# List of stars in Aquila

This is the list of 143 notable stars in the constellation Aquila, sorted by decreasing brightness.
| Name | B | F | G. | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| Altair | α | 53 | 86 | | 187642 | 97649 | 19$^h$ 50$^m$ 46.68$^s$ | +08° 52′ 02.6″ | 0.76 | 2.20 | 17 | A7IV-V | Atair, Al Nesr Al Tair, Vulture Volans; 12th brightest star; nearby; has two optical components; δ Sct variable, ΔV = 0.004$^m$, P = 0.06342 d |
| γ Aql | γ | 50 | | | 186791 | 97278 | 19$^h$ 46$^m$ 15.57$^s$ | +10° 36′ 47.8″ | 2.72 | −3.03 | 460 | K3II | Tarazed, Tarazad, Reda, Menkib al Nesr, Humerus Vulturis; double star; suspected variable |
| ζ Aql | ζ | 17 | | | 177724 | 93747 | 19$^h$ 05$^m$ 24.61$^s$ | +13° 51′ 49.4″ | 2.99 | 0.96 | 83 | A0Vn | Okab, Deneb el Okab, Denebokab Australis, Woo, Yuë (吳越), Dzeneb al Tair, Cauda (Vulturis) Volantis; triple star |
| θ Aql | θ | 65 | 117 | | 191692 | 99473 | 20$^h$ 11$^m$ 18.26$^s$ | −00° 49′ 17.3″ | 3.24 | −1.48 | 287 | B9.5III | Tseen Foo, Al Mizan III, Thanih Ras al Akab, Secunda Capitis Vulturis; spectroscopic binary; suspected variable |
| δ Aql | δ | 30 | 46 | | 182640 | 95501 | 19$^h$ 25$^m$ 29.75$^s$ | +03° 06′ 52.5″ | 3.36 | 2.43 | 50 | F0IV | Denebokab, Al Mizan I, Song, Sung, Djenubi Menkib al Nesr, Australior Humerus Vulturis; binary star; suspected variable |
| λ Aql | λ | 16 | 19 | | 177756 | 93805 | 19$^h$ 06$^m$ 14.95$^s$ | −04° 52′ 56.4″ | 3.43 | 0.51 | 125 | B9Vn | Al Thalimain |
| β Aql | β | 60 | 98 | | 188512 | 98036 | 19$^h$ 55$^m$ 18.77$^s$ | +06° 24′ 28.6″ | 3.71 | 3.03 | 45 | G8IVvar | Alshain, Alschain, Alschairn, Unuk al Ghyrab, Collum Corvi; binary star; suspected variable; triple star; suspected variable |
| η Aql | η | 55 | 89 | | 187929 | 97804 | 19$^h$ 52$^m$ 28.36$^s$ | +01° 00′ 20.4″ | 3.87 | −3.91 | 1173 | F6Ib-G4Ib | Al Mizan II; Cepheid variable, V$_{max}$ = 3.48$^m$, V$_{min}$ = 4.39$^m$, P = 7.17664 d |
| ε Aql | ε | 13 | | | 176411 | 93244 | 18$^h$ 59$^m$ 37.39$^s$ | +15° 04′ 06.5″ | 4.02 | 0.65 | 154 | K2III | Deneb el Okab, Denebokab Borealis, Woo, Yuë (吳越); triple star |
| 12 Aql | i | 12 | 9 | | 176678 | 93429 | 19$^h$ 01$^m$ 40.84$^s$ | −05° 44′ 20.5″ | 4.02 | 0.73 | 149 | K1IIIvar | suspected variable |
| 71 Aql | l | 71 | 146 | | 196574 | 101847 | 20$^h$ 38$^m$ 20.27$^s$ | −01° 06′ 18.3″ | 4.31 | −1.04 | 384 | G8III SB | spectroscopic binary |
| ι Aql | ι | 41 | 64 | | 184930 | 96468 | 19$^h$ 36$^m$ 43.28$^s$ | −01° 17′ 11.6″ | 4.36 | −0.51 | 307 | B5III | Al Thalimain; double star |
| μ Aql | μ | 38 | 58 | | 184406 | 96229 | 19$^h$ 34$^m$ 05.23$^s$ | +07° 22′ 45.5″ | 4.45 | 1.80 | 111 | K3III | multiple star; suspected variable |
