# List of stars in Sagitta

This is the list of notable stars in the constellation Sagitta, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| γ Sge | γ | 12 | | 189319 | 98337 | 19$^h$ 58$^m$ 45.39$^s$ | +19° 29′ 31.5″ | 3.51 | −1.11 | 274 | K5III | variable star, ΔV = 0.004$^m$, P = 6.37836 d |
| δ Sge | δ | 7 | | 187076 | 97365 | 19$^h$ 47$^m$ 23.27$^s$ | +18° 32′ 03.3″ | 3.82 | −1.87 | 448 | M2II + B6 | semiregular variable, V$_{max}$ = 3.75$^m$, V$_{min}$ = 3.83$^m$ |
| α Sge | α | 5 | | 185758 | 96757 | 19$^h$ 40$^m$ 05.78$^s$ | +18° 00′ 50.2″ | 4.38 | −1.42 | 473 | G0II | Sham, Alsahm |
| β Sge | β | 6 | | 185958 | 96837 | 19$^h$ 41$^m$ 02.93$^s$ | +17° 28′ 34.0″ | 4.38 | −1.39 | 466 | G8II | |
| ζ Sge | ζ | 8 | | 187362 | 97496 | 19$^h$ 48$^m$ 58.65$^s$ | +19° 08′ 31.1″ | 5.01 | 0.01 | 326 | A3V | |
| η Sge | η | 16 | | 190608 | 98920 | 20$^h$ 05$^m$ 09.47$^s$ | +19° 59′ 27.2″ | 5.09 | 1.61 | 162 | K2III | suspected variable |
| 13 Sge | | 13 | VZ | 189577 | 98438 | 20$^h$ 00$^m$ 03.31$^s$ | +17° 30′ 59.5″ | 5.33 | −1.47 | 746 | M4IIIa | semiregular variable, V$_{max}$ = 5.27$^m$, V$_{min}$ = 5.57$^m$ |
| 11 Sge | | 11 | | 189090 | 98234 | 19$^h$ 57$^m$ 45.44$^s$ | +16° 47′ 20.8″ | 5.54 | 0.07 | 404 | B9III | |
| 1 Sge | | 1 | | 180317 | 94620 | 19$^h$ 15$^m$ 17.34$^s$ | +21° 13′ 55.6″ | 5.65 | 0.71 | 318 | A4V | |
| ε Sge | ε | 4 | | 185194 | 96516 | 19$^h$ 37$^m$ 17.38$^s$ | +16° 27′ 46.0″ | 5.67 | −0.14 | 473 | G8IIIvar | suspected variable, V$_{max}$ = 5.64$^m$, V$_{min}$ = 5.67$^m$ |
| S Sge | | 10 | S | 188727 | 98085 | 19$^h$ 56$^m$ 01.26$^s$ | +16° 38′ 05.3″ | 5.71 | −4.89 | 4289 | G5Ibv SB | Cepheid variable, V$_{max}$ = 5.24$^m$, V$_{min}$ = 6.04$^m$, P = 8.382086 d |
| 15 Sge | | 15 | | 190406 | 98819 | 20$^h$ 04$^m$ 06.47$^s$ | +17° 04′ 16.2″ | 5.80 | 4.56 | 58 | G1V | binary star; suspected variable, V$_{max}$ = 5.77$^m$, V$_{min}$ = 5.80$^m$ |
| HD 193579 | | | | 193579 | 100276 | 20$^h$ 20$^m$ 21.40$^s$ | +17° 47′ 34.8″ | 5.82 | −0.01 | 477 | K5III | |
| HD 190211 | | | | 190211 | 98738 | 20$^h$ 03$^m$ 16.39$^s$ | +18° 30′ 03.7″ | 5.99 | −1.09 | 849 | K3Iab: | |
| HD 180242 | | | | 180242 | 94598 | 19$^h$ 15$^m$ 02.69$^s$ | +20° 12′ 11.3″ | 6.03 | −0.70 | 724 | G8III | suspected variable, V$_{max}$ = 6$^m$, V$_{min}$ = 6.04$^m$ |
| HD 178428 | | | | 178428 | 93966 | 19$^h$ 07$^m$ 57.28$^s$ | +16° 51′ 14.9″ | 6.08 | 4.47 | 68 | G5V | spectroscopic binary |
