Blazing Black Holes Spotted in X-ray View of Galaxy IC 342
January 7th, 2013
Credit: NASA/JPL-Caltech

This new view of spiral galaxy IC 342, also known as Caldwell 5, shows data from NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR. High-energy X-ray data from NuSTAR have been translated to the color magenta showing the only X-ray features visible in this galaxy. NuSTAR is the first orbiting telescope to take focused pictures of the cosmos in high-energy X-ray light; previous observations of this same galaxy taken at similar wavelengths blurred the entire object into one pixel.

The two magenta spots are blazing black holes first detected at lower-energy X-ray wavelengths by NASA's Chandra X-ray Observatory. With NuSTAR's complementary data, astronomers can start to home in on the black holes' mysterious properties. The black holes appear much brighter than typical stellar-mass black holes, such as those that pepper our own galaxy, yet they cannot be supermassive black holes or they would have sunk to the galaxy's center. Instead, they may be intermediate in mass, or there may be something else going on to explain their extremely energetic state. NuSTAR will help solve this puzzle.

IC 342 lies 7 million light-years away in the Camelopardalis constellation. The outer edges of the galaxy cannot be seen in this view.

This image shows NuSTAR X-ray data taken at 10 to 35 kiloelectron volts.

Observation

About the Object

Name
IC 342
Type
Galaxy > Type > Spiral
Galaxy > Type > Barred
Distance
10,700,000 Light Years
Redshift
0.000103

Color Mapping

Band Wavelength Telescope
X-ray 22.0 keV NuSTAR
X-ray 6.0 keV NuSTAR

Astrometrics

Position ()
RA = 3h 46m 48.5s
Dec = 68° 5' 46.9"
Field of View
28.3 x 28.3 arcminutes
Orientation
North is up