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Hubble finds most distant supernova yet

Images, taken in near-infrared light demonstrate how the astronomers found the supernova. The image at far left shows the host galaxy without the supernova; the middle image, taken a year earlier, reveals the galaxy with the supernova. The supernova cannot be seen because it is too close to the center of its host galaxy. To detect the supernova, astronomers subtracted the left image from the middle image to see the light from the supernova, shown in the image at far right. Credit: NASA, ESA, A. Riess (STScI and JHU), and D. Jones and S. Rodney (JHU)
Images, taken in near-infrared light demonstrate how the astronomers found the supernova. The image at far left shows the host galaxy without the supernova; the middle image, taken a year earlier, reveals the galaxy with the supernova. The supernova cannot be seen because it is too close to the center of its host galaxy. To detect the supernova, astronomers subtracted the left image from the middle image to see the light from the supernova, shown in the image at far right. Credit: NASA, ESA, A. Riess (STScI and JHU), and D. Jones and S. Rodney (JHU)

GREENBELT, Md., April 4 (UPI) -- The Hubble telescope has found the farthest supernova ever detected, a cosmic "tape measure" to help astronomers gauge the size of the universe, NASA says.

Supernova UDS10Wil, which exploded more than 10 billion years ago, belongs to a special class called Type Ia supernovae, a kind of light beacon prized by astronomers because they provide a consistent level of brightness that can be used to measure the expansion of space, the space agency reported Thursday.

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Although the newly discovered supernova is only 4 percent more distant than the previous record holder, it pushes roughly 350 million years farther back in time to a period when the universe was in its early formative years and stars were being born at a rapid rate, astronomers said.

"This new distance record holder opens a window into the early universe, offering important new insights into how these stars explode," astronomer David O. Jones of Johns Hopkins University in Baltimore said.

Knowing what triggers Type Ia supernovae will provide evidence of how quickly the Universe enriched itself with heavier elements such as iron. These exploding stars produce about half of the iron in the universe, the raw material for building planets and life.

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"We can test theories about how reliable these detonations are for understanding the evolution of the universe and its expansion," Jones said of the latest discovery.

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