This is the first time scientists have obtained current evidence of rain soaking Titan’s surface at low latitudes.
“Titan continues to surprise and amaze us,” said Alfred McEwen from the University of Arizona’s Lunar and Planetary Lab. “After years of dry weather in the tropics, an area the size of Arizona and New Mexico combined was darkened by methane rain over a period of just a few weeks.”
The new findings, combined with earlier results, show the weather systems of Titan’s thick atmosphere and the changes wrought on the moon’s surface are affected by the changing seasons.
“It’s amazing to be watching such familiar activity as rainstorms and seasonal changes in weather patterns on a distant, icy satellite,” said Elizabeth Turtle from Johns Hopkins University Applied Physics Lab in Laurel, Maryland. “These observations are helping us to understand how Titan works as a system, as well as similar processes on our own planet.”
The Saturn system experienced equinox, when the Sun lies directly over a planet’s equator and seasons change, in August 2009. Years of Cassini observations suggest Titan’s global atmospheric circulation pattern responds to the changes in solar illumination, influenced by its atmosphere and surface.
Cassini found the surface temperature responds more rapidly to sunlight changes than does the thick atmosphere. Its changing circulation pattern produces clouds in Titan’s equatorial region.
Clouds on Titan form from methane as part of an Earth-like cycle that uses methane instead of water. On Titan, methane fills lakes on the surface, saturates clouds in the atmosphere, and falls as rain.
Although there is evidence that liquids have flowed at Titan’s equator in the past, liquid hydrocarbons, such as methane and ethane, had only been observed on the surface in lakes at polar latitudes. The vast expanses of dunes that dominate Titan’s equatorial regions require a predominantly arid climate.
Scientists suspected that clouds might appear at Titan’s equatorial latitudes as spring in the northern hemisphere progressed. But they were not sure if dry channels previously observed formed because of seasonal rains or remained from an earlier, wetter climate.
An arrow-shaped storm appeared in the equatorial region September 27, 2010 — the equivalent of early April on Titan’s — and a broad band of clouds appeared the next month.
During the next few months, Cassini’s imaging science subsystem captured short-lived surface changes in images of Titan’s surface. A 193,000-square-mile (500,000-square-kilometer) region along the southern boundary of Titan’s Belet dune field, as well as smaller areas nearby, had become darker.
Scientists compared the imaging data to that obtained by other instruments and ruled out other possible causes for surface changes. They concluded this change in brightness is most likely the result of surface wetting by methane rain.
These observations suggest that recent weather on Titan is similar to that over Earth’s tropics. In tropical regions, Earth receives its most direct sunlight, creating a band of rising air and rain clouds that encircle the planet.
“These outbreaks may be the Titan equivalent of what creates Earth’s tropical rainforest climates, even though the delayed reaction to the change of seasons and the apparently sudden shift is more reminiscent of Earth’s behavior over the tropical oceans than over tropical land areas,” said Tony Del Genio from NASA’s Goddard Institute for Space Studies in New York.
On Earth, the tropical bands of rain clouds shift slightly with the seasons but are present within the tropics year-round. On Titan, such extensive bands of clouds may only be prevalent in the tropics near the equinoxes and move to much higher latitudes as the planet approaches its solstices.
The imaging team will monitor how Titan’s weather evolves as the seasons progress from spring toward northern summer in its northern hemisphere.
“It is patently clear that there is so much more to learn from Cassini about seasonal forcing of a complex surface-atmosphere system like Titan’s and, in turn, how it is similar to, or differs from, the Earth’s,” said Carolyn Porco, from the Space Science Institute in Boulder, Colorado. “We are eager to see what the rest of Cassini’s Solstice Mission will bring.”
This is the first time scientists have obtained current evidence of rain soaking Titan’s surface at low latitudes.
“Titan continues to surprise and amaze us,” said Alfred McEwen from the University of Arizona’s Lunar and Planetary Lab. “After years of dry weather in the tropics, an area the size of Arizona and New Mexico combined was darkened by methane rain over a period of just a few weeks.”
The new findings, combined with earlier results, show the weather systems of Titan’s thick atmosphere and the changes wrought on the moon’s surface are affected by the changing seasons.
“It’s amazing to be watching such familiar activity as rainstorms and seasonal changes in weather patterns on a distant, icy satellite,” said Elizabeth Turtle from Johns Hopkins University Applied Physics Lab in Laurel, Maryland. “These observations are helping us to understand how Titan works as a system, as well as similar processes on our own planet.”
The Saturn system experienced equinox, when the Sun lies directly over a planet’s equator and seasons change, in August 2009. Years of Cassini observations suggest Titan’s global atmospheric circulation pattern responds to the changes in solar illumination, influenced by its atmosphere and surface.
Cassini found the surface temperature responds more rapidly to sunlight changes than does the thick atmosphere. Its changing circulation pattern produces clouds in Titan’s equatorial region.
Clouds on Titan form from methane as part of an Earth-like cycle that uses methane instead of water. On Titan, methane fills lakes on the surface, saturates clouds in the atmosphere, and falls as rain.
Although there is evidence that liquids have flowed at Titan’s equator in the past, liquid hydrocarbons, such as methane and ethane, had only been observed on the surface in lakes at polar latitudes. The vast expanses of dunes that dominate Titan’s equatorial regions require a predominantly arid climate.
Scientists suspected that clouds might appear at Titan’s equatorial latitudes as spring in the northern hemisphere progressed. But they were not sure if dry channels previously observed formed because of seasonal rains or remained from an earlier, wetter climate.
An arrow-shaped storm appeared in the equatorial region September 27, 2010 — the equivalent of early April on Titan’s — and a broad band of clouds appeared the next month.
During the next few months, Cassini’s imaging science subsystem captured short-lived surface changes in images of Titan’s surface. A 193,000-square-mile (500,000-square-kilometer) region along the southern boundary of Titan’s Belet dune field, as well as smaller areas nearby, had become darker.
Scientists compared the imaging data to that obtained by other instruments and ruled out other possible causes for surface changes. They concluded this change in brightness is most likely the result of surface wetting by methane rain.
These observations suggest that recent weather on Titan is similar to that over Earth’s tropics. In tropical regions, Earth receives its most direct sunlight, creating a band of rising air and rain clouds that encircle the planet.
“These outbreaks may be the Titan equivalent of what creates Earth’s tropical rainforest climates, even though the delayed reaction to the change of seasons and the apparently sudden shift is more reminiscent of Earth’s behavior over the tropical oceans than over tropical land areas,” said Tony Del Genio from NASA’s Goddard Institute for Space Studies in New York.
On Earth, the tropical bands of rain clouds shift slightly with the seasons but are present within the tropics year-round. On Titan, such extensive bands of clouds may only be prevalent in the tropics near the equinoxes and move to much higher latitudes as the planet approaches its solstices.
The imaging team will monitor how Titan’s weather evolves as the seasons progress from spring toward northern summer in its northern hemisphere.
“It is patently clear that there is so much more to learn from Cassini about seasonal forcing of a complex surface-atmosphere system like Titan’s and, in turn, how it is similar to, or differs from, the Earth’s,” said Carolyn Porco, from the Space Science Institute in Boulder, Colorado. “We are eager to see what the rest of Cassini’s Solstice Mission will bring.”
