Zeta Pictoris

Star in the constellation Pictor From Wikipedia, the free encyclopedia

ζ Pictoris, Latinised as Zeta Pictoris, is a solitary[10] star in the southern constellation of Pictor. It is visible to the naked eye with an apparent visual magnitude of +5.43.[2] Based upon an annual parallax shift of 28.00 mas as seen from the Earth,[1] the system is located 116.5 light years from the Sun.

Quick Facts Constellation, Right ascension ...
Zeta Pictoris
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Pictor
Right ascension 05h 19 22.13548m [1]
Declination −50° 36 21.4820[1]
Apparent magnitude (V) +5.43[2]
Characteristics
Spectral type F6 IV[3]
U−B color index +0.01[2]
B−V color index +0.52[2]
Astrometry
Radial velocity (Rv)+43.8±0.2[4] km/s
Proper motion (μ) RA: +23.64[1] mas/yr
Dec.: +227.43[1] mas/yr
Parallax (π)28.00 ± 0.23 mas[1]
Distance116.5 ± 1.0 ly
(35.7 ± 0.3 pc)
Absolute magnitude (MV)2.65±0.04[5]
Details[6]
Mass1.39 M
Radius5.3[7] R
Surface gravity (log g)4.07±0.07 cgs
Temperature6,411±56 K
Metallicity [Fe/H]0.07 dex
Rotational velocity (v sin i)5.6±1.0[8] km/s
Age2.6 Gyr
Other designations
ζ Pic, CD−50° 1723, HD 35072, HIP 24829, HR 1767, SAO 233926[9]
Database references
SIMBADdata
Close

This is an evolving F-type subgiant star with a stellar classification of F6 IV.[3] It is a thin disk[11] star with an estimated 1.4[6] times the mass of the Sun and about 5.3[7] times the Sun's radius. At the age of 2.6[6] billion years, Zeta Pictoris is spinning with a projected rotational velocity of 5.6 km/s.[8]

References

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