HD 330075

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Template:Short description

HD 330075
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Norma
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 9.36[2]
Characteristics
Spectral type G5[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: -232.760[1] mas/yr
Dec.: -92.540[1] mas/yr
Parallax (π)22.0467±0.0443 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)5.89[2]
Details
MassScript error: No such module "val".[4] Template:Solar mass
RadiusScript error: No such module "val".[1] Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[4] cgs
TemperatureScript error: No such module "val".[1] K
Metallicity [Fe/H]Script error: No such module "val".[4] dex
AgeScript error: No such module "val".[4] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[5]
Database references
SIMBADdata

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HD 330075 is a star in the southern constellation of Norma. It has a yellow hue and an apparent visual magnitude of 9.36,[2] which makes it too faint to be seen with the naked eye – it is visible only with telescope or powerful binoculars. Parallax measurements provide a distance estimate of 148 light years from the Sun, and it is drifting further away with a radial velocity of 62 km/s.[1] The star is estimated to have come as close as Script error: No such module "convert". some 409 million years ago.[2]

This object appears to be a slightly evolved dwarf with a spectral class of G5. That is, it is nearing the end of its main sequence lifetimes and is becoming a subgiant star. The star has very low chromospheric activity and is around five billion years old.[3] It is smaller than the Sun with 86%[4] of the Sun's mass and 85%[1] of the solar radius. As a consequence, it is radiating just 39% of the luminosity of the Sun from its photosphere at an effective temperature of 4,967 K.[1] It has a super-solar metallicity, which means the abundance of elements other than hydrogen and helium appears much higher than in the Sun.[4]

Planetary system

In 2004, the discovery of a hot Jupiter planet orbiting close to the star was announced. This is the first planet discovered by the then-new HARPS spectrograph.[3]

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 Norma