| ν Aql | ν | 32 | 47 | | 182835 | 95585 | 19$^h$ 26$^m$ 31.09$^s$ | +00° 20′ 18.9″ | 4.64 | −8.12 | 11643 | F2Ib | double star; suspected variable |
| ξ Aql | ξ | 59 | 94 | | 188310 | 97938 | 19$^h$ 54$^m$ 14.882$^s$ | +08° 27′ 41.23″ | 4.722 | 0.74 | 204 | G9IIIb | Libertas, has a planet (b) |
| 69 Aql | | 69 | 141 | | 195135 | 101101 | 20$^h$ 29$^m$ 38.96$^s$ | −02° 53′ 07.7″ | 4.91 | 1.07 | 191 | K2III | |
| 70 Aql | | 70 | 144 | | 196321 | 101692 | 20$^h$ 36$^m$ 43.63$^s$ | −02° 32′ 59.7″ | 4.91 | −4.24 | 2203 | K5II | |
| κ Aql | κ | 39 | 63 | | 184915 | 96483 | 19$^h$ 36$^m$ 53.45$^s$ | −07° 01′ 38.9″ | 4.93 | −3.32 | 1455 | B0.5III | |
| 26 Aql | f | 26 | 38 | | 181391 | 95066 | 19$^h$ 20$^m$ 32.84$^s$ | −05° 24′ 57.1″ | 4.98 | 1.61 | 154 | G8III-IV... | spectroscopic binary |
| 4 Aql | | 4 | 2 | | 173370 | 91975 | 18$^h$ 44$^m$ 49.93$^s$ | +02° 03′ 36.3″ | 5.02 | −0.78 | 472 | B9V | |
| 36 Aql | e | 36 | 54 | | 183630 | 95937 | 19$^h$ 30$^m$ 39.82$^s$ | −02° 47′ 19.9″ | 5.03 | −0.91 | 502 | M1IIIvar | suspected variable |
| 18 Aql | | 18 | | Y | 178125 | 93867 | 19$^h$ 06$^m$ 58.60$^s$ | +11° 04′ 16.7″ | 5.07 | −0.89 | 507 | B8III | Y Aql; double star; eclipsing binary |
| 23 Aql | | 23 | 35 | | 180972 | 94885 | 19$^h$ 18$^m$ 32.49$^s$ | +01° 05′ 06.3″ | 5.10 | −0.24 | 381 | K2II-IIIvar | triple star |
| 37 Aql | | 37 | 59 | | 184492 | 96327 | 19$^h$ 35$^m$ 07.25$^s$ | −10° 33′ 37.6″ | 5.12 | −0.55 | 444 | G8III | |
| ο Aql | ο | 54 | | | 187691 | 97675 | 19$^h$ 51$^m$ 01.50$^s$ | +10° 24′ 57.8″ | 5.12 | 3.68 | 63 | F8V | multiple star system |
| 21 Aql | | 21 | 29 | V1288 | 179761 | 94477 | 19$^h$ 13$^m$ 42.70$^s$ | +02° 17′ 37.4″ | 5.14 | −1.33 | 640 | B8II-IIIp(Hg:) | V1288 Aql; double star; α$^2$ CVn variable, V$_{max}$ = 5.06$^m$, V$_{min}$ = 5.16$^m$, P = 1.73 d |
| 31 Aql | b | 31 | | | 182572 | 95447 | 19$^h$ 24$^m$ 57.77$^s$ | +11° 56′ 34.3″ | 5.17 | 4.27 | 49 | G8IVvar | triple star; suspected variable |
| σ Aql | σ | 44 | 68 | | 185507 | 96665 | 19$^h$ 39$^m$ 11.64$^s$ | +05° 23′ 52.0″ | 5.18 | −1.42 | 682 | B3V + B3V | β Lyr variable, ΔV = 0.2$^m$, P = 1.95026 d |
| 19 Aql | | 19 | 24 | | 178596 | 94068 | 19$^h$ 08$^m$ 59.92$^s$ | +06° 04′ 24.2″ | 5.23 | 2.03 | 142 | F0III-IV | |
| 11 Aql | | 11 | | | 176303 | 93203 | 18$^h$ 59$^m$ 05.73$^s$ | +13° 37′ 21.2″ | 5.27 | 1.88 | 155 | F8V | triple star; suspected variable |
| ω$^1$ Aql | ω$^1$ | 25 | | | 180868 | 94834 | 19$^h$ 17$^m$ 49.00$^s$ | +11° 35′ 43.4″ | 5.28 | −0.28 | 422 | F0IV | |
| χ Aql A | χ | 47 | | | 186203 | 96957 | 19$^h$ 42$^m$ 34.01$^s$ | +11° 49′ 35.8″ | 5.28 | −1.53 | 751 | F3V:+... | multiple star system |
| φ Aql | φ | 61 | | | 188728 | 98103 | 19$^h$ 56$^m$ 14.23$^s$ | +11° 25′ 25.4″ | 5.28 | 1.28 | 206 | A1IV | spectroscopic binary; suspected variable |
