Posted: Tuesday, September 21, 2010
The Herschel Space Observatory is providing its first results on Mars. An accurate globally-averaged temperature profile of the Martian atmosphere may cause scientists to revise their models about atmospheric circulation on Mars. The first sub-millimeter observation of molecular oxygen on the planet may lead to a completely new picture of the oxygen distribution in the Martian atmosphere. These are only a few of the new discoveries presented by Dr. Paul Hartogh at the European Planetary Science Congress in Rome, on Monday 20th September.
The Herschel Space Observatory (HSO) is a space-borne far-infrared observation facility of the European Space Agency, launched on 14 May 2009. The 'Water and related chemistry in the Solar System' project, was conceived with the sole aim to determine the origin, evolution, and distribution of water in Mars, the outer planets, Titan, Enceladus and the comets.
"Water vapor plays a key role in the Martian atmospheric chemistry and physics," says Dr. Hartogh of the Max Planck Institute for Solar System Research in Germany. Herschel has observed Mars with its three instruments, the Heterodyne Instrument for the Far Infrared (HIFI), the Photodetector Array Camera & Spectrometer, and the Spectral and Photometric Imaging Receiver (SPIRE).
SPIRE has provided the first continuous spectrum of the Martian atmosphere in the spectral range in the far-IR/sub-mm, as well as, the first complete set of water vapor and carbon monoxide (CO) content in this range.
"SPIRE was designed for very faint sources, however unexpectedly it could even provide high quality data from the brightest far infrared object Herschel observed in the solar system," says Dr. Hartogh.
HIFI observed Mars between 11-16 April 2010. Only a small part of the data has been analyzed up to now, but it already provided some interesting results: A globally averaged temperature profile has been retrieved from the first simultaneous observations of two carbon monoxide isotopes.
"The best fit of the Martian atmospheric model to these observations shows important differences compared to what we were predicting: between 40 and 80 km from the ground, the atmosphere appears to be more than 10 degrees Celsius colder than predicted," says Dr. Hartogh.
Scientists also report on the first sub-mm detection of molecular oxygen (O2) on Mars, with an observational accuracy at least 10 times better than was done before.
"Our sub-mm observations provide for the first time a vertical profile of molecular oxygen in the Martian atmosphere. We found that, contrary to the general assumption of a constant O2 content independently of altitude, the Martian atmosphere is richer in oxygen near the ground and then O2 decreases rapidly with altitude," says Dr. Hartogh. If this profile is confirmed it may imply different oxygen production and loss processes not considered before, leading to new insights about the Martian atmosphere.
"Obviously, much work still needs to be done on the vertical profile of O2 before we draw such conclusions," he adds cautiously.
Herschel will continue exploring our solar system in the next 2-3 years of its planned mission duration.
"We hope that surprises and major breakthroughs in our knowledge will keep coming in, and that at the end we will have gained a unified picture of the origin and evolution of water in the Solar System objects," says Dr. Hartogh.
Artist's impression of Herschel. Credit: ESA http://www.esa.int/esa-mmg/mmg.pl?b=b&type=I&mission=Herschel&single=y&start=7
The spectra can be found on the Europlanet outreach website: http://www.europlanet-eu.org/outreach/index.php?option=com_content&task=view&id=303&Itemid=41
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EUROPEAN PLANETARY SCIENCE CONGRESS (EPSC) 2010 EPSC 2010 is organized by Europlanet, a Research Infrastructure funded under the European Commission's Framework 7 Programme, in association with the European Geosciences Union, with the support of the Italian National Institute for Astrophysics (INAF) and the INAF Institute of Physics of Interplanetary Science (IFSI) in Rome. EPSC is the major meeting in Europe for planetary scientists. The 2010 program comprises 48 sessions and workshops covering a wide range of planetary topics. EPSC 2010 is taking place at the Angelicum Center - Pontifical University of St. Thomas Aquinas, Rome, Italy from Sunday 19 September to Friday 24 September 2010. For further details, see the meeting website: http://meetings.copernicus.org/epsc2010/
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