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- WR_102ea abstract "WR 102ea is a Wolf–Rayet star in the Sagittarius constellation. It is the second brightest star in the Quintuplet cluster after WR 102hb. With a luminosity of 2,500,000 times solar, it is also one of the most luminous stars known. Despite the high luminosity it can only be observed at infra-red wavelengths due to the dimming effect of intervening dust on visual light.".
- WR_102ea wikiPageID "28290171".
- WR_102ea wikiPageRevisionID "541381409".
- WR_102ea absmagK "−8.3".
- WR_102ea age "probably 4 × 106".
- WR_102ea appmag "8.8".
- WR_102ea appmag1Passband "K".
- WR_102ea class "32400.0".
- WR_102ea constell Sagittarius_(constellation).
- WR_102ea dec "−28° 48′ 30″".
- WR_102ea distLy "26".
- WR_102ea distPc "8".
- WR_102ea epoch "J2000".
- WR_102ea hasPhotoCollection WR_102ea.
- WR_102ea luminosity "2.5".
- WR_102ea mass "58".
- WR_102ea ra "63785.0".
- WR_102ea radialV "116".
- WR_102ea radius "86".
- WR_102ea simbad "WR_102ea".
- WR_102ea temperature "25100".
- WR_102ea type "Wolf Rayet".
- WR_102ea subject Category:Sagittarius_(constellation).
- WR_102ea subject Category:Wolf–Rayet_stars.
- WR_102ea type CelestialBody.
- WR_102ea type Star.
- WR_102ea type PhysicalBody.
- WR_102ea comment "WR 102ea is a Wolf–Rayet star in the Sagittarius constellation. It is the second brightest star in the Quintuplet cluster after WR 102hb. With a luminosity of 2,500,000 times solar, it is also one of the most luminous stars known. Despite the high luminosity it can only be observed at infra-red wavelengths due to the dimming effect of intervening dust on visual light.".
- WR_102ea label "QPM-241".
- WR_102ea label "QPM-241".
- WR_102ea label "WR 102ea".
- WR_102ea label "WR 102ea".
- WR_102ea sameAs QPM-241.
- WR_102ea sameAs WR_102ea.
- WR_102ea sameAs QPM-241.
- WR_102ea sameAs m.0cp1jnc.
- WR_102ea sameAs Q1090392.
- WR_102ea sameAs Q1090392.
- WR_102ea wasDerivedFrom WR_102ea?oldid=541381409.
- WR_102ea isPrimaryTopicOf WR_102ea.
- WR_102ea name "WR 102ea".