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IC 1805 • Sh2-190 • Heart Nebula in SHO, Douglas J Struble

IC 1805 • Sh2-190 • Heart Nebula in SHO

Getting plate-solving status, please wait...
IC 1805 • Sh2-190 • Heart Nebula in SHO, Douglas J Struble

IC 1805 • Sh2-190 • Heart Nebula in SHO

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Description

I captured 16.7 hours of data back in 2017 and wanted to add on to it this year pulling out some of the fainter nebulosity. There is a little blue, what I believe is a small planetary nebula towards the top, which I always found interesting.

The Heart Nebula, IC 1805, Sharpless 2-190, lies some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787. It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.

The brightest part of the nebula (a knot at its western edge) is separately classified as NGC 896, because it was the first part of the nebula to be discovered. The nebula's intense red output and its morphology are driven by the radiation emanating from a small group of stars near the nebula's center. This open cluster of stars, known as Melotte 15, contains a few bright stars nearly 50 times the mass of our Sun, and many more dim stars that are only a fraction of our Sun's mass.

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IC 1805 • Sh2-190 • Heart Nebula in SHO, Douglas J Struble

In these public groups

Sharpless2 Objects