How do telescopes allow us to see light sources millions of light years away?

In summary, the conversation discusses the concept of signal attenuation and how it affects the detection of light from faraway sources. It also explains the difference between power and intensity in relation to light sources. It is possible to see light sources millions of light years away due to the use of telescopes and the amount of time spent gathering light.
  • #1
Clay
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i have heard how our broadcasts will be seen by aliens far away or whatever.
but i realize those signals are going to "attenuate" by d^-2

anyway...
how come in astronomy we can see light sources millions of light years away? shouldn't those signals be far too weak to detect after such a long distance?furthermore i am confused about the concepts of "power" and "intensity"

say we have a 100kw isotropic radio antenna
so at, say, 5 meters away, what is our power? what is our intensity? (assume vacuum)
 
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  • #2
Clay said:
how come in astronomy we can see light sources millions of light years away? shouldn't those signals be far too weak to detect after such a long distance?
They start off as really really big signals.
 
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  • #3
Power is energy per unit time. Intensity is power per unit area (where the area is measured perpendicular to the direction the light is coming from).
 
  • #4
Clay said:
i have heard how our broadcasts will be seen by aliens far away or whatever.
but i realize those signals are going to "attenuate" by d^-2

anyway...
how come in astronomy we can see light sources millions of light years away? shouldn't those signals be far too weak to detect after such a long distance?
1. We use telescopes with large apertures that can gather much more light than our eyes can.
2. We spend a lot of time gathering light from what our telescope is pointed at. The Hubble telescope can spend weeks looking at a single spot in the sky, slowly collecting light in order to build up an image.
 
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FAQ: How do telescopes allow us to see light sources millions of light years away?

What is the inverse square law?

The inverse square law is a mathematical principle that describes the relationship between the strength of a physical quantity and the distance from its source. It states that the strength of a physical quantity decreases in proportion to the square of the distance from its source.

How is the inverse square law applied in science?

The inverse square law is applied in various fields of science, including physics, chemistry, and biology. It is used to explain phenomena such as gravity, light intensity, and sound propagation. It also helps scientists understand the behavior of electromagnetic fields and radiation.

What is the confusion surrounding the inverse square law?

The confusion surrounding the inverse square law arises from the fact that many people do not fully understand the concept and how it applies in different situations. Some also mistakenly believe that it can be applied to any physical quantity, which is not always the case.

Why is it important to understand the inverse square law?

Understanding the inverse square law is crucial in many scientific fields as it helps scientists make accurate predictions and calculations. It also allows them to design experiments and technologies that take into account the effects of distance on physical quantities.

How can the inverse square law be visualized?

The inverse square law can be visualized through graphical representations, such as graphs and charts, which show the relationship between the physical quantity and distance. It can also be demonstrated through real-life examples, such as the brightness of a light source decreasing as you move further away from it.

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