HD 103197 b
HD 103197 b (also known as HIP 57931 b) is an extrasolar planet which orbits the K-type main sequence star HD 103197, located approximately 170 light years away in the constellation Centaurus. This planet has at least one-tenth the mass of Jupiter and takes 48 days to orbit the star at a semimajor axis of 0.235 AU. Fitting the observational data with a Keplerian orbit leads to a solution with an insignificant eccentricity. This planet was announced by the Swiss-led HARPS team on October 19, 2009, together with 29 other planets.
HD 103197 b
HD 103197 b (also known as HIP 57931 b) is an extrasolar planet which orbits the K-type main sequence star HD 103197, located approximately 170 light years away in the constellation Centaurus. This planet has at least one-tenth the mass of Jupiter and takes 48 days to orbit the star at a semimajor axis of 0.235 AU. Fitting the observational data with a Keplerian orbit leads to a solution with an insignificant eccentricity. This planet was announced by the Swiss-led HARPS team on October 19, 2009, together with 29 other planets.
has abstract
HD 103197 b (also known as HIP ...... ogether with 29 other planets.
@en
HD 103197 b (también conocido ...... omún posible para HD 103197 b.
@es
Wikipage page ID
25,181,782
Wikipage revision ID
640,051,075
app mag
constell
discoverers
Mordasini et al.
discovery date
2009-10-19
discovery method
radial velocity
discovery site
discovery status
dist ly
eccentricity
period
period year
semimajor
semimajor gm
semimajor mas
subject
hypernym
comment
HD 103197 b (also known as HIP ...... ogether with 29 other planets.
@en
HD 103197 b (también conocido ...... omún posible para HD 103197 b.
@es
label
HD 103197 b
@en
HD 103197 b
@es