This is the list of notable stars in the constellation Carina, sorted by decreasing brightness.
This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Carina does not have a full complement of Greek-letter designations. For example, since Argo Navis's gamma star went to Vela, there is no Gamma Carinae.
Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes | ||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Canopus | α | 45348 | 30438 | 06h 23m 57.09s | −52° 41′ 44.6″ | −0.72 | −5.53 | 313 | A9 II [1] [2] | Suhel; [3] 2nd brightest star | |||||
β Car | β | 80007 | 45238 | 09h 13m 12.24s | −69° 43′ 02.9″ | 1.67 | −0.99 | 111 | A1 III [4] | Miaplacidus | |||||
ε Car | ε | 71129 | 41037 | 08h 22m 30.86s | −59° 30′ 34.3″ | 1.86 | −4.58 | 632 | K3III+B2V | Avior; suspected eclipsing binary, Vmax = 1.82m, Vmin = 1.94m | |||||
ι Car | ι | 80404 | 45556 | 09h 17m 05.43s | −59° 16′ 30.9″ | 2.23 | −4.43 | 692 | A8Ib | Aspidiske, Turais, Scutulum; suspected variable, Vmax = 2.23m, Vmin = 2.28m | |||||
θ Car | θ | 93030 | 52419 | 10h 42m 57.43s | −64° 23′ 40.1″ | 2.74 | −2.91 | 439 | B0Vp | in IC 2602 | |||||
υ Car | υ | 85123 | 48002 | 09h 47m 06.14s | −65° 04′ 19.3″ | 2.92 | −5.56 | 1622 | A9 | binary star | |||||
ω Car | ω | 89080 | 50099 | 10h 13m 44.28s | −70° 02′ 16.5″ | 3.29 | −1.99 | 370 | B8III | ||||||
p Car | p | PP | 91465 | 51576 | 10h 32m 01.48s | −61° 41′ 07.3″ | 3.30 | −2.62 | 497 | B4Vne | γ Cas variable, Vmax = 3.22m, Vmin = 3.55m | ||||
V337 Car | q | V337 | 89388 | 50371 | 10h 17m 05.01s | −61° 19′ 56.4″ | 3.39 | −3.38 | 736 | K3II | irregular variable, Vmax = 3.36m, Vmin = 3.44m | ||||
a Car | a | V357 | 79351 | 45080 | 09h 10m 58.11s | −58° 58′ 00.9″ | 3.43 | −2.11 | 418 | B2IV | eclipsing binary, Vmax = 3.41m, Vmin = 3.44m | ||||
χ Car | χ | 65575 | 38827 | 07h 56m 46.74s | −52° 58′ 56.6″ | 3.46 | −1.91 | 387 | B3IVp | β Cep variable, ΔV = 0.015m, P = 0.10 d | |||||
l Car | l | 84810 | 47854 | 09h 45m 14.83s | −62° 30′ 28.5″ | 3.69 | −4.64 | 1509 | G5Iab/Ib | classical Cepheid, Vmax = 3.28m, Vmin = 4.18m, P = 35.54 d | |||||
HD 94510 | u | 94510 | 53253 | 10h 53m 29.57s | −58° 51′ 11.8″ | 3.78 | 1.42 | 97 | K0III-IV... | suspected variable, Vmax = 3.75m, Vmin = 3.80m | |||||
HD 90853 | s | 90853 | 51232 | 10h 27m 52.75s | −58° 44′ 21.9″ | 3.81 | −3.71 | 1042 | F2II | suspected variable | |||||
HD 76728 | c | 76728 | 43783 | 08h 55m 02.86s | −60° 38′ 41.0″ | 3.84 | −1.06 | 312 | B8III | double star | |||||
V382 Car | x | V382 | 96918 | 54463 | 11h 08m 35.40s | −58° 58′ 30.2″ | 3.93 | −7.37 | 5927 | G0Ia0 | hypergiant; slow irregular variable, Vmax = 3.77m, Vmin = 4.05m | ||||
HD 79447 | i | 79447 | 45101 | 09h 11m 16.77s | −62° 19′ 01.3″ | 3.96 | −1.97 | 499 | B3IV | variable star, ΔV = 0.008m, P = 22.26 d | |||||
HD 90589 | I | 90589 | 50954 | 10h 24m 23.74s | −74° 01′ 53.6″ | 3.99 | 2.94 | 53 | F2IV | suspected variable, Vmax = 3.96m, Vmin = 4.00m | |||||
HD 83183 | h | 83183 | 46974 | 09h 34m 26.66s | −59° 13′ 47.2″ | 4.08 | −4.83 | 1976 | B5II | ||||||
V343 Car | d | V343 | 74375 | 42568 | 08h 40m 37.04s | −59° 45′ 39.7″ | 4.31 | −3.87 | 1411 | B1.5III | β Cep variable | ||||
HD 80230 | g | 80230 | 45496 | 09h 16m 12.10s | −57° 32′ 29.2″ | 4.34 | −1.74 | 536 | M1III | suspected variable, Vmax = 4.31m, Vmin = 4.35m | |||||
HD 47306 | N | 47306 | 31407 | 06h 34m 58.59s | −52° 58′ 32.3″ | 4.35 | −4.31 | 1762 | B9III | ||||||
HR 2554 | A | V415 | 50337 | 32761 | 06h 49m 51.32s | −53° 37′ 21.0″ | 4.39 | −1.74 | 553 | G6II | Algol variable, ΔV = 0.06m | ||||
HD 91942 | r | 91942 | 51849 | 10h 35m 35.31s | −57° 33′ 27.5″ | 4.45 | −3.68 | 1376 | K3/K4II | suspected variable | |||||
η Car | η | 93308 | 10h 45m 03.60s | −59° 41′ 03.0″ | 4.47 | 7500 | LBV | Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, Vmax = −0.8m, Vmin = 7.9m; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known. | |||||||
HR 3643 | G | 78791 | 44599 | 09h 05m 08.83s | −72° 36′ 09.7″ | 4.47 | −1.25 | 454 | F6II-III | ||||||
V344 Car | f | V344 | 75311 | 43105 | 08h 46m 42.56s | −56° 46′ 11.3″ | 4.50 | −1.62 | 546 | B3Vne | γ Cas variable, Vmax = 4.40m, Vmin = 4.51m | ||||
HD 83944 | m | 83944 | 47391 | 09h 39m 21.04s | −61° 19′ 41.2″ | 4.51 | 0.33 | 224 | B9V | suspected variable | |||||
V520 Car | w | V520 | 93070 | 52468 | 10h 43m 32.31s | −60° 33′ 59.9″ | 4.58 | −2.99 | 1065 | K3Ib | irregular variable, Vmax = 4.50m, Vmin = 4.59m | ||||
V533 Car | y | V533 | 97534 | 54751 | 11h 12m 36.02s | −60° 19′ 03.5″ | 4.59 | −8.34 | 12538 | A6Ia | α Cyg variable | ||||
HD 96566 | z1 | 96566 | 54301 | 11h 06m 32.47s | −62° 25′ 26.9″ | 4.62 | −0.65 | 370 | G8III | ||||||
V399 Car | P | V399 | 90772 | 51192 | 10h 27m 24.48s | −57° 38′ 19.7″ | 4.65 | A6Ia | semiregular variable, Vmax = 4.63m, Vmin = 4.72m, P = 88.3 d | ||||||
V345 Car | E | V345 | 78764 | 44626 | 09h 05m 38.38s | −70° 32′ 18.7″ | 4.67 | −2.94 | 1079 | B2IVe | γ Cas variable, Vmax = 4.67m, Vmin = 4.78m, P = 137.7 d | ||||
HD 92397 | t2 | 92397 | 52102 | 10h 38m 45.01s | −59° 10′ 58.8″ | 4.69 | −4.08 | 1852 | K4/K5III: | suspected variable | |||||
HD 91375 | K | 91375 | 51438 | 10h 30m 20.08s | −71° 59′ 33.8″ | 4.72 | 0.22 | 259 | A2III | ||||||
HR 3220 | B | 68456 | 39903 | 08h 09m 00.86s | −61° 18′ 06.1″ | 4.74 | 3.09 | 70 | F5V | ||||||
V518 Car | V518 | 92938 | 52370 | 10h 42m 14.14s | −64° 27′ 59.2″ | 4.76 | −0.97 | 456 | B3V | in IC 2602; γ Cas variable | |||||
HD 81101 | k | 81101 | 45856 | 09h 20m 56.83s | −62° 24′ 16.7″ | 4.79 | 0.62 | 223 | G6III | ||||||
