# List of stars in Sculptor

This is the list of notable stars in the constellation Sculptor, sorted by decreasing brightness.
| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Scl | α | | 5737 | 4577 | 00$^h$ 58$^m$ 36.35$^s$ | −29° 21′ 26.9″ | 4.30 | −2.27 | 672 | B7IIIp | SX Ari variable |
| β Scl | β | | 221507 | 116231 | 23$^h$ 32$^m$ 58.19$^s$ | −37° 49′ 06.1″ | 4.38 | 0.69 | 178 | B9.5IVMNpe. | suspected α$^2$ CVn variable, V$_{max}$ = 4.35$^m$, V$_{min}$ = 4.39$^m$ |
| γ Scl | γ | | 219784 | 115102 | 23$^h$ 18$^m$ 49.43$^s$ | −32° 31′ 54.6″ | 4.41 | 0.72 | 179 | K1III | variable star, ΔV = 0.004$^m$, P = 0.10 d |
| δ Scl | δ | | 223352 | 117452 | 23$^h$ 48$^m$ 55.48$^s$ | −28° 07′ 48.1″ | 4.59 | 1.37 | 143 | A0V | |
| η Scl | η | | 2429 | 2210 | 00$^h$ 27$^m$ 55.71$^s$ | −33° 00′ 25.4″ | 4.86 | −1.27 | 548 | M2/M3III | semiregular variable, V$_{max}$ = 4.8$^m$, V$_{min}$ = 4.9$^m$ |
| ζ Scl | ζ | | 224990 | 183 | 00$^h$ 02$^m$ 19.91$^s$ | −29° 43′ 13.6″ | 5.04 | −0.93 | 509 | B4V | |
| ι Scl | ι | | 1737 | 1708 | 00$^h$ 21$^m$ 31.18$^s$ | −28° 58′ 52.7″ | 5.18 | 0.29 | 310 | K0III | |
| θ Scl | θ | | 739 | 950 | 00$^h$ 11$^m$ 43.89$^s$ | −35° 08′ 00.2″ | 5.24 | 3.55 | 71 | F3/F5V | |
| π Scl | π | | 10537 | 7955 | 01$^h$ 42$^m$ 08.65$^s$ | −32° 19′ 36.7″ | 5.25 | 1.13 | 217 | K1II/III | |
| ε Scl | ε | | 10830 | 8209 | 01$^h$ 45$^m$ 38.65$^s$ | −25° 03′ 08.8″ | 5.29 | 3.10 | 89 | F2IV | suspected variable |
| μ Scl | μ | | 222433 | 116820 | 23$^h$ 40$^m$ 38.21$^s$ | −32° 04′ 22.8″ | 5.30 | 0.55 | 291 | K0III | suspected variable, V$_{max}$ = 5.30$^m$, V$_{min}$ = 5.33$^m$ |
| κ$^2$ Scl | κ$^2$ | | 720 | 930 | 00$^h$ 11$^m$ 34.42$^s$ | −27° 47′ 59.2″ | 5.41 | −0.85 | 581 | K2III | |
| κ$^1$ Scl | κ$^1$ | | 493 | 761 | 00$^h$ 09$^m$ 21.02$^s$ | −27° 59′ 16.5″ | 5.42 | 1.24 | 224 | F3V | |
| HD 9525 | | | 9525 | 7213 | 01$^h$ 32$^m$ 56.05$^s$ | −36° 51′ 54.7″ | 5.49 | 0.94 | 265 | K1/K2III | |
| σ Scl | σ | | 6178 | 4852 | 01$^h$ 02$^m$ 26.38$^s$ | −31° 33′ 07.4″ | 5.50 | 1.29 | 227 | A1/A2IV | α$^2$ CVn variable |
| HD 3059 | | | 3059 | 2661 | 00$^h$ 33$^m$ 41.06$^s$ | −29° 33′ 29.5″ | 5.55 | −0.37 | 497 | K1III | |
| ξ Scl | ξ | | 6055 | 4770 | 01$^h$ 01$^m$ 18.23$^s$ | −38° 54′ 59.9″ | 5.59 | −0.83 | 628 | K1III | |
| BU Scl | | BU | 224630 | 118277 | 23$^h$ 59$^m$ 27.90$^s$ | −29° 29′ 06.6″ | 5.59 | −1.56 | 879 | K5III | slow irregular variable |
| HD 218434 | | | 218434 | 114254 | 23$^h$ 08$^m$ 21.10$^s$ | −28° 49′ 24.8″ | 5.60 | 0.89 | 285 | G8III | |
