NASA’s Dragonfly mission to Saturn’s largest moon will contact down on a terrain of dunes and shattered, icy bedrock, based on a brand new evaluation of radar imagery from the Cassini spacecraft.
Launching in 2027, Dragonfly is a rotorcraft that may arrive in 2034 and discover Titan from the air. Its vary shall be far higher than that of a wheeled rover, with Dragonfly able to overlaying round 10 miles (16 kilometers) in every half-hour flight, according to NASA. Over the span of its two-year mission it would discover an space a whole bunch of miles or kilometers throughout. Nonetheless, earlier than taking to the sky by itself, Dragonfly should first arrive on Titan beneath a parachute, soft-landing on frozen terrain that’s hidden from simple viewing by the dense hydrocarbon smog that fills the moon’s environment.
Dragonfly’s touchdown website would be the Shangri-La dune subject, near the 50-mile-wide (80 kilometers) crater, Selk. This area was imaged by NASA’s Cassini spacecraft throughout its mission to Saturn between 2004 and 2017, and a staff of scientists led by planetary scientist Léa Bonnefoy of Cornell College has taken a brand new have a look at that knowledge to supply essentially the most correct evaluation of Dragonfly’s proposed touchdown website up to now.
“Dragonfly … goes to a scientifically outstanding space,” Bonnefoy mentioned in a statement (opens in new tab). “Dragonfly will land in an equatorial, dry area of Titan. It rains liquid methane generally, however it’s extra like a desert on Earth the place you might have dunes, some little mountains and an affect crater.”
Associated: Soar over the desert in footage from drone practicing for mission to Saturn’s strangest moon
Selk is an fascinating location. Estimated to be geologically younger, maybe a pair hundred million years previous, the affect that carved it out would have melted the native ice, prompting interactions between the recent liquid water and natural molecules current within the hydrocarbon soup on Titan’s floor. Astrobiologists are significantly within the prebiotic chemistry — chemistry involving carbon-rich molecules however not mediated by dwelling issues — that might have resulted.
But Cassini’s radar photographs of the world are restricted, with the decision at finest being 1,000 toes (300 meters) per pixel. “There are in all probability numerous small rivers and landscapes that we could not see,” Bonnefoy mentioned.Â
Scientists know that such rivers do exist on Titan, due to the European Area Company’s Huygens lander, which piggybacked on board Cassini earlier than parachuting right down to the floor of Titan in January 2005. These rivers, nevertheless, will not be filled with liquid water — the temperature of minus 290 levels Fahrenheit (minus 179 levels Celsius) is way too chilly for that. As a substitute, liquid methane and ethane rain from the frigid sky and wash off the water-ice bedrock and into river tributaries that feed massive lakes.
What Cassini’s imagery did present, nevertheless, is a number of viewing angles. Every time it flew previous Titan — it loved 127 shut approaches of the moon throughout its mission — it considered landmarks within the area of Dragonfly’s touchdown website from completely different angles, starting from inclinations of 5 levels to 72 levels.Â
By analyzing how the terrain produced different-shaped shadows based mostly on the viewing angle, Bonnefoy’s staff have been in a position to decide the topography of the area inside the limits of the picture decision, discovering no main show-stopping obstacles that Dragonfly would want to keep away from.Â
The scientists additionally calculated the peak of the rim of Selk crater, discovering it to range from lower than 650 toes (200 m) tall in some components as much as 2,000 toes (600 m), which is greater than anticipated, indicating a much less eroded crater rim.
The analysis was revealed Aug. 30 in The Planetary Science Journal (opens in new tab).
Observe Keith Cooper on Twitter @21stCenturySETI. Observe us on Twitter @Spacedotcom and on Facebook.Â