HD 63332
F-type star in the constellation Lynx
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HD 63332 is an F-type main-sequence star in the constellation Lynx. The star has 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]
 | |
| 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] |
| Astrometry | |
| Radial velocity (Rv) | 1.331±0.157[5] km/s |
| Proper motion (μ) | RA: -39.538 mas/yr[5] Dec.: 53.894 mas/yr[5] |
| Parallax (π) | 33.78±0.39 mas[4] |
| Distance | 97 ± 1 ly (29.6 ± 0.3 pc)[4] |
| Absolute magnitude (MV) | 3.66[6] |
| Details | |
| Mass | 1.3[7] M☉ |
| Radius | 1.375[4] R☉ |
| Luminosity | 2.671[4] L☉ |
| Surface gravity (log g) | 4.27[8] cgs |
| Temperature | 6,298[4] K |
| Metallicity [Fe/H] | -0.12[6]–+0.09[8] dex |
| Rotational velocity (v sin i) | 9[9] km/s |
| Age | 2.1[8] or 3.1[6] Gyr |
| Other designations | |
| BD+54 1177, HD 63332, HIP 38325, HR 3028, SAO 26535, PPM 31335, TIC 53336409, TYC 3783-1422-1, GSC 03783-01422, IRAS 07471+5415, 2MASS J07510571+5407452, Gaia DR2 984918228123275776, Gaia DR3 984918228123275776 | |
| Database references | |
| SIMBAD | data |
Characteristics
The star has a spectral classification of F6V,[3] meaning that is a F-type main-sequence star that is currently fusing hydrogen into helium in its core. It has 1.3 times the mass[7] and 1.375 times the radius of the Sun.[4] HD 63332 is 2.67 times more luminous than the Sun, emitting this energy from its photosphere at an effective temperature of 6,298 K, which is around 9% hotter than the Sun.[4] Its age is estimated at 2.1[8] or 3.1 billion years,[6] equivalent to 46% and 68% of the Solar System's age respectively,[a] and it rotates under its own axis at a velocity of 9 km/s.[9] The B-V color index of the star is 0.496, giving it the yellowish-white color of a late F-type star.[4][13]
HD 63332 is located in the northern hemisphere, 97 light-years from Earth,[4] within the constellation Lynx.[1] It has an apparent magnitude of 6.02, which makes it faintly visible to the naked eye, under dark skies.[10] The absolute magnitude, i.e. its brightness if it was seen at 10 pc (32.6 ly), is 3.66.[6] The star makes part of 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 debris disks have been detected around it as of 2016,[12] and no exoplanets were detected around it as of 2012.[11] It has a 27% possibility of hosting an exoplanet made up of volatiles, lithophiles, 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.