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1.8×106km
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To make this concrete rather than asymptotic, take the mass of Sagittarius A* as measured by the Event Horizon Telescope, M≈4×10^6\,M⊙ , giving a Schwarzschild radius rs≈1.18×10^{10}\,m and a horizon-scale acceleration factor GM/rs2≈3.80×10^{6}\,ms−2 [ 14 ] . At a clearance of just one kilometer above the horizon — a distance smaller than a millionth of the horizon’s own radius — f≈8.46×10^{-8} and the required proper acceleration is already a≈1.3×10^{10}\,ms−2 , more than a billion Earth gravities. Even at a clearance of 1.8×10^6\,km — about fifteen percent of the horizon’s own…
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Equation 69 · Evolutionary Physics
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To make this concrete rather than asymptotic, take the mass of Sagittarius A* as measured by the Event Horizon Telescope, M≈4×10^6\,M⊙ , giving a Schwarzschild radius rs≈1.18×10^{10}\,m and a horizon-scale acceleration factor GM/rs2≈3.80×10^{6}\,ms−2 [ 14 ] . At a clearance of just one kilometer above the horizon — a distance smaller than a millionth of the horizon’s own radius — f≈8.46×10^{-8} and the required proper acceleration is already a≈1.3×10^{10}\,ms−2 , more than a billion Earth gravities. Even at a clearance of 1.8×10^6\,km — about fifteen percent of the horizon’s own…
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