List of stars in Aquarius explained

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

NameBFG.VarHDHIPRADecvis.
mag.
abs.
mag.
Dist. (ly)Sp. classNotes
β 22 75 204867 106278 2.90 −3.47 612 G0Ib Sadalsuud, Sadalsud, Sad es Saud, Sadalsund, Saad el Sund, Nir Saad al Saaoud, Lucida Fortunæ Fortunarum,[1] part of Saʽd al Suʽud;[2] [3]
α 34 105 209750 109074 2.95 −3.88 758 G2Ib Sadalmelik, Sadal Melik, Sadalmelek, Sadlamulk, El Melik, Saad el Melik, Ruchbah; double star
δ 76 191 216627 113136 3.27 −0.18 159 A3V Skat, Scheat, Seat, Sheat
ζ1 55 150 213051 110960 3.65 1.14 103 F3III-IV Sadaltager, Sadaltajir, Altager, Achr al Achbiya, Postrema Tabernaculorum, part of al Aḣbiyah;[4] [5]
c2 88 211 218594 114341 3.68 −0.60 234 K1III
λ 73 185 216386 112961 3.73 −1.67 391 M2IIIvar Hydor, Ekkhysis;,
ε 2 8 198001 102618 3.78 −0.46 229 A1V Albali, Al Bali, Nir Saad Bula, Lucida Fortunæ Dissipantis, part of al Bulaʽ;[6] [7] suspected
γ 48 136 212061 110395 3.86 0.44 158 A0V Sadachbia, Sadalachbia, Aoul al Achbiya, Prima Tabernaculorum, part of al Aḣbiyah; double star
b1 98 231 220321 115438 3.96 0.48 162 K0III
η 62 163 213998 111497 4.04 0.29 183 B9IV-Vn Hydria, part of al Aḣbiyah
τ2 71 183 216032 112716 4.05 −1.28 380 K5III
suspected variable
θ 43 129 211391 110003 4.17 0.33 191 G8III-IV Ancha
φ 90 215 219215 114724 4.22 0.05 222 M2III suspected variable
ψ1 91 218 219449 114855 4.24 0.95 148 K0III multiple star; has a
ι 33 107 209819 109139 4.29 0.67 172 B8V
b2 99 235 220704 115669 4.38 −0.50 308 K4III suspected variable
ψ2 93 222 219688 115033 4.41 −0.56 322 B5Vn
variable,
ζ2 55 150 213052 4.42 -0.01 251 F3V component of the ζ Aqr system
k 3 9 EN 198026 102624 4.43 −1.24 445 M3IIIvar EN Aqr;,
c1 86 210 218240 114119 4.48 0.67 188 G8III binary star
ω2 105 259 222661 116971 4.49 1.12 154 B9V binary star
ν 13 47 201381 104459 4.50 1.00 164 G8III Albulaan, part of al Bulaʽ
ξ 23 81 205767 106786 4.68 0.99 179 A7V Bunda, Thanih Saad al Saaoud, Secunda Fortunæ Fortunarum, part of Saʽd al Suʽud; double star
g 66 176 215167 112211 4.68 −1.18 484 K3III suspected variable
b3 101 244 221565 116247 4.70 −0.26 320 A0V double star
c3 89 212 218640 114375 4.71 −1.31 521 A3IV: double star
μ 6 16 198743 103045 4.73 1.34 155 A3m Albulaan, part of al Bulaʽ; double star,
ο 31 103 209409 108874 4.74 −0.60 381 B7IVe Kae Uh; emission-line star;,
π 52 142 212571 110672 4.80 −2.84 1101 B1Ve Seat, Wasat al Achbiya, Media Tabernaculorum, part of al Aḣbiyah; emission-line star; γ Cas variable,
σ 57 154 213320 111123 4.82 0.27 265 A0IVs 貴子星 (Takako-boshi)
A2 104 257 222574 116901 4.82 −1.65 643 G2Ib/II triple star; suspected variable
χ 92 219 219576 114939 4.93 −1.54 640 M3III ,
ω1 102 253 222345 116758 4.97 1.91 134 A7IV
ψ3 95 223 219832 115115 4.99 0.58 249 A0V triple star
κ 63 166 214376 111710 5.04 0.76 234 K2III Situla; double star
d 25 84 206067 106944 5.10 0.76 241 K0III double star
47 135 212010 110391 5.12 1.37 183 K0III
1 3 196758 101936 5.15 0.77 245 K1III triple star
i3 108 270 ET 223640 117629 5.17 0.20 321 Ap Si ET Aqr; spectroscopic binary;,
94 224 115125 5.19 3.56 69 K2V component of the 94 Aqr system
97 230 220278 115404 5.19 0.88 237 A3V binary star
94 224 219834 115126 5.20 3.62 69 G6/G8IV binary star
υ 59 161 213845 111449 5.21 3.43 74 F7V
68 179 215721 112529 5.24 0.68 266 G8III
i1 106 261 222847 117089 5.24 0.20 331 B9V
258 G. Aqr258 222643 116957 5.27 0.60 280 K3III
i2 107 262 223024 117218 5.28 1.21 212 F0III double star
32 104 209625 108991 5.29 1.04 231 A5m
41 123 210960 109786 5.33 0.65 281 K1III multiple star
42 127 211361 110000 5.34 −0.52 484 K1III
ρ 46 134 211838 110273 5.35 −1.44 743 B8IIIMNp...
