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6 Equulei information


6 Equulei
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]
Distance380 ± 5 ly
(116 ± 1 pc)
Absolute magnitude (MV)+0.236[6]
Details
Mass2.59±0.14[3] M
Radius1.7[7] R
Luminosity70.6+19.4
−15.2
[3] L
Temperature9,078+169
−165
[3] K
Rotational velocity (v sin i)65[3] km/s
Age970[6] Myr
Other designations
γ Equulei D, BD+09°4735, HD 201616, HIP 104538, HR 8098, SAO 126597[8]
Database references
SIMBADdata

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]

  1. ^ a b c d e Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference clpl4_99 was invoked but never defined (see the help page).
  3. ^ a b c d e f g h i j k l Cite error: The named reference zorec2012 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference aaa498_3_961 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference gcsrv was invoked but never defined (see the help page).
  6. ^ a b c Cite error: The named reference wolframalpha was invoked but never defined (see the help page).
  7. ^ a b Cite error: The named reference aaa367_521 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Frankowski2007 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference wds2001 was invoked but never defined (see the help page).

and 23 Related for: 6 Equulei information

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6 Equulei

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6 Equulei is a probable (95% chance) astrometric binary star system in the northern constellation of Equuleus, located 380 light years from the Sun. It...

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Equuleus

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magnitude 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...

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Alpha Equulei

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Alpha EquuleiEquulei, abbreviated Alpha Equ, α Equ), officially named Kitalpha /kɪˈtælfə/, is a star in the constellation of Equuleus. It is a high...

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Beta Equulei

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Beta Equulei, Latinized from β Equulei, is the Bayer designation for a solitary star in the northern constellation of Equuleus. It is faintly visible...

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Sarah Lee Lippincott

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two typical examples: A determination of the parallax and mass-ratio of 6 Equulei by van de Kamp, Peter and Lippincott, Sarah Lee, Astronomical Journal...

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Delta Equulei

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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...

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2 Equulei

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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...

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Epsilon Equulei

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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...

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3 Equulei

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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...

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4 Equulei

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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...

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HD 199942

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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...

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HD 203842

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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...

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U Equulei

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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...

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HD 200964

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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...

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SY Equulei

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SY Equulei, also known as HD 203664, is a single variable star located in the equatorial constellation Equuleus. It has an average apparent magnitude...

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HD 200661

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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...

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HD 201507

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in the equatorial constellation Equuleus. It has an apparent magnitude of 6.43, placing it near the limit for naked eye visibility. Parallax measurements...

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List of proper names of stars

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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...

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HD 201298

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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...

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Beta Aquarii

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(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...

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Hume Cronyn Memorial Observatory

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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....

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HD 199223

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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...

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27 Arietis

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velocities - Paper 220: 60 Piscium, 27 Arietis, EZ Ursae Majoris, and 4 Equulei", The Observatory, 131 (5): 294–314, Bibcode:2011Obs...131..294G. Luck...

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