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pro vyhledávání: '"Nair Trógolo"'
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An increasing number of Near Earth Asteroids (NEAs) in the range of a few hundred metres to a few kilometres in size have relatively
An increasing number of Near Earth Asteroids (NEAs) in the range of a few hundred metres to a few kilometres in size have relatively
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::534cf5b0eec41898ad83acac14847b3a
http://arxiv.org/abs/2303.07333
http://arxiv.org/abs/2303.07333
Introduction: To understand the long-term history and age of a planetary surface, it is important to analyze the distribution of impact craters, including the case of fast-spinning asteroids. Two of such asteroids have recently been visited by space
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https://explore.openaire.eu/search/publication?articleId=doi_________::92672d9795da13b05dcf6b83a211625a
https://doi.org/10.5194/epsc2022-726
https://doi.org/10.5194/epsc2022-726
1Instituto Universitario de Física Aplicada a las Ciencias y a las Tecnologías, Universidad de Alicante. Alicante, Spain (nair.trogolo@ua.es) 2Observtorio Astronómico de Córdoba, Universidad Nacional de Córdoba. Córdoba, Argentina. 3Departament
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d298b7c5caf2c30b90ddf299bec1d314
https://doi.org/10.5194/epsc2022-1044
https://doi.org/10.5194/epsc2022-1044
Introduction In the frame of the H2020 NEO-MAPP project, we are studying the problem of determining the detailed gravitational field of an arbitrary body as a strategy to get information about the internal structure of irregular shaped and non-homoge
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https://explore.openaire.eu/search/publication?articleId=doi_________::3ccac61ff46842c6679cc07893f91bb5
https://doi.org/10.5194/epsc2022-995
https://doi.org/10.5194/epsc2022-995
In the frame of the H2020 NEO-MAPP project, we propose a Fast Fourier Transform (FFT) based algorithm for efficient computation of the gravity field created by a body with any arbitrary mass distribution defined by a mass density discretized with sui
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::307ba0a8f77c8365c770aece6748adfc
Introduction (65803) Didymos is a binary asteroid that orbits the Sun having a semi-major axis of 1.64 AU and is the target of the DART (NASA) and Hera (ESA) missions. The system is made up of a 780 m diameter primary body (Didymos) and a 160 m satel
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https://explore.openaire.eu/search/publication?articleId=doi_________::b5803ebf4d5ba74cf6b72a94057a3342
https://doi.org/10.5194/epsc2021-676
https://doi.org/10.5194/epsc2021-676
Introduction Determining the detailed gravitational field of a body is a way to get information about the internal structure of irregular shaped and non-homogenous small solar system objects, like asteroids. In the frame of the H2020 NEO-MAPP project
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::be4f27b75d5dcdbfb863a755a9672da3
https://doi.org/10.5194/epsc2021-674
https://doi.org/10.5194/epsc2021-674