HD 93194 | 93194 | 52502 | 10h 44m 06.94s | −63° 57′ 40.0″ | 4.80 | −1.06 | 484 | B5Vn | in IC 2602; suspected irregular variable, Vmax = 4.79m, Vmin = 4.84m | ||||||
HD 66591 | D | 66591 | 39138 | 08h 00m 19.97s | −63° 34′ 03.0″ | 4.81 | −1.29 | 542 | B3V | suspected variable | |||||
HD 73389 | e2 | 73389 | 42134 | 08h 35m 19.65s | −58° 00′ 33.5″ | 4.84 | 0.60 | 229 | K0III | ||||||
HD 93607 | 93607 | 52736 | 10h 46m 51.24s | −64° 23′ 00.6″ | 4.87 | −0.83 | 449 | B3IV | in IC 2602; suspected variable | ||||||
HD 61248 | Q | 61248 | 36942 | 07h 35m 39.70s | −52° 32′ 01.7″ | 4.93 | −0.48 | 394 | K3III | suspected variable | |||||
V376 Car | b1 | V376 | 77002 | 43937 | 08h 56m 58.43s | −59° 13′ 45.7″ | 4.93 | −1.47 | 621 | B2IV-V | β Cep variable, Vmax = 4.91m, Vmin = 4.96m, P = 0.021 d | ||||
HD 91496 | 91496 | 51495 | 10h 31m 02.07s | −73° 13′ 17.4″ | 4.94 | −2.42 | 964 | K4/K5III | suspected variable, Vmax = 4.87m, Vmin = 4.97m | ||||||
HD 90264 | L | 90264 | 50847 | 10h 22m 58.18s | −66° 54′ 05.5″ | 4.97 | −0.63 | 430 | B8V | ||||||
HD 92063 | t1 | 92063 | 51912 | 10h 36m 20.56s | −59° 33′ 51.5″ | 5.08 | 0.50 | 269 | K1III | ||||||
HD 59219 | 59219 | 36114 | 07h 26m 21.86s | −51° 01′ 06.6″ | 5.09 | −1.09 | 562 | K0III | |||||||
HD 96919 | z2 | V371 | 96919 | 54461 | 11h 08m 34.01s | −61° 56′ 49.8″ | 5.12 | −6.03 | 5525 | B9Ia | α Cyg variable, Vmax = 5.12m, Vmin = 5.19m | ||||
HD 53047 | 53047 | 33779 | 07h 00m 51.51s | −51° 24′ 09.5″ | 5.14 | −1.25 | 617 | M1III | semiregular variable | ||||||
V386 Car | V386 | 54118 | 34105 | 07h 04m 18.32s | −56° 44′ 59.0″ | 5.14 | 0.45 | 282 | A0p: | α2 CVn variable, ΔV = 0.026m, P = 3.28 d | |||||
HD 88981 | M | 88981 | 50083 | 10h 13m 30.68s | −66° 22′ 22.2″ | 5.15 | 0.31 | 304 | Am | ||||||
HD 69863 | C | 69863 | 40429 | 08h 15m 15.95s | −62° 54′ 56.2″ | 5.16 | 0.81 | 242 | A+... | binary star | |||||
HD 77370 | b2 | 77370 | 44143 | 08h 59m 24.38s | −59° 05′ 03.8″ | 5.17 | 3.08 | 85 | F3V | ||||||
HR 3153 | V460 | 66342 | 39070 | 07h 59m 37.55s | −60° 35′ 13.5″ | 5.19 | −2.34 | 1045 | M0II | in NGC 2516; semiregular variable, Vmax = 5.15m, Vmin = 5.3m | |||||
HD 97583 | 97583 | 54767 | 11h 12m 45.27s | −64° 10′ 11.2″ | 5.22 | 0.30 | 314 | B9V | double star | ||||||
HD 93549 | 93549 | 52701 | 10h 46m 29.61s | −64° 15′ 47.7″ | 5.23 | −0.37 | 429 | B7IV | in IC 2602 | ||||||
HD 88323 | 88323 | 49698 | 10h 08m 42.84s | −65° 48′ 55.9″ | 5.26 | 0.16 | 341 | K0III | optical double | ||||||
V524 Car | V524 | 94367 | 53154 | 10h 52m 30.85s | −57° 14′ 25.5″ | 5.26 | −6.08 | 6037 | B9Ia | α Cyg variable | |||||
HD 73390 | e1 | 73390 | 42129 | 08h 35m 15.58s | −58° 13′ 29.1″ | 5.27 | −2.08 | 962 | B3V+... | ||||||
HD 91056 | 91056 | 51313 | 10h 28m 52.60s | −64° 10′ 20.2″ | 5.27 | −4.64 | 3135 | K3Ib | slow irregular variable | ||||||
HD 80951 | 80951 | 45581 | 09h 17m 25.21s | −74° 53′ 39.8″ | 5.28 | −1.44 | 721 | A1V | |||||||
HD 84121 | 84121 | 47479 | 09h 40m 42.60s | −57° 59′ 00.9″ | 5.30 | 1.16 | 220 | A3IV | |||||||
HD 93540 | 93540 | 52678 | 10h 46m 16.58s | −64° 30′ 52.5″ | 5.33 | −0.45 | 466 | B7:V | in IC 2602; suspected variable | ||||||
HD 92964 | V519 | 92964 | 52405 | 10h 42m 40.57s | −59° 12′ 56.8″ | 5.36 | −6.23 | 6792 | B2.5Ia | α Cyg variable, Vmax = 5.32m, Vmin = 5.43m, P = 14.68 d | |||||
HD 57917 | 57917 | 35589 | 07h 20m 38.81s | −52° 05′ 09.3″ | 5.38 | −0.52 | 493 | B9V | |||||||
HD 80671 | 80671 | 45571 | 09h 17m 17.40s | −68° 41′ 22.5″ | 5.38 | 2.75 | 109 | F4V | |||||||
HD 49689 | 49689 | 32494 | 06h 46m 52.69s | −51° 15′ 55.6″ | 5.39 | −1.83 | 906 | K1II/IIIp+G: | suspected variable | ||||||
HD 73887 | 73887 | 42286 | 08h 37m 18.85s | −62° 51′ 12.3″ | 5.45 | 0.39 | 335 | K0III | |||||||
HD 82350 | 82350 | 46358 | 09h 27m 06.50s | −71° 36′ 07.5″ | 5.46 | 1.51 | 201 | K2III | |||||||
HD 83095 | H | 83095 | 46741 | 09h 31m 36.32s | −73° 04′ 51.3″ | 5.46 | −1.47 | 791 | K4III | ||||||
HD 92207 | V370 | 92207 | 52004 | 10h 37m 27.08s | −58° 44′ 00.0″ | 5.47 | −6.52 | 8150 | A0Ia | α Cyg variable, Vmax = 5.45m, Vmin = 5.52m, P = 1.33 d | |||||
V450 Car | V450 | 53921 | 34000 | 07h 03m 15.11s | −59° 10′ 41.3″ | 5.50 | −0.35 | 482 | B9IV | 53 Per variable, ΔV = 0.02m | |||||
HD 92664 | V364 | 92664 | 52221 | 10h 40m 11.46s | −65° 06′ 00.9″ | 5.51 | −0.26 | 466 | B9p Si | α2 CVn variable, Vmax = 5.48m, Vmin = 5.52m, P = 1.67 d | |||||
HD 67364 | 67364 | 39566 | 08h 05m 03.71s | −53° 06′ 28.5″ | 5.52 | 0.11 | 393 | K3/K4III | |||||||
HD 79698 | 79698 | 45219 | 09h 12m 55.62s | −59° 24′ 50.3″ | 5.54 | −0.28 | 475 | G6II | |||||||
HD 85656 | 85656 | 48310 | 09h 50m 55.60s | −62° 44′ 42.5″ | 5.56 | −1.78 | 959 | K1IIICN... | |||||||
HD 64067 | 64067 | 38152 | 07h 49m 06.72s | −56° 24′ 37.4″ | 5.57 | −1.72 | 934 | G5II | |||||||
HD 46569 | 46569 | 31079 | 06h 31m 18.22s | −51° 49′ 34.3″ | 5.58 | 2.73 | 121 | F8V | |||||||
HD 96706 | 96706 | 54327 | 11h 06m 49.93s | −70° 52′ 40.6″ | 5.58 | −2.12 | 1128 | B2V | variable star, ΔV = 0.004m, P = 1.74 d | ||||||
HD 65907 | 65907 | 38908 | 07h 57m 46.30s | −60° 18′ 12.1″ | 5.59 | 4.54 | 53 | G2V... | |||||||
HD 76113 | 76113 | 43499 | 08h 51m 36.53s | −57° 38′ 01.0″ | 5.59 | −1.12 | 716 | B8III | |||||||
V448 Car | O | V448 | 49877 | 32531 | 06h 47m 18.71s | −55° 32′ 24.2″ | 5.60 | −0.72 | 598 | K5III | semiregular variable | ||||
HD 65273 | 65273 | 38656 | 07h 54m 53.39s | −57° 18′ 10.4″ | 5.62 | 0.51 | 343 | K3/K4III | |||||||
