Planetary Fourier Spectrometer
The Planetary Fourier Spectrometer (PFS) is an
The main objective of the instrument is to provide temperature profiles of Mars's carbon dioxide atmosphere, and to the study composition of the planet's atmosphere through the infrared radiation that is reflected and emitted by the planet.
Methane in the Martian atmosphere
In March 2004, Professor Vittorio Formisano, the researcher in charge of the Mars Express Planetary Fourier Spectrometer, announced the discovery of methane in the Martian atmosphere. However, methane cannot persist in the Martian atmosphere for more than a few hundred years since it can be broken down by sunlight. Thus, this discovery suggests that the methane is being continually replenished by some unidentified volcanic or geologic process, or that some kind of extremophile life form similar to some existing on Earth is metabolising carbon dioxide and hydrogen and producing methane.[2] In July 2004, rumours began to circulate that Formisano would announce the discovery of ammonia at an upcoming conference. It later came to light that none had been found; in fact some noted that the PFS was not precise enough to distinguish ammonia from carbon dioxide anyway.[3]
See also
- Atmosphere of Mars
- ExoMars Trace Gas Orbiter
References
- ^ "PFS: Planetary Fourier Spectrometer". ESA. Retrieved August 31, 2006.
- ^ "Martian gases poses life question". BBC News. February 25, 2005. Retrieved August 31, 2006.
- S2CID 129317380. Retrieved March 19, 2006.