Mars Pathfinder

Bouncing & Roving



Mission Details

Landmark Dates
Craft
Destination

Mars Pathfinder

Launched: 4 Dec 1996
Vehicle: Delta II
Landed: 4 Jul 1997 16:57 UT


Mars

 

I name this rock "Scooby Doo"

This was the second of NASA's low cost planetary Discovery missions. It consisted of a stationary lander and a surface rover. The scientific objectives included atmospheric entry science, long-range and close-up surface imaging, with the general objectives being to characterise the Martian environment for further exploration.

 

The craft, using a revolutionary air bag landing system, first 'landed', or rather impacted the surface at a velocity of approximately 18 m/s (40mph) before bouncing around 15 metres into the air. Bouncing another 15 times and rolling along Pathfinder finally came to rest about 2.5 minutes later and about 1 km from the initial impact site.

The landing site in the Ares Vallis region is at 19.33 N, 33.55 W, and the pathfinder craft has been named the Sagan Memorial Station.

Pathfinder returned 2.6 billion pieces of information, including more than 1,000 images from the lander and 550 images from the rover as well as more than 15 chemical analyses of rocks and extensive data on winds and other weather factors.

Mission Results:

  • The possible identification of rounded pebbles and cobbles on the ground, and sockets and pebbles in some rocks, suggests conglomerates that formed in running water, during a warmer past in which liquid water was stable.
  • The atmospheric experiment package recorded a temperature profile different than expected from microwave measurements and Hubble observations. · Martian dust includes magnetic, composite particles with a mean size of one micron.
  • Dust is confirmed as the dominant absorber of solar radiation in Mars' atmosphere, which has important consequences for the transport of energy in the atmosphere and it's circulation.
  • Diversity of albedos, or variations in the brightness of the Martian surface, was similar to other observations, but there was no evidence for the types of crystalline hematite or pyroxene absorbtion features detected in other locations on Mars.
  • Rock size distribution was consistent with a flood - related deposit.
  • The moment of inertia of Mars was refined to a corresponding core radius of between 1.300 km and 2,600 km.
  • Rock chemistry at the landing site may be different from Martian meteorites found on Earth, and could be of basaltic andesite composition.
  • The weather was similar to that encountered by Viking I; there were rapid pressure and temperature variations, downslope winds at night, and light winds in general. Temperatures were about 10 degrees warmer than those measured by Viking I.
  • Frequent "dust devils" were found with an unmistakable temperature, wind, pressure signature, and morning turbulence. At least one of these may have contained dust, suggesting that these gusts are a mechanism for mixing dust into the atmosphere.
  • Morning atmospheric obscurations are due to clouds, not ground fog. Viking couldn't distinguish between these two possibilities.
  • The soil chemistry of Ares Vallis appears to be similar to that of the Viking I and II landing sites.
  • Evidence of wind abrasion of rocks and dune - shaped deposits was found, indicating the presence of sand.
  • The observed atmospheric clarity is higher than was expected from Earth - based microwave measurement and Hubble Space Telescope observations.

Still no sign of life, but we now have rocks named after cartoon characters, which can't be bad.

Rocks around the landing site were named: Yogi, Pooh Bear, Shaggy, Scooby Doo, Barnacle Bill, Stimpy, Mermaid, Snoopy and Casper.

Copyright © 2001 Captain Cosmos
with research by Sarah West