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List of stars in Aries

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

Name B F Var HD HIP RA Dec vis.
mag.
abs.
mag.
Dist. (ly) Sp. class Notes
Hamal α 13 12929 9884 02 07 10.29 +23° 27′ 46.0″ 2.01 0.48 66 K2III Hamal, Hemal, Hamul, Ras Hammel, El Nath; suspected variable, Vmax = 1.98, Vmin = 2.04; has a planet (b)
β Ari β 6 11636 8903 01 54 38.35 +20° 48′ 29.9″ 2.64 1.33 60 A5V... Sheratan, Sharatan, Al Sharatain; suspected variable, Vmax = 2.56, Vmin = 2.70
41 Ari c 41 17573 13209 02 49 58.99 +27° 15′ 38.8″ 3.61 0.16 159 B8Vn Bharani; suspected variable, Vmax = 3.60, Vmin = 3.64
δ Ari δ 57 19787 14838 03 11 37.67 +19° 43′ 36.1″ 4.35 0.79 168 K2IIIvar Botein, Nir al Botain, Lucida Ventris, part of Al Buṭain; suspected variable, Vmax = 4.33, Vmin = 4.37
HD 20644 20644 15549 03 20 20.37 +29° 02′ 54.6″ 4.47 −2.00 640 K2II-III
39 Ari 39 17361 13061 02 47 54.44 +29° 14′ 50.7″ 4.52 0.80 181 K1III Lilii Borea
γ Ari γ 5 11503 01 53 31.80 +19° 17′ 45.0″ 4.62 1.11 164.0 kA0hA3(IV)SiSr Mesarthim, Mesartim; binary star; α CVn variable, ΔV = 0.04, P = 1.6092 d
35 Ari 35 16908 12719 02 43 27.11 +27° 42′ 25.8″ 4.65 −0.62 370 B3V
γ Ari γ 5 11502 8832 01 53 31.77 +19° 17′ 38.7″ 4.70 1.19 164.0 B9.5IV component of the γ Ari system
λ Ari λ 9 11973 9153 01 57 55.78 +23° 35′ 45.9″ 4.79 1.73 133 F0V binary star
ζ Ari ζ 58 20150 15110 03 14 54.11 +21° 02′ 40.7″ 4.87 −0.22 340 A1V part of Al Buṭain
14 Ari 14 13174 10053 02 09 25.29 +25° 56′ 23.9″ 4.98 0.02 320 F2III
κ Ari κ 12 12869 9836 02 06 33.91 +22° 38′ 54.3″ 5.03 1.23 187 A2m spectroscopic binary
ι Ari ι 8 11909 9110 01 57 21.03 +17° 49′ 03.3″ 5.09 −1.44 659 K1p... spectroscopic binary
τ Ari τ 63 20893 15737 03 22 45.27 +20° 44′ 31.6″ 5.10 0.15 319 K3III
38 Ari 38 UV 17093 12832 02 44 57.51 +12° 26′ 45.5″ 5.18 2.26 125 A7III-IV δ Sct variable, Vmax = 5.18, Vmin = 5.22, P = 0.0355 d
ε Ari A ε 48 18519 02 59 12.70 +21° 20′ 25.0″ 5.2 0.16 332 A2Vs part of Al Buṭain; binary star
η Ari η 17 13555 10306 02 12 47.98 +21° 12′ 39.5″ 5.23 2.84 98 F5V
π Ari π 42 17543 13165 02 49 17.56 +17° 27′ 51.6″ 5.26 −1.07 603 B6V part of Al Buṭain; spectroscopic binary
τ Ari τ 61 20756 15627 03 21 13.61 +21° 08′ 49.7″ 5.27 −0.49 462 B5IV triple star system; Beta Lyrae variable
33 Ari 33 16628 12489 02 40 41.03 +27° 03′ 39.6″ 5.30 1.03 233 A3V
ν Ari ν 32 16432 12332 02 38 49.00 +21° 57′ 41.2″ 5.45 0.32 346 A7V
