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Reorientation of Sputnik Planitia implies a subsurface ocean on Pluto
F Nimmo1, D P Hamilton2, W B McKinnon3
1Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, California 95064, USA.
Nature
|November 17, 2016
Summary
Pluto's Sputnik Planitia basin may be an impact scar. Its location suggests a subsurface ocean, which would explain its gravity anomaly and allow for a long-lived ocean, crucial for understanding Pluto's geology.
Area of Science:
- Planetary Science
- Geophysics
- Astrobiology
Background:
- Sputnik Planitia on Pluto is a large, nitrogen-covered basin near the planet's tidal axis.
- Its current location suggests reorientation due to tidal and rotational forces.
- The basin presents a negative topography but requires a positive gravity anomaly for reorientation.
Purpose of the Study:
- To investigate the formation and current state of Sputnik Planitia.
- To determine the conditions necessary for the basin's observed gravity anomaly and location.
- To assess the role of a potential subsurface ocean in Pluto's geological evolution.
Main Methods:
- Analysis of gravitational anomalies and topographic data.
- Modeling of impact basin formation and planetary reorientation.
- Assessment of subsurface ocean dynamics and shell properties.
Main Results:
- A positive gravity anomaly in Sputnik Planitia is explained by shell thinning and ocean uplift, assuming an impact origin and a subsurface ocean.
- Without a subsurface ocean, an implausibly thick nitrogen layer would be required to explain the gravity anomaly.
- A rigid, conductive ice shell is necessary to maintain a long-lived subsurface ocean and its associated uplift.
Conclusions:
- The presence of a subsurface ocean is a likely explanation for Sputnik Planitia's characteristics.
- A subsurface ocean on Pluto could have persisted to the present day.
- Complex feedbacks between nitrogen deposition, loading, and planetary reorientation may have influenced Pluto's geological history.
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