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gptkbp:instance_of
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gptkb:observatory
|
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gptkbp:bfsLayer
|
4
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gptkbp:bfsParent
|
gptkb:Vesta_asteroid_family
|
|
gptkbp:atmosphere
|
gptkb:none
|
|
gptkbp:available_sizes
|
from a few hundred meters to several kilometers
|
|
gptkbp:body_style
|
irregular
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gptkbp:color
|
reddish to gray
|
|
gptkbp:composed_of
|
silicate minerals
metallic iron
|
|
gptkbp:discovered_by
|
gptkb:19th_century
telescopic observation
|
|
gptkbp:elevation
|
influenced by Jupiter's gravity
|
|
gptkbp:example
|
gptkb:101955_Bennu
gptkb:243_Ida
gptkb:433_Eros
gptkb:162173_Ryugu
gptkb:951_Gaspra
|
|
gptkbp:formed
|
from the early solar system
|
|
gptkbp:future_plans
|
none known
mining resources
|
|
gptkbp:has_spectral_type
|
S-type
|
|
gptkbp:historical_significance
|
first asteroids discovered
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
S-type asteroids
|
|
gptkbp:impact
|
low
|
|
gptkbp:is_essential_for
|
source of metals
|
|
gptkbp:is_explored_in
|
by spacecraft
|
|
gptkbp:is_reflected_in
|
higher than C-type asteroids
|
|
gptkbp:lighting
|
moderate
|
|
gptkbp:location
|
inner asteroid belt
|
|
gptkbp:mechanics
|
can create meteor showers
|
|
gptkbp:mission
|
gptkb:Hayabusa2
OSIRIS-R Ex
|
|
gptkbp:notable_feature
|
metallic core
silicate mantle
|
|
gptkbp:number
|
hundreds known
|
|
gptkbp:orbital_inclination
|
varies
|
|
gptkbp:orbital_period
|
varies
mostly between Mars and Jupiter
|
|
gptkbp:population
|
higher than C-type asteroids
|
|
gptkbp:research
|
studied for planetary formation
|
|
gptkbp:research_areas
|
planetary defense
space resource utilization
|
|
gptkbp:research_focus
|
asteroid mining technology
|
|
gptkbp:research_interest
|
for understanding solar system history
|
|
gptkbp:scientific_classification
|
based on spectral properties
|
|
gptkbp:size
|
varies
|
|
gptkbp:surface
|
craters
ridges
contains pyroxene
contains olivine
|