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Natural Analogue Constraints on Europa's Non‐ice Surface Material
Author(s) -
FoxPowell Mark G.,
Osinski Gordon R.,
Applin Daniel,
Stromberg Jessica M.,
Gázquez Fernando,
Cloutis Ed,
Allender Elyse,
Cousins Claire R.
Publication year - 2019
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2018gl081339
Subject(s) - sulfate , icy moon , astrobiology , geology , chloride , jupiter (rocket family) , mineralogy , reflectivity , geochemistry , natural (archaeology) , chemistry , planet , paleontology , physics , saturn , optics , organic chemistry , space shuttle , astronomy , astrophysics
Abstract Non‐icy material on the surface of Jupiter's moon Europa is hypothesized to have originated from its subsurface ocean and thus provide a record of ocean composition and habitability. The nature of this material is debated, but observations suggest that it comprises hydrated sulfate and chloride salts. Analogue spectroscopic studies have previously focused on single‐phase salts under controlled laboratory conditions. We investigated natural salts from perennially cold (<0 °C) hypersaline springs and characterized their reflectance properties at 100, 253, and 293 K. Despite similar major ion chemistry, these springs form mineralogically diverse deposits, which when measured at 100 K closely match reflectance spectra from Europa. In the most sulfate‐rich samples, we find that spectral features predicted from laboratory salts are obscured. Our data are consistent with sulfate‐dominated europan non‐icy material and further show that the emplacement of endogenic sulfates on Europa's surface would not preclude a chloride‐dominated ocean.