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gptkbp:instance_of
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gptkb:Asteroids
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gptkbp:archaeological_findings
|
noted by astronomers
|
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gptkbp:atmosphere
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gptkb:none
|
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gptkbp:available_sizes
|
1 km to 100 km
|
|
gptkbp:average_temperature
|
varies with distance from the Sun
|
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gptkbp:collaboration
|
international research teams
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gptkbp:collection
|
via telescopes
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gptkbp:collisional_history
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gptkb:complex
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gptkbp:color
|
dark
|
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gptkbp:community
|
actively studying
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gptkbp:composed_by
|
metallic minerals
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gptkbp:composed_of
|
silicates and metals
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gptkbp:country
|
none known
|
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gptkbp:discovery
|
observed in the 1970s
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gptkbp:eccentricity
|
varies
|
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gptkbp:environmental_impact
|
gptkb:unknown
|
|
gptkbp:example
|
(1862) Apollo
(433) Eros
(243) Ida
|
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gptkbp:formed
|
from the early solar system
|
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gptkbp:funding
|
grants available
|
|
gptkbp:future_prospects
|
none known
planned for the next decade
|
|
gptkbp:geological_formation
|
rare but possible
|
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gptkbp:has_color
|
varies
|
|
gptkbp:has_field
|
none known
|
|
gptkbp:has_spectral_type
|
L-type
|
|
gptkbp:historical_significance
|
early solar system studies
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
L-type asteroids
|
|
gptkbp:impact
|
low
|
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gptkbp:is_explored_in
|
by spacecraft
|
|
gptkbp:light_requirement
|
low
|
|
gptkbp:lighting
|
used for rotation studies
|
|
gptkbp:location
|
main asteroid belt
|
|
gptkbp:mechanics
|
can occur with Earth
|
|
gptkbp:mission
|
targeted for future exploration
|
|
gptkbp:orbit_type
|
around the Sun
|
|
gptkbp:orbital_altitude
|
influenced by Jupiter
|
|
gptkbp:orbital_inclination
|
varies
|
|
gptkbp:orbital_period
|
varies
with other bodies
|
|
gptkbp:population_density
|
higher than C-type asteroids
|
|
gptkbp:potential_for_mining
|
high
|
|
gptkbp:potential_for_resource_extraction
|
high interest
|
|
gptkbp:power_source
|
gptkb:unknown
|
|
gptkbp:provides_information_on
|
between institutions
|
|
gptkbp:public_interest
|
increased due to mining potential
|
|
gptkbp:research
|
gptkb:spectroscopy
|
|
gptkbp:research_interest
|
planetary science
|
|
gptkbp:rotation_period
|
varies
|
|
gptkbp:scientific_classification
|
gptkb:S-type_asteroid
|
|
gptkbp:scientific_models
|
used in simulations
|
|
gptkbp:significance
|
study of solar system formation
|
|
gptkbp:size
|
varies
|
|
gptkbp:size_classification
|
small to medium
|
|
gptkbp:size_distribution
|
varies widely
|
|
gptkbp:surface
|
rocky
craters
|
|
gptkbp:bfsParent
|
gptkb:Main_Belt_of_asteroids
|
|
gptkbp:bfsLayer
|
6
|