# Llista d'estrelles de Lira

La llista d'estrelles de la Lira pretén recollir de forma sintètica i mostrant algunes poques de les seves principals característiques de les estrelles notables de la constel·lació de la Lira, ordenades, a priori, per ordre decreixent de brillantor.
| Nom | B | F | Var | HD | HIP | RA | Dec | mag. ap. | mag. abs. | Dist. (al) | Tipus sp. | Notes |
| Vega | α | 3 | | 172167 | 91262 | 18$^h$ 36$^m$ 56.19$^s$ | +38° 46′ 58.8″ | 0.03 | 0.58 | 25 | A0Vvar | Wega, Fidis, Harp Star, Al Nesr al Waki, Vulture Cadens; 5ª estrella més brillant, té un disc protoplanetari; variable δ Sct, V$_{max}$ = -0.02$^m$, V$_{min}$ = 0.07$^m$, P = 0.19 d |
| γ Lyr | γ | 14 | | 176437 | 93194 | 18$^h$ 58$^m$ 56.62$^s$ | +32° 41′ 22.4″ | 3.25 | −3.20 | 634 | B9III | Sulafat, Sulaphat; es sospita que és una estrella variable, V$_{max}$ = 3.23$^m$, V$_{min}$ = 3.26$^m$ |
| β Lyr A | β | 10 | | 174638 | 92420 | 18$^h$ 50$^m$ 04.79$^s$ | +33° 21′ 45.6″ | 3.52 | −3.64 | 881 | A8:V comp SB | Sheliak, Shelyak, Shiliak; prototipus de variable β Lyr, V$_{max}$ = 3.30$^m$, V$_{min}$ = 4.35$^m$, P = 12.94061713 d |
| R Lyr | | 13 | R | 175865 | 92862 | 18$^h$ 55$^m$ 20.09$^s$ | +43° 56′ 45.2″ | 4.08 | −1.07 | 349 | M5IIIvar | variable semiregular, V$_{max}$ = 3.81$^m$, V$_{min}$ = 4.44$^m$, P = 46 d |
| δ² Lyr | δ² | 12 | | 175588 | 92791 | 18$^h$ 54$^m$ 30.29$^s$ | +36° 53′ 55.0″ | 4.22 | −2.98 | 898 | M4IIvar | variable semiregular, V$_{max}$ = 4.22$^m$, V$_{min}$ = 4.33$^m$ |
| κ Lyr | κ | 1 | | 168775 | 89826 | 18$^h$ 19$^m$ 51.72$^s$ | +36° 03′ 52.0″ | 4.33 | 0.02 | 238 | K2IIIvar | es sospita que és variable, V$_{max}$ = 4.31$^m$, V$_{min}$ = 4.35$^m$ |
| ζ¹ Lyr | ζ¹ | 6 | | 173648 | 91971 | 18$^h$ 44$^m$ 46.34$^s$ | +37° 36′ 18.2″ | 4.34 | 0.97 | 154 | Am | estrella variable, ΔV = 0.003$^m$, P = 1.53243 d |
| θ Lyr | θ | 21 | | 180809 | 94713 | 19$^h$ 16$^m$ 22.10$^s$ | +38° 08′ 01.4″ | 4.35 | −2.51 | 769 | K0II | es sospita que és variable, V$_{max}$ = 4.32$^m$, V$_{min}$ = 4.37$^m$ |
| η Lyr | η | 20 | | 180163 | 94481 | 19$^h$ 13$^m$ 45.49$^s$ | +39° 08′ 45.5″ | 4.43 | −3.09 | 1042 | B2.5IV | Aladfar; estrella variable, ΔV = 0.005$^m$, P = 19.73944 d |
| ε² Lyr A | ε² | 5 | | 173607 | 91926 | 18$^h$ 44$^m$ 22.78$^s$ | +39° 36′ 45.3″ | 4.60 | 1.13 | 160 | A8Vn | forma part del sistema ε Lyr; estrella binària; es sopita que és variable, ΔV = 0.02$^m$ |