| 132 G. Aql | | | 132 | | 194013 | 100541 | 20$^h$ 23$^m$ 10.71$^s$ | +05° 20′ 35.1″ | 5.30 | 0.91 | 246 | G8III-IV | |
| FF Aql | | | | FF | 176155 | 93124 | 18$^h$ 58$^m$ 14.75$^s$ | +17° 21′ 39.4″ | 5.33 | −4.07 | 2470 | F5Ia-F8Ia | double star; Cepheid variable, V$_{max}$ = 5.18$^m$, V$_{min}$ = 5.68$^m$, P = 4.47092 d |
| 20 Aql | | 20 | 28 | | 179406 | 94385 | 19$^h$ 12$^m$ 40.70$^s$ | −07° 56′ 22.2″ | 5.35 | −2.51 | 1216 | B3V | |
| 51 Aql | | 51 | 82 | | 187532 | 97650 | 19$^h$ 50$^m$ 46.80$^s$ | −10° 45′ 48.9″ | 5.38 | 3.27 | 86 | F0V | binary star |
| 14 Aql | g | 14 | 11 | | 176984 | 93526 | 19$^h$ 02$^m$ 54.49$^s$ | −03° 41′ 56.4″ | 5.40 | −0.53 | 499 | A1V | double star |
| 15 Aql | h | 15 | 15 | | 177463 | 93717 | 19$^h$ 04$^m$ 57.66$^s$ | −04° 01′ 52.9″ | 5.40 | 0.41 | 325 | K1III | double star; suspected variable |
| 66 Aql | | 66 | 123 | | 192107 | 99631 | 20$^h$ 13$^m$ 13.87$^s$ | −01° 00′ 33.4″ | 5.44 | −1.74 | 888 | K5III | |
| 42 Aql | | 42 | 65 | | 185124 | 96556 | 19$^h$ 37$^m$ 47.26$^s$ | −04° 38′ 51.0″ | 5.45 | 2.92 | 105 | F3IV | |
| 27 Aql | d | 27 | 40 | | 181440 | 95073 | 19$^h$ 20$^m$ 35.68$^s$ | −00° 53′ 31.8″ | 5.46 | −0.51 | 509 | B9III | |
| τ Aql | τ | 63 | 107 | | 190327 | 98823 | 20$^h$ 04$^m$ 08.31$^s$ | +07° 16′ 40.6″ | 5.51 | −0.53 | 527 | K0III | |
| 28 Aql | A | 28 | | V1208 | 181333 | 94982 | 19$^h$ 19$^m$ 39.35$^s$ | +12° 22′ 28.7″ | 5.53 | 0.39 | 347 | F0III | V1208 Aql; triple star; δ Sct variable, V$_{max}$ = 5.51$^m$, V$_{min}$ = 5.56$^m$, P = 0.149663 d |
| | | | | | 183492 | 95822 | 19$^h$ 29$^m$ 22.12$^s$ | +14° 35′ 45.9″ | 5.57 | 0.85 | 286 | K0III | |
| 62 Ser | | (62) | 69 | | 175515 | 92872 | 18$^h$ 55$^m$ 27.44$^s$ | +06° 36′ 55.8″ | 5.58 | 0.81 | 293 | G9III | 69 G. Aquilae, suspected variable |
| HD 180262 | | | | | 180262 | 94624 | 19$^h$ 15$^m$ 20.09$^s$ | +15° 05′ 01.2″ | 5.58 | −0.79 | 613 | G8II-III | double star |
| 22 Aql | | 22 | 32 | | 180482 | 94727 | 19$^h$ 16$^m$ 31.02$^s$ | +04° 50′ 05.4″ | 5.59 | −0.53 | 546 | A3IV | |
| 58 Aql | | 58 | 95 | | 188350 | 97980 | 19$^h$ 54$^m$ 44.77$^s$ | +00° 16′ 25.2″ | 5.60 | 0.48 | 345 | A0III | |
| V1291 Aql | | | 90 | V1291 | 188041 | 97871 | 19$^h$ 53$^m$ 18.72$^s$ | −03° 06′ 52.2″ | 5.63 | 0.99 | 277 | A5p(Sr-Cr-Eu) | α$^2$ CVn variable, V$_{max}$ = 5.61$^m$, V$_{min}$ = 5.67$^m$, P = 224.5 d |
| 45 Aql | | 45 | 70 | | 185762 | 96807 | 19$^h$ 40$^m$ 43.31$^s$ | −00° 37′ 16.7″ | 5.64 | 0.93 | 285 | A3IV | double star |
| HD 180555 | | | | | 180555 | 94720 | 19$^h$ 16$^m$ 26.78$^s$ | +14° 32′ 40.6″ | 5.65 | 0.36 | 372 | B9.5V | binary star |