| HD 220096 | | | 220096 | 115312 | 23$^h$ 21$^m$ 15.51$^s$ | −26° 59′ 12.3″ | 5.65 | 0.63 | 329 | G5IV | suspected variable |
| HD 1187 | | | 1187 | 1288 | 00$^h$ 16$^m$ 08.79$^s$ | −31° 26′ 46.8″ | 5.66 | 0.08 | 427 | K2III | |
| HD 344 | | | 344 | 655 | 00$^h$ 08$^m$ 03.52$^s$ | −33° 31′ 45.6″ | 5.67 | 0.67 | 325 | K1III | |
| τ Scl | τ | | 9906 | 7463 | 01$^h$ 36$^m$ 08.43$^s$ | −29° 54′ 26.8″ | 5.69 | 1.73 | 202 | F2V | |
| HD 10538 | | | 10538 | 7941 | 01$^h$ 42$^m$ 03.02$^s$ | −36° 49′ 56.2″ | 5.70 | 0.85 | 304 | A0V | |
| R Scl | | R | 8879 | 6759 | 01$^h$ 26$^m$ 58.10$^s$ | −32° 32′ 35.2″ | 5.72 | | 1545 | C | semiregular variable |
| HD 9377 | | | 9377 | 7118 | 01$^h$ 31$^m$ 43.25$^s$ | −30° 16′ 58.5″ | 5.79 | 0.95 | 304 | K0III | |
| HD 8498 | | | 8498 | 6502 | 01$^h$ 23$^m$ 30.97$^s$ | −30° 56′ 43.8″ | 5.84 | −1.34 | 888 | M0III | variable star, ΔV = 0.009$^m$, P = 10.62 d |
| HD 218619 | | | 218619 | 114366 | 23$^h$ 09$^m$ 44.62$^s$ | −28° 05′ 18.9″ | 5.88 | −0.73 | 685 | K2III | |
| λ$^2$ Scl | λ$^2$ | | 4211 | 3456 | 00$^h$ 44$^m$ 11.92$^s$ | −38° 25′ 19.1″ | 5.90 | 0.61 | 372 | K1III | |
| HD 9228 | | | 9228 | 7016 | 01$^h$ 30$^m$ 22.88$^s$ | −26° 12′ 28.3″ | 5.92 | 0.25 | 444 | K2III | |
| HD 942 | | | 942 | 1096 | 00$^h$ 13$^m$ 42.22$^s$ | −26° 01′ 19.8″ | 5.94 | −1.52 | 1012 | K5III | suspected variable, V$_{max}$ = 5.93$^m$, V$_{min}$ = 5.96$^m$ |
| HD 10142 | | | 10142 | 7643 | 01$^h$ 38$^m$ 27.49$^s$ | −36° 31′ 40.6″ | 5.94 | 0.96 | 323 | K0III | |
| AI Scl | | AI | 7312 | 5661 | 01$^h$ 12$^m$ 45.37$^s$ | −37° 51′ 23.1″ | 5.95 | 1.62 | 239 | A9IV: (+F/G) | δ Sct variable, V$_{max}$ = 5.89$^m$, V$_{min}$ = 5.98$^m$ |
| HD 2363 | | | 2363 | 2159 | 00$^h$ 27$^m$ 14.69$^s$ | −25° 32′ 49.7″ | 5.99 | −0.58 | 671 | K0III | |
| λ$^1$ Scl | λ$^1$ | | 4065 | 3356 | 00$^h$ 42$^m$ 42.89$^s$ | −38° 27′ 48.5″ | 6.05 | 0.44 | 432 | B9.5V | |
| AL Scl | | AL | 224113 | 117931 | 23$^h$ 55$^m$ 16.57$^s$ | −31° 55′ 17.3″ | 6.09 | −1.41 | 1032 | B6/B7 | Algol variable, V$_{max}$ = 6.06$^m$, V$_{min}$ = 6.33$^m$, P = 2.45 d |
| HD 5445 | | | 5445 | 4363 | 00$^h$ 55$^m$ 55.53$^s$ | −27° 46′ 33.0″ | 6.11 | −2.67 | 1863 | M1/M2III | variable star, ΔV = 0.014$^m$, P = 1.08 d |
| HD 9742 | | | 9742 | 7361 | 01$^h$ 34$^m$ 50.83$^s$ | −31° 53′ 32.0″ | 6.11 | 0.85 | 368 | K0/K1III | suspected variable |
| HD 943 | | | 943 | 1099 | 00$^h$ 13$^m$ 44.38$^s$ | −26° 17′ 05.9″ | 6.14 | −0.73 | 771 | K4III | |
