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Nuclear Spectroscopic Telescope Array (NuSTAR)

Orbital is designing, manufacturing, integrating and testing the Nuclear Spectroscopic Telescope Array (NuSTAR) scientific satellite under a contract from the California Institute of Technology and the Jet Propulsion Laboratory. The NuSTAR observatory will use high-energy X-rays to detect black holes and other energetic phenomena in the universe.

The NuSTAR program is being led by Principal Investigator Dr. Fiona Harrison of Caltech. Its mission is to help scientists answer fundamental questions about the universe, such as:

• How black holes are distributed throughout the cosmos
• How the elements of the universe were created
• What powers the most extreme active galaxies

With answers to these and other questions, NuSTAR will expand our understanding of the origins and destinies of stars and galaxies.

The NuSTAR spacecraft is based on Orbital’s proven LEOStar-2™ design. NuSTAR will be the seventh satellite to be based on this platform, taking advantage of a growing heritage of excellent in-orbit performance from previous missions. Other LEOStar-based satellites that Orbital has designed and built for previous NASA scientific missions include SORCE, GALEX and AIM.

Performance:
Orbit: 525 km, 27° inclination
Launch mass: 360 kg
Solar Arrays: 600 W, Articulated
Redundancy: Single String
Stabilization: 3-axis stabilized
Mission Life: 2 Years

Status:
In design. Launch is planned aboard a Pegasus XL Launch Vehicle in 2011

Customer:
California Institute of Technology/Jet Propulsion Laboratoy (JPL)

Mission:
Expanding our understanding of the origins and destinies of stars and galaxies.

Quick Links
Caltech’s NuSTAR web site

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