| ε¹ Lyr A | ε¹ | 4 | | 173582 | 91919 | 18$^h$ 44$^m$ 20.34$^s$ | +39° 40′ 11.9″ | 4.67 | 1.19 | 162 | F1V | forma part del sistema ε Lyr; estrella binària |
| HD 173780 | | | | 173780 | 92088 | 18$^h$ 46$^m$ 04.47$^s$ | +26° 39′ 43.5″ | 4.83 | 0.39 | 252 | K3III | |
| λ Lyr | λ | 15 | | 176670 | 93279 | 19$^h$ 00$^m$ 00.82$^s$ | +32° 08′ 43.8″ | 4.94 | −3.43 | 1538 | K3III | es sospita que és variable |
| 16 Lyr | | 16 | | 177196 | 93408 | 19$^h$ 01$^m$ 26.36$^s$ | +46° 56′ 06.1″ | 5.00 | 2.04 | 128 | A7V | es sospita que és variable, V$_{max}$ = 5.00$^m$, V$_{min}$ = 5.09$^m$ |
| μ Lyr | μ | 2 | | 169702 | 90191 | 18$^h$ 24$^m$ 13.80$^s$ | +39° 30′ 26.1″ | 5.11 | −0.55 | 441 | A3IVn | Alathfar, Al Athfar |
| HD 176051 | | | | 176051 | 93017 | 18$^h$ 57$^m$ 01.47$^s$ | +32° 54′ 05.8″ | 5.20 | 4.32 | 49 | G0V | té un planeta (b) |
| 17 Lyr | | 17 | | 178449 | 93917 | 19$^h$ 07$^m$ 25.50$^s$ | +32° 30′ 06.0″ | 5.20 | 2.16 | 132 | F0V | |
| ν Lyr | ν, ν² | 9 | | 174602 | 92405 | 18$^h$ 49$^m$ 52.92$^s$ | +32° 33′ 03.9″ | 5.22 | 0.90 | 238 | A3V | |
| ι Lyr | ι | 18 | | 178475 | 93903 | 19$^h$ 07$^m$ 18.13$^s$ | +36° 06′ 00.6″ | 5.25 | −1.78 | 832 | B6IV | Estrella Be |
| HD 176527 | | | | 176527 | 93256 | 18$^h$ 59$^m$ 45.43$^s$ | +26° 13′ 49.6″ | 5.26 | 0.12 | 348 | K2III | es sospita que es variable RS CVn |
| ε² Lyr B | ε² | 5 | | 173608 | | 18$^h$ 44$^m$ 22.90$^s$ | +39° 36′ 46.0″ | 5.37 | | | | forma part del sistema ε Lyr |
| HD 172044 | | | | 172044 | 91235 | 18$^h$ 36$^m$ 37.35$^s$ | +33° 28′ 08.5″ | 5.41 | −0.61 | 522 | B8II-IIIp.. | es sopita que es variable α² CVn, V$_{max}$ = 5.40$^m$, V$_{min}$ = 5.45$^m$ |
| HD 175740 | | | | 175740 | 92831 | 18$^h$ 54$^m$ 52.18$^s$ | +41° 36′ 09.8″ | 5.46 | 0.89 | 267 | G8III | |
| HD 171301 | | | | 171301 | 90923 | 18$^h$ 32$^m$ 49.95$^s$ | +30° 33′ 15.1″ | 5.47 | 0.22 | 365 | B8IV | |
| HD 178233 | | | | 178233 | 93843 | 19$^h$ 06$^m$ 37.68$^s$ | +28° 37′ 42.2″ | 5.53 | 2.48 | 133 | F0III | |
| HD 167965 | | | | 167965 | 89482 | 18$^h$ 15$^m$ 38.78$^s$ | +42° 09′ 33.6″ | 5.56 | −0.53 | 540 | B7IV | estrella variable star, ΔV = 0.008$^m$, P = 0.57460 d |
| δ¹ Lyr | δ¹ | 11 | | 175426 | 92728 | 18$^h$ 53$^m$ 43.56$^s$ | +36° 58′ 18.2″ | 5.58 | −2.02 | 1079 | B2.5V | es sospita que és variable, V$_{max}$ = 5.56$^m$, V$_{min}$ = 5.62$^m$ |
