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Detection of ammonia on Pluto's surface in a region of geologically recent tectonism.

Authors :
Dalle Ore CM
Cruikshank DP
Protopapa S
Scipioni F
McKinnon WB
Cook JC
Grundy WM
Schmitt B
Stern SA
Moore JM
Verbiscer A
Parker AH
Singer KN
Umurhan OM
Weaver HA
Olkin CB
Young LA
Ennico K
Source :
Science advances [Sci Adv] 2019 May 29; Vol. 5 (5), pp. eaav5731. Date of Electronic Publication: 2019 May 29 (Print Publication: 2019).
Publication Year :
2019

Abstract

We report the detection of ammonia (NH <subscript>3</subscript> ) on Pluto's surface in spectral images obtained with the New Horizons spacecraft that show absorption bands at 1.65 and 2.2 μm. The ammonia signature is spatially coincident with a region of past extensional tectonic activity (Virgil Fossae) where the presence of H <subscript>2</subscript> O ice is prominent. Ammonia in liquid water profoundly depresses the freezing point of the mixture. Ammoniated ices are believed to be geologically short lived when irradiated with ultraviolet photons or charged particles. Thus, the presence of NH <subscript>3</subscript> on a planetary surface is indicative of a relatively recent deposition or possibly through exposure by some geological process. In the present case, the areal distribution is more suggestive of cryovolcanic emplacement, however, adding to the evidence for ongoing geological activity on Pluto and the possible presence of liquid water at depth today.<br /> (Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).)

Details

Language :
English
ISSN :
2375-2548
Volume :
5
Issue :
5
Database :
MEDLINE
Journal :
Science advances
Publication Type :
Academic Journal
Accession number :
31608308
Full Text :
https://doi.org/10.1126/sciadv.aav5731