4.5 Article

Cryovolcanic flooding in Viking Terra on Pluto

Journal

ICARUS
Volume 356, Issue -, Pages -

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2020.113786

Keywords

Pluto; Volcanism; IR spectroscopy; Surface; Ices

Funding

  1. NASA's New Horizons project
  2. France's Centre National d'Etudes Spatiales (CNES)

Ask authors/readers for more resources

The prominent fossa trough and adjacent impact crater on Pluto's Viking Terra show evidence of being filled with a material of uniform texture and red-brown color, possibly cryolava. Spectral maps indicate the presence of H2O ice and ammoniated components in these structures, potentially ammonia hydrates or ammoniated salts. The study suggests that the crater and fossa trough were flooded by cryolava from Pluto's interior, which contained liquid water infused with red-brown pigment and ammonia compounds.
A prominent fossa trough (Uncama Fossa) and adjacent 28-km diameter impact crater (Hardie) in Pluto's Viking Terra, as seen in the high-resolution images from the New Horizons spacecraft, show morphological evidence of in-filling with a material of uniform texture and red-brown color. A linear fissure parallel to the trough may be the source of a fountaining event yielding a cryoclastic deposit having the same composition and color properties as is found in the trough and crater. Spectral maps of this region with the New Horizons LEISA instrument reveal the spectral signature of H2O ice in these structures and in distributed patches in the adjacent terrain in Viking Terra. A detailed statistical analysis of the spectral maps shows that the colored H2O ice filling material also carries the 2.2-mu m signature of an ammoniated component that may be an ammonia hydrate (NH3.nH(2)O) or an ammoniated salt. This paper advances the view that the crater and fossa trough have been flooded by a cryolava debouched from Pluto's interior along fault lines in the trough and in the floor of the impact crater. The now frozen cryolava consisted of liquid H2O infused with the red-brown pigment presumed to be a tholin, and one or more ammoniated compounds. Although the abundances of the pigment and ammoniated compounds entrained in, or possibly covering, the H2O ice are unknown, the strong spectral bands of the H2O ice are clearly visible. In consideration of the factors in Pluto's space environment that are known to destroy ammonia and ammoniawater mixtures, the age of the exposure is of order <= 10(9) years. Ammoniated salts may be more robust, and laboratory investigations of these compounds are needed.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.5
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available