Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Ursa Major |
Right ascension | 13h 34m 02.5394s [1] |
Declination | +53° 43′ 42.698″ [1] |
Apparent magnitude (V) | 8.06 [2] |
Characteristics | |
Spectral type | G0V [3] |
B−V color index | 0.699±0.012 [4] |
Astrometry | |
Radial velocity (Rv) | −29.07±0.24 [4] km/s |
Proper motion (μ) |
RA: −85.849(18)
mas/
yr
[1] Dec.: −78.888(20) mas/ yr [1] |
Parallax (π) | 10.8643 ± 0.0180 mas [1] |
Distance | 300.2 ± 0.5
ly (92.0 ± 0.2 pc) |
Absolute magnitude (MV) | 3.32 [2] |
Details [5] | |
Mass | 1.23±0.03 M☉ |
Radius | 2.00±0.10 R☉ |
Luminosity | 3.80±0.30 L☉ |
Surface gravity (log g) | 3.93±0.02 cgs |
Temperature | 5,741±35 K |
Metallicity [Fe/H] | 0.16 [2] dex |
Rotational velocity (v sin i) | 7.0 [2] km/s |
Age | 5.4±0.5 Gyr |
Other designations | |
Database references | |
SIMBAD | The star |
planet b | |
Exoplanet Archive | data |
HD 118203 is a star with an orbiting exoplanet located in the northern circumpolar constellation of Ursa Major. It has the proper name Liesma, which means flame, and it is the name of a character from the Latvian poem Staburags un Liesma (Staburags and Liesma). The name was selected in the NameExoWorlds campaign by Latvia, during the 100th anniversary of the IAU. [7] [8]
The apparent visual magnitude of HD 118203 is 8.06, [2] which means it is invisible to the naked eye but it can be seen using binoculars or a telescope. Based on parallax measurements, it is located at a distance of 300 light years from the Sun. [1] The star is drifting closer with a radial velocity of −29 km/s. [4] Based on its position and space velocity this is most likely (97% chance) an older thin disk star. [9] An exoplanet has been detected in a close orbit around the star. [10]
The spectrum of HD 118203 matches a G-type main-sequence star with a class of G0V. [3] It has a low level of chromospheric activity, which means a low level of radial velocity jitter for planet detection purposes. [10] The star has 1.23 [5] times the mass of the Sun and double the Sun's radius. It is around 5.4 billion years old and is spinning with a projected rotational velocity of 7.0 km/s. [2] HD 118203 is radiating 3.8 times the luminosity of the Sun from its photosphere at an effective temperature of 5,741 K. [5]
In 2006, a hot Jupiter candidate was reported in an eccentric orbit around this star. It was discovered using the radial velocity method based on observation of high- metallicity stars begun in 2004. [10] In 2020, it was found that this is a transiting planet, which allowed the mass and radius of the body to be determined. This exoplanet has more than double the mass of Jupiter and a 13% greater radius. It is named Staburags. The fact that the parent star is among the brighter known planet hosts (as of 2020) makes it an interesting object for further study. [9]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b / Staburags | 2.173+0.077 −0.080 MJ |
0.07082+0.00095 −0.00110 |
6.134980+0.000038 −0.000037 |
0.316±0.021 | 88.75+0.86 −1.0 ° |
1.133+0.031 −0.030 RJ |