Interstellar space travel and reference frames

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SUMMARY

The discussion focuses on calculating the speed and energy requirements for a spacecraft traveling to a star 10 light years away, where the astronaut ages only 1 year. The key equations involve relativistic effects, specifically T = To/sqrt(1-v^2/c^2) and the relationship d = vT. The total mass of the spacecraft is 10^5 kg, and the calculations must account for the conversion of time and distance into consistent units to avoid exceeding the speed of light.

PREREQUISITES
  • Understanding of special relativity concepts, including time dilation and length contraction.
  • Familiarity with the equation T = To/sqrt(1-v^2/c^2).
  • Ability to convert light years to meters and years to seconds for accurate calculations.
  • Knowledge of energy calculations in relativistic physics.
NEXT STEPS
  • Learn how to apply the Lorentz transformation in relativistic physics.
  • Study the concept of relativistic mass and its implications for energy calculations.
  • Explore the relationship between velocity, distance, and time in different reference frames.
  • Review examples of muon decay and similar relativistic problems for practical understanding.
USEFUL FOR

Students of physics, particularly those studying special relativity, astrophysicists, and anyone interested in the mechanics of interstellar travel and relativistic effects on time and energy.

sr57
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Homework Statement


A spacecraft with its astronaut has a total mass at rest of 10^5 kg. The astronaut is to travel to a star 10 light years away at a speed such that she only ages 1 year in her frame of reference
a) the quantity 1-v/c where v is her speed with respect to Earth is?
b) the total energy required to accelerate the spacecraft from rest to this velocity in units of 10^22 Joules is?

Homework Equations


The Attempt at a Solution



1 year = 356 days = 1.89 x 10^9
I tried converting 10 light years into km
Then tried using v = d/t to find V
 
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Hi sr57,

sr57 said:

Homework Statement


A spacecraft with its astronaut has a total mass at rest of 10^5 kg. The astronaut is to travel to a star 10 light years away at a speed such that she only ages 1 year in her frame of reference
a) the quantity 1-v/c where v is her speed with respect to Earth is?
b) the total energy required to accelerate the spacecraft from rest to this velocity in units of 10^22 Joules is?

Homework Equations


The Attempt at a Solution



1 year = 356 days = 1.89 x 10^9
I tried converting 10 light years into km
Then tried using v = d/t to find V

You did not say what units you converted a year to, but I don't think it's 1.89 x 10^9 seconds.

What did you find when you calculated v using your method? If you change 10 light years into meters, and convert a year into seconds, it looks like your equation will give a speed larger than the speed of light (greater than 3 x 10^8), which indicates this approach will not work.

Here the speed will be large enough that you need to incorporate relativistic effects into your approach.
 
Using relativistic approach:

T = To/square root of (1-v^2/c^2)

T = 10 light years x speed of light/ V --> I'm not sure abt this

To = 1 year = 3.15 z 10^7 seconds

I don't know how to find V when i substitute the numbers
 
sr57 said:
Using relativistic approach:

T = To/square root of (1-v^2/c^2)

T = 10 light years x speed of light/ V --> I'm not sure abt this

No, that can't be correct because it doesn't have the right units. (time on the left side, distance on the right)

But now that you have the time interval T in the Earth frame of reference, and the length in the Earth frame, you can use your original equation d=vT.


As an alternative, you could have kept everything in the astronaut's frame of reference. You have the time interval To, and you could find the length in his reference frame (it will be contracted). Then you could use d=vT in that reference frame.


This problem is much like the discussion on muon decay which your textbook probably covers; it might be a good idea to read over that to see how they calculate the same motion in two different reference frames.
 

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