| HD 177199 | | | | 177199 | 93523 | 19$^h$ 02$^m$ 52.62$^s$ | +19° 39′ 39.7″ | 6.11 | −2.26 | 1538 | K1III | |
| 18 Sge | | 18 | | 192836 | 99913 | 20$^h$ 16$^m$ 19.78$^s$ | +21° 35′ 55.5″ | 6.11 | 1.31 | 298 | K1III | |
| 9 Sge | | 9 | QZ | 188001 | 97796 | 19$^h$ 52$^m$ 21.77$^s$ | +18° 40′ 18.8″ | 6.23 | −6.96 | 14174 | O8e | spectroscopic eclipsing binary, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.23$^m$ |
| HD 191814 | | | | 191814 | 99445 | 20$^h$ 11$^m$ 03.53$^s$ | +21° 08′ 04.2″ | 6.24 | 0.25 | 514 | K0 | |
| 2 Sge | | 2 | | 182490 | 95398 | 19$^h$ 24$^m$ 22.08$^s$ | +16° 56′ 15.9″ | 6.27 | 1.08 | 355 | A2III-IV | |
| V340 Sge | | | V340 | 185622 | 96688 | 19$^h$ 39$^m$ 25.34$^s$ | +16° 34′ 16.1″ | 6.37 | −2.87 | 2296 | M0Iab-Ib SB | slow irregular variable |
| V344 Sge | | | V344 | 191178 | 99176 | 20$^h$ 08$^m$ 06.50$^s$ | +16° 39′ 51.7″ | 6.39 | −4.18 | 4234 | M3III | irregular variable |
| HD 180377 | | | | 180377 | 94646 | 19$^h$ 15$^m$ 33.37$^s$ | +18° 30′ 58.8″ | 6.46 | −1.13 | 1072 | M2III | semiregular variable |
| HD 176776 | | | | 176776 | 93374 | 19$^h$ 01$^m$ 05.43$^s$ | +19° 18′ 34.6″ | 6.47 | 0.74 | 457 | K1III | |
| U Sge | | | U | 181182 | 94910 | 19$^h$ 18$^m$ 48.41$^s$ | +19° 36′ 37.7″ | 6.50 | −0.96 | 1012 | B8III + K | Algol variable, V$_{max}$ = 6.45$^m$, V$_{min}$ = 9.28$^m$, P = 3.38061933 d |
| θ Sge A | θ | 17 | | 191570 | 99352 | 20$^h$ 09$^m$ 56.61$^s$ | +20° 54′ 53.2″ | 6.51 | 3.24 | 147 | F5IV | |
| V338 Sge | | | V338 | 179588 | 94377 | 19$^h$ 12$^m$ 34.45$^s$ | +16° 50′ 47.1″ | 6.69 | | 791 | B9IV | Eclipsing binary |
| 3 Sge | | 3 | | 182571 | 95435 | 19$^h$ 24$^m$ 45.39$^s$ | +16° 57′ 25.4″ | 6.84 | 1.36 | 407 | A0 | |
| HD 183143 | | | HT | 183143 | 95657 | 19$^h$ 27$^m$ 26.56$^s$ | +18° 17′ 45.2″ | 6.86 | | 7100 | B7Iae | Alpha Cygni variable, V$_{max}$ = 6.71$^m$, V$_{min}$ = 6.95$^m$, P = 40.44 d |
| θ Sge B | θ | 17 | | 191571 | | 20$^h$ 09$^m$ 52.30$^s$ | +20° 53′ 47.0″ | 8.90 | | | | component of the θ Sge system |
| HD 231701 | | | | 231701 | 96078 | 19$^h$ 32$^m$ 04.16$^s$ | +16° 28′ 27.4″ | 8.99 | 3.81 | 354 | F8V | Uruk; has a planet (b) |
| R Sge | | | R | 192388 | | 20$^h$ 14$^m$ 03.75$^s$ | +16° 43′ 35.1″ | 9.20 | | | G0Ib | RV Tauri variable, V$_{max}$ = 8.0$^m$, V$_{min}$ = 10.5$^m$, P = 70.77 d |
