The Ice-Covered Lakes Hypothesis in Gale Crater: Implications for the Early Hesperian Climate

• Main Authors: Bristow, Thomas F., Kling, Alexandre M., Haberle, Robert M., Rivera-Hernandez, Frances, McKay, Christopher P.
• Format: Other/Unknown Material
• Language: unknown
• Published: 2017
• Subjects: Lunar and Planetary Science and Exploration; Antarctic; The Antarctic; Antarc*
• Online Access: http://hdl.handle.net/2060/20170000745

Recent geological discoveries from the Mars Science Laboratory (MSL), including stream and lake sedimentary deposits, provide evidence that Gale crater may have intermittently hosted a fluviol-acustine environment during the Hesperian, with individual lakes lasting for a period of tens to hundreds of thousands of years. Estimates of the CO2 content of the atmosphere at the time the Gale sediments formed are far less than needed by any climate model to warm early Mars, given the low solar energy input available at Mars 3.5 Gya. We have therefore explored the possibility that the lakes in Gale during the Hesperian were perennially covered with ice using the Antarctic lakes as analogs.