| HD 1089 | | | 1089 | 1195 | 00$^h$ 14$^m$ 58.21$^s$ | −34° 54′ 15.1″ | 6.17 | −0.61 | 739 | K3III | |
| HD 10481 | | | 10481 | 7886 | 01$^h$ 41$^m$ 27.28$^s$ | −38° 07′ 58.7″ | 6.20 | 3.09 | 137 | F3/F5IV/V | |
| S Scl | | S | 1115 | 1236 | 00$^h$ 15$^m$ 22.27$^s$ | −32° 02′ 43.0″ | 6.20 | | 1100 | M7/M8IIIe | Mira variable, V$_{max}$ = 5.5$^m$, V$_{min}$ = 13.6$^m$, P = 367 d |
| HD 222872 | | | 222872 | 117107 | 23$^h$ 44$^m$ 29.10$^s$ | −26° 14′ 47.7″ | 6.23 | 2.07 | 222 | F3/F5V | |
| HD 219580 | | | 219580 | 114969 | 23$^h$ 17$^m$ 08.73$^s$ | −28° 26′ 16.9″ | 6.24 | −0.99 | 911 | M1/M2III | suspected variable |
| HD 224350 | | | 224350 | 118076 | 23$^h$ 57$^m$ 08.12$^s$ | −26° 37′ 24.6″ | 6.26 | −1.62 | 1226 | K3III | suspected variable |
| HD 6269 | | | 6269 | 4932 | 01$^h$ 03$^m$ 17.76$^s$ | −29° 31′ 32.8″ | 6.28 | 1.03 | 365 | G8IIICN... | |
| HD 220929 | | | 220929 | 115833 | 23$^h$ 28$^m$ 00.69$^s$ | −35° 32′ 40.2″ | 6.34 | −0.14 | 644 | K2III | |
| HD 223991 | | | 223991 | 117860 | 23$^h$ 54$^m$ 21.39$^s$ | −27° 02′ 34.5″ | 6.34 | 1.51 | 301 | A2V+... | |
| HD 219912 | | | 219912 | 115178 | 23$^h$ 19$^m$ 43.12$^s$ | −33° 42′ 28.7″ | 6.35 | 0.13 | 572 | K2III | |
| HD 9151 | | | 9151 | 6971 | 01$^h$ 29$^m$ 42.79$^s$ | −25° 37′ 04.0″ | 6.37 | 0.09 | 588 | K1III | |
| HD 225200 | | | 225200 | 345 | 00$^h$ 04$^m$ 20.30$^s$ | −29° 16′ 07.8″ | 6.38 | 0.83 | 421 | A1V | |
| HD 3074 | | | 3074 | 2663 | 00$^h$ 33$^m$ 43.85$^s$ | −35° 00′ 03.0″ | 6.41 | 3.62 | 118 | F8/G0V | |
| HD 3605 | | | 3605 | 3056 | 00$^h$ 38$^m$ 48.75$^s$ | −25° 06′ 28.0″ | 6.43 | −0.32 | 729 | K4III | |
| HD 6403 | | | 6403 | 5042 | 01$^h$ 04$^m$ 32.61$^s$ | −33° 31′ 58.0″ | 6.44 | 0.44 | 517 | K0III | |
| HD 223466 | | | 223466 | 117510 | 23$^h$ 49$^m$ 49.61$^s$ | −25° 19′ 52.6″ | 6.44 | 1.02 | 396 | A3V | |
| HD 219823 | | | 219823 | 115121 | 23$^h$ 19$^m$ 03.28$^s$ | −28° 23′ 16.3″ | 6.49 | −0.31 | 748 | K5III | |
| AV Scl | | AV | 1909 | 1830 | 00$^h$ 23$^m$ 12.61$^s$ | −31° 02′ 08.8″ | 6.56 | | 563 | B9IVmn | α$^2$ CVn variable |
| HD 6619 | | AW | 6619 | 5193 | 01$^h$ 06$^m$ 26.58$^s$ | −35° 39′ 38.4″ | 6.61 | | 494 | A1V | α$^2$ CVn variable |
| Z Scl | | Z | 3735 | 3142 | 00$^h$ 39$^m$ 57.82$^s$ | −33° 57′ 41.2″ | 6.69 | | 130.9 | F8V | suspected variable |
| HD 9770 | | BB | 9770 | 7372 | 01$^h$ 35$^m$ 01.04$^s$ | −29° 54′ 37.0″ | 7.10 | | 70.50 | K1V+M2V | eclipsing binary, V$_{max}$ = 7.1$^m$, V$_{min}$ = 7.17$^m$, P = 0.48 d |
