Impact trajectories of the asteroid Apophis in the 21st century

Author:

Sokolov L. L.,Bashakov A. A.,Borisova T. P.,Petrov N. A.,Pitjev N. P.,Shaidulin V. S.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. Alekseev, V.M., Lektsii po nebesnoi mekhanike (Lectures on Celestial Mechanics), Izhevsk: NITs: Regulyarnaya i khaoticheskaya dinamika, 2001.

2. Arnol’d, V.I., On Nonstability of Dynamic System with Several Degrees of Freedom, Dokl. Akad. Nauk SSSR, 1964, vol. 156, no. 1.

3. Asteroidnaya opasnost’: vchera, segodnya, zavtra (Asteroid Hazard: Yesterday, Today, Tomorrow), Shustov, B.M. and Rykhlova, L.V., Eds., Moscow: Fizmatlit, 2010.

4. Bykova, L.E. and Galushina, T.Yu., Evolution of Probable Area of Motion for 99942 Apophis, Okolozemnaya astronomiya 2007, Materialy mezhdunar. konf. 3–7 sentyabrya 2007 g., p. Terskol (Proc. Int. Conf. Near Earth Astronomy. Sept. 3–7, 2007, Terskol Town), Rykhlova, L.V. and Taradii, V.K., Eds., Nalchik, 2008, pp. 48–54.

5. Chesley, S.R., Potential Impact Detection for Near-Earth Asteroids: The Case of 99942 Apophis (2004 MN), Proc. 229th IAU Symp. Asteroids, Comets, Meteors. 2005, Cambridge: Univ. Press, 2006.

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