NASA’s Curiosity rover has been getting a good feel for the weather on Mars.
From the data gathered by Curiosity’s meteorological station, scientists think dust-devils may even have run over the robot.
It is not entirely unexpected. Vortices of dust whipped up by the wind have been pictured by previous Mars rovers.
“A dust-devil looks essentially like what you would expect from the movies - a tiny tornado that is lifting dust,” explained Manuel de la Torre Juarez of Nasa’s Jet Propulsion Laboratory (JPL) and a scientist on the Rover Environmental Monitoring Station (Rems) instrument.
“Understanding these phenomena is very important because the Martian climate is driven largely by its dust cycle.” This is most evident when the planet is gripped by dust storms that can envelop the whole globe. Dust in the atmosphere warms it.
The Rems instrument was the sole part of the rover that suffered damage when it touched down in the equatorial Gale Crater back in August.
One of its two wind probes was knocked out, most probably by a piece of grit kicked up by the rocket-powered descent stage that placed Curiosity on the surface. Nonetheless, Rems is returning very useful meteorological data, and scientists are learning to work around its deficiencies.
The instrument has established that winds generally blow east-west on the floor of the crater - something of a surprise to researchers who thought the rover’s position close to the northern slopes of Gale’s big central mountain might drive winds in a prevailing north-west direction as air moved up and down the peak in a day-night cycle. Rems has also been tracking the hourly and daily changes in air pressure.
Barometric readings have a predictable behaviour to them that sees a sharp fall when the Sun comes over the crater every Martian sol (day) to heat the column of air, expanding it upwards and off to the sides. This has the effect of lowering air pressure at the surface.
But Curiosity has also experienced a general increase in air pressure over time. This is consistent with the southern hemisphere moving from spring to summer. The shift to higher temperatures prompts Mars’ southern ice cap, which is made up entirely of frozen carbon dioxide, to start to evaporate and increase the mass of the atmosphere. In contrast, the northern hemisphere’s ice cap will grow as CO2 comes out of the cooling air and builds up on the ground.
“Each year, the Martian atmosphere basically shrinks and grows by about 30% because a portion of the atmosphere is freezing out to the poles in [autumn] and then vaporising again in spring; and that of course is unlike anything we see on Earth,” said Claire Newman, a Rems investigator at Ashima Research in California.
An interesting observation related to the rhythmical changes in air pressure has been made by another of Curiosity’s environmental sensors - its Radiation Assessment Detector (RAD). This instrument was put on the rover to chart the likely radiation conditions future astronauts at Mars might experience. –BBC