| HD 177808 | | | | 177808 | 93718 | 19$^h$ 04$^m$ 57.82$^s$ | +31° 44′ 39.3″ | 5.63 | −0.72 | 606 | M0III | |
| HD 175443 | | | | 175443 | 92768 | 18$^h$ 54$^m$ 13.25$^s$ | +27° 54′ 34.9″ | 5.64 | 0.17 | 405 | K4III | |
| HD 173417 | | | | 173417 | 91883 | 18$^h$ 43$^m$ 51.61$^s$ | +31° 55′ 36.9″ | 5.68 | 2.10 | 169 | F1III-IV | |
| HD 176871 | | | | 176871 | 93393 | 19$^h$ 01$^m$ 17.36$^s$ | +26° 17′ 29.2″ | 5.69 | −0.96 | 697 | B5V | |
| ζ² Lyr | ζ² | 7 | | 173649 | 91973 | 18$^h$ 44$^m$ 48.19$^s$ | +37° 35′ 40.4″ | 5.73 | 2.41 | 150 | F0IVvar | es sospita que és variable, V$_{max}$ = 5.68$^m$, V$_{min}$ = 5.74$^m$ |
| HD 182694 | | | | 182694 | 95352 | 19$^h$ 23$^m$ 56.49$^s$ | +43° 23′ 17.7″ | 5.85 | 0.38 | 404 | G6.5IIIa | |
| HD 180450 | | | | 180450 | 94630 | 19$^h$ 15$^m$ 24.84$^s$ | +30° 31′ 35.2″ | 5.88 | −2.25 | 1376 | M0III | estrella variable, ΔV = 0.014$^m$, P = 2.63213 d |
| V542 Lyr | | | V542 | 176318 | 93104 | 18$^h$ 58$^m$ 01.90$^s$ | +38° 15′ 58.3″ | 5.89 | −0.11 | 516 | B7IV | variable Algol |
| ν¹ Lyr | ν¹ | 8 | | 174585 | 92398 | 18$^h$ 49$^m$ 45.91$^s$ | +32° 48′ 46.2″ | 5.93 | −1.52 | 1009 | B3IV | es sospita que és variable, V$_{max}$ = 5.89$^m$, V$_{min}$ = 5.96$^m$ |
| 19 Lyr | | 19 | V471 | 179527 | 94311 | 19$^h$ 11$^m$ 46.01$^s$ | +31° 17′ 00.5″ | 5.93 | −1.46 | 979 | B9p Si | variable α² CVn, V$_{max}$ = 5.91$^m$, V$_{min}$ = 5.98$^m$, P = 1.160898 d |
| HD 175635 | | | | 175635 | 92833 | 18$^h$ 54$^m$ 52.52$^s$ | +33° 58′ 06.9″ | 5.99 | −2.06 | 1331 | G8III+... | |
| XY Lyr | | | XY | 172380 | 91373 | 18$^h$ 38$^m$ 06.47$^s$ | +39° 40′ 05.9″ | 6.02 | −1.81 | 1199 | M4.5II | semiregular variable, V$_{max}$ = 5.6$^m$, V$_{min}$ = 6.6$^m$, P = 120 d |
| ε¹ Lyr B | ε¹ | 4 | | 173583 | | 18$^h$ 44$^m$ 20.30$^s$ | +39° 40′ 16.0″ | 6.02 | | | | forma part del sistema ε Lyr |
| HD 176896 | | | | 176896 | 93354 | 19$^h$ 00$^m$ 55.20$^s$ | +33° 48′ 07.7″ | 6.04 | 0.62 | 396 | K0III: | |
| HD 173416 | | | | 173416 | 91852 | 18$^h$ 43$^m$ 36.11$^s$ | +36° 33′ 23.8″ | 6.06 | 0.41 | 440 | G8III | té un planeta (b) |
| HD 173936 | | | | 173936 | 92098 | 18$^h$ 46$^m$ 13.01$^s$ | +41° 26′ 30.5″ | 6.06 | −1.81 | 1221 | B6V | |
| HD 174179 | | | | 174179 | 92243 | 18$^h$ 47$^m$ 57.37$^s$ | +31° 45′ 24.6″ | 6.06 | −1.50 | 1062 | B3IVp | |
| HD 177809 | | | | 177809 | 93720 | 19$^h$ 04$^m$ 58.27$^s$ | +30° 44′ 00.4″ | 6.07 | −0.72 | 743 | M2III | es sospita que és variable |
