List of stars in Antlia
# List of stars in Antlia

This is the list of notable stars in the constellation Antlia, sorted by decreasing brightness.

| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| - | - | - | - | - | - | - | - | - | - | - | - |
| α Ant | α | | 90610 | 51172 | $10^h$ $27^m$ $09.16^s$ | −31° 04′ 04.1″ | 4.28 | −0.97 | 366 | K4III | suspected variable, $V_{max}$ = $4.22^m,$ $V_{min}$ = $4.29^m$ |
| ε Ant | ε | | 82150 | 46515 | $09^h$ $29^m$ $14.74^s$ | −35° 57′ 04.9″ | 4.51 | −2.15 | 700 | K3III | variable star, ΔV = $0.003^m,$ P = 0.09026 d |
| ι Ant | ι | | 94890 | 53502 | $10^h$ $56^m$ $43.00^s$ | −37° 08′ 14.9″ | 4.60 | 0.67 | 199 | K0III | |
| θ Ant | θ | | 84367 | 47758 | $09^h$ $44^m$ $12.13^s$ | −27° 46′ 10.4″ | 4.78 | −0.58 | 384 | A7V+... | binary star |
| η Ant | η | | 86629 | 48926 | $09^h$ $58^m$ $52.34^s$ | −35° 53′ 27.4″ | 5.23 | 2.66 | 106 | A8IV | double star |
| HD 90132 | | | 90132 | 50888 | $10^h$ $23^m$ $29.41^s$ | −38° 00′ 35.0″ | 5.34 | 2.30 | 132 | A8V | |
| HD 96146 | | | 96146 | 54173 | $11^h$ $04^m$ $54.21^s$ | −35° 48′ 16.9″ | 5.43 | −0.63 | 530 | A0V | binary star |
| HD 82205 | | | 82205 | 46578 | $09^h$ $29^m$ $54.52^s$ | −26° 35′ 22.6″ | 5.49 | −1.36 | 763 | K2IIICNII | double star |
| U Ant | | U | 91793 | 51821 | $10^h$ $35^m$ $12.88^s$ | −39° 33′ 45.3″ | 5.50 | −1.54 | 836 | C6,3(N0) | slow irregular variable, $V_{max}$ = $5.27^m,$ $V_{min}$ = $6.04^m$ |
| HR 4049 | | AG | 89353 | 50456 | $10^h$ $18^m$ $07.60^s$ | −28° 59′ 31.3″ | 5.52 | −3.60 | 2173 | B9.5Ib/II | protoplanetary nebula, $V_{max}$ = $5.29^m,$ $V_{min}$ = $5.83^m,$ P = 429 d |
| δ Ant A | δ | | 90972 | 51376 | $10^h$ $29^m$ $35.40^s$ | −30° 36′ 25.5″ | 5.56 | −0.27 | 481 | B9/B9.5V | component of the δ Ant system; suspected variable, $V_{max}$ = $5.55^m,$ $V_{min}$ = $5.60^m$ |
| HD 93905 | | | 93905 | 52965 | $10^h$ $49^m$ $57.05^s$ | −34° 03′ 29.5″ | 5.61 | 0.48 | 346 | A1V | |
| HD 83380 | | | 83380 | 47199 | $09^h$ $37^m$ $09.87^s$ | −32° 10′ 43.0″ | 5.62 | 1.05 | 267 | K1III | |
| HD 92845 | | | 92845 | 52407 | $10^h$ $42^m$ $43.21^s$ | −32° 42′ 56.4″ | 5.63 | −0.71 | 605 | A0V | double star |
| HD 83332 | | | 83332 | 47187 | $09^h$ $37^m$ $00.25^s$ | −25° 17′ 48.7″ | 5.68 | 0.91 | 293 | K0III | |
| $ζ^1$ Ant B | $ζ^1$ | | 82383 | 46657 | $09^h$ $30^m$ $46.08^s$ | −31° 53′ 21.0″ | 5.75 | 0.46 | 372 | A0 | binary star |