52 Ari A 52 19134 14376 03 05 26.69 +25° 15′ 18.7″ 5.45 0.00 402 B7Vn binary star
ξ Ari ξ 24 14951 11249 02 24 49.04 +10° 36′ 38.2″ 5.48 −0.85 603 B7IV variable star, ΔV = 0.007, P = 1.73515 d
ε Ari B ε 48 18519 13914 02 59 12.73 +21° 20′ 25.6″ 5.5 0.46 332 A2Vs component of the ε Ari system
64 Ari 64 21017 15861 03 24 18.46 +24° 43′ 27.1″ 5.50 1.26 230 K4III
σ Ari σ 43 17769 13327 02 51 29.57 +15° 04′ 55.7″ 5.52 −0.32 479 B7V
62 Ari 62 20825 15696 03 22 11.89 +27° 36′ 27.3″ 5.55 −1.82 973 G5III
21 Ari 21 13872 10535 02 15 42.83 +25° 02′ 35.7″ 5.57 2.16 157 F6V
θ Ari θ 22 14191 10732 02 18 07.55 +19° 54′ 04.2″ 5.58 0.21 387 A1Vn
ρ Ari ρ 46 18256 13702 02 56 25.98 +18° 01′ 25.1″ 5.58 2.83 115 F6V part of Al Buṭain; suspected BY Dra variable
HD 20149 20149 15154 03 15 20.45 +30° 33′ 24.0″ 5.61 −0.01 434 A1Vs
10 Ari 10 12558 9621 02 03 39.26 +25° 56′ 07.6″ 5.64 2.02 172 F8IV
31 Ari 31 16234 12153 02 36 37.75 +12° 26′ 52.2″ 5.64 2.91 115 F7V
HD 19270 19270 14439 03 06 23.69 +13° 11′ 14.6″ 5.64 0.69 319 K3III
15 Ari 15 AV 13325 10155 02 10 37.54 +19° 30′ 01.5″ 5.68 −0.87 665 M3III semiregular variable, Vmax = 5.67, Vmin = 5.74, P = 5.0320 d
19 Ari 19 13596 10328 02 13 03.25 +15° 16′ 47.7″ 5.72 −0.38 541 M0III suspected variable, Vmax = 5.68, Vmin = 5.76
μ Ari μ 34 16811 12640 02 42 21.92 +20° 00′ 41.7″ 5.74 0.66 338 A0V
55 Ari 55 19548 14677 03 09 36.73 +29° 04′ 37.6″ 5.74 −1.96 1128 B8III
7 Ari 7 RR 11763 8993 01 55 51.03 +23° 34′ 38.4″ 5.76 −0.26 522 K1III not variable
ρ Ari ρ 45 RZ 18191 13654 02 55 48.50 +18° 19′ 54.0″ 5.76 0.30 403 M6IIIvar semiregular variable, Vmax = 5.45, Vmin = 6.01
ο Ari ο 37 17036 12803 02 44 32.97 +15° 18′ 42.8″ 5.78 −0.07 482 B9Vn
56 Ari 56 SX 19832 14893 03 12 14.24 +27° 15′ 25.2″ 5.78 0.50 371 B9p Si prototype SX Ari variable, Vmax = 5.75, Vmin = 5.81, P = 0.727902 d
20 Ari 20 13871 10540 02 15 45.94 +25° 46′ 59.2″ 5.79 2.77 131 F6IV-V
47 Ari 47 18404 13834 02 58 05.08 +20° 40′ 07.7″ 5.80 3.29 104 F5IV suspected variable
1 Ari A 1 11154 8544 01 50 08.58 +22° 16′ 31.3″ 5.83 −0.40 574 K1III+... binary star
40 Ari 40 17459 13108 02 48 32.06 +18° 17′ 01.9″ 5.83 −0.11 502 K1III
4 Ari 4 10982 8387 01 48 10.90 +16° 57′ 20.3″ 5.86 1.14 287 B9.5V
HD 15524 15524 11670 02 30 32.31 +25° 14′ 06.8″ 5.88 2.34 166 F6IV
HD 12139 12139 9307 01 59 35.60 +21° 03′ 31.0″ 5.89 0.45 399 K0III-IV
