Simple ratios dilemma; telescopes and signals from out of space

In summary, the question asks for the power incident on a 1000-foot diameter radio telescope that can detect a signal with a power of only one picowatt that covers the entire surface of the Earth. The solution involves calculating the ratio of the Earth's surface area to the signal power and applying it to the surface area of the telescope. However, the incorrect total surface area of the Earth was used instead of the correct cross-sectional area, leading to an incorrect answer. The correct answer is 5.6 x 10E-22.
  • #1
T7
18
0
Hi,

Here's the question:

a) There is a radio telescope that is 1000 feet in diameter. It is claimed that it can detect a signal that lays down on the entire surface of the Earth a power of only one picowatt. What power would be incident on the antenna in this case?


It seems to me that this can be solved simply by considering the ratio of the surface area of the Earth to the power of the signal, and applying that to the surface of the telescope.

As far as I can see, given radius of Earth = 6.37 x 10E6 m and 1 foot = 0.3048m,

{ [ 1 x 10E-12 ] / [ 4 x pi x (6.37x10E6)^2 ] } x [ pi x (1/2 * 1000 * 0.3048)^2 ]

would give the answer. It actually gives 1.43 x 10E-22 when what is required is 5.6 x 10E-22 (4 times larger).

Can anyone spot what I'm doing wrong?

Cheers
 
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  • #2
You are using the total surface area of the entire Earth ([itex]4\pi r^2[/itex]), when you should only be using the cross-sectional area of the Earth ([itex]\pi r^2[/itex]).
 
  • #3
Tom Mattson said:
You are using the total surface area of the entire Earth ([itex]4\pi r^2[/itex]), when you should only be using the cross-sectional area of the Earth ([itex]\pi r^2[/itex]).

Yep. Thanks. :)
 

1. What is the "Simple ratios dilemma" in relation to telescopes and signals from out of space?

The "Simple ratios dilemma" refers to the challenge scientists face when trying to accurately measure and interpret signals from out of space using telescopes. This dilemma arises from the fact that the signals received by telescopes are often very faint and can be contaminated by various sources, making it difficult to determine the true ratio of the signal to the background noise.

2. How do scientists overcome the "Simple ratios dilemma" when studying signals from out of space?

Scientists use various techniques and technologies to overcome the "Simple ratios dilemma" when studying signals from out of space. This includes using advanced signal processing algorithms, building larger and more sensitive telescopes, and filtering out unwanted sources of noise.

3. Can simple ratios be used to accurately measure signals from out of space?

While simple ratios can provide a quick estimate of the strength of a signal from out of space, they are not always accurate due to the "Simple ratios dilemma." Scientists must use more advanced techniques to properly measure and interpret signals from out of space.

4. How do telescopes help us study signals from out of space?

Telescopes are essential tools for studying signals from out of space. They allow us to capture and analyze these signals, providing valuable information about the objects and phenomena that generate them. Telescopes also help us to better understand the universe and its many mysteries.

5. What are some potential sources of noise that can affect signals from out of space?

There are many sources of noise that can affect signals from out of space, including atmospheric interference, electronic noise from the telescope and its components, and interference from other sources such as radio transmissions. Scientists must carefully filter out these sources of noise to obtain accurate measurements of signals from out of space.

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