Complex Brines and Their Implications for Habitability

There is evidence that life on Earth originated in cold saline waters around scorching hydrothermal vents, and that similar conditions might exist or have existed on Mars, Europa, Ganymede, Enceladus, and other worlds. Could potentially habitable complex brines with extremely low freezing temperatur...

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Main Authors: Nilton O. Renno, Erik Fischer, Germán Martínez, Jennifer Hanley
Format: Article
Language:English
Published: MDPI AG 2021-08-01
Series:Life
Subjects:
Online Access:https://www.mdpi.com/2075-1729/11/8/847
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spelling doaj-d437ab5df3ea45d3a06d95afde19184c2021-08-26T13:59:20ZengMDPI AGLife2075-17292021-08-011184784710.3390/life11080847Complex Brines and Their Implications for HabitabilityNilton O. Renno0Erik Fischer1Germán Martínez2Jennifer Hanley3Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109, USADepartment of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109, USALunar and Planetary Institute, Universities Space Research Association, Houston, TX 75835, USALowell Observatory, Flagstaff, AZ 86001, USAThere is evidence that life on Earth originated in cold saline waters around scorching hydrothermal vents, and that similar conditions might exist or have existed on Mars, Europa, Ganymede, Enceladus, and other worlds. Could potentially habitable complex brines with extremely low freezing temperatures exist in the shallow subsurface of these frigid worlds? Earth, Mars, and carbonaceous chondrites have similar bulk elemental abundances, but while the Earth is depleted in the most volatile elements, the Icy Worlds of the outer solar system are expected to be rich in them. The cooling of ionic solutions containing substances that likely exist in the Icy Worlds could form complex brines with the lowest eutectic temperature possible for the compounds available in them. Indeed, here, we show observational and theoretical evidence that even elements present in trace amounts in nature are concentrated by freeze–thaw cycles, and therefore contribute significantly to the formation of brine reservoirs that remain liquid throughout the year in some of the coldest places on Earth. This is interesting because the eutectic temperature of water–ammonia solutions can be as low as ~160 K, and significant fractions of the mass of the Icy Worlds are estimated to be water substance and ammonia. Thus, briny solutions with eutectic temperature of at least ~160 K could have formed where, historically, temperature have oscillated above and below ~160 K. We conclude that complex brines must exist in the shallow subsurface of Mars and the Icy Worlds, and that liquid saline water should be present where ice has existed, the temperature is above ~160 K, and evaporation and sublimation have been inhibited.https://www.mdpi.com/2075-1729/11/8/847brinescomplex brinesliquid waterhabitabilityhabitablelife
collection DOAJ
language English
format Article
sources DOAJ
author Nilton O. Renno
Erik Fischer
Germán Martínez
Jennifer Hanley
spellingShingle Nilton O. Renno
Erik Fischer
Germán Martínez
Jennifer Hanley
Complex Brines and Their Implications for Habitability
Life
brines
complex brines
liquid water
habitability
habitable
life
author_facet Nilton O. Renno
Erik Fischer
Germán Martínez
Jennifer Hanley
author_sort Nilton O. Renno
title Complex Brines and Their Implications for Habitability
title_short Complex Brines and Their Implications for Habitability
title_full Complex Brines and Their Implications for Habitability
title_fullStr Complex Brines and Their Implications for Habitability
title_full_unstemmed Complex Brines and Their Implications for Habitability
title_sort complex brines and their implications for habitability
publisher MDPI AG
series Life
issn 2075-1729
publishDate 2021-08-01
description There is evidence that life on Earth originated in cold saline waters around scorching hydrothermal vents, and that similar conditions might exist or have existed on Mars, Europa, Ganymede, Enceladus, and other worlds. Could potentially habitable complex brines with extremely low freezing temperatures exist in the shallow subsurface of these frigid worlds? Earth, Mars, and carbonaceous chondrites have similar bulk elemental abundances, but while the Earth is depleted in the most volatile elements, the Icy Worlds of the outer solar system are expected to be rich in them. The cooling of ionic solutions containing substances that likely exist in the Icy Worlds could form complex brines with the lowest eutectic temperature possible for the compounds available in them. Indeed, here, we show observational and theoretical evidence that even elements present in trace amounts in nature are concentrated by freeze–thaw cycles, and therefore contribute significantly to the formation of brine reservoirs that remain liquid throughout the year in some of the coldest places on Earth. This is interesting because the eutectic temperature of water–ammonia solutions can be as low as ~160 K, and significant fractions of the mass of the Icy Worlds are estimated to be water substance and ammonia. Thus, briny solutions with eutectic temperature of at least ~160 K could have formed where, historically, temperature have oscillated above and below ~160 K. We conclude that complex brines must exist in the shallow subsurface of Mars and the Icy Worlds, and that liquid saline water should be present where ice has existed, the temperature is above ~160 K, and evaporation and sublimation have been inhibited.
topic brines
complex brines
liquid water
habitability
habitable
life
url https://www.mdpi.com/2075-1729/11/8/847
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