How Close Can You Safely Study a Black Hole?

In summary, the radius of a black hole, known as the event horizon, is determined by the mass of the black hole and the speed of light according to Einstein's general theory of relativity. A person wishing to study black holes at a distance of 50 times the event horizon's radius must take into account the difference in gravitational acceleration at their feet and head, with a maximum difference of 10 m/s^2. This leads to a complex equation to determine the maximum mass of the black hole that the person can tolerate at this distance.
  • #1
juliusqueezer
2
0

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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  • #2
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:

[tex] Fg_{feet} = \frac{GMm}{r^2} [/tex],

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

[tex] Fg_{head} = \frac{GMm}{(r+1.7)^2} [/tex]

The problem has said they wish to study at a distance of [itex]50 R_h[/itex]. 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.
 
  • #3
In the above formulae, the accn due to gravity is just GM/r^2. The 'm' is not necessary.
 
  • #4
thanks for all the help. Eventually it came down to Afeet-Ahead=10. It ended in a massive equation with a lot of arithmetic.
 

FAQ: How Close Can You Safely Study a Black Hole?

What is the force of gravity (Fg)?

The force of gravity, commonly referred to as Fg, is a fundamental force in nature that describes the attractive force between two objects with mass. It is responsible for keeping objects, such as planets, in orbit around larger bodies, such as stars.

How does Fg affect planetary motion?

Fg plays a crucial role in planetary motion as it is the force that keeps planets in orbit around the sun. Without Fg, planets would fly off into space in a straight line. The strength of Fg depends on the masses of the two objects and the distance between them.

What is the difference between Fg and centripetal force?

Fg is the force of gravity between two objects, while centripetal force is a force that acts towards the center of a circular motion. Fg is responsible for keeping objects in orbit, while centripetal force is responsible for keeping objects moving in a circular path.

How does the distance between two objects affect Fg?

The force of gravity is inversely proportional to the square of the distance between two objects. This means that as the distance between two objects increases, the force of gravity decreases. This is why planets in our solar system experience a weaker Fg from the sun compared to planets in other solar systems.

What is the relationship between Fg and the mass of an object?

The force of gravity is directly proportional to the masses of the two objects. This means that as the mass of one object increases, the force of gravity between that object and another object also increases. This is why larger planets, such as Jupiter, have a stronger Fg compared to smaller planets, such as Earth.

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