Dust evolution in protoplanetary discs and the formation of planetesimals: What have we learned from laboratory experiments?

J Blum - Space Science Reviews, 2018 - Springer
After 25 years of laboratory research on protoplanetary dust agglomeration, a consistent
picture of the various processes that involve colliding dust aggregates has emerged …

Five decades of radioglaciology

DM Schroeder, RG Bingham, DD Blankenship… - Annals of …, 2020 - cambridge.org
Radar sounding is a powerful geophysical approach for characterizing the subsurface
conditions of terrestrial and planetary ice masses at local to global scales. As a result, a wide …

DeepNIS: Deep neural network for nonlinear electromagnetic inverse scattering

L Li, LG Wang, FL Teixeira, C Liu… - IEEE Transactions on …, 2018 - ieeexplore.ieee.org
Nonlinear electromagnetic (EM) inverse scattering is a quantitative and super-resolution
imaging technique, in which more realistic interactions between the internal structure of …

The global shape, density and rotation of Comet 67P/Churyumov-Gerasimenko from preperihelion Rosetta/OSIRIS observations

L Jorda, R Gaskell, C Capanna, S Hviid, P Lamy… - Icarus, 2016 - Elsevier
Abstract The Rosetta spacecraft reached Comet 67P/Churyumov-Gerasimenko (hereafter
67P/CG) in August 2014 at an heliocentric distance of 3.6 au and was then put in orbit …

A homogeneous nucleus for comet 67P/Churyumov–Gerasimenko from its gravity field

M Pätzold, T Andert, M Hahn, SW Asmar, JP Barriot… - Nature, 2016 - nature.com
Cometary nuclei consist mostly of dust and water ice. Previous observations have found
nuclei to be low-density and highly porous bodies,,, but have only moderately constrained …

The landing (s) of Philae and inferences about comet surface mechanical properties

J Biele, S Ulamec, M Maibaum, R Roll, L Witte… - Science, 2015 - science.org
The Philae lander, part of the Rosetta mission to investigate comet 67P/Churyumov-
Gerasimenko, was delivered to the cometary surface in November 2014. Here we report the …

Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko

MN Drozdovskaya, EF van Dishoeck… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT Our modern day Solar System has 4.6× 109 yr of evolution behind it with just a
few relics of its birth conditions remaining. Comets are thought to be some of the most …

Evidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles

J Blum, B Gundlach, M Krause, M Fulle… - Monthly Notices of …, 2017 - academic.oup.com
The processes that led to the formation of the planetary bodies in the Solar system are still
not fully understood. Using the results obtained with the comprehensive suite of instruments …

[HTML][HTML] The primordial nucleus of comet 67P/Churyumov-Gerasimenko

BJR Davidsson, H Sierks, C Güttler, F Marzari… - Astronomy & …, 2016 - aanda.org
Context. We investigate the formation and evolution of comet nuclei and other trans-
Neptunian objects (TNOs) in the solar nebula and primordial disk prior to the giant planet …

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 …