chapter 7c mars: freeze-dried
DESCRIPTION
Chapter 7c Mars: Freeze-dried. Image from: http://pds.jpl.nasa.gov/planets/welcome.htm. Mars. Orbital distance: 227 940 000 km (1.52 AU) 2 nd most eccentric Year: 686.971 d Day: 1.025 d Temperature: Max: 35°C (95 °F) Summer Min: −125 °C (-193 °F) winter. Diameter: 6794 km - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/1.jpg)
Chapter 7cMars: Freeze-dried
Image from: http://pds.jpl.nasa.gov/planets/welcome.htm
![Page 2: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/2.jpg)
Mars• Orbital distance:
– 227 940 000 km (1.52 AU)– 2nd most eccentric
• Year:– 686.971 d
• Day:– 1.025 d
• Temperature:– Max: 35°C (95 °F) Summer
– Min: −125 °C (-193 °F)
winter
• Diameter:– 6794 km
• Density:– 3.933 g/cm3
• Composition:– Iron/nickel/sulfur core,
rock
• Axial Tilt: 25.1o
• Moons: two (may be captured asteroids)
• Other:– Has seasons
– Largest volcano in solar system
![Page 3: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/3.jpg)
7.3 Mars: A Victim of Planetary Freeze-drying
• Our Goals for Learning
• What geological features tell us that water once flowed on Mars?
• Why did Mars change?
![Page 4: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/4.jpg)
Mars vs. Earth
• 50% Earth’s radius, 10% Earth’s mass• 1.5 A.U from the Sun• Axis tilt about the same as Earth.• Similar rotation period.• Orbit is more elliptical than Earth’s: seasons
more extreme• Thin CO2 atmosphere: little greenhouse
![Page 5: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/5.jpg)
What geological features tell us water once flowed on Mars?
![Page 6: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/6.jpg)
Surface of Mars appears to have ancient river beds
![Page 7: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/7.jpg)
Condition of craters indicates surface history
Eroded crater
![Page 8: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/8.jpg)
Closeup of eroded crater
![Page 9: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/9.jpg)
![Page 10: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/10.jpg)
Volcanoes…as recent as 180 million years ago…
![Page 11: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/11.jpg)
Past tectonic activity…
![Page 12: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/12.jpg)
Low-lying regions may once have had oceans
![Page 13: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/13.jpg)
Low-lying regions may once have had oceans
![Page 14: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/14.jpg)
OpportunitySpirit
![Page 15: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/15.jpg)
• 2004 Opportunity Rover provided strong evidence for abundant liquid water on Mars in the distant past.•How could Mars have been warmer and wetter in the past?
![Page 16: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/16.jpg)
Today, most water lies frozen underground (blue regions)…
Some scientists believe accumulated snowpack melts to carve gullies even today
![Page 17: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/17.jpg)
Why did Mars change?
![Page 18: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/18.jpg)
Would “terraforming” Mars work?
• Yes
• No
• Rovers?
![Page 19: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/19.jpg)
What have we learned?• What geological features
tell us that water once flowed on Mars?
• Dry river channels, rock-strewn floodplains, and eroded craters all show that water once flowed on Mars, though any periods of rainfall seem to have ended at least 3 billion years ago. Mars today still has water ice underground and in its polar caps, and could possibly have pockets of underground liquid water.
![Page 20: Chapter 7c Mars: Freeze-dried](https://reader037.vdocuments.mx/reader037/viewer/2022102909/568137c3550346895d9f6237/html5/thumbnails/20.jpg)
What have we learned?• Why did Mars change? Mars’s atmosphere must once have been much
thicker with a much stronger greenhouse effect, so change must have occurred due to loss of atmospheric gas. Much of the lost gas probably was stripped away by the solar wind, which was able to reach the atmosphere as Mars cooled and lost its magnetic field and protective magnetosphere. Water was probably also lost because ultraviolet light could break apart water molecules in the atmosphere, and the lightweight hydrogen then escaped to space.