Will 3552 Don Quixote Escape from the Solar System?
AbstractAsteroid 1983 SA, well known as 3552 Don Quixote, is one of Near Earth Asteroids (NEAs) which is the most probable candidate for the cometary origin, or otherwise as Jupiter-Family-Comets (JFCs). The aim of this study is to investigate the possibility of 3552 Don Quixote to be ejected from the Solar System. This paper presents an orbital evolution of 100 hypothetical asteroids generated by cloning 3552 Don Quixote. Investigation of its orbital evolution is conducted by using the SWIFT subroutine package, where the gravitational perturbations of eight major planets in the Solar System are considered. Over very short time scales (220 kyr) relative to the Solar System life time (10 Gyr), the asteroid 3552 Don Quixote gave an example of chaotic motion that can cause asteroid to move outward and may be followed by escaping from the Solar System. Probability of ejection within the 220 kyr time scale is 50%.
Wetherill, G.W., Origin of the Asteroid Belt, in Asteroids II., R.P. Binzel., T. Gehrels. & M.S. Matthews (eds), pp. 661- 680, 1989.
Kortenkamp, S.J. &Wetherill, G.W., Terrestrial Planet and Asteroid Formation in the Presence of Giant Planets. I. Relatives Velocities of Planetesimals Subject to Jupiter and Saturn Perturbations, Icarus, 143, 60-73, 2000.
Leinhardt, Z.M. & Richardson, D.C., Planetesimals to Protoplanets. I. Effect of Fragmentation on Terrestrial Planet Formation, ApJ, 625, 427-440, 2005.
Siregar, S., Ecliptical Orthogonal Motion and Perihelion Distribution of the AAA Asteroids, PASA, 9(2), 315-316, 1991.
Siregar, S., Perihelion Distribution of the AAA Asteroids, in Proceedings of the Twenty-Fourth Symposium on Celestial Mechanics., H. Kinoshita & H. Yoshida (eds). pp. 32-37, 1991.
Siregar, S., Migration of Near Earth Asteroid to Jovian-Crosser Asteroid:Case Study 3552 Don Quixote, Jurnal Matematika dan Sains, 15(1), 34-38, 2010.
Lupishko, D.F., di Martino, M. & Lupishko, T.A., On the Origins of Earth-Approaching Asteroids, Solar System Research, 35(3), 227-233, 2001.
Siregar, S., On Near-Earth Asteroids Study at Department of Astronomy, Bandung Institute of Technology, in Proceedings of Seminar MIPA IV., Suprijadi (ed), pp. 224-230, 2004.
Siregar, S., On the Relation of AAA Asteroids and Comets, Supplement to J. Astrophysics Astr., 16, 392-393, 1995.
Fernandez, J.A., Gallardo, T. & Brunin, A., Are there Many Inactive Jupiter-Family Comets among the Near-Earth Asteroid Population, Icarus, 159(2), 358-368, 2002.
Yoshida, S. & Nakamura, T., Size Distribution of Small Main-belt Asteroids as the Source of Near-Earth Asteroids, in Proceedings of 35th COSPAR Scientific Assembly., B. T.Soifer (ed), pp. 3729, 2004.
Bottke, W.F., Vokrouhlicky, D., Rubincam, D.P. & Nesvorny, D., The Yarkovsky and Yorp Effects: Implications for Asteroid Dynamics, Ann. Rev. Earth. Planet. Sci, 34, 157-191, 2006.
Emel'yanenko, V.V. & Bailey, M.E., Dynamical Evolution of Comets and the Problem of Cometary Fading, Earth, Moon, and Planets, 72, 35-40, 1996.
Aarseth, S.J., Gravitational N-Body Simulations, Tools and Algorithms, Cambridge University Press, 2003.
Levison, H.F. & Duncan, M.J., The Long-Term Dynamical Behavior of Short-Period Comets, Icarus, 108, 18-36, 1994.
Kozai, Y., Secular Perturbations of Asteroids with High Inclination, AJ, 67(9), 591-598, 1962.
Michel, P. & Thomas, F., The Kozai Resonance for Near-Earth Asteroids with Semimajor Axes Smaller than 2 AU, A & A, 307, 310-318, 1996.
Froeschle, C. & Lega, E., On the Structure of Symplectic Mappings. The Lyapunov Indicator: A Very Sensitive Tool, Celestial Mechanics and Dynamical Astronomy, 78, 167-195, 2000.
Lega, E. & Froeschle, C., On The Relationship between Fast Lyapunov Indicator and Periodic Orbits for Symplectic Mappings, Celestial Mechanics and Dynamical Astronomy, 81, 129-147, 2001.
Farinella, P., Froeschle, Ch., Froeschle, C., Gonzi, R., Hahn, G., Morbidelli, A, & Valsechi, G.B., Asteroids Falling into the Sun, Nature, 371, 314-317, 1994.
Bailey, M.E., Chambers, J.E. & Hahn, G., Origin of Sun Grazers: A Frequent Cometary End-State, Astron. Astrophys, 257, 315-322, 1992.