How Close Can You Safely Study a Black Hole?

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Homework Help Overview

The discussion revolves around the gravitational effects experienced by a person studying black holes, specifically focusing on the difference in gravitational acceleration between their feet and head when positioned at a certain distance from the black hole. The context is rooted in general relativity and involves calculations related to the event horizon of black holes.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss how to calculate the gravitational acceleration at different heights of the person, questioning how to incorporate the difference in acceleration into their calculations. There is an exploration of the relationship between the mass of the black hole and the radial distance from it.

Discussion Status

Some participants have provided insights into the gravitational formulas and how to set up the problem, while others are still grappling with the implications of the acceleration difference. There is an acknowledgment of the complexity involved in the calculations, but no consensus has been reached on a definitive approach.

Contextual Notes

The problem imposes a specific constraint on the maximum allowable difference in gravitational acceleration (10 m/s²) and specifies the height of the individual (1.7 m), which are central to the discussion.

juliusqueezer
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Homework Statement



The radius Rh of a black hole is the radius of a mathematical sphere, called the event horizon, that is centered on the black hole. Information from events inside the event horizon cannot reach the outside world. According to Einstein's general theory of relativity, Rh = 2GM/c^2, where M is the mass of the black hole and c is the speed of light. Suppose that a person who is 1.7 m tall wishes to study black holes near them, at a radial distance of 50Rh. However, the person doesn't want the difference in gravitational acceleration between their feet and head to exceed dag = 10 m/s^2 when they are feet down (or head down) toward the black hole.

(a) As a multiple of our sun's mass, what is the limit to the mass of the black hole the person can tolerate at the given radial distance?


Homework Equations


Rh=(2GM)/c^2
Fg=G((Mm)/r^2)

The Attempt at a Solution



I can solve for Rh and eventually get a mass, but that in no way accounts for the acceleration difference of the person. My question is, how must I account for this?
 
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Hello,

Well, the problem states that the person is 1.7m tall. So the person is going to experience some acceleration due to gravity at their feet:

Fg_{feet} = \frac{GMm}{r^2},

and some different acceleration due to gravity at their head, which is further away, if they are feet first:

Fg_{head} = \frac{GMm}{(r+1.7)^2}

The problem has said they wish to study at a distance of 50 R_h. You need to find the maximum mass of the black hole, that will not create more than a 10 m/s^2 difference in accelerations, above.

Hope this helps.
 
In the above formulae, the accn due to gravity is just GM/r^2. The 'm' is not necessary.
 
thanks for all the help. Eventually it came down to Afeet-Ahead=10. It ended in a massive equation with a lot of arithmetic.
 

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