Unfortunately those of us who are participating in the web only class cannot easily participate in the “build a robot” assignment. So Dr. Brown arranged for us to have another assignment-basically research on robots, robotic innovators or something similiar.
I chose to report on Mars Rovers that NASA launched on June 10 and July 7, 2003, in search of answers about the history of water on Mars. They landed on Mars January 3 and January 24 PST, 2004. I pulled a lot of this commentary and information from NASA’s webpage Mars Rover.
This is a tremendously exciting robot as it allows us to see Mars! I think that most youngsters dream of exploring space at some point in adolescence but for most of us this is about as close as we will get.
There are some pictures of the actual robots that have traveled to Mars on this blog page. They look relatively simple and far from the clunky robots portrayed during my youth.

After the airbag-protected landing craft settled onto the surface (Mars) and opened, the rovers rolled out to take panoramic images. These images give scientists the information they need to select promising geological targets that tell part of the story of water in Mars’ past. Then, the rovers drive to those locations to perform on-site scientific investigations.
These are the primary science instruments carried by the rovers:
- Panoramic Camera (Pancam): for determining the mineralogy, texture, and structure of the local terrain.
- Miniature Thermal Emission Spectrometer (Mini-TES): for identifying promising rocks and soils for closer examination and for determining the processes that formed Martian rocks. The instrument is designed to look skyward to provide temperature profiles of the Martian atmosphere.
- Mössbauer Spectrometer (MB): for close-up investigations of the mineralogy of iron-bearing rocks and soils.
- Alpha Particle X-Ray Spectrometer (APXS): for close-up analysis of the abundances of elements that make up rocks and soils.
- Magnets: for collecting magnetic dust particles. The Mössbauer Spectrometer and the Alpha Particle X-ray Spectrometer are designed to analyze the particles collected and help determine the ratio of magnetic particles to non-magnetic particles. They can also analyze the composition of magnetic minerals in airborne dust and rocks that have been ground by the Rock Abrasion Tool.
- Microscopic Imager (MI): for obtaining close-up, high-resolution images of rocks and soils.
- Rock Abrasion Tool (RAT): for removing dusty and weathered rock surfaces and exposing fresh material for examination by instruments onboard.
Before landing, the goal for each rover was to drive up to 40 meters (about 44 yards) in a single day, for a total of up to one 1 kilometer (about three-quarters of a mile). Both goals have been far exceeded! Where are the rovers now?
Moving from place to place, the rovers perform on-site geological investigations. Each rover is sort of the mechanical equivalent of a geologist walking the surface of Mars. The mast-mounted cameras are mounted 1.5 meters(5 feet) high and provide 360-degree, stereoscopic, humanlike views of the terrain. The robotic arm is capable of movement in much the same way as a human arm with an elbow and wrist, and can place instruments directly up against rock and soil targets of interest. In the mechanical “fist” of the arm is a microscopic camera that serves the same purpose as a geologist’s handheld magnifying lens. The Rock Abrasion Tool serves the purpose of a geologist’s rock hammer to expose the insides of rocks.
Wikepedia says that on January 3 and January 24, 2010, Spirit and Opportunity marked six years on Mars, respectively.[24] On January 26, NASA announced that Spirit will be used as a stationary research platform after several months of unsuccessful attempts to free the rover from soft sand.[25]
NASA announced on March 24, 2010, that Opportunity, which has an estimated remaining drive distance of 12 km to Endeavour Crater, has traveled over 20 km since the start of its mission.[26] Each rover was designed with a mission driving distance goal of just 600 meters.[26] One week later, they announced that Spirit may have gone into hibernation for the Martian winter and might not wake up again for months.[27]
On September 8, 2010, it was announced that Opportunity had reached the halfway point of the 19-kilometer journey between Victoria crater and Endeavour crater.[28]
On May 24, 2011, NASA announced that it will cease attempts to contact Spirit, which has been stuck in a sand trap for two years. The last successful communication with the rover was on March 22, 2010. The final transmission to the rover was on May 25, 2011. [29]
Wikepedia has this to say about the operating system of the rovers. The rovers run a VxWorks embedded operating system on a radiation-hardened 20 MHz RAD6000 CPU with 128 MB of DRAM with error detection and correction and 3 MB of EEPROM. Each rover also has 256 MB of flash memory. To survive during the various mission phases, the rover’s vital instruments must stay within a temperature of −40 °C to +40 °C (−40 °F to 104 °F). At night, the rovers are heated by eight radioisotope heater units (RHU), which each continuously generate 1 W of thermal energy from the decay of radioisotopes, along with electrical heaters that operate only when necessary. A sputtered gold film and a layer of silica aerogel are used for insulation.
Additionally SAP software makes everything work on the Rovers. Wikepedia has this to say: The NASA team uses a software application called SAP to view images collected from the rover, and to plan its daily activities. There is a version available to the public called Maestro.
The Rovers show how far technology has come in my lifetime. When I was a child, a calculator that added/subtracted/multiplied and divided cost a lot and was about nine inches long. Now my phone does more than that calculator and it is smaller and costs less.
CNN now reports that the biggest Rover ever is ready to launch.
NASA’s biggest and most advanced Mars rover is scheduled for launch Saturday from Cape Canaveral, Florida. Curiosity is packed with 10 science experiments to determine whether Mars has ever been suitable for life and to find clues about past life forms that may have been preserved in rocks. Curiosity is twice as long and five times as heavy as the older Mars rovers, Spirit and Opportunity. Its science instruments weigh 15 times as much as its predecessors’ science payloads.
The rover has a mast that can extend to 7 feet (2.1 meters) to hoist a high-definition imaging system. It also will hold a laser-equipped camera that can zap rocks to study the sparks emitted for information about their composition.
A 7-foot-long robot arm will hold instruments for soil analysis. Unlike earlier rovers, Curiosity can gather rocks and soil to process inside its lab. The rover also has tools to look for water beneath the surface, to monitor the weather and to measure natural radiation.
Curiosity is designed to roll over obstacles up to 25 inches (about 65 centimeters) high and to travel about 660 feet (200 meters) per day. Its energy source will be a radioisotope power generator.
When Curiosity arrives at Mars, three satellites already in orbit will be listening: NASA’s Mars Odyssey and Mars Reconnaissance Orbiter and the European Space Agency’s Mars Express. The spacecraft will be positioned to receive transmissions about Curiosity’s status and relay information to Earth.