Produced by: Manoj Kumar
M87*’s rotational axis points away from Earth, confirmed by multi-year Event Horizon Telescope (EHT) data. The orientation impacts how its luminous ring is observed.
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The accretion disk’s turbulence caused a 30-degree shift in the ring’s brightest region, validating prior predictions about black hole dynamics.
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EHT data from 2017 and 2018 reveal that M87*’s turbulent environment evolves over time, offering a rare glimpse into black hole behavior.
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The black hole’s luminous ring, captured in 2017, remained stable in size at 43 microarcseconds in 2018, consistent with theoretical models.
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Researchers expanded their image simulation library to over 120,000 models, enabling precise analysis of black hole accretion dynamics.
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The plasma around M87* reveals a counter-rotating gas flow, adding new depth to our understanding of accretion variability near black holes.
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The bottom-bright ring suggests M87* spins in a direction aligned opposite to the gas flow, revealing new cosmic alignment mysteries.
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The study advances black hole theories, confirming predictions about their accretion flow and turbulent nature through enhanced observations.
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Analysis of 2021 and 2022 data promises deeper insights, with more robust models expected to refine our understanding of M87*’s turbulent environment.
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