Origin and evolution of the cometary reservoirs
L Dones, R Brasser, N Kaib, H Rickman - Space Science Reviews, 2015 - Springer
Comets have three known reservoirs: the roughly spherical Oort Cloud (for long-period
comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for …
comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for …
On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective
Presented here are the observations and interpretations from a comprehensive analysis of
16 representative particles returned from the C-type asteroid Ryugu by the Hayabusa2 …
16 representative particles returned from the C-type asteroid Ryugu by the Hayabusa2 …
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 …
The Winchcombe meteorite, a unique and pristine witness from the outer solar system
Direct links between carbonaceous chondrites and their parent bodies in the solar system
are rare. The Winchcombe meteorite is the most accurately recorded carbonaceous …
are rare. The Winchcombe meteorite is the most accurately recorded carbonaceous …
Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion
SN Raymond, A Izidoro - Icarus, 2017 - Elsevier
There is a long-standing debate regarding the origin of the terrestrial planets' water as well
as the hydrated C-type asteroids. Here we show that the inner Solar System's water is a …
as the hydrated C-type asteroids. Here we show that the inner Solar System's water is a …
Magnesium isotope evidence that accretional vapour loss shapes planetary compositions
It has long been recognized that Earth and other differentiated planetary bodies are
chemically fractionated compared to primitive, chondritic meteorites and, by inference, the …
chemically fractionated compared to primitive, chondritic meteorites and, by inference, the …
Insight into multi-step geological evolution of C-type asteroids from Ryugu particles
C-type asteroids are the source of the carbonaceous chondrite meteorites and represent
remnants of primitive planetesimals that formed at the outer margins of the early Solar …
remnants of primitive planetesimals that formed at the outer margins of the early Solar …
Hydrogen isotopes in lunar volcanic glasses and melt inclusions reveal a carbonaceous chondrite heritage
AE Saal, EH Hauri, JA Van Orman, MJ Rutherford - Science, 2013 - science.org
Water is perhaps the most important molecule in the solar system, and determining its origin
and distribution in planetary interiors has important implications for understanding the …
and distribution in planetary interiors has important implications for understanding the …
Growing the terrestrial planets from the gradual accumulation of submeter-sized objects
Building the terrestrial planets has been a challenge for planet formation models. In
particular, classical theories have been unable to reproduce the small mass of Mars and …
particular, classical theories have been unable to reproduce the small mass of Mars and …
Early aqueous activity on the ordinary and carbonaceous chondrite parent bodies recorded by fayalite
PM Doyle, K Jogo, K Nagashima, AN Krot… - Nature …, 2015 - nature.com
Chronology of aqueous activity on chondrite parent bodies constrains their accretion times
and thermal histories. Radiometric 53Mn–53Cr dating has been successfully applied to …
and thermal histories. Radiometric 53Mn–53Cr dating has been successfully applied to …