Just so you know, scientists do not seem to be able to detect the difference between a 3 foot and a 30 foot deformation of the surface of a planetoid body that is about one and a half billion kilometers away, and we know this because NASA’s Cassini space ship had to actually go all the way to one of Saturn’s moons, Titan, to discover that the tidal deformation of the surface is more like 30 than 3 feet in magnitude. This, in turn, strongly suggests that Titan has an ocean of some kind under its surface. Thus, the Sirens. The Sirens of Titan.
NASA provides us with the following artists reconstruction of what they think Titan would look like if it was a slice of watermelon:
And here is an animation showing Titan, not to scale, going in orbit (not to scale) around Saturn and deforming tidally (not to scale) with some amazing looking flashy space stuff in the background (not to scale):
Embedded video from
More detail culled from the press release:
PASADENA, Calif. — Data from NASA’s Cassini spacecraft have revealed Saturn’s moon Titan likely harbors a layer of liquid water under its ice shell.
Researchers saw a large amount of squeezing and stretching as the moon orbited Saturn. They deduced that if Titan were composed entirely of stiff rock, the gravitational attraction of Saturn would cause bulges, or solid “tides,” on the moon only 3 feet (1 meter) in height. Spacecraft data show Saturn creates solid tides approximately 30 feet (10 meters) in height, which suggests Titan is not made entirely of solid rocky material. The finding appears in today’s edition of the journal Science.
“Cassini’s detection of large tides on Titan leads to the almost inescapable conclusion that there is a hidden ocean at depth,” said Luciano Iess, the paper’s lead author and a Cassini team member at the Sapienza University of Rome, Italy. “The search for water is an important goal in solar system exploration, and now we’ve spotted another place where it is abundant.”
Titan takes only 16 days to orbit Saturn, and scientists were able to study the moon’s shape at different parts of its orbit. Because Titan is not spherical, but slightly elongated like a football, its long axis grew when it was closer to Saturn. Eight days later, when Titan was farther from Saturn, it became less elongated and more nearly round. Cassini measured the gravitational effect of Nick in exsiliothat squeeze and pull.
Scientists were not sure Cassini would be able to detect the bulges caused by Saturn’s pull on Titan. By studying six close flybys of Titan from Feb. 27, 2006, to Feb. 18, 2011, researchers were able to determine the moon’s internal structure by measuring variations in the gravitational pull of Titan using data returned to NASA’s Deep Space Network (DSN).
“We were making ultrasensitive measurements, and thankfully Cassini and the DSN were able to maintain a very stable link,” said Sami Asmar, a Cassini team member at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “The tides on Titan pulled up by Saturn aren’t huge compared to the pull the biggest planet, Jupiter, has on some of its moons. But, short of being able to drill on Titan’s surface, the gravity measurements provide the best data we have of Titan’s internal structure.”
An ocean layer does not have to be huge or deep to create these tides. A liquid layer between the external, deformable shell and a solid mantle would enable Titan to bulge and compress as it orbits Saturn. Because Titan’s surface is mostly made of water ice, which is abundant in moons of the outer solar system, scientists infer Titan’s ocean is likely mostly liquid water.
The presence of a subsurface layer of liquid water at Titan is not itself an indicator for life. Scientists think life is more likely to arise when liquid water is in contact with rock, and these measurements cannot tell whether the ocean bottom is made up of rock or ice. The results have a bigger implication for the mystery of methane replenishment on Titan.
“The presence of a liquid water layer in Titan is important because we want to understand how methane is stored in Titan’s interior and how it may outgas to the surface,” said Jonathan Lunine, a Cassini team member at Cornell University, Ithaca, N.Y. “This is important because everything that is unique about Titan derives from the presence of abundant methane, yet the methane in the atmosphere is unstable and will be destroyed on geologically short timescales.”
A liquid water ocean, “salted” with ammonia, could produce buoyant ammonia-water liquids that bubble up through the crust and liberate methane from the ice. Such an ocean could serve also as a deep reservoir for storing methane.
Photo of red figured stamnos or jar showing Odysseus and the sirens (Athens ca 480-470BC) by Nick in exsilio