List of stars in Grus
# List of stars in Grus

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

| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| - | - | - | - | - | - | - | - | - | - | - | - |
| α Gru | α | | 209952 | 109268 | $22^h$ $08^m$ $13.88^s$ | −46° 57′ 38.2″ | 1.73 | −0.73 | 101 | B7IV | Alnair (Al Nair, Al Na'ir); suspected variable, $V_{max}$ = $1.70^m,$ $V_{min}$ = $1.76^m$ |
| β Gru | β | | 214952 | 112122 | $22^h$ $42^m$ $39.93^s$ | −46° 53′ 04.4″ | 2.07 | −1.52 | 170 | M5III | Tiaki, semiregular variable, $V_{max}$ = $1.90^m,$ $V_{min}$ = $2.3^m,$ P = 37 d |
| γ Gru | γ | | 207971 | 108085 | $21^h$ $53^m$ $55.65^s$ | −37° 21′ 53.4″ | 3.00 | −0.97 | 203 | B8III | Al Dhanab |
| ε Gru | ε | | 215789 | 112623 | $22^h$ $48^m$ $33.20^s$ | −51° 19′ 00.1″ | 3.49 | 0.49 | 130 | A3V | suspected variable, $V_{max}$ = $3.47^m,$ $V_{min}$ = $3.53^m$ |
| ι Gru | ι | | 218670 | 114421 | $23^h$ $10^m$ $21.43^s$ | −45° 14′ 47.9″ | 3.88 | 0.11 | 185 | K0III SB | |
| $δ^1$ Gru | $δ^1$ | | 213009 | 110997 | $22^h$ $29^m$ $16.15^s$ | −43° 29′ 44.0″ | 3.97 | −0.82 | 296 | G6/G8III | |
| ζ Gru | ζ | | 217364 | 113638 | $23^h$ $00^m$ $52.87^s$ | −52° 45′ 14.8″ | 4.11 | 1.42 | 112 | G8III | |
| $δ^2$ Gru | $δ^2$ | | 213080 | 111043 | $22^h$ $29^m$ $45.45^s$ | −43° 44′ 57.2″ | 4.12 | −0.87 | 325 | M4.5IIIa | semiregular variable, $V_{max}$ = $3.99^m,$ $V_{min}$ = $4.2^m$ |
| θ Gru | θ | | 218227 | 114131 | $23^h$ $06^m$ $52.77^s$ | −43° 31′ 13.2″ | 4.28 | 1.23 | 133 | F5me... | |
| λ Gru | λ | | 209688 | 109111 | $22^h$ $06^m$ $06.90^s$ | −39° 32′ 35.0″ | 4.47 | 0.07 | 247 | M0III | |
| $μ^1$ Gru | $μ^1$ | | 211088 | 109908 | $22^h$ $15^m$ $36.88^s$ | −41° 20′ 48.3″ | 4.79 | 0.26 | 262 | G8III+... | |
| ρ Gru | ρ | | 215104 | 112203 | $22^h$ $43^m$ $29.97^s$ | −41° 24′ 50.8″ | 4.84 | 0.68 | 222 | K0III | |
| η Gru | η | | 215369 | 112374 | $22^h$ $45^m$ $37.85^s$ | −53° 30′ 00.6″ | 4.84 | −0.57 | 394 | K2IIICNIV | variable star, ΔV = $0.006^m,$ P = 2.76870 d |
| $μ^2$ Gru | $μ^2$ | | 211202 | 109973 | $22^h$ $16^m$ $26.57^s$ | −41° 37′ 37.9″ | 5.11 | 0.78 | 240 | G8III | variable star, ΔV = $0.004^m,$ P = 0.13316 d |
| ξ Gru | ξ | | 204783 | 106327 | $21^h$ $32^m$ $05.86^s$ | −41° 10′ 45.6″ | 5.29 | −0.06 | 383 | K0III | |
| HD 211415 | | | 211415 | 110109 | $22^h$ $18^m$ $15.18^s$ | −53° 37′ 31.9″ | 5.36 | 4.69 | 44 | G1V | |
