|
gptkbp:instance_of
|
gptkb:musical_instruments
|
|
gptkbp:analyzes
|
atmospheric gases
|
|
gptkbp:collaborated_with
|
NASA's missions
|
|
gptkbp:collaborates_with
|
gptkb:European_Space_Agency
|
|
gptkbp:conducts_research_on
|
Venusian atmosphere studies
|
|
gptkbp:contributes_to
|
understanding of Venus's climate
|
|
gptkbp:control_system
|
ground control team
|
|
gptkbp:data_type
|
digital data
|
|
gptkbp:data_usage
|
1 Mbps
|
|
gptkbp:designed_for
|
gptkb:Venus_Express
|
|
gptkbp:developed_by
|
gptkb:Italian_Space_Agency
|
|
gptkbp:has_community
|
planetary scientists
|
|
gptkbp:has_operational_life
|
designed for 5 years minimum
|
|
gptkbp:has_programs
|
custom data processing software
|
|
gptkbp:has_publications
|
numerous scientific papers
|
|
gptkbp:has_user_interface
|
ground control software
|
|
gptkbp:has_view_of
|
up to 30 degrees
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
VIRTIS
|
|
gptkbp:includes
|
two channels
|
|
gptkbp:is_analyzed_in
|
laboratory measurements
scientific algorithms
regular calibration procedures
|
|
gptkbp:is_designed_to
|
withstand harsh conditions
|
|
gptkbp:is_documented_in
|
mission reports
|
|
gptkbp:is_evaluated_by
|
peer review process
|
|
gptkbp:is_implemented_in
|
gptkb:Venus_Express_orbiter
|
|
gptkbp:is_integrated_with
|
other scientific instruments
|
|
gptkbp:is_part_of
|
Venus Express spacecraft
|
|
gptkbp:is_part_of_data_set
|
Venus Express data archive
|
|
gptkbp:is_subject_to
|
regular maintenance checks
|
|
gptkbp:is_supported_by
|
various funding agencies
|
|
gptkbp:is_tested_for
|
thermal vacuum tests
|
|
gptkbp:is_used_for
|
mapping surface temperature
|
|
gptkbp:is_used_to
|
detect surface changes
|
|
gptkbp:is_utilized_for
|
atmospheric modeling
|
|
gptkbp:launch_vehicle
|
gptkb:Soyuz-FG_rocket
|
|
gptkbp:launched
|
November 9, 2005
|
|
gptkbp:legacy
|
Venus exploration history
|
|
gptkbp:lighting
|
April 2006
|
|
gptkbp:mass
|
approximately 20 kg
|
|
gptkbp:measures
|
gptkb:infrared_radiation
|
|
gptkbp:mission
|
gptkb:ESA's_Venus_Express_mission
|
|
gptkbp:mission_duration
|
approximately 8 years
|
|
gptkbp:operated_by
|
ESA and ASI
|
|
gptkbp:operates_in
|
infrared spectrum
|
|
gptkbp:operates_under
|
wavelengths from 1 to 5 micrometers
|
|
gptkbp:operational_status
|
active
|
|
gptkbp:powers
|
30 watts
|
|
gptkbp:products
|
spectral maps
|
|
gptkbp:provides_information_on
|
surface composition
onboard sensors
|
|
gptkbp:provides_spectra_for
|
surface mineralogy
|
|
gptkbp:resolution
|
up to 300 meters per pixel
|
|
gptkbp:scientific_goals
|
study Venus's geology
|
|
gptkbp:storage
|
solid-state memory
|
|
gptkbp:team
|
international scientific team
|
|
gptkbp:type
|
gptkb:spectrometer
|
|
gptkbp:type_of
|
gptkb:spectrometer
|
|
gptkbp:uses_technology
|
cryogenic cooling
|
|
gptkbp:bfsParent
|
gptkb:Rosetta_spacecraft
gptkb:Rosetta
gptkb:Rosetta_mission
gptkb:Venus_Express
gptkb:ESA's_Venus_Express
|
|
gptkbp:bfsLayer
|
5
|