Theta Persei

From Wikipedia, the free encyclopedia

Theta Persei A/B

Stars of Perseus
Observation data
Epoch J2000
Constellation
(pronunciation)
Perseus
Right ascension 02h 44m 11.99s
Declination +49° 13' 42.4"
Apparent magnitude (V) 4.12/10
Characteristics
Spectral type F7V/M1V
U-B color index 0/0.99
B-V color index 0.49/1.48
Astrometry
Radial velocity (Rv) +25.0 km/s
Proper motion (μ) RA: 334.02 mas/yr
Dec.: -89.96 mas/yr
Parallax (π) 89.03 ± 0.79 mas
Distance 36.6 ± 0.3 ly
(11.23 ± 0.1 pc)
Absolute magnitude (MV) 3.89/9.8
Visual binary orbit
Companion Theta Persei B
Period (P) 2720 yr
Semimajor axis (a) 22.29"
Eccentricity (e) 0.13
Inclination (i) 75.44°
Longitude of the node (Ω) 128°
Periastron epoch (T) ?
Details
Mass 1.14/? M
Radius ?/? R
Luminosity 2.82/? L
Temperature ?/? K
Metallicity ?
Rotation ?
Age ? years
Other designations
Theta Persei, 13 Persei, GJ 107, HR 799, BD+47°746, HD 16895, LTT 10894, SAO 38288, HIP 12777, GC 3277, ADS 2081, CCDM J02441+4913

Theta Persei (θ Per) is a star system 37 light years away from Earth, in the constellation Perseus. The primary star is a yellowish dwarf (main sequence) star of spectral type F7V, which is somewhat larger and brighter than our sun, but still within the range considered to have the potential for Earth-like planets. There is also a red dwarf companion of spectral type M1V, orbiting about 250 AU from the primary.

[edit] External links

Languages