A5065777135- Astro and Planetary Science
- Planetary Science and Exploration
- Astronomical Observations and Instrumentation
- Stellar, planetary, and galactic studies
- Geomagnetism and Paleomagnetism Studies
- Isotope Analysis in Ecology
- Astronomy and Astrophysical Research
- Space Satellite Systems and Control
- Solar and Space Plasma Dynamics
- Gamma-ray bursts and supernovae
- Geophysics and Gravity Measurements
- Spacecraft and Cryogenic Technologies
- Advanced Research in Science and Engineering
- Nuclear physics research studies
- Adversarial Robustness in Machine Learning
- Magnetic confinement fusion research
- Mass Spectrometry Techniques and Applications
- Sociopolitical Dynamics in Russia
- Scientific Research and Discoveries
- Space Exploration and Technology
- Spacecraft Dynamics and Control
- Space Science and Extraterrestrial Life
- Security, Politics, and Digital Transformation
- Advanced Measurement and Metrology Techniques
- Calibration and Measurement Techniques
Academy of Public Administration under the aegis of the President of the Republic of Belarus
2024
Akdeniz University
2017-2019
Technion – Israel Institute of Technology
2014-2016
Institut de Mécanique Céleste et de Calcul des Éphémérides
2008-2015
Université Paris Sciences et Lettres
2015
Observatoire de Paris
2015
Sorbonne Université
2015
Centre National de la Recherche Scientifique
2015
Weizmann Institute of Science
2015
Laboratoire de Tribologie et Dynamique des Systèmes
2008-2013
Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gaia-FUN-SSO) play a key role in ensuring that moving objects first detected ESA's mission remain recoverable after their discovery. An observation campaign on potentially hazardous asteroid (99 942) Apophis was conducted during asteroid's latest period of visibility, from 12/21/2012 to 5/2/2013, test coordination and evaluate overall performance Gaia-FUN-SSO . The 2732 high quality astrometric...
The article discusses the main directions of ensuring information sovereignty in Republic Belarus and Russian Federation, as well ways to improve them. To date, some problems have been identified that relate security sphere Federation Belarus, which made it possible create specific measures resolve Aim. In countries such various studies a comprehensive plan were conducted by scientists, politicians, military. Thanks these studies, today there is theoretical basis for improving entire...
Asteroid masses are the key values for physical studies of their internal structure and also dynamics asteroid families. Dynamical method is based on analysis perturbing effects a bigger mass orbit smaller body (another asteroid, spacecraft, satellite). The use recent ground-based observations by CCD astrometry, reduced using contemporary astrometric catalogues, makes it possible to improve previously adopted determine new ones. present study made at Nikolaev Observatory, TUBITAK National...
Abstract Close encounters of Near Earth Objects (NEOs) with large asteroids are a possible source systematic errors in trajectory propagations and asteroid mitigation. It is, thus, necessary to identify those that have be considered as perturbers NEO orbit modeling. Using the Standard Dynamical Model we searched for between 1649 numbered Asteroids (NEAs) 2191 having sizes greater than 20 km. Investigating 21 st century A. D. found 791 close 195 different lead substantial scattering NEOs.
Among the currently known Near Earth Objects (NEOs), roughly 1400 are classified as being potentially hazardous asteroids. The recent Chelyabinsk event has shown that these objects can pose a real threat to mankind. We illustrate high precision asteroid astrometry plays vital role in determining potential impact risks, selecting targets for deflection demonstration missions and evaluating mitigation mission success. After brief introduction NEOShield project, an international effort...
In order to test the coordination and evaluate overall performance of Gaia-FUN-SSO, an observation campaign on Potentially Hazardous Asteroid (99 942) Apophis was conducted from 12/21/2012 5/2/2013 providing 2732 high quality astrometric observations. We show that a consistent reduction campaigns with reliable stellar catalogs substantially improves results. present evidence new data will help reduce orbit uncertainty during its close approach in 2029.
Orbital resonances are believed to be responsible for the delivery of main belt asteroids inner Solar System. Several possibilities have been suggested transport and their fragments into mean motion secular including non-gravitational forces gravitational scattering. We investigate future resonance crossings known that occur in over next century. Our goal is identify potentially observable injections source regions Near Earth Objects (NEOs) as well determine role close encounters among this process.