Theta Capricorni

Theta Capricorni
Location of θ Capricorni (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Capricornus
Right ascension 21h 05m 56.82783s
Declination −17° 13′ 58.3021″
Apparent magnitude (V) +4.07
Characteristics
Evolutionary stage main sequence
Spectral type A1 V
U−B color index +0.01
B−V color index −0.01
Astrometry
Radial velocity (Rv)−10.9 km/s
Proper motion (μ) RA: +79.33 mas/yr
Dec.: −62.01 mas/yr
Parallax (π)20.11±0.28 mas
Distance162 ± 2 ly
(49.7 ± 0.7 pc)
Absolute magnitude (MV)+0.60
Orbit
PrimaryA
NameB
Period (P)143 days
Semi-major axis (a)0.78 AU
Details
A
Mass2.54 M
Radius2.35 R
Luminosity65 L
Surface gravity (log g)4.19±0.14 cgs
Temperature10,221 K
Metallicity [Fe/H]+0.26 dex
Rotational velocity (v sin i)104 km/s
Age280 Myr
B
Mass0.56 M
Radius0.52 R
Temperature3,900 K
Age280 Myr
Other designations
Udang, Dorsum, θ Cap, 23 Cap, BD−17°6174, FK5 1552, HD 200761, HIP 104139, HR 8075, SAO 164132
Database references
SIMBADdata

Theta Capricorni, Latinized from θ Capricorni, (Theta Cap or θ Cap) formally named Udang, is a binary star system in the southern constellation of Capricornus, positioned 0.58° south of the ecliptic. It can be seen with the naked eye, having an apparent visual magnitude of +4.07. Based upon an annual parallax shift of 20.11 mas as seen from the Earth, the star is about 162 light-years (50 pc) from the Sun. It is drifting closer with a radial velocity of −11 km/s.

The star or star system is almost eclipsed by the Sun on about 3 February, when it will figure behind the Sun's corona if there is a full solar eclipse. Thus the star can be viewed the whole night, crossing the sky, in early August (in the current epoch). It can be occulted by the Moon.