DP Leonis
Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Leo |
Right ascension | 11h 17m 16.00s[1] |
Declination | +17° 57′ 41.1″[1] |
Apparent magnitude (V) | 17.5-19[2] |
Characteristics | |
Spectral type | DA / M5V? |
Variable type | XM[2] |
Astrometry | |
Radial velocity (Rv) | 0 km/s |
Distance | 1304 ly (400[3] pc) |
Absolute magnitude (MV) | 9.5-11 |
Details | |
Mass | 0.6/0.09 [4] M☉ |
Radius | 0.0114 [4]/0.12? R☉ |
Luminosity | 0.00449/0.00105? L☉ |
Temperature | 13,500/3000? K |
Orbit | |
Period (P) | 0.0001708 yr |
Semi-major axis (a) | 0.0027 AU" |
Eccentricity (e) | 0.0 |
Inclination (i) | 79.5 [4]° |
Other designations | |
V* DP Leo, X 11146+182[2]
|
|
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Extrasolar Planets Encyclopaedia |
data |
DP Leonis (abbreviated DP Leo) is an eclipsing binary system approximately 1304 light-years away from the Sun,[4] probably a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises an eclipsing white dwarf and red dwarf in tight orbit (nearly 1.5 hours) and an extrasolar planet.[3]
Planetary system
In 2010, Qian et al. announced the detection of a third body of planetary mass around the eclipsing binary system. The presence of a third body had already been suspected in 2002.[4] The object is roughly 6 times more massive than Jupiter and is located 8.6 AU from the binary.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (years) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥6.1 ± 0.5 MJ | 8.2 ± 0.4 | 28.0 ± 2.0 | 0.39 ± 0.13 | — | — |
See also
References
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Coordinates: 11h 17m 16.00s, +17° 57′ 41.1″
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