Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  LBN 633  ·  PK128-04.1  ·  Sh2-188
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Sh2-188, Gary Imm
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Sh2-188

Getting plate-solving status, please wait...
Sh2-188, Gary Imm
Powered byPixInsight

Sh2-188

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Description

This object is a beautiful planetary nebula that is located approximately 850 light-years from Earth in the constellation of Cassiopeia. This nebula was first thought to be the remnant of a supernova explosion that appeared recently, but the nebula was later confirmed to be an asymmetrical planetary nebula with a crescent-like shape. Most planetary nebulae simply expand outwards symmetrically, forming a spherical shell around the dying star. It is believed that this nebula gets its interesting shape from the speed at which the gas is moving and interacting with the interstellar medium. The sun-like star responsible for expelling all of the gases into space is thought to be moving at about 300,000 mph, and is visible in the image as the brightest orange star just to the right of the center of the nebula. The motion of the star is to the lower right, which creates the visible bow shock of primarily reddish hydrogen gas. Some oxygen is also present as indicated by the bluish tint behind the initial bow wave.

Looking closely at the section towards the center of the nebula, I like how the faint vertical reddish stripes define the bow wave which is coming in our direction, giving the nebula a subtle 3-D look.

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