The electric solar wind sail is a novel propellantless space propulsion concept. According to numerical estimates, the electric solar wind sail can produce a large total impulse per propulsion system mass. Here we consider using a 0.5 N electric solar wind sail for boosting a 550 kg spacecraft to Uranus in less than 6 years. The spacecraft is a stack consisting of the electric solar wind sail module which is jettisoned roughly at Saturn distance, a carrier module and a probe for Uranus atmospheric entry. The carrier module has a chemical propulsion ability for orbital corrections and it uses its antenna for picking up the probe's data transmission and later relaying it to Earth. The scientific output of the mission is similar to what the Galileo Probe did at Jupiter. Measurements of the chemical and isotope composition of the Uranian atmosphere can give key constraints to different formation theories of the Solar System. A similar method could also be applied to other giant planets and Titan by using a fleet of more or less identical probes.
Fast E-sail Uranus entry probe mission
MENGALI, GIOVANNIPenultimo
Investigation
;QUARTA, ALESSANDRO ANTONIOUltimo
Writing – Review & Editing
2014-01-01
Abstract
The electric solar wind sail is a novel propellantless space propulsion concept. According to numerical estimates, the electric solar wind sail can produce a large total impulse per propulsion system mass. Here we consider using a 0.5 N electric solar wind sail for boosting a 550 kg spacecraft to Uranus in less than 6 years. The spacecraft is a stack consisting of the electric solar wind sail module which is jettisoned roughly at Saturn distance, a carrier module and a probe for Uranus atmospheric entry. The carrier module has a chemical propulsion ability for orbital corrections and it uses its antenna for picking up the probe's data transmission and later relaying it to Earth. The scientific output of the mission is similar to what the Galileo Probe did at Jupiter. Measurements of the chemical and isotope composition of the Uranian atmosphere can give key constraints to different formation theories of the Solar System. A similar method could also be applied to other giant planets and Titan by using a fleet of more or less identical probes.File | Dimensione | Formato | |
---|---|---|---|
PSS_vol104_nA_2014.pdf
non disponibili
Descrizione: versione finale pubblicata
Tipologia:
Versione finale editoriale
Licenza:
Importato da Ugov Ricerca - Accesso privato/ristretto
Dimensione
614.39 kB
Formato
Adobe PDF
|
614.39 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
[2014] Fast E-sail Uranus entry probe mission.pdf
accesso aperto
Descrizione: Versione finale identica in tutto a quella pubblicata fuorché nell’impaginazione editoriale.
Tipologia:
Documento in Post-print
Licenza:
Creative commons
Dimensione
177.73 kB
Formato
Adobe PDF
|
177.73 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.