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M≈4×106 M⊙M\approx4\times10^6\,M_\odot

Why this formula appears here

To make this concrete rather than asymptotic, take the mass of Sagittarius A* as measured by the Event Horizon Telescope, M≈\approx4×\times10^6\,M⊙M_\odot , giving a Schwarzschild radius rsr_s≈\approx1.18×\times10^{10}\,m\mathrm m and a horizon-scale acceleration factor GM/rs2r_s^2≈\approx3.80×\times10^{6}\,m s−2\mathrm{m\,s^{-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≈\approx8.46×\times10^{-8} and the required proper acceleration is already a≈\approx1.3×\times10^{10}\,m s−2\mathrm{m\,s^{-2}} , more than a billion Earth gravities. Even at a clearance of 1.8×\times10^6\,km\mathrm{km} — about fifteen percent of the horizon’s own…

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MM

Symbol M

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M⊙M_\odot

Symbol M_odot

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Published contexts (1)

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M≈4×106 M⊙M\approx4\times10^6\,M_\odot

Equation 64 · Evolutionary Physics

A Horizon Is a Toll Booth, Not a Loophole

This mathematical expression combines the displayed quantities; its precise role follows from the surrounding article text.

To make this concrete rather than asymptotic, take the mass of Sagittarius A* as measured by the Event Horizon Telescope, M≈\approx4×\times10^6\,M⊙M_\odot , giving a Schwarzschild radius rsr_s≈\approx1.18×\times10^{10}\,m\mathrm m and a horizon-scale acceleration factor GM/rs2r_s^2≈\approx3.80×\times10^{6}\,m s−2\mathrm{m\,s^{-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≈\approx8.46×\times10^{-8} and the required proper acceleration is already a≈\approx1.3×\times10^{10}\,m s−2\mathrm{m\,s^{-2}} , more than a billion Earth gravities. Even at a clearance of 1.8×\times10^6\,km\mathrm{km} — about fifteen percent of the horizon’s own…

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