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When we talk about relative velocity in the context of the Doppler Effect, we're referring to the speed at which an object is moving in relation to another. Here, it's the speed of the spaceship compared to the space station. The Doppler Effect in physics helps us understand how the frequency of a wave changes when the source and observer are in motion relative to each other.
In the exercise, we determined the relative speed by using the Doppler Effect formula:

• The emitted frequency of the laser light was calculated from the spaceship's perspective.
• The observed frequency was determined as the spaceship approached the space station.
• The change in frequency gives insight into the spaceship's speed compared to the space station.

The formula used was:\[f' = \frac{f}{1+\frac{v}{c}}\]By rearranging, the velocity \(v\) was calculated, showing how quickly the spaceship moves towards the space station. A negative value here suggests that the distance between the spaceship and the space station is decreasing, hence getting closer.

Wavelength shift happens when there is a change in the observed wavelength due to the relative motion of the source and the observer - a result of the Doppler Effect. For this problem, the red light emitted from the spaceship appeared blue to the astronauts on the space station.
Here's how it works:

• The original wavelength of the laser emitted from the spaceship was 632.8 nm.
• Upon reaching the space station, this wavelength was observed as 514.5 nm, a shorter wavelength associated with blue light.

These changes in wavelength are quantified as a Wavelength Shift. It's crucial in astrophysics for determining the movement and speed of astronomical objects relative to Earth.
The difference in wavelength, \(\Delta \lambda\), is computed by:\[\Delta \lambda = \lambda' - \lambda\]In our problem, this wavelength shift highlights the spaceship's quick approach towards the space station, evidenced by the shift towards the blue end of the spectrum.

Frequency conversion is a critical step in resolving problems involving the Doppler Effect. To understand how waves change from one form (or frequency) to another, we use the speed of light equation:\(c = \lambda f\).
Here’s the breakdown:

• Start with the emitted wavelength \(\lambda\) on the spaceship: 632.8 nm.
• Convert this into its frequency \(f\) by rearranging the formula, which gives us \(f = \frac{c}{\lambda}\).
• Next, take the observed wavelength\(\lambda'\) of 514.5 nm as seen by the station astronauts.
• Convert this to the observed frequency \(f'\) using the same formula: \(f' = \frac{c}{\lambda'}\).

This process translates the problem into terms of frequency, which can then be used in the Doppler Effect equation to find the relative velocity. This step is invaluable because it mathematically bridges the shift in wavelength (color change from red to blue) to actual speeds.