A1 103 256 222547 116889 5.36 −0.91 584 K4/K5III
e 38 117 210424 109472 5.43 −0.75 561 B5III
h 83 208 218060 113996 5.44 1.63 188 F2V triple star
18 67 203705 105668 5.48 2.07 157 F0V suspected variable
21 70 203926 105767 5.48 −0.01 408 K4III
7 24 199345 103401 5.49 −0.84 601 K5III triple star; suspected variable
12 37 200496 103981 7.31 A3V optical double
49 137 212271 110529 5.53 0.93 272 K0IIICN...
77 193 216640 113148 5.53 2.36 140 K1III suspected variable
5 13 198667 103005 5.55 −1.27 753 B9III suspected variable
30 102 209396 108868 5.55 0.95 271 K0III
f 53 146 212697 110778 5.55 4.04 65 G3V multiple star
217 G. Aqr217 219402 114822 5.56 1.30 231 A3V
96 226 219877 115142 5.56 2.85 114 F3IV
28 99 209128 108691 5.60 −0.94 661 K4III:
26 85 206445 107144 5.66 −2.77 1583 K2III
250 222093 116591 5.66 0.96 283 K0III double star
τ1 69 180 215766 112542 5.68 1.17 260 B9V multiple star
269 G. Aqr269 223559 117567 5.70 −0.05 460 K4III
19 68 203875 105761 5.71 1.07 276 F0IV
94 G. Aqr 94 208111 108102 5.71 0.96 291 K2III
195 216718 113184 5.72 0.95 293 K0III-IV double star
264 G. Aqr264 223170 117314 5.74 0.61 346 K0III
44 131 211434 110023 5.75 0.65 341 G6III suspected variable
50 140 212430 110602 5.76 −0.35 542 K0III
h 273 223807 117756 5.76 −0.61 612 K0III
80 G. Aqr80 205423 106592 5.79 0.13 441 G9III:
51 139 212404 110578 5.79 0.22 424 A0V multiple star
35 112 210191 109332 5.80 −5.79 6792 B2III
130 211392 110009 5.80 0.64 351 K3III: suspected variable
74 187 HI 216494 113031 5.80 −0.72 657 B8IV/V HI Aqr; double star; α2 CVn variable,
15 58 202753 105164 5.83 −1.56 979 B5V
271 G. Aqr271 223774 117722 5.85 1.13 286 K2III
11 G. Aqr11 198431 102891 5.87 1.45 250 K1III
16 62 203222 105412 5.87 0.80 336 G7III:
60 160 213789 111394 5.88 0.21 444 G6III triple star
12 200497 5.89 -0.21 541 G4III optical component of 12 Aqr
255 G. Aqr255 222493 116853 5.89 0.56 379 K0III
138 G. Aqr138 212320 110532 5.92 0.18 466 G8Ib/II(w)
268 G. Aqr268 223524 117541 5.93 1.06 307 K0IV
202 G. Aqr202217563 113686 5.94 −3.61 1011 G5II/III
27 DV 199603 103545 5.95 1.31 276 A9V ,
246 G. Aqr246221745 116368 5.95 0.79 351 K4III
45 133 211676 110179 5.96 0.78 354 K0III
225 G. Aqr225 219879 115144 5.96 −1.71 1116 K2/K3III
162 G. Aqr162 213986 111515 5.97 0.89 337 K1III
205 G. Aqr205 217703 113801 5.97 1.54 251 K0III
118 210434 109466 5.98 1.30 282 K0III-IV double star
4 12 198571 102945 5.99 2.14 192 F5IV-V multiple star; suspected variable
17 65 203525 105574 5.99 −0.73 720 M0III
39 120 210705 109624 6.04 2.85 142 F0V binary star; suspected variable
26199442 103414 6.06 1.11 318 K2III triple star
265223311 117420 6.09 −0.64 723 K4III suspected variable
119 G. Aqr119210464 109509 6.10 2.33 185 F6/F7V
74 G. Aqr74204121 105864 6.12 2.72 156 F5V
198 G. Aqr198217251 113531 6.12 −0.40 656 K3/K4III
216 219279 114750 6.13 −0.91 836 K5III multiple star
157 213429 111170 6.15 4.12 83 F7V double star
155 G. Aqr155 213428 111171 6.15 0.34 473 K0
207 218061 113998 6.15 0.01 552 K4III double star