| HD 182272 | | | | 182272 | 95235 | 19$^h$ 22$^m$ 33.35$^s$ | +33° 31′ 05.6″ | 6.09 | 1.01 | 339 | K0III | |
| HD 171780 | | | | 171780 | 91119 | 18$^h$ 35$^m$ 13.50$^s$ | +34° 27′ 28.8″ | 6.10 | −1.42 | 1038 | B5Vn | es sospita que és variable |
| HD 174959 | | | | 174959 | 92551 | 18$^h$ 51$^m$ 36.52$^s$ | +36° 32′ 20.8″ | 6.10 | −1.58 | 1120 | B6IV | |
| HD 168322 | | | | 168322 | 89604 | 18$^h$ 17$^m$ 06.95$^s$ | +40° 56′ 11.7″ | 6.12 | 0.98 | 348 | G9III | |
| V473 Lyr | | | V473 | 180583 | 94685 | 19$^h$ 15$^m$ 59.49$^s$ | +27° 55′ 34.7″ | 6.18 | −2.38 | 1680 | F6Ib-II | Cefeida clàssica, V$_{max}$ = 5.99$^m$, V$_{min}$ = 6.35$^m$, P = 1.49078 d |
| V543 Lyr | | | V543 | 176502 | 93177 | 18$^h$ 58$^m$ 46.59$^s$ | +40° 40′ 45.1″ | 6.20 | −1.12 | 948 | B3V | variable β Cep |
| HD 179583 | | | | 179583 | 94280 | 19$^h$ 11$^m$ 23.16$^s$ | +40° 25′ 45.0″ | 6.20 | 0.40 | 471 | A3V | |
| V533 Lyr | | | V533 | 172187 | 91250 | 18$^h$ 36$^m$ 45.53$^s$ | +43° 13′ 18.6″ | 6.21 | 0.71 | 411 | F0V | variable β Lyr |
| HD 174881 | | | | 174881 | 92550 | 18$^h$ 51$^m$ 35.89$^s$ | +28° 47′ 01.2″ | 6.22 | −2.23 | 1598 | K1II-III | |
| HD 172671 | | | | 172671 | 91491 | 18$^h$ 39$^m$ 33.03$^s$ | +40° 56′ 06.2″ | 6.25 | −0.72 | 807 | B9V | |
| HD 181470 | | | | 181470 | 94932 | 19$^h$ 19$^m$ 01.15$^s$ | +37° 26′ 43.1″ | 6.25 | −0.29 | 663 | A0III | |
| HD 175132 | | | | 175132 | 92599 | 18$^h$ 52$^m$ 07.25$^s$ | +41° 22′ 59.7″ | 6.28 | −1.59 | 1221 | B9p Si | estrella variable, ΔV = 0.009$^m$, P = 8.03084 d |
| HD 181655 | | | | 181655 | 94981 | 19$^h$ 19$^m$ 39.04$^s$ | +37° 19′ 51.5″ | 6.29 | 4.28 | 82 | G8V | |
| HD 168009 | | | | 168009 | 89474 | 18$^h$ 15$^m$ 32.53$^s$ | +45° 12′ 34.5″ | 6.30 | 4.52 | 74 | G2V | |
| HD 181828 | | | | 181828 | 95067 | 19$^h$ 20$^m$ 33.05$^s$ | +35° 11′ 09.4″ | 6.30 | −0.44 | 726 | B9V | |
| HR 7403 | | | V558 | 183362 | 95673 | 19$^h$ 27$^m$ 36.40$^s$ | +37° 56′ 28.3″ | 6.30 | −2.71 | 2063 | B3Ve | Estrella Be |
| HD 178003 | | | | 178003 | 93770 | 19$^h$ 05$^m$ 47.13$^s$ | +29° 55′ 18.1″ | 6.32 | −1.70 | 1309 | M0III | es sospita que és variable |
| HD 179422 | | | | 179422 | 94290 | 19$^h$ 11$^m$ 30.96$^s$ | +26° 44′ 09.4″ | 6.35 | 3.18 | 141 | F5V | |
| Gliese 758 | | | | 182488 | 95319 | 19$^h$ 23$^m$ 34.01$^s$ | +33° 13′ 19.1″ | 6.37 | 5.42 | 51 | G8V | està acompanyada d'una nana marró |
