Distance of a point on the earth from the sun

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Discussion Overview

The discussion revolves around the relative difference in distance from the sun for two locations on Earth: Montreal, Canada, and Melbourne, Australia. Participants explore the implications of Earth's axial tilt, curvature, and other factors affecting this distance, with a focus on understanding how these differences might influence temperature experienced at the surface.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant calculates the horizontal distance from the equator for Montreal and Melbourne based on their latitudes and considers the Earth's axial tilt to find a relative distance difference of 1585km.
  • Another participant raises considerations about the curvature of the Earth and the Sun, the time of day, and the time of year affecting distance calculations.
  • Questions are posed regarding whether to account for the Earth's axial wobble and altitude, as well as the Earth's oblateness in these calculations.
  • A participant expresses interest in how the distance from the sun affects ground temperature, acknowledging the importance of various factors mentioned by others.
  • A resource link is provided for modeling the Earth's surface, with a note on the potential for excessive accuracy to become meaningless.

Areas of Agreement / Disagreement

Participants do not reach a consensus, as multiple competing views and considerations remain regarding the factors influencing the distance from the sun and its implications.

Contextual Notes

Limitations include assumptions about the spherical nature of the Earth, the impact of axial tilt, and the need for clarity on what point on the Sun is being referenced. The discussion also highlights the complexity of accurately modeling these distances due to various factors.

Adyssa
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A question was posed that I decided to have a crack at, and I want to check my understanding. This isn't homework by the way, just trivia. Also the thread title is not really correct but I didn't want to complicate things! Here's the question:

What is the relative difference in the distance from the sun of two points on the earth. Specifically Montreal, Canada and Melbourne, Australia.

I started by finding out their respective latitudes. With these in hand, I drew a circle and some interior right triangles and set about finding the horizontal distance component from the equator to the point on the circle. I'm pretty sure I have these correct, here is my data so far:

Radius of Earth: 6378.1km

Montreal:
-Latitude: 45.5081° N
-Horizontal distance from equator: 1908.3km

Melbourne:
-Latitude: 37.7833° S
-Horizontal distance from equator: 1337.3km

Now, I need to account for the axial tilt of the earth, which is 23°. Given that it's the middle of summer/winter, the difference in distance from the sun will be at a maximum. What I did was to get the horizontal distance component for a point (the equator) at 23° latitude, which is 507km, and +/- from my above results, and I get a relative difference in distance of 1585km between the two cities.

Anyone care to comment or correct my reasoning? :)

Also, what is a good resource for astronomical measurements? I'd like to turn this into a program but I need to know about the elliptical orbit of the earth.
 
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Some considerations:

On a scale that the curvature of the Earth is important (as here) the curvature of the Sun is also important.
So - distance from "where" on the Sun?

The distance will depend on the time of day.
The distance will depend (as you've noticed) on the time of year.

Do you also want to account for the Earth's axial wobble? What about altitude? You know the Earth is not exactly a sphere - so would you want to consider the "oblacity" as well?

What usually governs the form of these sorts of calculations is what you want to use the end result for.
 
Thanks Simon, you've brought up some things I had not considered. It's just an exercise for curiosities sake at the moment, but it would be nice to arrive at an accurate answer. The question was posed to get some perspective on how the distance from the sun affects the temperature experienced on the ground in different locations. To this end, I think all of the things you have mentioned are important, particularly altitude, and, as you say, "oblacity" - I've never heard the word but I guess you are referring to the fact that the Earth is a squashed sphere which I believe is due to centrifugal force from rotation. Distance from "where" on the sun is an interesting one. Perhaps I will think about that a little more.
 
For ideas about modelling the Earth's surface:
http://kartoweb.itc.nl/geometrics/reference%20surfaces/body.htm

There is such a thing as being too "accurate" ... at some point the extra decimal places will be meaningless.
 

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