XIV

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This is: the: list of notable stars in the——constellation Volans, sorted by, "decreasing brightness."

Name B G. Var HD HIP RA Dec vis.
mag. 		abs.
mag. 		Dist. (ly) Sp. class Notes
γ Vol γ 9 55865 34481 07 08 44.82 −70° 29′ 57.1″ 3.62 0.59 142 G8IIIvar double star with γ Vol; suspected variable, Vmax = 3.56, Vmin = 3.62
β Vol β 29 71878 41312 08 25 44.25 −66° 08′ 11.5″ 3.77 1.17 108 K2IIIvar suspected variable, Vmax = 3.76, Vmin = 3.79
ζ Vol ζ 16 63295 37504 07 41 49.20 −72° 36′ 22.1″ 3.93 0.86 134 K0III
δ Vol δ 10 57623 35228 07 16 49.83 −67° 57′ 25.8″ 3.97 −2.56 660 F6II
α Vol α 46 78045 44382 09 02 26.80 −66° 23′ 45.0″ 4.00 1.09 124 A5Vm
ε Vol ε 22 68520 39794 08 07 55.84 −68° 37′ 01.7″ 4.35 −2.12 560 B6IV
24 G. Vol 24 70514 40680 08 18 18.78 −65° 36′ 47.7″ 5.06 0.27 296 K1III
6 G. Vol 6 53501 33682 06 59 50.58 −67° 55′ 01.2″ 5.18 0.44 290 K3III
θ Vol θ 35 74405 42425 08 39 05.13 −70° 23′ 11.9″ 5.19 0.86 239 A0V
η Vol η 27 71576 41003 08 22 04.52 −73° 24′ 00.2″ 5.28 0.09 356 A0/A1IV/V
κ Vol κ 25 71046 40817 08 19 49.00 −71° 30′ 54.0″ 5.33 −0.06 390 B9III/IV part of the κ Vol triple star system
43 G. Vol 43 76143 43414 08 50 34.68 −66° 47′ 35.6″ 5.34 1.74 171 F5IV
ι Vol ι 5 51557 32912 06 51 26.98 −70° 57′ 48.5″ 5.41 −0.76 558 B7IV
30 G. Vol 30 72337 41451 08 27 16.79 −70° 05′ 36.9″ 5.51 0.80 285 A0V
κ Vol κ 26 71066 40834 08 20 00.56 −71° 30′ 19.7″ 5.63 0.21 395 A0p part of the κ Vol triple star system; suspected variable, ΔV = 0.03
γ Vol γ 8 55864 34473 07 08 42.34 −70° 29′ 50.4″ 5.68 2.41 147 F2 double star with γ Vol
19 G. Vol 19 64484 38210 07 49 41.00 −66° 11′ 45.5″ 5.78 0.04 458 B9V
45 G. Vol 45 77887 44283 09 01 08.49 −68° 41′ 02.1″ 5.89 −0.95 762 M1III slow irregular variable, ΔV = 0.012, P = 4.46488 d
28 G. Vol 28 71863 41321 08 25 51.62 −64° 36′ 02.4″ 5.95 0.75 358 G8/K0III
41 G. Vol 41 75171 42895 08 44 30.05 −65° 49′ 32.5″ 6.03 2.12 198 A9V
4 G. Vol 4 50002 32332 06 44 55.67 −70° 26′ 01.6″ 6.10 −0.33 629 K3III
44 G. Vol 44 76270 43351 08 49 50.14 −72° 33′ 04.5″ 6.10 −3.84 3165 A3m... suspected variable
33 G. Vol 33 73468 41907 08 32 41.88 −73° 21′ 25.1″ 6.11 0.77 381 G8III
18 G. Vol 18 63584 37720 07 44 13.10 −69° 49′ 17.8″ 6.16 0.70 403 A0IV/V
15 G. Vol 15 62153 36914 07 35 21.66 −74° 16′ 30.0″ 6.33 −1.01 959 B9IV + B9IV double star
20 G. Vol 20 66920 39041 07 59 15.78 −73° 14′ 38.8″ 6.33 0.84 409 A3III
40 G. Vol 40 75116 42850 08 43 54.33 −68° 12′ 41.9″ 6.33 −1.21 1052 K3III:
3 G. Vol 3 49947 32222 06 43 36.73 −73° 07′ 04.7″ 6.36 0.81 420 G8III
17 G. Vol 17 63513 37773 07 44 43.88 −66° 04′ 19.4″ 6.37 −0.12 648 G6/G8III
12 G. Vol 12 60150 36346 07 28 51.40 −64° 30′ 35.2″ 6.38 −0.22 681 K5III
7 G. Vol 7 55151 34270 07 06 14.30 −68° 50′ 15.3″ 6.47 0.54 501 K0III
11 G. Vol 11 59640 35946 07 24 37.11 −71° 28′ 14.7″ 6.49 2.04 253 A3V
2 G. Vol 2 49268 31977 06 40 57.56 −71° 46′ 30.3″ 6.50 0.88 433 K1IIICN...
13 G. Vol 13 61312 36735 07 33 21.80 −68° 46′ 06.69″ 6.59 0.42 547 A1/2V
1 G. Vol 1 49306 32106 06 42 25.55 −67° 50′ 35.16″ 6.70 1.08 445 B9.5/A0V
32 G. Vol 32 73391 41837 08 31 44.63 −74° 51′ 17.98″ 6.71 0.61 688 K0/1III suspected variable
21 G. Vol 21 67559 39406 08 03 21.16 −69° 58′ 17.66″ 6.74 -0.42 961 B8III
31 G. Vol 31 72719 41478 08 27 33.85 −75 21 31.25° 6.81 1.58 357 A2V
14 G. Vol 14 61950 37007 07 36 19.26 −69° 03′ 23.54″ 6.87 -1.23 1343 B8V
HD 76920 76920 43803 08 55 17.0 −67° 15′ 56″ 7.8 603 K1III has a planet (b)
HD 76700 76700 43686 08 53 55.52 −66° 48′ 03.6″ 8.13 4.25 195 G6V has a planet (b)
R Vol R 07 05 36.21 −73° 00′ 52.02″ 8.70 -0.91 2728 CVIIe+ Carbon star and Mira variable, Vmax = 8.78, Vmin = 11.50, P = 445.46 d
HD 68402 68402 39589 08 05 24.0 −74° 24′ 38″ 9.11 254 G5IV/V has a planet (b)
S Vol S 07 29 45.57 −73° 22′ 43.97″ 12.97 3.06 3130.7 M4IIIe Mira variable, Vmax = 8.96, Vmin = 13.80, P = 395.84 d
L 97-12 07 53 08.15 −67° 47′ 31.38″ 14.09 25.822 DA9.0 one of the closest known white dwarfs
RR Vol RR 08 27 28.73 −69° 53′ 55.42″ 15.93 2.78 12102.28 A9V Algol variable
UY Vol UY 07 48 33.30 −67° 45′ 00.0″ 16.9 2.39 26,000 M X-ray burster and eclipsing binary, Vmax = 16.9, Vmin = <23.0, P = 0.159 d
Table legend:

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