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Zeta Delphini

ζ Delphini
Delphinus constellation map.svg
Red circle.svg

Location of ζ Delphini (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Delphinus
Right ascension 20h 35m 18.53563s
Declination +14° 40′ 27.1675″
Apparent magnitude (V) +4.647
Characteristics
Spectral type A3Va / L5
U−B color index +0.14
B−V color index +0.105
Astrometry
Radial velocity (Rv) −25 ± 2 km/s
Proper motion (μ) RA: 45.52 mas/yr
Dec.: 11.74 mas/yr
Parallax (π) 14.82 ± 0.23mas
Distance 220 ± 3 ly
(67 ± 1 pc)
Absolute bolometric
magnitude
 (Mbol)
0.523 / 14.59
Details
ζ Del A
Mass 2.5 ± 0.2 M
Luminosity 48.63 ± 1.66 L
Surface gravity (log g) 3.72 cgs
Temperature 8336 K
Metallicity [Fe/H] −0.05 dex
Age 525 ± 125 Myr
ζ Del B
Mass 55 ± 10 MJup
Luminosity 0.00012 ± 0.00001 L
Surface gravity (log g) 5.0+0.5
−1.0
 cgs
Temperature 1550+250
−100
 K
Age 525 ± 125 Myr
Other designations
BD+14° 4353, HD 196180, HIP 101589, HR 7871, SAO 106274
Database references
SIMBAD ζ Del
ζ Del B

Zeta Delphini (ζ Del) is a star in the constellation of Delphinus. With an apparent magnitude of about 4.6, it is faintly visible to the naked eye. Parallax measurements of the system made by the Hipparcos spacecraft put it at a distance of about 220 light-years, or 67 parsecs.

Zeta Delphini has a spectral type of A3V, implying it is an A-type main-sequence star. These types of stars are bluish-white colored, and have effective temperatures between 7100 and 11500 K: Zeta Delphini has a temperature of 8336 K. Its age is estimated to be around 500 million light years, considerably younger than the Sun.

In 2014, the discovery of a brown dwarf around Zeta Delphini was announced. Zeta Delphini B is a brown dwarf with a spectral type of L5 (but may be from L3 to L7), and has a mass of about 55 Jupiters. At over 13 arcseconds away, this brown dwarf is separated at least 910 AU from Zeta Delphini.

Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. 


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