X-ray Images
Chandra Mission
X-ray Astronomy
Chandra People
Chandra in HD
Standard Definition
The Invisible Sky
Two Inch Universe
By Date/Category
Other Features
Animations & Video
Special Features
3D Files and Resources
Q & A
Acronym Guide
Further Reading
Desktop Images
iPhone Wallpapers
By Date/Category
Image Handouts
Chandra Lithographs
Chandra Infographics
Educational Activities
Printable Games
Chandra Fact Sheets
Entire Collection
By Date
By Category
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
Problems Viewing?
Having trouble viewing a movie? Make sure you update your video plug-ins. Visit our download center for help.
More Information
Quasars & Active Galaxies
X-ray Astronomy Field Guide
Quasars & Active Galaxies
Questions and Answers
Quasars & Active Galaxies
Chandra Images
Quasars & Active Galaxies
Animations & Video: Quasars & Active Galaxies
Page 12345
Click for high-resolution animation
1. A Tour of RGG 118
QuicktimeMPEG Oxymorons are often thought of as gaffes in language, but a new black hole discovery shows they can also represent important scientific advances. Astronomers using NASA's Chandra X-ray Observatory and the 6.5-meter Clay Telescope in Chile have identified the smallest giant black hole known. This oxymoronic object could provide clues to how much larger black holes formed along with their host galaxies billion of years in the past.

Astronomers estimate this supermassive black hole is about 50,000 times the mass of the Sun. This is less than half the previous lowest mass for a black hole at the center of a galaxy. The tiny heavyweight black hole is located at the center of a dwarf disk galaxy, called RGG 118, about 340 million light years from Earth.

Researchers estimated the mass of the black hole by studying the motion of cool gas near the center of the galaxy using visible light data from the Clay Telescope. They used the Chandra data to figure out the brightness in X-rays of hot gas swirling toward the black hole. They found that the outward push of radiation pressure of this hot gas is about 1% of the black hole's inward pull of gravity. This matches the properties of other supermassive black holes.

The black hole in RGG 118 is nearly 100 times less massive than the supermassive black hole found in the center of the Milky Way. It is also about 200,000 times less massive than the heaviest black holes found in the centers of other galaxies.

Researchers will keep looking for other supermassive black holes that are comparable in size or even smaller than the one in RGG 118. It is important to gather a large sample because black holes of this size might be seeds that lead to the formation of much larger supermassive black holes.
[Runtime: 02:10]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
2. Tour of Space-time Foam
QuicktimeMPEG At the smallest scales of distance and duration that we can measure, space-time - that is, the three dimensions of space plus time - appears to be smooth and structureless. Think of flying over the ocean in an airplane. From 30,000 feet or so, the ocean appears completely smooth. However, if your plane were to descend low enough, you could make out the waves and swells of the water. Certain aspects of quantum mechanics, the highly successful theory scientists have developed to explain the physics of atoms and subatomic particles, predict that space-time may act the same way. Instead of being totally smooth, it would have a foamy, jittery nature if we could look at small enough scales -- like those waves on the ocean. In these models, space-time would consist of many small, ever-changing, regions for which space and time are constantly fluctuating.

Since space-time foam, as it is called, is so tiny, scientists cannot observe it directly. However, they can hunt for evidence for its existence - or non-existence - in things we can see. By looking at the light from distant quasars in X-rays from Chandra as well as gamma-ray telescopes, a team of scientists set out to test some of the models of space-time foam.

What did they find? The researchers say their evidence can help rule out two different models of space-time foam. While their work does not eliminate the existence of space-time foam entirely, it does suggest that space-time is less foamy than some models predict. Scientists will continue to test the nature of space and time on the very smallest scales using every experiment they can think of, including using high-energy light from across the Universe.
[Runtime: 02:02]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
3. Tour of 3 Quasars
QuicktimeMPEG A group of unusual giant black holes may be consuming excessive amounts of matter, according to a new study using NASA's Chandra X-ray Observatory. This finding may help astronomers understand how the largest black holes were able to grow so rapidly in the early Universe.

Astronomers have known for some time that supermassive black holes - with masses ranging from millions to billions of times the mass of the Sun and residing at the centers of galaxies - can gobble up huge quantities of gas and dust that have fallen into their gravitational pull. As the matter falls towards these black holes, it glows with such brilliance that they can be seen billions of light years away. Astronomers call these extremely ravenous black holes "quasars."

