# List of stars in Scutum

This is the list of notable stars in the constellation Scutum, sorted by decreasing brightness.
| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Sct | α | | 171443 | 91117 | 18$^h$ 35$^m$ 12.44$^s$ | −08° 14′ 35.9″ | 3.85 | 0.21 | 174 | K2III | suspected variable, V$_{max}$ = 3.81$^m$, V$_{min}$ = 3.87$^m$ |
| β Sct | β | | 173764 | 92175 | 18$^h$ 47$^m$ 10.48$^s$ | −04° 44′ 52.2″ | 4.22 | −2.41 | 689 | G5II... | |
| ζ Sct | ζ | | 169156 | 90135 | 18$^h$ 23$^m$ 39.55$^s$ | −08° 56′ 04.2″ | 4.66 | 0.82 | 191 | K0III | |
| γ Sct | γ | | 170296 | 90595 | 18$^h$ 29$^m$ 11.85$^s$ | −14° 33′ 56.9″ | 4.67 | −0.09 | 291 | A1IV/V | |
| δ Sct | δ | | 172748 | 91726 | 18$^h$ 42$^m$ 16.42$^s$ | −09° 03′ 09.2″ | 4.70 (4.60–4.79) | 0.91 | 187 | F2IIIp d Del | triple star; prototype Delta Scuti variable, V$_{max}$ = 4.6$^m$, V$_{min}$ = 4.79$^m$, P = 0.1937697 d |
| η Sct | η | | 175751 | 93026 | 18$^h$ 57$^m$ 03.63$^s$ | −05° 50′ 46.4″ | 4.83 | 0.82 | 207 | K1III | |
| ε Sct | ε | | 173009 | 91845 | 18$^h$ 43$^m$ 31.24$^s$ | −08° 16′ 30.9″ | 4.88 | −1.14 | 522 | G8II | |
| HD 175156 | | | 175156 | 92814 | 18$^h$ 54$^m$ 43.12$^s$ | −15° 36′ 10.9″ | 5.08 | −3.46 | 1663 | B3II | |
| HD 171391 | | | 171391 | 91105 | 18$^h$ 35$^m$ 02.36$^s$ | −10° 58′ 37.9″ | 5.12 | 0.38 | 290 | G8III | suspected variable |
| R Sct | | R | 173819 | 92202 | 18$^h$ 47$^m$ 28.98$^s$ | −05° 42′ 18.3″ | 5.38 (4.5–8.2) | −2.79 | 1405 | K0Ibpvar | RV Tauri variable, V$_{max}$ = 4.2$^m$, V$_{min}$ = 8.6$^m$, P = 146.5 d |
| V450 Sct | | V450 | 170975 | 90913 | 18$^h$ 32$^m$ 43.32$^s$ | −14° 51′ 56.4″ | 5.47 | −2.48 | 1268 | K3Iab | semiregular variable |
| HD 173638 | | | 173638 | 92136 | 18$^h$ 46$^m$ 43.32$^s$ | −10° 07′ 30.1″ | 5.69 | | | F2Ib-II | suspected irregular variable, V$_{max}$ = 5.64$^m$, V$_{min}$ = 5.81$^m$ |
| HD 169033 | | | 169033 | 90096 | 18$^h$ 23$^m$ 12.17$^s$ | −12° 00′ 52.9″ | 5.71 | −0.66 | 612 | B5V | |
| HD 171130 | | | 171130 | 90991 | 18$^h$ 33$^m$ 39.00$^s$ | −14° 51′ 12.9″ | 5.74 | 1.68 | 211 | A0/A1V | |
| HD 170740 | | | 170740 | 90804 | 18$^h$ 31$^m$ 25.69$^s$ | −10° 47′ 44.9″ | 5.77 | −0.87 | 694 | B2V | double star; suspected variable |
| HD 172348 | | | 172348 | 91532 | 18$^h$ 40$^m$ 00.40$^s$ | −07° 47′ 26.5″ | 5.82 | −0.22 | 527 | K4III | |
| HD 174464 | | | 174464 | 92488 | 18$^h$ 50$^m$ 58.51$^s$ | −09° 46′ 26.8″ | 5.82 | −2.51 | 1509 | F2Ib | |
