Curious About Curiosity’s Chemistry Mission?

The Mars Science Laboratory will be seeking clues to the planetary puzzle about life on Mars, the Curiosity rover is one of the best-outfitted chemistry missions ever. Scientists say Curiosity is the next best thing to launching a team of trained chemists to Mars’ surface.

“The Mars Science Laboratory mission has the goal of understanding whether its landing site on Mars was ever a habitable environment, a place that could have supported microbial life,” says MSL Deputy Project Scientist, Ashwin Vasavada, who provides a look “under the hood” in this informative video from the American Chemical Society.

“Curiosity is really a geochemical experiment, and a whole laboratory of chemical equipment is on the rover,” says Vasavada. “It will drill into rocks, and analyze material from those rocks with sophisticated instruments.”

Curiosity will drive around the landing site at Gale Crater and sample the soil, layer by layer, to piece together the history of Mars, trying to determine if and when the planet went from a wetter, warmer world to its current cold and dry conditions.

The payload includes mast-mounted instruments to survey the surroundings and assess potential sampling targets from a distance, and there are also instruments on Curiosity’s robotic arm for close-up inspections. Laboratory instruments inside the rover will analyze samples from rocks, soils and the atmosphere.

The two instruments on the mast are a high-definition imaging system, and a laser-equipped, spectrum-reading camera called ChemCam that can hit a rock with a special laser beam, and using Laser Induced Breakdown Spectroscopy, can observe the light emitted from the laser’s spark and analyze it with the spectrometer to understand the chemical composition of the soil and rock on Mars.

The tools on the turret at the end of Curiosity’s 2.1-meter-long (7-foot-long) robotic arm include a radiation-emitting instrument that reads X-ray clues to targets’ composition and a magnifying-lens camera. The arm can deliver soil and powdered-rock samples to an instrument that uses X-ray analysis to identify minerals in the sample and to an instrument that uses three laboratory methods for assessing carbon compounds and other chemicals important to life and indicative of past and present processes.

The three methods are an evolved gas experiment, which uses a mass spectrometer to look for potential long chain organic molecules on Mars; CheMin, an X-ray diffraction experiment to determine mineralogy; and an Alpha Particle X-Ray Spectrometer (APXS) on Curiosity’s robotic arm, like its predecessors on the arms of all previous Mars rovers, will identify chemical elements in rocks and soils.

In total Curiosity has 10 different instruments on board the roving laboratory, and test results from these instruments will pave the way for future Mars missions, and may provide insight in the search for life on other planets.

Image caption: Artist depiction of the Curiosity rover on Mars. Credit: NASA

Sources: NASA, ACS

Landing Sites for Mars Science Lab Narrowed to Six

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Where should the next spacecraft land on Mars? The Mars Science Laboratory (MSL) rover is scheduled to launch in the fall of 2009. MSL is a long-range rover that will explore a region on Mars with the goal of determining if Mars has or ever had conditions capable of supporting microbial life. Over fifty landing sites have been proposed by various planetary scientists, and recently, the selection committee narrowed the field down to six possible sites. The final site and a backup will be selected in September of 2008. Here’s a look at the six final candidates:

Mawrth Vallis: Location:Northern Plains, east of Pathfinder rover site (24.65°N, 340.10°E)
Mars Global Surveyor MOLA Instrument
This is an ancient channel carved by catastrophic floods. Spectrometers on the Mars Reconnaissance Orbiter (MRO) have detected clay minerals which contain water, and may also preserve organic materials, so there is great interest in studying these deposits to understand past environments that could have supported life. Images from the MRO HiRise camera show hills with several layers and intriguing boulders.

Nili Fossae Trough: Location: Near Isidis Planitia, and near the Beagle 2 intended landing site. (21°N, 74.2°E)
Nilli Fossae Trough.  Image Credit:  Mars Global Surveyor MOLA Instrument
This region has one of the largest and most diverse exposures of clays minerals that have been detected from orbit. Again, clay minerals contain water, and possibly organic materials. The area is a linear depression about 25 km wide that was created from tectonic activity.

Holden Crater: Location: South of Vallis Marineris (26.4°S, 325.3°E)
Holden Crater.  Image Credit:  Mars Global Surveyor MOLA Instrument
This crater contains deep gullies carved by running water as well as examples of what are assumed to be lake beds and sediments deposited by streams. These deposits are more than three billion years old, which dates back to a wetter period on Mars. Scientists believe Holden Crater once was a lake, and when the water disappeared, wind eroded the surface and formed the ripples and dunes that have been imaged by the HiRise instrument.

Eberswalde Crater: Location: South of Vallis Marineris (23.20°S, 326.75°E)
Eberswalde Delta.  Image Credit:  Mars Global Surveyor MOLA Instrument
The Eberswalde delta is the most convincing evidence on Mars for the persistent flow of a river into a standing body of water. HiRise images show many channels within the delta that have become inverted, which occurs as sediments deposited by flowing water solidify over time and become resistant to erosion. High resolution HiRise images show individual boulders breaking off from the channel deposits.

Miyamoto Crater: Location: Merdiani Planum, near Opportunity Rover site. (1.7°S, 352.4°E)
Miyamato Crater.  Image Credit:  Mars Global Surveyor MOLA Instrument
Located along the western boundary of Meridiani Planum, this 150-km crater has hematite and sulfate-bearing minerals, possibly created from lakes or groundwater. The southwestern part of the crater floor has been stripped by erosion, revealing clay minerals.

Northern Meridiani: Location: Meridiani Planum,2.34°N, 6.69°E
Meridiani.  Image Credit:  Mars Global Surveyor MOLA Instrument
This is the same area that the Opportunity rover has studied. By landing here, the MSL rover could increase our knowledge of the Meridiani region, which Opportunity has revealed to have a complex geologic history that involves flowing water, groundwater, lakes and wind. If chosen as a landing site, the MSL rover would study the smooth plains before driving to the ridged plains to the north.

MSL will arrive on Mars in 2010. Once on the surface, the rover will be able to roll over obstacles up to 75 centimeters (29 inches) high and travel up to 90 meters (295 feet) per hour. On average, the rover is expected to travel about 30 meters (98 feet) per hour, based on power levels, slippage, steepness of the terrain, visibility, and other variables. The science instruments on board include cameras, spectrometers, radiation detectors and environmental sensors.

Original News Source: HiRise Blog