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Search and study of the space debris and asteroids within ISON project.
Molotov, Igor E; Krugly, Yurij N; Elenin, Leonid V; Schildknecht, Thomas; Rumyantsev, Vasilij V; Inasaridze, Raguli Ya; Aivazyan, Vova R; Kapanadze, Givi V; Canals, Lluis R; Graziani, Filippo; Teofilatto, Paolo; Ehgamberdiev, Shuhrat A; Burkhonov, Otabek A; Chornaya, Ekaterina D; Kochergin, Anton V; Abdel-Aziz, Yehia A; Abdelaziz, Ahmed M; Kouprianov, Vladimir V; Zakhvatkin, Mikhail V; Stepanyants, Victor A; Reva, Inna V; Serebryanskiy, Alexander V; Schmalz, Sergei E; Nikolenko, Igor V.
Afiliação
  • Molotov IE; Keldysh Institute of Applied Mathematics, RAS, Miusskaya sq. 4, 125047, Moscow, Russia.
  • Krugly YN; Institute of Astronomy, V.N. Karazin Kharkiv National University, Sumska Street 35, 61022, Kharkiv, Ukraine.
  • Elenin LV; Keldysh Institute of Applied Mathematics, RAS, Miusskaya sq. 4, 125047, Moscow, Russia.
  • Schildknecht T; Astronomical Institute, University of Bern, Sidlerstrasse 5, 3012, Bern, Switzerland.
  • Rumyantsev VV; Crimean Astrophysical Observatory, RAS, Nauchny, 298409, Crimea, Russia.
  • Inasaridze RY; Kharadze Abastumani Astrophysical Observatory, Ilya State University, K. Cholokashvili Avenue 3/5, 0162, Tbilisi, Georgia.
  • Aivazyan VR; Samtskhe-Javakheti State University, Rustaveli Street 113, 0080, Akhaltsikhe, Georgia.
  • Kapanadze GV; Kharadze Abastumani Astrophysical Observatory, Ilya State University, K. Cholokashvili Avenue 3/5, 0162, Tbilisi, Georgia.
  • Canals LR; Samtskhe-Javakheti State University, Rustaveli Street 113, 0080, Akhaltsikhe, Georgia.
  • Graziani F; Kharadze Abastumani Astrophysical Observatory, Ilya State University, K. Cholokashvili Avenue 3/5, 0162, Tbilisi, Georgia.
  • Teofilatto P; Samtskhe-Javakheti State University, Rustaveli Street 113, 0080, Akhaltsikhe, Georgia.
  • Ehgamberdiev SA; Real Instituto y Observatorio de la Armada, Calle Cecilio Pujazуn, s/n, 11100, San Fernando, Cadiz, Spain.
  • Burkhonov OA; Group of Astrodynamics for the Use of Space Systems, Via Sambuca Pistoiese 70, 00138, Rome, Italy.
  • Chornaya ED; Sapienza University of Rome, Piazzale Aldo Moro, 5, 00185, Rome, Italy.
  • Kochergin AV; Ulugh Beg Astronomical Institute, Astronomicheskaya Street 33, 100052, Tashkent, Uzbekistan.
  • Abdel-Aziz YA; Ulugh Beg Astronomical Institute, Astronomicheskaya Street 33, 100052, Tashkent, Uzbekistan.
  • Abdelaziz AM; Institute of Applied Astronomy, RAS, 10 Kutuzova Embankment, 191187, Saint-Petersburg, Russia.
  • Kouprianov VV; Institute of Applied Astronomy, RAS, 10 Kutuzova Embankment, 191187, Saint-Petersburg, Russia.
  • Zakhvatkin MV; National Research Institute of Astronomy and Geophysics, EL Marsad Street 1, Helwan, 11421, Cairo, Egypt.
  • Stepanyants VA; National Research Institute of Astronomy and Geophysics, EL Marsad Street 1, Helwan, 11421, Cairo, Egypt.
  • Reva IV; University of North Carolina, Department of Physics and Astronomy, 120 E. Cameron Ave., Phillips Hall CB3255, Chapel Hill, NC 27599, U.S.A.
  • Serebryanskiy AV; Keldysh Institute of Applied Mathematics, RAS, Miusskaya sq. 4, 125047, Moscow, Russia.
  • Schmalz SE; Keldysh Institute of Applied Mathematics, RAS, Miusskaya sq. 4, 125047, Moscow, Russia.
  • Nikolenko IV; Fesenkov Astrophysical Institute, Observatory 23, 050020, Almaty, Kazakhstan.
An Acad Bras Cienc ; 93(suppl 1): e20200145, 2021.
Article em En | MEDLINE | ID: mdl-33624725
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.