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Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson
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Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Jan 15, 2016

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Page 1: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Astronomy190 - Topics in Astronomy

Astronomy and Astrobiology

Lecture 14 : Modern Mars

Ty Robinson

Page 2: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions of the Day

• How has our understanding of Mars changed over the last 100 years?

• What did the Viking Biological Experiments tell us about the habitability of Mars’ surface?

• How has the Phoenix Lander influenced our perspective on the present-day habitability of Mars?

Page 3: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Perspective

Page 4: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Circa 1900

hand drawn map1894

The Good The Bad The Imaginative

Page 5: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

What We Learned

• Polar Caps• Seasons• Atmosphere

Page 6: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Mariner 4

Launch: Nov. 1964Flyby: July 1965

~300km = 200miles

~300km = 200miles

Instruments: - camera - magnetometer

QuestionWhat can we learn?

Page 7: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

What We Learned

• Atmosphere– Thin (~0.01 bars)

• Climate– Cold (-100 °C)

• Polar Caps– CO2 ice

– H2O ice

Page 8: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions?Mariner 4 failed to measure a strong magnetic field around Mars. This is tells us…

Mars does not rotate fast enough

Mars’ composition is very different from that of Earth

Mars is not within the Habitable Zone

Mars does not have a liquid, conducting core

Page 9: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions?Mars does not have a liquid, conducting core. This tells us…

Mars cannot support life

Mars’ composition is very different from that of Earth

Mars is geologically inactive

Mars atmosphere is not volcanically-derived

Page 10: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Viking Landers

Launch: Aug., Sep. 1975Operation: 1976-1982

Instruments: - cameras - temp. sensors - wind sensors - seismometer - gas sensors

QuestionWhat can we learn?

Page 11: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

What We Learned

• Geological Activity– None at present

• Polar Caps– CO2 ice

– H2O ice

• Atmosphere– Thin (~0.01 bars)

– Composition (CO2, N2, O2)

• Weather– Dust storms

• Climate– Cold (-100 °C)– T. Var’n (-140 to 30 °C)

Page 12: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Viking Biological Experiments

1 - carbon assimilation experiment

2 - gas exchange experiment

3 - labeled release experiment

4 - gas chromatograph experiment

Page 13: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Carbon Assimilation

+ + +

+ +

=

In the chamber… add Martian soil… and radioactive carbon…

and water… and light.

Evacuate the chamber and bake the soil to release volatiles.

Page 14: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Gas Exchange

+ + =

Controls: - add only water - perform experiment without light - bake the soil before the experiment

Question

What are some control experiments?

In the chamber… add Martian soil… and nutrients.

Monitor the gases inside the chamber through time.

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

Labeled Release

+ +

=

Control = heat the soil first

In the chamber… add Martian soil…

and nutrients containing radioactive carbon.

Monitor the gases inside the chamber through time.

Page 16: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Gas Chromatograph

+ + =

Result : Martian soil contains even less organic material than Lunar soils returned by the Apollo astronauts.

Life on Mars’ Surface

In the chamber… add Martian soil… and bake.

Look for organic-derived gases.

Page 17: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Mars Odyssey

Page 18: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Landing Sites

Page 19: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Phoenix Lander

Launch: Aug. 2007Operation: Aug-Nov 2008

Instruments: - cameras - weather sensors - soil analysis tools

Page 20: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

What We Learned

• Geological Activity– None at present

• Polar Caps– CO2 ice

– H2O ice

• Atmosphere– Thin (~0.01 bars)

– Composition (CO2, N2, O2)

• Weather– Dust storms

• Climate – Cold (-100 °C)

– T. Var’n (-140 to 30 °C)

• Sub-surface– H2O ice

Page 21: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Phoenix Descent

Heimdall Crater (10km Wide)

Phoenix Lander parachuting to surface

Page 22: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Phoenix Landed

heat shield

parachute

Phoenix

Page 23: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Phase Diagram

Credit : Toby Smith

Page 24: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Mars Present-Day Habitability I

Page 25: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Mars Present-Day Habitability II

Page 26: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Methane?

Page 27: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions?If the methane on bars is due to life, the type of organism most likely responsible for creating the methane is…

chemoautotroph

chemoheterotroph

photoautotroph

photoheterotroph

Page 28: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions?

Assuming chemoautotrophs are responsible for methane on Mars, what might explain the observations that methane levels vary seasonally?

Page 29: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Mars Overview

Polar caps

Atmosphere

Weather

Climate

Subsurface ice

Page 30: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Questions of the Day

• How has our understanding of Mars changed over the last 100 years?

• What did the Viking Biological Experiments tell us about the habitability of Mars’ surface?

• How has the Phoenix Lander influenced our perspective on the present-day habitability of Mars?

Page 31: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.

Quiz

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

2 - Explain the arguments for why we might expect to find subsurface liquid water on Mars. What evidence do we have for this?

1 - In light of the Viking Biological Experiments, why do most scientists rule out the possibility of life on the surface of modern-day Mars?