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Published: 2016-05-19

Extraterrestrial oceans – beneath the surface!

NEWS Icy objects in our solar system have large oceans under their surfaces and here life could evolve and flourish. This according to a recent dissertation by Jesper Lindkvist, doctoral student at the Swedish Institute of Space Physics and Umeå University. The dissertation will be defended on Tuesday 31 May at the Swedish Institute of Space Physics in Kiruna, Sweden.

The inside of Jupiter’s moon Callisto, Artist’s impression by NASA/JPL. Source: Wikipedia

There has long been speculation as to whether Jupiter’s large, icy moon Callisto has an ocean beneath its surface. Observations of Callisto’s near-space environment by instruments on board the spacecraft Galileo, which is orbiting Jupiter, lead us to believe that there is such a sub-surface ocean. Computer simulations of the space plasma interactions support this belief.

“If you find an ocean beneath the surface of one moon, perhaps the same is true of other icy objects in space,” says Jesper Lindkvist.

Outflow of water vapour has been detected from the surface of the dwarf planet Ceres, which is in the asteroid belt between Mars and Jupiter. This could indicate a reservoir of water, also related to a large sea beneath the surface. The spacecraft Dawn is at Ceres right now, trying to answer this question.

Jesper Lindkvist comes from the town of Vidsel in Northern Sweden. He has a Masters degree in engineering physics from Luleå University of Technology. Photo: IRF

“If someone was planning to build a future space base on one of these Solar System objects, for example to seek after signs of life, I would suggest they take an extra long ice bore and their fishing equipment,” jokes Jesper Lindkvist.

The outflow of water vapour from moons and dwarf planets is similar to that we see from comets. The icy comet 67P/Churyumov-Gerasimenko which rounded the sun in the summer of 2015 has been followed closely by the European spacecraft Rosetta. Measurements of the space environment around it show that the water flowing out from the comet’s nucleus forms a prominent atmosphere which interacts with the constant flow of ionised particles from the sun, the so-called solar wind.

“Understanding their origin and how icy bodies evolve is one more piece of the puzzle we need to lay in order to explain the origin of our Solar System and its eventual fate,” says Jesper Lindkvist.

Read a digital publication of the dissertation

For more information, please contact:

Jesper Lindkvist, doctoral student, Swedish Institute of Space PhysicsPhone: +46-980-79124
Email: jesper@irf.se

Rick McGregor, Information Officer, Swedish Institute of Space PhysicsPhone: +46-980-79178
Email: rick@irf.se

About the public defence of the dissertation:

On Tuesday 31 May, Jesper Lindkvist at the Swedish Institute of Space Physics in Kiruna and the Department of Physics at Umeå University, will defend his dissertation entitled: Plasma Interactions with Icy Bodies in the Solar System.

The public defence of the dissertation will take place at 9:00 in the Aula at the Swedish Institute of Space Physics in Kiruna.

The opponent is Dr Elias Roussos, Max Planck Institute for Solar System Research, Göttingen, Germany. Supervisors are Associate Professor Mats Holmström and Dr Martin Wieser at the Swedish Institute of Space Physics, Kiruna.

Editor: Ingrid Söderbergh