Statements (51)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Asteroids
|
| gptkbp:atmospheric_interaction |
minimal due to lack of atmosphere
|
| gptkbp:available_sizes |
from a few hundred meters to several kilometers
|
| gptkbp:average_temperature |
varies based on distance from the Sun
|
| gptkbp:collaborations |
studied by international research teams
|
| gptkbp:collection |
data collected from telescopes and space missions
|
| gptkbp:collisional_family |
may belong to specific collisional families
|
| gptkbp:collisional_history |
influenced by gravitational interactions
|
| gptkbp:color |
typically reddish to grayish
|
| gptkbp:composed_by |
silicate minerals
|
| gptkbp:discovery |
notable discoveries include 1862 Apollo
|
| gptkbp:educational_value |
used in educational programs about space science
|
| gptkbp:example |
gptkb:433_Eros
|
| gptkbp:formed |
formed in the early solar system
|
| gptkbp:future_prospects |
considered unlikely due to harsh conditions
ongoing studies to better understand their properties |
| gptkbp:geological_formation |
potential source of meteorites
|
| gptkbp:has_field |
generally weakly magnetic
|
| gptkbp:has_spectral_type |
Q-type
|
| gptkbp:historical_impact |
subject to collisions with other bodies
|
| gptkbp:historical_significance |
provide clues about early solar system conditions
|
| https://www.w3.org/2000/01/rdf-schema#label |
Q-type asteroids
|
| gptkbp:is_explored_in |
targeted by missions like NEOWISE
|
| gptkbp:light_requirement |
moderate
|
| gptkbp:location |
main asteroid belt
|
| gptkbp:mission |
planned missions to study asteroids further.
|
| gptkbp:number_of_known_objects |
dozens identified
|
| gptkbp:orbital_altitude |
affected by Jupiter's gravity
|
| gptkbp:orbital_period |
similar to S-type asteroids
varies from a few years to several decades |
| gptkbp:population_density |
generally low density
|
| gptkbp:potential_for_mining |
may contain valuable resources
|
| gptkbp:potential_hazards |
could pose impact threats to Earth
|
| gptkbp:public_interest |
increasing interest in asteroid mining and exploration
|
| gptkbp:reflectance_spectrum |
shows features of both S-type and C-type asteroids
|
| gptkbp:relationship_to_comets |
distinct from comets but share some characteristics
|
| gptkbp:relationship_to_other_types |
intermediate between S-type and C-type asteroids
|
| gptkbp:research |
difficult to observe due to size and distance
studied using infrared spectroscopy used to study planetary formation |
| gptkbp:research_importance |
important for understanding asteroid composition
|
| gptkbp:research_interest |
target for future space missions
|
| gptkbp:role_in_solar_system_evolution |
contribute to understanding of solar system history
|
| gptkbp:rotation_period |
varies widely
|
| gptkbp:scientific_classification |
part of the broader asteroid classification system
|
| gptkbp:size |
varies
|
| gptkbp:space_weathering |
surface altered by solar wind and cosmic rays
|
| gptkbp:spectral_analysis |
reveals mineralogical composition
|
| gptkbp:surface |
may have regolith
|
| gptkbp:bfsParent |
gptkb:Main_Belt_of_asteroids
|
| gptkbp:bfsLayer |
6
|