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Flux Pinning Laboratory Projects

Microgravity Technology Demonstrations

Flux-pinning demo in zero-g

Laura Jones (left) and William Wilson (right) demonstrate flux pinning of a mockup CubeSat to a dewar containing superconductors in microgravity. This CubeSat mockup contains a flux-pinned revolute joint.

A Space Systems Design Studio team participated in the NASA Facilitated Access to the Space Environment for Technology Development and Training (FAST) program for microgravity flights in August 2009 and September 2010. For both experiments the team flew two mockup CubeSat modules with a flux-pinned interface through 67 microgravity parabolas on a Zero-G Corporation aircraft. These flights demonstrated the flux-pinning concept in small spacecraft, with low stiffness and small separation distances. These experiments have been critical to increasing the technology readiness levels of flux-pinned interfaces and flux-pinned revolute joints.

Microgravity experiment overview and flight week activity highlights

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Air-Leviated Small-Spacecraft Dynamics Testbed

FloatCube

One of the FloatCube testbed platforms

The Space Systems Design Studio has developed a set of nanosatellite-scale, air-levitated vehicles for testing spacecraft dynamics and technologies in a low-friction, 2D environment. These vehicles, slightly larger than CubeSats, currently serve an important role in the verification of our microgravity hardware and procedures. In the future, these modular, customizable vehicles will serve as platform for testing not only flux pinning technologies, but also other spacecraft technologies, sensors, and control strategies.

For more information, see:

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Characterization of Flux Pinning

The flux pinning effect creates effective stiffness and damping for small motions in multiple degrees of freedom. Other researchers have focused mainly on the vertical and lateral stiffness of a connection as applied to levitation systems. The additional stiffness and damping associated with the relative attitude of the components, however, represents a valuable augmentation to the general rigid body motion of vehicles in orbit. By pinning a magnetic field in various relative positions and orientations to a HTSC and observing the system's response to an input, we can estimate the linearized properties at these specific points in configuration space. Fitting an appropriate curve to this data provides an experimentally based description of flux pinning, which informs design choices when creating a flux-pinned formation.

Separation distance vs magnet mass

Flux-pinning stiffness versus intermodule separation and magnet mass (a proxy for permanent magnet dipole strength or electromagnet power) from a model calibrated to experimental results, with several potential applications illustrated.

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Team Members

  • Jessica Gersh
  • Laura Jones
  • Michael Norman

Graduate Alumni

  • Jillian Gorsuch
  • Joseph Shoer
  • William Wilson

Funding

  • Northrop Grumman Space Technologies
  • NASA Institute for Advanced Concepts