Results 31 to 40 of about 157 (99)

The relationship between the `limiting' Yarkovsky drift speed and asteroid families' Yarkovsky V-shape [PDF]

open access: yesSerbian Astronomical Journal, 2020
The Yarkovsky effect is an important force to consider in order to understand the long-term dynamics of asteroids. This non-gravitational force affects the orbital elements of objects revolving around a source of heat, especially their semi ...
Milić-Žitnik I.
doaj   +1 more source

On Stable Chaos in The Asteroid Belt [PDF]

open access: yesInternational Astronomical Union Colloquium, 1999
AbstractThe twenty most chaotic objects found among first hundred of numbered asteroids are studied. Lyapunov time calculated with and without inner planets indicates that for eleven of those asteroids the strongest chaotic effect results from the resonances with Mars.
openaire   +2 more sources

The transiting dust clumps in the evolved disc of the Sun-like UXor RZ Psc [PDF]

open access: yesRoyal Society Open Science, 2017
RZ Psc is a young Sun-like star, long associated with the UXor class of variable stars, which is partially or wholly dimmed by dust clumps several times each year.
Grant M. Kennedy   +6 more
doaj   +1 more source

The distribution of basaltic asteroids in the Main Belt [PDF]

open access: yesIcarus, 2008
We present the observational results of a survey designed to target and detect asteroids whose colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. Fifty basaltic candidates were selected with orbital elements that lie outside of the Vesta dynamical family.
Ronald Fevig   +7 more
openaire   +3 more sources

Phase Curves of Kuiper Belt Objects, Centaurs, and Jupiter-family Comets from the ATLAS Survey

open access: yesThe Planetary Science Journal, 2023
The Kuiper Belt objects (KBOs), the Centaurs, and the Jupiter-family comets (JFCs) form an evolutionary continuum of small outer solar system objects, and their study allows us to gain insight into the history and evolution of the solar system. Broadband
Matthew M. Dobson   +11 more
doaj   +1 more source

Intelligent Interplanetary Satellite Communication Network for the Exploration of Celestial Bodies

open access: yesEngineering Proceedings, 2023
Recently, a significant interest in space exploration has emerged, driven by the lack of resources and the quest for answers to issues like climate change.
Abraham Urieta-Ortega   +2 more
doaj   +1 more source

Physical properties of asteroids

open access: yesВісник Астрономічної школи, 2000
The most significant data on the physical properties of main-belt and near-Earth asteroids obtained by photometric, polarimetric, spectroscopic and other techniques, including space missions «Galileo» and NEAR, are presented.
D. F. Lupishko
doaj   +1 more source

Scaling, Mirror Symmetries and Musical Consonances Among the Distances of the Planets of the Solar System

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Orbital systems are often self-organized and/or characterized by harmonic relations. Inspired by music theory, we rewrite the Geddes and King-Hele (QJRAS, 24, 10–13, 1983) equations for mirror symmetries among the distances of the planets of the Solar ...
Michael J. Bank, Nicola Scafetta
doaj   +1 more source

The Mid-plane of the Main Asteroid Belt [PDF]

open access: yesThe Astronomical Journal, 2018
Abstract We measure the mid-plane of the main asteroid belt by using the observational data of a nearly complete and unbiased sample of asteroids and find that it has inclination and longitude of ascending node
Saverio Cambioni, Renu Malhotra
openaire   +3 more sources

Asteroid Collisions: Expected Visibility and Rate

open access: yesThe Astronomical Journal
Asteroid collisions are one of the main processes responsible for the evolution of bodies in the main belt. Using observations of the Dimorphos impact by the DART spacecraft, we estimate how asteroid collisions in the main belt may look in the first ...
Eran O. Ofek   +11 more
doaj   +1 more source

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