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In-Space Propulsion Program Overview and StatusNASA's In-Space Propulsion (ISP) Program is designed to develop advanced propulsion technologies that can enable or greatly enhance near and mid-term NASA science missions by significantly reducing cost, mass, and/or travel times. These technologies include: Electric Propulsion (Solar and Nuclear Electric) [note: The Nuclear Electric Propulsion work will be transferred to the NSI program in FY03]; Propellantless Propulsion (aerocapture, solar sails, plasma sails, and momentum exchange tethers); Advanced Chemical Propulsion. The ISP approach to identifying and prioritizing these most promising technologies is to use mission analysis and subsequent peer review. These technologies under consideration are mid-Technology Readiness Level (TRL) up to TRL-6 for incorporation into mission planning within three - five years of initiation. In addition, maximum use of open competition is encouraged to seek optimum solutions under ISP. Several NASA Research Announcements (NRAs) have been released asking industry, academia and other organizations to propose propulsion technologies designed to improve our ability to conduct scientific study of the outer planets and beyond. The ISP Program is managed by NASA HQ (Headquarters) and implemented by the Marshall Space Flight Center in Huntsville, Alabama.
Document ID
20020067442
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Carroll, Carol
(NASA Headquarters Washington, DC United States)
Johnson, Les
(NASA Marshall Space Flight Center Huntsville, AL United States)
Baggett, Randy
(NASA Marshall Space Flight Center Huntsville, AL United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2002
Subject Category
Spacecraft Propulsion And Power
Meeting Information
Meeting: 28th International Electric Propulsion Conference (IEPC)
Location: Toulouse
Country: France
Start Date: March 17, 2003
End Date: March 21, 2003
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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