# List of stars in Pyxis

This is the list of notable stars in the constellation Pyxis, sorted by decreasing brightness.
| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Pyx | α | | 74575 | 42828 | 08$^h$ 43$^m$ 35.55$^s$ | −33° 11′ 11.1″ | 3.68 | −3.39 | 845 | B1.5III | β Cep variable, V$_{max}$ = 3.67$^m$, V$_{min}$ = 3.70$^m$ |
| β Pyx | β | | 74006 | 42515 | 08$^h$ 40$^m$ 06.14$^s$ | −35° 18′ 29.9″ | 3.97 | −1.41 | 388 | G5II/III | |
| γ Pyx | γ | | 75691 | 43409 | 08$^h$ 50$^m$ 32.01$^s$ | −27° 42′ 36.2″ | 4.02 | −0.01 | 209 | K3III | |
| κ Pyx | κ | | 78541 | 44824 | 09$^h$ 08$^m$ 02.86$^s$ | −25° 51′ 30.7″ | 4.62 | −1.25 | 487 | K4/K5III | variable star, ΔV = 0.006$^m$, P = 8.50919 d |
| θ Pyx | θ | | 80874 | 45902 | 09$^h$ 21$^m$ 29.60$^s$ | −25° 57′ 55.5″ | 4.71 | −1.31 | 522 | M0III | semiregular variable |
| λ Pyx | λ | | 81169 | 46026 | 09$^h$ 23$^m$ 12.34$^s$ | −28° 50′ 02.1″ | 4.71 | 0.98 | 182 | G8III | |
| ζ Pyx | ζ | | 73898 | 42483 | 08$^h$ 39$^m$ 42.49$^s$ | −29° 33′ 39.1″ | 4.86 | 0.56 | 236 | G5III | |
| δ Pyx | δ | | 76483 | 43825 | 08$^h$ 55$^m$ 31.52$^s$ | −27° 40′ 53.9″ | 4.87 | 0.66 | 226 | A3IV | |
| HD 73752 | | | 73752 | 42430 | 08$^h$ 39$^m$ 08.07$^s$ | −22° 39′ 46.5″ | 5.05 | 3.55 | 65 | G3/G5V | |
| HD 75605 | | | 75605 | 43352 | 08$^h$ 49$^m$ 51.50$^s$ | −32° 46′ 49.5″ | 5.19 | 0.96 | 229 | G8III | |
| η Pyx | η | | 73495 | 42334 | 08$^h$ 37$^m$ 52.17$^s$ | −26° 15′ 17.9″ | 5.24 | 0.89 | 242 | A0V | suspected variable |
| HD 72310 | | | 72310 | 41817 | 08$^h$ 31$^m$ 30.94$^s$ | −19° 34′ 38.8″ | 5.42 | 0.08 | 381 | B9.5IV/V | |
| ε Pyx | ε | | 78922 | 45001 | 09$^h$ 09$^m$ 56.41$^s$ | −30° 21′ 55.0″ | 5.59 | 1.52 | 212 | A4IV | variable star, ΔV = 0.006$^m$, P = 6.15574 d |
| HD 72227 | | | 72227 | 41723 | 08$^h$ 30$^m$ 28.62$^s$ | −32° 09′ 33.4″ | 5.61 | −2.21 | 1194 | K3III | |
| HD 74824 | | | 74824 | 42923 | 08$^h$ 44$^m$ 51.93$^s$ | −37° 08′ 50.1″ | 5.74 | −2.47 | 1430 | B2III | variable star, ΔV = 0.013$^m$, P = 2.72703 d |
| XY Pyx | | XY | 71801 | 41515 | 08$^h$ 27$^m$ 59.43$^s$ | −35° 06′ 49.6″ | 5.75 | −1.68 | 1000 | B2V | β Lyr variable |
| HD 75629 | | | 75629 | 43370 | 08$^h$ 50$^m$ 02.24$^s$ | −29° 27′ 46.8″ | 5.86 | −1.44 | 939 | G8III | |
