Even though dust covered, there were several ‘crater-like’ features visible rising above the dust .
Carl Sagan took a polaroid of the TV screen in the headquarters of Mariner 9 – he rushed into a group of scientists in the next room and they realized that these were volcanic calderas!!
Slide 11
349 days in orbit (circled Mars twice daily for a year)
Mariner 9 transmitted 7,329 images, covering over 80% of Mars' surface
lowest altitude images distance of spacecraft ~900 miles above surface
An infrared radiometer was included to detect volcanic activity
Mars' tiny moons, Phobos and Deimos, were also photographed.
Channels on the flanks of the
volcano Hecates Tholus. Various
radial channels have been interpreted
as erosional ash channels,
lava channels or channels eroded
by fluvial processes.
Mariner 9 narrow angle camera.
Slide 12
The images revealed structures
resembling river beds
The images revealed structures
resembling river beds
Olympus Mons – 3x as high
as volcanoes on Earth
Slide 13
Valles Marineris – picture from Mariner
Valles Marineris - system of canyons over 4,000 km (2,500 miles)
- revived people’s interest in possible water/life
Slide 14
- streches for at least 2500 miles (NYC ßà LA)
- “rift valley” – region broken by crust motions earlier in Mars’ history
signs of river erosion in early history of Mars (3-4 Billion yrs ago) like Grand Canyon
Slide 15
Viking 1 and 2 – Orbiter & Lander
Slide 16
This image is a mosaic of the
Schiaparelli hemisphere of Mars.
The center of this image is near
the impact crater Schiaparelli,
450 kilometers (280 miles) across!.
Bright white areas to the south,
including the Hellas impact basin
at extreme lower right, are covered
by carbon dioxide frost.
Slide 17
Viking Orbiter
This image is a mosaic of the
Valles Marineris hemisphere of Mars.
The center is the Valles Marineris system – 3,000 km (1,860 miles) long and up to 8 km (5 miles) deep.
Many huge ancient river channels begin from the chaotic terrain and north-central canyons and run north.