| HD 177109 | | | | 177109 | 93437 | 19$^h$ 01$^m$ 48.37$^s$ | +33° 37′ 16.5″ | 6.39 | −1.27 | 1109 | B5IV | |
| HD 169646 | | | | 169646 | 90163 | 18$^h$ 23$^m$ 57.27$^s$ | +38° 44′ 21.0″ | 6.41 | −0.69 | 858 | K2 | |
| HD 172958 | | | | 172958 | 91675 | 18$^h$ 41$^m$ 41.31$^s$ | +31° 37′ 03.3″ | 6.41 | −1.24 | 1105 | B8V | |
| HD 172631 | | | | 172631 | 91533 | 18$^h$ 40$^m$ 01.93$^s$ | +30° 50′ 57.8″ | 6.43 | 0.18 | 580 | K0 | |
| HD 176582 | | | V545 | 176582 | 93210 | 18$^h$ 59$^m$ 12.29$^s$ | +39° 13′ 02.4″ | 6.43 | −0.58 | 821 | B5IV | variable 53 Per |
| HD 182635 | | | | 182635 | 95370 | 19$^h$ 24$^m$ 06.05$^s$ | +36° 27′ 06.9″ | 6.44 | 1.22 | 360 | K1III | |
| HD 172741 | | | | 172741 | 91552 | 18$^h$ 40$^m$ 12.19$^s$ | +38° 22′ 01.8″ | 6.45 | 0.52 | 501 | A6m | |
| HD 173383 | | | | 173383 | 91820 | 18$^h$ 43$^m$ 16.57$^s$ | +39° 18′ 00.3″ | 6.45 | −1.65 | 1358 | K5 | |
| V550 Lyr | | | V550 | 178329 | 93808 | 19$^h$ 06$^m$ 17.00$^s$ | +41° 24′ 50.0″ | 6.49 | | 2038 | B3V | variable 53 Per |
| HD 173087 | | | | 173087 | 91707 | 18$^h$ 42$^m$ 08.09$^s$ | +34° 44′ 46.7″ | 6.49 | −1.55 | 1320 | B5V | |
| HD 180314 | | | | 180314 | 94576 | 19$^h$ 14$^m$ 50.21$^s$ | +31° 51′ 37.3″ | 6.61 | | 430 | K0 | té un planeta no confirmat (b) |
| HD 178911 | | | | 178911 | 94076 | 19$^h$ 09$^m$ 04.38$^s$ | +34° 36′ 01.6″ | 6.74 | 3.29 | 160 | G1V | estrella binària; component B; té un planeta (b) |
| HD 181068 | | | | 181068 | 94780 | 19$^h$ 17$^m$ 08.98$^s$ | +41° 15′ 53.3″ | 7.09 | | 811 | G5 | triple binària eclipsant |
| RR Lyr | | | RR | 182989 | 95497 | 19$^h$ 25$^m$ 27.91$^s$ | +42° 47′ 03.7″ | 7.13 | 0.34 | 744 | F5 | prototipus de variable RR Lyr, V$_{max}$ = 7.06$^m$, V$_{min}$ = 8.12$^m$, P = 0.56686776 d |
| HD 177830 | | | | 177830 | 93746 | 19$^h$ 05$^m$ 20.77$^s$ | +25° 55′ 14.4″ | 7.18 | 3.32 | 192 | K0 | té dos planetes (b i c) |
| β Lyr B | β | 10 | | 174664 | | 18$^h$ 50$^m$ 06.60$^s$ | +33° 21′ 05.0″ | 7.20 | | | | forma part del sistema β Lyr |
| W Lyr | | | W | 167740 | 89419 | 18$^h$ 14$^m$ 55.88$^s$ | +36° 40′ 13.2″ | 7.30 | | | M3.5-7e | variable Mira, V$_{max}$ = 7.3$^m$, V$_{min}$ = 13$^m$, P = 197.88 d |
| V478 Lyr | | | V478 | 178450 | 93926 | 19$^h$ 07$^m$ 32.39$^s$ | +30° 15′ 16.2″ | 7.63 | | 91.16 | G8VSB | RS CVn variable, ΔV = 0.032$^m$, P = 2.185 d |
