HD 30177

from Wikipedia, the free encyclopedia
Star
HD 30177
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Swordfish
Right ascension 04 h 41 m 54.37 s
declination -58 ° 01 ′ 14.7 ″
Apparent brightness 8.41 mag
Typing
Known exoplanets 1
Spectral class G8 V
Astrometry
parallax (18.93 ± 0.63)  mas
distance (172 ± 6)  ly
(52.8 ± 1.8)  pc  
Visual absolute brightness M vis +4.80 mag
Proper movement 
Rec. Share: (66.15 ± 0.74)  mas / a
Dec. portion: (-11.45 ± 0.77)  mas / a
Physical Properties
Dimensions approx. 0.95  M
radius approx. 1.1  R
Effective temperature approx. 5610  K
Metallicity [Fe / H] 0.25
Age approx. 8 · 10 9  a
Other names
and catalog entries
Cordoba Survey CD -58 ° 984
Henry Draper Catalog HD 30177 [1]
Hipparcos catalog HIP 21850 [2]
SAO catalog SAO 233633 [3]
Tycho catalog TYC 8515-1843-1 [4]Template: Infobox star / maintenance / specification of the TYC catalog
annotation
  1. ↑ Calculated from apparent brightness and distance.

HD 30177 is a main sequence star of the spectral class G8 in the constellation Doradus, about 172  light years away . It has an apparent magnitude of 8.4 mag.

In 2002 Paul Butler discovered a potential extrasolar planet orbiting this star using the radial velocity method . This has the systematic designation HD 30177 b .

HD 30177 b

HD 30177 b is a potential exoplanet that orbits the central star every 2770 days . It orbits its star at a distance of about 3.95 astronomical units with an eccentricity of 0.19 and has a mass of at least about 10 Jupiter's masses.

Web links

Individual evidence

  1. a b c Hipparcos catalog (ESA 1997)
  2. a b c Hipparcos, the New Reduction (van Leeuwen, 2007)