- #1
Adyssa
- 203
- 3
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.
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.