| HK Lyr | | | HK | 173291 | 91774 | 18$^h$ 42$^m$ 50.00$^s$ | +36° 57′ 30.9″ | 7.65 | | | C | semiregular variable, V$_{max}$ = 7.5$^m$, V$_{min}$ = 8.4$^m$, P = 186 d |
| T Lyr | | | T | | 90883 | 18$^h$ 32$^m$ 20.10$^s$ | +39° 59′ 55.6″ | 7.84 | | 2350 | C | variable irregular lenta, V$_{max}$ = 7.5$^m$, V$_{min}$ = 9.2$^m$ |
| V Lyr | | | V | 178876 | | 19$^h$ 09$^m$ 04.55$^s$ | +29° 39′ 29.3″ | 8.2 | | | M7e | variable Mira, V$_{max}$ = 8.2$^m$, V$_{min}$ = 15.7$^m$, P = 373.53 d |
| FL Lyr | | | FL | 179890 | 94335 | 19$^h$ 12$^m$ 04.86$^s$ | +46° 19′ 26.9″ | 9.36 | | 424 | G0V | variable Algol, V$_{max}$ = 9.27$^m$, V$_{min}$ = 9.89$^m$, P = 2.178152 d |
| Kepler-37 | | | | | | 18$^h$ 58$^m$ 23.1$^s$ | +44° 31′ 05″ | 9.77 | | 215 | G8V | té tres planetes (b, c i d) |
| S Lyr | | | S | | | 19$^h$ 13$^m$ 11.80$^s$ | +26° 00′ 27.8″ | 9.8 | | | SC | variable Mira, V$_{max}$ = 9.3$^m$, V$_{min}$ = 16.0$^m$, P = 438.4 d |
| EP Lyr | | | EP | | | 19$^h$ 18$^m$ 19.55$^s$ | +27° 51′ 03.2″ | 9.96 | | | G2II | variable RV Tau, V$_{max}$ = 9.96$^m$, V$_{min}$ = 10.90$^m$, P = 83.34 d |
| KX Lyr | | | KX | | | 18$^h$ 33$^m$ 15.23$^s$ | +40° 10′ 22.7″ | 10.38 | | | F0 | variable RR Lyr, V$_{max}$ = 10.38$^m$, V$_{min}$ = 11.47$^m$, P = 0.44090446 d |
| UZ Lyr | | | UZ | | | 19$^h$ 21$^m$ 08.91$^s$ | +37° 56′ 11.5″ | 10.40 | | | A2 | variable Algol, V$_{max}$ = 9.9$^m$, V$_{min}$ = 11$^m$, P = 1.89127025 d |
| HP Lyr | | | HP | | | 19$^h$ 21$^m$ 39.07$^s$ | +39° 56′ 08.1″ | 10.43 | | | A6 | variable semiregular, V$_{max}$ = 10.18$^m$, V$_{min}$ = 10.80$^m$, P = 68.88 d |
| WASP-3 | | | | | | 18$^h$ 34$^m$ 31.62$^s$ | +35° 39′ 41.5″ | 10.49 | 3.75 | 727 | F7V | té un planeta en trànsit (b) |
| TT Lyr | | | TT | | | 19$^h$ 27$^m$ 36.30$^s$ | +41° 42′ 05.4″ | 10.88 | | | B2V | variable Algol, V$_{max}$ = 9.34$^m$, V$_{min}$ = 11.43$^m$, P = 5.243727 d |
| Kepler-65 | | | | | | 19$^h$ 14$^m$ 45.3$^s$ | +41° 09′ 04.2″ | 11.018 | | | B | té tres planetes (b, c i d) |
| TZ Lyr | | | TZ | | 89498 | 18$^h$ 15$^m$ 49.67$^s$ | +41° 06′ 37.9″ | 11.16 | | 736 | F5V | variable β Lyr, V$_{max}$ = 1.087$^m$, V$_{min}$ = 11.85$^m$, P = 0.5288269 d |
| EZ Lyr | | | EZ | | 92221 | 18$^h$ 47$^m$ 40.32$^s$ | +35° 59′ 34.2″ | 11.34 | | 265.7 | A9.7 | variable RR Lyr, V$_{max}$ = 10.8$^m$, V$_{min}$ = 11.8$^m$, P = 0.52526769 d |
