A pair of new papers report measurements of the Martian atmosphere's composition
by NASA's Curiosity rover, providing evidence about loss of much of Mars'
original atmosphere.
Curiosity's Sample Analysis at Mars (SAM) suite of laboratory instruments
inside the rover has measured the abundances of different gases and different
isotopes in several samples of Martian atmosphere. Isotopes are variants of the
same chemical element with different atomic weights due to having different
numbers of neutrons, such as the most common carbon isotope, carbon-12, and a
heavier stable isotope, carbon-13.
SAM checked ratios of heavier to lighter isotopes of carbon and oxygen in the
carbon dioxide that makes up most of the planet's atmosphere. Heavy isotopes of
carbon and oxygen are both enriched in today's thin Martian atmosphere compared
with the proportions in the raw material that formed Mars, as deduced from
proportions in the sun and other parts of the solar system. This provides not
only supportive evidence for the loss of much of the planet's original
atmosphere, but also a clue to how the loss occurred.
"As atmosphere was lost, the signature of the process was embedded in the
isotopic ratio," said Paul Mahaffy of NASA Goddard Space Flight Center,
Greenbelt, Md. He is the principal investigator for SAM and lead author of one
of the two papers about Curiosity results in the July 19 issue of the journal
Science.
Curiosity measured the same pattern in isotopes of hydrogen, as well as
carbon and oxygen, consistent with a loss of a substantial fraction of Mars'
original atmosphere. Enrichment in heavier isotopes in the Martian atmosphere
has previously been measured on Mars and in gas bubbles inside meteorites from
Mars. Meteorite measurements indicate much of the atmospheric loss may have
occurred during the first billion years of the planet's 4.6-billion-year
history. The Curiosity measurements reported this week provide more precise
measurements to compare with meteorite studies and with models of atmospheric
loss.
The Curiosity measurements do not directly measure the current rate of
atmospheric escape, but NASA's next mission to Mars, the Mars Atmosphere and
Volatile Evolution Mission (MAVEN), will do so. "The current pace of the loss is
exactly what the MAVEN mission now scheduled to launch in November of this year
is designed to determine," Mahaffy said.
The new reports describe analysis of Martian atmosphere samples with two
different SAM instruments during the initial 16 weeks of the rover's mission on
Mars, which is now in its 50th week. SAM's mass spectrometer and tunable laser
spectrometer independently measured virtually identical ratios of carbon-13 to
carbon-12. SAM also includes a gas chromatograph and uses all three instruments
to analyze rocks and soil, as well as atmosphere.
"Getting the same result with two very different techniques increased our
confidence that there's no unknown systematic error underlying the
measurements," said Chris Webster of NASA's Jet Propulsion Laboratory, Pasadena,
Calif. He is the lead scientist for the tunable laser spectrometer and the lead
author for one of the two papers. "The accuracy in these new measurements
improves the basis for understanding the atmosphere's history."
Curiosity landed inside Mars' Gale Crater on Aug. 6, 2012 Universal Time (on
Aug. 5 PDT). The rover this month began a drive of many months from an area
where it found evidence for a past environment favorable for microbial life,
toward a layered mound, Mount Sharp, where researchers will seek evidence about
how the environment changed.
No comments:
Post a Comment
Note: Only a member of this blog may post a comment.