Organic compounds found in plumes ejected by Saturn's moon Enceladus
Organic compounds found in plumes ejected by Saturn's moon Enceladus
Data from the Cassini mission has revealed organic compounds in plumes ejected from Enceladus similar to those involved in the development of life on Earth.
Organic compounds have been discovered in plumes bursting through the surface crust of Saturn's icy moon Enceladus. The discovery is the latest boost in the search for conditions that could support life beyond Earth.
Enceladus is known to have a liquid water ocean hidden below its frozen crust, and hydrothermal vents regularly eject liquid water, ice and material from the moon's core out into space.
The newly-discovered molecules have been identified as nitrogen and oxygen-bearing compounds.
Similar compounds are involved in chemical reactions on Earth that produce amino acids: the building blocks of life.
Data collected by Cassini throughout the mission will continue to be analysed by scientists for years to come.
A diagram showing the process by which material is ejected from below the surface of Saturn's moon Enceladus. Credit: NASA/JPL-Caltech
"If the conditions are right, these molecules coming from the deep ocean of Enceladus could be on the same reaction pathway as we see here on Earth," says Nozair Khawaja, who led the team behind the research, based at the Free University of Berlin.
"We don't yet know if amino acids are needed for life beyond Earth, but finding the molecules that form amino acids is an important piece of the puzzle."
The team analysed data from Cassini's Cosmic Dust Analyzer (CDA), which detected ice grains in plumes emitted from the moon.
Mass spectrometer measurements were then used to analyse the organic material in the sample and define its composition.
The organics had originally dissolved in the ocean below Enceladus's surface before evaporating, condensing and freezing onto ice grains within fractures in the moon's crust.
A rising plume then blew the ice grains into space, where they were analysed by the CDA.
"Here we are finding smaller and soluble organic building blocks," says study co-author Jon Hillier, "potential precursors for amino acids and other ingredients required for life on Earth."
10 mesmerising Cassini images of Saturn and its moons
15th October 1997. Launch of Titan IVB/Centaur carrying the Cassini orbiter to Saturn. Taken from Hangar AF on Cape Canaveral Air Force Station. (Credit: NASA)
15th September 2006. Saturn sheltering Cassini from the blinding glare of the Sun, brightening microscopic particles and revealing previously unknown faint rings. (Credit: NASA/JPL/Space Science Institute)
21st November 2009. A view of Enceladus’s south pole. The amazing fissures along the moon's linear depressions, known as its 'tiger stripes', emit icy particles, water vapour and organic compounds from the moon's surface. (Credit: NASA/JPL/Space Science Institute)
19th July 2013. Rare image of Earth from over 1.4 billion kilometers away, showing us as a tiny spec of dot in the vast openness of space. (Credit: NASA/JPL-Caltech/Space Science Institute)
8th March 2014. Spectacular view of Saturn’s rings with Pandora. The gravitational pull from the moon helps confine the outer F ring and keep it from spreading. (Credit: NASA/JPL-Caltech/Space Science Institute)
Near-infrared colour mosaic of Titan’s north pole showing the sunlight reflecting off its seas. (Credit: NASA/JPL-Caltech/Univ. Arizona/Univ. Idaho)
25th May 2015. Enceladus appears to sit on top of Saturn’s rings, with the vastness of the planet behind it. (Credit: NASA/JPL-Caltech/Space Science Institute)
14th October 2015. Zoomed-in view of Enceladus’ north pole, showing the extent of a global system of fractures on the moon's surface. (Credit: NASA/JPL-Caltech/Space Science Institute)
23rd November 2015. Saturn’s moon Tethys floating in the foreground of its parent planet. The moon is composed mainly of water ice, much like the rings of Saturn. (Credit: NASA/JPL-Caltech/Space Science Institute)
6th December 2015. One of Saturn’s many small moons, Epimetheus has had its surface heavily pitted as a result of eons of bombardment. (Credit: NASA/JPL-Caltech/Space Science Institute)