| CN Lyr | | | CN | | 91634 | 18$^h$ 41$^m$ 15.95$^s$ | +28° 43′ 21.1″ | 11.38 | | | F5 | variable RR Lyr, V$_{max}$ = 11.07$^m$, V$_{min}$ = 11.76$^m$, P = 0.41138232 d |
| RV Lyr | | | RV | | | 19$^h$ 16$^m$ 17.97$^s$ | +32° 25′ 15.0″ | 11.47 | | | A5 | variable Algol |
| RZ Lyr | | | RZ | | | 18$^h$ 43$^m$ 37.88$^s$ | +32° 47′ 54.0″ | 11.57 | | | A2 | variable RR Lyr, V$_{max}$ = 10.6$^m$, V$_{min}$ = 12.03$^m$, P = 0.5112423 d |
| WASP-58 | | | | | | 18$^h$ 18$^m$ 48.0$^s$ | +45° 10′ 19″ | 11.66 | | 978 | G2V | té un planeta en trànsit (b) |
| V404 Lyr | | | V404 | | | 19$^h$ 19$^m$ 05.95$^s$ | +38° 22′ 00.5″ | 11.77 | | | | variable Algol |
| GSC 02652-01324 | | | | | | 19$^h$ 04$^m$ 09.84$^s$ | +36° 37′ 57.5″ | 11.79 | 5.81 | 512 | K0V | té un planeta en trànsit (TrES-1) |
| HAT-P-5 | | | | | | 18$^h$ 17$^m$ 37.30$^s$ | +36° 37′ 16.9″ | 11.95 | 4.29 | 1110 | G | té un planeta en trànsit (b) |
| CC Lyr | | | CC | | 91015 | 18$^h$ 33$^m$ 57.41$^s$ | +31° 38′ 24.2″ | 12.46 | | | F0p... | variable W Vir, V$_{max}$ = 11.65$^m$, V$_{min}$ = 12.45$^m$, P = 24.16 d |
| β Lyr C | β | 10 | | 174639 | | 18$^h$ 50$^m$ 01.20$^s$ | +33° 21′ 26.0″ | 13.40 | | | | forma part del sistema β Lyr |
| Kepler-138 | | | | | | 19$^h$ 21$^m$ 32.0$^s$ | +43° 17′ 35″ | 13.50 | | | M1V | té dos planetes en trànsit (b i c) |
| Kepler-412 | | | | | | 19$^h$ 04$^m$ 26.0$^s$ | +43° 40′ 51″ | 13.73 | | 3444 | G3V | té un planeta en trànsit (b) |
| Kepler-62 | | | | | | 18$^h$ 52$^m$ 51.0$^s$ | +45° 20′ 60″ | 13.75 | | ~1200 | K2V | té cinc planetes en trànsit (b, c, d, e i f) |
| Kepler-8 | | | | | | 18$^h$ 45$^m$ 09.15$^s$ | +42° 27′ 03.9″ | 13.9 | 3.3 | 4338 | F9 | té un planeta en trànsit (b) |
| Kepler-7 | | | | | | 19$^h$ 14$^m$ 19.56$^s$ | +41° 05′ 23.3″ | 13.3 | 3.9 | 1200 | G1 | té un planeta en trànsit (b) |
| Kepler-9 | | | | | | 19$^h$ 02$^m$ 18$^s$ | +38° 24′ 03″ | 13.9 | | 2300 | G2V | té un planeta en trànsit (b, c i d) |
| Kepler-38 | | | | | | 19$^h$ 07$^m$ 19.0$^s$ | +42° 16′ 45″ | 14.3 | | | | l'estrella A té un planeta en trànsit (b) |
| Kepler-60 | | | | | | 19$^h$ 15$^m$ 51.0$^s$ | +42° 15′ 54″ | 14.5 | | | | té tres planetes en trànsit (b, c i d) |
| Kepler-59 | | | | | | 19$^h$ 08$^m$ 09.0$^s$ | +46° 38′ 24″ | 14.8 | | | | té dos planetes en trànsit (b i c) |
| V477 Lyr | | | V477 | | | 18$^h$ 31$^m$ 18.29$^s$ | +26° 56′ 12.9″ | 15.07 | | | O9k | variable Algol; estrella central de la nebulosa planetària Abell 46 |
