NASA telescope uncovers new mystery in supernova first spotted by Chinese astronomers 2,000 years ago —‬ Space photo of the week

NASA's Imaging X-ray Polarimetry Explorer observed the outer rim of the supernova remnant highlighted in purple in the inset. (Image credit: X-ray: Chandra: NASA/CXC/SAO, XMM: ESA/XMM-NEWTON, IXPE: NASA/MSFC; Optical: NSF/NOIRLab; Image Processing: NASA/CXC/SAO/J. Schmidt) Copy link Facebook X Whatsapp Reddit Pinterest Flipboard Email Share this article 0 Join the conversation Follow us Add us as a preferred source on Google Newsletter Sign up for the Live Science daily newsletter now Get the world’s most fascinating discoveries delivered straight to your inbox. By submitting your information you agree to the Terms & Conditions and Privacy Policy and are aged 16 or over. You are now subscribed Your newsletter sign-up was successful Want to add more newsletters? Join the club Get full access to premium articles, exclusive features and a growing list of member rewards. Explore An account already exists for this email address, please log in. Subscribe to our newsletter Quick facts What it is: RCW 86, a supernova remnant Where it is: 8,000 light-years away, in the constellation Circinus When it was shared: March 24, 2026 One of the oldest recorded astronomical events observed by humans has gotten a fresh look from a new NASA space telescope. In A.D. 185, Chinese astronomers recorded the appearance of a "guest star" in the night sky. The star shone for about eight months in the direction of Alpha Centauri, one of the closest star systems to the sun. This stellar visitor was a supernova — a large and extremely bright explosion marking the end of a massive star's life. It left a remnant — a ring of glowing debris — in the night sky that's now known as RCW 86. It's all that remains of the exploded white dwarf star, but there's a mystery surrounding it: why it appears to have expanded far more quickly than other supernova remnants. Although RCW 86 has been imaged many times before — notably by NASA's Chandra X-ray Observatory and the Dark Energy Camera — new data from NASA's Imaging X-ray Polarimetry Explorer (IXPE) has delivered a fresh perspective. Launched in 2021, IXPE captures X-ray data and high-energy, short-wavelength light with an all-new level of sensitivity to examine the most extreme objects in the universe, including supernova remnants. IXPE was put to work on RCW 86 because of the remnant's irregular shape and the strange way it's expanding. Earlier observations from Chandra suggested that the supernova spread into a low-density "cavity," allowing it to grow faster than other supernova remnants. This image combines data from IXPE, Chandra and the European Space Agency 's XMM-Newton telescope, with low-energy X-rays shown in yellow and higher-energy emissions in blue. IXPE's data is crucial because it can highlight polarized X-ray emissions, revealing magnetic-field structures in the remnant's outer rim. This region, marked in purple, is particularly significant because it shows where the supernova's expansion likely slowed at the edge of the