| FG Sge | | | FG | | 99527 | 20$^h$ 11$^m$ 56.06$^s$ | +20° 20′ 04.4″ | 9.45 | | 606 | B4Ieq-K2Ib | V$_{max}$ = 8.7$^m$, V$_{min}$ = 18.1$^m$ |
| V Sge | | | V | | | 20$^h$ 20$^m$ 14.69$^s$ | +21° 06′ 10.44″ | 9.6-13 | | 7800 | | prototype V Sagittae variable, V$_{max}$ = 8.16$^m$, V$_{min}$ = 13.9$^m$, P = 0.514195 d |
| GY Sge | | | GY | | | 19$^h$ 35$^m$ 13.63$^s$ | +19° 12′ 08.6″ | 9.84 | | | | Cepheid variable, V$_{max}$ = 9.84$^m$, V$_{min}$ = 10.60$^m$, P = 51.0625 d |
| HAT-P-34 | | | | | | 20$^h$ 12$^m$ 47$^s$ | +17° 37′ 41.2″ | 10.16 | | 838 | F8 | Sansuna; has a transiting planet (b) |
| SV Sge | | | SV | | 93987 | 19$^h$ 08$^m$ 11.77$^s$ | +16° 43′ 35.1″ | 10.3 | | | Rv... | R Coronae Borealis variable, V$_{max}$ = 10.3$^m$, V$_{min}$ = 16.5$^m$, P = 56.64 d |
| HD 187282 | | | QT | 187282 | 97456 | 19$^h$ 48$^m$ 32.20$^s$ | +18° 12′ 03.7″ | 10.51 | | | WN4 | Wolf–Rayet star, ΔV = 0.04$^m$ |
| QW Sge | | | QW | | | 19$^h$ 45$^m$ 49.54$^s$ | +18° 36′ 47.8″ | 11.0 | | | M6 | Z Andromedae variable, V$_{max}$ = 11.0$^m$, V$_{min}$ = 12.8$^m$, P = 517 d |
| HM Sge | | | HM | | | 19$^h$ 41$^m$ 57.09$^s$ | +16° 44′ 39.9″ | 11.10 | | | M7 | Nova and Mira variable |
| WR 124 | | | QR | | 94289 | 19$^h$ 11$^m$ 30.88$^s$ | +16° 51′ 38.2″ | 11.12 | | | WN8 | Merrill's Star; Wolf–Rayet star, V$_{max}$ = 11.04$^m$, V$_{min}$ = 11.12$^m$ |
| RZ Sge | | | RZ | | | 20$^h$ 03$^m$ 18.47$^s$ | +17° 02′ 51.9″ | 12.3 | | | | SU Ursae Majoris variable, V$_{max}$ = 12.3$^m$, V$_{min}$ = 17.7$^m$, P = 0.0682803 d |
| QY Sge | | | QY | | | 20$^h$ 07$^m$ 54.62$^s$ | +18° 42′ 54.5″ | 12.37 | | | G0e... | semiregular variable, V$_{max}$ = 12.37$^m$, V$_{min}$ = 12.57$^m$ |
| UU Sge | | | UU | | | 19$^h$ 42$^m$ 10.30$^s$ | +17° 05′ 14.4″ | 14.67 | | | sdO+G | Algol variable in planetary nebula, V$_{max}$ = 14.18$^m$, V$_{min}$ = 15.59$^m$, P = 0.46506918 d |
| WZ Sge | | | WZ | | | 20$^h$ 07$^m$ 36.50$^s$ | +17° 42′ 14.8″ | 15.20 | | | DAepv | prototype WZ Sagittae variable |
| Black Widow Pulsar | | | QX | | | 19$^h$ 59$^m$ 36.77$^s$ | +20° 48′ 15.1″ | 20.4 | | | | eclipsing binary/millisecond pulsar, V$_{max}$ = 20.4$^m$, V$_{min}$ = 23.0$^m$, P = 0.381967 d |
| WY Sge | | | WY | | | 19$^h$ 32$^m$ 43.82$^s$ | +17° 44′ 55.9″ | | | | | nova; dwarf nova; Algol variable |
| PSR B1944+17 | | | | | | 19$^h$ 46$^m$ 53.04$^s$ | +18° 05′ 41.2″ | | | | | pulsar |
| 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.] |||||||||||||