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Section 37.3 Einstein's Principle of Relativity An out-of-control alien spacecraft is diving into a star at a speed of \(1.0 \times 10^{8} \mathrm{m} / \mathrm{s} .\) At what speed, relative to the spacecraft. is the starlight approaching?

Short Answer

Expert verified
The speed of the starlight relative to the spacecraft is \(3.0 \times 10^{8} m/s\).

Step by step solution

01

Understand the problem

The problem is asking to find the speed of starlight relative to the diving spacecraft.
02

Apply Einstein's principle of relativity

According to Einstein's principle of relativity, the speed of light is constant and does not change due to the velocity of the observer. Therefore, the relative speed of the starlight approaching the spacecraft is the same as the speed of light in a vacuum.
03

Calculate the speed

The speed of light in a vacuum is known to be approximately \(3.0 \times 10^{8} m/s\). Thus, this will be the speed of the starlight relative to the spacecraft.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Speed of Light
The speed of light is a fundamental constant in physics. It is denoted by the letter "c" and its value is approximately \(3.0 \times 10^8 \text{ meters per second}\). This speed is remarkably fast and is the maximum speed at which all information and matter can travel in the universe. When we talk about light traveling through a vacuum, it always moves at this constant speed, regardless of the movement of its source or observer.
  • The constancy of the speed of light forms the basis for Einstein's theory of special relativity.
  • It impacts electromagnetic waves, like visible light, radio waves, and X-rays.
  • This speed remains the same even when light moves through mediums like air or glass, although it might temporarily slow down through such materials.
An important implication of the speed of light's constancy is that it challenges our intuitions about how speeds add up in classical mechanics, as we'll discuss further in relative velocity.
Relative Velocity
Relative velocity is a way to understand how the speed of one object looks to another. In everyday experiences, like cars on a highway, we add or subtract velocities. However, when dealing with the speed of light, things are different due to Einstein's principle of relativity. Normally, if two objects are moving towards each other or the same direction, you'd sum or use the difference of their speeds to find the relative velocity.
  • But light is special! Its speed is always constant, even if both the observer and the source are moving at high speeds.
  • Whether you're moving towards light or away from it, the speed you observe is always \(3.0 \times 10^8 \text{ m/s}\).
  • This concept prevents the addition of classical velocities from applying to light's speed.
This was a revolutionary idea because it changed our understanding of how motion and speed work in the universe compared to Newtonian physics.
Special Relativity
Einstein's Special Relativity redefined the way we understand space and time. It incorporates the idea that the laws of physics are the same for all observers, no matter their velocity, especially the behavior of light. Special relativity brought forward two main ideas:
  • The speed of light is constant and is not affected by the motion of its source or observer.
  • Time and space are interconnected and relative to the observer's motion.
A key outcome of this theory is the concept of time dilation, where time can move slower or faster depending on the relative speeds of observers. Similarly, length contraction means objects can appear shorter in the direction of motion to an observer moving at similar high speeds.
These concepts help explain why, in the exercise scenario, the starlight's velocity remains unchanged relative to the spaceship, no matter its velocity. Light always maintains its constant speed, demonstrating how special relativity shapes our understanding beyond the limits of classical physics.

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Most popular questions from this chapter

You are flying your personal rocket craft at \(0.9 c\) from Star \(\mathbf{A}\) toward Star B. The distance between the stars, in the stars" reference frame, is 1.0 ly. Both stars happen to explode simultaneously in your reference frame at the instant you are exactly halfway between them. Do you see the flashes simultaneously? If not, which do you see first and what is the time difference between the two?

The star Delta goes supernova. One year later and 2 ly away, as measured by astronomers in the galaxy, star epsilon explodes. Let the explosion of Delta be at \(x_{\mathrm{D}}=0\) and \(t_{\mathrm{D}}=0 .\) The explosions are observed by three spaceships cruising through the galaxy in the direction from Delta to Epsilon at velocities \(v_{1}=0.3 c, v_{2}=0.5 c,\) and \(v_{3}=0.7 c.\) a. What are the times of the two explosions as measured by scientists on each of the three spaceships? b. Does one spaceship find that the explosions are simultaneous? If so, which one? c. Does one spaceship find that Epsilon explodes before Delta? If so, which one? d. Do your answers to parts \(b\) and \(c\) violate the idea of causality? Bxplain.

Section 37.10 looked at the inelastic collision \(e^{-}\) (fast) \(+\) \(c^{-}(\text {at rest }) \rightarrow c^{-}+c^{-}+c^{-}+c^{+}.\) a. What is the threshold kinetic energy of the fast electron? That is, what minimum kinetic energy must the electron have to allow this process to occur? b. What is the speed of an electron with the threshold kinetic energy?

A cube has a density of \(2000 \mathrm{kg} / \mathrm{m}^{3}\) while at rest in the laboratory. What is the cube's density as measured by an experimenter in the laboratory as the cube moves through the laboratory at \(90 \%\) of the speed of light in a direction perpendicular to one of its faces?

A billiard ball has a perfectly elastic collision with a second billiard ball of equal mass. Afterward, the first ball moves to the left at \(2.0 \mathrm{m} / \mathrm{s}\) and the second to the right at \(4.0 \mathrm{m} / \mathrm{s} .\) Use reference frames and the Chapter 10 result for perfectly elastic collisions to find the speed and direction of each ball before the collision.

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