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Mission Overview
December 7, 2012
 

Artist concept of NuSTAR, fully extended after launch Artist concept of NuSTAR fully extended after launch. Image credit: NASA/JPL-Caltech
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The NuSTAR mission has deployed the first orbiting telescopes to focus light in the high energy X-ray (6 - 79 keV) region of the electromagnetic spectrum. Our view of the universe in this spectral window has been limited because previous orbiting telescopes have not employed true focusing optics, but rather have used coded apertures that have intrinsically high backgrounds and limited sensitivity.

 

During a two-year primary mission phase, NuSTAR will map selected regions of the sky in order to:

 

  1. Take a census of collapsed stars and black holes of different sizes by surveying regions surrounding the center of own Milky Way Galaxy and performing deep observations of the extragalactic sky;
  2. Map recently-synthesized material in young supernova remnants to understand how stars explode and how elements are created; and
  3. Understand what powers relativistic jets of particles from the most extreme active galaxies hosting supermassive black holes.

 

In addition to its core science program, NuSTAR will offer opportunities for a broad range of science investigations, ranging from probing cosmic ray origins to studying the extreme physics around collapsed stars to mapping microflares on the surface of the Sun. NuSTAR will also respond to targets of opportunity including supernovae and gamma-ray bursts.

 

The NuSTAR instrument consists of two co-aligned grazing incidence telescopes with specially coated optics and newly developed detectors that extend sensitivity to higher energies as compared to previous missions such as Chandra and XMM. After launching into orbit on a small rocket, the NuSTAR telescope extends to achieve a 10-meter focal length. The observatory will provide a combination of sensitivity, spatial, and spectral resolution factors of 10 to 100 improved over previous missions that have operated at these X-ray energies.

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Page Last Updated: November 21st, 2013
Page Editor: NASA Administrator