HD 192263

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Stern
HD 192263
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Eagle
Right ascension 20 h 13 m 59.85 s
declination -00 ° 52 ′ 0.8 ″
Apparent brightness 7.79 likes
Typing
Known exoplanets 1
Spectral class K0
Variable star type BY-Draconis mutable 
Astrometry
Radial velocity (−10.8 ± 0.2) km / s
parallax (51.77 ± 0.78)  mas
distance (63.0 ± 1.0)  ly
(19.3 ± 0.3)  pc  
Visual absolute brightness M vis +6.4 mag
Proper movement 
Rec. Share: (−61.13 ± 1.21)  mas / a
Dec. portion: (+261.37 ± 0.50)  mas / a
Physical Properties
Dimensions 0.81  M
radius 0.75  R
Effective temperature approx. 5000  K
Metallicity [Fe / H] −0.2
Age approx. 570 mill.  a
Other names
and catalog entries
Bonn survey BD −1 ° 3925
Henry Draper Catalog HD 192263 [1]
Hipparcos catalog HIP 99711 [2]
SAO catalog SAO 144192 [3]
Tycho catalog TYC 5161-868-1 [4]Template: Infobox star / maintenance / specification of the TYC catalog
Other names V1703 Aquilae
annotation
  1. ↑ Estimated from apparent brightness and distance.

HD 192263 is a star of the eighth magnitude class in the constellation Aquila . It is a main sequence star of the spectral class K0. The star is therefore a little cooler and a little less bright than our sun . With very good binoculars and telescopes , the star is easy to see at night. HD 192263 is a BY Draconis variable .

Discoveries by companions of the star were announced again and again, which could not be confirmed in retrospect. The fact that the star is practically on the equatorial plane of the earth may have contributed to this. However, it has been clear since 1999 that at least one planet orbits HD 192263.

HD 192263 b

Main article: HD 192263 b

Since, due to the large number of newly discovered planets, they no longer receive proper names (i.e. not the name of a god like Mars , Jupiter etc., for example), newly discovered objects are numbered alphabetically. Therefore the companion of the star is simply called "b", ie HD 192263 b.

The mass of the companion found is at least three quarters of the mass of Jupiter, its almost circular orbit around the star lasts about 24 days. The distance to the star is about 0.15  AU , which is significantly smaller than the distance between the earth and the sun.

credentials

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)