| HD 174208 | | | 174208 | 92391 | 18$^h$ 49$^m$ 40.96$^s$ | −05° 54′ 46.2″ | 5.99 | −2.31 | 1489 | K2Ib | |
| V432 Sct | | V432 | 170397 | 90651 | 18$^h$ 29$^m$ 46.75$^s$ | −14° 34′ 55.3″ | 6.02 | 1.32 | 284 | Ap | α² CVn variable, ΔV = 0.012$^m$, P = 2.1912 d |
| HD 172831 | | | 172831 | 91751 | 18$^h$ 42$^m$ 36.12$^s$ | −07° 04′ 25.1″ | 6.13 | 1.77 | 243 | K0.5III | |
| HD 170547 | | | 170547 | 90692 | 18$^h$ 30$^m$ 14.30$^s$ | −05° 43′ 26.9″ | 6.27 | 0.02 | 579 | G8II-III | |
| HD 174866 | | | 174866 | 92674 | 18$^h$ 53$^m$ 01.80$^s$ | −09° 34′ 32.0″ | 6.27 | 1.23 | 332 | A7Vn | |
| HD 169370 | | | 169370 | 90238 | 18$^h$ 24$^m$ 42.05$^s$ | −07° 04′ 33.1″ | 6.28 | 1.61 | 281 | K0 | |
| HD 173093 | | | 173093 | 91880 | 18$^h$ 43$^m$ 51.22$^s$ | −06° 49′ 04.8″ | 6.30 | 2.09 | 227 | F7V | |
| HD 169009 | | | 169009 | 90083 | 18$^h$ 23$^m$ 02.10$^s$ | −10° 13′ 08.1″ | 6.32 | 1.21 | 343 | B9.5V | suspected variable |
| HD 170902 | | | 170902 | 90884 | 18$^h$ 32$^m$ 20.66$^s$ | −14° 38′ 39.2″ | 6.36 | 2.01 | 241 | A4/A5IV/V | |
| HD 171149 | | | 171149 | 90967 | 18$^h$ 33$^m$ 22.71$^s$ | −05° 54′ 41.9″ | 6.36 | 1.07 | 373 | A0Vn | |
| HD 172594 | | | 172594 | 91677 | 18$^h$ 41$^m$ 42.46$^s$ | −14° 33′ 51.3″ | 6.40 | −4.34 | 4592 | F2/F3Ib/II | |
| HD 174328 | | | 174328 | 92456 | 18$^h$ 50$^m$ 31.17$^s$ | −13° 34′ 20.1″ | 6.48 | −2.03 | 1638 | K1II/III | |
| HD 171957 | | | 171957 | 91369 | 18$^h$ 38$^m$ 04.48$^s$ | −14° 00′ 17.1″ | 6.49 | −0.15 | 694 | B8II/III | |
| HD 174005 | | | 174005 | 92296 | 18$^h$ 48$^m$ 39.49$^s$ | −06° 00′ 15.8″ | 6.49 | 0.45 | 527 | A2 | |
| HD 169913 | | | 169913 | 90437 | 18$^h$ 27$^m$ 08.86$^s$ | −08° 02′ 25.6″ | 6.50 | 1.51 | 325 | K0 | |
| HD 169454 | | V430 | 169454 | 90281 | 18$^h$ 25$^m$ 15.19$^s$ | −13° 58′ 42.3″ | 6.64 | | | B1Ia | α Cyg variable, V$_{max}$ = 6.5$^m$, V$_{min}$ = 6.64$^m$ |
| S Sct | | S | 174325 | 92442 | 18$^h$ 50$^m$ 20.04$^s$ | −07° 54′ 27.4″ | 6.80 | | 1260 | C | semiregular variable, V$_{max}$ = 6.6$^m$, V$_{min}$ = 7.3$^m$, P = 149.7 d |
| V496 Sct | | V496 | | | 18$^h$ 43$^m$ 45.57$^s$ | −07° 36′ 42.0″ | 7.10 | | | | nova, V$_{max}$ = 7.10$^m$, V$_{min}$ = <19$^m$ |
| RZ Sct | | RZ | 169753 | 90382 | 18$^h$ 26$^m$ 33.52$^s$ | −09° 12′ 06.0″ | 7.53 | | 2260 | B3Ib | Algol variable, V$_{max}$ = 7.34$^m$, V$_{min}$ = 8.84$^m$, P = 15.1902079 d |
