How fast must a pion be moving on average to travel 28 m before it decays? The average lifetime, at rest, is 2.6 x 10-8 s.
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35. Special Relativity
Consequences of Relativity
Problem 10c
Textbook Question
A star is 23.5 light-years from Earth. How long would it take a spacecraft traveling 0.950c to reach that star as measured by observers: What is the distance traveled according to observers on the spacecraft?

1
Step 1: Begin by understanding the problem. The spacecraft is traveling at a speed of 0.950c (where c is the speed of light) toward a star that is 23.5 light-years away. We need to calculate the distance traveled according to observers on the spacecraft (part c) and the speed computed by the spacecraft occupants (part d). This involves concepts of special relativity, particularly length contraction and relative velocity.
Step 2: For part (c), use the formula for length contraction in special relativity: , where L₀ is the proper length (distance measured in the rest frame of the star and Earth, which is 23.5 light-years), v is the velocity of the spacecraft (0.950c), and c is the speed of light. Substitute the given values into the formula to calculate the contracted length L as observed from the spacecraft.
Step 3: For part (d), the spacecraft occupants will compute their speed using the formula , where d is the contracted distance (calculated in part c) and t is the time measured by the spacecraft occupants. To find t, use the time dilation formula: , where t₀ is the time measured by Earth observers (calculated in part b, which is not explicitly provided here but can be derived using ). Substitute the values to compute t and then use it to find the speed.
Step 4: Combine the results from part (c) and part (d). The contracted distance L (from part c) and the time t (from part d) will allow the spacecraft occupants to compute their speed. Note that the speed they compute should match the given velocity of 0.950c, as the laws of physics are consistent in all inertial frames.
Step 5: Verify the results conceptually. The contracted distance should be shorter than the proper length (23.5 light-years), and the computed speed should align with the given velocity of 0.950c. This ensures consistency with the principles of special relativity.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Relativity of Time and Distance
In the theory of relativity, time and distance are not absolute but depend on the relative motion of observers. As an object approaches the speed of light, time dilates for the moving observer, meaning they experience time more slowly compared to stationary observers. This leads to differences in how distances are perceived, particularly in high-speed travel scenarios.
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Intro to Relative Motion (Relative Velocity)
Lorentz Transformation
The Lorentz transformation equations describe how measurements of time and space change for observers in different inertial frames of reference. These equations are essential for calculating time dilation and length contraction, which occur at relativistic speeds. They allow us to relate the time and distance measured by stationary observers to those measured by observers moving at a significant fraction of the speed of light.
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Lorentz Transformations of Velocity
Speed Calculation in Relativity
In the context of relativity, the speed of an object is calculated differently than in classical mechanics. For a spacecraft traveling at a significant fraction of the speed of light, the speed as perceived by the occupants can differ from that measured by stationary observers due to time dilation and length contraction. This requires careful application of relativistic formulas to determine the effective speed experienced by the spacecraft's occupants.
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Intro to Relative Motion (Relative Velocity)
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