Magnetic De-spinning of Space Objects

Metadata Updated: February 28, 2019

Objects in orbit about the earth rotate such that a service spacecraft cannot grapple to them. There are few techniques available to despin a space object without damaging it so that grappling can occur. Electrostatic approaches have been considered, but magnetic approaches have not been sufficiently studied. The basic theory has been developed by the PI and partners when the space object can be modeled as a hollow sphere. Need to explore the parameter space and study a variety of magnetic configurations, large weak fields versus small intense fields and steady state versus time varying. Need to account for orbital dynamics and approach range and time scale issues.Both NASA and the military have future requirements where a satellite must mate to a tumbling space item.[HTML_REMOVED] NASA would like to refuel defunct satellites (this was an early requirement of the Restore Project) and attach to small asteroids, while the military would like to deorbit space debris without creating more debris. In all cases, a grappling satellite must connect with a tumbling item without causing damage to either itself or the item.One possible way to do this is to use magnetic fields to induce a de-spinning torque, slowing the tumbling item down until mating can occur.[HTML_REMOVED] We have shown theoretically and through tabletop experiments that this concept has merit and is deserving of further study. [HTML_REMOVED]The proposed project would have Youngquist and Nurge predict the lateral forces and torques created under various scenarios and then have orbital dynamics experts, Professor Mason Peck of Cornell University and Dr. Frederick Leve of the Air Force Research Lab (AFRL), determine the relative motion and response of each of the interacting objects.[HTML_REMOVED]The goal of this work is to develop a methodology for determining what magnetic field and orbital configuration is optimal to de-spin various space objects; should large, but weak, magnetic fields be used versus small, strong fields?[HTML_REMOVED] What is the time scale of the de-spinning process? How is conservation of angular momentum resolved between the satellite and the tumbling object?[HTML_REMOVED] What relative orbit should be used to help resolve induced lateral forces? Answering these questions will pave the way for the eventual implementation of this concept.

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Public: This dataset is intended for public access and use. License: U.S. Government Work

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Dates

Metadata Created Date August 1, 2018
Metadata Updated Date February 28, 2019

Metadata Source

Harvested from NASA Data.json

Additional Metadata

Resource Type Dataset
Metadata Created Date August 1, 2018
Metadata Updated Date February 28, 2019
Publisher Space Technology Mission Directorate
Unique Identifier TECHPORT_91664
Maintainer
TECHPORT SUPPORT
Maintainer Email
Public Access Level public
Bureau Code 026:00
Metadata Context https://project-open-data.cio.gov/v1.1/schema/catalog.jsonld
Metadata Catalog ID https://data.nasa.gov/data.json
Schema Version https://project-open-data.cio.gov/v1.1/schema
Catalog Describedby https://project-open-data.cio.gov/v1.1/schema/catalog.json
Harvest Object Id 7d690fa2-37f3-43e9-b6f2-3be5a59b77ef
Harvest Source Id 39e4ad2a-47ca-4507-8258-852babd0fd99
Harvest Source Title NASA Data.json
Data First Published 2017-02-01
Homepage URL https://techport.nasa.gov/view/91664
License http://www.usa.gov/publicdomain/label/1.0/
Data Last Modified 2018-07-19
Program Code 026:027
Source Datajson Identifier True
Source Hash e12cee17b2337f064dc795852db07b95509cbc54
Source Schema Version 1.1

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