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      Search and study of the space debris and asteroids within ISON project

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          Abstract

          Abstract International Scientific Optical Network (ISON) is an open international voluntary project specializing in observations of the near-Earth space objects. Observatories collaborating with ISON provide the global coverage and successfully combine the observations of the space debris and asteroids. The network includes more than 50 telescopes of 27 observatories in 15 countries and has been working since 2005. ISON monitors the whole GEO region and tracks the objects at GEO, GTO, HEO and LEO. ISON data allowing maintenance of the database of the space objects orbits, validating space debris population model and providing conjunction assessment analysis for satellites at high orbits. ISON develops the technology of asteroid survey with small telescopes and arranges regular photometry observations of near-Earth asteroids (NEA) to investigate the YORP effect, search new binary NEAs, and support radar experiments.

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          Most cited references34

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          THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics

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            Effects of thermal radiation on the dynamics of binary NEAs

            J. Burns, M Cuk (2005)
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              Acceleration of the rotation of asteroid 1862 Apollo by radiation torques

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                Author and article information

                Journal
                aabc
                Anais da Academia Brasileira de Ciências
                An. Acad. Bras. Ciênc.
                Academia Brasileira de Ciências (Rio de Janeiro, RJ, Brazil )
                0001-3765
                1678-2690
                2021
                : 93
                : suppl 1
                : e20200145
                Affiliations
                [6] Akhaltsikhe orgnameSamtskhe-Javakheti State University Georgia
                [10] Tashkent orgnameUlugh Beg Astronomical Institute Uzbekistan
                [15] Moscow orgnameInstitute of Astronomy orgdiv1RAS Russia
                [12] Cairo orgnameNational Research Institute of Astronomy and Geophysics Egypt
                [9] Rome orgnameSapienza University of Rome orgdiv1Piazzale Aldo Moro Italy
                [2] Kharkiv orgnameInstitute of Astronomy orgdiv1V.N. Karazin Kharkiv National University Ukraine
                [11] Saint-Petersburg orgnameInstitute of Applied Astronomy orgdiv1RAS Russia
                [4] Crimea orgnameCrimean Astrophysical Observatory orgdiv1RAS Russia
                [1] Moscow orgnameKeldysh Institute of Applied Mathematics orgdiv1RAS Russia
                [7] San Fernando Cadiz orgnameReal Instituto y Observatorio de la Armada orgdiv1Calle Cecilio Pujazуn Spain
                [3] Bern Bern orgnameUniversity of Bern orgdiv1Astronomical Institute Switzerland
                [14] Almaty orgnameFesenkov Astrophysical Institute Kazakhstan
                [13] Chapel Hill orgnameUniversity of North Carolina orgdiv1Department of Physics and Astronomy United States
                [8] Rome orgnameGroup of Astrodynamics for the Use of Space Systems Italy
                [5] Tbilisi orgnameKharadze Abastumani Astrophysical Observatory orgdiv1Ilya State University Georgia
                Article
                S0001-37652021000200402 S0001-3765(21)09300000402
                10.1590/0001-3765202120200145
                299ad3ea-22a9-4c30-9e08-cc7dbbe6884f

                This work is licensed under a Creative Commons Attribution 4.0 International License.

                History
                : 07 February 2020
                : 30 August 2020
                Page count
                Figures: 0, Tables: 0, Equations: 0, References: 36, Pages: 0
                Product

                SciELO Brazil

                Categories
                Physical Sciences

                binary system,photometry,survey,optical telescopes,near-Earth asteroids,space debris

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