| HD 173219 | | V447 | 173219 | 91946 | 18$^h$ 44$^m$ 33.34$^s$ | −07° 06′ 38.2″ | 7.88 | | | B1:V:npe | Be star, ΔV = 0.12$^m$ |
| SS Sct | | SS | 173058 | 91867 | 18$^h$ 43$^m$ 43.51$^s$ | −07° 43′ 51.9″ | 7.90 | | | F8 | Cepheid variable, V$_{max}$ = 7.9$^m$, V$_{min}$ = 8.43$^m$, P = 3.671253 d |
| EW Sct | | EW | 171955 | 91342 | 18$^h$ 37$^m$ 51.11$^s$ | −06° 47′ 48.5″ | 7.96 | | 1450 | G5 | double-mode Cepheid variable, V$_{max}$ = 7.6$^m$, V$_{min}$ = 8.2$^m$, P = 5.82363 d |
| V475 Sct | | V475 | | | 18$^h$ 49$^m$ 37.60$^s$ | −09° 33′ 15.9″ | | | | | nova, V$_{max}$ = 8.4$^m$, V$_{min}$ = <16$^m$ |
| RU Sct | | RU | 172730 | 91697 | 18$^h$ 41$^m$ 56.38$^s$ | −04° 06′ 38.4″ | 8.84 | | 801 | G5 | Cepheid variable, V$_{max}$ = 8.84$^m$, V$_{min}$ = 9.96$^m$, P = 19.7035 d |
| RY Sct | | RY | 169515 | 90303 | 18$^h$ 25$^m$ 31.48$^s$ | −12° 41′ 24.2″ | 9.12 | | | B1IIIpe | Beta Lyrae variable, V$_{max}$ = 9.12$^m$, V$_{min}$ = 9.72$^m$, P = 11.12471 d |
| HD 173637 | | V455 | 173637 | 92128 | 18$^h$ 46$^m$ 38.08$^s$ | −07° 55′ 55.1″ | 9.29 | | | B1IV | γ Cas variable |
| EV Sct | | EV | | 91239 | 18$^h$ 36$^m$ 39.60$^s$ | −08° 11′ 05.4″ | 9.90 | | | G0II | Cepheid variable, V$_{max}$ = 9.9$^m$, V$_{min}$ = 10.32$^m$, P = 3.09099 d |
| RS Sct | | RS | | 92340 | 18$^h$ 49$^m$ 11.25$^s$ | −10° 14′ 27.8″ | 9.95 | | 860 | G0 | Beta Lyrae variable, V$_{max}$ = 9.78$^m$, V$_{min}$ = 10.91$^m$, P = 0.6642384 d |
| AS 314 | | V452 | | 91477 | 18$^h$ 39$^m$ 26.11$^s$ | −13° 50′ 47.2″ | 10.01 | | 32600 | A3:Ia | α Cyg variable; candidate luminous blue variable |
| X Sct | | X | | 90791 | 18$^h$ 31$^m$ 19.75$^s$ | −13° 06′ 29.5″ | 10.07 | | 1330 | F5... | Cepheid variable, V$_{max}$ = 9.5$^m$, V$_{min}$ = 10.42$^m$, P = 4.19807 d |
| V443 Sct | | V443 | | | 18$^h$ 49$^m$ 38.95$^s$ | −06° 11′ 15.9″ | 10.48 | | | | nova, V$_{max}$ = 8.5$^m$, V$_{min}$ = <13.2$^m$ |
| UY Sct | | UY | | | 18$^h$ 27$^m$ 36.53$^s$ | −12° 27′ 58.9″ | 10.56 | | | M2-4Ia-Iab | One of the largest known stars; semiregular variable |
| UZ Sct | | UZ | | | 18$^h$ 31$^m$ 22.37$^s$ | −22° 55′ 43.34″ | | 10.91 | 176.35275 | G0 D | Yellow giant. |
| CM Sct | | CM | | 91738 | 18$^h$ 42$^m$ 26.82$^s$ | −05° 20′ 27.0″ | 10.93 | | | | Cepheid variable, V$_{max}$ = 10.79$^m$, V$_{min}$ = 11.49$^m$, P = 3.916997 d |
| TY Sct | | TY | | 91706 | 18$^h$ 42$^m$ 07.92$^s$ | −04° 17′ 36.5″ | 11.00 | | 733 | F8 | Cepheid variable, V$_{max}$ = 10.31$^m$, V$_{min}$ = 11.25$^m$, P = 11.05302 d |