128 G. Aqr128 211356 109984 6.16 1.63 262 A5Vn
89 G. Aqr89 207235 107596 6.17 1.70 256 A7V
126 G. Aqr126 211364 110018 6.17 0.16 519 K0III
228 220035 115257 6.17 0.72 400 K0III suspected variable
82 204 217701 113781 6.18 −1.72 1240 M2III suspected variable
234 G. Aqr234 220465 115528 6.18 0.92 367 K0III
70 181 FM 215874 112615 6.19 0.87 377 A9III-IV FM Aqr;,
78 192 216637 113127 6.20 −0.16 609 K3III
238 G. Aqr238 221081 115906 6.20 −2.95 2203 K0
11 31 199960 103682 6.21 4.10 86 G1V
266 G. Aqr266 223428 117494 6.21 0.64 424 K1/K2III
82 205765 106758 6.22 0.78 399 A2V binary star
2 G. Aqr2 196712 101921 6.23 −1.65 1230 B7IIIn
167 214448 111761 6.23 0.49 459 G1IV-V double star
81 201 217531 113674 6.23 0.69 418 K5III
274 G. Aqr274 223884 117797 6.23 1.41 300 A5V
IQ 198272 102770 6.24 −1.06 942 M3
35 200375 103892 6.24 2.14 215 F5V triple star
95 208177 108144 6.24 2.02 227 F5IV double star
98 G. Aqr98 208801 108506 6.24 3.46 117 K2V
100 242 221357 116118 6.24 1.72 261 F0V
239 221148 115953 6.26 2.81 159 K3IIIvar suspected variable
49 G. Aqr49 201567 104557 6.27 1.14 346 K0III
200 G. Aqr200 217498 113673 6.27 1.26 327 A2V
7 G. Aqr7 197954 102561 6.28 −0.63 787 K2
100 G. Aqr100 209240 108784 6.28 1.64 277 K0III
115 G. Aqr115 210419 109442 6.28 1.05 362 A1Vnn
172 LP 214983 112078 6.28 −1.78 1336 M0 multiple star; irregular variable,
144 G. Aqr144 212643 110746 6.29 0.38 495 A0V
197 G. Aqr197 216953 113345 6.31 0.80 413 G9III
171 214810 111965 6.32 3.70 109 F6V binary star
96 G. Aqr96 208703 108453 6.33 2.60 181 F5IV
221 219659 115015 6.33 0.94 389 A1/A2IV/V suspected variable
38 G. Aqr38 200663 104048 6.34 0.96 388 G5
f 53 212698 6.35 component of the 53 Aqr system
113 G. Aqr113 210244 109375 6.36 0.37 514 G8III
56 153 213236 111086 6.36 −0.08 633 B8II
196 G. Aqr196 216727 113204 6.36 −0.28 695 K4/K5III
R 222800 117054 6.36 -0.11 643 M7IIIpev ,
189 G. Aqr189 216553 113080 6.37 0.53 481 K5III
237 G. Aqr237 220957 115839 6.37 1.10 369 G6/G8III
15 G. Aqr15 198802 103077 6.38 3.11 147 G1V
52 202259 104872 6.38 −0.23 685 M1III suspected variable
20 69 203843 105729 6.38 2.37 213 F0V
251 G. Aqr251 222125 116624 6.38 1.30 338 K0III
29 101 DX 209278 108797 6.39 0.59 471 A0/1V + K1/2 DX Aqr; triple star, spectroscopic binary;,
121 G. Aqr121 210763 109647 6.39 1.53 305 F7V
132 211575 110091 6.39 3.30 135 F3V
58 156 213464 111200 6.39 2.20 225 A8III
61 164 214028 111539 6.39 0.62 465 K4III
240 G. Aqr240 221308 116060 6.39 −2.97 2433 K0
67 175 215143 112179 6.40 1.14 368 A0Vn
248 G. Aqr248 221835 116428 6.40 0.68 453 G5III:
57 G. Aqr57 202606 105079 6.41 0.05 609 A1V
79 IZ 205358 106544 6.41 −1.98 1552 M3 irregular variable,
152 G. Aqr152 213198 111066 6.41 1.86 264 F2/F3IV/V
213 G. Aqr213 218639 114371 6.43 1.31 345 A0V
236 G. Aqr236 220766 115709 6.43 1.01 396 K0III double star
18 G. Aqr18 198949 103154 6.44 2.20 230 F1IV
14 54 IW 202466 105019 6.45 −2.30 1831 M4III: IW Aqr; double star; semiregular variable,
72 G. Aqr72 204041 105819 6.45 1.75 284 A1IV