HR 830 (16) VZ 17471 13121 02 48 45.87 +25° 11′ 17.1″ 5.89 0.14 460 A0V 16 Trianguli; Alpha² CVn variable, Vmax = 5.82, Vmin = 5.89
1 Ari B 1 11155 01 50 08.50 +22° 16′ 33.0″ 5.90 component of the 1 Ari system
49 Ari 49 18769 14109 03 01 54.15 +26° 27′ 44.4″ 5.91 1.82 214 A3m suspected variable, Vmax = 5.90, Vmin = 5.94
59 Ari 59 20618 15514 03 19 55.81 +27° 04′ 16.7″ 5.91 1.91 205 G8IV
54 Cet (54) 11257 8588 01 50 52.01 +11° 02′ 36.4″ 5.93 2.77 139 F2Vw suspected variable, Vmax = 5.93, Vmin = 5.97
HD 18700 18700 14036 03 00 44.09 +10° 52′ 13.7″ 5.93 0.27 441 K6
HD 13522 13522 10296 02 12 37.51 +24° 10′ 04.1″ 5.96 −0.23 565 K0
HD 12479 12479 9533 02 02 35.08 +13° 28′ 36.2″ 5.97 −1.10 845 M2III suspected variable
HD 19698 19698 14764 03 10 38.78 +11° 52′ 21.7″ 5.97 −0.05 522 B8V
29 Ari 29 15814 11843 02 32 54.15 +15° 02′ 04.1″ 6.00 3.71 94 F8V
11 Ari 11 12885 9859 02 06 49.22 +25° 42′ 16.5″ 6.01 −1.75 1160 B9IV-Vn
16 Ari 16 13363 10203 02 11 12.06 +25° 56′ 13.0″ 6.01 −0.94 801 K4III
HD 19637 19637 14748 03 10 27.04 +26° 53′ 45.9″ 6.02 0.54 406 K3III
66 Ari 66 21467 16181 03 28 26.57 +22° 48′ 15.4″ 6.03 1.83 226 K0IV
65 Ari 65 21050 15870 03 24 26.11 +20° 48′ 12.6″ 6.07 1.23 303 A1V
HD 12140 12140 9295 01 59 25.88 +12° 17′ 41.8″ 6.09 1.51 269 A6V
HD 19789 19789 14821 03 11 21.93 +13° 02′ 52.1″ 6.11 0.99 344 K0IIIp
53 Ari 53 UW 19374 14514 03 07 25.69 +17° 52′ 47.9″ 6.13 −0.69 755 B1.5V not variable; runaway star
HD 15152 15152 11415 02 27 07.26 +27° 00′ 45.3″ 6.14 0.37 464 K5III suspected variable
26 Ari 26 UU 15550 11678 02 30 38.37 +19° 51′ 19.4″ 6.14 1.94 226 A9V δ Sct variable, Vmax = 6.10, Vmin = 6.15, P = 0.0676 d
60 Ari 60 20663 15557 03 20 25.57 +25° 39′ 46.7″ 6.14 1.40 289 K3III:
HD 15385 15385 11578 02 29 13.63 +23° 28′ 08.7″ 6.20 1.65 264 A5m
27 Ari 27 15596 11698 02 30 54.38 +17° 42′ 14.6″ 6.21 1.30 313 G5III-IV
HD 12594 12594 9627 02 03 42.61 +18° 15′ 11.8″ 6.24 −1.83 1342 K4III
54 Ari 54 19460 14586 03 08 21.09 +18° 47′ 42.3″ 6.25 0.03 570 M0III semiregular variable, Vmax = 6.25, Vmin = 6.28
HD 17918 17918 13448 02 53 11.66 +16° 29′ 01.0″ 6.30 1.14 352 F5III
85 Cet (85) 16861 12647 02 42 28.95 +10° 44′ 30.4″ 6.32 0.74 426 A2V suspected variable, Vmax = 6.28, Vmin = 6.34
HD 16955 16955 12744 02 43 51.25 +25° 38′ 18.0″ 6.35 1.19 352 A3V
HD 19080 19080 14318 03 04 40.65 +15° 51′ 22.5″ 6.37 −0.06 631 K3III
HD 18928 18928 14232 03 03 30.11 +28° 16′ 11.8″ 6.38 2.89 163 F0V
