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File:K61 - Gemini1108a.jpg

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English: k61 Planetary Nebula


Gemini Observatory image of Kronberger 61 showing the ionized shell of expelled gas resembling a soccer ball. The light of the nebula is primarily due to ionized oxygen (oxygen-III) emission and its central star can be seen as the slightly bluer star very close to the center of the nebula. The field of view is 2.2 x 3.4 arcminutes with north up (rotated 22 degrees west of north). Image processing by Travis Rector, University of Alaska Anchorage. A color composite image, it consists of two narrow-band images (O-III and Hydrogen-alpha with three, 500-second integrations each) obtained with the Gemini Multi-Object Spectrograph (GMOS) on the Gemini North telescope on Mauna Kea in Hawai‘i. Below the bright star at left is a barred spiral galaxy in the distant background, careful inspection will reveal several additional distant galaxies in the image.

Credit:

International Gemini Observatory/AURA
Date June 30, 2020
Source https://noirlab.edu/public/images/gemini1108a/
Author Credit: International Gemini Observatory/AURA
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current16:22, 22 November 2021Thumbnail for version as of 16:22, 22 November 2021900 × 1,400 (861 KB)Fabian RRRR== {{int:filedesc}} == {{Information |description={{en|1='''k61 Planetary Nebula Gemini Observatory image of Kronberger 61 showing the ionized shell of expelled gas resembling a soccer ball. The light of the nebula is primarily due to ionized oxygen (oxygen-III) emission and its central star can be seen as the slightly bluer star very close to the center of the nebula. The field of view is 2.2 x 3.4 arcminutes with north up (rotated 22 degrees west of north). Image processing by Travis Rect...

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