| 62 Aql | | 62 | 106 | | 190299 | 98844 | 20$^h$ 04$^m$ 23.15$^s$ | −00° 42′ 32.5″ | 5.67 | −0.59 | 582 | K4III | |
| π Aql B | π | 52 | | | 187260 | | 19$^h$ 48$^m$ 42.10$^s$ | +11° 48′ 55.0″ | 5.70 | | | | component of the π Aql system |
| 57 Aql A | | 57 | 93 | | 188293 | 97966 | 19$^h$ 54$^m$ 37.65$^s$ | −08° 13′ 38.0″ | 5.70 | 0.64 | 335 | B7Vn | double star |
| 14 Sge | | (14) | | | 190229 | 98754 | 20$^h$ 03$^m$ 30.01$^s$ | +16° 01′ 52.6″ | 5.73 | −0.72 | 637 | B9MNp... | |
| π Aql | π | 52 | | | 187259 | 97473 | 19$^h$ 48$^m$ 42.05$^s$ | +11° 48′ 57.3″ | 5.75 | −0.46 | 570 | F2V:+... | component of the π Aql system |
| | | | | | 182900 | 95572 | 19$^h$ 26$^m$ 24.13$^s$ | +13° 01′ 25.2″ | 5.76 | 2.03 | 182 | F6III | |
| 56 Aql | | 56 | 92 | | 188154 | 97928 | 19$^h$ 54$^m$ 08.27$^s$ | −08° 34′ 27.0″ | 5.76 | 0.35 | 394 | K5III | double star |
| 35 Aql | c | 35 | 51 | V1431 | 183324 | 95793 | 19$^h$ 29$^m$ 00.99$^s$ | +01° 57′ 01.9″ | 5.79 | 1.94 | 192 | A0V | V1431 Aql; rapidly oscillating α$^2$ CVn variable, ΔV = 0.04$^m$ |
| 42 G. Aql | | | 42 | | 181907 | 95222 | 19$^h$ 22$^m$ 21.51$^s$ | −00° 15′ 08.2″ | 5.81 | 0.58 | 363 | G8III: | |
| 13 G. Aql | | | 13 | | 177178 | 93580 | 19$^h$ 03$^m$ 32.24$^s$ | +01° 49′ 08.2″ | 5.82 | 2.11 | 180 | A4V | |
| 49 G. Aql | | | 49 | | 183227 | 95732 | 19$^h$ 28$^m$ 20.80$^s$ | +02° 55′ 48.2″ | 5.84 | −1.65 | 1025 | B6III | |
| 100 G. Aql | | | 100 | | 189340 | 98416 | 19$^h$ 59$^m$ 47.49$^s$ | −09° 57′ 26.2″ | 5.87 | 3.92 | 80 | F8V | |
| 5 Aql | | 5 | 3 | | 173654 | 92117 | 18$^h$ 46$^m$ 28.58$^s$ | −00° 57′ 41.9″ | 5.89 | 1.40 | 258 | A2m | binary star |
| υ Aql | υ | 49 | 78 | | 186689 | 97229 | 19$^h$ 45$^m$ 39.92$^s$ | +07° 36′ 47.4″ | 5.89 | 2.22 | 176 | A3IV | |
| 103 G. Aql | | | 103 | | 189695 | 98526 | 20$^h$ 00$^m$ 58.97$^s$ | +08° 33′ 28.0″ | 5.90 | −1.30 | 898 | K5III | |
| 10 Aql | | 10 | | V1286 | 176232 | 93179 | 18$^h$ 58$^m$ 46.92$^s$ | +13° 54′ 24.4″ | 5.91 | 1.55 | 242 | A4p(Eu-Cr-Sr) | V1286 Aql; α$^2$ CVn variable, V$_{max}$ = 5.83$^m$, V$_{min}$ = 5.93$^m$, P = 6.05 d |
| 64 Aql | | 64 | 113 | | 191067 | 99171 | 20$^h$ 08$^m$ 01.75$^s$ | −00° 40′ 40.9″ | 5.97 | 2.57 | 156 | K1IV | |
| HD 185018 | | | | | 185018 | 96481 | 19$^h$ 36$^m$ 52.45$^s$ | +11° 16′ 23.5″ | 5.98 | −1.74 | 1140 | G0Ib | multiple star |
| QS Aql | | | | QS | 185936 | 96840 | 19$^h$ 41$^m$ 05.53$^s$ | +13° 48′ 56.5″ | 5.98 | −2.54 | 1646 | B5V | double star; Algol variable, V$_{max}$ = 5.93$^m$, V$_{min}$ = 6.06$^m$, P = 2.51329 d |
| 80 G. Aql | | | 80 | | 187195 | 97499 | 19$^h$ 49$^m$ 02.19$^s$ | −10° 52′ 14.6″ | 6.00 | 1.29 | 285 | K5III | |
| ω$^2$ Aql | ω$^2$ | 29 | | | 181383 | 95002 | 19$^h$ 19$^m$ 53.04$^s$ | +11° 32′ 05.7″ | 6.03 | 1.37 | 278 | A2V | |
