This animated illustration shows one possible scenario for the rocky 55 e, nearly two times the size of Earth. New Spitzer data show that one side of the planet is much hotter than the other – which could be explained by a possible presence of lava pools.
- Rover examines geological contact zone near ‘Marias Pass’
- Silica-rich rocks identified nearby with laser-firing instrument
- Test of rover’s drill prepares for next use on Mars rock
Approaching the third anniversary of its landing on Mars, NASA’s Curiosity Mars rover has found a target unlike anything it has studied before — bedrock with surprisingly high levels of silica. Silica is a rock-forming compound containing silicon and oxygen, commonly found on Earth as quartz.
This area lies just downhill from a geological contact zone the rover has been studying near “Marias Pass” on lower Mount Sharp.
In fact, the Curiosity team decided to back up the rover 46 meters (151 feet) from the geological contact zone to investigate the high-silica target dubbed “Elk.” The decision was made after they analyzed data from two instruments, the laser-firing Chemistry & Camera (ChemCam) and Dynamic Albedo of Neutrons (DAN), which showed higher amounts of silicon and hydrogen, respectively. High levels of silica in the rock could indicate ideal conditions for preserving ancient organic material, if present, so the science team wants to take a closer look.
“One never knows what to expect on Mars, but the Elk target was interesting enough to go back and investigate,” said Roger Wiens, the principal investigator of the ChemCam instrument from the Los Alamos National Laboratory in New Mexico. ChemCam is coming up on its 1,000th target, having already fired its laser more than 260,000 times since Curiosity landed on Mars Aug. 6, 2012, Universal Time (evening of Aug. 5, Pacific Time).
In other news, an engineering test on the rover’s sample-collecting drill on July 18 is aiding analysis of intermittent short circuits in the drill’s percussion mechanism, in preparation for using the drill in the area where the rover has been working for the past two months. The latest test did not result in any short circuits, so the team plans to continue with more tests, performed on the science targets themselves.
Before Curiosity began further investigating the high-silica area, it was busy scrutinizing the geological contact zone near Marias Pass, where a pale mudstone meets darker sandstone.
“We found an outcrop named Missoula where the two rock types came together, but it was quite small and close to the ground. We used the robotic arm to capture a dog’s-eye view with the MAHLI camera, getting our nose right in there,” said Ashwin Vasavada, the mission’s project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California. MAHLI is short for Mars Hand Lens Imager.
The rover had reached this area after a steep climbed a 20-foot (6-meter) hill. Near the top of the climb, the ChemCam instrument fired its laser at the target Elk, and took a spectral reading of its composition.
“ChemCam acts like eyes and ears of the rover for nearby objects,” said Wiens.
The rover had moved on before analyzing the Elk data, so the rover performed a U-turn to get more data. Upon its return, the rover was able to study a similar target, “Lamoose,” up close with the MAHLI camera and the arm-mounted Alpha Particle X-ray Spectrometer (APXS).
Curiosity has been working on Mars since early August 2012. It reached the base of Mount Sharp last year after fruitfully investigating outcrops closer to its landing site and then trekking to the mountain. The main mission now is to look at successively higher layers of Mount Sharp.
The U.S. Department of Energy’s Los Alamos National Laboratory developed ChemCam in partnership with scientists and engineers funded by the French national space agency. Russia’s space agency provided Curiosity’s DAN instrument. JPL, a division of the California Institute of Technology in Pasadena, built the rover and manages the project for NASA’s Science Mission Directorate in Washington.