List of stars in Lupus explained

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

NameBFVarHDHIPRADecvis.
mag.		abs.
mag.		Dist. (ly)Sp. classNotes
α 129056 71860 2.30 −3.83 548 B1.5III Men; β Cep variable, . 70% likelihood of being a member of Scorpius–Centaurus association.[1]
β 132058 73273 2.68 −3.35 523 B2III Kekouan
γ 138690 76297 2.80 −3.40 567 B2IV rotating ellipsoidal variable. 91% likelihood of being a member of Scorpius–Centaurus association.
δ 136298 75141 3.22 −2.75 510 B1.5IV β Cep variable,
ε 136504 75264 3.37 −2.58 504 B2IV-V β Cep variable,
ζ 134505 74395 3.41 0.65 116 G8III
η 143118 78384 3.42 −2.48 493 B2.5IV suspected variable
ι 125238 69996 3.55 −1.61 352 B2.5IV β Cep variable,
φ1 136422 75177 3.57 −1.43 326 K5III variable star,
κ1 134481 74376 3.88 0.14 182 B9V Qízhènjiāngjūn (騎陣將軍)[2]
π 133242 73807 3.91 −2.01 497 B5
χ 5 141556 77634 3.97 −0.03 206 B9.5III-IV
ρ 128345 71536 4.05 −0.84 310 B5V 53 Per variable,
λ 133955 74117 4.07 −1.41 406 B3V
θ 144294 78918 4.22 −1.28 411 B2.5Vn suspected variable
μ 135734 74911 4.27 −0.48 291 B8V
ο 130807 72683 4.32 −1.16 408 B5IV suspected variable,
τ2 126354 70576 4.33 −0.59 314 A7:+...
ω 139127 76552 4.34 0.10 230 K4.5III
f 2 135758 74857 4.35 −0.53 308 K1II/III
σ 127381 71121 4.44 −1.79 574 B2III SX Ari variable,
φ2 136664 75304 4.54 −1.81 606 B4V
d KT 138769 76371 4.55 −1.07 434 B3IVp Be star
τ1 126341 70574 4.56 −2.95 1035 B2IV β Cep variable,
k 137058 75501 4.60 −0.70 374 A0V
g 139664 76829 4.64 3.42 57 F5IV-V
ψ1 3 139521 76705 4.66 0.28 245 G8/K0III
ψ2 4 140008 76945 4.75 −0.67 396 B5V
125442 70104 4.78 1.49 149 F0IV suspected variable
e 134687 74449 4.83 −0.89 454 B3IV suspected slow irregular variable
143699 78655 4.90 −1.14 527 B6III/IV suspected variable
i 1 135153 74604 4.91 −2.81 1140 F3III
ν1 136351 75206 4.99 2.32 111 F8V
143009 78323 4.99 −0.34 380 G8III
133340 73826 5.13 −0.13 367 G8III
ξ1 142629 78105 5.14 1.21 199 A3V
135345 74707 5.15 −2.83 1283 F:+...
b 129893 72290 5.22 0.72 259 G6III
h 139980 76939 5.23 0.63 271 G8/K0III
137709 75828 5.26 −1.91 886 K4III suspected variable
υ 136933 75439 5.36 0.00 384 Ap...
126983 70931 5.38 1.21 222 A1V suspected variable
c 131562 73095 5.38 1.27 216 A2III
a 128266 71500 5.39 −2.67 1336 K0III
138816 76397 5.44 −1.09 659 M0III suspected variable
132955 73624 5.45 0.30 350 B3V
134270 74305 5.45 −3.52 2025 G2Ib/II
137432 75647 5.46 −0.08 418 B5V
126981 70915 5.51 −0.31 477 B8Vn suspected variable
128068 71419 5.54 −0.90 637 K3III suspected variable,
125383 70054 5.55 0.19 384 G8III
GG 135876 74950 5.59 −0.40 514 B9V β Lyr variable
ξ2 142630 78106 5.59 1.70 196 B9V
140784 77286 5.61 0.23 388 B8V
131657 73111 5.62 −0.80 626 B+...
ν2 136352 75181 5.65 4.83 47 G2V has three planets (b, c & d)
κ2 134482 74380 5.70 1.84 193 A3IV
144415 78970 5.72 2.14 170 F0/F2V
129858 72250 5.74 0.65 340 A1V
HR 133880 74066 5.79 0.24 413 B8IV Si SX Ari variable,
133631 74006 5.77 0.62 349 G8III
142691 78142 5.78 −1.49 929 K0/K1III+..
138505 76207 5.82 −2.71 1655 M2III suspected semiregular variable
126504 70663 5.83 2.00 190 Am suspected variable
133937 74100 5.85 0.18 444 B7V
127501 71182 5.86 0.76 341 K0III
127486 71184 5.86 1.15 285 F6IV-V
143928 78747 5.91 2.91 130 F3V
140285 77086 5.93 0.18 461 A0V + B suspected variable
135235 74696 5.96 2.39 169 A3m
HZ 133652 73937 5.96 1.06 312 Ap Si α2 CVn variable
