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Space-weathering of solar system bodies: A laboratory perspective
In the past few years, several major space missions have been completed (eg, Deep Impact,
LCROSS, Chandrayaan-1, Stardust, Hayabusa), and a number of spacecraft are currently …
LCROSS, Chandrayaan-1, Stardust, Hayabusa), and a number of spacecraft are currently …
Cassini-Huygens' exploration of the Saturn system: 13 years of discovery
L Spilker - Science, 2019 - science.org
The Cassini-Huygens mission to Saturn provided a close-up study of the gas giant planet, as
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …
Dynamical evidence for a late formation of Saturn's moons
M Ćuk, L Dones, D Nesvorný - The Astrophysical Journal, 2016 - iopscience.iop.org
We explore the past evolution of Saturn's moons using direct numerical integrations. We find
that the past Tethys–Dione 3: 2 orbital resonance predicted in standard models likely did not …
that the past Tethys–Dione 3: 2 orbital resonance predicted in standard models likely did not …
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 …
Rimmed and rippled accretion disc models to explain AGN continuum lags
DA Starkey, J Huang, K Horne… - Monthly Notices of the …, 2023 - academic.oup.com
We propose a solution to the problem of accretion disc sizes in active galactic nuclei being
larger when measured by reverberation map** than predicted by theory. Considering the …
larger when measured by reverberation map** than predicted by theory. Considering the …
Origin of Saturn's rings and inner moons by mass removal from a lost Titan-sized satellite
RM Canup - Nature, 2010 - nature.com
The origin of Saturn's rings has not been adequately explained. The current rings are more
than 90 to 95 per cent water ice, which implies that initially they were almost pure ice …
than 90 to 95 per cent water ice, which implies that initially they were almost pure ice …
Global models of runaway accretion in white dwarf debris discs
BD Metzger, RR Rafikov… - Monthly Notices of the …, 2012 - academic.oup.com
A growing number of young white dwarfs (WDs) with metal-enriched atmospheres are
accompanied by excess infrared (IR) emission, indicating that they are encircled by a …
accompanied by excess infrared (IR) emission, indicating that they are encircled by a …
Runaway accretion of metals from compact discs of debris on to white dwarfs
RR Rafikov - Monthly Notices of the Royal Astronomical Society …, 2011 - academic.oup.com
It was recently proposed that metal-rich white dwarfs (WDs) accrete their metals from
compact discs of debris found to exist around more than a dozen of them. At the same time …
compact discs of debris found to exist around more than a dozen of them. At the same time …
Metal accretion onto white dwarfs caused by Poynting–Robertson drag on their debris disks
RR Rafikov - The Astrophysical Journal Letters, 2011 - iopscience.iop.org
Recent discoveries of compact (sizes≲ R☉) debris disks around more than a dozen metal-
rich white dwarfs (WDs) suggest that pollution of these stars with metals may be caused by …
rich white dwarfs (WDs) suggest that pollution of these stars with metals may be caused by …
Plato's cube and the natural geometry of fragmentation
Plato envisioned Earth's building blocks as cubes, a shape rarely found in nature. The solar
system is littered, however, with distorted polyhedra—shards of rock and ice produced by …
system is littered, however, with distorted polyhedra—shards of rock and ice produced by …