Dynamical evolution of the early solar system
D Nesvorný - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Several properties of the Solar System, including the wide radial spacing of the giant
planets, can be explained if planets radially migrated by exchanging orbital energy and …
planets, can be explained if planets radially migrated by exchanging orbital energy and …
Solar System evolution from compositional map** of the asteroid belt
FE DeMeo, B Carry - Nature, 2014 - nature.com
Advances in the discovery and characterization of asteroids over the past decade have
revealed an unanticipated underlying structure that points to a dramatic early history of the …
revealed an unanticipated underlying structure that points to a dramatic early history of the …
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 …
Age of Jupiter inferred from the distinct genetics and formation times of meteorites
The age of Jupiter, the largest planet in our Solar System, is still unknown. Gas-giant planet
formation likely involved the growth of large solid cores, followed by the accumulation of gas …
formation likely involved the growth of large solid cores, followed by the accumulation of gas …
Ryugu's nucleosynthetic heritage from the outskirts of the Solar System
Little is known about the origin of the spectral diversity of asteroids and what it says about
conditions in the protoplanetary disk. Here, we show that samples returned from Cb-type …
conditions in the protoplanetary disk. Here, we show that samples returned from Cb-type …
Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion
Chondrules are millimeter-sized spherules that dominate primitive meteorites (chondrites)
originating from the asteroid belt. The incorporation of chondrules into asteroidal bodies …
originating from the asteroid belt. The incorporation of chondrules into asteroidal bodies …
Preliminary results from NEOWISE: an enhancement to the wide-field infrared survey explorer for solar system science
A Mainzer, J Bauer, T Grav, J Masiero… - The Astrophysical …, 2011 - iopscience.iop.org
ABSTRACT The Wide-field Infrared Survey Explorer (WISE) has surveyed the entire sky at
four infrared wavelengths with greatly improved sensitivity and spatial resolution compared …
four infrared wavelengths with greatly improved sensitivity and spatial resolution compared …
Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres
Studies of the dwarf planet (1) Ceres using ground-based and orbiting telescopes have
concluded that its closest meteoritic analogues are the volatile-rich CI and CM …
concluded that its closest meteoritic analogues are the volatile-rich CI and CM …
The provenances of asteroids, and their contributions to the volatile inventories of the terrestrial planets
Determining the source (s) of hydrogen, carbon, and nitrogen accreted by Earth is important
for understanding the origins of water and life and for constraining dynamical processes that …
for understanding the origins of water and life and for constraining dynamical processes that …
Density of asteroids
B Carry - Planetary and Space Science, 2012 - Elsevier
The small bodies of our solar system are the remnants of the early stages of planetary
formation. A considerable amount of information regarding the processes that occurred …
formation. A considerable amount of information regarding the processes that occurred …