Results 41 to 50 of about 274 (116)
Terrestrial planet and asteroid belt formation by Jupiter-Saturn chaotic excitation. [PDF]
Sci Rep, 2023 Lykawka PS, Ito T.
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A first look at the damocloids [PDF]
, 2005 The Damocloids are objects thought, on dynamical grounds, to be inactive Halley-family and long-period comets. We present optical measurements of 12 such objects, finding that their mean Kron-Cousins colors are BÀV ¼ 0:79 AE 0:01, V ÀR ¼ 0:48 AE 0:01 ...
David Jewitt
core
An Automated Occultation Network for Gravitational Mapping of the Trans-Neptunian Solar System
We explore the potential of an array of ${ \mathcal O }(100)$ small fixed telescopes, aligned along a meridian and automated to measure millions of occultations of Gaia stars by minor planets, to constrain gravitational signatures from a “Planet X” mass ...
Daniel C. H. Gomes, Gary M. Bernstein
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Igneous processes in the small bodies of the Solar System I. Asteroids and comets. [PDF]
iScience, 2023 Leone G, Tanaka HKM.
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CORTO: The Celestial Object Rendering TOol at DART Lab. [PDF]
Sensors (Basel), 2023 Pugliatti M, Buonagura C, Topputo F.
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Determinação da forma de asteroides a partir da inversão de curvas de luz
, 2016 The ligthcurves are obtanied through the monitoring of variation of the intensity of reflect luminosity by one object in fuction of the time. In the case of asteroid, the shape of the ligthcurves depending of its physical characteristics, of its spin ...
Lattari, Victor Correa [UNESP]
core
A novel method for extracting metals from asteroids using non-aqueous deep eutectic solvents. [PDF]
Sci Rep, 2023 Rivera RM +3 more
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, 2014 Simulations of dynamical processes in planetary systems represent an important tool for studying their orbital evolution. Using modern numerical integration methods, it is possible to model systems containing many thousands of objects over time scales ...
Hahn, G. +4 more
core
Olivine-rich achondrites from Vesta and the missing mantle problem. [PDF]
Nat Commun, 2021 Vaci Z +9 more
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