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Featured researches published by Steven R. Oleson.


40th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit | 2004

Electric Propulsion Technology Development for the Jupiter Icy Moons Orbiter Project

Steven R. Oleson

During 2004 the Jupiter Icy Moons Orbiter project, a part of NASAs Project Prometheus, continued efforts to develop electric propulsion technologies. These technologies addressed the challenges of propelling a spacecraft to several moons of Jupiter. Specific challenges include high power, high specific impulse, long lived ion thrusters, high power / high voltage power processors, accurate feed systems and large propellant storage systems. Critical component work included high voltage insulators and isolators as well as ensuring that the thruster materials and components could operate in the substantial Jupiter radiation environment. A review of these developments along with future plans is discussed.


32nd Joint Propulsion Conference and Exhibit | 1996

Launch vehicle and power level impacts on electric GEO insertion

Steven R. Oleson; Roger M. Myers

Solar Electric Propulsion (SEP) has been shown to increase net geosynchronous spacecraft mass when used for station keeping and final orbit insertion. The impact of launch vehicle selection and power level on the benefits of this approach were examined for 20 and 25 kW systems launched using the Ariane 5, Atlas IIAR, Long March, Proton, and Sea Launch vehicles. Two advanced on-board propulsion technologies, 5 kW ion and Hall thruster systems, were used to establish the relative merits of the technologies and launch vehicles. GaAs solar arrays were assumed. The analysis identifies the optimal starting orbits for the SEP orbit raising/plane changing while considering the impacts of radiation degradation in the Van Allen belts, shading, power degradation, and oblateness. This use of SEP to provide part of the orbit insertion results in net mass increases of 15 - 38% and 18 - 46% for one to two month trip times, respectively, over just using SEP for 15 years of north/south station keeping. SEP technology was shown to have a greater impact on net masses of launch vehicles with higher launch latitudes when avoidance of solar array and payload degradation is desired. This greater impact of SEP could help reduce the plane changing disadvantage of high latitude launch sites. Comparison with results for 10 and 15 kW systems show clear benefits of incremental increases in SEP power level, suggesting that an evolutionary approach to high power SEP for geosynchronous spacecraft is possible.


38th AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit | 2002

Radioisotope Electric Propulsion for Fast Outer Planetary Orbiters

Steven R. Oleson; Scott W. Benson; Leon Gefert; Michael J. Patterson; Jeffrey Schreiber

Recent interest in outer planetary targets by the Office of Space Science has spurred the search for technology options to enable relatively quick missions to outer planetary targets. Several options are being explored including solar electric propelled stages combined with aerocapture at the target and nuclear electric propulsion. Another option uses radioisotope powered electric thrusters to reach the outer planets. Past work looked at using this technology to provide faster flybys. A better use for this technology is for outer planet orbiters. Combined with medium class launch vehicles and a new direct trajectory these small, sub-kilowatt ion thrusters and Stirling radioisotope generators were found to allow missions as fast as 5 to 12 years for objects from Saturn to Pluto, respectively. Key to the development is light spacecraft and science payload technologies.


AIAA SPACE 2011 Conference & Exposition | 2011

Benefits of Power and Propulsion Technology for a Piloted Electric Vehicle to an Asteroid

Carolyn R. Mercer; Steven R. Oleson; Eric J. Pencil; Michael F. Piszczor; Lee S. Mason; Kristen M. Bury; David H. Manzella; Thomas W. Kerslake; Jeffrey S. Hojnicki; John P. Brophy

