HD 219828

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Star
HD 219828
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Pegasus
Right ascension 23 h 18 m 46.74 s
declination + 18 ° 38 ′ 44.6 ″
Apparent brightness 8.04 mag
Typing
Known exoplanets 1
Spectral class G0 IV
Astrometry
Radial velocity (−24.2 ± 0.3) km / s
parallax (13.83 ± 0.74)  mas
distance (236 ± 13)  ly
(72.3 ± 4)  pc  
Visual absolute brightness M vis +3.7 mag
Proper movement 
Rec. Share: (−4.15 ± 0.84)  mas / a
Dec. portion: (+4.14 ± 0.70)  mas / a
Physical Properties
Dimensions (1.2 ± 0.1)  M
Luminosity

L

Effective temperature (5891 ± 18)  K.
Metallicity [Fe / H] 0.19 ± 0.03
Other names
and catalog entries
Bonn survey BD +17 4896
Henry Draper Catalog HD 219828 [1]
Hipparcos catalog HIP 115100 [2]
SAO catalog SAO 108536 [3]
Tycho catalog TYC 1716-1182-1 [4]Template: Infobox star / maintenance / specification of the TYC catalog
annotation
  1. ↑ Estimated from apparent brightness and distance.

HD 219828 is the name of a star approx. 70  parsecs (approx. 240  light years ) away from the Sun , which is orbited by an exoplanet . The star in the constellation Pegasus is a subgiant of the spectral type G0 and with its apparent magnitude of 8.04 mag is invisible to the naked eye. With a surface temperature of approx. 5900 K, the star is relatively similar to the sun.

The planet

Due to the large number of newly found, extrasolar planets, newly discovered companions are no longer given proper names. Therefore the planet orbiting HD 219828 is simply called “b”, ie HD 219828 b. HD 219828 b is a planet similar to Neptune, and is at least 21 times as heavy as Earth. It is not yet known whether the object is an ice planet, a gas planet or even a stone planet, which would then be something like "super earth".

Web links

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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)