Science of global climate modeling confirmed by discoveries on MarsOctober 16, 2012 in Astronomy & Space / Space Exploration
(Phys.org)—Scientific modeling methods that predicted climate change on Earth have been found to be accurate on Mars as well, according to a paper presented at an international planetary sciences conference Tuesday.
An international team of researchers from the Planetary Science Institute in Tucson, working with French colleagues, found that an unusual concentration of glacial features on Mars matches predictions made by global climate computerized models, in terms of both age and location.
PSI Senior Scientist William K. Hartmann led the team, which included François Forget (Université Paris), who did the Martian climate modeling, and Veronique Ansan and Nicolas Mangold (Université de Nantes) and Daniel Berman (PSI), all of who analyzed spacecraft measurements regarding the glaciers.
"Some public figures imply that modeling of global climate change on Earth is 'junk science,' but if climate models can explain features observed on other planets, then the models must have at least some validity," said team leader Hartmann.
Hartmann presented the report, "Science of Global Climate Modeling: Confirmation from Discoveries On Mars," at the annual meeting of the Division of Planetary Sciences of the American Astronomical Society in Reno, Nev.
The scientific team reached their conclusions by combining four different aspects of Martian geological mapping and Martian climate science in recent years. They noted that the climate models, the presence of glaciers, the ages of the glacial surface layers, and radar confirmation of ice in same general area, all gave consistent results – that the glaciers formed in a specific region of Mars, due to unusual climate circumstances, just as indicated by the climate model.
The work has a long background. As early 1993, astronomers analyzed the changing tilt of Mars's rotational axis and found that during high-tilt Martian episodes, the axis tilt can exceed 45 degrees. Under this extreme condition, the summer hemisphere is strongly tilted toward the sun, and Mars's polar ice cap in that hemisphere evaporates, increasing water vapor in the Martian air, thus increasing the chances for snowfall in the dark, cold, winter hemisphere. The last such episodes happened on Mars 5 million to 20 million years ago.
By 2001-2006, various French and American researchers applied the global climate computer models to study this effect. The computer programs were originally developed for planet Earth to estimate climate effects, from hurricane paths to CO2 greenhouse warming. Planetary scientists simply applied the Martian topography, atmosphere, and gravity, in order to run the computer calculations for Mars. The calculations indicated a strong concentration of winter snow and ice in a mid-latitude southern region of Mars, just east of a huge Martian impact basin named Hellas.
At the same time, the PSI scientists independently discovered an unusual concentration of glacial features in a 40-mile-wide crater named "Greg" centered in the same region. Their analysis showed that the surface layers of the glaciers formed at the same time as the predicted climate extremes, about 5 million to 20 million years ago.
"The bottom line is that the global climate models indicate that the last few intense deposits of ice occurred about 5 million to 15 million years ago, virtually centered on Greg crater, and that's just where the spacecraft data reveal glaciers whose surface layers date from that time," Hartmann said. "If global climate models indicate specific concentration of ice-rich features where and when we actually see them on a distant planet, then climate modeling should not be sarcastically dismissed. Our results provide an important, teachable refutation of the attacks on climate science on our home planet."
Provided by Planetary Science Institute
"Science of global climate modeling confirmed by discoveries on Mars" October 16, 2012 https://phys.org/news/2012-10-science-global-climate-discoveries-mars.html