File:Multi-Wavelength View of NGC 1300 (51888310050).jpg

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This image of spiral galaxy NGC 1300 combines observations to map stellar populations and gas. Radio light observed by the Atacama Large Millimeter/submillimeter Array is represented in yellow and highlight the clouds of cold molecular gas that provide the raw material from which stars form. Data from the Very Large Telescopeâs Multi Unit Spectroscopic Explorer (MUSE) instrument are represented in red and magenta, capturing the impact of young, massive stars on their surrounding gas. Visible and ultraviolet light captured by the Hubble Space Telescope highlight dust lanes in gold and very young, hot stars in blue. High-resolution infrared images from the Webb Space Telescope will help researchers identify where stars are forming behind dust and study the earliest stages of star formation in this galaxy.

Read more: www.nasa.gov/feature/goddard/2022/capturing-all-that-glit...
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Source Multi-Wavelength View of NGC 1300
Author NASA's James Webb Space Telescope from Greenbelt, MD, USA

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This file is licensed under the Creative Commons Attribution 2.0 Generic license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
This image was originally posted to Flickr by James Webb Space Telescope at https://flickr.com/photos/50785054@N03/51888310050. It was reviewed on 6 June 2023 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

6 June 2023

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Date/TimeThumbnailDimensionsUserComment
current21:07, 6 June 2023Thumbnail for version as of 21:07, 6 June 20231,761 × 1,757 (3.91 MB)Astromessier (talk | contribs)Transferred from Flickr via #flickr2commons

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