Statements (54)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:Asteroids
|
gptkbp:atmosphere |
gptkb:none
|
gptkbp:available_sizes |
from a few hundred meters to several kilometers
|
gptkbp:collaboration |
between astronomers and planetary scientists
|
gptkbp:collaborations |
involve international space agencies
|
gptkbp:collection |
involves ground-based and space-based telescopes
|
gptkbp:color |
reddish
|
gptkbp:community_outreach |
educational programs about asteroids
|
gptkbp:composed_by |
metallic minerals
|
gptkbp:country |
some have small moons
|
gptkbp:discovery |
first identified in the 1970s
|
gptkbp:example |
gptkb:243_Ida
gptkb:433_Eros gptkb:162173_Ryugu |
gptkbp:formed |
formed in the early solar system
|
gptkbp:geological_formation |
can provide insights into planetary formation
|
gptkbp:has_spectral_type |
K-type
|
gptkbp:historical_significance |
contribute to understanding of solar system history
|
https://www.w3.org/2000/01/rdf-schema#label |
K-type asteroids
|
gptkbp:impact |
can cause significant damage if they collide with Earth
|
gptkbp:is_explored_in |
planned for further study
target for future missions |
gptkbp:is_observed_in |
studied using telescopes
|
gptkbp:is_reflected_in |
moderate to high
|
gptkbp:light_requirement |
varies among different asteroids
|
gptkbp:location |
main asteroid belt
|
gptkbp:mechanics |
can collide with other celestial bodies
|
gptkbp:mineralogy |
contains silicates and metals
|
gptkbp:mission |
may include sample return missions.
targeted by missions like Hayabusa2 |
gptkbp:natural_resources |
may contain water ice
|
gptkbp:notable_work |
test theories of solar system formation
|
gptkbp:orbital_altitude |
affected by gravitational interactions
|
gptkbp:orbital_period |
varies widely
can be influenced by Jupiter's gravity similar to other asteroids |
gptkbp:population_density |
higher than C-type asteroids
|
gptkbp:potential_hazards |
could impact Earth
|
gptkbp:public_interest |
often featured in media and documentaries
|
gptkbp:relationship |
related to S-type asteroids
|
gptkbp:research |
important for planetary science
provide data on asteroid composition use of radar and spectroscopy |
gptkbp:research_interest |
study of early solar system
potential for mining |
gptkbp:rotation_period |
can be fast or slow
|
gptkbp:scientific_classification |
part of the broader asteroid classification system
|
gptkbp:scientific_models |
help in understanding asteroid evolution
|
gptkbp:size |
varies
|
gptkbp:space_weathering |
affects surface characteristics
|
gptkbp:spacecraft_encounters |
provide close-up data
|
gptkbp:surface |
craters and grooves
|
gptkbp:bfsParent |
gptkb:Main_Belt_of_asteroids
|
gptkbp:bfsLayer |
6
|