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Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

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Page 1: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Astronomy190 - Topics in Astronomy

Astronomy and Astrobiology

Lecture 15 : Ancient Mars

Ty Robinson

Page 2: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Questions of the Day

• What is the evidence for liquid water on early Mars?

• What was different about early Mars that made it possible for liquid water to exist on its surface?

• What processes have subsequently affected Mars’ ability to sustain liquid water on its surface?

Page 3: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Surface Ages

Page 4: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence from Space I

Mars

Earth

Mars

Riverbeds

Page 5: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence from Space II

Mars

Earth

Mars

Sedimentary Layers

Page 6: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence from Space III

Flooding

Page 7: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence for Water I

• Satellite Images– Riverbeds– Sedimentary layers– Flooding

Evidence for Water

Page 8: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Follow the Water

Page 9: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Mars Pathfinder

Launch: Dec. 1996Operation: Jul-Sep 1997

Instruments: - cameras - weather sensors - rock analysis tools

Page 10: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Pathfinder Landing

landing video

Page 11: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence for Water II

• Satellite Images– Riverbeds– Sedimentary layers– Flooding

• Pathfinder– Maghemite– Flood plain

Evidence for Water

Page 12: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Mars Exploration Rovers

Launch: Jun, Jul 2003Operation: Jan 2004 - ?

Instruments: - cameras - weather sensors - rock analysis tools - microscope

Page 13: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Landing Sites

Page 14: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Gusev Crater

Page 15: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Extended Mission

Page 16: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Landing Sites

Page 17: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Minerals from Space

Page 18: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Opportunity Landing Site

Page 19: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Extended Mission

Page 20: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Chlorine and Sediments

Page 21: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Evidence for Water III

• Satellite Images– Riverbeds– Sedimentary layers– Flooding

• Pathfinder– Maghemite– Flood plain

• Spirit– Silica deposits

• Opportunity– Sediments– Blueberries– Chlorine concentration

Evidence for Water

Page 22: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Questions?Liquid water is not stable on the surface of modern-day Mars because…

temperatures are too low

surface pressure is too low

both surface temperatures and pressures are too low

water does not exist on Mars

Page 23: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Questions?What must have been different about Mars in the past so that liquid water was stable on its surface?

thicker atmosphere

thicker atmosphere with more greenhouse gases

Mars must have had a stronger magnetic field

Mars must have been closer to the Sun

Page 24: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Greenhouse

Page 25: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Summary

Page 26: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Atmospheric Escape

Impact Erosion

Photolysis

Solar Wind

Page 27: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Questions of the Day

• What is the evidence for liquid water on early Mars?

• What was different about early Mars that made it possible for liquid water to exist on its surface?

• What processes have subsequently affected Mars’ ability to sustain liquid water on its surface?

Page 28: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Quiz

3 - What is one thing you did not understand from today’s lecture?

2 - Explain why increasing chlorine concentrations with depth in a crater is evidence for the existence of water there in the past.

1 - What are three pieces of evidence that point to a wet early Mars which can be seen from space?