The thermal, mechanical, structural, and dielectric properties of cometary nuclei after Rosetta

O Groussin, N Attree, Y Brouet, V Ciarletti… - Space Science …, 2019 - Springer
The physical properties of cometary nuclei observed today relate to their complex history
and help to constrain their formation and evolution. In this article, we review some of the …

Formation of comets

J Blum, D Bischoff, B Gundlach - Universe, 2022 - mdpi.com
Questions regarding how primordial or pristine the comets of the solar system are have been
an ongoing controversy. In this review, we describe comets' physical evolution from dust and …

Could solar radiation pressure explain 'Oumuamua's peculiar acceleration?

S Bialy, A Loeb - The Astrophysical Journal Letters, 2018 - iopscience.iop.org
Abstract'Oumuamua (1I/2017 U1) is the first object of interstellar origin observed in the solar
system. Recently, Micheli et al. reported that'Oumuamua showed deviations from a …

Synthesis of the morphological description of cometary dust at comet 67P/Churyumov-Gerasimenko

C Güttler, T Mannel, A Rotundi, S Merouane… - Astronomy & …, 2019 - aanda.org
Before Rosetta, the space missions Giotto and Stardust shaped our view on cometary dust,
supported by plentiful data from Earth based observations and interplanetary dust particles …

The dynamical origins of the dark comets and a proposed evolutionary track

AG Taylor, JK Steckloff, DZ Seligman, D Farnocchia… - Icarus, 2024 - Elsevier
So-called 'dark comets' are small, morphologically inactive near-Earth objects (NEOs) that
exhibit nongravitational accelerations inconsistent with radiative effects. These objects …

On the activity of comets: understanding the gas and dust emission from comet 67/Churyumov–Gerasimenko's south-pole region during perihelion

B Gundlach, M Fulle, J Blum - Monthly Notices of the Royal …, 2020 - academic.oup.com
When comets approach the Sun, their surface is heated and the volatile species start to
sublimate. Due to the increasing gas pressure, dust is ejected off the surface, which can be …

A re-assessment of the Kuiper belt size distribution for sub-kilometer objects, revealing collisional equilibrium at small sizes

A Morbidelli, D Nesvorny, WF Bottke, S Marchi - Icarus, 2021 - Elsevier
In this work we combine several constraints provided by the crater records on Arrokoth and
the worlds of the Pluto system to compute the size-frequency distribution (SFD) of the crater …

Shapes, structures, and evolution of small bodies

Y Zhang, P Michel - Astrodynamics, 2021 - Springer
Small bodies are among the best tracers of our Solar System's history. A large number of
space missions to small bodies (past and future) offer a unique opportunity to use these …

Ejection of porous dust–ice agglomerates from the surface of the cometary nucleus

M Wesołowski - Icarus, 2024 - Elsevier
This paper presents two problems related to the ejection of particles from the surface of the
cometary nucleus. The first problem is related to the phase of quiet sublimation. This part of …

Optical spectropolarimetry of large C-complex asteroids: Polarimetric evidence for heterogeneous surface compositions

YG Kwon, S Bagnulo, A Cellino - Astronomy & Astrophysics, 2023 - aanda.org
This study presents the first optical (420–930 nm) spectropolarimetric study of a sample of
large (≳ 100 km in diameter) C-complex asteroids in observing circumstances for which light …