Statements (50)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:observatory
|
gptkbp:bfsLayer |
3
|
gptkbp:bfsParent |
gptkb:Vesta
|
gptkbp:average_temperature |
varies widely
|
gptkbp:composed_of |
rocky bodies
metallic bodies |
gptkbp:contains |
gptkb:Hygiea
gptkb:Vesta gptkb:Ceres gptkb:Pallas asteroids dwarf planets |
gptkbp:depicted_in |
gptkb:physicist
|
gptkbp:discovered_by |
gptkb:19th_century
|
https://www.w3.org/2000/01/rdf-schema#label |
Main Asteroid Belt
|
gptkbp:is_associated_with |
meteor showers
asteroid impacts on Earth |
gptkbp:is_characterized_by |
different orbits of asteroids
different sizes of asteroids irregular shapes of asteroids varied compositions of asteroids |
gptkbp:is_divided_into |
gptkb:inner_belt
gptkb:outer_belt |
gptkbp:is_home_to |
thousands of asteroids
many small asteroids some larger asteroids the asteroid belt's dynamic processes the asteroid belt's gravitational interactions the asteroid belt's unique environment the fourth largest asteroid Hygiea the largest asteroid Ceres the majority of asteroids in the Solar System the second largest asteroid Vesta the third largest asteroid Pallas the asteroid belt's largest population of asteroids |
gptkbp:is_part_of |
gptkb:observatory
the asteroid belt region |
gptkbp:is_studied_in |
gptkb:spacecraft
gptkb:Hubble_Space_Telescope gptkb:NASA's_Dawn_spacecraft planetary formation theories asteroid mining potential European Space Agency missions understanding the early Solar System |
gptkbp:length |
about 1.1 to 1.9 AU from the Sun
|
gptkbp:located_in |
gptkb:Jupiter
gptkb:Mars |
gptkbp:mass |
about 4% of the Moon's mass
|
gptkbp:orbital_period |
about 4.6 years
|
gptkbp:religion |
remnants of planet formation
|