CaltechAUTHORS
  A Caltech Library Service

Sublimation pit distribution indicates convection cell surface velocities of ∼10 cm per year in Sputnik Planitia, Pluto

Buhler, Peter B. and Ingersoll, Andrew P. (2018) Sublimation pit distribution indicates convection cell surface velocities of ∼10 cm per year in Sputnik Planitia, Pluto. Icarus, 300 . pp. 327-340. ISSN 0019-1035. http://resolver.caltech.edu/CaltechAUTHORS:20170921-101750166

[img] PDF - Accepted Version
See Usage Policy.

1820Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20170921-101750166

Abstract

The ∼10^6 km^2 Sputnik Planitia, Pluto is the upper surface of a vast basin of nitrogen ice. Cellular landforms in Sputnik Planitia with areas in the range of a few × 10^2–10^3 km^2 are likely the surface manifestation of convective overturn in the nitrogen ice. The cells have sublimation pits on them, with smaller pits near their centers and larger pits near their edges. We map pits on seven cells and find that the pit radii increase by between 2.1 ± 0.4 × 10^(−3) and 5.9 ± 0.8 × 10^(−3) m m^(−1) away from the cell center, depending on the cell. This is a lower bound on the size increase because of the finite resolution of the data. Accounting for resolution yields upper bounds on the size vs. distance distribution of between 4.2 ± 0.2 × 10^(−3) and 23.4 ± 1.5 × 10^(−3)m m^(−1). We then use an analytic model to calculate that pit radii grow via sublimation at a rate of 3.6_(−0.6)^(+2.1)×10^(−4) m yr^(−1), which allows us to convert the pit size vs. distance distribution into a pit age vs. distance distribution. This yields surface velocities between 1.5_(−0.2)^(+1.0) and 6.2_(−1.4)^(+3.4) cm yr^(−1) for the slowest cell and surface velocities between 8.1_(−1.0)^(+5.5) and 17.9_(−5.1)^(+8.9) cm yr^(−1) for the fastest cell. These convection rates imply that the surface ages at the edge of cells reach ∼4.2–8.9 × 10^5 yr. The rates are comparable to rates of ∼6 cm yr^(−1) that were previously obtained from modeling of the convective overturn in Sputnik Planitia (McKinnon et al., 2016). Finally, we investigate the surface rheology of the convection cells and estimate that the minimum ice viscosity necessary to support the geometry of the observed pits is of order 10^(16)–10^(17) Pa s, based on the argument that pits would relax away before growing to their observed radii of several hundred meters if the viscosity were lower than this value.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1016/j.icarus.2017.09.018DOIArticle
http://www.sciencedirect.com/science/article/pii/S0019103516308004PublisherArticle
ORCID:
AuthorORCID
Ingersoll, Andrew P.0000-0002-2035-9198
Alternate Title:Sublimation Pit Distribution Indicates Convection Cell Surface Velocities of ∼10 Centimeters per Year in Sputnik Planitia, Pluto
Additional Information:© 2017 Elsevier Inc. Received 2 December 2016, Revised 6 September 2017, Accepted 11 September 2017, Available online 21 September 2017. We thank Heather Knutson for insightful conversations on statistical analysis and Dave Stevenson for illuminating discussions about ice rheology. We also appreciate helpful discussions with Orkan Umurhan and Bill McKinnon. Input from Francis Nimmo and two anonymous reviewers improved the quality of this paper. We are grateful for funding from NASA Earth and Space Science Fellowship grant #16-PLANET16F-0071.
Funders:
Funding AgencyGrant Number
NASA Earth Space and Science Fellowship16-PLANET16F-0071
Record Number:CaltechAUTHORS:20170921-101750166
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170921-101750166
Official Citation:Peter B. Buhler, Andrew P. Ingersoll, Sublimation pit distribution indicates convection cell surface velocities of ∼10 cm per year in Sputnik Planitia, Pluto, In Icarus, Volume 300, 2018, Pages 327-340, ISSN 0019-1035, https://doi.org/10.1016/j.icarus.2017.09.018. (http://www.sciencedirect.com/science/article/pii/S0019103516308004)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:81672
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Sep 2017 17:31
Last Modified:27 Nov 2017 17:09

Repository Staff Only: item control page