HD 68434 | 68434 | 39957 | 08h 09m 33.63s | −56° 05′ 07.7″ | 5.66 | 0.33 | 380 | A3m... | |||||||
HD 89715 | 89715 | 50520 | 10h 19m 05.12s | −64° 40′ 34.6″ | 5.66 | 0.90 | 292 | A1V | |||||||
V372 Car | V372 | 64722 | 38438 | 07h 52m 29.75s | −54° 22′ 01.9″ | 5.69 | −2.56 | 1462 | B1.5IV | β Cep variable, ΔV = 0.027m, P = 0.12 d | |||||
HD 88661 | QY | 88661 | 49934 | 10h 11m 46.47s | −58° 03′ 38.0″ | 5.70 | −2.29 | 1294 | B2IVnpe | γ Cas variable, Vmax = 5.63m, Vmin = 5.83m | |||||
S Car | S | 88366 | 49751 | 10h 09m 22.01s | −61° 32′ 57.1″ | 5.71 | 1780 | K5-M6e | Mira variable, Vmax = 4.5m, Vmin = 9.9m, P = 149.49 d | ||||||
HD 97670 | 97670 | 54829 | 11h 13m 30.79s | −59° 37′ 09.5″ | 5.73 | −3.00 | 1821 | B1.5V | suspected variable | ||||||
HD 65662 | 65662 | 38783 | 07h 56m 18.65s | −60° 31′ 35.3″ | 5.74 | −2.17 | 1244 | K4II | in NGC 2516 | ||||||
HD 93163 | 93163 | 52487 | 10h 43m 51.21s | −64° 14′ 56.6″ | 5.75 | −1.71 | 1009 | B3:V | suspected eclipsing binary, ΔV = 0.03m | ||||||
HD 66194 | V374 | 66194 | 38994 | 07h 58m 50.56s | −60° 49′ 28.2″ | 5.77 | −1.72 | 1028 | B2IVnpe | in NGC 2516; γ Cas variable, Vmax = 5.72m, Vmin = 5.84m | |||||
HD 81830 | 81830 | 46225 | 09h 25m 27.38s | −61° 57′ 02.2″ | 5.77 | 1.47 | 236 | A4V+... | |||||||
HD 64185 | 64185 | 38160 | 07h 49m 12.95s | −60° 17′ 02.5″ | 5.78 | 3.06 | 114 | F1V | spectroscopic binary | ||||||
HD 76538 | 76538 | 43669 | 08h 53m 48.67s | −60° 21′ 14.2″ | 5.78 | −2.35 | 1376 | B5III | |||||||
HD 85655 | 85655 | 48339 | 09h 51m 12.03s | −59° 25′ 32.4″ | 5.79 | −1.01 | 746 | K2IIICNp... | |||||||
HD 77615 | 77615 | 44256 | 09h 00m 45.75s | −60° 57′ 49.8″ | 5.80 | −2.13 | 1259 | G8II | |||||||
HD 84152 | 84152 | 47498 | 09h 41m 02.10s | −57° 15′ 34.0″ | 5.80 | 0.57 | 362 | K0/K1III | |||||||
HD 88473 | 88473 | 49764 | 10h 09m 30.20s | −68° 40′ 58.2″ | 5.80 | −0.46 | 583 | A0IV | |||||||
HD 49517 | 49517 | 32402 | 06h 45m 53.72s | −52° 24′ 35.0″ | 5.81 | −2.32 | 1376 | K3III | |||||||
HD 93943 | 93943 | 52922 | 10h 49m 24.46s | −59° 19′ 25.6″ | 5.85 | −1.24 | 853 | B9.5IV/V | |||||||
HD 80950 | 80950 | 45585 | 09h 17m 27.63s | −74° 44′ 04.8″ | 5.86 | 1.32 | 264 | A0V | |||||||
HD 60060 | 60060 | 36444 | 07h 29m 59.74s | −52° 39′ 04.6″ | 5.87 | 0.84 | 330 | K0III | |||||||
HD 66441 | 66441 | 39184 | 08h 00m 49.96s | −54° 09′ 04.7″ | 5.87 | −0.79 | 700 | B5Vn | suspected variable | ||||||
V482 Car | V482 | 82536 | 46620 | 09h 30m 23.45s | −58° 21′ 42.9″ | 5.88 | −1.68 | 1058 | M2III | semiregular variable | |||||
V514 Car | V514 | 92287 | 52043 | 10h 38m 02.66s | −57° 15′ 22.7″ | 5.89 | −2.08 | 1278 | B3IV | rotating ellipsoidal variable, Vmax = 5.88m, Vmin = 5.92m, P = 2.90 d | |||||
HD 82406 | 82406 | 46460 | 09h 28m 30.60s | −66° 42′ 07.2″ | 5.90 | 1.33 | 268 | A0V | |||||||
HD 82347 | 82347 | 46482 | 09h 28m 47.19s | −62° 16′ 23.5″ | 5.91 | 0.06 | 482 | K1III | |||||||
HD 87283 | 87283 | 49164 | 10h 02m 00.11s | −60° 25′ 15.2″ | 5.93 | −4.03 | 3196 | A9IV | possibly in NGC 3114 | ||||||
HD 90454 | 90454 | 50993 | 10h 24m 59.50s | −58° 34′ 34.7″ | 5.93 | 1.13 | 297 | F2III | |||||||
T Car | T | 94776 | 53394 | 10h 55m 17.26s | −60° 31′ 01.9″ | 5.93 | 1.07 | 306 | K0III | not variable | |||||
HD 60228 | 60228 | 36496 | 07h 30m 30.91s | −54° 23′ 58.0″ | 5.95 | 0.33 | 433 | M1III | |||||||
HD 94683 | 94683 | 53334 | 10h 54m 29.60s | −61° 49′ 35.8″ | 5.95 | −2.59 | 1663 | K4III | suspected variable | ||||||
HD 54732 | 54732 | 34349 | 07h 07m 13.30s | −51° 58′ 06.2″ | 5.96 | −0.23 | 564 | K0III | |||||||
HD 56705 | 56705 | 35084 | 07h 15m 21.27s | −52° 29′ 58.3″ | 5.96 | 0.58 | 389 | K0V | |||||||
HD 70839 | 70839 | 40932 | 08h 21m 12.10s | −57° 58′ 23.6″ | 5.96 | −3.36 | 2380 | B1.5III | |||||||
HD 92436 | 92436 | 52127 | 10h 38m 59.70s | −58° 49′ 00.8″ | 5.96 | −0.53 | 648 | M1III | |||||||
HD 91533 | 91533 | 51623 | 10h 32m 47.82s | −58° 40′ 00.3″ | 5.98 | −6.71 | 11241 | A2Iab | suspected variable | ||||||
V522 Car | V522 | 93737 | 52827 | 10h 48m 05.42s | −59° 55′ 09.0″ | 5.98 | A0Ia | α Cyg variable | |||||||
HD 81613 | 81613 | 46101 | 09h 24m 05.50s | −61° 38′ 55.6″ | 5.99 | 0.92 | 337 | K0III | |||||||
HD 94650 | 94650 | 53272 | 10h 53m 42.13s | −70° 43′ 13.2″ | 5.99 | −0.89 | 776 | B6V | |||||||
HD 98560 | 98560 | 55280 | 11h 19m 16.84s | −64° 34′ 57.4″ | 5.99 | 3.12 | 122 | F6IV | |||||||
HD 90874 | 90874 | 51194 | 10h 27m 25.40s | −65° 42′ 17.0″ | 6.00 | 1.76 | 229 | A2V | |||||||
HD 53349 | 53349 | 33800 | 07h 01m 05.18s | −58° 56′ 25.1″ | 6.01 | 2.36 | 175 | F0V | suspected variable | ||||||
HD 76346 | 76346 | 43620 | 08h 53m 03.80s | −56° 38′ 58.5″ | 6.02 | 1.23 | 296 | A0V | has a planet (b) | ||||||
HD 80094 | 80094 | 45418 | 09h 15m 17.66s | −58° 23′ 18.2″ | 6.02 | 0.00 | 522 | B7IV | variable star, ΔV = 0.008m, P = 1.56 d | ||||||
HD 56239 | 56239 | 34780 | 07h 12m 01.98s | −63° 11′ 24.2″ | 6.03 | −0.29 | 598 | A0IV/V | |||||||
HD 57852 | 57852 | 35564 | 07h 20m 21.46s | −52° 18′ 42.8″ | 6.05 | 113 | F5V | component of the HIP 35564 system; suspected variable | |||||||
HD 82068 | 82068 | 46328 | 09h 26m 44.18s | −64° 55′ 47.5″ | 6.05 | 1.88 | 223 | A3Vn | |||||||
V390 Car | V390 | 61966 | 37248 | 07h 39m 00.34s | −53° 16′ 24.2″ | 6.06 | −0.05 | 544 | B9IV-Vp... | α2 CVn variable, ΔV = 0.004m | |||||
V535 Car | V535 | 98292 | 55140 | 11h 17m 19.02s | −67° 49′ 24.6″ | 6.06 | −2.52 | 1698 | M2III | slow irregular variable | |||||
HD 88825 | 88825 | 50044 | 10h 13m 01.16s | −59° 55′ 05.1″ | 6.07 | −2.84 | 1976 | B4Ve | |||||||