This new result suggests that some quasars are even more adept at devouring material than previously thought, about five to ten times the rate of typical quasars. A team of astronomers examined data from Chandra for 51 quasars that are located at a distance between about 5 billion and 11.5 billion light years from Earth. Based on their findings, the researchers think some of these quasars contain black holes that are surrounded by a thick, donut-shaped disk of material. This torus would block much of the light - including X-rays and ultraviolet light -- that would otherwise be observed by Chandra and other telescopes. The important implication for these thick-disk quasars is that they may be harboring black holes that are growing an extraordinarily rapid rate.
[Runtime: 01:53]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
4. The Most Attractive Stars in the Universe
QuicktimeMPEG Have you ever played with magnets? You might have done an experiment where you lay a magnet onto a table and place an iron nail nearby. If you push the magnet slowly toward the nail, there will come a point when the nail jumps across and sticks to the magnet. That's because magnets have something invisible that extends all around them, called a 'magnetic field'. It can cause a pushing or pulling force on other objects, even if the magnet isn't actually touching them.

The most powerful magnets in the Universe are called magnetars. These are tiny, super-compact stars, 50 times more massive than our Sun, squashed into a ball just 20 kilometers across. (That's about the size of a small city!)

Astronomers think magnetars may be created when some massive stars die in a supernova explosion. The star's gases blow out into space creating a colourful cloud like the one in this picture, called Kes 73. At the same time, the core of the star squashes down to form a magnetar.

At the center of the cosmic cloud in this photograph lies a tiny magnetar. But what this star lacks in size it makes up for in energy, shooting out powerful jets of X-rays every few seconds! You can see the X-ray jets in blue in this photograph.
[Runtime: 02:04]
(NASA/CXC/April Jubett)

Related Chandra Images:

Click for high-resolution animation
5. A Tour of IYL 2015
QuicktimeMPEG The year of 2015 has been declared the International Year of Light, or IYL for short, by the United Nations. Organizations, institutions, and individuals involved in the science and applications of light will be joining together for this year-long celebration to help spread the word about the wonders of light.

In many ways, astronomy uses the science of light. By building telescopes that can detect light in its many forms from radio waves on one end of the "electromagnetic spectrum" to gamma rays on the other, scientists can get a better understanding of the processes at work in the Universe.

NASA's Chandra X-ray Observatory explores the Universe in X-rays, a high-energy form of light. By studying X-ray data and comparing them with observations in other types of light, scientists can develop a better understanding of objects that generate temperatures of millions of degrees and produce X-rays.

To recognize the start of IYL, the Chandra X-ray Center is releasing a collection of images that combine data from telescopes tuned to different wavelengths of light. From a distant galaxy to the relatively nearby debris field of an exploded star, these images demonstrate the myriad ways that information about the Universe is communicated to us through light.

So join us in celebrating IYL and all of the amazing things that light can do, including how it helps us understand the Universe we live in.
[Runtime: 01:58]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
6. Chandra's Archives Come to Life
QuicktimeMPEG Every year, NASA's Chandra X-ray Observatory looks at hundreds of objects throughout space to help expand our understanding of the Universe. Ultimately, these data are stored in the Chandra Data Archive, an electronic repository that provides access to these unique X-ray findings for anyone who would like to explore them. With the passing of Chandra's 15th anniversary, in operation since August 26, 1999, the archive continues to grow as each successive year adds to the enormous and invaluable dataset.

