The Chandra X-ray Observatory, studying high-energy radiation from a star that periodically dims and brightens, has found evidence suggesting the catastrophic collision of two infant planets, producing a huge cloud of debris, including significant amounts of iron, that would explain the star’s most recent change in intensity.
The star, known as RW Aur A, is located in the Taurus-Auriga constellation some 450 light years from Earth where thousands of young stars blaze in stellar nurseries. RW Aur A fades every few decades and then brightens again, prompting speculation about the effects of dusty clouds of debris orbiting the star, or other, unknown processes going on closer in.
But astronomers using the Chandra X-Ray Observatory to study RW Aur A’s most recent dimming obtained spectra showing significant amounts of iron in the star’s light, indicating the possible collision of two young planets.
“Computer simulations have long predicted that planets can fall...
Read More