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Observing asteroids and trans-Neptunian objects with MICADO/MORFEO
International audienceUnderstanding how our Solar System was formed 4.5 billion years ago and how it has evolved since represents one of the major challenges of modern astrophysics.
Arcidiacono, Carmelo +4 more
core +4 more sources
The long-term evolution of the outer solar system is subject to the influence of the giant planets, however, perturbations from other massive bodies located in the region imprint secular signatures, which are discernible in long-term simulations. In this
Marco A. Muñoz-Gutiérrez +2 more
doaj +1 more source
Ryugu's nucleosynthetic heritage from the outskirts of the Solar System. [PDF]
Hopp T +91 more
europepmc +1 more source
Physical properties of trans-Neptunian objects
In 1992, the first body beyond Neptune since the discovery of Pluto in 1930 was found. Since then, nearly a thousand solid bodies, including some of planetary size, have been discovered in the outer Solar System, largely beyond Neptune.
Cruikshank, Dale P. +14 more
core
The Lowell Trans-Neptunian Object [PDF]
openaire +1 more source
Auroral emissions from Uranus and Neptune. [PDF]
Lamy L.
europepmc +1 more source
Ice giant system exploration in the 2020s: an introduction. [PDF]
Fletcher LN +7 more
europepmc +1 more source
Pluto: dazzling, dynamic, and so not dead. [PDF]
Johnson PE, Proudfoot B.
europepmc +1 more source
Exploring the Bimodal Solar System via Sample Return from the Main Asteroid Belt: The Case for Revisiting Ceres. [PDF]
Burbine TH, Greenwood RC.
europepmc +1 more source
GAUSS - genesis of asteroids and evolution of the solar system: A sample return mission to Ceres. [PDF]
Shi X +28 more
europepmc +1 more source