HD 96544 | 96544 | 54294 | 11h 06m 29.30s | −58° 40′ 30.1″ | 6.07 | −1.81 | 1226 | K2II/III | |||||||
HD 92682 | 92682 | 52150 | 10h 39m 15.94s | −74° 29′ 36.2″ | 6.08 | −1.57 | 1105 | K3II | variable star, ΔV = 0.005m, P = 0.084 d | ||||||
HD 63382 | 63382 | 37854 | 07h 45m 35.52s | −56° 43′ 21.3″ | 6.10 | −1.20 | 942 | F0II | |||||||
R Car | R | 82901 | 46806 | 09h 32m 14.60s | −62° 47′ 20.0″ | 6.10 | 416 | M6.5 IIIpev | Mira variable, Vmax = 3.9m, Vmin = 10.5m, P = 308.71 d | ||||||
HD 91619 | V369 | 91619 | 51676 | 10h 33m 25.40s | −58° 11′ 24.6″ | 6.11 | −6.99 | 13583 | B7Ia | α Cyg variable, ΔV = 0.1m, P = 1.12 d | |||||
U Car | U | 95109 | 53589 | 10h 57m 48.19s | −59° 43′ 55.9″ | 6.11 | G3Ia | classical Cepheid, Vmax = 5.74m, Vmin = 6.96m, P = 38.83 d | |||||||
HD 70982 | 70982 | 40926 | 08h 21m 07.65s | −64° 06′ 21.4″ | 6.11 | 0.34 | 464 | G6/G8III | |||||||
V461 Car | V461 | 66546 | 39225 | 08h 01m 23.05s | −54° 30′ 56.0″ | 6.12 | −1.92 | 1320 | B2IV-V | Algol variable | |||||
HD 65908 | 65908 | 38863 | 07h 57m 12.76s | −63° 17′ 48.8″ | 6.14 | 0.37 | 464 | B8V | |||||||
V478 Car | V478 | 80710 | 45615 | 09h 17m 51.67s | −67° 03′ 03.2″ | 6.14 | −1.96 | 1358 | K2III | semiregular variable | |||||
HD 87543 | 87543 | 49281 | 10h 03m 34.14s | −61° 53′ 02.6″ | 6.14 | −2.49 | 1734 | B4:Vne | |||||||
HD 95208 | 95208 | 53546 | 10h 57m 15.81s | −75° 05′ 59.2″ | 6.16 | −3.12 | 2345 | K1II | |||||||
HD 95324 | 95324 | 53701 | 10h 59m 14.05s | −61° 19′ 14.7″ | 6.16 | 0.93 | 363 | B8IV | |||||||
HD 96088 | 96088 | 54082 | 11h 04m 00.25s | −57° 57′ 19.2″ | 6.16 | −3.63 | 2964 | B3III | |||||||
HD 47001 | 47001 | 31265 | 06h 33m 26.31s | −52° 19′ 45.5″ | 6.18 | −0.17 | 607 | G8III | |||||||
V492 Car | V492 | 86659 | 48782 | 09h 56m 59.84s | −69° 06′ 06.6″ | 6.18 | −1.43 | 1087 | B3V | 53 Per variable | |||||
HD 87436 | 87436 | 49233 | 10h 02m 59.95s | −60° 10′ 43.3″ | 6.18 | −3.80 | 3228 | A6II/III | suspected variable | ||||||
HD 90630 | 90630 | 50976 | 10h 24m 44.56s | −73° 58′ 18.3″ | 6.18 | 0.53 | 441 | A2/A3V | suspected variable | ||||||
V655 Car | V655 | 91272 | 51425 | 10h 30m 08.81s | −66° 59′ 04.8″ | 6.19 | −1.70 | 1235 | B4IV | Algol variable, Vmax = 6.19m, Vmin = 6.36m, P = 16.93 d | |||||
HD 62897 | 62897 | 37599 | 07h 42m 53.36s | −58° 13′ 48.5″ | 6.20 | −0.23 | 629 | K0III | |||||||
HD 75086 | 75086 | 42936 | 08h 45m 05.55s | −58° 43′ 27.6″ | 6.20 | −1.23 | 997 | B7III | |||||||
HD 87238 | 87238 | 49160 | 10h 01m 58.09s | −57° 20′ 59.4″ | 6.20 | −0.62 | 753 | K1II | |||||||
HD 84850 | 84850 | 47913 | 09h 45m 55.82s | −58° 47′ 38.4″ | 6.22 | 1.68 | 264 | F5IV | |||||||
HD 89263 | 89263 | 50287 | 10h 16m 03.26s | −59° 54′ 12.4″ | 6.22 | 1.63 | 270 | A5V | |||||||
V532 Car | V532 | 97451 | 54708 | 11h 12m 03.60s | −58° 25′ 24.1″ | 6.24 | −0.53 | 736 | M4III | semiregular variable | |||||
HD 91767 | 91767 | 51732 | 10h 34m 12.72s | −60° 59′ 15.5″ | 6.25 | −0.78 | 830 | K2/K3III | suspected variable | ||||||
HD 65750 | V341 | 65750 | 38834 | 07h 56m 50.70s | −59° 07′ 35.0″ | 6.25 | 967 | M0III | semiregular variable, Vmax = 6.2m, Vmin = 7.1m | ||||||
HD 93344 | 93344 | 52520 | 10h 44m 20.10s | −70° 51′ 35.0″ | 6.25 | 1.12 | 346 | A5IV/V | |||||||
HD 52603 | 52603 | 33588 | 06h 58m 39.81s | −55° 43′ 44.1″ | 6.26 | 1.59 | 280 | K2III | |||||||
HD 74622 | 74622 | 42717 | 08h 42m 20.90s | −55° 46′ 28.8″ | 6.26 | 1.23 | 331 | K2III | |||||||
υ Car B | υ | 85124 | 09h 47m 06.70s | −65° 04′ 21.0″ | 6.26 | 1623 | A8 Ib | component of the υ Car system | |||||||
HD 93372 | 93372 | 52535 | 10h 44m 27.25s | −72° 26′ 37.1″ | 6.26 | 3.74 | 104 | F6V | |||||||
HD 93502 | 93502 | 52679 | 10h 46m 17.12s | −60° 36′ 10.4″ | 6.26 | 1.01 | 365 | A0IV | |||||||
HD 94491 | 94491 | 53231 | 10h 53m 21.18s | −58° 53′ 36.5″ | 6.26 | −2.16 | 1575 | B5V | |||||||
HD 82858 | 82858 | 46737 | 09h 31m 33.05s | −66° 43′ 08.6″ | 6.27 | −0.40 | 703 | K1III | |||||||
HD 66607 | 66607 | 39238 | 08h 01m 31.58s | −55° 27′ 16.8″ | 6.28 | −0.28 | 668 | B4V | |||||||
V375 Car | V375 | 67536 | 39530 | 08h 04m 42.94s | −62° 50′ 10.9″ | 6.29 | 1249 | B2.5Vn | β Cep variable, ΔV = 0.04m, P = 1.02 d | ||||||
HD 61031 | 61031 | 36856 | 07h 34m 39.58s | −51° 28′ 28.3″ | 6.29 | −1.76 | 1331 | A1III/IV | |||||||
HD 93662 | 93662 | 52797 | 10h 47m 38.41s | −57° 28′ 02.7″ | 6.29 | −3.35 | 2763 | M1II | suspected variable, Vmax = 6.28m, Vmin = 6.41m | ||||||
HD 94275 | 94275 | 53100 | 10h 51m 46.93s | −57° 16′ 20.3″ | 6.29 | −0.05 | 604 | A6III | |||||||
HD 63926 | 63926 | 38087 | 07h 48m 19.51s | −56° 28′ 15.9″ | 6.30 | −2.91 | 2264 | K0III+... | |||||||
HD 66341 | 66341 | 39073 | 07h 59m 40.09s | −60° 12′ 26.6″ | 6.30 | −1.81 | 1364 | B8III | in NGC 2516 | ||||||
HD 81502 | 81502 | 46049 | 09h 23m 27.33s | −60° 18′ 08.4″ | 6.30 | −2.91 | 2264 | K1/K2II/III | |||||||
HD 86606 | 86606 | 48715 | 09h 56m 09.76s | −71° 23′ 21.5″ | 6.30 | −2.69 | 2050 | B1Ib | |||||||
HD 68423 | 68423 | 39843 | 08h 08m 24.65s | −63° 48′ 03.0″ | 6.32 | −0.58 | 782 | B6V | suspected variable | ||||||
HD 80126 | 80126 | 45437 | 09h 15m 34.73s | −57° 34′ 39.9″ | 6.32 | −1.32 | 1098 | G8II | |||||||
QZ Car | QZ | 93206 | 52526 | 10h 44m 22.92s | −59° 59′ 36.0″ | 6.32 | −3.23 | 2650 | B0Ib: | in Collinder 228; β Lyr variable, Vmax = 6.16m, Vmin = 6.49m, P = 6.00 d | |||||
HD 82458 | 82458 | 46407 | 09h 27m 49.19s | −71° 46′ 52.3″ | 6.33 | 2.57 | 184 | F3/F5V | |||||||
V486 Car | V486 | 84416 | 47591 | 09h 42m 12.99s | −66° 54′ 53.4″ | 6.33 | 0.04 | 592 | A0V | β Lyr variable | |||||
