Celestial hemisphere:  Northern  ·  Constellation: Perseus (Per)  ·  Contains:  46 ksi Per  ·  California nebula  ·  IC 2005  ·  Menkib  ·  NGC 1499  ·  Sh2-220  ·  The star ξPer
California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
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California Nebula SHO - NGC 1499 - a cosmic Rainbow

California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
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California Nebula SHO - NGC 1499 - a cosmic Rainbow

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Description

Object description (wikipedia.org):

The California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus. It is so named because it appears to resemble the outline of the US State of California on long exposure photographs. It is almost 2.5° long on the sky and, because of its very low surface brightness, it is extremely difficult to observe visually. It can be observed with a Hβ filter (isolates the Hβ line at 486 nm) in a rich-field telescope under dark skies. It lies at a distance of about 1,000 light years from Earth. Its fluorescence is due to excitation of the Hβ line in the nebula by the nearby prodigiously energetic O7 star, xi Persei (also known as Menkib, seen at center below it in the inset at right).

The California Nebula was discovered by E. E. Barnard in 1884.

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  • California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
    Original
  • California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
    B
  • California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
    C
  • California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
    D
  • Final
    California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter
    E

C

Description: adjusted shadows and highlights

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D

Description: New processing and lower saturation

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California Nebula SHO - NGC 1499 - a cosmic Rainbow, Thomas Richter