File:Water in Protoplanetary Disk of PDS 70 (MIRI Emission Spectrum) (2023-130).jpg

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Summary

Description
English: A spectrum of the protoplanetary disk of PDS 70, obtained with Webb’s MIRI (Mid-Infrared Instrument), displays a number of emission lines from water vapor. Scientists determined that the water is in the system’s inner disk, at distances of less than 100 million miles from the star – the region where rocky, terrestrial planets may be forming. NASA, ESA, CSA, Joseph Olmsted (STScI)
Date 24 July 2023 (upload date)
Source Water in Protoplanetary Disk of PDS 70 (MIRI Emission Spectrum)
Author Illustration
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Licensing

Public domain This file is in the public domain because it was created by NASA, ESA and CSA. NASA Webb material is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA/CSA is credited as the source of the material. This license does not apply if source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-03127. Copyright statement at webbtelescope.org.
For material created by the European Space Agency on the esawebb.org site, use the {{ESA-Webb}} tag.

Captions

A spectrum of the protoplanetary disk of PDS 70, obtained with Webb’s MIRI (Mid-Infrared Instrument), displays a number of emission lines from water vapor.

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24 July 2023

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current10:30, 25 July 2023Thumbnail for version as of 10:30, 25 July 20233,840 × 2,160 (666 KB)OptimusPrimeBot#Spacemedia - Upload of https://stsci-opo.org/STScI-01H5MY1NGTKXY4NC0YVG2D0VEQ.jpg via Commons:Spacemedia
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