To celebrate Chandra's decade and a half in space, and to honor October as American Archive Month, a variety of objects have been selected from Chandra's archive. Each of the new images we have produced combines Chandra data with those from other telescopes. This technique of creating "multiwavelength" images allows scientists and the public to see how X-rays fit with data of other types of light, such as optical, radio, and infrared. As scientists continue to make new discoveries with the telescope, the burgeoning archive will allow us to see the high-energy Universe as only Chandra can.
[Runtime: 01:27]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
7. Tour of NGC 4258 (M106)
QuicktimeMPEG NGC 4258, also known as Messier 106, is a spiral galaxy like the Milky Way. This galaxy is famous, however, for something that our Galaxy doesn’t have – two extra spiral arms that glow in X-ray, optical, and radio light. These features, or anomalous arms, are not aligned with the plane of the galaxy, but instead intersect with it. The X-ray image from Chandra reveals huge bubbles of hot gas above and below the plane of the galaxy. These bubbles indicate that much of the gas that was originally in the disk of the galaxy has been heated to millions of degrees and ejected into the outer regions by the jets from the black hole. The ejection of gas from the disk by the jets has important implications for the fate of this galaxy. Researchers estimate that all of the remaining gas will be ejected within the next 300 million years -- very soon on cosmic time scales – unless it is somehow replenished. Without this gas, relatively few stars can form there. In fact, scientists estimate that that star formation in the central region of NGC 4258 is already being choked off, with stars forming at a rate ten times less than in the Milky Way galaxy.
[Runtime: 01:42]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
8. Tour of RX J1131-1231
QuicktimeMPEG Black holes seem like such mysterious and complicated objects. On one hand, they are, and astronomers have been studying them for decades to learn more. On the other, black holes are actually quite simple. By this, we mean that black holes are defined by just two simple characteristics: their mass and their spin. While astronomers have long been able to measure black hole masses very effectively, determining their spins has been much more difficult. A new result from researchers using data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton takes a step in addressing the spin question. By a lucky alignment, the light from a quasar some 6 billion light years has been magnified and amplified due to an effect called gravitational lensing. This allowed researchers to get detailed information about the amount of X-rays seen at different energies. This, in turn, gave the researchers information about how fast the supermassive black hole at the center of the quasar is spinning. When combined with the spins from other black holes using more indirect methods, astronomers are beginning to better understand just how black holes grow over time across the Universe.
[Runtime: 01:30]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
9. A New Look at an Old Friend
QuicktimeMPEG Just weeks after NASA's Chandra X-ray Observatory began operations in 1999, the telescope pointed at Centaurus A (Cen A, for short). This galaxy, at a distance of about 12 million light years from Earth, contains a gargantuan jet blasting away from a central supermassive black hole.

Since then, Chandra has returned its attention to this galaxy, each time gathering more data. And, like an old family photo that has been digitally restored, new processing techniques are providing astronomers with a new look at this old galactic friend.

This new image of Cen A contains data from observations, equivalent to over nine and a half days worth of observing time, taken between 1999 and 2012. In this image, the lowest-energy X-rays Chandra detects are in red, while the medium-energy X-rays are green, and the highest-energy ones are blue.

As in all of Chandra's images of Cen A, this one shows the spectacular jet of outflowing material that is generated by the giant black hole at the galaxy's center. The new image also highlights a dust lane that wraps around the waist of the galaxy. Astronomers think this feature is a remnant of a collision that Cen A experienced with a smaller galaxy millions of years ago.

In addition to allowing for the creation of new images, the data housed in Chandra's extensive archive on Cen A provide a rich resource for a wide range of scientific investigations. For example, just last year researchers published new findings on the point-like X-ray sources in Cen A. They found that these sources had masses that fell into two categories. These separate groups correspond to systems where either a neutron star or a black hole is pulling material from a companion star. Information like this may tell us important details about the way the massive stars explode, and gives us even more reason to appreciate this new view of a familiar object.
[Runtime: 02:22]
(NASA/CXC/A. Hobart)

Related Chandra Images:

Click for high-resolution animation
10. The Invisible Universe Exposed

Pictures of space are often gorgeous. But one of the most exciting things about them is that, very often, they show us things that are invisible to the human eye. This picture in particular does that. In the middle of the photograph lurks an invisible monster, called a super-massive black hole To make this invisible object even harder to study, it is hidden under a thick cloud of dust at the centre of its home galaxy! Even the bright blobs of colour you can see are patches of light that our eyes cannot detect naturally. The pink colour shows radio light, and X-rays are shown in blue.

A black hole is anything but empty space, don't let the name fool you. It is a huge amount of material packed into a very tiny area - this one has about 100 million times the mass of our Sun! Anything that wanders too close to a Black Hole is pulled into it with no chance of escape, including light. This is why we cannot see black holes, they are invisible even to telescopes that detect X-rays, radio waves and other types of light.

The only way we can spot black holes is by detecting its effect on other things. For example, in this picture, the brightest blue patches, along the edge of the galaxy reveal where a high-energy jet has ploughed into clumps of galactic dust. The jet was made up of particles that were heated as they were pulled into the black hole. This gave them energy and sent them speeding away from the black hole at millions of miles per hour! Two similar jets can be seen in pink, shooting to the North and South of the galaxy.

[Runtime: 02:12]
(NASA/CXC/April Jubett)

Related Chandra Images:

Page 12345