File:PN A66 78 (Abell 78).png

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Not one of HST's favored children, this planetary nebula is not available in enough filters to create a color image. I went ahead and gave it a fictitious color palette, and although the color is fake, it is not entirely unrealistic. The nebula emits strongly in [O III], giving it a greenish cyan coloration. The central stars of planetary nebulas tend to be blue, while other stars are comparatively yellow or red.

Many of the details are rather faint, especially the hazy outer shell, but I think it is a very beautiful object. Most planetary nebulas are. This one is said to be "born again" as it experienced some kind of secondary event after its initial formation, leading to some extra ejected material.

Data from the following proposal were used to create this image: Witnessing the Expansion of Hydrogen-Poor Ejecta in Born-Again Planetary Nebulae

All channels: WFC3/UVIS F502N

North is 64.36° counter-clockwise from up.
Date
Source PN A66 78 (Abell 78)
Author Judy Schmidt from USA

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This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/49481586101 (archive). It was reviewed on 3 February 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

3 February 2020

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Date/TimeThumbnailDimensionsUserComment
current12:06, 3 February 2020Thumbnail for version as of 12:06, 3 February 20203,110 × 3,222 (16.71 MB)Fabian RRRR (talk | contribs)=={{int:filedesc}}== {{Information |Description=Not one of HST's favored children, this planetary nebula is not available in enough filters to create a color image. I went ahead and gave it a fictitious color palette, and although the color is fake, it is not entirely unrealistic. The nebula emits strongly in [O III], giving it a greenish cyan coloration. The central stars of planetary nebulas tend to be blue, while other stars are comparatively yellow or red. Many of the details are rather...

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