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2/23/10 7:44 PM A Saturn Ring Observer Mission Using Multi-Mission Radioisotope Power Systems Page 1 of 1 http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=APCPCS000813000001000155000001&idtype=cvips&gifs=yes&ref=no Scitation | AIP Journals | Purchasing Info | Librarians | Alerts | Top 20 Articles | Contact | Help | Exit Copyright © 2010 American Institute of Physics Copyright Statement : Rights & Permissions : Permitted/Prohibited Uses Your GOOGLE Search Was Run Search in Saturn Ring Observer This Journal Search AIP Conf. Proc. / Volume 813 / Issue 1 A Saturn Ring Observer Mission Using Multi-Mission Radioisotope Power Systems AIP Conf. Proc. -- January 20, 2006 -- Volume 813, pp. 155-162 SPACE TECH.&APPLIC.INT.FORUM-STAIF 2006: 10th Conf Thermophys Applic Microgravity; 23rd Symp Space Nucl Pwr &Propulsion; 4th Conf Human/Robotic Tech &Nat'l Vision for Space Explor.; 4th Symp Space Coloniz.; 3rd Symp on New Frontiers &Future Concepts; doi:10.1063/1.2169191 Issue Date: 20 January 2006 You are not logged in. Log in ABSTRACT Robert D. Abelson, Thomas R. Spilker, and James H. Shirley Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 301- 445W, Pasadena, CA 91109-8099 Saturn remains one of the most fascinating planets within the solar system. To better understand the complex ring structure of this planet, a conceptual Saturn Ring Observer (SRO) mission is presented that would spend one year in close proximity to Saturn's A and B rings, and perform detailed observations and measurements of the ring particles and electric and magnetic fields. The primary objective of the mission would be to understand ring dynamics, including the microphysics of individual particles and small scale (meters to a few kilometers) phenomena such as particle agglomeration behavior. This would be accomplished by multispectral imaging of the rings at multiple key locations within the A and B rings, and by ring-particle imaging at an unprecedented resolution of 0.5 cm/pixel. The SRO spacecraft would use a Venus-Earth-Earth-Jupiter Gravity Assist (VEEJGA) and be aerocaptured into Saturn orbit using an advanced aeroshell design to minimize propellant mass. Once in orbit, the SRO would stand off from the ring plane 1 to 1.4 km using chemical thrusters to provide short propulsive maneuvers four times per revolution, effectively causing the SRO vehicle to "hop" above the ring plane. The conceptual SRO spacecraft would be enabled by the use of a new generation of multi-mission Radioisotope Power Systems (RPSs) currently being developed by NASA and DOE. These RPSs include the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Stirling Radioisotope Generator (SRG). The RPSs would generate all necessary electrical power ( 330 W e at beginning of life) during the 10-year cruise and 1-year science mission (~11 years total). The RPS heat would be used to maintain the vehicle's operating and survival temperatures, minimizing the need for electrical heaters. Such a mission could potentially launch in the 2015–2020 timeframe, with operations at Saturn commencing in approximately 2030. ©2006 American Institute of Physics Permalink: http://link.aip.org/link/?APCPCS/813/155/1 BUY THIS ARTICLE (US$28) Connotea CiteULike del.icio.us BibSonomy DOWNLOAD CITATION MySCITATION EMAIL ABSTRACT PERMISSIONS/REPRINTS ERRATUM ALERT RESEARCH TOOLKIT BLOG THIS ARTICLE PRINTER FRIENDLY KEYWORDS and PACS Keywords power systems , radioisotope thermoelectric generators, space power generation, space research, Saturn, planetary rings PACS 28.50.Hw Power and production reactors 84.60.Rb Thermoelectric, electrogasdynamic and other direct energy conversion excluding electrochemical, photoelectric, magnetohydrodynamic, and thermionic conversion 07.87.+v Spaceborne and space research instruments, apparatus, and components PUBLICATION DATA Home About Authors Conf Organizers Permissions Terms of Use Volume: Page/Article: Retrieve Search Browse

