# List of stars in Piscis Austrinus

This is the list of notable stars in the constellation Piscis Austrinus, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| Fomalhaut | α | 24 | | 216956 | 113368 | 22$^h$ 57$^m$ 38.83$^s$ | −29° 37′ 18.6″ | 1.17 | 1.74 | 25 | A3V | Fom Alhout Algenubi, Os Piscis Meridiani, Os Piscis Meridionalis, Os Piscis Notii, Difda al Auwel; 18th brightest star; has a circumstellar disk; suspected variable |
| ε PsA | ε | 18 | | 214748 | 111954 | 22$^h$ 40$^m$ 39.33$^s$ | −27° 02′ 37.0″ | 4.18 | −2.61 | 744 | B8V | suspected variable, V$_{max}$ = 4.12$^m$, V$_{min}$ = 4.24$^m$ |
| δ PsA | δ | 23 | | 216763 | 113246 | 22$^h$ 55$^m$ 56.89$^s$ | −32° 32′ 22.9″ | 4.20 | 0.61 | 170 | G8III | Tiāngāng (天綱) |
| β PsA | β | 17 | | 213398 | 111188 | 22$^h$ 31$^m$ 30.29$^s$ | −32° 20′ 45.7″ | 4.29 | 1.00 | 148 | A1V | |
| ι PsA | ι | 9 | | 206742 | 107380 | 21$^h$ 44$^m$ 56.79$^s$ | −33° 01′ 32.0″ | 4.35 | 0.36 | 205 | B9.5V | |
| γ PsA | γ | 22 | | 216336 | 112948 | 22$^h$ 52$^m$ 31.56$^s$ | −32° 52′ 31.6″ | 4.46 | 0.29 | 222 | A0III | suspected variable, V$_{max}$ = 4.45$^m$, V$_{min}$ = 4.50$^m$ |
| μ PsA | μ | 14 | | 210049 | 109285 | 22$^h$ 08$^m$ 22.95$^s$ | −32° 59′ 18.2″ | 4.50 | 1.49 | 130 | A2V | suspected variable |
| τ PsA | τ | 15 | | 210302 | 109422 | 22$^h$ 10$^m$ 08.48$^s$ | −32° 32′ 54.4″ | 4.94 | 3.58 | 61 | F6V | |
| υ PsA | υ | | | 210066 | 109289 | 22$^h$ 08$^m$ 25.93$^s$ | −34° 02′ 37.4″ | 4.99 | −1.06 | 528 | K4III | |
| θ PsA | θ | 10 | | 207155 | 107608 | 21$^h$ 47$^m$ 44.17$^s$ | −30° 53′ 53.9″ | 5.02 | −0.06 | 339 | A1V | |
| π PsA | π | | | 217792 | 113860 | 23$^h$ 03$^m$ 29.76$^s$ | −34° 44′ 58.6″ | 5.12 | 2.84 | 93 | A9V | γ Dor variable, V$_{max}$ = 5.10$^m$, V$_{min}$ = 5.12$^m$, P = 1.06039 d |
| HD 210271 | | | | 210271 | 109404 | 22$^h$ 09$^m$ 55.71$^s$ | −34° 00′ 54.1″ | 5.37 | 1.30 | 212 | A5IV | |
| η PsA | η | 12 | | 209014 | 108661 | 22$^h$ 00$^m$ 50.22$^s$ | −28° 27′ 13.5″ | 5.43 | −2.03 | 1012 | B8/B9V+... | suspected variable, V$_{max}$ = 5.33$^m$, V$_{min}$ = 5.44$^m$ |
| λ PsA | λ | 16 | | 210934 | 109789 | 22$^h$ 14$^m$ 18.74$^s$ | −27° 46′ 00.9″ | 5.45 | −0.51 | 508 | B7V | |
| WX PsA | | | WX | 217236 | 113532 | 22$^h$ 59$^m$ 35.76$^s$ | −29° 27′ 44.4″ | 5.51 | 0.26 | 366 | F0V | δ Sct variable |
| HD 217484 | | | | 217484 | 113669 | 23$^h$ 01$^m$ 19.35$^s$ | −28° 51′ 14.1″ | 5.55 | −0.72 | 584 | K3III | |
| HD 210848 | | | | 210848 | 109737 | 22$^h$ 13$^m$ 44.39$^s$ | −25° 10′ 51.3″ | 5.58 | 1.43 | 221 | F7II | |
