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Variable star in the constellation of Equuleus
R Equulei is a class M Mira variable star in the constellation Equuleus. Its brightness varies between a minimum magnitude of 15.0 to a maximum of 8.7
R_Equulei
Constellation in the northern celestial hemisphere
6.1, 6 Equulei. It is divisible in binoculars. 6 Equulei is an astrometric binary system itself, with an apparent magnitude of 6.07. R Equulei is a Mira
Equuleus
Star in the constellation Equuleus
Alpha Equulei (α Equulei, abbreviated Alpha Equ, α Equ), officially named Kitalpha /kɪˈtælfə/, is the brightest star in the constellation of Equuleus.
Alpha_Equulei
Chemically peculiar A-type main sequence star in the constellation Equuleus
Gamma Equulei, Latinized from γ Equulei, is a double star in the northern constellation of Equuleus. It is located at a distance of around 118 light-years
Gamma_Equulei
Star in the constellation Equuleus
Epsilon Equulei, Latinized from ε Equulei, is a star system of apparent magnitude +5.23 in the constellation of Equuleus. It is located 180 light years
Epsilon_Equulei
Star in the constellation Equuleus
Beta Equulei, Latinized from β Equulei, is the Bayer designation for a solitary star in the northern constellation of Equuleus. It is faintly visible
Beta_Equulei
Star in the constellation Equuleus
Delta Equulei, also named Tepennekhet, is the second brightest star in the constellation Equuleus. Delta Equulei is a binary star system about 60 light-years
Delta_Equulei
Star in the constellation Equuleus
9 Equulei is an M-type star in the constellation Equuleus. It is an asymptotic giant branch (AGB) star, a star that has exhausted its core helium and
9_Equulei
K-type giant star in the constellation Equuleus
3 Equulei is a single star located in the small northern constellation of Equuleus. It is faintly visible to the naked eye at an apparent visual magnitude
3_Equulei
Double star system in the constellation Equuleus
2 Equulei is a double star system in the constellation of Equuleus. The primary component of the 2 Equulei pair is an F-type star. As of 2015, the secondary
2_Equulei
Binary star system in the constellation Equuleus
331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release
HD_199942
Star in the constellation Equuleus
331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3.
HD_200661
Star in the constellation Equuleus
6 Equulei, also named Protome, is a probable (95% chance) astrometric binary star system in the northern constellation of Equuleus, located 440 light
6_Equulei
High proper motion star in the constellation Equuleus
has 1.45 times the mass of the Sun and a slightly enlarged radius of 2.2 R☉ due to its evolved state. It shines with a luminosity of about 9 L☉ from
HD_201507
Star in the constellation Equuleus
331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3.
HD_203842
High proper motion star; Equuleus
1365-2966.2009.16182.x. eISSN 1365-2966. ISSN 0035-8711. Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Robinson, P. E. (October 2003). "Contributions
HD_200779
Star in the constellation Equuleus
4 Equulei is a binary star system in the constellation of Equuleus, located about 3° to the east of Alpha Equulei. With an apparent visual magnitude of
4_Equulei
Variable star in the constellation Equuleus
U Equulei (U Equ / IRAS 20547+0247) is a variable star in the Equuleus constellation with an apparent magnitude of +14.50 in the B band. It lies at an
U_Equulei
Type of star larger than main-sequence but smaller than a giant
β Aurigae, λ Ursae Majoris, β Serpentis, α Ophiuchi A3: δ Herculis, β Equulei, F2: δ Geminorum, ζ Serpentis F5: Procyon, 110 Herculis, η Scorpii F6:
Subgiant
H. Jr. (November 1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally
List_of_proper_names_of_stars
Star in the constellation Equuleus
331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3.
HD_200964
High galactic latitude β Cephei variable
SY Equulei, also known as HD 203664, is a single variable star located in the equatorial constellation Equuleus. It has an average apparent magnitude
SY_Equulei
Double star in the constellation Aquarius
(asterism), refers to an asterism consisting of Beta Aquarii and Alpha Equulei. Consequently, the Chinese name for Beta Aquarii itself is 虛宿一 (Xū Xiù
Beta_Aquarii
doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR. Barry, Don C. (January 1970), "Spectral Classification of a and F Stars"
List of star systems within 400–450 light-years
List_of_star_systems_within_400–450_light-years
within 65–70 light-years List of nearest stars and brown dwarfs "Delta Equulei". University of Illinois Astronomy department. Archived from the original
List of star systems within 60–65 light-years
List_of_star_systems_within_60–65_light-years
Double star in the constellation Delphinus
subgiant. It has 163% of the mass of the Sun and an enlarged radius of 7.71 R☉. It shines at 36.5 times the luminosity of the Sun from its photosphere at
HD_199223
Zodiac constellation straddling the celestial equator
with the constellation Xu ("emptiness"), formed by Beta Aquarii and Alpha Equulei; it represented a bleak place associated with death and funerals. Wei,
Aquarius_(constellation)
Star in the constellation Equuleus
solitary star located in the northern constellation Equuleus, just next to 3 Equulei. It has an apparent magnitude of 6.14, making it barely visible to the
HD_201298
Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (March 2021). "Estimating distances from parallaxes. V: Geometric and photogeometric
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR. Barry, Don C. (January 1970), "Spectral Classification of a and F Stars"
List of star systems within 350–400 light-years
List_of_star_systems_within_350–400_light-years
Constellations that are no longer widely recognised
cartography. New York, New York: Springer. p. 131. ISBN 978-0-387-71668-8. Gent, R.H. van. "A Pair of Puzzling Star Maps and Two Unknown Constellations". webspace
Former_constellations
doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR. Barry, Don C. (January 1970), "Spectral Classification of a and F Stars"
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Bibcode:2025A&A...697A..32S. doi:10.1051/0004-6361/202453500. Ducati, J. R. (2002), "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's
List_of_exoplanet_extremes
Constellations recognized by the International Astronomical Union
Tales: Constellation Mythology and History – Ian Ridpath's Star Tales. VizieR – CDS's archive of constellation boundaries. The text file constbnd.dat gives
IAU_designated_constellations
The guide to the galaxy. CUP Archive. p. 31. ISBN 0-521-45882-X. Kepple, G. R.; Sanner, G. W. (1998). The Night Sky Observer's Guide. Vol. 1. Willmann-Bell
List_of_Arabic_star_names
Star in the constellation Aries
Arietis, EZ Ursae Majoris, and 4 Equulei", The Observatory, 131 (5): 294–314, Bibcode:2011Obs...131..294G. Luck, R. Earle (2015), "Abundances in the
27_Arietis
Astronomical observatory in Ontario, Canada
was also used in the published search for variability in the stars Gamma Equulei and HD 149728, using 1958 and 1959 data from the refracting telescope.
Hume Cronyn Memorial Observatory
Hume_Cronyn_Memorial_Observatory
331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Statistical technique
"MOST photometry and modeling of the rapidly oscillating (roAp) star γ Equulei". Astronomy and Astrophysics. 480 (1): 223–232. arXiv:0801.0863. Bibcode:2008A&A
SigSpec
Star in the constellation Boötes
ISBN 978-3-319-22794-8. Wehlau, William (August 1962). "Photometry of γ Equulei and HD 140728". Publications of the Astronomical Society of the Pacific
BP_Boötis
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