Emission nebula | |
---|---|
Planetary nebula | |
Observation data: J2000.0 epoch | |
Right ascension | 07h 29m 02.69s[1][2] |
Declination | +13° 14′ 48.4″[1][2] |
Distance | 1,500 ly (460 pc)[3] ly |
Apparent magnitude (V) | 15.99[1] |
Apparent dimensions (V) | 10.25 x 10.25 arcmin[1] |
Constellation | Gemini |
Physical characteristics | |
Radius | 4 [3] ly |
Absolute magnitude (V) | 7.68 |
Notable features | Very large & very low surface brightness |
Designations | Sharpless 2-274, PK 205+14 1, Abell 21 [1] |
The Medusa Nebula is a planetary nebula in the constellation of Gemini. It is also known as Abell 21 and Sharpless 2-274. It was originally discovered in 1955 by University of California, Los Angeles astronomer George O. Abell, who classified it as an old planetary nebula.[4] With the computation of expansion velocities and the thermal character of the radio emission, Soviet astronomers in 1971 concluded that it was most likely a planetary nebula.[4] As the nebula is so large, its surface brightness is very low, with surface magnitudes of between +15.99 and +25 reported.[citation needed]
The central star of the planetary nebula is an PG 1159 star.[5]