Water vapour plumes on Jupiter's moon Europa (artist's impression)
Water vapour plumes on Jupiter’s moon Europa (artist’s impression)
Water vapour plumes over Europa
Videos
The NASA/ESA Hubble Space Telescope has
discovered water vapour erupting from the frigid surface of Jupiter’s
moon Europa, in one or more localised plumes near its south pole.
Europa is already thought to harbour a liquid ocean beneath its icy
crust, making the moon one of the main targets in the search for
habitable worlds away from Earth. This new finding is the first
observational evidence of water vapour being ejected off the moon's
surface.
"The discovery that water vapour is ejected near the south pole
strengthens Europa's position as the top candidate for potential
habitability," said lead author Lorenz Roth of the Southwest Research Institute in San Antonio, Texas. "However, we do not know yet if these plumes are connected to subsurface liquid water or not."
The Hubble findings will be published in the 12 December online issue
of Science Express, and are being reported today at the meeting of the
American Geophysical Union in San Francisco, California, USA.
The Hubble discovery makes Europa only the second moon in the Solar
System known to have water vapour plumes. In 2005, plumes of water
vapour and dust were detected by NASA's Cassini orbiter spewing off the
surface of the Saturnian moon Enceladus.
The Europa plumes were discovered by Hubble observations in December
2012. The Space Telescope Imaging Spectrograph (STIS) detected faint
ultraviolet light from an aurora at the moon's south pole. This aurora
is driven by Jupiter's intense magnetic field, which causes particles to
reach such high speeds that they can split the water molecules in the
plume when they hit them, resulting in oxygen and hydrogen ions which
leave their telltale imprint in the colours of the aurora.
So far, only water vapour has been detected — unlike the plumes on Enceladus, which also contain ice and dust particles.
"We pushed Hubble to its limits to see this very faint emission,"
said co-lead author and principal investigator of the Hubble observing
campaign Joachim Saur of the University of Cologne, Germany. "Only
after a particular camera on the Hubble Space Telescope had been
repaired on the last servicing mission by the Space Shuttle did we gain
the sensitivity to really search for these plumes."
Roth suggests long cracks on Europa's surface, known as linea, might
be venting water vapour into space. Similar fissures have been
photographed near Enceladus's south pole by the Cassini spacecraft. It
is unknown how deep inside Europa's crust the source of the water may
be. Roth asks, "Do the vents extend down to a subsurface ocean or
are the ejecta simply from warmed ice caused by friction stresses near
the surface?"
Also like Enceladus, the Hubble team found that the intensity of the
plumes varies with Europa's orbital position. Active geysers have only
been seen when the moon is furthest from Jupiter. But the researchers
could not detect any sign of venting when Europa is closer to Jupiter.
One explanation is that the long fractures in the ice crust
experience more stress as gravitational tidal forces push and pull on
the moon and so open vents at larger distances from Jupiter. The vents
are narrowed or closed when at closest approach to the gas giant planet [1]. Team member Kurt Retherford, also of the Southwest Research Institute, points out that "the
plume variability supports a key prediction that we should see this
kind of tidal effect if there is a subsurface ocean on Europa".
Future space probe missions to Europa could confirm that the exact
locations and sizes of vents and determine whether they connect to
liquid subsurface reservoirs. It is important news for missions such as
ESA's JUpiter ICy moons Explorer,
a mission planned for launch in 2022, and which aims to explore both
Jupiter and three of its largest moons: Ganymede, Callisto, and Europa.
Notes
[1] When Europa orbits around Jupiter,
the moon experiences varying tidal forces at different points in its
orbit. The tidal stresses compress the vents at the south pole region
when Europa is closest to Jupiter, and stretch them when Europa is
furthest away, making it possible for the vents to open up. A subsurface
ocean would allow the stresses on Europa's surface to be much stronger
as the interior would be malleable and flexible.
Notes for editors
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.
The international team of astronomers in this study consists of L.
Roth (Southwest Research Institute, USA; University of Cologne,
Germany), J. Saur (University of Cologne, Germany), K. D. Retherford
(Southwest Research Institute, USA), D. F. Strobel (The Johns Hopkins
University, USA), P. D. Feldman (The Johns Hopkins University, USA), M.
A. McGrath (NASA Marshall Space Flight Center, USA), F. Nimmo
(University of California, USA).
More information
Image credit: NASA, ESA, L. Roth (Southwest Research Institute, USA/University of Cologne, Germany) and M. Kornmesser.
Links
Contacts
Lorenz RothSouthwest Research Institute, San Antonio, Texas, USA
University of Cologne, Germany
Tel: +1-210-522-2225
Email: lorenz.roth@swri.org
Joachim Saur
University of Cologne
Germany
Tel: +49-221-470-2310
Email: jsaur@uni-koeln.de
Nicky Guttridge
ESA/Hubble Public Information Officer
Garching, Germany
Tel: +49-89-3200-6855
Cell: +44 7512 318322
Email: nguttrid@partner.eso.org
Ray Villard
Space Telescope Science Institute
Baltimore, Maryland, USA
Tel: +1-410-338-4514
Email: villard@stsci.edu
