International audience• Tectonic activity at Enceladus' south pole is consistent with clockwise block rotation tectonics. • Regional right-lateral strike-slip kinematics induces transtensional and transpressional regimes in the south polar region. • An evolutionary tectonic model is proposed for the past, present and future settings of Enceladus' south polar structures
On Cassini’s 121st orbit, the onboard ISS camera acquired high-resolution (15-30 m/pxl) images in En...
We investigate the underlying physical processes that govern the formation and evolution of Titan's ...
We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn’s mo...
International audience• Tectonic activity at Enceladus' south pole is consistent with clockwise bloc...
The South Polar Terrain (SPT) of Enceladus is a site with eruptions of gas and water ice particle pl...
Cassini’s Imaging Science Subsystem (ISS) coverage obtained to date shows that the Saturnianmoon Enc...
Enceladus is remarkable not only for its active water ice eruptions near the south pole, but also be...
Until November 2009 the relation of the tectonic styles on the leading hemisphere of Enceladus to th...
The Cassini spacecraft executed a close flyby of Enceladus on August 11 (altitude: 50km); two more ...
Earth's orientation relative to its spin axis is determined by its nonhydrostatic inertia tensor. We...
Earth’s spin axis follows the maximum moment of inertia axis of mantle convection, with some delay d...
Cassini spacecraft images of Enceladus' surface have revealed diverse terrains---some heavily crater...
The rotation of the Earth is not regular. It changes on virtually every timescale we know in both po...
Enceladus, one of the satellites of Saturn, exhibits evidence of recent fault activity, which may be...
Cassini has identified a geologically active province at the south pole of Saturn's moon Enceladus. ...
On Cassini’s 121st orbit, the onboard ISS camera acquired high-resolution (15-30 m/pxl) images in En...
We investigate the underlying physical processes that govern the formation and evolution of Titan's ...
We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn’s mo...
International audience• Tectonic activity at Enceladus' south pole is consistent with clockwise bloc...
The South Polar Terrain (SPT) of Enceladus is a site with eruptions of gas and water ice particle pl...
Cassini’s Imaging Science Subsystem (ISS) coverage obtained to date shows that the Saturnianmoon Enc...
Enceladus is remarkable not only for its active water ice eruptions near the south pole, but also be...
Until November 2009 the relation of the tectonic styles on the leading hemisphere of Enceladus to th...
The Cassini spacecraft executed a close flyby of Enceladus on August 11 (altitude: 50km); two more ...
Earth's orientation relative to its spin axis is determined by its nonhydrostatic inertia tensor. We...
Earth’s spin axis follows the maximum moment of inertia axis of mantle convection, with some delay d...
Cassini spacecraft images of Enceladus' surface have revealed diverse terrains---some heavily crater...
The rotation of the Earth is not regular. It changes on virtually every timescale we know in both po...
Enceladus, one of the satellites of Saturn, exhibits evidence of recent fault activity, which may be...
Cassini has identified a geologically active province at the south pole of Saturn's moon Enceladus. ...
On Cassini’s 121st orbit, the onboard ISS camera acquired high-resolution (15-30 m/pxl) images in En...
We investigate the underlying physical processes that govern the formation and evolution of Titan's ...
We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn’s mo...