Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  HD14695  ·  HD14749  ·  HD14794  ·  HD14795  ·  HD14817  ·  HD15069  ·  HD15238  ·  HD15239  ·  HD15250  ·  HD15382  ·  HD15522  ·  HD15557  ·  HD15558  ·  HD15570  ·  HD15629  ·  HD15640  ·  HD15665  ·  HD15785  ·  HD15851  ·  HD15862  ·  HD16038  ·  HD16088  ·  HD16183  ·  HD16218  ·  HD16349  ·  HD16410  ·  HD16429  ·  HD236966  ·  IC 1795  ·  IC 1805  ·  And 27 more.
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Heart Nebula, IC 1805, Jared Willson
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Heart Nebula, IC 1805

Getting plate-solving status, please wait...
Heart Nebula, IC 1805, Jared Willson
Powered byPixInsight

Heart Nebula, IC 1805

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Description

The Heart Nebula (IC 1805) lies roughly 7,500 light years from Earth in the Perseus arm of the Milky Way. It was first observed and cataloged by prolific observer William Herschel in 1787 and is composed primarily of ionized hydrogen interspersed with darker dust lanes. The knot of gas at the lower right of this image is separately cataloged as NGC 896. The source of energy creating all the ionized gas is the cluster of stars Collinder 26 (also known as Melotte 15) located near the center of the Heart nebula. It contains stars that are up to fifty times the mass of the sun. These very hot, very energetic starts emit a large amount of ultraviolet light which is energetic enough to ionize the surrounding gas. The surface brightness of the Heart Nebula is moderately low, with an integrated magnitude of 18.3 spread over more than two degrees of sky.

This image of the Heart Nebula was captured using a 3nm Hydrogen Alpha filter. Due to the large amount of sky covered by the Heart Nebula, this image is a four panel mosaic. All data were collected with a nearly full moon, hence the need for a narrow band filter exclusively. Integration time listed is for each panel, so total exposure time across all four panels is 4x that listed.

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Heart Nebula, IC 1805, Jared Willson