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- OGLE-2005-BLG-071Lb abstract "OGLE-2005-BLG-071Lb is an planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using gravitational microlensing. According to the best fit model, it has about 3.5 times the mass of Jupiter and a projected separation of 3.6 astronomical units from the star. This would result in an effective temperature around 50 K, similar to that of Neptune. However, an alternative model which gives a slightly lower mass of 3.3 times that of Jupiter and a projected separation of 2.1 AU is only slightly less likely. It may be the most massive planet currently known around a red dwarf star (though only lower limits are known for those planets detected by the radial velocity method).".
- OGLE-2005-BLG-071Lb thumbnail Planet_OGLE_05-071-Lb.png?width=300.
- OGLE-2005-BLG-071Lb wikiPageID "16782239".
- OGLE-2005-BLG-071Lb wikiPageRevisionID "582063558".
- OGLE-2005-BLG-071Lb class "M?".
- OGLE-2005-BLG-071Lb colwidth "30".
- OGLE-2005-BLG-071Lb constell Scorpius.
- OGLE-2005-BLG-071Lb discoverers "Udalski et al.".
- OGLE-2005-BLG-071Lb discoveryDate "2005-05-27".
- OGLE-2005-BLG-071Lb discoveryMethod Methods_of_detecting_exoplanets.
- OGLE-2005-BLG-071Lb discoveryStatus "Published".
- OGLE-2005-BLG-071Lb distLy "approx. 11000".
- OGLE-2005-BLG-071Lb distPc "approx. 3300".
- OGLE-2005-BLG-071Lb hasPhotoCollection OGLE-2005-BLG-071Lb.
- OGLE-2005-BLG-071Lb planet "b".
- OGLE-2005-BLG-071Lb simbad "NAME+EWS+2005-BLG-071Lb".
- OGLE-2005-BLG-071Lb star OGLE-2005-BLG-071L.
- OGLE-2005-BLG-071Lb star "OGLE-05-071L".
- OGLE-2005-BLG-071Lb subject Category:Exoplanets.
- OGLE-2005-BLG-071Lb subject Category:Exoplanets_detected_by_microlensing.
- OGLE-2005-BLG-071Lb subject Category:Exoplanets_discovered_in_2005.
- OGLE-2005-BLG-071Lb subject Category:Gas_giants.
- OGLE-2005-BLG-071Lb subject Category:Scorpius_(constellation).
- OGLE-2005-BLG-071Lb type CelestialBody.
- OGLE-2005-BLG-071Lb type Planet.
- OGLE-2005-BLG-071Lb type PhysicalBody.
- OGLE-2005-BLG-071Lb comment "OGLE-2005-BLG-071Lb is an planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using gravitational microlensing. According to the best fit model, it has about 3.5 times the mass of Jupiter and a projected separation of 3.6 astronomical units from the star. This would result in an effective temperature around 50 K, similar to that of Neptune.".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071L b".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071L b".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071Lb".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071Lb".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071Lb".
- OGLE-2005-BLG-071Lb label "OGLE-2005-BLG-071Lb".
- OGLE-2005-BLG-071Lb sameAs OGLE-2005-BLG-071L_b.
- OGLE-2005-BLG-071Lb sameAs OGLE-2005-BLG-071Lb.
- OGLE-2005-BLG-071Lb sameAs OGLE-2005-BLG-071Lb.
- OGLE-2005-BLG-071Lb sameAs OGLE-2005-BLG-071Lb.
- OGLE-2005-BLG-071Lb sameAs m.04y5q7s.
- OGLE-2005-BLG-071Lb sameAs Q429564.
- OGLE-2005-BLG-071Lb sameAs Q429564.
- OGLE-2005-BLG-071Lb wasDerivedFrom OGLE-2005-BLG-071Lb?oldid=582063558.
- OGLE-2005-BLG-071Lb depiction Planet_OGLE_05-071-Lb.png.
- OGLE-2005-BLG-071Lb isPrimaryTopicOf OGLE-2005-BLG-071Lb.