| HD 4208 | | | 4208 | 3479 | 00$^h$ 44$^m$ 26.65$^s$ | −26° 30′ 56.4″ | 7.79 | 5.22 | 107 | G7V | Cocibolca, has a planet (b) |
| HD 4113 | | | 4113 | 3391 | 00$^h$ 49$^m$ 12.60$^s$ | −37° 58′ 57.5″ | 7.91 | 4.69 | 144 | G5V | has a planet (b) |
| HD 9578 | | | 9578 | 7240 | 01$^h$ 33$^m$ 17.14$^s$ | −38° 14′ 42.1″ | 8.20 | 4.41 | 187 | G1V | has a planet (b) |
| HD 6532 | | AP | 6532 | 5150 | 01$^h$ 05$^m$ 55.70$^s$ | −26° 43′ 44.0″ | 8.40 | | 531 | A5p | rapidly oscillating Ap star |
| Gliese 1 | | | 225213 | 439 | 00$^h$ 05$^m$ 24.43$^s$ | −37° 21′ 26.5″ | 8.63 | | 14.148 | M1.5 | suspected BY Dra variable, ΔV = 0.02$^m$ |
| HD 1097 | | AU | 1097 | 1210 | 00$^h$ 15$^m$ 07.97$^s$ | −29° 00′ 23.0″ | 9.05 | | 1150 | A4mF4Sr | δ Sct variable |
| WASP-8 | | | | | 23$^h$ 59$^m$ 36.07$^s$ | −35° 01′ 52.9″ | 9.89 | 6.45 | 159 | G6 | has a transiting planet (b) |
| RT Scl | | RT | | | 00$^h$ 36$^m$ 28.09$^s$ | −25° 40′ 22.9″ | 10.31 | | | A5N+F3 | β Lyr variable, V$_{max}$ = 10.18$^m$, V$_{min}$ = 10.89$^m$, P = 0.51 d |
| WASP-173 A | | | | | 23$^h$ 36$^m$ 40.0$^s$ | −34° 36′ 41″ | 11.3 | | | G3 | has a transiting planet (b) |
| CD -38 245 | | | | 3635 | 00$^h$ 46$^m$ 36.19$^s$ | −37° 39′ 33.6″ | 12.00 | | | K1Ivw | very metal-poor star |
| WASP-45 | | | | | 00$^h$ 20$^m$ 57.00$^s$ | −35° 59′ 53.8″ | 12.00 | | | K2V | has a transiting planet (b) |
| SY Scl | | SY | | | 00$^h$ 07$^m$ 36.25$^s$ | −25° 29′ 39.9″ | 12.15 | | | M8: | Mira variable, V$_{max}$ = 10.4$^m$, V$_{min}$ = <14.6$^m$, P = 411 d |
| VY Scl | | VY | | | 23$^h$ 29$^m$ 00.48$^s$ | −29° 46′ 45.9″ | | | | O... | prototype VY Scl star |
| GD 659 | | | | | 00$^h$ 53$^m$ 17.44$^s$ | −32° 59′ 56.6″ | 13.36 | | | DA1.4 | white dwarf |
| BX Scl | | BX | | | 23$^h$ 43$^m$ 54.45$^s$ | −28° 18′ 34.5″ | 13.56 | | | A | SX Phe variable, V$_{max}$ = 13.42$^m$, V$_{min}$ = 13.71$^m$, P = 0.037 d |
| WD 0137-349 | | | | | 01$^h$ 39$^m$ 42.85$^s$ | −34° 42′ 39.3″ | 15.33 | | | DA | white dwarf, has a brown dwarf companion |
| VZ Scl | | VZ | | | 23$^h$ 50$^m$ 09.25$^s$ | −26° 22′ 52.7″ | 15.6 | | | B9IVmn | VY Scl variable and eclipsing binary, V$_{max}$ = 15.6$^m$, V$_{min}$ = 18.4$^m$, P = 0.14 d |
| BW Scl | | BW | | | 23$^h$ 53$^m$ 00.86$^s$ | −38° 51′ 46.6″ | 16.20 | | | CV | WZ Sge variable and ZZ Cet variable, V$_{max}$ = 8.9$^m$, V$_{min}$ = 17.2$^m$, P = 0.054 d |
| 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.] ||||||||||||