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The Juno Gravity Science Instrument
Authors:Sami W Asmar  Scott J Bolton  Dustin R Buccino  Timothy P Cornish  William M Folkner  Roberto Formaro  Luciano Iess  Andre P Jongeling  Dorothy K Lewis  Anthony P Mittskus  Ryan Mukai  Lorenzo Simone
Institution:1.Jet Propulsion Laboratory,California Institute of Technology,Pasadena,USA;2.Southwest Research Institute Space,San Antonio,USA;3.Italian Space Agency,Rome,Italy;4.Dipartimento di Ingegneria Aerospaziale ed Astronautica,Università La Sapienza,Rome,Italy;5.Thales Alenia Space-Italy,Rome,Italy
Abstract:The Juno mission’s primary science objectives include the investigation of Jupiter interior structure via the determination of its gravitational field. Juno will provide more accurate determination of Jupiter’s gravity harmonics that will provide new constraints on interior structure models. Juno will also measure the gravitational response from tides raised on Jupiter by Galilean satellites. This is accomplished by utilizing Gravity Science instrumentation to support measurements of the Doppler shift of the Juno radio signal by NASA’s Deep Space Network at two radio frequencies. The Doppler data measure the changes in the spacecraft velocity in the direction to Earth caused by the Jupiter gravity field. Doppler measurements at X-band (\(\sim 8\) GHz) are supported by the spacecraft telecommunications subsystem for command and telemetry and are used for spacecraft navigation as well as Gravity Science. The spacecraft also includes a Ka-band (\(\sim 32\) GHz) translator and amplifier specifically for the Gravity Science investigation contributed by the Italian Space Agency. The use of two radio frequencies allows for improved accuracy by removal of noise due to charged particles along the radio signal path.
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