 || || || || 134758 || 74391 || {{RA|15|12|12.04}} || {{DEC|−19|06|23.1}} || 6.49 || 0.33 || 555 || K4III || |- | HD 140722 || || || || 140722 || 77235 || {{RA|15|46|12.89}} || {{DEC|−28|03|41.1}} || 6.49 || 2.33 || 222 || F0V || |- | HD 136646 || || || || 136646 || 75272 || {{RA|15|22|45.19}} || {{DEC|−29|20|30.9}} || 6.50 || 0.83 || 443 || K0III || |- | [[HD 133112]] || || || || 133112 || 73608 || {{RA|15|02|44.9}} || {{DEC|-03|01|53}} || 6.60 || || 323 || A6IV-V || style="text-align:left;" | WASP-189, has a planet ([[HD 133112b|b]])<ref name="EA-20200928">{{cite news |author=University of Bern |author-link=University of Bern |title=First study with CHEOPS data describes one of the most extreme planets in the universe |url=https://www.eurekalert.org/pub_releases/2020-09/uob-fsw092520.php |date=28 September 2020 |work=[[EurekAlert!]] |access-date=28 September 2020 }}</ref> |- | 17 Lib || || 17 || || 132230 || 73249 || {{RA|14|58|13.42}} || {{DEC|−11|09|17.1}} || 6.61 || 1.30 || 376 || A1V || |- | [[33 Librae|33 Lib]] || ζ<sup>2</sup> || 33 || GZ || 137949 || 75848 || {{RA|15|29|34.78}} || {{DEC|−17|26|27.4}} || 6.69 || 1.94 || 291 || Ap || [[rapidly oscillating Ap star]], {{Variable star|6.66|6.71|4.85}} |- | [[HD 141569]] || || || || 141569 || 77542 || {{RA|15|49|57.75}} || {{DEC|−03|55|16.3}} || 7.12 || || 379 || A0Ve || has a [[protoplanetary disk]] |- | 3 Lib || || 3 || || 128756 || 71652 || {{RA|14|39|22.01}} || {{DEC|−25|01|43.0}} || 7.20 || || 663 || K0III || |- | [[HD 140283]] || || || || 140283 || 76976 || {{RA|15|43|03.10}} || {{DEC|−10|56|00.6}} || 7.21 || || 190 || sdF3 || one of the oldest stars known; suspected variable |- | FY Lib || || || FY || 132112 || 73213 || {{RA|14|57|46.55}} || {{DEC|−12|26|15.3}} || 7.23 || || 1310 || M5III || semiregular variable, {{Variable star|6.5|7.78|179.7}} |- | [[Alpha Librae#|KU Lib]] || || || KU || 128987 || 71743 || {{RA|14|40|31.11}} || {{DEC|−16|12|33.4}} || 7.23 || || 77 || G8V || BY Dra variable; member of the α Lib system |- | ES Lib || || || ES || 135681 || 74765 || {{RA|15|16|48.61}} || {{DEC|−13|02|21.1}} || 7.25 || || 378 || A3III || [[Beta Lyrae variable|β Lyr variable]], {{Variable star|7.1|7.57|0.88}} |- | [[HD 141937|HD&nbsp;141937]] || || || || 141937 || 77740 || {{RA|15|52|17.55}} || {{DEC|−18|26|09.8}} || 7.25 || 4.63 || 109 || G2/G3V || style="text-align:left;" | has a planet ([[HD 141937 b|b]]) |- | HD&nbsp;134796 || || || || 134796 || 74401 || {{RA|15|12|20.95}} || {{DEC|−16|24|39.86}} || 7.28 || 7.26 || || B9V || |- | HD 136905 || || || GX || 136905 || 75325 || {{RA|15|23|26.06}} || {{DEC|−06|36|37.8}} || 7.31 || || 378 || G8IVp || RS CVn variable, {{VSA|0.08|11.13}} |- | HD 134214 || || || HI || 134214 || 74145 || {{RA|15|09|02.41}} || {{DEC|−13|59|58.7}} || 7.48 || || 335 || Ap... || rapidly oscillating Ap star, {{VSA|0.007}} |- | HM Lib || || || HM || 137613 || 75694 || {{RA|15|27|48.32}} || {{DEC|−25|10|10.1}} || 7.54 || || 1940 || C || [[PV Telescopii variable|PV Tel variable]], {{Variable star|7.42|7.63}} |- | HD&nbsp;134701 || || || || 134701 || || {{RA|15|11|51.55}} || {{DEC|−16|36|40.16}} || 7.70 || 8.20 || || F5V || |- | HD 133803 || || || || 133803 || 73990 || {{RA|15|07|15.0}} || {{DEC|-29|30|16}} || 8.12 || || 408 || A9V || style="text-align:left;" | has two planets |- | [[HD 133131]] A || || || || 133131 || 73674 || {{RA|15|03|35.8}} || {{DEC|-27|50|28}} || 8.4 || || || G2V || style="text-align:left;" | has two planets |- | [[HD 133131]] B || || || || 133131 || 73674 || {{RA|15|03|35.8}} || {{DEC|-27|50|28}} || 8.42 || || || G2 || style="text-align:left;" | has a planet |- | [[HD 128598]] || || || || 128598 || 71567 || {{RA|14|38|11.78}} || {{DEC|−14|57|17.2}} || 8.76 || || 3080 || K1IV/V || used to discover Uranus's rings |- | UZ Lib || || || UZ || || 76086 || {{RA|15|32|23.21}} || {{DEC|−08|32|00.9}} || 9.12 || || 525 || K0III || RS CVn variable, {{Variable star|8.85|9.62|4.77}} |- | [[HD 134440]] || || || || 134440 || 74234 || {{RA|15|10|12.97}} || {{DEC|−16|27|47.5}} || 9.43 || || 93 || K2V || peculiar metal abundance; suspected variable |- | EH Lib || || || EH || || 73315 || {{RA|14|58|55.92}} || {{DEC|−00|56|53.1}} || 9.83 || 2.00 || 1,197 || A5V || [[Delta Scuti variable|δ Sct variable]], {{Variable star|9.35|10.08|0.09}} |- | [[HD 139139]] || || || || 139139 || || {{RA|15|37|06.21}} || {{DEC|-19|08|33.1}} || 9.84 || || 351 || G3/5V || has unusual dimming periods |- | VZ Lib || || || VZ || || 76050 || {{RA|15|31|51.76}} || {{DEC|−15|41|10.2}} || 10.27 || || 667 || F5 || [[W Ursae Majoris variable|W UMa variable]], {{Variable star|10.13|10.63|0.36}} |- | [[Gliese 581]] || || || HO || || 74995 || {{RA|15|19|26.82}} || {{DEC|−07|43|20.2}} || 10.55 || 11.57 || 20 || M3 || style="text-align:left;" | BY Dra variable, {{Variable star|10.56|10.58}}; has 3 planets ([[Gliese 581 b|b]], [[Gliese 581 c|c]], [[Gliese 581 e|e]]) |- | WASP-109 || || || || || || {{RA|15|28|13.0}} || {{DEC|-16|24|39}} || 11.4 || 3.81 || 1076 || F4V || style="text-align:left;" | has a transiting planets |- | [[HE 1523-0901]] || || || || || || {{RA|15|26|01.07}} || {{DEC|−09|11|38.9}} || 11.50 || || || || one of the oldest stars known |- | HP Lib || || || HP || || || {{RA|15|35|53.08}} || {{DEC|−14|13|12.2}} || 13.65 || || || Bpec || [[AM Canum Venaticorum star|AM CVn star]] and [[V777 Herculis variable|V777 Her variable]], {{Variable star|13.65|13.8|0.013}} |- | [[K2-315]] || || || || || || {{RA|15|12|5.06}} || {{DEC|-20|06|29.39}} || 17.67 || 13.89 || 185.3 || M3.5V || style="text-align:left;" | has a transiting planet ([[K2-315|b]]) |- | [[2MASS 1507-1627]] || || || || || || {{RA|15|07|47.69}} || {{DEC|−16|27|38.6}} || 22.14 || || 23.9 || L5.5 || [[brown dwarf]] |- | GW Lib || || || GW || || || {{RA|15|19|55.35}} || {{DEC|−25|00|24.5}} || || || || || [[WZ Sagittae variable|WZ Sge variable]] |- | [[WISE 1541-2250]] || || || || || || {{RA|15|41|51.66}} || {{DEC|−22|50|25.0}} || || || 18.6 || Y0 || brown dwarf |- | IC 1059 || || || || || || {{RA|14|50|42.54}} || {{DEC|-00|52|33.1}} || || || || || a [[galaxy]] discovered in 1893 by Stephane Javelle<ref>[http://cseligman.com/text/atlas/ic10a.htm#ic1059 csligman.com]</ref><ref>WikiSky, [http://server1.wikisky.org/starview?object_type=2&object_id=33322 "IC 1059"] (accessed 2010-10-27)</ref><ref>SIMBAD, [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=IC+1059&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id "IC 1059"] (accessed 2010-10-27)</ref>