HD 92536 | 92536 | 52160 | 10h 39m 22.85s | −64° 06′ 42.5″ | 6.33 | 0.49 | 479 | B8V | in IC 2602 | ||||||
HD 74341 | 74341 | 42579 | 08h 40m 43.55s | −57° 32′ 43.9″ | 6.34 | 2.13 | 227 | A3V | |||||||
HD 90074 | 90074 | 50785 | 10h 22m 10.48s | −58° 15′ 56.3″ | 6.34 | 1.23 | 343 | G6III | |||||||
HD 90289 | 90289 | 50916 | 10h 23m 50.66s | −57° 57′ 14.1″ | 6.34 | −0.59 | 793 | K5Ib-II | suspected variable, Vmax = 6.33m, Vmin = 6.35m | ||||||
HD 93649 | 93649 | 52730 | 10h 46m 48.09s | −69° 12′ 35.3″ | 6.34 | −2.04 | 1545 | A2IV | |||||||
HD 97472 | 97472 | 54673 | 11h 11m 29.57s | −71° 26′ 10.3″ | 6.34 | 0.08 | 583 | K2/K3III | |||||||
HD 74148 | 74148 | 42440 | 08h 39m 13.24s | −60° 19′ 02.4″ | 6.35 | 0.71 | 437 | A0V | |||||||
HD 89805 | 89805 | 50562 | 10h 19m 42.04s | −65° 08′ 14.1″ | 6.35 | −2.59 | 2000 | K2II | |||||||
WR 22 | V429 | 92740 | 52308 | 10h 41m 17.52s | −59° 40′ 36.9″ | 6.35 | −4.72 | 5344 | WN7 + A(SB1) | Wolf–Rayet star and Algol variable, Vmax = 6.33m, Vmin = 6.52m, P = 80.34 d; one of the most luminous stars known | |||||
HD 93739 | 93739 | 52785 | 10h 47m 30.62s | −69° 26′ 15.8″ | 6.35 | −1.57 | 1249 | B2IV | |||||||
HD 65189 | 65189 | 38667 | 07h 55m 00.44s | −52° 35′ 00.1″ | 6.36 | −1.08 | 1003 | B8III | |||||||
HD 72322 | 72322 | 41653 | 08h 29m 36.40s | −55° 11′ 27.3″ | 6.36 | −0.36 | 721 | G0V | |||||||
V473 Car | V473 | 76640 | 43763 | 08h 54m 54.05s | −58° 14′ 22.9″ | 6.36 | −0.77 | 869 | B5V | 53 Per variable | |||||
HD 79699 | 79699 | 45214 | 09h 12m 50.63s | −60° 55′ 00.5″ | 6.36 | 0.21 | 553 | B9V | |||||||
HD 78632 | 78632 | 44665 | 09h 06m 07.61s | −64° 29′ 59.7″ | 6.37 | 0.08 | 590 | K3III | |||||||
HD 61394 | 61394 | 36977 | 07h 36m 01.62s | −55° 53′ 15.8″ | 6.39 | 0.06 | 601 | K1/K2IIICN. | |||||||
HD 96568 | 96568 | 54289 | 11h 06m 24.32s | −64° 50′ 23.8″ | 6.39 | 0.58 | 473 | A3V | |||||||
HD 44267 | 44267 | 29913 | 06h 17m 51.74s | −52° 43′ 58.9″ | 6.40 | −0.70 | 858 | K2/K3III | variable star, ΔV = 0.008m, P = 1.32 d | ||||||
HD 62758 | 62758 | 37530 | 07h 42m 10.22s | −58° 37′ 51.4″ | 6.40 | −1.18 | 1069 | B2.5V | |||||||
V368 Car | V368 | 88647 | 49926 | 10h 11m 35.49s | −58° 49′ 40.2″ | 6.40 | 801 | M3III | semiregular variable, Vmax = 6.1m, Vmin = 6.4m | ||||||
HD 51210 | 51210 | 33012 | 06h 52m 45.44s | −59° 20′ 28.6″ | 6.41 | 0.62 | 470 | A3m... | |||||||
HD 87438 | 87438 | 49223 | 10h 02m 49.42s | −62° 09′ 24.0″ | 6.41 | −3.23 | 2763 | K3Ib | irregular variable, Vmax = 6.38m, Vmin = 6.43m | ||||||
HD 91270 | 91270 | 51461 | 10h 30m 39.24s | −61° 21′ 23.4″ | 6.41 | −0.57 | 811 | M2III | suspected variable | ||||||
HD 84046 | 84046 | 47422 | 09h 39m 45.15s | −62° 56′ 34.7″ | 6.42 | 0.01 | 623 | B8/B9III/IVw... | suspected variable, Vmax = 6.42m, Vmin = 6.8m | ||||||
HD 88907 | 88907 | 50067 | 10h 13m 21.20s | −61° 39′ 31.8″ | 6.42 | −1.06 | 1022 | B2V | |||||||
V507 Car | V507 | 90966 | 51265 | 10h 28m 18.28s | −63° 09′ 52.5″ | 6.42 | −2.56 | 2037 | B2/B3III:ne | Be star | |||||
HD 91094 | 91094 | 51327 | 10h 29m 03.67s | −65° 10′ 34.8″ | 6.42 | 0.00 | 627 | M1III | semiregular variable | ||||||
HD 98025 | 98025 | 55003 | 11h 15m 42.76s | −57° 21′ 21.1″ | 6.42 | 0.16 | 583 | A3V | |||||||
HD 78293 | 78293 | 44565 | 09h 04m 48.00s | −57° 51′ 09.5″ | 6.43 | −1.21 | 1101 | A8III | |||||||
HD 93359 | 93359 | 52537 | 10h 44m 32.42s | −70° 51′ 18.9″ | 6.43 | 1.25 | 354 | A6IV | |||||||
HD 65867 | 65867 | 38963 | 07h 58m 21.47s | −51° 26′ 54.9″ | 6.44 | 0.43 | 518 | A8/A9IV | suspected eclipsing binary | ||||||
V469 Car | V469 | 72303 | 41644 | 08h 29m 29.82s | −54° 12′ 42.5″ | 6.44 | −0.28 | 720 | Ap Si | α2 CVn variable | |||||
HD 49705 | 49705 | 32477 | 06h 46m 41.70s | −54° 41′ 42.2″ | 6.45 | 0.93 | 414 | G6III | |||||||
HD 81896 | 81896 | 46143 | 09h 24m 37.16s | −70° 04′ 32.8″ | 6.45 | 0.06 | 617 | K1III | |||||||
V495 Car | V495 | 88158 | 49642 | 10h 07m 56.64s | −62° 13′ 17.2″ | 6.45 | −0.55 | 817 | Ap Si | α2 CVn variable | |||||
WR 24 | 93131 | 52488 | 10h 43m 52.27s | −60° 07′ 04.0″ | 6.46 | −5.05 | 6520 | WN7 + A | in Collinder 228; Wolf–Rayet star, Vmax = 6.46m, Vmin = 6.49m, P = 4.76 d; one of the most luminous stars known | ||||||
HD 52622 | 52622 | 33577 | 06h 58m 36.39s | −56° 23′ 41.2″ | 6.46 | 1.46 | 326 | F2II | suspected variable | ||||||
HD 54967 | 54967 | 34350 | 07h 07m 16.28s | −59° 42′ 59.2″ | 6.46 | −1.79 | 1455 | B3V | |||||||
HD 93738 | 93738 | 52815 | 10h 47m 53.55s | −64° 15′ 46.3″ | 6.46 | 0.67 | 469 | B9.5V | in IC 2602 | ||||||
HD 49219 | 49219 | 32269 | 06h 44m 12.81s | −54° 41′ 43.9″ | 6.47 | −0.30 | 736 | B5/B6V | variable star, ΔV = 0.011m, P = 1.60 d | ||||||
HD 70267 | 70267 | 40655 | 08h 17m 55.79s | −59° 10′ 00.3″ | 6.47 | 2.01 | 254 | F5V | |||||||
V487 Car | V487 | 84809 | 47893 | 09h 45m 40.64s | −57° 11′ 09.8″ | 6.47 | −0.66 | 869 | B8III/IV | α2 CVn variable | |||||
HD 93695 | 93695 | 52806 | 10h 47m 44.34s | −59° 52′ 30.9″ | 6.47 | −1.41 | 1230 | B5Vvar | |||||||
HD 95122 | 95122 | 53556 | 10h 57m 20.22s | −69° 02′ 17.0″ | 6.48 | −0.55 | 832 | B7V | suspected variable | ||||||
HD 92399 | 92399 | 52103 | 10h 38m 45.39s | −59° 15′ 44.7″ | 6.50 | −1.82 | 1502 | B4/B5III/IV | |||||||
HD 96248 | V414 | 96248 | 54179 | 11h 04m 57.57s | −59° 51′ 32.0″ | 6.58 | 3700 | B1Iab | α Cyg variable, Vmax = 6.53m, Vmin = 6.62m, P = 8.52 d | ||||||
HD 57853 | 57853 | 35564 | 07h 20m 21.43s | −52° 18′ 31.91″ | 6.63 | 113 | F9V | component of the HIP 35564 system | |||||||
