HD 33283

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Template:Short description

HD 33283
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lepus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 8.05[2]
Characteristics
Spectral type G3/5V[2] + M4–5[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val".[1] mas/yr
Dec.: Script error: No such module "val".[1] mas/yr
Parallax (π)11.0993±0.0286 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.19[2]
Details
HD 33283
MassScript error: No such module "val".[4]
Script error: No such module "val".[5] Template:Solar mass
RadiusScript error: No such module "val".[4]
Script error: No such module "val".[5] Template:Solar radius
LuminosityScript error: No such module "val".[4] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[4] cgs
TemperatureScript error: No such module "val".[4] K
Metallicity [Fe/H]Script error: No such module "val".[2] dex
Rotational velocity (v sin i)Script error: No such module "val".[6] km/s
AgeScript error: No such module "val".[4] Gyr
HD 33283 B
Mass0.17[3] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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HD 33283 is a star in the southern constellation Lepus with one planet and a co-moving stellar companion.[3] With an apparent visual magnitude of 8.05,[2] the star is too faint to be seen with the naked eye. It is located at a distance of 294 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +4.5.[2]

This is an ordinary G-type main-sequence star with a stellar classification of G3/5V.[2] It is about 3.6 billion years old and is chromospherically inactive. The star is spinning slowly with a projected rotational velocity of 1 km/s[6] and an estimated rotation period of about 55.5 days.[5] It is larger and more massive than the Sun. HD 33283 is radiating over four times the luminosity of the Sun from its photosphere at an effective temperature of 5,985 K.[4]

In 2014, a co-moving red dwarf companion star, HD 33283 B, of spectral class M4–M5 was detected at an angular separation of Script error: No such module "val"., corresponding to a projected separation of Script error: No such module "val"..[3]

Planetary system

In 2006, J. A. Johnson and associates found a jovian planet orbiting HD 33283 with the radial velocity method.[5] It is orbiting at a distance of Script error: No such module "convert". from the host star with a period of 18.2 days and an eccentricity (ovalness) of 0.4.[8]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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External links

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Template:Sky Template:Stars of Lepus