NASA's Chandra X-ray Observatory has released a groundbreaking video that shows the evolution of Kepler's Supernova Remnant over more than two and a half decades. This remarkable footage is made possible by the longevity of Chandra, which has been capturing data since 1999.
The video, featuring X-ray data from 2000, 2004, 2006, 2014, and 2025, offers a unique glimpse into the history of Kepler's star, which exploded in 1604. Scientists believe that this Type Ia supernova was caused by a white dwarf star exceeding its critical mass, pulling material from a companion star or merging with another white dwarf.
The remnant, located about 17,000 light-years from Earth, is visible as a cloudy neon blue ring with a diagonal cross line stretching across it. The video shows the ring expanding over time, like a slowly inflating balloon, with the bottom of the remnant growing faster than the top. This difference in speed suggests that the gas being plowed into the remnant at the bottom is denser than the gas at the top.
Researchers used this data to gain insights into the environment into which Kepler's star exploded and how remnants change over time. By analyzing the widths of the rims forming the blast wave of the explosion, scientists can learn more about both the explosion itself and its surroundings.
"This video is a game-changer for our understanding of supernovae," said Jessye Gassel, a graduate student at George Mason University who led the research team. "We're not just watching a star's remains expand; we're witnessing the very fabric of space-time being reshaped."
The findings from this study will contribute to NASA's mission to understand our cosmic history and the lifeblood of new stars and planets.
To learn more about Chandra, visit: https://science.nasa.gov/chandra
Or explore the full story here: https://www.nasa.gov/chandra
The video, featuring X-ray data from 2000, 2004, 2006, 2014, and 2025, offers a unique glimpse into the history of Kepler's star, which exploded in 1604. Scientists believe that this Type Ia supernova was caused by a white dwarf star exceeding its critical mass, pulling material from a companion star or merging with another white dwarf.
The remnant, located about 17,000 light-years from Earth, is visible as a cloudy neon blue ring with a diagonal cross line stretching across it. The video shows the ring expanding over time, like a slowly inflating balloon, with the bottom of the remnant growing faster than the top. This difference in speed suggests that the gas being plowed into the remnant at the bottom is denser than the gas at the top.
Researchers used this data to gain insights into the environment into which Kepler's star exploded and how remnants change over time. By analyzing the widths of the rims forming the blast wave of the explosion, scientists can learn more about both the explosion itself and its surroundings.
"This video is a game-changer for our understanding of supernovae," said Jessye Gassel, a graduate student at George Mason University who led the research team. "We're not just watching a star's remains expand; we're witnessing the very fabric of space-time being reshaped."
The findings from this study will contribute to NASA's mission to understand our cosmic history and the lifeblood of new stars and planets.
To learn more about Chandra, visit: https://science.nasa.gov/chandra
Or explore the full story here: https://www.nasa.gov/chandra