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Recent Podcast
A Tour of The Big, Bad & Beautiful Universe with Chandra
A Tour of The Big, Bad & Beautiful Universe with Chandra
To celebrate the 15th anniversary of NASA's Chandra X-ray Observatory, we have released four new images of supernova remnants. These show Chandra's ability to study the remains of supernova explosions, using images that are the sharpest available in X-ray astronomy. The images of the Tycho and G292.0+1.8 supernova remnants show how Chandra can trace the expanding debris of an exploded star. The images show shock waves, similar to sonic booms from a supersonic plane, that travel through space at speeds of millions of miles per hour. The images of the Crab Nebula and 3C58 show the effects of very dense, rapidly spinning neutron stars created when a massive star explodes. These neutron stars can create clouds of high-energy particles that glow brightly in X-rays. The image for G292 shows oxygen (yellow and orange), and other elements such as magnesium (green) and silicon and sulfur (blue) that were forged in the star before it exploded. For the other images, the lower energy X-rays are shown in red and green and the highest energy X-rays are shown in blue. (2014-07-22)


Star (X-ray) Light, Star (X-ray) Bright

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NASA: We have booster ignition and liftoff of Columbia, reaching new heights for women and X-ray Astronomy.

Martin Elvis: The main thing Chandra does is take these superb, sharp images.

Narrator: Remember the line from the children's saying that goes: "Starlight, star bright, first star I see tonight"? Looking at the light from stars is exactly how astronomers can learn about them. But, stars do not just off so-called visible light, the type we can see with the human eye. Rather, astronomers need to study stars in many different types of radiation to get a complete picture of what is really happening of them.

Dr. Nancy Brickhouse studies stars with the Chandra X-ray Observatory and other telescopes and instruments. She explains some of the basics of what stars are.

Nancy: A star is a ball of hot gas and in the center it's very, very dense and in the center a star is producing nuclear fusion reactions, and that's basically what makes the star hot. As you go out into the atmosphere of the star, eventually you reach what we call the photosphere which is the surface of the star. The visible light color of the star is actually coming from the photosphere.

Narrator: But, even though that might sound straightforward, there's really nothing simple about stars. To begin with, there are many different kinds of stars: huge red stars called red giants, small hot white stars called white dwarfs, small cool brown stars called brown dwarfs, and more. Dr. Brickhouse explains how astronomers can keep track and X-rays are used to help categorize these very different objects.

Nancy: Stars have a temperature that's related to the color of the star so the blue stars are hotter than the yellow and red stars, and so we have a classification scheme that's going from hot to cool and the sun is considered to be a cool star. And this is based on their visible light properties. The color is basically related to the color of the photosphere. When we look at these stars in X-rays we're looking above that surface, so we're looking higher up in the atmosphere of the star, where the gas is really not as dense, but it's much hotter. And it turns out that both hot stars and cool stars make X-rays but the processes are different. So when we look at cool stars we're looking at processes that are more like the Sun.

Narrator: But where does our Sun fit into the scheme of things? What does Chandra and its X-ray data tell us about our nearest star?

Nancy: We can look at the Sun with other satellites and there have been X-ray missions for just studying the sun, but it would wipe out Chandra's detectors if we used Chandra to look at the Sun, but we can study other stars and it turns out that 10 to a hundred thousand times more energy is produced in X-rays than what the sun produces, so by the standards of other stars, the Sun is kind of a wimpy X-ray producer.

Narrator: So, astronomers can't use Chandra to study our Sun directly. But, what kind of insight do astronomers actually get by studying other Sun-like stars using Chandra. It turns out to be a very valuable thing to do.

Nancy: One of the reasons to look at other stars is to get some understanding of what the processes are that cause the X-ray emission and what kind of diversity there might be because it will help our models if we just have one system to look at even though we can look at it in a lot of detail we don't necessarily understand the possibilities that would help us constrain our models.

Narrator: Studying all kinds of stars - including those like our Sun and those that are very different - remains an important area of research in astronomy and astrophysics. The starlight we wish upon in that rhyme turns out to be much more complicated and informative than we may have ever expected. Researchers using Chandra are helping to address some of questions whose answers may only be found in their X-ray light.

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