| V476 Sct | | V476 | | | 18$^h$ 32$^m$ 04.75$^s$ | −06° 43′ 34.3″ | 11.10 | | | | nova, V$_{max}$ = 11.1$^m$, V$_{min}$ = <17$^m$ |
| LS 5039 | | V479 | | | 18$^h$ 26$^m$ 15.06$^s$ | −14° 50′ 54.3″ | 11.23 | | | O(f)N6.5V | High-mass X-ray binary; microquasar; gamma-ray emitter; V$_{max}$ = 11.22$^m$, V$_{min}$ = 11.35$^m$, P = 3.906 d |
| V367 Sct | | V367 | | | 18$^h$ 33$^m$ 35.24$^s$ | −10° 25′ 38.0″ | 11.58 | | | F5II | double-mode Cepheid variable, V$_{max}$ = 11.21$^m$, V$_{min}$ = 11.91$^m$, P = 6.29307 d |
| FR Sct | | FR | | 90115 | 18$^h$ 23$^m$ 22.79$^s$ | −12° 40′ 51.8″ | 11.60 | | | M1:II | slow irregular variable; Algol variable |
| MWC 300 | | V431 | | 90617 | 18$^h$ 29$^m$ 25.69$^s$ | −06° 04′ 37.3″ | 11.60 | | | Bpe | α$^2$ CVn variable, V$_{max}$ = 11.6$^m$, V$_{min}$ = 12.1$^m$, P = 2.1510141 d |
| BX Sct | | BX | | | 18$^h$ 50$^m$ 09.24$^s$ | −04° 22′ 05.2″ | 11.70 | | | F6 | Cepheid variable, V$_{max}$ = 11.7$^m$, V$_{min}$ = 12.62$^m$, P = 6.41133 d |
| CoRoT-17 | | | | | 18$^h$ 34$^m$ 47$^s$ | −06° 36′ 44″ | 15.46 | | 3001 | G2V | has a transiting planet (b) |
| 4U 1850-087 | | | | | 18$^h$ 53$^m$ 04.89$^s$ | −08° 42′ 19.7″ | 21.00 | | 22500 | | Low-mass X-ray binary |
| CRL 2136 | | | | | 18$^h$ 22$^m$ 26.59$^s$ | −13° 30′ 15.7″ | | | | | massive young star |
| OH 17.7-2.0 | | V445 | | | 18$^h$ 30$^m$ 30.62$^s$ | −14° 28′ 55.8″ | | | | K2/K3:II/III: | semiregular variable |
| OH 26.5+0.6 | | V437 | | | 18$^h$ 37$^m$ 32.51$^s$ | −05° 23′ 59.2″ | | | | M | Mira variable |
| PSR B1829-10 | | | | | 18$^h$ 32$^m$ 40.9$^s$ | −10° 21′ 34″ | | | | n/a | pulsar |
| PSR B1822-09 | | | | | 18$^h$ 25$^m$ 30.55$^s$ | −09° 35′ 22.1″ | | | | | pulsar |
| PSR B1823-13 | | | | | 18$^h$ 26$^m$ 13.18$^s$ | −13° 34′ 46.8″ | | | | | pulsar |
| PSR B1828-10 | | | | | 18$^h$ 30$^m$ 47.57$^s$ | −10° 59′ 27.9″ | | | | | pulsar; possible planetary companion |
| PSR J1833-1034 | | | | | 18$^h$ 33$^m$ 33.57$^s$ | −10° 34′ 07.5″ | | | | | pulsar |
| 1E 1841-045 | | | | | 18$^h$ 41$^m$ 19.34$^s$ | −04° 56′ 11.16″ | | | | | magnetar in supernova remnant |
| EU Sct | | EU | | | 18$^h$ 56$^m$ 13.12$^s$ | −04° 12′ 32.3″ | | | | | nova |
| V368 Sct | | V368 | | | 18$^h$ 45$^m$ 43.53$^s$ | −08° 33′ 00.9″ | | | | | nova |
| V373 Sct | | V373 | | | 18$^h$ 55$^m$ 26.71$^s$ | −07° 43′ 05.5″ | | | | | nova |
| 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.] ||||||||||||