HD 13201 13201 10050 02 09 23.03 +17° 13′ 28.7″ 6.40 3.43 128 F5V
HD 20367 20367 15323 03 17 40.0468 +31° 07′ 37.9″ 6.40 4.23 88 G0V has a planet (b)
HD 19549 19549 14649 03 09 20.10 +20° 45′ 40.1″ 6.41 0.45 506 K2
HD 19600 19600 14719 03 10 08.83 +27° 49′ 11.6″ 6.42 0.09 601 A0V
HD 14262 14262 10795 02 18 57.96 +23° 10′ 04.2″ 6.45 1.34 343 A7V
36 Ari 36 17017 12784 02 44 19.09 +17° 45′ 50.5″ 6.46 0.89 413 K2III suspected variable, ΔV = 0.07
UX Ari UX 21242 16042 03 26 35.36 +28° 42′ 55.2″ 6.47 2.97 164 G5IV RS CVn variable, Vmax = 6.35, Vmin = 6.71, P = 6.388 d
30 Ari A 30 16246 12189 02 37 00.44 +24° 38′ 50.1″ 6.48 3.46 131 F6III binary star
HD 14067 14067 10657 02 17 10.4 +23° 46′ 04″ 6.51 0.44 533 G9 III has a planet (b)
51 Ari 51 18803 14150 03 02 25.87 +26° 36′ 34.7″ 6.62 4.99 69 G8V
VW Ari VW 15165 11390 02 26 45.65 +10° 33′ 55.1″ 6.69 1.16 416 F0IV δ Sct variable, Vmax = 6.64, Vmin = 6.76, P = 0.1606 d
AF Ari AF 14595 11035 02 22 06.62 +22° 52′ 24.9″ 6.71 0.50 615 G3III Algol type variable, Vmax = 6.30, Vmin = 7.10, P = 153 d
VY Ari VY 17433 13118 02 48 43.72 +31° 06′ 54.7″ 6.76 3.65 136.5 K0 RS CVn variable, Vmax = 6.68, Vmin = 7.15, P = 16.1996 d
50 Ari 50 18654 14021 03 00 31.50536 +18° 00′ 17.9143″ 6.80 A0V
23 Ari 23 14305 10810 02 19 08.72041 +19° 41′ 15.7463″ 6.83 F8V
52 Ari B 52 19135 03 05 26.70 +25° 15′ 19.0″ 7.00 component of the 52 Ari system
ρ Ari ρ 44 18091 13579 02 54 55.17 +17° 44′ 05.3″ 7.01 2.10 313 A3
30 Ari B 30 16232 12184 02 36 57.64 +24° 38′ 53.1″ 7.09 4.11 129 F6V component of the 30 Ari system; has a planet (b)
R Ari R 13913 10576 02 16 07.11 +25° 03′ 23.7″ 7.40 -2.99 3900 M3-6e Mira variable, Vmax = 7.1, Vmin = 14.3, P = 185.67 d
HD 12661 12661 9683 02 04 34.29 +25° 24′ 51.5″ 7.44 4.59 121 K0V has two planets (b & c)
HD 17674 17674 13291 02 51 04.3 +30° 17′ 12″ 7.56 145 G0V has two planets (b)
HD 14787 14787 11130 02 50 53.0 +29° 01′ 21″ 7.63 390 G5 has a planet (b)
HIP 14810 14810 03 11 14.23 +21° 05′ 50.5″ 8.52 4.90 172 G5V has three planets (b, c & d)
BD +20°307 8920 01 54 50.79 +21° 18′ 22.5″ 9.01 4.19 300 G0V has a circumstellar disk
X Ari X 19510 14601 03 08 30.89 +10° 26′ 45.2″ 9.04 -1.23 3700 F0.5 RR Lyr variable, Vmax = 9.036, Vmin = 9.966, P = 0.6511796 d
RX Ari RX 02 15 20.78 +22° 34′ 11.1″ 9.41 F2V Algol variable, Vmax = 9.40, Vmin = 10.1, P = 1.029626 d
HAT-P-47 02 33 14.0 +30° 21′ 38″ 10.6 874 has a transiting planet (b)