134255 74224 5.98 0.20 467 G6III
125869 70363 5.99 0.85 348 K1III
143790 78665 6.00 2.31 178 F5IV/V
140901 77358 6.01 5.09 50 G6IV
125810 70325 6.03 −0.93 803 K2III
142448 78046 6.04 −0.40 632 B9V
135348 74716 6.05 −1.14 893 B3IV suspected variable,
139271 76608 6.05 −0.37 626 A4:m...
128582 71639 6.06 3.28 117 F7V
HX 125721 70270 6.06 −3.25 2415 B1III rotating ellipsoidal variable,
129932 72308 6.07 −3.28 2415 A1III/IV
134837 74479 6.09 0.86 362 B8V
132242 73354 6.10 −2.61 1801 F5III
137465 75742 6.10 −2.21 1495 G2Ib
143902 78726 6.12 0.65 400 F3III suspected variable,
135896 74929 6.18 −1.25 997 G6/G8III
136014 75003 6.19 0.83 385 G8III/IV
136334 75164 6.21 1.26 319 A1V
139599 76809 6.21 −0.95 883 K5/M0III variable star,
142407 77985 6.21 0.79 396 K4III
143248 78445 6.21 0.93 370 A0V
137919 75915 6.23 0.29 503 B9V
138204 76063 6.23 2.58 175 A3III
138923 76395 6.26 1.00 367 B8/B9V
133550 73901 6.27 −1.84 1364 K5III
142542 78058 6.29 2.77 165 F3/F5V
130073 72338 6.30 −0.06 609 K1III
135730 74875 6.30 1.78 262 Am
142889 78236 6.31 −0.06 612 K0III
134597 74418 6.32 0.52 471 K2III
143404 78486 6.33 0.20 550 K4III
131923 73241 6.34 4.39 80 G5V
139613 76739 6.35 −0.10 635 K3III
138564 76234 6.36 1.12 364 B9V
128617 71658 6.37 2.64 182 F3IV
GM 133220 73764 6.38 −0.18 640 M6III semiregular variable,
141832 77729 6.38 1.86 263 K0III suspected variable,
126759 70809 6.40 0.51 491 Ap... suspected variable
133518 73966 6.40 −1.07 1016 B3III
138395 76165 6.40 0.04 610 K0III
125809 70320 6.41 −3.57 3228 G5Ib
140861 77350 6.41 0.89 414 G8III/IVp..
126093 70451 6.43 0.53 494 K0/K1III
129624 72135 6.44 −1.23 1116 K4III
134444 74336 6.44 1.06 389 K1III
135468 74775 6.44 2.81 174 F6V
137785 75818 6.44 2.44 205 F2V
135430 74769 6.46 0.27 565 G8III
133469 73850 6.48 3.96 104 F6V
133399 73881 6.48 −2.11 1707 B3V
128154 71494 6.49 −0.20 710 K2/K3III
136607 75324 6.49 0.58 495 G8III
138221 76048 6.49 0.77 453 B6/B7V
135760 74890 7.05 299 K1III has a planet (b)
126525 70695 7.85 124 G4V has a planet (b)
NZ 141943 7.98 G2 BY Dra variable,
142527 78092 8.34 760 F6III has a circumstellar disk
EX 325367 8.50 M0 prototype EXor,
135344B 8.71 F8V has a circumstellar disk
135778 74865 9.00 375 F3V has a planet (b)
FW 136483 75234 9.05 2080 F5IV RR Lyr variable,
76074 9.31 19.329 M2.5V suspected variable
FT 132316 9.82 F0+K2V β Lyr variable
9.95 1363 A1IV-V has a transiting planet (b)
RY 78317 10.2 422 G0V: UX Ori star,
70849 10.4 8.50 78 K7Vk has a planet (b)
RU 142560 78094 10.51 393 G5V:e T Tau star
GQ 11.40 500 K7V T Tau star, ; has a planet or a brown dwarf (b)
73391 11.88 WC10 protoplanetary nebula
12.4 391 K4 has a transiting planet (b)
NY 14.50 K+DA:... DQ Her variable,
14.78 350 sdK5 previously misclassified as a white dwarf
IL 14.9 A2V low-mass X-ray binary,
17.4 5.2 8950 K1V has a planet (b)
IM 78053 M0 T Tau star
BR SU UMa variable
II C Mira variable

See also

References

Notes and References

  1. Rizzuto . Aaron . Ireland. Michael . Robertson . J. G. . Multidimensional Bayesian membership analysis of the Sco OB2 moving group . Monthly Notices of the Royal Astronomical Society . 2011 . 416 . 4 . 3108–17 . 10.1111/j.1365-2966.2011.19256.x . 2011MNRAS.416.3108R . 1106.2857 . 54510608 .
  2. AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 29 日

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