Statements (53)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Asteroids
|
| 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: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_believed_to |
remnants of planet formation
|
| 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:star
the asteroid belt region |
| gptkbp:is_studied_for |
gptkb:space_mission
planetary formation theories asteroid mining potential understanding the early Solar System |
| gptkbp:is_studied_in |
gptkb:Hubble_Space_Telescope
gptkb:NASA's_Dawn_spacecraft gptkb:space_mission European Space Agency missions |
| gptkbp:is_visible_from |
gptkb:Earth
|
| 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:bfsParent |
gptkb:Vesta
gptkb:asteroid_16_Psyche gptkb:Pallas |
| gptkbp:bfsLayer |
5
|