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(c) Typically, black holes catch stars rather than people. Find the distance from the black hole at which a star of mass m and radius r will be disrupted by tidal forces, assuming that the two halves of the star are held together by gravity Use your result to check whether a 1M star will get disrupted before it plunges through the horizon of a 10 M black hole. (If the disruption occurs inside the horizon, there will be no visible effect, since any emission produced during this event will not make it out of the black hole.)

(c) Typically, black holes catch stars rather than people. Find the distance from the black hole at which a star of mass m and radius r will be disrupted by tidal forces, assuming that the two halves of the star are held together by gravity Use your result to check whether a 1M star will get disrupted before it plunges through the horizon of a 10 M black hole. (If the disruption occurs inside the horizon, there will be no visible effect, since any emission produced during this event will not make it out of the black hole.)

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(c) Typically, black holes catch stass rather than people. Find the distance from the black hole at which a star of massmand rudiusrwill be disrupted by tidal forces, assuming that the two halves of the star are helil togegther hy gravity Ifse your mesult. to rherk whother a1M0​s star will get disnupted before t plunges through the horizon of a108Mg​black hole. (If the disruption occurs inside the horizon, there will be no visible effect, since any enission produced during this event will not make it out of the black hole.)

(c) Typically, black holes catch stars rather than people. Find the distance from the black hole at which a star of mass m and radius r will be disrupted by tidal forces, assuming that the two halves of the star are held together by gravity Use your result to check whether a 1M star will get disrupted before it plunges through the horizon of a 10 Mg, black hole. (If the disruption occurs inside the horizon, there will be no visible effect, since any emission produced during this event will not make it out of the black hole.)
Transcribed Image Text:(c) Typically, black holes catch stars rather than people. Find the distance from the black hole at which a star of mass m and radius r will be disrupted by tidal forces, assuming that the two halves of the star are held together by gravity Use your result to check whether a 1M star will get disrupted before it plunges through the horizon of a 10 Mg, black hole. (If the disruption occurs inside the horizon, there will be no visible effect, since any emission produced during this event will not make it out of the black hole.)
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