{{Starlist Legend}} |}

==See also== *[[List of stars by constellation]] Color=Blue

==References== *{{cite web | last = ESA | author-link = European Space Agency | title = The Hipparcos and Tycho Catalogues | date = 1997 | url = http://cdsarc.u-strasbg.fr/viz-bin/Cat?I/239 | access-date = 2006-12-26 }} *{{cite web | last = Kostjuk | first = N. D. | title = HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index | date = 2002 | url = http://cdsarc.u-strasbg.fr/viz-bin/Cat?IV/27 | access-date = 2006-12-26 }} *{{cite web | last = Roman | first = N. G. | title = Identification of a Constellation from a Position | date = 1987 | url = http://cdsarc.u-strasbg.fr/viz-bin/Cat?VI/42 | access-date = 2006-12-26 }} *{{cite web |last=Gould |first=B. A. |title=Uranometria Argentina |publisher=Reprinted and updated by Pilcher, F |url=http://www.uranometriaargentina.com/ |access-date=2010-07-16 |url-status=usurped |archive-url=https://web.archive.org/web/20120227032716/http://www.uranometriaargentina.com/ |archive-date=2012-02-27 }} *{{ cite web | title = Naming Stars | url = https://www.iau.org/public/themes/naming_stars/ | access-date = 13 December 2017 }} {{Reflist}} {{Lists of stars by constellation}} {{Stars of Libra}}

[[Category:Libra (constellation)|*List]] [[Category:Lists of stars by constellation|Libra]]