| κ Gru | κ | | 217902 | 113957 | $23^h$ $04^m$ $39.57^s$ | −53° 57′ 52.7″ | 5.37 | −0.02 | 390 | K5III | |
| HD 216149 | | | 216149 | 112832 | $22^h$ $51^m$ $02.15^s$ | −39° 09′ 24.5″ | 5.43 | −2.22 | 1105 | K3III | |
| HD 208321 | | | 208321 | 108294 | $21^h$ $56^m$ $22.79^s$ | −37° 15′ 13.1″ | 5.45 | 0.52 | 315 | A3V | |
| ν Gru | ν | | 212953 | 110936 | $22^h$ $28^m$ $39.18^s$ | −39° 07′ 53.0″ | 5.47 | 0.94 | 262 | G8III | |
| HD 208737 | | | 208737 | 108543 | $21^h$ $59^m$ $17.88^s$ | −38° 23′ 42.3″ | 5.50 | 0.09 | 393 | K1II/III | |
| HD 215405 | | | 215405 | 112381 | $22^h$ $45^m$ $40.81^s$ | −46° 32′ 50.3″ | 5.52 | −1.02 | 664 | K3III | |
| ο Gru | ο | | 220729 | 115713 | $23^h$ $26^m$ $36.54^s$ | −52° 43′ 18.9″ | 5.53 | 3.01 | 104 | F4V | |
| φ Gru | φ | | 219693 | 115054 | $23^h$ $18^m$ $09.79^s$ | −40° 49′ 26.6″ | 5.54 | 2.84 | 113 | F5V | |
| HD 204960 | | | 204960 | 106429 | $21^h$ $33^m$ $23.53^s$ | −44° 50′ 55.3″ | 5.57 | −0.83 | 622 | K0III | |
| HD 207129 | | | 207129 | 107649 | $21^h$ $48^m$ $15.61^s$ | −47° 18′ 10.4″ | 5.57 | 4.60 | 51 | G2V | |
| $π^2$ Gru | $π^2$ | | 212132 | 110506 | $22^h$ $23^m$ $07.79^s$ | −45° 55′ 42.0″ | 5.62 | 2.58 | 132 | F3III-IV | |
| υ Gru | υ | | 218242 | 114132 | $23^h$ $06^m$ $53.60^s$ | −38° 53′ 32.3″ | 5.62 | 0.84 | 294 | A0V | |
| HD 217403 | | | 217403 | 113657 | $23^h$ $01^m$ $07.50^s$ | −50° 57′ 00.1″ | 5.68 | −0.16 | 481 | K3III | |
| $τ^3$ Gru | $τ^3$ | | 216823 | 113307 | $22^h$ $56^m$ $47.82^s$ | −47° 58′ 09.2″ | 5.72 | 1.11 | 272 | Am... | |
| HD 220440 | | | 220440 | 115537 | $23^h$ $24^m$ $13.24^s$ | −51° 53′ 27.9″ | 5.75 | −0.39 | 552 | M0III | suspected variable |
| HD 219263 | | | 219263 | 114775 | $23^h$ $14^m$ $58.53^s$ | −41° 06′ 18.5″ | 5.77 | 1.49 | 234 | K2III | |
| HD 217842 | | | 217842 | 113902 | $23^h$ $03^m$ $59.63^s$ | −41° 28′ 44.5″ | 5.79 | 0.97 | 301 | K0III | variable star, ΔV = $0.004^m,$ P = 0.27350 d |
| HD 218269 | | | 218269 | 114167 | $23^h$ $07^m$ $14.81^s$ | −50° 41′ 11.8″ | 5.81 | 2.81 | 130 | F6.5IV-V+.. | suspected variable |
| HD 218630 | | | 218630 | 114382 | $23^h$ $09^m$ $57.64^s$ | −42° 51′ 40.2″ | 5.83 | 3.13 | 113 | F4IV | |
| $σ^2$ Gru | $σ^2$ | | 214150 | 111643 | $22^h$ $36^m$ $58.82^s$ | −40° 35′ 27.1″ | 5.85 | 1.71 | 219 | A1V | |
| DL Gru | | DL | 218655 | 114407 | $23^h$ $10^m$ $09.72^s$ | −40° 35′ 29.2″ | 5.90 | −1.05 | 799 | M4III | semiregular variable |