174 215114 112168 6.45 0.06 617 A5V multiple star
1 G. Aqr1 196676 101911 6.46 2.18 234 K0
233 G. Aqr233 220466 115522 6.46 2.48 204 F3IV/V double star
50 EW 201707 104634 6.47 0.82 439 Fm delta Del low-amplitude δ Sct variable,
55 G. Aqr55 202554 105046 6.48 −0.59 845 K0
34 G. Aqr34 200340 103889 6.50 −1.75 1455 B6V
241 G. Aqr241 221356 116106 6.50 4.41 86 F8V
10 Aqr10 199944 103681 6.52 400 A5V [8] [9]
9 Aqr9 200004 103728 6.55 700 G6/8III [10] [11] [12] [13]
114 210277 109378 6.63 4.99 69 G0V has a planet (b)
37 Aqr 37 116 210422 109460 6.64 0.97 444 K0 suspected variable[14] [15]
24 83 206058 106942 6.66 3.48 141 F7III triple star
8 199828 103640 6.60 290 A3/4 IV
85 Aqr 85 218173 114054 6.69 B9 V [16]
75 Aqr 75 216567 113085 6.86 K2/K3III [17]
54 Aqr 54 212741 110786 6.98 270 A3III/IV
36 Aqr 36 210269 109369 6.98 520 G8/K0III/IV a yellow giant star or subgiant star
72 Aqr 72 216182 112813 7.00 K0 III [18]
65 Aqr 65 215097 112161 7.04 K0 III [19]
84 Aqr 84 218081 114006 7.08 G8III [20]
87 Aqr 87 218331 114164 7.37 A0/1 IV [21]
212771 110813 7.60 2.17 397 G8IV Lionrock; has a planet (b)
222582 116906 7.70 4.59 137 G5 has a planet (b)
220689 115662 7.77 4.53 145 G3V has a planet (b)
Gliese 884 217357 113576 7.87 8.34 26.8 K7V + M0-2V double star
215152 112190 8.13 6.47 70 K0 has four planets (b, c, d & e)
HD 221416 221416 116158 8.15 310 K0IV/V has a planet (b)
206610 107251 8.34 2.19 555 K0III Bosona; has a planet (b)
Gliese 898 221503 116215 8.607 7.68 45.5 K6V
A2 104 222561 116904 8.52 1.29 911 A6V: component of the 104 Aqr system
9.87 6.38 163 K5 has a transiting planet (b)
IL 113020 10.17 11.81 15.3 M3.5V IL Aqr; nearby red dwarf, BY Dra variable, ; has four planets (b, c, d & e)
109388 10.42 10.70 29 M3.5 has two planets (b & c)
WASP-70 A 10.79 3.84 799 G4 has a transiting planet (b)
11.45 4.38 848 F9 has a transiting planet (b)
AE 101991 11.6 6.56 333 K2Ve + pec(e+cont) DQ Her-type cataclysmic variable,
11.6 581 K2 has a transiting planet (b)
11.9 5.4 652 G9V style=text-align:left; has four transiting planets (b, c, d & e)
EZ 12.18 14.49 11.3 M5.5Ve-M7e 12th closest star system; triple star; flare star
12.4 4.96 1001 G8 Márohu; has a transiting planet (b)
12.31 1389 G4 has a transiting planet (b)
12.62 M4V Fomalhaut C
12.69 G6 has a transiting planet (b)
13.2013.99 15330 KIIvwSneden's Star
ultra-metal-poor star
FO 13.5 DQ Her-type cataclysmic variable,

See also

References

Notes and References

  1. http://articles.adsabs.harvard.edu//full/1895MNRAS..55..429K/0000431.000.html E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
  2. Consisting with β Aqr (Sadalsuud), ξ Aqr (Bunda) and 46 Cap (c Cap), were Saʽd al Suʽud, the Luck of Lucks. See Star Name – R.H.Allen p. 52
  3. as Nir Saad al Saaoud or Lucida Fortunæ Fortunarum (the brightest of luck of lucks) and as Thanih Saad al Saaoud or Secunda Fortunæ Fortunarum (the second of luck of lucks). should be Thalath Fortunæ Fortunarum or Tertia Fortunæ Fortunarum (the third of luck of lucks) consistently, but Al Achsasi Al Mouakket was not designated the title for this star with uncleared consideration. Possibly according to the differences of opinion with R.H.Allen
