New findings from NASA’s Curiosity rover provide clues to how Mars lost its original atmosphere, which scientists believe was much thicker than the one left today.

“The beauty of these measurements lies in the fact that these are the first really high-precision measurements of the composition of Mars’ atmosphere,” said Sushil Atreya, prof. of atmospheric, oceanic and space sciences at the Univ. of Michigan.

Atreya is co-author of two related papers published in Science, and co-investigator on Curiosity’s Sample Analysis at Mars (SAM) suite of instruments, considered the rover’s cornerstone laboratory.

SAM measured the abundances of different gases and isotopes in samples of Martian air, according to NASA. Isotopes are variations of the same chemical element that contain different numbers of neutrons, such as the most common carbon isotope, carbon-12, and a heavier stable isotope, carbon-13, which contains an additional neutron.

SAM analyzed the ratios of heavier to lighter isotopes of carbon and oxygen in the carbon dioxide that makes up most of Mars’ atmosphere today. Measurements showed that heavy isotopes of carbon and oxygen were more abundant in today’s thin atmosphere compared with the proportions in the raw material that formed the planet (which scientists can deduce from proportions in the sun and other parts of the solar system). This provides not only supportive evidence for the loss of much of Mars’ original atmosphere, but also gives clues to how the loss occurred. It suggests that the planet’s atmosphere escaped from the top, rather than due to the lower atmosphere interacting with the ground, NASA’s Web story states.

“The isotope data are unambiguous and robust, having been independently confirmed by the quadrupole mass spectrometer and the tunable laser spectrometer, two of the SAM suite instruments,” Atreya said. “These data are clear evidence of a substantially more massive atmosphere, hence a warmer, wetter Mars in the past than the cold, arid planet we find today.”

Curiosity landed inside Mars’ Gale Crater on Aug. 6, 2012, Universal Time.

Isotope Ratios of H, C, and O in CO2 and H2O of the Martian Atmosphere

Abundance and Isotopic Composition of Gases in the Martian Atmosphere from the Curiosity Rover

Source: Univ. of Michigan