PASADENA, California, April 9, 2014 (ENS) – A large underground ocean has been discovered on Saturn’s moon Enceladus, arousing scientific interest in the small, icy moon as a possible extraterrestrial environment that supports living microbes.
The evidence comes from signals sent back to Earth by NASA’s Cassini spacecraft and received by NASA’s Deep Space Network, an international array of giant radio antennas that supports interplanetary spacecraft missions. The Deep Space Network is operated by NASA’s Jet Propulsion Laboratory, which also operates many of the agency’s interplanetary robotic space missions.
New data on the moon’s gravity field reported in the April 4, 2014, edition of the journal “Science” strengthen the case for an ocean hidden inside Enceladus.
The gravity measurements suggest a large, possibly regional, ocean about six miles (10 kilometers) deep, beneath an ice shell about 19 to 25 miles (30 to 40 kilometers) thick.
The subsurface ocean evidence supports the inclusion of Enceladus among the most likely places in our solar system to host microbial life, although the moon is barely 300 miles (500 kilometers) in diameter.
“The Cassini gravity measurements show a negative gravity anomaly at the south pole that however is not as large as expected from the deep depression detected by the onboard camera,” says the paper’s lead author, Luciano Iess of Sapienza University of Rome.
“Hence the conclusion that there must be a denser material at depth that compensates the missing mass – very likely liquid water, which is seven percent denser than ice. The magnitude of the anomaly gave us the size of the water reservoir,” said Iess.
Cassini has flown near Enceladus 19 times. Three flybys, from 2010 to 2012, yielded precise trajectory measurements.
The gravitational tug of a planetary body, such as Enceladus, alters a spacecraft’s flight path. Variations in the gravity field, such as those caused by mountains on the surface or differences in underground composition, can be detected as changes in the spacecraft’s velocity, measured from Earth.
The technique of analyzing a radio signal between Cassini and the Deep Space Network can detect changes in velocity as small as less than one foot per hour (90 microns per second). With this precision, the flyby data yielded evidence of a zone inside the southern end of the moon with higher density than other portions of the interior.
“The way we deduce gravity variations is a concept in physics called the Doppler Effect, the same principle used with a speed-measuring radar gun,” says Sami Asmar of NASA’s Jet Propulsion Laboratory in Pasadena, California, a coauthor of the paper.
“As the spacecraft flies by Enceladus, its velocity is perturbed by an amount that depends on variations in the gravity field that we’re trying to measure. We see the change in velocity as a change in radio frequency, received at our ground stations here all the way across the solar system.”
Researchers theorized that Enceladus contains an interior reservoir of liquid water in 2005 when Cassini discovered water vapor and ice spewing from vents near the moon’s south pole.
“This provides one possible story to explain why water is gushing out of these fractures we see at the south pole,” said David Stevenson of the California Institute of Technology, Pasadena, one of the paper’s co-authors.
The south pole area has a surface depression that causes a dip in the local tug of gravity. However, the magnitude of the dip is less than expected given the size of the depression, leading researchers to conclude the depression’s effect is partially offset by a high-density feature in the region, beneath the surface.
There is no certainty the subsurface ocean supplies the water plume spraying out of surface fractures near the south pole of Enceladus, however, scientists reason it is a real possibility. The fractures may lead down to a part of the moon that is tidally heated by the moon’s repeated flexing, as it follows an eccentric orbit around Saturn.
Much of the excitement about the Cassini mission’s discovery of the Enceladus water plume arises from the possibility that the plume originates from a wet environment that could be a favorable environment for microbial life.
“Material from Enceladus’ south polar jets contains salty water and organic molecules, the basic chemical ingredients for life,” says Linda Spilker, Cassini’s project scientist at NASA’s Jet Propulsion Lab.
“Their discovery expanded our view of the ‘habitable zone’ within our solar system and in planetary systems of other stars,” Spilker said. “This new validation that an ocean of water underlies the jets furthers understanding about this intriguing environment.”
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