  4. Consisting with γ Aqr (Sadachbia), π Aqr (Seat), ζ Aqr (Sadaltager / Achr al Achbiya) and η Aqr (Hydria), were al Aḣbiyah, the Tent. See Star Name – R.H.Allen p. 52
  5. as Aoul al Achbiya or Prima Tabernaculorum (the first of luck of the homes or tents), as Wasat al Achbiya or Media Tabernaculorum (the middle of luck of the homes or tents) and as Achr al Achbiya or Postrema Tabernaculorum (the end of luck of the homes or tents). should be designated as al Achbiya consistently, but it was not designated as the name except the name Hydria or Deli
  6. Consisting with ε Aqr (Albali), μ Aqr (Albulaan) and ν Aqr (Albulaan), were al Bulaʽ, the Swallower. See Star Name – R.H.Allen p. 53
  7. as Nir Saad Bula or Lucida Fortunæ Dissipantis (the brightest of luck of the swallower) and the common name is Albali. and was already designated as the common name Albulaan, the plural form of al Bulaʽ
  8. 1999MSS...C05....0H. Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5. Michigan Spectral Survey. 5. Houk, N.. Swift, C.. 1999.
  9. Validation of the new Hipparcos reduction . van Leeuwen . F. . Astronomy and Astrophysics . 474 . 2 . 653–664 . 2007 . 0708.1752 . 2007A&A...474..653V . 10.1051/0004-6361:20078357 . 18759600. dead . https://web.archive.org/web/20160402233353/http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A&A...474..653VFUL . 2016-04-02 . Vizier catalog entry
  10. Validation of the new Hipparcos reduction. van Leeuwen, F. . Astronomy and Astrophysics. 474. 2. 653–664. 2007. 0708.1752. 2007A&A...474..653V. 10.1051/0004-6361:20078357. 18759600 .
  11. The Tycho-2 catalogue of the 2.5 million brightest stars. Høg, E.. etal. 2000. Astronomy and Astrophysics. 355. L27–L30. 2000A&A...355L..27H.
  12. 1988mcts.book.....H. Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume 4, Declinations -26°.0 to -12°.0.. Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. 4. Houk, N.. Smith-Moore, M.. 1988.
  13. General catalogue of stellar radial velocities. Carnegie Institute Washington D.C. Publication. Wilson, Ralph Elmer. 1953. 1953GCRV..C......0W.
  14. 2004ApJS..155..175A. Spectral Classification of Stars in A Supplement to the Bright Star Catalogue. The Astrophysical Journal Supplement Series. Abt, Helmut A.. 2004. 155. 1. 175–177. 10.1086/423803 . free.
  15. Wilson . R. E. . 1953 . General Catalogue of Stellar Radial Velocities . Carnegie Institute Washington D.C. Publication . Carnegie Institute of Washington D.C. . 1953GCRV..C......0W .
  16. SIMBAD, 85 Aquarii (accessed 24 July 2012)
  17. SIMBAD, 75 Aquarii (accessed 2 December 2019)
  18. SIMBAD, 72 Aquarii (accessed 24 July 2012)
  19. 65 Aqr . 2019-05-18 .
  20. SIMBAD, 84 Aquarii (accessed 24 July 2012)
  21. SIMBAD, 87 Aquarii (accessed 24 July 2012)