| HD 86267 | | | 86267 | 48748 | $09^h$ $56^m$ $35.47^s$ | −33° 25′ 06.8″ | 5.83 | −0.01 | 479 | K1III | |
| HD 82514 | | | 82514 | 46736 | $09^h$ $31^m$ $32.93^s$ | −35° 42′ 51.6″ | 5.86 | 1.15 | 285 | K3III | triple star |
| $ζ^2$ Ant | $ζ^2$ | | 82513 | 46734 | $09^h$ $31^m$ $32.19^s$ | −31° 52′ 18.6″ | 5.91 | 0.61 | 374 | A9IV | |
| HD 88809 | | | 88809 | 50103 | $10^h$ $13^m$ $45.98^s$ | −40° 20′ 45.9″ | 5.91 | 0.21 | 450 | K1III | double star |
| HD 85206 | | | 85206 | 48191 | $09^h$ $49^m$ $28.15^s$ | −37° 11′ 12.4″ | 5.95 | 0.47 | 407 | K2III | |
| HD 83441 | | | 83441 | 47224 | $09^h$ $37^m$ $28.42^s$ | −36° 05′ 45.6″ | 5.96 | 0.89 | 337 | K2III | |
| HD 88218 | | | 88218 | 49769 | $10^h$ $09^m$ $32.09^s$ | −35° 51′ 24.5″ | 6.14 | 3.70 | 100 | G1V | binary star |
| HD 82165 | | | 82165 | 46517 | $09^h$ $29^m$ $16.25^s$ | −38° 24′ 12.8″ | 6.15 | 2.18 | 203 | A6V | |
| HD 89015 | | | 89015 | 50234 | $10^h$ $15^m$ $20.89^s$ | −36° 31′ 03.8″ | 6.17 | 0.91 | 367 | K0III | |
| $ζ^1$ Ant A | $ζ^1$ | | 82384 | | $09^h$ $30^m$ $46.10^s$ | −31° 53′ 22.0″ | 6.18 | | | | component of the $ζ^1$ Ant system |
| HD 90071 | | | 90071 | 50868 | $10^h$ $23^m$ $13.14^s$ | −30° 09′ 44.0″ | 6.25 | 2.60 | 175 | A9IV | |
| HD 87606 | | | 87606 | 49418 | $10^h$ $05^m$ $15.28^s$ | −36° 23′ 03.7″ | 6.27 | 0.71 | 422 | K1III | |
| HD 85725 | | | 85725 | 48468 | $09^h$ $52^m$ $58.21^s$ | −27° 19′ 56.7″ | 6.28 | 2.50 | 186 | G1V | double star |
| HD 88522 | | | 88522 | 49967 | $10^h$ $12^m$ $02.88^s$ | −28° 36′ 21.4″ | 6.28 | 0.31 | 509 | A0V | double star |
| HD 89442 | | | 89442 | 50492 | $10^h$ $18^m$ $37.88^s$ | −36° 48′ 16.5″ | 6.31 | −0.04 | 608 | K2/K3III | |
| BF Ant | | BF | 86301 | 48776 | $09^h$ $56^m$ $54.14^s$ | −27° 28′ 30.8″ | 6.32 | 0.38 | 502 | A4V | δ Scuti variable, ΔV = $0.01^m$ |
| HD 88836 | | | 88836 | 50122 | $10^h$ $13^m$ $56.58^s$ | −40° 18′ 38.7″ | 6.33 | 0.64 | 448 | G8III | double star |
| HD 88013 | | | 88013 | 49645 | $10^h$ $08^m$ $01.67^s$ | −37° 20′ 00.5″ | 6.34 | 0.05 | 590 | K0III | |
| HD 85296 | | | 85296 | 48219 | $09^h$ $49^m$ $51.36^s$ | −36° 16′ 06.5″ | 6.36 | 0.20 | 555 | K0III | |
| HD 92589 | | | 92589 | 52273 | $10^h$ $40^m$ $51.56^s$ | −35° 44′ 30.2″ | 6.36 | −0.28 | 695 | G8/K0III+.. | double star |
