Zeta Serpentis
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000 Equinox J2000 |
|
---|---|
Constellation | Serpens |
Right ascension | 18h 00m 29.0s[1] [2] |
Declination | −03° 41′ 25″[1] [2] |
Apparent magnitude (V) | 4.63 [3] |
Characteristics | |
Spectral type | F2V [4] |
B−V color index | +0.36 [3] |
Astrometry | |
Radial velocity (Rv) | -50.70[5] km/s |
Proper motion (μ) | RA: +155.51[2] mas/yr Dec.: -44.43[2] mas/yr |
Parallax (π) | 42.46 ± 0.34[2] mas |
Distance | 76.8 ± 0.6 ly (23.6 ± 0.2 pc) |
Absolute magnitude (MV) | 2.77 [6] |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Serpentis (ζ Ser, ζ Serpentis) is a star in the constellation Serpens.
Zeta Serpentis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.63.[3] It is approximately 76.8 light years from Earth.[2] This star has nearly double the radius of the Sun and is radiating 6.3 times the Sun's luminosity from its outer atmosphere at an effective temperature of 6,529 K.[1]
References
- ↑ 1.0 1.1 1.2 Lua error in package.lua at line 80: module 'strict' not found.. See Table 10.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Lua error in package.lua at line 80: module 'strict' not found. Vizier catalog entry
- ↑ 3.0 3.1 3.2 3.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Absolute magnitude calculated as
, where
is the star's absolute magnitude,
is the star's apparent magnitude, and
is the star's measured parallax in arcseconds.
<templatestyles src="Asbox/styles.css"></templatestyles>