SS Ari SS 02 04 18.41 +24° 00′ 02.2″ 10.15 3.52 692 G0 W UMa variable, Vmax = 10.10, Vmin = 10.63, P = 0.40598257 d
TT Ari TT 02 06 53.08 +15° 17′ 41.8″ 10.2 Bep: VY Scl star, Vmax = 10.2, Vmin = 16.5, P = 0.137551 d
RV Ari RV 02 15 07.50 +18° 04′ 27.9″ 11.61 A0 double-mode δ Sct variable, Vmax = 11.61, Vmin = 12.30, P = 0.0931281 d
WASP-11/HAT-P-10 03 09 28.55 +30° 40′ 24.9″ 11.89 6.41 408 K3V has a transiting planet (b)
HAT-P-48 02 57 53.0 +30° 37′ 33″ 12.16 995 has a transiting planet (b)
L 1159-16 TZ 02 00 12.79 +13° 03′ 11.2″ 12.26 13.99 14.5 M4.5 flare star and BY Dra variable
LkHα 264 WY 02 56 37.56 +20° 05′ 37.1″ 12.46 K5/6e T Tau star, Vmax = 12.25, Vmin = 12.88
RW Ari RW 02 16 03.72 +17° 31′ 59.0″ 12.51 B8 RR Lyr variable, Vmax = 12.12, Vmin = 12.60, P = 0.3543006 d
HAT-P-25 03 13 45 +25° 11′ 51″ 13.19 5.83 969 G5 has a transiting planet (b)
HAT-P-52 02 50 53.0 +29° 01′ 21″ 14.07 6.14 1256 has a transiting planet (b)
WX Ari WX 02 47 36.22 +10° 35′ 37.7″ 15.3 CV VY Scl star and eclipsing binary, Vmax = 14.5, Vmin = <16.7, P = 0.1393512 d
Teegarden's star 02 53 00.89 +16° 52′ 52.7″ 15.40 17.47 12.6 M7.5
XY Ari XY 02 56 08.19 +19° 26′ 34.1″ WD+M0V DQ Her variable and eclipsing binary
PSR B0301+19 03 04 33.12 +19° 32′ 51.4″ 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 mv), also known as apparent magnitude
 • abs. mag. = absolute magnitude (Mv)
 • 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

See also

References

  1. Knobel, E. B. (1895). "1895MNRAS..55..429K Page 432". Monthly Notices of the Royal Astronomical Society. 55: 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
  2. ^ Consisting with δ Ari (Botein), ε Ari, ζ Ari, π Ari, and ρ Ari, were Al Buṭain, the dual of Al Baṭn, the Belly. See Star Name – R.H.Allen p. 83
  3. ^ δ Ari as Nir al Botain or Lucida Ventris (the brightest of the belly). ε Ari, ζ Ari, π Ari, and ρ Ari was not designated by Al Achsasi Al Mouakket. Jack W. Rhoads was designated these stars of Al Buṭain were Al Buṭain I (π Ari), Al Buṭain II (ρ Ari), Al Buṭain III (ε Ari) and Al Buṭain IV (ζ Ari)
  4. SIMBAD, 50 Arietis (Retrieved 27 July 2012)
  5. Abt, Helmut A. (2008). "Visual Multiples. IX. MK Spectral Types". The Astrophysical Journal Supplement Series. 176 (1): 216–217. Bibcode:2008ApJS..176..216A. doi:10.1086/525529.
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