|
gptkbp:instance_of
|
gptkb:Asteroids
|
|
gptkbp:atmosphere
|
no
|
|
gptkbp:average_temperature
|
~230 K
|
|
gptkbp:country
|
gptkb:none
yes
|
|
gptkbp:diameter
|
525 kilometers
|
|
gptkbp:discovered_by
|
gptkb:Heinrich_Wilhelm_Olbers
|
|
gptkbp:discovery_year
|
March 29, 1807
|
|
gptkbp:geological_formation
|
yes
|
|
gptkbp:has_basins
|
yes
|
|
gptkbp:has_color
|
dark gray
|
|
gptkbp:has_ridges
|
yes
|
|
gptkbp:has_spectral_type
|
V-type
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
asteroid 4 Vesta
|
|
gptkbp:is_considered
|
protoplanet
a target for exploration
a remnant of early solar system
a candidate for future missions
|
|
gptkbp:is_inhabited_by
|
gptkb:none
|
|
gptkbp:is_known_for
|
its large size
its geological diversity
its bright surface
its unique surface features
its role in understanding solar system formation
|
|
gptkbp:is_located_at
|
2.36 AU from the Sun
|
|
gptkbp:is_one_of
|
largest asteroids
|
|
gptkbp:is_part_of
|
the Vesta family of asteroids
the asteroid belt between Mars and Jupiter
Vesta family
the Vesta asteroid family
|
|
gptkbp:is_part_of_asteroid_belt
|
yes
|
|
gptkbp:is_studied_in
|
gptkb:European_Space_Agency
gptkb:NASA
gptkb:astronomy
planetary scientists
|
|
gptkbp:is_visible_from
|
yes
|
|
gptkbp:is_visible_to_telescope
|
yes
|
|
gptkbp:is_visited_by
|
gptkb:Dawn_spacecraft
|
|
gptkbp:light_requirement
|
0.42
|
|
gptkbp:location
|
gptkb:Asteroid_Belt
|
|
gptkbp:mass
|
2.59 × 10^20 kg
|
|
gptkbp:named_after
|
Vesta, the Roman goddess
|
|
gptkbp:orbit_type
|
gptkb:the_Sun
|
|
gptkbp:orbital_period
|
gptkb:Jupiter
3.63 years
|
|
gptkbp:region
|
yes
|
|
gptkbp:rotation_period
|
5.34 hours
|
|
gptkbp:surface
|
yes
basalt and eucrite
|
|
gptkbp:bfsParent
|
gptkb:Heinrich_Wilhelm_Olbers
|
|
gptkbp:bfsLayer
|
5
|