Can an object falling towards a super massive planet reach the speed of light?

Click For Summary

Discussion Overview

The discussion revolves around the question of whether an object falling towards a supermassive planet can reach the speed of light, particularly in the context of general and special relativity. Participants explore the implications of gravitational acceleration, relativistic effects, and the nature of coordinate systems in curved spacetime.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions what would prevent an object from being accelerated to the speed of light by the gravitational field of a supermassive planet, assuming no air resistance.
  • Another participant asserts that classical calculations are insufficient for such scenarios and emphasizes the need for relativistic physics, noting that infinite kinetic energy is never achieved.
  • It is mentioned that as an object approaches the speed of light, the relationship between force and acceleration changes, leading to a decrease in acceleration despite a constant gravitational field.
  • One participant introduces the concept of proper acceleration and questions its implications in the context of relativistic speeds.
  • Another participant discusses the dual perspectives of an observer and a free-falling individual, suggesting that the latter could exceed the speed of light relative to their starting point under certain conditions, such as falling towards a black hole.
  • A claim is made that a general relativistic calculation indicates that an object falling from rest at infinity reaches the speed of light at the event horizon of a Schwarzschild black hole.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the behavior of objects falling towards a supermassive planet and the implications of relativity. There is no consensus on whether an object can reach the speed of light, and the discussion remains unresolved.

Contextual Notes

Participants note the limitations of classical mechanics in this context and the complexities introduced by relativistic effects. The discussion highlights the dependence on coordinate systems and the distinction between local and global frames of reference in general relativity.

Goalie33
Messages
33
Reaction score
0
This question has bothered me for few weeks:

Lets say I was at some height above a super massive planet that has no atmosphere (i.e. no air resistance. If I were to begin falling what would stop me from being accelerated by the gravitational field of this planet to the speed of light? Assume that the mass of the planet and my height above the surface are enough to get me past c (if only the classical calculation is done.)
 
Physics news on Phys.org
Goalie33 said:
This question has bothered me for few weeks:

Lets say I was at some height above a super massive planet that has no atmosphere (i.e. no air resistance. If I were to begin falling what would stop me from being accelerated by the gravitational field of this planet to the speed of light? Assume that the mass of the planet and my height above the surface are enough to get me past c (if only the classical calculation is done.)

The classical calculation is incorrect for that scale. You need physics that can deal with velocities close to c, and that requires relativity.

One way to think about it is this. You never get past c because you never get to infinite kinetic energy. No matter how far you fall, there's a finite amount of potential energy involved, according to any stationary observer. (The velocity is going to depend on who is measuring it and with what co-ordinates.)

Cheers -- sylas
 
F is not equal to ma once you reach relativistic speeds. As you get close to the speed of light your acceleration will decrease, even if the gravitational field does not change. IIRC the result is [tex]F = \gamma^3ma[/tex] [1], where [tex]\gamma[/tex] is the usual Lorentz factor, which gets large as you approach the speed of light, causing the acceleration to get small, so you never actually reach the speed of light.

[1] This is for the force, acceleration and velocity all in the same direction. If you want to work with vectors, then the relation becomes more complex, and depends on the angle between the force and the velocity.
 
Thanks to both of you,

I understood that it would involve Special Relativity. (I knew classical mechanics would break down, I know now that the comment towards the end was misleading.) I just didn't know how to incorporate SR.

I think I've got it now, thanks again!
 
F is not equal to ma once you reach relativistic speeds.

what if you use proper acceleration instead?
 
kanato said:
F is not equal to ma once you reach relativistic speeds. As you get close to the speed of light your acceleration will decrease, even if the gravitational field does not change. IIRC the result is [tex]F = \gamma^3ma[/tex] [1], where [tex]\gamma[/tex] is the usual Lorentz factor, which gets large as you approach the speed of light, causing the acceleration to get small, so you never actually reach the speed of light.

[1] This is for the force, acceleration and velocity all in the same direction. If you want to work with vectors, then the relation becomes more complex, and depends on the angle between the force and the velocity.

There are two realities here, one from an observers point of view as described above and one from the person in freefall who is quite unaware of any force acting on him. In his freefalling environment he is quite at liberty to achieve a speed of separation faster than c (relative to his original frame/starting point). For instance, if he was falling towards a black hole, say from near infinity, I would imagine that he would exceed c once past the event horizon.
 
Nickelodeon said:
There are two realities here, one from an observers point of view as described above and one from the person in freefall who is quite unaware of any force acting on him. In his freefalling environment he is quite at liberty to achieve a speed of separation faster than c (relative to his original frame/starting point). For instance, if he was falling towards a black hole, say from near infinity, I would imagine that he would exceed c once past the event horizon.
The speed of light limit is only meant to apply in inertial coordinate systems, even in flat spacetime with no gravity it's quite possible for objects to have a coordinate velocity greater than c if you pick the right non-inertial coordinate system. In GR, no global coordinate system in curved spacetime can ever qualify as inertial, but because of the http://www.aei.mpg.de/einsteinOnline/en/spotlights/equivalence_principle/index.html an observer in freefall who is only paying attention to a small region of spacetime around him can have a "locally inertial" frame in that region where the laws of physics should look the same as in SR (assuming the region is chosen small enough that tidal forces are undetectable), and any objects passing by him in that region will be moving at less than c (or exactly c in the case of photons or other massless particles) in his locally inertial frame.
 
Last edited by a moderator:
A general relativistic calculation shows that a body falling from rest at infinity towards a Schwarzschild source, reaches c wrt to the source exactly on the event horizon (!).

See ( for instance ) arXiv:gr-qc/0411060.
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 21 ·
Replies
21
Views
3K
  • · Replies 30 ·
2
Replies
30
Views
3K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 130 ·
5
Replies
130
Views
17K
  • · Replies 15 ·
Replies
15
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 9 ·
Replies
9
Views
3K