Abstract NASA’s goal for human spaceflight is to expand permanent human presence beyond low Earth orbit (LEO). NASA is identifying potential missions and technologies needed to achieve this goal. Mission options include crewed destinations to LEO and the International Space Station; high Earth orbit and geosynchronous orbit; cis-lunar space, lunar orbit, and the surface of the Moon; near-Earth objects; and the moons of Mars, Mars orbit, and the surface of Mars. NASA generated a series of design reference missions to drive out required functions and capabilities for these destinations, focusing first on a piloted mission to a near-Earth asteroid. One conclusion from this exercise was that a solar electric propulsion stage could reduce mission cost by reducing the required number of heavy lift launches and could increase mission reliability by providing a robust architecture for the long-duration crewed mission. Similarly, solar electric vehicles were identified as critical for missions to Mars, including orbiting Mars, landing on its surface, and visiting its moons. This paper describes the parameterized assessment of power and propulsion technologies for a piloted solar electric vehicle to a near-Earth asteroid. The objective of the assessment was to determine technology drivers to advance the stateof the art of electric propulsion systems for human exploration. Sensitivity analyses on the performance characteristics of the propulsion and power systems were done to determine potential system-level impacts of improved technology. Starting with a “reasonable vehicle configuration” bounded by an assumed launch date, we introduced technology improvements to determine the system-level benefits (if any) that those technologies might provide. The results of this assessment are discussed and recommendations for future work are described.


41st AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit | 2005

The Prometheus 1 Spacecraft Preliminary Electric Propulsion System Design

Thomas M. Randolph; Ryan Dougherty; Steven R. Oleson; Douglas I. Fiehler; Neil Dipprey

The proposed Prometheus 1 mission is an ambitious plan to orbit and explore the Jovian moons of Callisto, Ganymede, and Europa. Such an ambitious mission is enabled by the first interplanetary nuclear electric propulsion (EP) system.


38th AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit | 2002

Solar Electric Propulsion Vehicle Design Study for Cargo Transfer to Earth-Moon L1

Timothy R. Sarver-Verhey; Thomas W. Kerslake; Vincent K. Rawlin; Robert D. Falck; Leonard J. Dudzinski; Steven R. Oleson

ABSTRACTA design study for a cargo transfer vehicle using solar electric propulsion was performed for NASA’s Revolu-tionary Aerospace Systems Conceptsprogram. Targetedfor 2016, the solar electric propulsion (SEP) transfervehicle is required to deliver a propellant supply module with a mass ofapproximately 36 metric tons fromLow Earth Orbit to the first Earth-Moon libration point (LL1) within 270 days. Following an examination ofpropulsion and power technology options, a SEP transfer vehicle design was selected that incorporated large-area (~2700 m 2 ) thin film solar arrays and a clustered engine configuration of eight 50 kW gridded ionthrusters mountedonanarticulatedboom. Refinement of the SEP vehicle designwasperformediteratively toproperly estimate the required xenon propellant load for the out-bound orbit transfer. The SEP vehicle per-formance, including the xenon propellant estimation, was verified via the SNAP trajectory code. Further ef-fortsare underway to extendthissystem model to otherorbit transfer missions.INTRODUCTION


43rd AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit | 2007

NEXT Ion Propulsion System Configurations and Performance for Saturn System Exploration

Scott W. Benson; John Riehl; Steven R. Oleson

*† ‡ The successes of the Cassini/Huygens mission have heightened interest to return to the Saturn system with focused robotic missions. The desire for a sustained presence at Titan, through a dedicated orbiter and in-situ vehicle, either a lander or aerobot, has resulted in definition of a Titan Explorer flagship mission as a high priority in the Solar System Exploration Roadmap. The discovery of active water vapor plumes erupting from the “tiger stripes” on the moon Enceladus has drawn the attention of the space science community. The NASA’s Evolutionary Xenon Thruster (NEXT) ion propulsion system is well suited to future missions to the Saturn system. NEXT is used within the inner solar system, in combination with a Venus or Earth gravity assist, to establish a fast transfer to the Saturn system. The NEXT system elements are accommodated in a separable Solar Electric Propulsion (SEP) module, or are integrated into the main spacecraft bus, depending on the mission architecture and performance requirements. This paper defines a range of NEXT system configurations, from two to four thrusters, and the Saturn system performance capability provided. Delivered mass is assessed parametrically over total trip time to Saturn. Launch vehicle options, gravity assist options, and input power level are addressed to determine performance sensitivities. A simple twothruster NEXT system, launched on an Atlas 551, can deliver a spacecraft mass of over 2400 kg on a transfer to Saturn. Similarly, a four-thruster system, launched on a Delta 4050 Heavy, delivers more than 4000 kg spacecraft mass. A SEP module conceptual design, for a two thruster string, 17 kW solar array, configuration is characterized.


