Mars Dead or Alive: Mars Up Close

Resource for Grades 6-12

WGBH: Nova
Mars Dead or Alive: Mars Up Close

Media Type:
Interactive

Running Time:
Size: 51.2 KB


Source: NOVA: "Mars"

This resource can be found on the NOVA: "Mars Dead or Alive" & "Welcome to Mars" Web site.

Resource Produced by:

WGBH Educational Foundation

Collection Developed by:

WGBH Educational Foundation

Collection Credits

Collection Funded by:

National Science Foundation

Since landing on Mars in January 2004, the Mars Exploration Rovers have helped scientists learn an amazing amount about the red planet. The sophisticated rovers far exceeded expectations with the geological clues they have dug up about the planet's past. In this interactive tour from NOVA Online, the mission's principal science investigator, Steve Squyres, describes some of the great discoveries made by Spirit and Opportunity.

Alternate Media Available:

Mars Dead or Alive: Mars Up Close (HTML version) (Document)

open Background Essay

The Mars Exploration Rover mission was launched in 2003 with the goal of finding out more about the geological history of the planet and investigating the role liquid water may have played there. Life, at least all life as we know it, cannot survive without liquid water. While Mars has been declared a cold and lifeless place, scientists have had reason to believe that it may have once had a wetter and warmer environment able to support life. In an effort to find out if there was ever a chance for life on Mars, NASA's exploration strategy was to "follow the water."

On Earth, when water interacts with rock or sediment substrates, it may leave behind a variety of telltale signs. For example, flowing water carves out surface features or produces characteristic formations in rocks and sediments. Small holes in rocks, called vugs, may be found where crystals once existed but have since been either dissolved by a change in the water chemistry or eroded away. High concentrations of sulfate minerals are found in rocks that were formed in or have had long exposures to water. Certain minerals, such as gray hematite, are often formed by interaction with water. Other minerals, such as the uncommon jarosite, are only formed in acidic water. If these or similar features were found on Mars, they would be clues that water once existed there.

Twin robotic geologists, Spirit and Opportunity, were sent to Mars to look for such evidence. Both rovers were designed to have great mobility and were equipped with identical sets of five custom-made scientific instruments. Each rover body has a panoramic camera that creates high-resolution images and a spectrometer to determine mineralogy. Each rover also has a robotic arm that holds and maneuvers miniature versions of instruments used by geologists on Earth: a spectrometer to identify the elemental composition of rocks and soil, another spectrometer to specialize in iron-rich minerals, and a microscopic imager to enable close-up views of Martian features -- the first ever seen. In addition, the rovers also have a rock-abrasion tool to scrape off the outer surfaces of rocks and expose fresh interiors for study. Using evidence collected by all these tools and their knowledge of how water interacts with materials on Earth, many scientists have become convinced that Mars once had a watery environment that may have been able to support life.


open Discussion Questions

  • What clues did the scientists find that indicate that there may have been water on Mars?
  • Steve Squyres stated that scientists had made a hypothesis about the crater and believed it was an ancient lakebed. On what information did they base this hypothesis? How did the data coming from the Rover support or challenge the scientists' hypothesis?
  • Compare and contrast the formation of sedimentary and volcanic rock.
  • How did our knowledge of Earth surface processes help scientists in their analysis of ancient Mars environments?
  • What instruments do geologists use to analyze rocks on Mars - a location they cannot explore in person?

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