| HD 88742 | | | 88742 | 50075 | $10^h$ $13^m$ $24.99^s$ | −33° 01′ 54.8″ | 6.38 | 4.60 | 74 | G0V | |
| HD 84224 | | | 84224 | 47627 | $09^h$ $42^m$ $41.37^s$ | −35° 30′ 06.2″ | 6.39 | −1.80 | 1417 | Asp... | |
| HD 87477 | | | 87477 | 49343 | $10^h$ $04^m$ $23.39^s$ | −39° 58′ 33.1″ | 6.42 | −0.03 | 637 | K1III | |
| S Ant | | S | 82610 | 46810 | $09^h$ $32^m$ $18.45^s$ | −28° 37′ 40.4″ | 6.43 | 2.05 | 245 | A9V | W Uma variable, $V_{max}$ = $6.27^m,$ $V_{min}$ = $6.83^m,$ P = 0.6483489 d |
| HD 82785 | | | 82785 | 46874 | $09^h$ $33^m$ $07.71^s$ | −39° 07′ 45.0″ | 6.43 | 2.12 | 237 | F2IV/V | binary star |
| HD 84567 | | | 84567 | 47868 | $09^h$ $45^m$ $22.01^s$ | −30° 12′ 09.9″ | 6.45 | -3.7 | 3500 | B0.5IIIn | suspected variable |
| HD 83108 | | | 83108 | 47039 | $09^h$ $35^m$ $11.88^s$ | −35° 49′ 25.5″ | 6.48 | 2.47 | 207 | F5V | |
| HD 92987 | | | 92987 | 52472 | $10^h$ $43^m$ $36.0^s$ | −39° 03′ 31″ | 7.0 | | 142 | G2/3V | has a planet (b) |
| HD 93083 | | | 93083 | 52521 | $10^h$ $44^m$ $20.91^s$ | −33° 34′ 37.2″ | 8.33 | 6.03 | 94 | K2V | Macondo; has a planet (b) |
| T Ant | | T | | 46924 | $09^h$ $33^m$ $50.86^s$ | −36° 36′ 56.7″ | 9.26 | -0.7 | 3200 | G5 | Classical Cepheid, $V_{max}$ = $8.88^m,$ $V_{min}$ = $9.82^m,$ P = 5.898053 d |
| δ Ant B | δ | BZ | 90972B | | $10^h$ $29^m$ $34.77^s$ | −30° 36′ 33.1″ | 9.65 | 3.81 | 481 | F9Ve | component of the δ Ant system; T Tauri star, ΔV = $0.04^m,$ P = 3.3 d |
| TWA 6 | | BX | | | $10^h$ $18^m$ $28.70^s$ | −31° 50′ 02.9″ | 10.65 | | | M0Ve | T Tauri star, ΔV = $0.149^m,$ P = 0.5409 d |
| WASP-66 | | | | | $10^h$ $32^m$ $54.0^s$ | −34° 59′ 23″ | 11.6 | 3.7 | 1239 | F4 | has a transiting planet (b) |
| TWA 7 | | CE | | | $10^h$ $42^m$ $30.06^s$ | −33° 40′ 16.6″ | 11.73 | | | M2Ve | T Tauri star, ΔV = $0.11^m,$ P = 5.00 d |
| UX Ant | | UX | | | $10^h$ $57^m$ $09.0^s$ | −37° 23′ 56″ | 12.37 | | | | R CrB variable, $V_{max}$ = $11.5^m,$ $V_{min}$ = $<18.0^m$ |
| DEN 1048-3956 | | | | | $10^h$ $48^m$ $15^s$ | −39° 56′ 06″ | 17.53 | 4.52 | 13.051 | M9V | brown dwarf |
| XTE J0929-314 | | BW | | | $09^h$ $29^m$ $20.19^s$ | −31° 29′ 03.2″ | 18.63 | | | | X-ray pulsar, $V_{max}$ = $18.63^m,$ $V_{min}$ = $22.89^m,$ P = 0.030263 d |
| 2MASS 0939-2448 | | | | | $09^h$ $39^m$ $39.49^s$ | −24° 48′ 27.9″ | | | 17 | T8 | binary brown dwarf |
| 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.] ||||||||||||