50th AIAA/ASME/SAE/ASEE Joint Propulsion Conference | 2014

Mission and System Advantages of Iodine Hall Thrusters

John Dankanich; James Szabo; Bruce Pote; Steven R. Oleson; Hani Kamhawi

The exploration of alternative propellants for Hall thrusters continues to be of interest to the community. Investments have been made and continue for the maturation of iodine based Hall thrusters. Iodine testing has shown comparable performance to xenon. However, iodine has a higher storage density and resulting higher V capability for volume constrained systems. Iodines vapor pressure is low enough to permit low-pressure storage, but high enough to minimize potential adverse spacecraft-thruster interactions. The low vapor pressure also means that iodine does not condense inside the thruster at ordinary operating temperatures. Iodine is safe, it stores at sub-atmospheric pressure, and can be stored unregulated for years on end; whether on the ground or on orbit. Iodine fills a niche for both low power ( 10kW) electric propulsion regimes. A range of missions have been evaluated for direct comparison of Iodine and Xenon options. The results show advantages of iodine Hall systems for both small and microsatellite application and for very large exploration class missions.


photovoltaic specialists conference | 2008

Advanced solar cell and array technology for NASA deep space missions

Michael F. Piszczor; Scott W. Benson; David A. Scheiman; David B. Snyder; Homer J. Fincannon; Steven R. Oleson; Geoffrey A. Landis

A recent study by the NASA Glenn Research Center assessed the feasibility of using photovoltaics (PV) to power spacecraft for outer planetary, deep space missions. While the majority of spacecraft have relied on photovoltaics for primary power, the drastic reduction in solar intensity as the spacecraft moves farther from the sun has either limited the power available (severely curtailing scientific operations) or necessitated the use of nuclear systems. A desire by NASA and the scientific community to explore various bodies in the outer solar system and conduct “long-term” operations using smaller, “lower-cost” spacecraft has renewed interest in exploring the feasibility of using photovoltaics for missions to Jupiter, Saturn and beyond. With recent advances in solar cell performance and continuing development in lightweight, high power solar array technology, the study determined that photovoltaics is indeed a viable option for many of these missions.


40th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit | 2004

Neptune Orbiters Utilizing Solar and Radioisotope Electric Propulsion

Douglas I. Fiehler; Steven R. Oleson

†In certain cases, Radioisotope Electric Propulsion (REP), used in conjunction with other propulsion systems, could be used to reduce the trip times for outer planetary orbiter spacecraft. It also has the potential to improve the maneuverability and power capabilities of the spacecraft when the target body is reached as compared with non-electric propulsion spacecraft. Current missions under study baseline aerocapture systems to capture into a science orbit after a Solar Electric Propulsion (SEP) stage is jettisoned. Other options under study would use all REP transfers with small payloads. Compared to the SEP stage / Aerocapture scenario, adding REP to the science spacecraft as well as a chemical capture system can replace the aerocapture system but with a trip time penalty. Eliminating both the SEP stage and the aerocapture system and utilizing a slightly larger launch vehicle, Star 48 upper stage, and a combined REP / Chemical capture system the trip time can nearly be matched, while providing over a kilowatt of science power reused from the REP maneuver. A Neptune Orbiter mission is examined utilizing single propulsion systems and combinations of SEP, REP, and chemical systems to compare concepts.

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