Veritate

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Stern
Veritate
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Andromeda
Right ascension 23 h 31 m 17.41 s
declination + 39 ° 14 ′ 10.3 ″
Apparent brightness 5.22 mag
Typing
Known exoplanets 1
B − V color index +1.02 
U − B color index +0.87 
Spectral class K0III
Astrometry
Radial velocity −59.99 ± 0.2 km / s
parallax 12.63 ± 0.27  mas
distance 249.18 ± 13.37  Lj
76.4 ± 4.1  pc  
Proper movement 
Rec. Share: 286.72 ± 0.23  mas / a
Dec. portion: −84.22 ± 0.17  mas / a
Physical Properties
Dimensions 2.2 ± 0.2  M
radius 11 ± 1  R
Effective temperature 4,813  K
Metallicity [Fe / H] −0.24
Other names
and catalog entries
Flamsteed name 14 Andromedae
Bonn survey BD + 38 ° 5023
Bright Star Catalog HR 8930 [1]
Henry Draper Catalog HD 221345 [2]
Hipparcos catalog HIP 116076 [3]
SAO catalog SAO 73311 [4]
Tycho catalog TYC 3231-323-1 [5]Template: Infobox star / maintenance / specification of the TYC catalog
2MASS catalog 2MASS J23311742 + 3914102 [6]

Veritate ( Flamsteed designation : 14 Andromedae , abbreviated 14 And ) is a red giant in the constellation Andromeda , the approximately 249 light years from the sun away. It is a 5th magnitude star and can therefore be seen with the naked eye in a moonless night sky and without light pollution . Veritate has a planetary system with at least one known exoplanet .

Origin of name

The star, inconspicuous to the naked eye, was mainly known under its Flamsteed name until 2015 and had no historical proper name. After a public competition by the International Astronomical Union (IAU) to name exoplanets and their central stars, 14 Andromedae received the official name Veritate on December 15, 2015 , derived from the Latin word "Veritas" for "truth". The name originally proposed by the Thunder Bay Center of the Royal Astronomical Society of Canada was Veritas , but it was changed because of the similarity to the asteroid (490) Veritas .

properties

Veritate is a red giant of the spectral class K with more than twice the solar mass and about eleven times the solar radius . It may also be a variable star . In the past it was classified as a main sequence star of the spectral class A or F in an early stage of development.

Planetary system

Main article: Spe (exoplanet)

In 2008, a planet orbiting the star with approximately five times the minimum mass of Jupiter was detected using the radial velocity method . This was given the official name Spe by the IAU in 2015 .

Individual evidence

  1. a b c d SIMBAD: Veritate. Retrieved January 5, 2016 .
  2. a b c d e f g The Extrasolar Planets Encyclopaedia: Planet 14 And b. Retrieved January 5, 2016 .
  3. ^ A b International Astronomical Union: NameExoWorlds - The Approved Names. Retrieved January 5, 2016 .