Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Equuleus
Right ascension
21h 10m 31.31996s[1]
Declination
10° 02′ 56.1180″[1]
Apparent magnitude (V)
6.07[2]
Characteristics
Evolutionary stage
main sequence[3]
Spectral type
A2 Vs[3] (A1 Si Sr Cr)[4]
U−B color index
+0.04[2]
B−V color index
+0.02[2]
Astrometry
Radial velocity (Rv)
+6.9[5] km/s
Proper motion (μ)
RA: –2.696[1] mas/yr Dec.: +15.802[1] mas/yr
Parallax (π)
8.5862 ± 0.1086 mas[1]
Distance
380 ± 5 ly (116 ± 1 pc)
Absolute magnitude (MV)
+0.236[6]
Details
Mass
2.59±0.14[3]M☉
Radius
1.7[7]R☉
Luminosity
70.6+19.4 −15.2[3]L☉
Temperature
9,078+169 −165[3] K
Rotational velocity (v sin i)
65[3] km/s
Age
970[6] Myr
Other designations
γ Equulei D, BD+09°4735, HD 201616, HIP 104538, HR 8098, SAO 126597[8]
Database references
SIMBAD
data
6 Equulei is a probable (95% chance) astrometric binary[9] star system in the northern constellation of Equuleus, located 380 light years from the Sun. It is barely visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 6.07.[2] The system is moving further away from the Earth with a heliocentric radial velocity of +6.9 km/s.[5] It forms a wide optical double with γ Equulei, at an angular separation of 336 arcseconds in 2011.[10]
The visible component is an Ap star[3] with a stellar classification of A2Vs,[3] matching the evolutionary state of an A-type main sequence star while displaying "sharp" absorption lines. It is an estimated 970[6] million years old with a projected rotational velocity of 65 km/s.[3] The star has 2.6[3] times the mass of the Sun and around 1.7[7] times the Sun's radius. It is radiating 71[3] times the luminosity of the Sun from its photosphere at an effective temperature of 9,078 K.[3]
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6Equulei is a probable (95% chance) astrometric binary star system in the northern constellation of Equuleus, located 380 light years from the Sun. It...
magnitude 6.1, 6Equulei. It is divisible in binoculars. 6Equulei is an astrometric binary system itself, with an apparent magnitude of 6.07. R Equulei is a...
Alpha Equulei (α Equulei, abbreviated Alpha Equ, α Equ), officially named Kitalpha /kɪˈtælfə/, is a star in the constellation of Equuleus. It is a high...
Beta Equulei, Latinized from β Equulei, is the Bayer designation for a solitary star in the northern constellation of Equuleus. It is faintly visible...
two typical examples: A determination of the parallax and mass-ratio of 6Equulei by van de Kamp, Peter and Lippincott, Sarah Lee, Astronomical Journal...
Delta Equulei, Latinized from δ Equulei, is the second brightest star in the constellation Equuleus. Delta Equulei is a binary star system about 60 light...
2 Equulei is a double star system in the constellation of Equuleus. The primary component of the 2 Equulei pair is an F-type main sequence star. As of...
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...
naked eye at an apparent visual magnitude of 5.6. Based upon an annual parallax shift of 4.24 mas, 3 Equulei is roughly 770 light-years (240 parsecs) distant...
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...
and an eccentricity of 0.295. The primary component is of visual magnitude 6.23 and is a chemically-peculiar F-type main-sequence star with a class of...
star located in the constellation Equuleus. It has an apparent magnitude of 6.32, placing it near the limit for naked eye visibility, even under ideal conditions...
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...
northern constellation of Equuleus. It has an apparent visual magnitude of +6.48, which puts it at the lower limit of visibility to the naked eye, but binoculars...
SY Equulei, also known as HD 203664, is a single variable star located in the equatorial constellation Equuleus. It has an average apparent magnitude...
in the equatorial constellation Equuleus. It has an apparent magnitude of 6.41, placing it near the max naked eye visibility. The star is situated at...
in the equatorial constellation Equuleus. It has an apparent magnitude of 6.43, placing it near the limit for naked eye visibility. Parallax measurements...
batches of names were approved on 21 August, 12 September, 5 October, and 6 November 2016. These were listed in a table of 102 stars included in the WGSN's...
in the northern constellation Equuleus just next to 3 Equulei It has an apparent magnitude of 6.14, making it barely visible to the naked eye under ideal...
(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...
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....
at a position angle of 282° as of 2016. They have apparent magnitudes of 6.34 and 7.49 and distances of 354 and 359 light years respectively. The system...