1 day / second
0.5 AU
A large, elongated, and irregularly shaped asteroid that tumbles chaotically through space while making frequent close approaches to Earth, notable for its complex rotation and unusual peanut-like shape.
orbital regime | Inner System |
learn more | Wikipedia |
mass | 1.9000e+13 kg |
radius | 1.225 km |
hill radius | 206.879 km |
semi-major axis | 2.532 AU |
eccentricity | 0.629 |
inclination | 0.446º |
longitude of the ascending node | 124.3º |
argument of periapsis | 278.75º |
orbital period | 4.029 years |
discovery date | January 4, 1989 |
discovered by | Christian Pollas at Côte d'Azur Observatory, Caussols |
name origins | Named after Teutates, a Celtic god |
dimensions | 5.4 kilometers in diameter |
material composition | S-type asteroid |
density | 2.1 g/cm³ |
albedo | 0.13 |
Flyby
Launched in 2010, visited in 2012
Chang'e 2 completed a close flyby of asteroid Toutatis on December 13, 2012, capturing detailed images from just 3.2 kilometers away while traveling at a relative speed of 10.73 kilometers per second.
A joint mission to Mercury launched in 2018 consisting of two orbiters that will study the planet's composition, magnetosphere, and exosphere after arriving in late 2025 following a complex series of gravity assists from Earth, Venus, and Mercury itself.
Launched in 2007, SELENE (also known as Kaguya) orbited the Moon for 20 months, producing the most detailed lunar gravity map to date and the first high-definition video of an Earthrise over the lunar surface before intentionally impacting the Moon in 2009.
OSIRIS-REx traveled to asteroid Bennu, studied it for two years while in orbit, collected surface samples in 2020 with its touch-and-go sampling mechanism, and returned the samples to Earth in September 2023.
2024-2025
@gordonhart/atlasof.space