| 131 G. Aql | | | 131 | | 193329 | 100232 | 20$^h$ 19$^m$ 43.24$^s$ | −01° 04′ 42.9″ | 6.05 | 0.58 | 405 | K0 | |
| 8 Aql | | 8 | 5 | V1729 | 174589 | 92524 | 18$^h$ 51$^m$ 22.16$^s$ | −03° 19′ 04.1″ | 6.08 | 1.44 | 276 | F2III | V1729 Aql; Delta Scuti variable |
| HD 183589 | | | 53 | | 183589 | 95898 | 19$^h$ 30$^m$ 10.53$^s$ | +02° 54′ 14.7″ | 6.08 | −2.46 | 1663 | K5Ib | multiple star; suspected variable |
| V923 Aql | | | 55 | V923 | 183656 | 95929 | 19$^h$ 30$^m$ 33.11$^s$ | +03° 26′ 39.8″ | 6.09 | −1.26 | 962 | B5.5IIIpe-B8V | γ Cas variable, ΔV = 0.12$^m$ |
| R Aql | | | 22 | R | 177940 | 93820 | 19$^h$ 06$^m$ 22.25$^s$ | +08° 13′ 48.0″ | 6.09 | −2.04 | 1400 | M6.5-9e | Mira variable, V$_{max}$ = 5.5$^m$, V$_{min}$ = 12.0$^m$, P = 270.5 d |
| 137 G. Aql | | | 137 | | 194454 | 100758 | 20$^h$ 25$^m$ 42.53$^s$ | −02° 48′ 01.0″ | 6.10 | −0.60 | 713 | K1III: | |
| V500 Aql | | | | V500 | | | 19$^h$ 52$^m$ 27.98$^s$ | +08° 28′ 41.6″ | 6.1 | | | pec(NOVA) – e+cont | Nova Aquilae; V$_{max}$ = 6.1$^m$, V$_{min}$ = 17.8$^m$ |
| 85 G. Aql | | | 85 | | 187660 | 97687 | 19$^h$ 51$^m$ 11.10$^s$ | −02° 27′ 39.2″ | 6.12 | −0.09 | 570 | K5III | |
| 68 Aql | | 68 | 139 | | 194939 | 100977 | 20$^h$ 28$^m$ 24.89$^s$ | −03° 21′ 27.9″ | 6.12 | −0.04 | 557 | B9V | double star |
| HD 188385 | | | 96 | | 188385 | 97970 | 19$^h$ 54$^m$ 40.18$^s$ | +07° 08′ 25.3″ | 6.14 | 1.60 | 263 | A2V | double star |
| HD 194244 | | | 135 | | 194244 | 100664 | 20$^h$ 24$^m$ 37.49$^s$ | +01° 04′ 06.2″ | 6.14 | −0.92 | 840 | B9V | triple star; suspected variable |
| HD 187923 | | | | | 187923 | 97767 | 19$^h$ 52$^m$ 03.64$^s$ | +11° 37′ 44.9″ | 6.16 | 3.95 | 90 | G0V | double star; suspected variable |
| 101 G. Aql | | | 101 | | 189322 | 98385 | 19$^h$ 59$^m$ 22.63$^s$ | +01° 22′ 39.1″ | 6.17 | −0.69 | 769 | G8III | |
| 34 G. Aql | | | 34 | | 180782 | 94833 | 19$^h$ 17$^m$ 48.18$^s$ | +02° 01′ 54.5″ | 6.19 | 1.56 | 275 | A1Vn | |
| 6 G. Aql | | | 6 | | 175640 | 92963 | 18$^h$ 56$^m$ 22.66$^s$ | −01° 47′ 59.3″ | 6.20 | 0.17 | 525 | B9III | |
| 145 G. Aql | | | 145 | | 196426 | 101746 | 20$^h$ 37$^m$ 18.38$^s$ | +00° 05′ 49.2″ | 6.21 | −0.26 | 643 | B8IIIp | |
| 7 G. Aql | | | 7 | | 176095 | 93138 | 18$^h$ 58$^m$ 23.71$^s$ | +06° 14′ 24.7″ | 6.22 | 2.45 | 185 | F5IV | |
| 4 G. Aql | | | 4 | | 174240 | 92386 | 18$^h$ 49$^m$ 37.18$^s$ | +00° 50′ 10.4″ | 6.24 | 0.01 | 575 | A1V | |
| 12 G. Aql | | | 12 | | 176981 | 93488 | 19$^h$ 02$^m$ 21.56$^s$ | +08° 22′ 24.7″ | 6.25 | −0.83 | 849 | K2III | |
| 52 G. Aql | | | 52 | | 183387 | 95812 | 19$^h$ 29$^m$ 18.02$^s$ | +00° 14′ 46.0″ | 6.25 | −0.08 | 603 | K2 | |
| ψ Aql | ψ | 48 | | | 186547 | 97139 | 19$^h$ 44$^m$ 34.19$^s$ | +13° 18′ 10.1″ | 6.25 | −0.72 | 809 | B9III-IV | |
