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.3 min read

NuSTAR's First Five Years in Space

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ June 13, 2017
This artist's concept shows NASA's Nuclear Spectroscopic Telescope Array (NuSTAR) spacecraft on orbit.› Full image and caption
Credit: NASA/JPL-Caltech

To celebrate the fifth anniversary of NASA's NuSTAR space mission, the mission's lead scientist, Fiona Harrison of Caltech, talks about some of her favorite images.

Five years ago, on June 13, 2012, Caltech's Fiona Harrison, principal investigator of NASA's NuSTAR mission, watched with her team as their black-hole-spying spacecraft was launched into space aboard a rocket strapped to the belly of an aircraft. The launch occurred over the Kwajalein Atoll in the Marshall Islands. Many members of the team anxiously followed the launch from the mission's operations center at the University of California, Berkeley, anxious to see what NuSTAR would find.

Now, Harrison shares her take on five of the mission's many iconic images and artist concepts -- ranging from our flaring sun to distant, buried black holes. NuSTAR is the first telescope capable of focusing high-energy X-rays -- and it has taken the most detailed images of the sky in this energy regime to date.

This artist's concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies.
This artist's concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies.
Credit: NASA/JPL-Caltech

"This is an artist's concept of a region very near a black hole," Harrison said. "It was made to go along with some of our very first results, where we measured the spin of a supermassive black hole unambiguously for the first time. NuSTAR's high-energy X-ray vision allowed us to distinguish between models that explain what produces black holes' X-ray emissions, and this information led us to conclude that the observed black hole is rapidly spinning."

This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.
This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.
Credit: NASA/JPL-Caltech/CXC/SAO

"This is a beautiful image, and one of the things we built NuSTAR to do -- to make the first-ever map of emission from radioactivity in the remnant of an exploded star," Harrison said. "We spent years developing specialized detectors to have the capability to make this image. From the image, we were able to determine the mechanism that caused the star to explode." NuSTAR data show high-energy X-rays from radioactive material in blue. Non-radioactive materials are red, yellow and green.

The bulk of a galaxy called Messier 82 (M82), or the 'Cigar galaxy,' is seen in visible-light data captured by the National Optical Astronomy Observatory's 2.1-meter telescope at Kitt Peak in Arizona.
The bulk of a galaxy called Messier 82 (M82), or the 'Cigar galaxy,' is seen in visible-light data captured by the National Optical Astronomy Observatory's 2.1-meter telescope at Kitt Peak in Arizona.
Credit: NASA/JPL-Caltech/SAO/NOAO

"This result was one of the biggest surprises from NuSTAR. We detected X-ray pulses from an object in a galaxy that everybody had assumed was a black hole, thereby showing it was actually a stellar remnant called a pulsar. At the time, it was by far the brightest pulsar known. At first nobody believed it, but the signal was so strong and clear," Harrison said. Since this discovery two other extremely bright pulsars have been found -- prompted by NuSTAR's discovery. High-energy X-rays from the pulsar are seen in pink at the center of the image.

Flaring, active regions of our sun are highlighted in this image combining observations from several telescopes. During the observations, microflares went off, which are smaller versions of the larger flares that also erupt from the sun's surface.
Flaring, active regions of our sun are highlighted in this image combining observations from several telescopes. During the observations, microflares went off, which are smaller versions of the larger flares that also erupt from the sun's surface.
Credit: NASA/JPL-Caltech/GSFC/JAXA

"With NuSTAR, we see flaring, active regions of the sun where high-energy particles are being created. NuSTAR was built as an astrophysics mission, not to study the sun," Harrison said. "People thought we were crazy at first to point such a sensitive observatory at the sun and potentially ruin it. But now, by studying the sun with much greater sensitivity in high-energy X-rays, we are making important contributions to the field of solar physics."

NGC 1448, a galaxy with an active galactic nucleus hidden by gas and dust, is seen in this image combining data from the Carnegie-Irvine Galaxy Survey in the optical range and NASA's NuSTAR in the X-ray range.
NGC 1448, a galaxy with an active galactic nucleus hidden by gas and dust, is seen in this image combining data from the Carnegie-Irvine Galaxy Survey in the optical range and NASA's NuSTAR in the X-ray range.
Credit: NASA/JPL-Caltech/Carnegie-Irvine Galaxy Survey

"This image illustrates another major accomplishment NuSTAR was designed for -- to find hidden black holes buried by dust and gas," Harrison said. "This is a wonderful result, led by two graduate students. What they found is that there is a thick layer of gas and dust hiding the active black hole in the galaxy NGC 1448 from our sight."

NuSTAR is a Small Explorer mission led by Caltech and managed by JPL for NASA's Science Mission Directorate in Washington. NuSTAR was developed in partnership with the Danish Technical University and the Italian Space Agency (ASI). The spacecraft was built by Orbital Sciences Corp., Dulles, Virginia. NuSTAR's mission operations center is at UC Berkeley, and the official data archive is at NASA's High Energy Astrophysics Science Archive Research Center. ASI provides the mission's ground station and a mirror archive. JPL is managed by Caltech for NASA.

For more information on NuSTAR, visit:

https://www.nasa.gov/nustar

http://www.nustar.caltech.edu

News Media Contact

Elizabeth Landau

NASA Headquarters, Washington

202-358-0845

elandau@nasa.gov

Whitney Clavin

Caltech

626-395-1944

wclavin@caltech.edu

2017-166

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