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Transneptunian space
We provide a nonspecialist overview of the current state of understanding of the structure
and origin of our Solar System's transneptunian region (often called the Kuiper Belt) …
and origin of our Solar System's transneptunian region (often called the Kuiper Belt) …
[HTML][HTML] Formation of comets
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 …
an ongoing controversy. In this review, we describe comets' physical evolution from dust and …
Thresholds for particle clum** by the streaming instability
The streaming instability (SI) is a mechanism to aerodynamically concentrate solids in
protoplanetary disks and trigger the formation of planetesimals. The SI produces strong …
protoplanetary disks and trigger the formation of planetesimals. The SI produces strong …
CO depletion in protoplanetary disks: a unified picture combining physical sequestration and chemical processing
The gas-phase CO abundance (relative to hydrogen) in protoplanetary disks decreases by
up to two orders of magnitude from its interstellar medium value of∼ 10− 4, even after …
up to two orders of magnitude from its interstellar medium value of∼ 10− 4, even after …
The geology and geophysics of Kuiper Belt object (486958) Arrokoth
INTRODUCTION On 1 January 2019, the New Horizons spacecraft passed 3538 km from
Kuiper Belt object (KBO)(486958) Arrokoth. Arrokoth is a contact binary consisting of two …
Kuiper Belt object (KBO)(486958) Arrokoth. Arrokoth is a contact binary consisting of two …
The Geophysical Environment of (486958) Arrokoth—A Small Kuiper Belt Object Explored by New Horizons
NASA's New Horizons mission performed the first flyby of a small Kuiper Belt Object
(KBO),(486958) Arrokoth on 1 January 2019. The fast flyby revealed a fascinating, flattened …
(KBO),(486958) Arrokoth on 1 January 2019. The fast flyby revealed a fascinating, flattened …
OSSOS finds an Exponential Cutoff in the Size Distribution of the Cold Classical Kuiper belt
The cold main classical Kuiper Belt consists of the nonresonant small solar system bodies
with low orbital inclinations and orbital semimajor axes between 42.4 and 47.7 au. These …
with low orbital inclinations and orbital semimajor axes between 42.4 and 47.7 au. These …
Color, composition, and thermal environment of Kuiper Belt object (486958) Arrokoth
WM Grundy, MK Bird, DT Britt, JC Cook, DP Cruikshank… - Science, 2020 - science.org
INTRODUCTION The New Horizons spacecraft flew past (486958) Arrokoth (provisional
designation 2014 MU69) on 1 January 2019. Arrokoth is a member of the subclass of trans …
designation 2014 MU69) on 1 January 2019. Arrokoth is a member of the subclass of trans …
The collisional evolution of the primordial Kuiper Belt, its destabilized population, and the Trojan asteroids
The tumultuous early era of outer solar system evolution culminated when Neptune migrated
across the primordial Kuiper Belt (PKB) and triggered a dynamical instability among the …
across the primordial Kuiper Belt (PKB) and triggered a dynamical instability among the …
Sublimation of ices during the early evolution of Kuiper belt objects
A Parhi, D Prialnik - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
Kuiper belt objects, such as Arrokoth, the probable progenitors of short-period comets,
formed and evolved at large heliocentric distances, where the ambient temperatures appear …
formed and evolved at large heliocentric distances, where the ambient temperatures appear …