Typically on Earth, days usually have a temperature maximum somewhere after lunch, and a minimum during the night. But for Mars, things are pretty different:
“We see a temperature maximum in the middle of the day, but we also see a temperature maximum a little after midnight,” said Armin Kleinboehl of NASA’s Jet Propulsion Laboratory in Pasadena, Calif., who is the lead author of a new report on these findings.
Temperatures swing as much as 32 degrees Celsius (58 Fahrenheit) in this odd, bipolar type of climate – as detected by the orbiter’s Mars Climate Sounder instrument.
Global changes in wind, temperature and pressure repeating each day or fraction of a day are called atmospheric tides. Unlike oceanic tides, which are caused by gravity, atmospheric tides are caused by variation in heating between day and night. Earth has atmospheric tides as well, but they produce very little difference in the lower atmosphere. When there’s one cycle repeating throughout the day, it’s called diurnal; when it happens twice a day, it’s called semi-diurnal.
“We were surprised to find this strong twice-a-day structure in the temperatures of the non-dusty Mars atmosphere,” Kleinboehl said. “While the diurnal tide as a dominant temperature response to the day-night cycle of solar heating on Mars has been known for decades, the discovery of a persistent semi-diurnal response even outside of major dust storms was quite unexpected, and caused us to wonder what drove this response.”
But why does this happen? Kleinboehl and his team have found the answer in the water-ice clouds of Mars. The Martian atmosphere has water-ice clouds for most of the year. During daytime, equatorial clouds at 10-30 km from the ground absorb infrared light emitted from the surface during daytime. These clouds are very thin, and relatively transparent – this absorbtion is enough to heat the middle atmosphere each day. The observed semi-diurnal temperature pattern, with its maximum temperature swings occurring away from the tropics, was also unexpected, but has been replicated in Mars climate models when the radiative effects of water-ice clouds are included.
“We think of Mars as a cold and dry world with little water, but there is actually more water vapor in the Martian atmosphere than in the upper layers of Earth’s atmosphere,” Kleinboehl said. “Water-ice clouds have been known to form in regions of cold temperatures, but the feedback of these clouds on the Mars temperature structure had not been appreciated. We know now that we will have to consider the cloud structure if we want to understand the Martian atmosphere. This is comparable to scientific studies concerning Earth’s atmosphere, where we have to better understand clouds to estimate their influence on climate.”
Dr. Andrei Mihai is a geophysicist and founder of ZME Science. He has a Ph.D. in geophysics and archaeology and has completed courses from prestigious universities (with programs ranging from climate and astronomy to chemistry and geology). He is passionate about making research more accessible to everyone and communicating news and features to a broad audience.
