Dawn XV

GPTKB entity

Statements (50)
Predicate Object
gptkbp:instance_of gptkb:spacecraft
gptkbp:bfsLayer 7
gptkbp:bfsParent gptkb:Operation_Dominic_VI
gptkbp:communication gptkb:X-band_radio
gptkbp:data_usage up to 1 Mbps
gptkbp:elevation performed multiple thrusts
gptkbp:end_date November 1, 2018
gptkbp:height 1.5 m
https://www.w3.org/2000/01/rdf-schema#label Dawn XV
gptkbp:instrument gptkb:visible_and_infrared_mapping_spectrometer
framing camera
gamma ray and neutron detector
gravity science experiment
ion and electron sensor
gptkbp:is_a_destination_for gptkb:Vesta
gptkb:Ceres
gptkbp:launch_date September 27, 2007
gptkbp:launch_vehicle gptkb:Delta_II_7925
gptkbp:launched gptkb:NASA
gptkbp:length 2.5 m
gptkbp:mass 1,100 kg
gptkbp:mission gptkb:spacecraft
map surface composition
study protoplanets
analyze geological history
gptkbp:mission_duration 11 years
gptkbp:notable_achievement first spacecraft to orbit two extraterrestrial bodies
contributed to understanding of solar system formation
discovered organic materials on Ceres
mapped Ceres' surface and composition
provided detailed images of Vesta's surface
gptkbp:notable_work Ceres has a complex surface geology
Ceres has a large crater called Occator
Ceres has a thin atmosphere
Ceres has a unique surface composition
Ceres has bright spots of sodium carbonate
Ceres shows signs of cryovolcanism
Vesta has a large impact crater called Rheasilvia
Ceres has a complex history of impact events
Ceres has water ice on its surface
Ceres may have a subsurface ocean
Vesta has a differentiated structure
Vesta is believed to be a remnant protoplanet.
Vesta's equatorial region is heavily cratered
Vesta's poles have different geological features
Vesta's surface is covered in basaltic rock
Vesta's surface shows evidence of ancient water activity
gptkbp:operational_status completed
gptkbp:power_output ion propulsion system
gptkbp:width 2.2 m