NGC 2392 Eskimo Nebula

Description

NGC 2392 Eskimo Nebula is small but bright object. It is difficult to process and acquire. You would need a long focus large aperture instrument.

The Eskimo Nebula (NGC 2392), also known as the Clown Face Nebula, Lion Nebula, or Caldwell 39, is a bipolar double-shell planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. The formation resembles a person’s head surrounded by a parka hood. It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by a strong wind of particles from the central star. The outer disk contains unusual, light-year-long filaments.

NGC 2392 lies about 6500 light-years away, and is visible with a small telescope in the constellation of Gemini.

At the center of NGC 2392, there is an O-type star (designated HD 59088[7]) with a spectral type of O(H)6f.

 

Data/Processing Attribution

This is my data and processing.

Distances/Size

Distance to the object: 6,520 light-years, size in the sky 48” X 48″

Equipment

Mount-PlaneWave L-350; Scope-PlaneWave CDK14″, 356 mm aperture, 2563 mm focal length; Camera-Moravian C3-61000, 0.30 arcsec/pixel.

Observatory

The image was taken in the Prairies Skies Astro remote observatories.

Exposure

The total exposure using SHORGB filters is 21 hours and 15 minutes 30 secons, with each sub-exposure lasting 300  and 90 seconds. This is the processing of the data taken in December  2025 and January 2026.

SHORGB Filters for stars

Ha- 96X300 and 90= 3 hours 48 minutes

O3- 96X300 and 90= 3 hours 48 minutes

S2- 85X300 and 90= 2 hours 53 minutes

R- 144X90=  3 hours 34 minutes 30 sec

G-144X90= 3 hours 36 minutes

B-148X90= 3 hours 36 minutes

Processing is done in PixInsight, Photoshop, and Lightroom Classic

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