| HD 73072 | | | 73072 | 42147 | 08$^h$ 35$^m$ 28.72$^s$ | −26° 50′ 36.7″ | 5.95 | −1.10 | 838 | A1V+... | |
| HD 74879 | | | 74879 | 43002 | 08$^h$ 45$^m$ 49.30$^s$ | −25° 23′ 17.2″ | 6.07 | 0.87 | 357 | A3IV/V | |
| HD 74706 | | | 74706 | 42928 | 08$^h$ 44$^m$ 55.16$^s$ | −21° 10′ 04.2″ | 6.10 | 1.63 | 255 | A5V | |
| HD 73900 | | | 73900 | 42455 | 08$^h$ 39$^m$ 22.21$^s$ | −36° 36′ 24.5″ | 6.12 | 3.10 | 131 | F3/F5V | |
| HD 81753 | | | 81753 | 46329 | 09$^h$ 26$^m$ 44.91$^s$ | −28° 47′ 15.7″ | 6.12 | −2.32 | 1590 | B5V | variable star, ΔV = 0.010$^m$, P = 1.23490 d |
| HD 78676 | | | 78676 | 44887 | 09$^h$ 08$^m$ 43.56$^s$ | −26° 46′ 03.5″ | 6.15 | 0.86 | 373 | A4IV | |
| HD 75649 | | | 75649 | 43394 | 08$^h$ 50$^m$ 21.65$^s$ | −28° 37′ 03.4″ | 6.17 | 0.91 | 368 | B9V | |
| HD 72626 | | | 72626 | 41949 | 08$^h$ 33$^m$ 04.85$^s$ | −24° 36′ 24.8″ | 6.19 | 1.72 | 255 | F2IV/V | |
| HD 77361 | | | 77361 | 44290 | 09$^h$ 01$^m$ 11.40$^s$ | −26° 39′ 48.9″ | 6.20 | 0.81 | 389 | K1IIICN... | |
| HD 77087 | | | 77087 | 44130 | 08$^h$ 59$^m$ 15.85$^s$ | −28° 48′ 21.9″ | 6.24 | 0.44 | 472 | G8III | |
| HD 73603 | | | 73603 | 42394 | 08$^h$ 38$^m$ 40.29$^s$ | −19° 44′ 12.9″ | 6.32 | −0.90 | 906 | M1III | suspected variable |
| HD 71622 | | | 71622 | 41449 | 08$^h$ 27$^m$ 16.43$^s$ | −31° 40′ 21.8″ | 6.33 | −0.28 | 685 | G8III | |
| AI Pyx | | AI | 75112 | 43114 | 08$^h$ 46$^m$ 49.25$^s$ | −34° 37′ 22.7″ | 6.33 | −0.86 | 896 | B3V | irregular variable |
| VX Pyx | | VX | 72688 | 41939 | 08$^h$ 32$^m$ 58.51$^s$ | −34° 38′ 02.6″ | 6.36 | 0.78 | 426 | G8III | RS CVn variable, V$_{max}$ = 6.32$^m$, V$_{min}$ = 6.42$^m$ |
| HD 72673 | | | 72673 | 41926 | 08$^h$ 32$^m$ 52.26$^s$ | −31° 30′ 09.7″ | 6.38 | 5.95 | 40 | K0V | |
| HD 79456 | | | 79456 | 45249 | 09$^h$ 13$^m$ 21.53$^s$ | −29° 39′ 51.9″ | 6.38 | −0.98 | 964 | K5III | |
| HD 76512 | | | 76512 | 43853 | 08$^h$ 55$^m$ 55.93$^s$ | −23° 49′ 06.3″ | 6.39 | 2.16 | 229 | A4V | |
| HD 72913 | | | 72913 | 42071 | 08$^h$ 34$^m$ 29.73$^s$ | −27° 05′ 53.5″ | 6.40 | −1.11 | 1035 | K3III | variable star, ΔV = 0.006$^m$, P = 7.67872 d |
| HD 80590 | | | 80590 | 45754 | 09$^h$ 19$^m$ 47.94$^s$ | −34° 06′ 11.9″ | 6.40 | −0.20 | 681 | B8V | |
| HD 72954 | | | 72954 | 42075 | 08$^h$ 34$^m$ 31.95$^s$ | −32° 35′ 54.2″ | 6.41 | 2.42 | 205 | G5V | |
