File:Gas Absorbing Starlight (4772).jpg

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Hubble’s ULLYSES program will observe the ultraviolet light stars emit—and spread that light into its component wavelengths, which are known as spectra.

Summary[edit]

Description
English: Hubble’s ULLYSES program will observe the ultraviolet light stars emit—and spread that light into its component wavelengths, which are known as spectra. This graph, which shows two spectra, maps how much far-ultraviolet light the two stars are emitting through the gas in their surrounding galaxies. The star in the dwarf galaxy Sextans A, represented in purple, has emitted light, but there isn’t much gas nearby absorbing it. In contrast, the star in the Large Magellanic Cloud, represented in teal, shows that there is sulfur blocking some of its light. By analyzing the elements between us and the stars, researchers can learn about the conditions and history of the gas and dust surrounding stars in distant galaxies.
Date 5 November 2020 (upload date)
Source Gas Absorbing Starlight
Author , , and Z. Levy ()

Licensing[edit]

Public domain This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) 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 is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.
For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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