Webb sharpens its view of a black hole's dusty feeding disk

JWST’s high-contrast observations of the Circinus galaxy reveal the clearest view yet of the dusty torus feeding its central supermassive black hole. About 87% of the infrared emission comes from the inner disk near the hole, less than 1% from the outflow known as the North Arc, and ~12% from dust farther out. The findings, based on two 2024–2025 Webb observations using a seven‑aperture setup, provide an effective resolution like a 13‑meter telescope and challenge decades of outflow‑driven infrared models, confirming the torus as the primary fuel reservoir for black hole growth. The study was published Jan. 13 in Nature Communications.