| HD 219507 | | | 219507 | 114921 | $23^h$ $16^m$ $39.79^s$ | −44° 29′ 20.9″ | 5.92 | 1.19 | 288 | K1III | |
| HD 214953 | | | 214953 | 112117 | $22^h$ $42^m$ $36.88^s$ | −47° 12′ 36.0″ | 5.99 | 4.13 | 77 | G0 | suspected variable, $V_{max}$ = $5.97^m,$ $V_{min}$ = $6.02^m$ |
| S Gru | | S | 212539 | 110736 | $22^h$ $26^m$ $05.47^s$ | −48° 26′ 18.8″ | 6.00 | | 1450 | M8IIIe | Mira variable, $V_{max}$ = $6^m,$ $V_{min}$ = $15^m,$ P = 401.51 d |
| $τ^1$ Gru | $τ^1$ | | 216435 | 113044 | $22^h$ $53^m$ $37.74^s$ | −48° 35′ 53.1″ | 6.03 | 3.42 | 109 | G3IV | has a planet |
| HD 220003 | | | 220003 | 115272 | $23^h$ $20^m$ $50.13^s$ | −50° 18′ 23.0″ | 6.04 | 1.26 | 294 | Fm... | |
| HD 214987 | | | 214987 | 112127 | $22^h$ $42^m$ $43.05^s$ | −44° 14′ 53.2″ | 6.06 | 1.10 | 320 | K1IV | suspected variable, $V_{max}$ = $6.05^m,$ $V_{min}$ = $6.07^m$ |
| HD 211053 | | | 211053 | 109902 | $22^h$ $15^m$ $35.03^s$ | −44° 27′ 05.4″ | 6.10 | −0.16 | 583 | G8/K0III | |
| HD 220401 | | | 220401 | 115496 | $23^h$ $23^m$ $45.41^s$ | −43° 07′ 28.0″ | 6.12 | −1.55 | 1116 | K3III | |
| HD 220392 | | DQ | 220392 | 115510 | $23^h$ $23^m$ $54.45^s$ | −53° 48′ 31.2″ | 6.13 | 0.29 | 480 | A4III | δ Scuti variable |
| BZ Gru | | BZ | 208435 | 108347 | $21^h$ $57^m$ $02.14^s$ | −37° 44′ 48.7″ | 6.18 | 0.53 | 440 | F2/F3V | δ Scuti variable, $V_{max}$ = $6.13^m,$ $V_{min}$ = $6.21^m$ |
| HD 210918 | | | 210918 | 109821 | $22^h$ $14^m$ $38.21^s$ | −41° 22′ 47.1″ | 6.23 | 4.51 | 72 | G5V | |
| HD 206642 | | | 206642 | 107344 | $21^h$ $44^m$ $29.41^s$ | −38° 33′ 07.7″ | 6.28 | −0.62 | 782 | K1IIICN... | |
| $σ^1$ Gru | $σ^1$ | | 214085 | 111594 | $22^h$ $36^m$ $29.27^s$ | −40° 34′ 57.0″ | 6.28 | 2.07 | 226 | A3Vn | |
| HD 205096 | | | 205096 | 106500 | $21^h$ $34^m$ $17.18^s$ | −42° 55′ 28.8″ | 6.32 | 1.34 | 323 | K1IIICN... | |
| HD 218255 | | | 218255 | 114159 | $23^h$ $07^m$ $09.43^s$ | −49° 36′ 22.1″ | 6.33 | −1.68 | 1304 | K4III | |
| HD 216666 | | | 216666 | 113189 | $22^h$ $55^m$ $14.87^s$ | −36° 23′ 18.9″ | 6.40 | −0.33 | 723 | K2III | |
| $π^1$ Gru | $π^1$ | | 212087 | 110478 | $22^h$ $22^m$ $44.18^s$ | −45° 56′ 52.5″ | 6.42 | 0.50 | 498 | S5,7: | semiregular variable, $V_{max}$ = $5.31^m,$ $V_{min}$ = $7.01^m,$ P = 195.5 d |
| HD 210204 | | | 210204 | 109408 | $22^h$ $09^m$ $57.82^s$ | −48° 06′ 27.0″ | 6.43 | −0.19 | 686 | K3III | |
