NuSTAR's View of Galaxy NGC 1068
December 17th, 2015
Credit: NASA/ESA/JPL-Caltech/Roma Tre Univ.

Galaxy NGC 1068 is shown in visible light and X-rays in this composite image. High-energy X-rays (magenta) captured by NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, are overlaid on visible-light images from both NASA's Hubble Space Telescope and the Sloan Digital Sky Survey. The X-ray light is coming from an active supermassive black hole, also known as a quasar, in the center of the galaxy. This supermassive black hole has been extensively studied due to its relatively close proximity to our galaxy. NGC 1068 is about 47 million light-years away in the constellation Cetus.

The supermassive black hole is also one of the most obscured known, blanketed by thick clouds of gas and dust. NuSTAR's high-energy X-ray view is the first to penetrate the walls of this black hole's hidden lair.

Observation

About the Object

Name
Messier 77 M77 NGC 1068
Type
Galaxy > Type > Spiral
Galaxy > Activity > AGN
Distance
47,000,000 Light Years
Redshift
0.003793

Color Mapping

Band Wavelength Telescope
Optical 606 nm Hubble WFPC2
Optical 658 nm Hubble ACS
Infrared 814 nm Hubble ACS
Optical 550 nm SDSS
Optical 700 nm SDSS
Infrared 814 nm SDSS
X-ray 10.0 keV NuSTAR

Astrometrics

Position (2000.0)
RA = 2h 42m 40.7s
Dec = 0° 0' 47.8"
Field of View
6.0 x 6.0 arcminutes
Orientation
North is 90.0° right of vertical