| Emission nebula | |
|---|---|
| Planetary nebula | |
| Medusa nebula, Mayall Telescope | |
| 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 a PG 1159 star. [5]