| HD 217642 | | | 217642 | 113784 | $23^h$ $02^m$ $34.07^s$ | −36° 25′ 14.9″ | 6.46 | 0.93 | 415 | K1III | |
| HD 215504 | | | 215504 | 112432 | $22^h$ $46^m$ $28.22^s$ | −49° 41′ 06.4″ | 6.49 | −0.35 | 760 | K0III-IV | |
| HD 219531 | | | 219531 | 114937 | $23^h$ $16^m$ $49.85^s$ | −41° 11′ 40.0″ | 6.49 | 0.61 | 489 | K0III | |
| HD 215456 | | | 215456 | 112414 | $22^h$ $46^m$ $08^s$ | −48° 58′ 4″ | 6.63 | | 124 | G0.5V | has two planets (b & c) |
| $τ^2$ Gru | $τ^2$ | | 216656 | 113190 | $22^h$ $55^m$ $16.19^s$ | −48° 29′ 30.8″ | 6.67 | 3.33 | 152 | F7V: | component of the $τ^2$ Gru system |
| $τ^2$ Gru | $τ^2$ | | 216655 | 113191 | $22^h$ $55^m$ $16.35^s$ | −48° 27′ 57.4″ | 7.04 | 3.71 | 151 | G5 | component of the $τ^2$ Gru system |
| HD 213240 | | | 213240 | 111143 | $22^h$ $31^m$ $00.37^s$ | −49° 25′ 59.8″ | 6.80 | 3.75 | 133 | G0/G1V | has a planet (b) |
| HD 208487 | | | 208487 | 108375 | $21^h$ $57^m$ $19.85^s$ | −37° 45′ 49.0″ | 7.48 | 4.26 | 143 | G2V: | Itonda, has two planets (b & c) |
| HD 217522 | | BP | 217522 | 113711 | $23^h$ $01^m$ $46.82^s$ | −44° 50′ 26.9″ | 8.26 | | 287.0 | Ap... | rapidly oscillating Ap star |
| RS Gru | | RS | 206379 | 107231 | $21^h$ $43^m$ $04.22^s$ | −48° 11′ 22.2″ | 8.26 | | 776 | A9IV | δ Sct variable, $V_{max}$ = $7.94^m,$ $V_{min}$ = $8.48^m,$ P = 0.1470117 d |
| Gliese 832 | | | 204961 | 106440 | $21^h$ $33^m$ $33.98^s$ | −49° 00′ 32.4″ | 8.67 | 10.20 | 16.1 | M1.5V | has a planet (b) |
| W Gru | | W | 214791 | 112009 | $22^h$ $41^m$ $18.67^s$ | −43° 50′ 28.6″ | 8.96 | | 1140 | F5V | AR Lac variable |
| WASP-95 | | | | | $22^h$ $29^m$ $50.0^s$ | −48° 00′ 11″ | 10.1 | | | G2 | has a transiting planet (b) |
| BC Gru | | BC | | | $22^h$ $44^m$ $49.11^s$ | −48° 10′ 13.0″ | 10.60 | | | | W UMa variable, $V_{max}$ = $10.60^m,$ $V_{min}$ = $10.94^m,$ P = 0.30735686 d |
| U Gru | | U | | | $21^h$ $31^m$ $48.77^s$ | −45° 02′ 42.5″ | 11.38 | | | A5 | Algol variable |
| RZ Gru | | RZ | | | $22^h$ $47^m$ $12.01^s$ | −42° 44′ 38.72″ | 12.04 | | | B6 | nova-like star |
| CE Gru | | CE | | | $21^h$ $37^m$ $56.38^s$ | −43° 42′ 13.1″ | 17.4 | | | | AM Her variable, $V_{max}$ = $17.4^m,$ $V_{min}$ = $19.5^m,$ P = 0.0754 d |
| PSR J2144-3933 | | | | | $21^h$ $44^m$ $12.0^s$ | −39° 33′ 55.2″ | | | | | pulsar |
| 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.] ||||||||||||
