Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Leo |
Right ascension | 11h 17m 15.92381s[2] |
Declination | +17° 57′ 41.6804″[2] |
Apparent magnitude (V) | 17.5-19[3] |
Characteristics | |
Variable type | AM Her[3] |
Astrometry | |
Radial velocity (Rv) | 0.0[4] km/s |
Proper motion (μ) | RA: −28.700 mas/yr[2] Dec.: −1.444 mas/yr[2] |
Parallax (π) | 3.2781 ± 0.3110 mas[2] |
Distance | 990 ± 90 ly (310 ± 30 pc) |
Orbit | |
Period (P) | 0.0623628426[5] yr |
Eccentricity (e) | 0.0 (fixed) |
Inclination (i) | 79.5[6]° |
Details | |
White dwarf | |
Mass | 0.6[6] M☉ |
Temperature | 13,500[5] K |
Donor star | |
Mass | 0.09[6] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
DP Leonis (abbreviated DP Leo) is a binary star system in the equatorial constellation of Leo. It is a variable star that ranges in apparent visual magnitude from 17.5 down to 19.[3] The system is located at a distance of approximately 990 light-years from the Sun based on parallax.[2] It is 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.[8] This eclipsing variable was discovered by P. Biermann and associates in 1982 as the optical counterpart to the EINSTEIN X-ray source E1114+182.[9]
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