The Eskimo Nebula (NGC 2392), also known as the Clownface Nebula, is a bipolar double-shell planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. From the ground, it resembles a person's head surrounded by a parka hood. In 2000, the Hubble Space Telescope produced an image of it. From space, the nebula displays gas clouds so complex that they are not fully understood.
Its inner shell measures 18″ × 15″ and is bright and elliptical and marked on its south rim by two blister-like protrusions. Its outer shell is nearly circular measuring 24″ radius and contains a set of complex low-ionization features. It is observed to have high-dispersion spectra of optical nebular lines which indicate a fast collimated outflow with a velocity along our line of sight of nearly 200 km/s producing dynamic interaction with nebular material. As of 2003, it is estimated to be only ≥1060 years old. The earth's perspective is almost along its axis of symmetry. Its knots have a highly developed symmetry along a radius vector from the PN's central star, except their tails are somewhat irregular. The tails are well developed and frequently of a discernible optical thickness in the visual spectrum. The knots are bright rimmed and have low ionization (as compared to those found in NGC 7293) which indicates their location being inside the ionized zone yet close to the boundary. The knots' heads have local photoionization fronts which appear as bright cusps. At the cusps, the knots become optically thick to Lyc photons from the central star.
It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by strong wind of particles from the central star. The outer disk contains unusual light-year long orange filaments.