Delta Equulei

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Template:Short description

Delta Equulei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Equuleus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.19 + 5.52[2]
Characteristics
Spectral type F7V + F7V[3]
U−B Template:Engvar −0.03[4]
B−V Template:Engvar +0.49[4]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: +42.39[1] mas/yr
Dec.: −304.19[1] mas/yr
Parallax (π)54.89±0.50 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+3.14[6]
Orbit[7]
Period (P)Script error: No such module "val".
Semi-major axis (a)Script error: No such module "val".
Eccentricity (e)Script error: No such module "val".
Inclination (i)Script error: No such module "val".°
Longitude of the node (Ω)Script error: No such module "val".°
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Details
δ Equ A
MassScript error: No such module "val".[7] Template:Solar mass
RadiusScript error: No such module "val".[3] Template:Solar radius
Luminosity2.25[3] Template:Solar luminosity
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]Script error: No such module "val".[3] dex
Age3.0[5] Gyr
δ Equ B
MassScript error: No such module "val".[7] Template:Solar mass
RadiusScript error: No such module "val".[3] Template:Solar radius
Luminosity2.07[3] Template:Solar luminosity
TemperatureScript error: No such module "val".[3] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
δ Equ, 7 Equulei, BD+09°4746, GJ 822.0, HD 202275, HIP 104858, HR 8123, LTT 16227, SAO 126643[8]
Database references
SIMBADdata

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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 years away,[9] with components of class G0 and F5.[10] Their combined magnitude is 4.47, and their absolute magnitude is 3.142. There is controversy as to the exact masses of the stars. One study puts the larger at 1.22 solar masses and the smaller at 1.17, while another pegs them at 1.66 and 1.593.[10] The luminosity of the larger star is calculated to be 2.23 solar, and the smaller to be 2.17.[10]

System

William Herschel listed Delta Equulei as a wide binary. Friedrich Georg Wilhelm von Struve later showed this to be an unrelated optical double star. However his son Otto Wilhelm von Struve while making follow-up observations in 1852 found that while the separation of the optical double continued to increase, Delta Equulei itself appeared elongated. He concluded that it is a much more compact binary.[11]

References

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External links

Template:Stars of Equuleus