7 Camelopardalis

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Template:Short description

7 Camelopardalis
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Camelopardalis
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.43[2] (4.49 + ? + 7.90 + 11.30)[3]
Characteristics
Evolutionary stage main sequence
Spectral type A1 V[4]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: −24.51[1] mas/yr
Dec.: +7.71[1] mas/yr
Parallax (π)8.77±0.60 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.84[2]
Orbit[6]
Primary7 Cam Aa
Companion7 Cam Ab
Period (P)3.884 d
Eccentricity (e)0
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Details
7 Cam Aa
MassScript error: No such module "val".[7] Template:Solar mass
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
TemperatureScript error: No such module "val".[7] K
Rotational velocity (v sin i)40[7] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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7 Camelopardalis is a multiple star system[9] in the northern circumpolar constellation of Camelopardalis. It is located approximately 370 light years from the Sun, as determined from its parallax.[1] This system is visible to the naked eye as a faint, white-hued star with a combined apparent visual magnitude of 4.43.[2] It is moving closer to the Earth with a heliocentric radial velocity of −10 km/s.[5]

The primary member of the group, designated component A, is a single-lined spectroscopic binary system with a circular orbit and a period of 3.88 days.[6] The visible component of this pair is a magnitude 4.49[3] A-type main-sequence star with a stellar classification of A1 V.[4] It has 3.2 times the mass of the Sun and is spinning with a projected rotational velocity of 40 km/s. The star is radiating 222 times the Sun's luminosity from its photosphere at an effective temperature of 9,226 K.[7]

The magnitude 7.90[3] component B has an orbital solution with the Aa/Ab pair, which yields a period of 284 years and an eccentricity of 0.74. However, Drummond (2014) found the data to be discordant and instead determined that they are an optical pair with no physical association.[10] The fourth member, component C, is a magnitude 11.30 star at an angular separation of Script error: No such module "val". along a position angle of 242° from the primary, as of 2003.[3] It shares a common proper motion with the primary star.[11]

References

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  4. a b Script error: No such module "citation/CS1".
  5. a b Script error: No such module "citation/CS1".
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  11. Template:Cite Gaia EDR3

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Template:Stars of Camelopardalis