| 88 G. Aql | | | 88 | | 187753 | 97697 | 19$^h$ 51$^m$ 17.73$^s$ | +09° 37′ 47.8″ | 6.25 | 0.92 | 380 | A1m | |
| HD 191984 | | | 120 | | 191984 | 99585 | 20$^h$ 12$^m$ 35.12$^s$ | +00° 52′ 01.6″ | 6.25 | −0.08 | 603 | A0 | double star |
| 37 G. Aql | | | 37 | | 181122 | 94916 | 19$^h$ 18$^m$ 52.75$^s$ | +09° 37′ 05.4″ | 6.31 | 0.31 | 517 | G9III | Les Grey |
| 43 G. Aql | | | 43 | | 182038 | 95281 | 19$^h$ 23$^m$ 04.44$^s$ | −07° 24′ 02.0″ | 6.31 | 0.41 | 493 | K0 | |
| HD 183144 | | | | | 183144 | 95664 | 19$^h$ 27$^m$ 33.90$^s$ | +14° 16′ 57.0″ | 6.31 | −0.73 | 834 | B4III | suspected variable |
| 71 G. Aql | | | 71 | | 185966 | 96917 | 19$^h$ 42$^m$ 02.90$^s$ | −09° 11′ 36.4″ | 6.31 | 1.26 | 334 | K2 | |
| 60 G. Aql | | | 60 | | 184573 | 96356 | 19$^h$ 35$^m$ 29.79$^s$ | −07° 27′ 36.7″ | 6.32 | 1.13 | 355 | K0 | |
| 46 Aql | | 46 | | | 186122 | 96931 | 19$^h$ 42$^m$ 12.81$^s$ | +12° 11′ 35.8″ | 6.33 | −0.39 | 720 | B9III | |
| 25 G. Aql | | | 25 | | 178744 | 94149 | 19$^h$ 09$^m$ 51.59$^s$ | −00° 25′ 41.2″ | 6.34 | −0.80 | 874 | B5Vn | |
| 44 G. Aql | | | 44 | | 182101 | 95253 | 19$^h$ 22$^m$ 48.35$^s$ | +09° 54′ 46.4″ | 6.34 | 3.58 | 116 | F6V | |
| | | | | | 191263 | 99234 | 20$^h$ 08$^m$ 38.28$^s$ | +10° 43′ 33.1″ | 6.34 | −2.42 | 1842 | B3IV | |
| V450 Aql | | | | V450 | 184313 | 96204 | 19$^h$ 33$^m$ 46.03$^s$ | +05° 27′ 56.8″ | 6.35 | −0.75 | 858 | M5III-M8III | semiregular variable, V$_{max}$ = 6.30$^m$, V$_{min}$ = 6.65$^m$, P = 64.20 d |
| 67 G. Aql | | | 67 | | 185423 | 96630 | 19$^h$ 38$^m$ 48.99$^s$ | +03° 22′ 53.5″ | 6.36 | | | B3III | |
| HD 174569 | | | | | 174569 | 92475 | 18$^h$ 50$^m$ 45.55$^s$ | +10° 58′ 35.0″ | 6.37 | −2.41 | 1863 | K5III+... | double star |
| U Aql | | | 50 | U | 183344 | 95820 | 19$^h$ 29$^m$ 21.36$^s$ | −07° 02′ 38.6″ | 6.37 | −2.07 | 1590 | F5-G1I-II | Cepheid variable, V$_{max}$ = 6.08$^m$, V$_{min}$ = 6.86$^m$, P = 7.02393 d |
| 61 G. Aql | | | 61 | | 184663 | 96351 | 19$^h$ 35$^m$ 25.13$^s$ | +02° 54′ 48.5″ | 6.37 | 3.25 | 137 | F6IV | |
| | | | | | 184944 | 96428 | 19$^h$ 36$^m$ 15.68$^s$ | +14° 23′ 28.2″ | 6.37 | 1.19 | 354 | K0II-III | |
| V1472 Aql | | | | V1472 | 190658 | 98954 | 20$^h$ 05$^m$ 26.53$^s$ | +15° 30′ 01.3″ | 6.37 | −0.44 | 749 | M2 comp | eclipsing variable, ΔV = ~0.16$^m$ |
| V1401 Aql | | (64) | 108 | V1401 | 190390 | 98910 | 20$^h$ 05$^m$ 05.42$^s$ | −11° 35′ 57.8″ | 6.38 | −1.58 | 1273 | F1III | 64 Sagittarii; semiregular variable, V$_{max}$ = 6.18$^m$, V$_{min}$ = 6.55$^m$ |
| 24 Aql | | 24 | 36 | | 181053 | 94913 | 19$^h$ 18$^m$ 50.93$^s$ | +00° 20′ 20.4″ | 6.40 | 0.52 | 488 | K0II-III:.. | multiple star |
| 136 G. Aql | | | 136 | | 194263 | 100672 | 20$^h$ 24$^m$ 41.75$^s$ | +01° 22′ 07.0″ | 6.41 | −0.71 | 865 | K5 | |
