HD 63332
Appearance
Coordinates: 07h 51m 05.7s, +54° 07′ 45.3″
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lynx[1] |
Right ascension | 07h 51m 05.71s[2] |
Declination | +54° 07′ 45.3″[2] |
Apparent magnitude (V) | 6.02±0.009[2] |
Characteristics | |
Evolutionary stage | F-type main-sequence star |
Spectral type | F6V[3] |
Apparent magnitude (B) | 6.493[2] |
Apparent magnitude (G) | 5.913[2] |
Apparent magnitude (J) | 5.116[2] |
Apparent magnitude (H) | 4.914[2] |
Apparent magnitude (K) | 4.861[2] |
B−V color index | 0.496±0.004[4] |
Absolute magnitude (MV) | 3.66[6] |
Details | |
Gyr | |
J07510571+5407452 | |
Database references | |
SIMBAD | data |
HD 63332 is an
apparent brightness of 6.02,[2] meaning that it is faintly visible to the naked eye under dark skies.[10] Parallax measurements derive a distance of 29.6 parsecs (97 light-years) to HD 63332.[4] Considering the apparent magnitude and distance from Earth, the star's absolute magnitude is 3.66.[6] No debris disks or exoplanets were detected around it.[11][12]
Characteristics
The star has a
HD 63332 is located in the
thin disk population of the Milky Way,[11] being located at a maximum distance of 60 parsecs (200 ly) from the galactic plane.[6] Its orbit around the galaxy has a low eccentricity of 0.06.[6]
No
siderophiles and iron.[14] The habitable zone is located at a distance of 1.63 astronomical units from the star.[7]
Notes
- ^ The Solar System's age is 4.568 billion years.
References
- ^ a b Ford, Dominic. "HIP-38325 (Star)". In-The-Sky.org. Retrieved 2024-05-14.
- ^ a b c d e f g h i "HD 63332". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-05-14.
- ^ in VizieR.
- ^ in VizieR.
- ^ in VizieR.
- ^ in VizieR.
- ^ in VizieR.
- ^ in VizieR.
- ^ at VizieR.
- ^ a b "University Lowbrow Astronomers Naked Eye Observer's Guide". websites.umich.edu. Retrieved 2024-05-14.
- ^ in VizieR.
- ^ in VizieR.
- ^ "The Colour of Stars". Australia Telescope National Facility. 6 March 2024. Retrieved May 14, 2024.
- in VizieR.