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S301

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S301: The Milky Way's Fastest Star Offers a Decade-Long Path to Measuring Black Hole Spin
astronomy1 month ago

S301: The Milky Way's Fastest Star Offers a Decade-Long Path to Measuring Black Hole Spin

Astronomers have identified S301, a faint star on the shortest known orbit around the Milky Way's central black hole, Sagittarius A*. With an 8.7-year period and pericentre speed exceeding 8% of light speed, S301 passes roughly ten times closer to the black hole than the previously known record holder, S2. While current data confirm general relativistic precession, the star's extreme proximity offers a unique opportunity to measure the black hole's spin within the next decade, provided future instruments achieve the required precision.

S301: The Milky Way’s Fastest Star Offers a New Window into Black Hole Spin
science2 months ago

S301: The Milky Way’s Fastest Star Offers a New Window into Black Hole Spin

Astronomers have identified S301, a faint star orbiting the Milky Way’s central black hole, Sagittarius A*, at record-breaking speeds. With an 8.7-year orbital period and a peak velocity of 25,000 km/s (8% the speed of light), S301 passes closer to the black hole than any previously observed star. This extreme proximity allows scientists to test Einstein’s general relativity and potentially measure the black hole’s spin within the next decade, a feat previously thought to require decades of observation.

Relativity Goes Extreme: Star S301 Dances Close to the Milky Way’s Black Hole
space3 months ago

Relativity Goes Extreme: Star S301 Dances Close to the Milky Way’s Black Hole

Astronomers have found star S301, a Sun-like star in the highly elliptical 8.7-year orbit around the Milky Way’s central supermassive black hole Sag A*, approaching within about 24 AU at closest approach and reaching speeds near 0.08c. The orbit shows relativistic precession of about 2° per pass, along with gravitational redshift and transverse Doppler effects, enabling tests of general relativity and potential constraints on alternative gravity theories. While dust and faintness hinder spectral data today, future observatories like the Giant Magellan Telescope could measure higher-order relativistic effects, further probing gravity near a black hole.