Astronomers See Historical Supernova From a New Angle (w/ Video)

March 31, 2010
Chandra X-ray Observatory image of the supernova remnant Cassiopeia A (Cas A). The red, green, and blue regions in this X-ray image of Cas A show where the intensity of low, medium, and high-energy X-rays, respectively, is greatest. While this photo shows the remains of the exploded star, light echoes show us reflected light from the explosion itself. Credit: NASA/CXC/MIT/UMass Amherst/M.D.Stage et al.

( -- Since Galileo first pointed a telescope at the sky 400 years ago, a myriad of technological advances have allowed astronomers to look at very faint objects, very distant objects, and even light that's invisible to the human eye. Yet, one aspect usually remains out of reach - the benefit of a 3-D perspective.

Our telescopes show the Milky Way galaxy only as it appears from one vantage point: our solar system. Now, using a simple but powerful technique, a group of astronomers led by Armin Rest of Harvard University has seen an or supernova from several angles.

"The same event looks different from different places in the Milky Way," said Rest. "For the first time, we can see a supernova from an alien perspective."

The supernova left behind the gaseous remnant . The supernova's light washed over the Earth about 330 years ago. But light that took a longer path, reflecting off clouds of interstellar dust, is just now reaching us. This faint, reflected light is what the astronomers have detected.

The technique is based on the familiar concept of an echo, but applied to light instead of sound. If you yell, "Echo!" in a cave, sound waves bounce off the walls and reflect back to your ears, creating echoes. Similarly, light from the supernova reflects off interstellar dust to the Earth. The acts like a mirror, creating light echoes that come from different directions depending on where the clouds are located.

"Just like mirrors in a changing room show you a clothing outfit from all sides, clouds act like mirrors to show us different sides of the supernova," explained Rest.

Moreover, an audible echo is delayed since it takes time for the sound waves to bounce around the cave and back. Light echoes also are delayed by the time it takes for light to travel to the dust and reflect back. As a result, light echoing from the supernova can reach us hundreds of years after the supernova itself has faded away.

Not only do light echoes give astronomers a chance to directly study historical supernovae, they also provide a 3-D perspective since each echo comes from a spot with a different view of the explosion.

Three light echoes from the Cas A supernova are shown here in three rows. For each row, the left panel is a reference image while the middle panel shows the same field of view at a later time. Right panels show the difference between the two previous shots, highlighting the (changing) light echo. The position and size of the spectroscopy slit is indicated by the rectangular overlay. For all images, north is up and east is to the left. Credit: CfA/KPNO

Most people think a supernova is like a powerful fireworks blast, expanding outward in a round shell that looks the same from every angle. But by studying the light echoes, the team discovered that one direction in particular looked significantly different than the others.

They found signs of gas from the stellar explosion streaming toward one point at a speed almost 9 million miles per hour (2,500 miles per second) faster than any other observed direction.

"This supernova was two-faced!" said Smithsonian co-author and Clay Fellow Ryan Foley. "In one direction the exploding star was blasted to a much higher speed."

Previous studies support the team's finding. For example, the neutron star created when the star's core collapsed is zooming through space at nearly 800,000 miles per hour in a direction opposite the unique light echo. The explosion may have kicked gas one way and the neutron star out the other side (a consequence of Newton's third law of motion, which states that every action has an equal and opposite reaction).

By combining the new light-echo measurements and the movement of the neutron star with X-ray data on the supernova remnant, astronomers have assembled a 3-D perspective, giving them new insight into the Cas A supernova.

"Now we can connect the dots from the explosion itself, to the supernova's light, to the remnant," said Foley.

Cassiopeia A is located about 16,000 light-years from Earth and contains matter at temperatures of around 50 million degrees F, causing it to glow in X-rays.

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A 3-D computer model of the remnant. Credit: Visualization: NASA/CXC/D.Berry; Model: NASA/CXC/MIT/T.Delaney et al.

The Mayall 4-meter telescope at Kitt Peak National Observatory was used to locate the light echoes. Follow-up spectra were obtained with the 10-meter Keck I Telescope.

The journal paper describing this discovery is available online.

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5 / 5 (2) Apr 01, 2010
All I can think is, isn't it incredibly beautiful?
(as I play and replay the visualisation)
not rated yet Apr 01, 2010
It will be interesting to see if this technique can be applied to other supernovae remnants in our galaxy or the nearby Magellanic Clouds. Asymmetric detonations seem to better explain observations of certain supernovae, SNRs and GRBs.
not rated yet Apr 07, 2010
Could this technique eventually be evolved to such extend that they can pinpoint some centre of the galaxy? I know the space as it is has only expanded and that each point had always been present, but you could "shrink" the current universe to a set of coordinates currently known and thus creating some kind of "origin".
not rated yet Apr 11, 2010
Could this technique eventually be evolved to such extend that they can pinpoint some centre of the galaxy? I know the space as it is has only expanded and that each point had always been present, but you could "shrink" the current universe to a set of coordinates currently known and thus creating some kind of "origin".

Yes, and no. I assume you mean finding the center of the universe from light echoes of the big bang. There is a remnant, now red-shifted down to microwave frequencies (the cosmic microwave background radiation--CMBR), but it is very symmetric. You can use it to determine the Earth's speed relative to the universe, but there is no center. You can try to impute a velocity relative to the rest of the universe to individual galaxies and galaxy clusters, but the "residual" velocities are small, and mostly due to the gravitational effects of the lumpy universe.

These deviations in the CMBR and red shifts of remote galaxies are in fractions of a percent.

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