| VZ PsA | | | VZ | 214484 | 111809 | 22$^h$ 38$^m$ 51.46$^s$ | −33° 04′ 53.0″ | 5.66 | 0.04 | 435 | A0V | Algol variable, V$_{max}$ = 5.66$^m$, V$_{min}$ = 5.83$^m$, P = 5.76333 d |
| HD 217303 | | | | 217303 | 113562 | 23$^h$ 00$^m$ 05.77$^s$ | −25° 09′ 50.4″ | 5.66 | −1.02 | 706 | K0IICNIII | |
| 8 PsA | | 8 | | 205471 | 106654 | 21$^h$ 36$^m$ 10.90$^s$ | −26° 10′ 17.2″ | 5.73 | 2.07 | 176 | A7/A8IV | |
| HD 214122 | | | | 214122 | 111600 | 22$^h$ 36$^m$ 35.47$^s$ | −31° 39′ 49.3″ | 5.82 | 0.92 | 312 | K2III | |
| HD 214690 | | | | 214690 | 111934 | 22$^h$ 40$^m$ 22.38$^s$ | −30° 39′ 30.1″ | 5.88 | −0.59 | 642 | K2/K3III | suspected variable, V$_{max}$ = 5.86$^m$, V$_{min}$ = 5.89$^m$ |
| HD 213135 | | | | 213135 | 111045 | 22$^h$ 29$^m$ 45.94$^s$ | −27° 06′ 26.0″ | 5.95 | 2.83 | 137 | F0V | suspected variable, V$_{max}$ = 5.94$^m$, V$_{min}$ = 5.99$^m$ |
| 6 PsA | | 6 | | 204854 | 106340 | 21$^h$ 32$^m$ 14.58$^s$ | −33° 56′ 40.6″ | 5.97 | 0.46 | 412 | A2V | |
| UU PsA | | | UU | 209522 | 108975 | 22$^h$ 04$^m$ 36.76$^s$ | −26° 49′ 20.4″ | 5.97 | −1.73 | 1128 | B3V (+B) | Be star |
| 21 PsA | | 21 | | 216210 | 112862 | 22$^h$ 51$^m$ 20.94$^s$ | −29° 32′ 10.6″ | 5.99 | 0.71 | 370 | G8/K0III | |
| HD 216761 | | | | 216761 | 113234 | 22$^h$ 55$^m$ 51.54$^s$ | −31° 37′ 59.5″ | 6.09 | −1.23 | 948 | K3III | |
| 7 PsA | | 7 | | 205529 | 106703 | 21$^h$ 36$^m$ 48.75$^s$ | −33° 02′ 52.4″ | 6.10 | 1.79 | 237 | A5V | |
| 19 PsA | | 19 | | 214966 | 112102 | 22$^h$ 42$^m$ 22.08$^s$ | −29° 21′ 39.6″ | 6.12 | −0.23 | 607 | M3III | semiregular variable |
| HD 211291 | | | | 211291 | 109990 | 22$^h$ 16$^m$ 37.44$^s$ | −25° 53′ 53.3″ | 6.14 | −0.07 | 568 | K1II/III | |
| HD 217096 | | | | 217096 | 113447 | 22$^h$ 58$^m$ 35.01$^s$ | −35° 31′ 22.6″ | 6.15 | 1.70 | 253 | F7V | |
| HD 210739 | | | | 210739 | 109667 | 22$^h$ 12$^m$ 57.50$^s$ | −26° 19′ 39.8″ | 6.19 | 2.37 | 189 | A3V | |
| HD 205872 | | | | 205872 | 106907 | 21$^h$ 39$^m$ 06.07$^s$ | −33° 40′ 43.5″ | 6.28 | 3.01 | 147 | G8IV | |
| HD 215669 | | | | 215669 | 112501 | 22$^h$ 47$^m$ 19.21$^s$ | −34° 09′ 42.4″ | 6.28 | 1.32 | 320 | K1III | |
| HD 214599 | | | | 214599 | 111879 | 22$^h$ 39$^m$ 44.12$^s$ | −28° 19′ 32.0″ | 6.30 | 0.53 | 466 | K0/K1III | |
| HD 217358 | | | | 217358 | 113593 | 23$^h$ 00$^m$ 24.58$^s$ | −25° 37′ 36.3″ | 6.30 | 0.71 | 428 | K1III | |
| HD 215782 | | | | 215782 | 112567 | 22$^h$ 47$^m$ 56.13$^s$ | −25° 54′ 42.3″ | 6.31 | 0.31 | 517 | G8III | |
