Statements (79)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:space_mission
|
| gptkbp:aired_on |
Jupiter's north pole
|
| gptkbp:collaboration |
gptkb:Sw_RI
gptkb:Lockheed_Martin gptkb:NASA_Ames_Research_Center gptkb:NASA_Goddard_Space_Flight_Center |
| gptkbp:collaborations |
gptkb:Jet_Propulsion_Laboratory
gptkb:NASA_Marshall_Space_Flight_Center gptkb:NASA_Glenn_Research_Center gptkb:Sw_RI gptkb:University_of_California,_Berkeley gptkb:University_of_Colorado_Boulder gptkb:University_of_Maryland gptkb:University_of_Iowa gptkb:Harvard-Smithsonian_Center_for_Astrophysics gptkb:NASA_Langley_Research_Center gptkb:NASA_Ames_Research_Center gptkb:NASA_Jet_Propulsion_Laboratory gptkb:NASA_Johnson_Space_Center gptkb:NASA_Kennedy_Space_Center gptkb:NASA_Goddard_Space_Flight_Center |
| gptkbp:communication |
X-band
|
| gptkbp:data_transmission |
downlink to Earth
downlink data to Earth |
| gptkbp:end_of_mission_plan |
deorbit into Jupiter
|
| gptkbp:first_perijove |
October 2016
|
| https://www.w3.org/2000/01/rdf-schema#label |
Juno mission
|
| gptkbp:instruments |
gptkb:Juno's_Gravity_Science
gptkb:Juno_Energetic_Particle_Detector gptkb:radio_station gptkb:Juno_Gravity_Science gptkb:Juno_Cam gptkb:Juno's_Ultraviolet_Spectrograph gptkb:magnetometer Juno Waves |
| gptkbp:is_a_destination_for |
gptkb:Jupiter
|
| gptkbp:landing_site |
July 4, 2016
|
| gptkbp:launch_date |
August 5, 2011
|
| gptkbp:launch_vehicle |
gptkb:Atlas_V_551
|
| gptkbp:launched |
gptkb:NASA
|
| gptkbp:mission |
active
February 2021 |
| gptkbp:mission_duration |
approximately 20 months
|
| gptkbp:notable_work |
Jupiter has a large amount of water in its atmosphere
Jupiter has a complex and dynamic atmosphere Jupiter has intense auroras Jupiter's atmosphere has a complex cloud structure Jupiter's atmosphere has a deep layer of clouds Jupiter's atmosphere has deep weather systems Jupiter's core is smaller than previously thought Jupiter's equatorial region has a unique structure Jupiter's magnetic field is tilted and offset Jupiter's poles have cyclonic storms Jupiter's rings are faint and made of dust Jupiter's winds are faster than expected Jupiter's polar regions have unique weather patterns Jupiter's atmosphere is more turbulent than expected Jupiter's internal structure is still being studied. Jupiter's gravity field is more complex than expected Jupiter's atmosphere has a high concentration of ammonia Jupiter's magnetic field is generated by a metallic hydrogen layer |
| gptkbp:objective |
study Jupiter's atmosphere
|
| gptkbp:orbital_period |
53 days
|
| gptkbp:payload_capacity |
3,600 kg
|
| gptkbp:power_source |
solar panels
solar energy |
| gptkbp:scientific_goals |
map Jupiter's magnetic field
measure water and ammonia in Jupiter's atmosphere investigate the planet's polar regions understand Jupiter's magnetic field map Jupiter's gravitational field measure atmospheric composition study the origin and evolution of Jupiter understand the origin and evolution of Jupiter |
| gptkbp:spacecraft |
gptkb:Orbital
|
| gptkbp:sustainability |
three
|
| gptkbp:team |
gptkb:Scott_Bolton
|
| gptkbp:bfsParent |
gptkb:NASA
|
| gptkbp:bfsLayer |
3
|