QX Car | QX | 86118 | 48589 | 09h 54m 33.88s | −58° 25′ 16.6″ | 6.64 | 1610 | B2V | Algol variable, Vmax = 6.6m, Vmin = 7.21m, P = 4.48 d | ||||||
HD 96446 | V430 | 96446 | 54266 | 11h 06m 05.82s | −59° 56′ 59.6″ | 6.68 | 1540 | B2k | β Cep variable, ΔV = 0.03m | ||||||
HD 53143 | 53143 | 33690 | 06h 59m 59.66s | −61° 20′ 10.3″ | 6.68 | 59.74 | G9V | has a circumstellar disk | |||||||
VY Car | VY | 93203 | 52538 | 10h 44m 32.69s | −57° 33′ 55.3″ | 6.91 | 9100 | F7Iab/Ib | classical Cepheid, Vmax = 6.91m, Vmin = 8.00m, P = 18.89 d | ||||||
AG Car | AG | 94910 | 53461 | 10h 56m 11.58s | −60° 27′ 12.8″ | 6.96 | 17000 | B2-3Ib/WN11 | luminous blue variable, Vmax = 5.7m, Vmin = 8.3m, P = 371.4 d | ||||||
BO Car | BO | 93420 | 10h 45m 50.63s | −59° 29′ 19.5″ | 7.18 | M4Iab: | semiregular variable, Vmax = 7.15m, Vmin = 7.95m, P = 130.7 d | ||||||||
HD 93403 | 93403 | 52628 | 10h 45m 44.12s | −59° 24′ 28.1″ | 7.30 | 2670 | O5.5I+O7V | binary star | |||||||
HD 93129A | 93129A | 10h 43m 57.46s | −59° 32′ 51.2″ | 7.31 | 7500 | O2If*+O3.5 | in Trumpler 14; binary star; primary is one of the most luminous stars known | ||||||||
V Car | V | 72275 | 41588 | 08h 28m 43.70s | −60° 07′ 21.3″ | 7.31 | 5600 | G2Iab: | classical Cepheid, Vmax = 7.08m, Vmin = 7.82m, P = 6.70 d | ||||||
HD 93843 | 93843 | 10h 48m 37.78s | −60° 13′ 25.5″ | 7.33 | O5III(f)v | irregular variable, Vmax = 7.31m, Vmin = 7.35m | |||||||||
HD 95086 | 95086 | 53524 | 10h 57m 03.0s | −68° 40′ 02″ | 7.36 | 295 | A8III | has a planet (b) | |||||||
HD 93250 | 93250 | 52558 | 10h 44m 45.03s | −59° 33′ 54.7″ | 7.50 | 7500 | O4IIIfc | in Trumpler 16; suspected variable | |||||||
HR Car | HR | 90177 | 50843 | 10h 22m 53.84s | −59° 37′ 28.4″ | 7.57 | 17700 | B3Iaep | luminous blue variable, Vmax = 6.8m, Vmin = 8.80m | ||||||
WR 40 | V385 | 96548 | 54283 | 11h 06m 17.20s | −65° 30′ 35.2″ | 7.70 | 5900 | WN8h | Wolf–Rayet star and rotating ellipsoidal variable, ΔV = 0.04m, P = 4.76 d; one of the most luminous stars known | ||||||
HD 93205 | V560 | 93205 | 10h 44m 33.74s | −59° 44′ 15.5″ | 7.75 | 7500 | O3.5V((f+)) | in Trumpler 16; rotating ellipsoidal variable, Vmax = 7.74m, Vmin = 7.76m, P = 6.08 d | |||||||
IW Car | IW | 82084 82085 | 09h 26m 53.30s | −63° 37′ 48.9″ | 7.90 | A4Iab/II: | RV Tau variable, Vmax = 7.77m, Vmin = 9.10m, P = 143.6 d | ||||||||
HD 65216 | 65216 | 38558 | 07h 53m 41.3s | −63° 38′ 50.4″ | 7.98 | 112 | G5V | has two planets (b & c) | |||||||
HD 97152 | V431 | 97152 | 54574 | 11h 10m 04.08s | −60° 58′ 45.0″ | 8.07 | 4000 | WC7+O7V | Wolf–Rayet star; eclipsing binary, Vmax = 7.97m, Vmin = 8.08m, P = 1.62 d | ||||||
HD 63765 | 63765 | 38041 | 07h 47m 49.72s | −54° 15′ 50.9″ | 8.10 | 5.53 | 106 | G9V | Tapecue; has a planet (b) | ||||||
Y Car | Y | 91565 | 51653 | 10h 33m 10.85s | −58° 29′ 55.1″ | 8.16 | 3050 | F2 | double-mode Cepheid, Vmax = 7.53m, Vmin = 8.48m, P = 3.64 d | ||||||
HD 51608 | 51608 | 33229 | 06h 54m 51s | −55° 15′ 34″ | 8.17 | 114 | K0IV | has two planets (b & c) | |||||||
HD 85628 A | 85628 | 09h 50m 19.2s | −66° 06′ 50″ | 8.19 | 559 | A3V | has a planet (b) | ||||||||
YZ Car | YZ | 90912 | 51262 | 10h 28m 16.85s | −59° 21′ 00.7″ | 8.24 | 5900 | G5 | classical Cepheid, Vmax = 8.24m, Vmin = 9.08m, P = 18.17 d | ||||||
WR 16 | V396 | 86161 | 48617 | 09h 54m 52.90s | −57° 43′ 38.3″ | 8.32 | WN8h | rotating ellipsoidal variable, ΔV = 0.06m; one of the most luminous stars known | |||||||
EM Car | EM | 97484 | 11h 12m 04.51s | −61° 05′ 42.9″ | 8.52 | O8V | Algol variable | ||||||||
RT Car | RT | 303310 | 52562 | 10h 44m 47.15s | −59° 24′ 48.1″ | 8.55 | 1430 | M2Iab: | possibly in Trumpler 15; irregular variable, Vmax = 8.2m, Vmin = 9.9m, one of the largest stars known | ||||||
HD 85567 | V596 | 85567 | 48269 | 09h 50m 28.54s | −60° 58′ 03.0″ | 8.57 | 6900 | B2 | FS CMa variable, Vmax = 8.44m, Vmin = 8.75m | ||||||
UX Car | UX | 91039 | 51338 | 10h 29m 11.24s | −57° 36′ 48.3″ | 8.62 | 2530 | F2II | classical Cepheid, Vmax = 7.81m, Vmin = 8.67m, P = 3.68 d | ||||||
XZ Car | XZ | 305996 | 54101 | 11h 04m 13.47s | −60° 58′ 47.7″ | 8.67 | B2:pe | classical Cepheid, Vmax = 8.05m, Vmin = 9.12m, P = 16.65 d | |||||||
GG Car | GG | 94878 | 53444 | 10h 55m 58.92s | −60° 23′ 33.4″ | 8.70 | B0/2eq | Be star and re-radiating binary system, Vmax = 8.44m, Vmin = 9.08m, P = 31.03 d | |||||||
V403 Car | V403 | 10h 35m 40.67s | −58° 12′ 44.6″ | 8.74 | 8400 | B1III | in NGC 3293; β Cep variable, ΔV = 0.033m, P = 0.25 d | ||||||||
Tr 16-104 | V572 | 10h 44m 47.31s | −59° 43′ 53.2″ | 8.75 | 7500 | O7V((f))+ O9.5V+ B0.2IV | in Trumpler 16; Algol variable, Vmax = 8.66m, Vmin = 9.07m, P = 2.15 d | ||||||||
V348 Car | V348 | 90707 | 10h 29m 59.00s | −57° 40′ 32.8″ | 8.78 | B1III | β Lyr variable, Vmax = 8.55m, Vmin = 8.93m, P = 5.56 d | ||||||||
WR 25 | 93162 | 10h 44m 10.34s | −59° 43′ 11.4″ | 8.80 | 7500 | O2.5If*/WN6 | in Trumpler 16; Wolf–Rayet star; one of the most luminous stars known | ||||||||
HD 60435 | V409 | 60435 | 36537 | 07h 30m 56.99s | −57° 59′ 28.2″ | 8.89 | 739 | Ap... | rapidly oscillating Ap star | ||||||
WR 23 | 92809 | 52331 | 10h 41m 38.32s | −58° 46′ 18.7″ | 9.03 | 3400 | WC6 | Wolf–Rayet star | |||||||
HD 92024 | V381 | 92024 | 10h 36m 08.31s | −58° 13′ 04.77″ | 9.04 | 8400 | B1III | in NGC 3293; β Cep variable, Vmax = 9.04m, Vmin = 9.06m, P = 0.17 d | |||||||
GH Car | GH | 306077 | 54621 | 11h 10m 44.59s | −60° 45′ 01.0″ | 9.20 | G0 | classical Cepheid, Vmax = 9m, Vmin = 9.35m, P = 5.73 d | |||||||