| HD 216042 | | | | 216042 | 112746 | 22$^h$ 49$^m$ 59.25$^s$ | −32° 48′ 19.4″ | 6.34 | 2.12 | 228 | F0V | |
| HD 210111 | | | | 210111 | 109306 | 22$^h$ 08$^m$ 42.63$^s$ | −33° 07′ 32.7″ | 6.37 | 1.89 | 257 | A2III/IV | δ Sct variable, ΔV = 0.04$^m$ |
| HD 208285 | | | | 208285 | 108259 | 21$^h$ 55$^m$ 55.60$^s$ | −30° 36′ 21.1″ | 6.41 | 0.90 | 412 | G8III | |
| HD 205265 | | | | 205265 | 106564 | 21$^h$ 34$^m$ 52.99$^s$ | −29° 41′ 45.9″ | 6.42 | −0.22 | 695 | B8IIIw | suspected variable |
| ζ PsA | ζ | | | 213296 | 111138 | 22$^h$ 30$^m$ 53.75$^s$ | −26° 04′ 24.8″ | 6.43 | 0.99 | 399 | K1III | |
| HD 210300 | | | | 210300 | 109412 | 22$^h$ 10$^m$ 00.13$^s$ | −28° 17′ 33.0″ | 6.44 | 1.27 | 353 | A5V | |
| 13 PsA | | 13 | | 209476 | 108952 | 22$^h$ 04$^m$ 23.83$^s$ | −29° 54′ 59.5″ | 6.45 | −1.55 | 1299 | K5III | |
| HD 214462 | | | | 214462 | 111801 | 22$^h$ 38$^m$ 44.70$^s$ | −28° 44′ 53.5″ | 6.46 | 1.00 | 403 | K1III | |
| TW PsA | | | TW | 216803 | 113283 | 22$^h$ 56$^m$ 23.83$^s$ | −31° 33′ 54.6″ | 6.48 | 7.07 | 25 | K4Vp | Fomalhaut B; BY Dra variable, V$_{max}$ = 6.44$^m$, V$_{min}$ = 6.51$^m$, P = 10.3 d |
| 5 PsA | | 5 | | 204394 | 106067 | 21$^h$ 29$^m$ 03.73$^s$ | −31° 14′ 18.7″ | 6.52 | 1.21 | 377 | A1V | |
| 20 PsA | | 20 | | 215452 | 112362 | 22$^h$ 45$^m$ 31.3$^s$ | −25° 14′ 22.5″ | 6.56 | | 284 | A0IV | |
| 11 PsA | | 11 | | 208851 | 108571 | 21$^h$ 59$^m$ 33.4$^s$ | −27° 37′ 58.6″ | 7.31 | | 247 | F2V | |
| Lacaille 9352 | | | | 217987 | 114046 | 23$^h$ 05$^m$ 52.04$^s$ | −35° 51′ 11.1″ | 7.34 | 9.75 | 11 | M0.5V | one of the nearest known star systems |
| HD 216770 | | | | 216770 | 113238 | 22$^h$ 55$^m$ 53.70$^s$ | −26° 39′ 31.6″ | 8.10 | 5.21 | 124 | K1V | has a planet (b) |
| HD 205739 | | | | 205739 | 106824 | 21$^h$ 38$^m$ 08.41$^s$ | −31° 44′ 14.9″ | 8.56 | 3.78 | 295 | G3IV | Sāmaya; has a planet (b) |
| HD 207832 | | | | 207832 | 107985 | 21$^h$ 52$^m$ 36.0$^s$ | −26° 01′ 36″ | 8.79 | | 177 | G5V | has two planets (b and c ) |
| RW PsA | | | RW | | | 22$^h$ 09$^m$ 46.92$^s$ | −27° 04′ 01.7″ | 11.16 | | | | W UMa variable, V$_{max}$ = 11.05$^m$, V$_{min}$ = 11.76$^m$, P = 0.36045101 d |
| WASP-124 | | | | | | 22$^h$ 10$^m$ 51.0$^s$ | −30° 44′ 58″ | 12.7 | | 1412 | F9 | has a transiting planet (b) |
| WASP-112 | | | | | | 22$^h$ 37$^m$ 57.0$^s$ | −35° 09′ 14″ | 13.3 | | 1468 | G6 | has a transiting planet (b) |
| TY PsA | | | TY | | | 22$^h$ 49$^m$ 39.90$^s$ | −27° 06′ 53.2″ | | | | DA | SU UMa variable |
| 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.] |||||||||||||