File:Webb’s Mid-Infrared Spectroscopy Will Reveal Molecules, Elements.png

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English: This portion of the MIRI MRS wavelength range shows engineering calibration data obtained of the Seyfert galaxy NGC 6552 (red line) in the constellation Draco. The strong emission feature is due to molecular hydrogen, with an additional weaker feature nearby. The blue line shows a lower spectral resolution Spitzer IRS spectrum of a similar galaxy for comparison. The Webb test observations were obtained to establish the wavelength calibration of the spectrograph. Credit: NASA, ESA, and the MIRI Consortium.
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Source https://www.flickr.com/photos/nasawebbtelescope/52184594070/
Author NASA's James Webb Space Telescope

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This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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  • 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@N03/52184594070. It was reviewed on 2 July 2022 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

2 July 2022

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current09:22, 2 July 2022Thumbnail for version as of 09:22, 2 July 20222,048 × 1,358 (1.25 MB)Erick Soares3 (talk | contribs)Uploaded a work by NASA's James Webb Space Telescope from https://www.flickr.com/photos/nasawebbtelescope/52184594070/ with UploadWizard

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