Images by Date
Images by Category
Solar System
White Dwarfs
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Galaxy Clusters
Cosmology/Deep Field
Images by Interest
Space Scoop for Kids
Sky Map
Photo Blog
Top Rated Images
Image Handouts
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
IC 10 Animations
A Tour of IC 10
(Credit: NASA/CXC/A. Jubett)
[Runtime: 3:19]

Quicktime MPEG With closed-captions (at YouTube)

Long before Starburst® became a popular brand of candy, starbursts were known to astronomers. In 1887, American astronomer Lewis Swift discovered a glowing cloud, or nebula, that turned out to be a small galaxy about 2.2 million light years from Earth. Today, it is known as the "starburst" galaxy IC 10, referring to the intense star formation activity occurring there.

More than a hundred years after Swift's discovery, astronomers are studying IC 10 with the most powerful telescopes of the 21st century. New observations with NASA's Chandra X-ray Observatory reveal many pairs of stars that may one day become sources of perhaps the most exciting cosmic phenomenon observed in recent years: gravitational waves.

By analyzing Chandra observations of IC 10 spanning a decade, astronomers found over a dozen black holes and neutron stars feeding off gas from young, massive stellar companions. Such double star systems are known as "X-ray binaries" because they emit large amounts of X-ray light. As a massive star orbits around its compact companion, either a black hole or neutron star, material can be pulled away from the giant star to form a disk of material around the compact object. Frictional forces heat the infalling material to millions of degrees, producing a bright X-ray source.

When the massive companion star runs out fuel, it will undergo a catastrophic collapse that will produce a supernova explosion, and leave behind a black hole or neutron star. The end result is two compact objects: either a pair of black holes, a pair of neutron stars, or a black hole and neutron star. If the separation between the compact objects becomes small enough as time passes, they will produce gravitational waves. Over time, the size of their orbit will shrink until they merge. LIGO has found three examples of black hole pairs merging in this way in the past two years.

Astronomers will continue to study IC 10 and other similar galaxies to better understand more about X-ray binaries and their connection to the exciting and evolving field of gravitational wave astronomy.

Timelapse of IC 10
(Credit: NASA/CXC/UMass Lowell/S.Laycock et al. )
[Runtime: 0:09]

This time lapse animation shows the starburst galaxy IC 10 in a series of 10 Chandra X-ray images spanning 2003-2010. Bright points are X-ray active stars, including binaries containing a neutron star or black hole pulling gas from a companion star. Some of them appear in only one frame, while others are always active. The brightest source near the center of the frame is known as IC 10 X-1, the changes in its brightest are caused by eclipses of the black hole by its huge companion star. Changes in the field of view are caused by the changing orientation of Chandra, which always keeps its solar panels aligned to the Sun. Only the brighter X-ray sources are visible in this processing.

A Quick Look at IC 10
(Credit: NASA/CXC/A. Hobart)
[Runtime: 1:06]

IC 10 is a galaxy about 2.2 million light years from Earth undergoing a period of intense star formation.

Observations with the Chandra X-ray Observatory reveal over 100 sources that glow in X-rays.

Of these, about a dozen are systems where a black hole or neutron star is in orbit with a young, massive companion star.

These systems, called X-ray binaries, are interesting because some of them could become sources of gravitational waves in the future.

Astronomers using Chandra and other telescopes will continue to study X-ray binaries to better understand how they behave.

Return to IC 10 (August 10, 2017)