Can someone explain abberation of starlight?

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Discussion Overview

The discussion revolves around the concept of aberration of starlight, focusing on its general explanation, underlying mechanics, and its distinction from parallax. Participants explore the implications of velocity on aberration and seek clarification on specific aspects related to its effects and mathematical representations.

Discussion Character

  • Exploratory
  • Conceptual clarification
  • Homework-related

Main Points Raised

  • One participant seeks a general explanation of aberration of starlight for an astronomy class, indicating a need for foundational understanding.
  • Another participant suggests that the original poster clarify their understanding to better address their confusion regarding the topic.
  • A participant explains that aberration differs from parallax, noting that it increases with a planet's proximity to the Sun due to higher orbital velocities.
  • The analogy of running in the rain is used to illustrate how velocity affects the perceived angle of incoming light, prompting questions about the impact of latitude on telescope alignment.
  • A participant raises a question about the mathematical relationship between expected and actual observations of aberration, specifically the difference between tan(theta) and sin(theta) in the context of velocity and the speed of light.

Areas of Agreement / Disagreement

The discussion reflects a lack of consensus on certain aspects of aberration, particularly regarding its mathematical representation and the effects of latitude on telescope alignment. Participants express curiosity and seek clarification rather than reaching definitive conclusions.

Contextual Notes

Participants express uncertainty about specific mathematical relationships and the visual representation of aberration ellipses, indicating potential gaps in understanding that depend on further exploration of definitions and concepts.

Pharaoness
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Hello everyone,
I was wondering if anyone can explain how the abberation of starlight works in general terms, as well as what exactly it is. I am a first year astronomy student and this is for my astronomy/physics class, and would like a general explanation of what it is. This is all my professor would require for the upcoming midterm, so if anyone can help that would be great. Thanks!
 
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Welcome to PF;
The best use of these forums is to give your ideas of what it is and that will help us pinpoint the source of your confusion. Have a go reading through:
http://en.wikipedia.org/wiki/Aberration_of_light
... and telling us where you get lost.
 


Thank you for responding Simon! I guess I should have elaborated on what I understand and what I would like to know. So I know that this is not like parallax in that it depends on velocity, so while parallax increases the further out you go in the solar system, aberration of starlight increases the closer to the Sun a planet is (because the closer to the Sun a planet is, the faster its orbital velocity). Hence, from Mercury the aberration ellipse is greater than aberration ellipses on Earth.
I guess what I'd like to know is how exactly aberration works? My professor was explaining it to be almost like walking, or running in the rain, if the rain is falling straight down (ie, perpendicular to the floor) but you are running, because of your velocity, it is like they are falling on an angle, so you would need to tilt your umbrella to shield the rain. So does the latitude of a person have an effect on the amount a telescope needs to be tilted? And what exactly does an aberration ellipse look like? Does that make sense? Thanks!
 
Additionally, what I read about aberration online is that what you expect to see is tan (theta) = v/c, but what you actually find is that sin (theta) = v/c. Why is this, and what does it mean? On Wikipedia it says the same thing. I'll read it in its entirety, but if you can help with that that would be great. Thanks! :)
 

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