WZ Car | WZ | 94777 | 53397 | 10h 55m 18.73s | −60° 56′ 24.0″ | 9.37 | 4700 | F8 | classical Cepheid, Vmax = 8.63m, Vmin = 9.88m, P = 23.02 d | ||||||
CPD -59° 2635 | V731 | 10h 45m 12.72s | −59° 44′ 46.2″ | 9.43 | 7500 | O8V+O9.5V | in Trumpler 16; Algol variable, Vmax = 9.27m, Vmin = 9.78m, P = 2.30 d | ||||||||
V392 Car | V392 | 07h 58m 10.47s | −60° 51′ 57.5″ | 9.49 | A2Vp... | in NGC 2516; Algol and α2 CVn variable, Vmax = 9.49m, Vmin = 9.67m | |||||||||
XY Car | XY | 308149 | 53945 | 11h 02m 16.07s | −64° 15′ 46.5″ | 9.49 | G5 | classical Cepheid, Vmax = 8.82m, Vmin = 9.77m, P = 12.43 d | |||||||
HD 87643 | V640 | 87643 | 10h 04m 30.29s | −58° 39′ 52.1″ | 9.50 | B2e | Orion variable, Vmax = 7.4m, Vmin = 9.8m | ||||||||
CPD -59 2628 | V573 | 10h 45m 08.23s | −59° 40′ 49.5″ | 9.52 | 7500 | O9.5V+B0.3V | in Trumpler 16; Algol variable | ||||||||
HD 90657 | V398 | 90657 | 51109 | 10h 26m 31.41s | −58° 38′ 26.2″ | 9.69 | 3500 | WN5+O4-6 | Wolf–Rayet star; eclipsing binary, ΔV = 0.035m | ||||||
GL Car | GL | 306168 | 11h 14m 39.84s | −60° 39′ 36.3″ | 9.70 | B3:V | Algol variable | ||||||||
DW Car | DW | 305543 | 10h 43m 10.07s | −60° 02′ 11.7″ | 9.85 | B2:pe | in Collinder 228; Algol variable | ||||||||
SS73 17 | V648 | 10h 11m 02.95s | −57° 48′ 13.9″ | 9.99 | M3pe+OB | Z And variable, Vmax = 9.6m, Vmin = 10.0m, P = 520 d | |||||||||
CPD -57 2874 | 10h 15m 21.97s | −57° 51′ 42.7″ | 10.16 | sgB1[e] | B[e] star | ||||||||||
GZ Car | GZ | 302719 | 50615 | 10h 20m 20.37s | −59° 22′ 35.8″ | 10.20 | 2400 | G5 | double-mode Cepheid, Vmax = 9.98m, Vmin = 10.47m, P = 4.16 d | ||||||
HH Car | HH | 303503 | 10h 53m 36.47s | −59° 27′ 18.2″ | 10.31 | B | Algol variable, Vmax = 10.3m, Vmin = 10.82m, P = 3.23 d | ||||||||
EY Car | EY | 52380 | 10h 42m 23.03s | −61° 09′ 57.3″ | 10.35 | B2:pe | double-mode Cepheid, Vmax = 10.01m, Vmin = 10.56m, P = 2.88 d | ||||||||
HD 307938 | V557 | 307938 | 10h 42m 41.52s | −64° 21′ 04.4″ | 10.57 | G2V | BY Dra variable, ΔV = 0.21m | ||||||||
WR 18 | V500 | 89358 | 50368 | 10h 17m 02.27s | −57° 54′ 47.9″ | 10.6 | 6300 | WN4-s | Wolf–Rayet star | ||||||
HD 94546 | V428 | 94546 | 53274 | 10h 53m 44.82s | −59° 30′ 46.7″ | 10.7 | WN4+O8V | Wolf–Rayet star; eclipsing binary, ΔV = 0.05m | |||||||
He 3-519 | 10h 53m 59.59s | −60° 26′ 44.3″ | 10.85 | WN11 | Wolf–Rayet star, Vmax = 10.6m, Vmin = 11.0m | ||||||||||
NGC 3603-A1 | 97950A | 11h 15m 07.31s | −61° 15′ 38.4″ | 11.12 | 20000 | WN6ha+O3V | in NGC 3603; Algol variable, ΔV = 0.45m, P = 3.77 d both components among the most luminous and massive stars known | ||||||||
CR Car | CR | 10h 32m 54.07s | −58° 31′ 15.5″ | 11.30 | B2:pe | classical Cepheid, Vmax = 11.3m, Vmin = 11.89m, P = 9.76 d | |||||||||
NGC 3603-B | 97950B | 11h 15m 07.41s | −61° 15′ 38.6″ | 11.33 | WN6h+abs | one of the most luminous and most massive stars known | |||||||||
Innes' star | 11h 16m 00.21s | −57° 32′ 51.6″ | 11.52 | 41.31 | M3.5 | has a planet | |||||||||
QU Car | QU | 310376 | 54226 | 11h 05m 42.49s | −68° 37′ 58.2″ | 11.54 | 1290 | B+... | V Sge variable, Vmax = 10.9m, Vmin = 11.7m, P = 0.45 d | ||||||
WR 30 | V541 | 94305 | 10h 51m 06.01s | −62° 17′ 01.7″ | 11.73 | WC6+O7.5V | Algol variable, ΔV = 0.09m | ||||||||
Wray 15-751 | V432 | 11h 08m 40.06s | −60° 42′ 51.7″ | 11.79 | WR: | luminous blue variable, Vmax = 10.7m, Vmin = 12.43m | |||||||||
NGC 3603-C | 97950C | 11h 15m 07.59s | −61° 15′ 18.0″ | 11.89 | WN6h+abs | spectroscopic binary | |||||||||
FO 15 | V662 | 10h 45m 36.32s | −59° 48′ 23.2″ | 12.09 | 7500 | O5.5V+O9.5V | in Trumpler 16; Algol variable, Vmax = 12.09m, Vmin = 12.7m, P = 1.41 d | ||||||||
Sher 25 | 11h 15m 07.8s | −61° 15′ 17″ | 12.27 | B1.5Iab | in NGC 3603; potential supernova progenitor | ||||||||||
WR 30a | V574 | 10h 51m 38.93s | −60° 56′ 35.2″ | 12.73 | WR+... | Algol variable, ΔV = 0.05m | |||||||||
GJ 1128 | 09h 42m 46.356s | −68° 53′ 06.04″ | 12.78 | M4.0V | |||||||||||
He 2-38 | V366 | 09h 54m 43.29s | −57° 18′ 52.4″ | 12.92 | M5-7.5 | Mira and Z And variable, Vmax = 12.1m, Vmin = 14.4m, P = 433 d | |||||||||
BPM 6502 | V727 | 10h 44m 10.23s | −69° 18′ 18.0″ | 13.09 | DA2.2+M | re-radiating binary system | |||||||||
WR 20a | V712 | 10h 23m 58.00s | −57° 45′ 49.0″ | 13.5 | O3If*/WN6+ O3If*/WN6 | in Westerlund 2; Algol variable | |||||||||
LHS 288 | 10h 44m 21.32s | −61° 12′ 38.4″ | 13.92 | 15.602 | M4 | ||||||||||
OGLE-TR-113 | V752 | 10h 52m 24.4s | −61° 26′ 48.5″ | 14.42 | 1800 | K | has a transiting planet (b) | ||||||||
MTT 68 | 11h 14m 59.50s | −61° 14′ 33.89″ | 14.72 | −6.4 | 25,000 | O2If* | rare O2If* type, along with HD 93129A | ||||||||
2S 0921-630 | V395 | 09h 22m 35.20s | −63° 17′ 38.5″ | 15.3 | K0IIIe | low-mass X-ray binary | |||||||||
OGLE-TR-123 | V816 | 11h 06m 51.1s | −61° 11′ 10.5″ | 15.47 | FV+MV | possibly has a transiting planet | |||||||||
OGLE-TR-111 | V759 | 10h 53m 17.9s | −61° 24′ 20.3″ | 15.55 | 5000 | G | has a transiting planet (b) and a possible second planet | ||||||||
OGLE-TR-132 | V742 | 10h 50m 34.7s | −61° 57′ 25.9″ | 15.72 | 7110 | F | has a transiting planet (b) | ||||||||
OY Car | OY | 10h 06m 22.07s | −70° 14′ 04.6″ | 16.2 | 277 | M5/M6:... | SU UMa variable and eclipsing binary, Vmax = 11.2m, Vmin = 16.2m, P = 0.063 d | ||||||||
OGLE-TR-182 | 11h 09m 18.73s | −61° 05′ 42.93″ | 16.84 | 12700 | G | has a transiting planet (b) | |||||||||
OGLE-TR-211 | 10h 40m 14.39s | −62° 27′ 20.2″ | 5300 | F | has a transiting planet (b) | ||||||||||
