Curiosity: Update 8 – Methane-less Mars

Shooting Lasers from MSL’s TLS instrument

Mars has lost at least half its atmosphere since the planet’s inception, Curiosity confirms. Mars’ atmosphere is 100 times thinner than Earth’s. Other than shielding life from harmful UV radiation, atmosphere also controls the fluctuations in climate. Because Mars’ atmosphere contains more heavier varieties of carbon dioxide than lighter ones, the ratio suggest the planet has sadly lost much of its atmosphere. Mars’ thin atmosphere has nearly untraceable amounts of methane, only a few parts of methane per billion parts of Martian atmosphere. Microbes like bacteria emit methane. In fact, 95% of methane on Earth is produced by biological processes. Though Curiosity failed to find traces of methane in Gale Crater, Mars may yet host methane elsewhere.

Curiosity used its SAM instruments (Sample Analysis at Mars) and TLS (Tunable Laser Spectrometer). In the near future, SAM will analyze its first solid sample to search for organic compounds in rocks.

In addition, air samples from Curiosity match ones from trapped air bubbles in meteorites found on Earth. Ergo, those meteorites definitely originated from Mars. 1 billion years ago, a large asteroid collided into Mars and split into fragments.


 “NASA Rover Finds Clues to Changes in Mars’ Atmosphere.” JPL Caltech. JPL, 2 Nov 2012. Web. 5 Nov 2012. <;.

Vergano, Dan. “NASA’s Curiosity rover confirms Mars lost atmosphere.” USA Today. USA Today, 2 Nov 2012. Web. 5 Nov 2012. <;.


Curiosity: Update 7 – Fingerprinting Martian Materials

X-Ray View of Martian Soil

The latest of Curiosity’s analyses show that the Martian minerals is similar to “weathered basaltic salts of volcanic origin in Hawaii.”  Curiosity’s CheMin (Chemistry and Mineralogy) instrument refines and identifies minerals in X-ray diffraction analysis on Mars. X-ray diffraction records hows minerals’ internal structures’ crystals react with X-rays. Identifying minerals in rocks and soil is crucial in assessing past environmental conditions. Each mineral has evidence of its unique formation. These minerals have similar chemical compositions but different structures and properties. The samples taken at “Rocknest” were consistent with scientists’ initial ideas of the deposits in Gale Crater. Ancient rocks suggest flowing water, while minerals in younger soil suggest limited interaction with water.


“NASA Rover’s First Soil Studies Help Fingerprint Martian Minerals First X-ray View of Martian Soil” JPL Caltech. JPL, 30 Oct 2012. Web. 5 Nov 2012.