| Kepler-24 | | | | | | 19$^h$ 21$^m$ 39$^s$ | +38° 20′ 38″ | 15.5 | | | | té dos planetes en trànsit (b i c) i dos planetes no confirmats (d i e) |
| Kepler-30 | | | | | | 19$^h$ 01$^m$ 08.0$^s$ | +38° 56′ 50″ | 15.5 | | | | té tres planetes en trànsit (b, c i d) |
| Kepler-26 | | | | | | 18$^h$ 59$^m$ 46$^s$ | +46° 34′ 00″ | 16 | | | | té dos planetes en trànsit (b i c) i un planeta no confirmat (d) |
| Kepler-53 | | | | | | 19$^h$ 21$^m$ 51.0$^s$ | +40° 33′ 45″ | 16 | | | | té dos planetes en trànsit (b i c) |
| Kepler-55 | | | | | | 19$^h$ 00$^m$ 40.0$^s$ | +44° 01′ 35″ | 16.3 | | | | té dos planetes en trànsit (b i c) |
| HR Lyr | | | HR | 175268 | | 18$^h$ 53$^m$ 25.05$^s$ | +29° 13′ 37.7″ | 16.6 | | | | nova, V$_{max}$ = 6.5$^m$, V$_{min}$ = 16.6$^m$ |
| CY Lyr | | | CY | | | 18$^h$ 52$^m$ 41.38$^s$ | +26° 45′ 31.5″ | 18.0 | | | | variable SS Cyg, V$_{max}$ = 12.9$^m$, V$_{min}$ = 18.0$^m$, P = 0.1951 d |
| DM Lyr | | | DM | | | 18$^h$ 58$^m$ 44.43$^s$ | +30° 15′ 33.0″ | 18 | | | | variable SU UMa, V$_{max}$ = 13$^m$, V$_{min}$ = 18$^m$, P = 0.065409 d |
| 2MASS 1835+3259 | | | | | | 18$^h$ 35$^m$ 39.90$^s$ | +32° 59′ 54.6″ | 18.27 | | 18.48 | M8.5V | nana marró |
| V344 Lyr | | | V344 | | | 18$^h$ 44$^m$ 39.18$^s$ | +43° 22′ 28.1″ | 19 | | | | variable SU UMa, V$_{max}$ = 13.8$^m$, V$_{min}$ = 19$^m$, P = 0.087904 d |
| V361 Lyr | | | V361 | | | 19$^h$ 02$^m$ 28.12$^s$ | +46° 58′ 57.8″ | | | | F9V | variable Algol |
| AY Lyr | | | AY | | | 18$^h$ 44$^m$ 26.73$^s$ | +37° 59′ 51.8″ | | | | G... | variable SU UMa |
| MV Lyr | | | MV | | | 19$^h$ 07$^m$ 16.29$^s$ | +44° 01′ 07.8″ | | | | Op+... | nova |
| WISE 1828+2650 | | | | | | 18$^h$ 28$^m$ 31.08$^s$ | +26° 50′ 37.8″ | | | 47 | Y0 | nana marró |

## Vegeu també

* Llista d'estrelles per constel·lació

## Referències

* ↑ E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
* ESA. «The Hipparcos and Tycho Catalogues», 1997. [Consulta: 4 gener 2015].
* Gould, B. A. «Uranometria Argentina». Reprinted and updated by Pilcher, F. Arxivat de l'original el 2012-02-27. [Consulta: 4 gener 2015].
* Kostjuk, N. D. «HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index», 2002. [Consulta: 4 gener 2015].
* Roman, N. G. «Identification of a Constellation from a Position», 1987. [Consulta: 4 gener 2015].