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The interstellar interlopers
Interstellar interlopers are bodies formed outside of the Solar System but observed passing
through it. The first two identified interlopers, 1I/'Oumuamua and 2I/Borisov, exhibited …
through it. The first two identified interlopers, 1I/'Oumuamua and 2I/Borisov, exhibited …
The planet nine hypothesis
Over the course of the past two decades, observational surveys have unveiled the intricate
orbital structure of the Kuiper Belt, a field of icy bodies orbiting the Sun beyond Neptune. In …
orbital structure of the Kuiper Belt, a field of icy bodies orbiting the Sun beyond Neptune. In …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …
classical planet formation theory, developed when the only known planetary system was our …
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 …
Planetesimal rings as the cause of the Solar System's planetary architecture
Astronomical observations reveal that protoplanetary disks around young stars commonly
have ring-and gap-like structures in their dust distributions. These features are associated …
have ring-and gap-like structures in their dust distributions. These features are associated …
A rich population of free-floating planets in the Upper Scorpius young stellar association
The nature and origin of free-floating planets (FFPs) are still largely unconstrained because
of a lack of large homogeneous samples to enable a statistical analysis of their properties …
of a lack of large homogeneous samples to enable a statistical analysis of their properties …
Direct confirmation of the radial-velocity planet β Pictoris c
M Nowak, S Lacour, AM Lagrange, P Rubini… - Astronomy & …, 2020 - aanda.org
Context. Methods used to detect giant exoplanets can be broadly divided into two
categories: indirect and direct. Indirect methods are more sensitive to planets with a small …
categories: indirect and direct. Indirect methods are more sensitive to planets with a small …
Early Solar System instability triggered by dispersal of the gaseous disk
Abstract The Solar System's orbital structure is thought to have been sculpted by an episode
of dynamical instability among the giant planets,,–. However, the instability trigger and timing …
of dynamical instability among the giant planets,,–. However, the instability trigger and timing …
Magma ocean, water, and the early atmosphere of Venus
The current state and surface conditions of the Earth and its twin planet Venus are drastically
different. Whether these differences are directly inherited from the earliest stages of …
different. Whether these differences are directly inherited from the earliest stages of …
Can Jupiter's Atmospheric Metallicity Be Different from the Deep Interior?
Updated formation and structure models of Jupiter predict a metal-poor envelope. This is at
odds with the two to three times solar metallicity measured by the Galileo probe …
odds with the two to three times solar metallicity measured by the Galileo probe …