Title: Orientation and Rotational Parameters of Asteroid 4179 Toutatis: New Insights from Chang'e-2's Close Flyby Author: Yuhui Zhao, Jianghui Ji, Jiangchuan Huang, Shoucun Hu, Xiyun Hou, Yuan Li, Wing-Huen Ip
In this work, we investigate the rotational dynamics of the ginger-shaped near-Earth asteroid 4179 Toutatis, which was closely observed by Chang'e-2 at a distance of 770±120 meters from the asteroid's surface during the outbound flyby Huang2013 on 13 December 2012. A sequence of high-resolution images was acquired during the flyby mission. In combination with ground-based radar observations collected over the last two decades, we analyze these flyby images and determine the orientation of the asteroid at the flyby epoch. The 3-1-3 Euler angles of the conversion matrix from the J2000 ecliptic coordinate system to the body-fixed frame are evaluated to be -20.1°±1°, 27.6°±1° and 42.2°±1°, respectively. The least-squares method is utilized to determine the rotational parameters and spin state of Toutatis. The characteristics of the spin-state parameters and angular momentum variations are extensively studied using numerical simulations, which confirm those reported by Takahashi2013. The large amplitude of Toutatis' precession is assumed to be responsible for its tumbling attitude as observed from Earth. Toutatis' angular momentum orientation is determined to be described by lambdaH=180.2+0.2°-0.3° and BetaH=-54.75+0.15°-0.10°, implying that it has remained nearly unchanged for two decades. Furthermore, using Fourier analysis to explore the change in the orientation of Toutatis' axes, we reveal that the two rotational periods are 5.38 and 7.40 days, respectively, consistent with the results of the former investigation. Hence, our investigation provides a clear understanding of the state of the rotational dynamics of Toutatis.
Title: Orbital Evolution of 4179 Toutatis Authors: Suryadi Siregar, Endang Soegiartini
Asteroid 1934 CT;1989 AC, well known as 4179 Toutatis, is an Apollo and Mars-crosser asteroid with a chaotic orbit produced by a 3:1 resonance with Jupiter and a 1:4 resonance with the Earth, and frequent close approaches to the Earth. It is listed as a potential hazardous object (PHA). The aim of this study is to investigate the possibility of 4179 Toutatis to be ejected from the Solar System. This paper presents an orbital evolution of 4179 Toutatis in time interval of ~300 kyr. Investigation of its orbital evolution is conducted by using the Mercury subroutine package, where the gravitational perturbations of eight major planets in the Solar System are considered. Over very short time scales (~300 kyr) relative to the Solar System life time (~10 Gyr), the asteroid 4179 Toutatis gave an example of chaotic motion that can cause asteroid to move outward and may be followed by escaping from the Solar System.
Dan Marcus, observatory director of the Buffalo Astronomical Association, was manning the telescopes at the Beaver Meadow Audubon Centre in North Java Tuesday night to capture the images Read more
The 5400 metre wide asteroid 4179 Toutatis will make a close pass (18.0 lunar distances, 0.0463 AU), travelling at 11.91 km/second, to the Earth-Moon system on the 12th December, 2012 @ 06:40 UT ±00:01.
Title: Composition of Near-Earth Asteroid (4179) Toutatis Authors: Vishnu Reddy, Juan Andreas Sanchez, Michael Gaffey, Paul Abell, Lucille Le Corre, Paul Hardersen
Surface composition of near-Earth asteroid (4179) Toutatis is consistent with an undifferentiated L-chondrite composition. This is inconsistent with early observations that suggested high pyroxene iron content and a differentiated body.