|
gptkbp:instance_of
|
gptkb:astronomy
|
|
gptkbp:contains
|
asteroids
comets
dwarf planets
|
|
gptkbp:has_average_distance_from_sun
|
2.7 AU
|
|
gptkbp:has_largest_asteroid
|
gptkb:Ceres
|
|
gptkbp:has_number_of_asteroids
|
over 1 million
|
|
gptkbp:has_second_largest_asteroid
|
gptkb:Vesta
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Asteroid belt
|
|
gptkbp:is_believed_to
|
remnants of planet formation
|
|
gptkbp:is_divided_into
|
gptkb:inner_belt
gptkb:outer_belt
|
|
gptkbp:is_explored_in
|
gptkb:OSIRIS-REx
gptkb:Dawn_spacecraft
gptkb:NEAR_Shoemaker
gptkb:Hayabusa2
|
|
gptkbp:is_home_to
|
gptkb:Centaur
gptkb:Hygiea
gptkb:Vesta
gptkb:Ceres
gptkb:Trojans
gptkb:Pallas
trans-Neptunian objects
binary asteroids
primitive asteroids
carbonaceous asteroids
differentiated asteroids
irregularly shaped asteroids
metal-rich asteroids
silicate asteroids
Hilda asteroids
asteroidal families
icy asteroids
metallic asteroids
organic-rich asteroids
rocky asteroids
rubble pile asteroids
silicate-rich asteroids
smaller asteroids
volatile-rich asteroids
|
|
gptkbp:is_located_in
|
ecliptic plane
|
|
gptkbp:is_part_of
|
gptkb:star
inner solar system
outer solar system
main asteroid belt
|
|
gptkbp:is_studied_for
|
gptkb:space_weather
planetary formation
asteroid mining
resource potential
impact hazards
|
|
gptkbp:is_studied_in
|
gptkb:space_mission
|
|
gptkbp:is_subject_to
|
collisions
orbital resonances
gravitational influences
|
|
gptkbp:is_visible_from
|
gptkb:Earth
|
|
gptkbp:located_in
|
gptkb:Jupiter
gptkb:Mars
|
|
gptkbp:mass
|
4.1 x 10^21 kg
|
|
gptkbp:orbital_period
|
3.3 years
|
|
gptkbp:bfsParent
|
gptkb:nave
gptkb:Asteroids
gptkb:star
|
|
gptkbp:bfsLayer
|
4
|