1 day / second
0.5 AU
A large main-belt asteroid about 100 kilometers in diameter that was visited by the Rosetta spacecraft in 2010, revealing a heavily cratered, irregular surface with regions of varying geological age.
orbital regime | Asteroid Belt |
learn more | Wikipedia |
mass | 1.7000e+18 kg |
radius | 49 km |
hill radius | 20,055 km |
semi-major axis | 2.435 AU |
eccentricity | 0.163 |
inclination | 3.064º |
longitude of the ascending node | 80.867º |
argument of periapsis | 249.997º |
orbital period | 3.8 years |
sidereal rotation period | 8.166 hours |
axial tilt | 96º |
surface gravity | 0.005 g |
discovery date | November 15, 1852 |
discovered by | Hermann Goldschmidt at the Paris Observatory |
name origins | Named after Lutetia, the ancient Roman name for Paris |
dimensions | 96 km diameter |
albedo | 0.221 |
material composition | X-type and M-type asteroid, suggesting metallic composition |
asteroid group | Located in main asteroid belt |
Flyby
Launched in 2004, visited in 2010
Rosetta flew within 3,162 kilometers of asteroid Lutetia on July 10, 2010, capturing detailed images of its cratered surface and revealing it to be one of the largest and densest asteroids visited by a spacecraft.
A massive yellow dwarf star that contains 99.86% of the Solar System's mass and powers almost all life and weather on Earth through nuclear fusion of hydrogen into helium in its core.
MESSENGER orbited Mercury from 2011 to 2015, capturing over 270,000 images and revealing previously unknown features like volcanic vents and water ice deposits in permanently shadowed craters near the planet's poles.
A large, reddish plutino roughly 650 km in diameter that orbits in a 3:2 resonance with Neptune at an average distance of 30 AU from the Sun.
2024-2025
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