The Influence of Temperature and Photobleaching on Irradiated Sodium Chloride at Europa-like Conditions
Abstract
Europa's leading-hemisphere chaos regions have a spectral feature at 450 nm that has been attributed to absorption by crystal defects in irradiated sodium chloride, known as F-centers. Some discrepancies exist between the laboratory data of irradiated sodium chloride and the observations, including a ∼10 nm shift in central wavelength of the F-center band and the lack of the prominent 720 nm absorption on Europa from M-centers, which result from the coalescence of pairs of F-centers. Here, we perform irradiation experiments on sodium chloride in an attempt to understand these discrepancies. We show that careful control of the temperature of the sample at 120 K yields F-centers with an absorption wavelength comparable to that of Europa. In addition, we measure the effect of photobleaching—the destruction of F-centers by photons—and show that at the energetic particle and photon flux on Europa, an equilibrium will be reached where only a modest F-center absorption develops. The density of F-centers never reaches high enough values for the creation of secondary M-centers. Our experiments predict that F-centers grow during the night on Europa in the absence of photobleaching and then partially decay during the daytime. We show observations from the Hubble Space Telescope consistent with this prediction. All observations of the 450 nm F-center on Europa are now consistent with laboratory measurements of sodium chloride, confirming the presence of this salt on Europa.
Additional Information
© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2021 July 30; revised 2021 October 25; accepted 2021 October 27; published 2022 February 2. This work was supported by grant number 668346 from the Simons Foundation. The observations were made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. These observations are associated with program # 14650. This work is also associated with archival program # 15789. This data was obtained from the Mikulski Archive for Space Telescopes (MAST). This specific observations analyzed can be accessed via 10.17909/t9-awev-6407. Support for program #15789 was provided by NASA through grants from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. S.K.T. is supported by the Heising–Simons Foundation through a 51 Pegasi b postdoctoral fellowship.Attached Files
Published - Denman_2022_Planet._Sci._J._3_26.pdf
Accepted Version - 2201.01332.pdf
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Additional details
- Eprint ID
- 113254
- Resolver ID
- CaltechAUTHORS:20220203-317920000
- Simons Foundation
- 668346
- NASA
- NAS5-26555
- Heising-Simons Foundation
- 51 Pegasi b Fellowship
- Created
-
2022-02-03Created from EPrint's datestamp field
- Updated
-
2022-02-03Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)