HD 142022

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Double star
HD 142022 A
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Octant
Right ascension 16 h 10 m 15.02 s
declination -84 ° 13 ′ 53.8 ″
Apparent brightness 7.7 likes
Typing
Known exoplanets 1
Spectral class K0 V
Astrometry
Radial velocity (−9.6 ± 0.4) km / s
parallax (29.13 ± 0.57)  mas
distance (112 ± 2)  Lj
(34.33 ± 0.67)  pc  
Visual absolute brightness M vis +5.02 mag
Proper movement 
Rec. Share: (−336.32 ± 0.56)  mas / a
Dec. portion: (−31.77 ± 0.70)  mas / a
Physical Properties
Dimensions 0.99  M
radius 0.705 (± 0.135)  R
Effective temperature 5382  K
Metallicity [Fe / H] 0.19
Age 13.3 · 10 9  a
Other names
and catalog entries
Henry Draper Catalog HD 142022 [1]
Hipparcos catalog HIP 79242 [2]
SAO catalog SAO 258738 [3]
annotation
  1. ↑ Calculated from apparent brightness and distance.

HD 142022 A is a late main sequence star 112 light years away from Earth with a right ascension of 16h 10m 15s and a declination of −84 ° 13 '53 ". It has an apparent magnitude of 7.7 mag. Anne Eggenberger discovered one in 2005 extrasolar planet orbiting this star, which is called HD 142022 Ab . Furthermore, there is also a second star in this system called HD 142022 B, which orbits HD 142022 A. This makes this system a double star .

Web links

Individual evidence

  1. a b c Hipparcos catalog (ESA 1997)
  2. Pulkovo radial velocities for 35493 HIP stars
  3. a b c Hipparcos, the New Reduction (van Leeuwen, 2007)