NGC 3242

NGC 3242 (also known as the Ghost of Jupiter or Caldwell 59) is a planetary nebula located in the constellation Hydra.

NGC 3242
Emission nebula
Planetary nebula
A Hubble Space Telescope (HST) image of core region of NGC 3242.
Credit: HST/NASA/ESA.
Observation data: J2000 epoch
Right ascension10h 24m 46.1s[1]
Declination−18° 38′ 32.6″[1]
Distance4800±500[2] ly
Apparent magnitude (V)8.60
Apparent dimensions (V)25″
ConstellationHydra
DesignationsGhost of Jupiter, Jupiter's Ghost, Eye Nebula, Caldwell 59

William Herschel discovered the nebula on February 7, 1785, and cataloged it as H IV.27. John Herschel observed it from the Cape of Good Hope, South Africa, in the 1830s, and numbered it as h 3248, and included it in the 1864 General Catalogue as GC 2102; this became NGC 3242 in J. L. E. Dreyer's New General Catalogue of 1888.

This planetary nebula is most frequently called the Ghost of Jupiter, or Jupiter's Ghost due to its similar size to the planet, but it is also sometimes referred to as the Eye Nebula.[3] The nebula measures around two light years long from end to end, and contains a central white dwarf with an apparent magnitude of eleven. The inner layers of the nebula were formed some 1,500 years ago.[4] The two ends of the nebula are marked by FLIERs, lobes of fast moving gas often tinted red in false-color pictures.[5] NGC 3242 can easily be observed with amateur telescopes and appears bluish-green to most observers. Larger telescopes can distinguish the outer halo as well.[6]

See also

References
  1. "NGC 3242". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-04-20.
  2. Gaia Collaboration et al. (2018b): Summary of the contents and survey properties
  3. Frommert, Hartmut. "NGC 3242". SEDS. Retrieved 22 June 2014.
  4. Mobberley, Martin (2009). The Caldwell Objects and How to Observe Them. New York: Springer Science+Business Media, LLC. p. 128. ISBN 978-1-4419-0326-6.
  5. "NGC 3242, Ghost of Jupiter". ESA. Retrieved 22 June 2014.
  6. "The Ghost of Jupiter". Retrieved 2010-02-25.
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