A Saturn Ring Observer Mission Using Multi-Mission Radioisotope Power Systems

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2/23/10 7:44 PMA Saturn Ring Observer Mission Using Multi-Mission Radioisotope Power Systems

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Copyright © 2010 American Institute of PhysicsCopyright Statement : Rights & Permissions : Permitted/Prohibited Uses

Your GOOGLE Search Was Run Search inSaturn Ring Observer This Journal Search

AIP Conf. Proc. / Volume 813 / Issue 1

A Saturn Ring Observer Mission Using Multi-MissionRadioisotope Power SystemsAIP Conf. Proc. -- January 20, 2006 -- Volume 813, pp. 155-162SPACE TECH.&APPLIC.INT.FORUM-STAIF 2006: 10th Conf Thermophys ApplicMicrogravity; 23rd Symp Space Nucl Pwr &Propulsion; 4th Conf Human/Robotic Tech&Nat'l Vision for Space Explor.; 4th Symp Space Coloniz.; 3rd Symp on New Frontiers&Future Concepts; doi:10.1063/1.2169191

Issue Date: 20 January 2006

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ABSTRACT

Robert D. Abelson, Thomas R. Spilker, and James H. ShirleyJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 301-445W, Pasadena, CA 91109-8099

Saturn remains one of the most fascinating planets within the solar system. To betterunderstand the complex ring structure of this planet, a conceptual Saturn Ring Observer(SRO) mission is presented that would spend one year in close proximity to Saturn's Aand B rings, and perform detailed observations and measurements of the ring particlesand electric and magnetic fields. The primary objective of the mission would be tounderstand ring dynamics, including the microphysics of individual particles and smallscale (meters to a few kilometers) phenomena such as particle agglomeration behavior.This would be accomplished by multispectral imaging of the rings at multiple keylocations within the A and B rings, and by ring-particle imaging at an unprecedentedresolution of 0.5 cm/pixel. The SRO spacecraft would use a Venus-Earth-Earth-JupiterGravity Assist (VEEJGA) and be aerocaptured into Saturn orbit using an advancedaeroshell design to minimize propellant mass. Once in orbit, the SRO would stand offfrom the ring plane 1 to 1.4 km using chemical thrusters to provide short propulsivemaneuvers four times per revolution, effectively causing the SRO vehicle to "hop" abovethe ring plane. The conceptual SRO spacecraft would be enabled by the use of a newgeneration of multi-mission Radioisotope Power Systems (RPSs) currently beingdeveloped by NASA and DOE. These RPSs include the Multi-Mission RadioisotopeThermoelectric Generator (MMRTG) and Stirling Radioisotope Generator (SRG). TheRPSs would generate all necessary electrical power ( 330 We at beginning of life)during the 10-year cruise and 1-year science mission (~11 years total). The RPS heatwould be used to maintain the vehicle's operating and survival temperatures, minimizingthe need for electrical heaters. Such a mission could potentially launch in the 2015–2020timeframe, with operations at Saturn commencing in approximately 2030. ©2006American Institute of Physics

Permalink: http://link.aip.org/link/?APCPCS/813/155/1

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Connotea CiteULike del.icio.us BibSonomy

DOWNLOADCITATION MySCITATION

EMAIL ABSTRACT PERMISSIONS/REPRINTS

ERRATUM ALERT RESEARCH TOOLKIT

BLOG THIS ARTICLE PRINTER FRIENDLY

KEYWORDS and PACS

Keywords

power systems, radioisotope thermoelectricgenerators, space power generation, spaceresearch, Saturn, planetary rings

PACS

28.50.HwPower and production reactors

84.60.RbThermoelectric, electrogasdynamic andother direct energy conversion excludingelectrochemical, photoelectric,magnetohydrodynamic, and thermionicconversion

07.87.+vSpaceborne and space researchinstruments, apparatus, and components(satellites, space vehicles, etc.)

96.30.WrPlanetary rings

YEAR: 2006

PUBLICATION DATA

Home About Authors Conf Organizers Permissions Terms of Use Volume: Page/Article: Retrieve Search Browse