Thermal and magmatic evolution of the Moon
CK Shearer, PC Hess… - … in Mineralogy and …, 2006 - pubs.geoscienceworld.org
As with all science, our continually develo** concepts of lunar evolution are firmly tied to
both new types of observations and the integration of these observations to the known pool …
both new types of observations and the integration of these observations to the known pool …
Exploring the Saturn system in the thermal infrared: The composite infrared spectrometer
FM Flasar, VG Kunde, MM Abbas… - The Cassini-Huygens …, 2004 - Springer
Abstract The Composite Infrared Spectrometer (CIRS) is a remote-sensing Fourier
Transform Spectrometer (FTS) on the Cassini orbiter that measures thermal radiation over …
Transform Spectrometer (FTS) on the Cassini orbiter that measures thermal radiation over …
Dynamics of lunar formation
RM Canup - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract The giant impact theory is the leading hypothesis for the origin of the Moon. This
review focuses on dynamical aspects of an impact-induced lunar formation, in particular …
review focuses on dynamical aspects of an impact-induced lunar formation, in particular …
[PDF][PDF] Origin and evolution of the natural satellites
SJ Peale - Annual Review of Astronomy and Astrophysics, 1999 - researchgate.net
The natural satellites of planets in the solar system display a rich variety of orbital
configurations and surface characteristics that have intrigued astronomers, physicists, and …
configurations and surface characteristics that have intrigued astronomers, physicists, and …
The Cassini ultraviolet imaging spectrograph investigation
Abstract The Cassini Ultraviolet Imaging Spectrograph (UVIS) is part of the remote sensing
payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that …
payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that …
Lunar accretion from an impact-generated disk
Although the mechanism by which the Moon was formed is currently unknown, several lines
of evidence point to its accretion from a circumterrestrial disk of debris generated by a giant …
of evidence point to its accretion from a circumterrestrial disk of debris generated by a giant …
Size distribution of particles in Saturn's rings from aggregation and fragmentation
Saturn's rings consist of a huge number of water ice particles, with a tiny addition of rocky
material. They form a flat disk, as the result of an interplay of angular momentum …
material. They form a flat disk, as the result of an interplay of angular momentum …
Accretion of Saturn's mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons
S Charnoz, A Crida, JC Castillo-Rogez, V Lainey… - Icarus, 2011 - Elsevier
The origin of Saturn's inner mid-sized moons (Mimas, Enceladus, Tethys, Dione and Rhea)
and Saturn's rings is debated. Charnoz et al.[Charnoz, S., Salmon J., Crida A., 2010. Nature …
and Saturn's rings is debated. Charnoz et al.[Charnoz, S., Salmon J., Crida A., 2010. Nature …
The recent formation of Saturn's moonlets from viscous spreading of the main rings
The regular satellites of the giant planets are believed to have finished their accretion
concurrent with the planets, about 4.5 Gyr ago,,,. A population of Saturn's small moons …
concurrent with the planets, about 4.5 Gyr ago,,,. A population of Saturn's small moons …
The formation of Jupiter's faint rings
JA Burns, MR Showalter, DP Hamilton, PD Nicholson… - Science, 1999 - science.org
Observations by the Galileo spacecraft and the Keck telescope showed that Jupiter's
outermost (gossamer) ring is actually two rings circumscribed by the orbits of the small …
outermost (gossamer) ring is actually two rings circumscribed by the orbits of the small …