Produced by: Manoj Kumar
Despite being 27% of the universe, dark matter eludes direct detection, only seen through its gravitational pull.
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Invisible to light and unable to reflect or absorb it, dark matter hides in plain sight, influencing galaxies without leaving a trace.
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Researchers analyze how galaxies rotate and behave to track dark matter’s gravitational footprint, revealing hidden forces shaping cosmic structures.
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Using cutting-edge infrared spectrographs on the Magellan Clay Telescope, scientists hunt dark matter traces in distant galaxies.
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Infrared analysis of Leo V and Tucana II galaxies lets scientists separate dark matter signals from cosmic noise like zodiacal light, enhancing search precision.
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Advanced detectors filter through atmospheric interference to isolate potential dark matter decay light, marking a leap in cosmic observation technology.
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Studying axionlike particles, researchers set new lifetime limits—over 10 million to 100 million times older than the universe—redefining dark matter boundaries.
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Though direct detection failed, new lifetime estimates for dark matter particles narrow the search field and sharpen future experimental focus.
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Next-gen telescopes like James Webb will join the quest, pushing past current detection limits to reveal dark matter’s hidden form.
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