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James Webb Space Telescope discovers how black holes feed themselves

New observations from the James Webb Space Telescope reveal complex gas recycling processes that fuel supermassive black holes.

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The story so far

The James Webb Space Telescope (JWST) has observed a river of cool gas flowing into an 800-light-year disk at 600 kilometers per second to feed the supermassive black hole within NGC 4696. Coverage from outlets including Space, NASA, and ZME Science indicates that this mechanism involves magnetic gas rivers and internal fuel recycling.

Reports from Tech Times, Space Daily, and Hindustan Times highlight that JWST data also identified a metal-poor, primitive dwarf galaxy producing iron and silicon-carbide dust earlier than previously established models suggested. Scientific analysis associated with the Inter-University Centre for Astronomy and Astrophysics (IUCAA) and UK-based researchers is credited with helping interpret these observations.

Future updates will likely focus on whether these gas-recycling processes are consistent across other supermassive black holes in the early universe. Coverage does not yet specify how these findings will impact existing cosmological models regarding the rate of galactic evolution.

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The obvious questions

What specific black hole behavior did the telescope capture?

The telescope mapped a gas pipeline where cool gas flows into an 800-light-year disk to fuel a supermassive black hole, involving a recycling process.

What was discovered about early galaxies?

JWST identified a metal-poor dwarf galaxy capable of producing iron and silicon-carbide dust, which contradicts previous expectations for early-universe galaxies.

How far away is the observed galaxy NGC 4696?

The galaxy NGC 4696 is located 145 million light-years away.

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