| 75 G. Aql | | | 75 | | 186535 | 97144 | 19$^h$ 44$^m$ 41.27$^s$ | +08° 43′ 35.7″ | 6.43 | 1.00 | 398 | K0 | |
| HD 191104 | | | 114 | | 191104 | 99158 | 20$^h$ 07$^m$ 50.34$^s$ | +09° 23′ 59.1″ | 6.43 | 3.25 | 141 | F3V | double star |
| | | | | | 187203 | 97454 | 19$^h$ 48$^m$ 30.51$^s$ | +10° 41′ 38.8″ | 6.44 | −2.22 | 1762 | F8Ib-II | |
| HD 192699 | | | 128 | | 192699 | 99894 | 20$^h$ 16$^m$ 06.03$^s$ | +04° 34′ 51.3″ | 6.44 | 2.30 | 220 | G8IV | Chechia, has a planet (b) |
| HD 179791 | | | 30 | | 179791 | 94478 | 19$^h$ 13$^m$ 44.02$^s$ | +05° 30′ 56.3″ | 6.47 | 0.15 | 598 | A3V | suspected variable |
| 77 G. Aql | | | 77 | | 186660 | 97244 | 19$^h$ 45$^m$ 52.23$^s$ | −02° 53′ 00.4″ | 6.47 | −1.14 | 1087 | B3III | |
| 87 G. Aql | | | 87 | | 187734 | 97709 | 19$^h$ 51$^m$ 26.84$^s$ | +04° 05′ 19.1″ | 6.47 | | | K0... | double star |
| 110 G. Aql | | | 110 | | 190664 | 99024 | 20$^h$ 06$^m$ 12.19$^s$ | −04° 04′ 41.2″ | 6.47 | 1.37 | 341 | K0 | |
| 122 G. Aql | | | 122 | | 192086 | 99624 | 20$^h$ 13$^m$ 04.43$^s$ | −00° 19′ 50.9″ | 6.47 | −1.94 | 1567 | K5 | |
| 142 G. Aql | | | 142 | | 195617 | 101339 | 20$^h$ 32$^m$ 20.40$^s$ | +02° 07′ 58.1″ | 6.47 | −1.23 | 1132 | K2 | |
| V1339 Aql | | | 84 | V1339 | 187567 | 97607 | 19$^h$ 50$^m$ 17.48$^s$ | +07° 54′ 08.7″ | 6.49 | −1.90 | 1552 | B2.5IVe | Be star; γ Cas variable, V$_{max}$ = 6.33$^m$, V$_{min}$ = 6.52$^m$ |
| 57 Aql B | | 57 | | | 188294 | 97967 | 19$^h$ 54$^m$ 38.06$^s$ | −08° 14′ 13.1″ | 6.49 | 1.27 | 361 | B8V | component of the 57 Aql system |
| HD 188405 | | | 97 | | 188405 | 98038 | 19$^h$ 55$^m$ 19.49$^s$ | −06° 44′ 04.7″ | 6.49 | 1.83 | 279 | F2V | double star |
| V1691 Aql | | | 45 | V1691 | 182475 | 95453 | 19$^h$ 25$^m$ 01.51$^s$ | −04° 53′ 04.4″ | 6.50 | 1.48 | 329 | A9V | δ Sct variable, ΔV = 0.04$^m$, P = 0.0781 d |
| V Aql | | | | V | 177336 | 93666 | 19$^h$ 04$^m$ 24.15$^s$ | −05° 41′ 05.4″ | 6.78 | −1.36 | 1207 | C5,4 – C6,4(N6) | carbon star; semiregular variable, V$_{max}$ = 6.6$^m$, V$_{min}$ = 8.4$^m$, P = 353 d |
| TT Aql | | | | TT | 178359 | 93990 | 19$^h$ 08$^m$ 13.75$^s$ | +01° 17′ 55.2″ | 7.10 | −4.84 | 7951 | F6-G5 | Cepheid variable, V$_{max}$ = 6.46$^m$, V$_{min}$ = 7.70$^m$, P = 13.7546 d |
| HD 186641 | | | | | 186641 | 97233 | 19$^h$ 45$^m$ 41.0$^s$ | −00° 41′ 48″ | 7.34 | 2.2 | 347 | K0 | has a planet (b) |
| V604 Aql | | | | V604 | | | 19$^h$ 02$^m$ 6.33$^s$ | −04° 26′ 43.2″ | 7.6 | | | pec(NOVA) – e+cont | Nova Aquilae; V$_{max}$ = 7.6$^m$, V$_{min}$ = 18.0$^m$ |
| HD 183263 | | | | | 183263 | 95740 | 19$^h$ 28$^m$ 24.57$^s$ | +08° 21′ 29.0″ | 7.86 | 4.25 | 172 | G2IV | has two planets (b & c) |
