- DP Leonis
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DP Leonis Observation data
Epoch J2000.0 Equinox J2000.0Constellation 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 Semimajor 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 NStED data Extrasolar Planets
Encyclopaediadata 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 star and red dwarf star 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.
The DP Leonis system[3] Companion
(in order from star)Mass Semimajor axis
(AU)Orbital period
(years)Eccentricity b ≥6.28 MJ 8.6 23.8 ? References
- ^ a b "V* DP Leo -- Cataclysmic Var. AM Her type". SIMBAD. Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=DP+Leo. Retrieved 2009-12-16.
- ^ a b c "Query= DP Leo". General Catalogue of Variable Stars. Centre de Données astronomiques de Strasbourg. http://www.sai.msu.su/gcvs/cgi-bin/search.cgi?search=DP+Leo. Retrieved 2009-12-16.
- ^ a b c Qianet al.; Liao, W.-P.; Zhu, L.-Y.; Dai, Z.-B. (2010). "DETECTION OF A GIANT EXTRASOLAR PLANET ORBITING THE ECLIPSING POLAR DP LEO". The Astrophysical Journal 708 (1): 66–68. Bibcode 2010ApJ...708L..66Q. doi:10.1088/2041-8205/708/1/L66. http://www.iop.org/EJ/abstract/2041-8205/708/1/L66.
- ^ a b c d e Schwope et al.; Hambaryan, V.; Schwarz, R.; Kanbach, G.; G�Nsicke, B. T. (2002). "A multiwavelength timing analysis of the eclipsing polar DP Leo". Astronomy and Astrophysics 392 (2): 541–551. arXiv:astro-ph/0111457. Bibcode 2002A&A...392..541S. doi:10.1051/0004-6361:20011651.
See also
- AM Herculis
- NN Serpentis
- QS Virginis
- List of extrasolar planets
Coordinates: 11h 17m 16.00s, +17° 57′ 41.1″
Bayer α (Regulus) • β (Denebola) • γ (Algieba) • δ (Zosma) • ε (Algenubi) • ζ (Adhafera) • η • θ (Chertan) • ι • κ (Al Minliar al Asad) • λ (Alterf) • μ (Rasalas) • ν • ξ • ο (Subra) • π • ρ • σ • τ • υ • φ • χ • ψ • ω • b • c • d • e • f • g • h • k • l • m • n • o • p¹ • p² • p³ • AFlamsteed 1 (κ, Al Minliar al Asad) • 2 (ω) • 3 • 4 (λ, Alterf) • 5 (ξ) • 6 (h) • 7 • 8 • 9 • 10 • 11 • 12 • 13 • 14 (ο, Subra) • 15 (f) • 16 (ψ) • 17 (ε, Algenubi) • 18 • 19 • 20 • 21 • 22 (g) • 23 • 24 (μ, Rasalas) • 27 (ν) • 29 (π) • 30 (η) • 31 (A) • 32 (α, Regulus) • 34 • 35 • 36 (ζ, Adhafera) • 37 • 39 • 40 • 41 (γ, Algieba) • 42 • 43 • 44 • 45 • 46 • 47 (ρ) • 48 • 49 • 50 • 51 (m) • 52 (k) • 53 (l) • 54 • 55 • 56 • 58 (d) • 59 (c) • 60 (b) • 61 (p²) • 62 (p³) • 63 (χ) • 64 • 67 • 68 (δ, Zosma) • 70 (θ, Chertan) • 71 • 72 • 73 (n) • 74 (φ) • 75 • 76 • 77 (σ) • 78 (ι) • 79 • 80 • 81 • 83 • 84 (τ) • 85 • 86 • 87 (e) • 88 • 89 • 90 • υ (91) • 92 • 93 • 94 (β, Denebola) • 95 • 18 LMi • 37 Sex • 52 LMiNearby Wolf 359 • AD • 2MASS 0937+2931 • Gliese 408 • EE • Gliese 436Other List This extrasolar planet related article is a stub. You can help Wikipedia by expanding it.