Measuring the Distance to an Exploded Star

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The Crab Nebula, a remnant of a supernova observed in 1054 AD, displays a red light frequency of 4.586 × 10^14 Hz, slightly higher than the laboratory frequency of heated hydrogen at 4.568 × 10^14 Hz. This frequency difference suggests the nebula is expanding, and the Doppler effect can be applied to estimate the speed of this expansion. The angular size of the nebula is approximately 5 arc minutes, which can be used to calculate its distance from Earth in light years. By assuming constant expansion since the explosion, one can also estimate the average radius of the Crab Nebula as of 2006 and determine the year of the supernova event. Understanding these measurements provides insight into the dynamics of stellar remnants.
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The gas cloud known as the Crab Nebula can be seen with
even a small telescope. It is the remnant of a supernova, a
cataclysmic explosion of a star. The explosion was seen
on the Earth on July 4, 1054 AD. The streamers in the
figure glow with the characteristic red color of heated
hydrogen gas. In the laboratory on earth, heated hydrogen
produces red light with frequency 4.568 × 1014 Hz; the red
light received from the streamers in the Crab Nebula
pointed at the Earth has a frequency of 4.586 × 1014 Hz.

a) Assume that the speed of the center of the nebula relative to the Earth is negligible.
Estimate the speed with which the outer edges of the Crab Nebula are expanding.
b) Assuming that the expansion has been constant since the supernova explosion, estimate the
average radius of the Crab Nebula in year 2006. (Immediately after the explosion, the size of the
Crab Nebula was neligible.) Give your answer in light years.
The angular size of the Crab Nebula, as seen from the earth, is about 4 arc minutes by 6 arc
minutes, for an average of 5 arc minutes. (1 arc minute = 1/60 of a degree)
c) Estimate the distance (in light years) to the Crab Nebula.
d) Estimate in what year BC the supernova explosion actually took place.
A light-year (ly) is the distance traveled by light in one year.
You may find it helpful to use the the first terms of the binomial expansion: (1+ε)^p ≅ 1 + pε

Hi, I'm not too sute how to approach this question but I think it has soething to do with the Doppler effect for light. If this is the case I would employ the following formula:

f_r = sqrt((c-v/c+v))(f_s)

where f_r is the frequency measured by the reciever and f_s the frequency of the source. What confuses me here is that both the frequencies are the same so I'm not sure how to set up the problem.

But, since they say to assume that the speed of the center of the nebula relative to the Earth is negligible, could I write the formula as follows?f_r = (1 + v/c)^(-1/2)

4.586 × 1014 Hz = (1 + v/(3.0 x 10^8))^-1/2

before I start solving for v, could you guys give me any hints on whether my setup is correct or not?

thank you !
 
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In the laboratory on earth, heated hydrogen
produces red light with frequency 4.568 × 1014 Hz; the red
light received from the streamers in the Crab Nebula
pointed at the Earth has a frequency of 4.586 × 1014 Hz.
The frequencies are different.

One needs to know the distance as a function of reshift, or vice versa.

The angle subtended by an arc is given by \theta=s/d, where s is the arc length and d is the distance, and the angle is in radians. For small angles, the arc length is very nearly the linaer dimension (shortest distance between two points).
 
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