OGLE-TR-122 | V817 | 11h 06m 52.0s | −60° 51′ 45.7″ | has a transiting brown dwarf | |||||||||||
OGLE2-TR-L9 | 11h 07m 55s | −61° 08′ 46″ | 2935 | F3 | has a transiting planet (b) | ||||||||||
1E 1048.1-5937 | 10h 50m 08.93s | −59° 53′ 19.9″ | Be | anomalous X-ray pulsar | |||||||||||
DENIS J081730.0-615520 | 08h 17m 30.01s | −61° 55′ 15.8″ | 16.1 | T6 | brown dwarf | ||||||||||
PSR J1048-5832 | 10h 48m 12.20s | −58° 32′ 05.8″ | pulsar | ||||||||||||
PSR J1119-6127 | 11h 19m 14.30s | −61° 27′ 49.5″ | pulsar | ||||||||||||
Table legend:
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: CS1 maint: multiple names: authors list (link)Argo Navis, or simply Argo, is one of Ptolemy's 48 constellations, now a grouping of three IAU constellations. It is formerly a single large constellation in the southern sky. The genitive is "Argus Navis", abbreviated "Arg". Flamsteed and other early modern astronomers called it Navis, genitive "Navis", abbreviated "Nav".
A Bayer designation is a stellar designation in which a specific star is identified by a Greek or Latin letter followed by the genitive form of its parent constellation's Latin name. The original list of Bayer designations contained 1,564 stars. The brighter stars were assigned their first systematic names by the German astronomer Johann Bayer in 1603, in his star atlas Uranometria. Bayer catalogued only a few stars too far south to be seen from Germany, but later astronomers supplemented Bayer's catalog with entries for southern constellations.
Carina is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was the southern foundation of the larger constellation of Argo Navis until it was divided into three pieces, the other two being Puppis, and Vela.
Puppis ("stern") is a constellation in the southern sky. It was originally part of the traditional constellation of Argo Navis, which was divided into three parts, the other two being Carina, and Vela. Puppis is the largest of the three constellations in square degrees. It is one of the 88 modern constellations recognized by the International Astronomical Union.
Vela is a constellation in the southern sky, which contains the Vela Supercluster. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis. With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star Gamma Velorum, one component of which is the closest and brightest Wolf-Rayet star in the sky. Delta and Kappa Velorum, together with Epsilon and Iota Carinae, form the asterism known as the False Cross. 1.95-magnitude Delta is actually a triple or quintuple star system.
In astronomy, a variable-star designation is a unique identifier given to variable stars. It uses a variation on the Bayer designation format, with an identifying label preceding the Latin genitive of the name of the constellation in which the star lies. See List of constellations for a list of constellations and the genitive forms of their names. The identifying label can be one or two Latin letters or a V plus a number. Examples are R Coronae Borealis, YZ Ceti, V603 Aquilae.
Gamma Velorum is a quadruple star system in the constellation Vela. This name is the Bayer designation for the star, which is Latinised from γ Velorum and abbreviated γ Vel. At a combined magnitude of +1.72, it is one of the brightest stars in the night sky, and contains by far the closest and brightest Wolf–Rayet star. It has the traditional name Suhail al Muhlif and the modern name Regor, but neither is approved by the International Astronomical Union, making it the brightest star by apparent magnitude without an IAU approved name.
Omicron Velorum is a star in the constellation Vela. It is the brightest member of the loose naked eye open cluster IC 2391, also known as the ο Velorum Cluster.
V357 Carinae is an astrometric and spectroscopic binary in the constellation Carina. It is approximately 419 light years from Earth. The mean apparent magnitude of the system is +3.43.
V533 Carinae is a A-type supergiant and a Alpha Cygni variable star with a mean apparent magnitude of +4.59 in the constellation Carina. It is located at a distance of about 13,000 light years.
HR 3803 or N Velorum is a 3rd-magnitude star on the border between the southern constellations Carina and Vela. Based upon parallax measurements, it is approximately 223 light-years from Earth.
DL Crucis is a variable star in the constellation Crux.
k Puppis is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis.
Omicron Puppis (ο Puppis) is candidate binary star system in the southern constellation of Puppis. It is visible to the naked eye, having a combined apparent visual magnitude of +4.48. Based upon an annual parallax shift of 2.30 mas as seen from Earth, it is located roughly 1,400 light years from the Sun.
WR 24 is a Wolf-Rayet star in the constellation Carina. It is one of the most luminous stars known. At the edge of naked eye visibility it is also one of the brightest Wolf Rayet stars in the sky.
CK Carinae is a variable star in the constellation Carina, the keel of Argo Navis. It is a member of the star association Carina OB1-D, at a distance of around 2,300 parsecs or 7,500 light years.
8 Draconis, formally named Taiyi, is a single star in the northern circumpolar constellation of Draco. Based upon an annual parallax shift of 34.14 mas as seen from the Earth, the star is located approximately 96 light-years from the Sun. It is moving further away with a heliocentric radial velocity of +9 km/s, having come within 40.6 ly some 2.6 million years ago.