| HD 76072 | | | 76072 | 43590 | 08$^h$ 52$^m$ 38.70$^s$ | −36° 32′ 43.2″ | 6.41 | −1.15 | 1062 | G8III+... | suspected variable, ΔV = 0.15$^m$ |
| HD 74475 | | | 74475 | 42775 | 08$^h$ 42$^m$ 57.01$^s$ | −35° 56′ 36.1″ | 6.42 | 0.77 | 439 | A0V | |
| AK Pyx | | AK | 75306 | 43215 | 08$^h$ 48$^m$ 14.63$^s$ | −28° 38′ 19.6″ | 6.42 | −0.45 | 771 | M5III | semiregular variable |
| HD 75495 | | | 75495 | 43338 | 08$^h$ 49$^m$ 44.94$^s$ | −21° 02′ 53.9″ | 6.48 | 1.96 | 261 | A6IV | |
| HD 76001 | | | 76001 | 43573 | 08$^h$ 52$^m$ 26.14$^s$ | −32° 30′ 33.5″ | 6.49 | −0.48 | 807 | K2/K3III | |
| HD 71815 | | | 71815 | 41572 | 08$^h$ 28$^m$ 36.06$^s$ | −23° 04′ 15.5″ | 6.50 | 0.49 | 519 | A1/A2V | |
| TY Pyx | | TY | 77137 | 44164 | 08$^h$ 59$^m$ 42.72$^s$ | −27° 48′ 58.7″ | 6.87 | | 183.9 | G5IV+G5IV | RS CVn variable, V$_{max}$ = 6.85$^m$, V$_{min}$ = 7.5$^m$, P = 3.1985787 d |
| HD 73256 | | CS | 73256 | 42214 | 08$^h$ 36$^m$ 23.02$^s$ | −30° 02′ 15.5″ | 8.08 | 5.27 | 119 | G9V | BY Dra variable, ΔV = 0.03$^m$, P = 13.97 d; has a planet (b) |
| HD 77338 | | | 77338 | 44291 | 09$^h$ 01$^m$ 00.0$^s$ | −24° 28′ 23″ | 8.63 | | 133 | K0V | has a planet (b) |
| HD 73267 | | | 73267 | 42202 | 08$^h$ 36$^m$ 17.78$^s$ | −34° 27′ 35.9″ | 8.90 | 5.20 | 179 | G5V | has a planet (b) |
| RZ Pyx | | RZ | 75920 | 43541 | 08$^h$ 52$^m$ 04.40$^s$ | −27° 29′ 01.5″ | 9.17 | | 1220 | B7V | β Lyr variable |
| R Pyx | | R | | 42975 | 08$^h$ 45$^m$ 30.70$^s$ | −28° 12′ 02.8″ | 10.40 | | 1860 | C | Mira variable, V$_{max}$ = 7.8$^m$, V$_{min}$ = 12.0$^m$, P = 364.7 d |
| XX Pyx | | XX | | | 08$^h$ 58$^m$ 39.04$^s$ | −24° 35′ 10.6″ | 11.49 | | | A4V | δ Sct and rotating ellipsoidal variable |
| Gliese 317 | | | | | 08$^h$ 40$^m$ 59.21$^s$ | −23° 27′ 22.6″ | 11.98 | | 49.9 | M3.5 | has a planet (b) and an unconfirmed planet (c) |
| WASP-170 | | | | | 09$^h$ 01$^m$ 39.9$^s$ | −20° 43′ 14″ | 12.79 | | | G1 | has a transiting planet (b) |
| T Pyx | | T | | | 09$^h$ 04$^m$ 41.50$^s$ | −32° 22′ 47.5″ | 15.5 | | | | recurrent nova, V$_{max}$ = 6.2$^m$, V$_{min}$ = 15.5$^m$, P = 0.07622886 d |
| VZ Pyx | | VZ | | | 08$^h$ 59$^m$ 19.84$^s$ | −24° 28′ 55.4″ | 16.8 | | | | SU UMa variable, V$_{max}$ = 11.8$^m$, V$_{min}$ = 16.8$^m$, P = 0.07332 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.] ||||||||||||