| HD 179079 | | | | | 179079 | 94256 | 19$^h$ 11$^m$ 09.83$^s$ | −02° 38′ 18.2″ | 7.96 | 3.94 | 208 | G5IV | has a planet (b) |
| V1703 Aql | | | | V1703 | 192263 | 99711 | 20$^h$ 13$^m$ 59.85$^s$ | −00° 52′ 00.8″ | 8.10 | 6.61 | 65 | K2V | Phoenicia, double star; has a planet (b); BY Draconis variable, ΔV = 0.03$^m$, P = 23.98 d |
| HD 176986 | | | | | 176986 | 93540 | 19$^h$ 03$^m$ 06.0$^s$ | −11° 02′ 38″ | 8.45 | | 86 | K2.5V | has two planets (b & c) |
| HD 181234 | | | | | 181234 | 95015 | 19$^h$ 20$^m$ 00.0$^s$ | −09° 19′ 25″ | 8.59 | | 156 | G5 | has a planet (b) |
| Gliese 726 | | | | | 173818 | 92200 | 18$^h$ 47$^m$ 27$^s$ | −03° 38′ 23″ | 8.70 | 8.17 | 46.07 | K5V | |
| V1494 Aql | | | | V1494 | | | 19$^h$ 23$^m$ 5.38$^s$ | +04° 57′ 20.1″ | 8.8 | | | pec(NOVA) – e+cont | Nova Aquilae; V$_{max}$ = 5.03$^m$, V$_{min}$ = 16.0$^m$ |
| WASP-74 | | | | | | | 20$^h$ 18$^m$ 10.0$^s$ | −01° 04′ 33″ | 9.7 | 4.31 | 391 | F9 | has a transiting planet (b) |
| HAT-P-41 | | | | | | | 19$^h$ 49$^m$ 17.0$^s$ | +04° 40′ 21″ | 11.09 | 3.63 | 1014 | | has a transiting planet (b) |
| V603 Aql | | | | V603 | 174107 | 92316 | 18$^h$ 48$^m$ 54.64$^s$ | +00° 35′ 02.9″ | 11.64 | 4.76 | 776 | pec(NOVA) – e+cont | Nova Aquilae 1918; V$_{max}$ = −1.4$^m$, V$_{min}$ = 12.03$^m$ |
| WASP-80 | | | | | | | 20$^h$ 12$^m$ 40.0$^s$ | −02° 08′ 44″ | 11.88 | 7.99 | 196 | | Petra, has a transiting planet (b) |
| IRC -10414 | | | | | | | 19$^h$ 42$^m$ 37.90$^s$ | +11° 50′ 31.0″ | 12.0 | | 6,520 | M7 I | |
| χ Aql B | χ | 47 | | | 186204 | | 19$^h$ 42$^m$ 37.90$^s$ | +11° 50′ 31.0″ | 12.30 | 5.35 | 800 | G0:+A3V | component of the χ Aql system |
| CoRoT-2 | | | | | | | 19$^h$ 27$^m$ 07$^s$ | +01° 23′ 02″ | 12.57 | 5.29 | 930 | G7V | has a transiting planet (b) |
| CoRoT-3 | | | | | | | 19$^h$ 28$^m$ 13.27$^s$ | +00° 07′ 18.6″ | 13.3 | 4.16 | 2200 | F3V | has a transiting brown dwarf (b) |
| SS 433 | | | | V1343 | | | 19$^h$ 11$^m$ 49.56$^s$ | +04° 58′ 57.6″ | 14.2 | | 15093 | A7Ib | Sanduleak-Stephenson Star; eclipsing X-ray binary |
| CoRoT-8 | | | | | | | 19$^h$ 26$^m$ 21.24$^s$ | +01° 25′ 35.2″ | 14.80 | 6.89 | ~1250 | K1V | has a transiting planet (b) |
| CoRoT-10 | | | | | | | 19$^h$ 24$^m$ 15.30$^s$ | +00° 44′ 46.0″ | 15.22 | 7.53 | ~1130 | K1V | has a transiting planet (b) |
| VB 10 | | | | | | | 19$^h$ 16$^m$ 57.62$^s$ | +05° 09′ 02.2″ | 17.30 | 18.47 | 19 | M8V | van Biesbroeck's Star |
| V606 Aql | | | | V606 | | | 19$^h$ 20$^m$ 24.3$^s$ | −00° 08′ 7.0″ | | | 700 | pec(NOVA) – e+cont | Nova Aquilae; V$_{max}$ = 5.5$^m$, V$_{min}$ = 17.3$^m$ |
| W50 (nebula) | | | | | | | 19$^h$ 11$^m$ 49$^s$ | −04° 59′ 12.0″ | | | 16000 | | Supernova remnant |
| 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.] ||||||||||||||