A question about the theory of relativity

AI Thread Summary
When observing a star while traveling near the speed of light, relativistic effects such as length contraction may alter the perceived size of the star, but this does not change its actual appearance or properties. A black hole, which emits no light, would still be fundamentally different from a regular star, and its characteristics would not change due to the observer's speed. The relativistic mass of the star increases with speed, but its rest mass remains constant, and the process of a star collapsing into a black hole is a physical event, not merely an observational effect. The conditions for a star to become a black hole, such as the Chandrasekhar limit, are based on its rest frame and would differ in a moving reference frame. This suggests a complex relationship between velocity, mass, and the formation of black holes that requires careful consideration of relativistic principles.
IDOGAWACONAN
Messages
10
Reaction score
0

Homework Statement


If I fly at the speed which is similar to the speed of light,and I am watching a still star,then because of the theory of relativity,the size of the star will change.If the size of the star turn to the size of a neutron star or a black hole,what will happen?Will I see a neutron star or a black hole?(My English is terrible,so I am sorry if you can't understand it well)

Homework Equations





The Attempt at a Solution

 
Physics news on Phys.org
Well I am not an expert on relativity in any way really, but the length contraction caused by the lorentz equations would only possibly alter the size of the object that you see, not what it actually "looks" like. A black star "looks" completely different to a star as light cannot escape its gravity, but you moving similar to the speed of light wouldn't make much difference I don't think.
 
Welcome to PF!

You may want to search your references for "Penrose-Terrell Rotation" and see if that will allow you to draw your own conclusion regarding your questions.
 
But the mass of the star will grow.When it's beyond the Chandrasekhar'limit,should it become a black hole?
 
The relativistic mass of the star will grow, but not the rest mass. A star collapsing to a black hole is a very real, local, physical process and not an "observational" effect only, like relativistic mass. You can think of relativistic mass as a kind of a "transformation cheat" used in special relativity to make many other mechanical interactions appear Newtonian.

Others here may be able to offer you a better explanation.
 
Filip Larsen said:
The relativistic mass of the star will grow, but not the rest mass. A star collapsing to a black hole is a very real, local, physical process and not an "observational" effect only, like relativistic mass. You can think of relativistic mass as a kind of a "transformation cheat" used in special relativity to make many other mechanical interactions appear Newtonian.
Excellent points.

As far as I know, the conditions under which a star is able to become a black hole (i.e. Chandrasekhar limit) only apply when measured in the rest frame of the star. If you wanted to figure out the conditions required for a star to become a black hole in a reference frame in which the star is moving with some constant velocity, they would presumably be different. In particular, the critical density required to form the black hole would probably be higher. I haven't done the math, so I might be wrong, but it seems like there would be a logical inconsistency if a black hole (i.e. event horizon) existed in one distant inertial reference frame but not another.
 
I multiplied the values first without the error limit. Got 19.38. rounded it off to 2 significant figures since the given data has 2 significant figures. So = 19. For error I used the above formula. It comes out about 1.48. Now my question is. Should I write the answer as 19±1.5 (rounding 1.48 to 2 significant figures) OR should I write it as 19±1. So in short, should the error have same number of significant figures as the mean value or should it have the same number of decimal places as...
Thread 'Collision of a bullet on a rod-string system: query'
In this question, I have a question. I am NOT trying to solve it, but it is just a conceptual question. Consider the point on the rod, which connects the string and the rod. My question: just before and after the collision, is ANGULAR momentum CONSERVED about this point? Lets call the point which connects the string and rod as P. Why am I asking this? : it is clear from the scenario that the point of concern, which connects the string and the rod, moves in a circular path due to the string...
Thread 'A cylinder connected to a hanging mass'
Let's declare that for the cylinder, mass = M = 10 kg Radius = R = 4 m For the wall and the floor, Friction coeff = ##\mu## = 0.5 For the hanging mass, mass = m = 11 kg First, we divide the force according to their respective plane (x and y thing, correct me if I'm wrong) and according to which, cylinder or the hanging mass, they're working on. Force on the hanging mass $$mg - T = ma$$ Force(Cylinder) on y $$N_f + f_w - Mg = 0$$ Force(Cylinder) on x $$T + f_f - N_w = Ma$$ There's also...

Similar threads

Back
Top