XANTHE TERRA OUTFLOW CHANNEL GEOLOGY AT THE MARS PATHFINDER LANDING SITE. D.M. Nelson, R. Greeley. Department of Geology, Box[removed], Arizona State University, Tempe, Arizona, [removed], USA. E-mail: [removed]

Source URL: mars.jpl.nasa.gov

• Geomorphology
• Outflow channels
• Chryse Planitia
• Ares Vallis
• Vallis
• Valles Marineris
• Noachian
• Hesperian
• Iani Chaos
• Mars
• Planetary geology
• Planetary science

XANTHE TERRA OUTFLOW CHANNEL GEOLOGY AT THE MARS PATHFINDER LANDING SITE. D.M. Nelson, R. Greeley. Department of Geology, Box[removed], Arizona State University, Tempe, Arizona, [removed], USA. E-mail: [removed]

Source URL: marsprogram.jpl.nasa.gov

• Geomorphology
• Outflow channels
• Chryse Planitia
• Ares Vallis
• Vallis
• Valles Marineris
• Noachian
• Hesperian
• Iani Chaos
• Mars
• Planetary geology
• Planetary science

Iani Chaos, Margaritifer Terra, Mars The source of the outflow channel Ares Vallis on Mars is called Iani Chaos. It was most likely formed

Source URL: www.lpi.usra.edu

Iani Chaos, Margaritifer Terra, Mars The source of the outflow channel Ares Vallis lies in an area of jumbled and broken slabs of rock. This area, called Iani Chaos, probably formed when

Source URL: www.lpi.usra.edu

Iani Chaos as a landing site for the Mars Science Laboratory. T. D. Glotch1, 1Jet Propulsion Laboratory, California Institute of Technology. [removed] Iani Chaos, the source region of Ares Valles, is centered at ~342°E, 2°S. The chaotic terrain is widelybelieved to have formed via the removal of subsurface

Source URL: marsoweb.nas.nasa.gov

• Iani Chaos
• Albedo features on Mars
• Meridiani Planum
• Hematite
• Mars Exploration Rover
• Aram Chaos
• Outflow channels
• Chaos terrain
• Vallis
• Mars
• Margaritifer Sinus quadrangle
• Planetary geology