Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Norma |
Right ascension | 15h 49m 37.69382s[1] |
Declination | –49° 57′ 48.6771″[1] |
Apparent magnitude (V) | 9.36[2] |
Characteristics | |
Spectral type | G5[3] |
B−V color index | 0.935±0.005[2] |
Astrometry | |
Radial velocity (Rv) | 61.67±0.24[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] |
Distance | 147.9 ± 0.3 ly (45.36 ± 0.09 pc) |
Absolute magnitude (MV) | 5.89[2] |
Details | |
Mass | 0.86±0.02[4] M☉ |
Radius | 0.85+0.02 −0.03[1] R☉ |
Luminosity | 0.393±0.001[1] L☉ |
Surface gravity (log g) | 4.68±0.09[4] cgs |
Temperature | 4,967+88 −65[1] K |
Metallicity [Fe/H] | 0.18±0.04[4] dex |
Age | 5.30±4.22[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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 111.5 light-years 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]
GaiaDR2
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was invoked but never defined (see the help page).