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Polarized Emissions from an Extragalactic Black Hole

Santhosh Kumar 20/11/2023
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Polarized Emissions from an Extragalactic Black Hole upsc mind map Groundbreaking discovery By Indian Institute of Technology Guwahati and ISRO Detection of polarized emissions From extragalactic black hole In Large Magellanic Cloud X-3 Binary star system Comprising Black hole Normal star Hotter and larger than Sun Discovered in 1971 200,000 light-years away X-ray polarimetry Analyzes polarization properties Offers insights into Matter drawn toward black holes Accretion process Technology and tools used The Imaging X-ray Polarimetry Explorer (IXPE) NASA mission Neutron Star Interior Composition Explorer (NICER) Nuclear Spectroscopic Telescope Array (NuSTAR) Constraining black hole spin Significance X-ray polarimetry Identifies radiation source near black holes Explains effect of gravitational fields Polarization of emitted light Observations LMC X-3 emits powerful X-rays 10,000 times more than Sun Likely harbors Black hole with low rotation rate Surrounded by slim disc structure Glossary Accretion Process of matter accumulation Black hole Dense astronomical object with strong gravity X-ray polarimetry Study of polarization in X-ray light

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