NGC 1514

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NGC 1514
Observation data
(Epoch J2000)
Right ascension 04h 09m 16.984s[1]
Declination +30° 46′ 33.47″[1]
Distance ~600[a]
Apparent magnitude (V) 9.43[1]
Apparent dimensions (V) 2′.2
Constellation Taurus
Physical characteristics
See also: Planetary nebula, Lists of nebulae

NGC 1514 was discovered by William Herschel on November 13th 1790 describing it "A most singular phoenomenoa" and forcing him to rethink his ideas on the construction of the heavens. Up until this point Herschel was convinced that all nebulae consisted of masses of stars too remote to resolve, but now here was a single star "surrounded with a faintly luminous atmosphere."[2] He went on to conclude "Our judgement I may venture to say, will be, that the nebulosity about the star is not of a starry nature".

It has since been conjectured that the nebula in fact envelops a tightly orbiting double star with a period of up to 10 days. Gas is presumably expanding away from the larger star of the pair.[3]

[edit] Notes

  1. ^ Parallax = 5.40 ± 1.70 mas[1]
  1. ^ a b c d SIMBAD 2007
  2. ^ Herschel 1791
  3. ^ Muthu & Anandarao 2003

[edit] References

[edit] External links