NuSTAR (Nuclear Spectroscopic Telescope Array) is a space-based X-ray telescope that uses a conical approximation to a Wolter telescope to focus high energy X-rays from astrophysical sources, especially for nuclear spectroscopy, and operates in the range of 3 to 79 keV. It is the eleventh mission of the NASA Small Explorer satellite program (SMEX-11) and the first space-based direct-imaging X-ray telescope at energies beyond those of the Chandra X-ray Observatory and XMM-Newton. It was successfully launched on 13 June 2012, having previously been delayed from 21 March due to software issues with the launch vehicle.
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| - NuSTAR (Nuclear Spectroscopic Telescope Array) is a space-based X-ray telescope that uses a conical approximation to a Wolter telescope to focus high energy X-rays from astrophysical sources, especially for nuclear spectroscopy, and operates in the range of 3 to 79 keV. It is the eleventh mission of the NASA Small Explorer satellite program (SMEX-11) and the first space-based direct-imaging X-ray telescope at energies beyond those of the Chandra X-ray Observatory and XMM-Newton. It was successfully launched on 13 June 2012, having previously been delayed from 21 March due to software issues with the launch vehicle.
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dbkwik:nasa/proper...iPageUsesTemplate
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Footer
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Previous Mission
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Power
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spacecraft bus
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telescope area
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- 78(xsd:integer)
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SATCAT
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launch contractor
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Caption
| - Black hole with corona, an X-ray source .
- Blurring of X-rays near Black hole .
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| - 220(xsd:integer)
- 300(xsd:integer)
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Instruments
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orbit mean anomaly
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Image caption
| - Artist's concept of NuSTAR in orbit
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Manufacturer
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orbit period
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Operator
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direction
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header
| - Blurring of an X-ray source near a Black hole.
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telescope type
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Image
| - Black Holes - Monsters in Space.jpg
- PIA18467-NuSTAR-Plot-BlackHole-BlursLight-20140812.png
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launch site
| - Stargazer
- Kwajalein Atoll, Marshall Islands
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names list
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telescope resolution
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apsis
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orbit regime
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Programme
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Website
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orbit arg periapsis
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Next Mission
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abstract
| - NuSTAR (Nuclear Spectroscopic Telescope Array) is a space-based X-ray telescope that uses a conical approximation to a Wolter telescope to focus high energy X-rays from astrophysical sources, especially for nuclear spectroscopy, and operates in the range of 3 to 79 keV. It is the eleventh mission of the NASA Small Explorer satellite program (SMEX-11) and the first space-based direct-imaging X-ray telescope at energies beyond those of the Chandra X-ray Observatory and XMM-Newton. It was successfully launched on 13 June 2012, having previously been delayed from 21 March due to software issues with the launch vehicle. Its primary scientific goals are to conduct a deep survey for black holes a billion times more massive than the Sun, to investigate how particles are accelerated to very high energy in active galaxies, and to understand how the elements are created in the explosions of massive stars by imaging the remains, which are called supernova remnants. After its primary mission of 2 years (to 2014) it is now in a 2-year mission extension to 2016.
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