|
gptkbp:instance_of
|
gptkb:spectrometer
|
|
gptkbp:analyzes
|
gptkb:Jupiter's_moons
gptkb:asteroid_Lutetia
gptkb:comet_67_P/_Churyumov-Gerasimenko
Mars surface
Venus atmosphere
|
|
gptkbp:calibrated_by
|
ground-based observations
|
|
gptkbp:collaborates_with
|
gptkb:European_Space_Agency
|
|
gptkbp:collaborative_projects
|
international space organizations
|
|
gptkbp:contributes_to
|
atmospheric studies
cometary studies
surface composition analysis
|
|
gptkbp:data_type
|
spectral cubes
|
|
gptkbp:designed_for
|
planetary exploration
|
|
gptkbp:developed_by
|
gptkb:Italian_Space_Agency
|
|
gptkbp:has_applications_in
|
geology
planetary science
astrochemistry
|
|
gptkbp:has_component
|
gptkb:cosmic_ray_detector
data processing unit
optical system
|
|
gptkbp:has_impact_on
|
understanding of solar system
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
VIRTIS spectrometer
|
|
gptkbp:is_analyzed_in
|
laboratory measurements
|
|
gptkbp:is_designed_to
|
study celestial bodies
|
|
gptkbp:is_funded_by
|
national space agencies
|
|
gptkbp:is_integrated_with
|
other scientific instruments
|
|
gptkbp:is_part_of
|
Rosetta mission payload
|
|
gptkbp:is_recognized_for
|
its contributions to space science.
|
|
gptkbp:is_tested_for
|
space environment simulations
|
|
gptkbp:is_used_for
|
remote sensing
|
|
gptkbp:launched
|
gptkb:Rosetta_mission
|
|
gptkbp:lighting
|
gptkb:2004
|
|
gptkbp:measures
|
gptkb:infrared_radiation
|
|
gptkbp:operated_by
|
scientists and engineers
|
|
gptkbp:operates_in
|
gptkb:2016
near-infrared range
visible range
|
|
gptkbp:operates_under
|
wavelengths from 0.25 to 5.1 micrometers
|
|
gptkbp:provides
|
spectral data
|
|
gptkbp:provides_information_on
|
gptkb:scientific_community
planetary formation
cometary evolution
surface processes
|
|
gptkbp:resolution
|
spatial resolution
high spectral resolution
|
|
gptkbp:uses
|
gptkb:Rosetta_spacecraft
|
|
gptkbp:uses_technology
|
Fourier-transform spectroscopy
imaging spectroscopy
|
|
gptkbp:bfsParent
|
gptkb:Rosetta
gptkb:Rosetta_mission
|
|
gptkbp:bfsLayer
|
5
|