Nicknamed the Spare-tyre nebula,[3] IC 5148 is a planetary nebula located around 1 degree west of Lambda Gruis in the constellation of Grus (The Crane).[4] It was discovered by Australian amateur astronomer Walter Gale in 1894. Around 3000 light-years distant, it is expanding at a rate of 50 kilometres a second, one of the fastest of all planetary nebulae.[3]
| Emission nebula | |
|---|---|
| Planetary nebula | |
 IC 5148, nicknamed the Spare Tyre Nebula, taken by the ESO Faint Object Spectrograph and Camera (EFOSC2) on the New Technology Telescope.[1] | |
| Observation data: J2000 epoch | |
| Right ascension | 21h 59m 35.2s[2] |
| Declination | −39° 23′ 08″[2] |
| Distance | 3000 light years[1] ly |
| Apparent magnitude (V) | 16.5[2] |
| Apparent dimensions (V) | 2 ′ x 2 ′[2] |
| Constellation | Grus |
| Designations | IC 5150, PK 002-52 1, PSCz P21565-3937, ESO 344-5, IRAS 21565-3937, PN G002.7-52.4 |
The central star of the planetary nebula has a spectral type of hgO(H).[5]
References edit
- ^ a b "From Cosmic Spare Tyre to Ethereal Blossom". Picture of the Week. European Southern Observatory. Retrieved 15 October 2012.
- ^ a b c d "Search Results for IC 5148". Astronomical Database. SIMBAD. Retrieved 15 October 2012.
- ^ a b ESO (2012). "From Cosmic Spare Tyre to Ethereal Blossom". Picture of the Week. European Southern Observatory. Retrieved 6 February 2014.
- ^ Streicher, Magda (December 2010). "Grus—An Elegant Starry Bird" (PDF). Deepsky Delights. The Astronomical Society of Southern Africa. pp. 56–59. Retrieved 7 February 2014.
- ^ González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. (2021). "Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity". Astronomy & Astrophysics. 656: A51. arXiv:2109.12114. Bibcode:2021A&A...656A..51G. doi:10.1051/0004-6361/202141916. S2CID 237940344.
External links edit
Media related to IC 5148 at Wikimedia Commons
 | This nebula-related article is a stub. You can help Wikipedia by expanding it. |