How often are mars and earth diametrically apart

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Mars orbits the sun at a mean distance of 228 Gm with an orbital period of 687 days, while Earth has a mean distance of 149.6 Gm and orbits in 365 days. The angle swept by Mars during one Earth year is approximately 191 degrees. Mars and the Sun are in opposition every 779 days, which is derived from the formula 1/T = 1/E - 1/M, where E is the Earth year and M is the Mars year. The relative angular velocity between Earth and Mars is calculated to be 0.2311 degrees per day, leading to the conclusion that they are diametrically opposed every 779 days. Understanding this relationship clarifies the orbital dynamics between the two planets.
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Homework Statement



Mars orbits the sun at a mean orbital radius of 228 Gm ( 1 G = 10^9 m) and has an orbital radius of 687 days. Earth orbits the sun at a mean orbital radius of 149.6 Gm.
The earth-sun line sweeps out an angle of 360 during one Earth year. Approximately what line is swept out by the Mars-Sun line during one Earth-year?
How frequently are Mars and the Sun in opposition (on diametrically opposite sides of the earth?)

Homework Equations



365 days = 360 degrees for earth
687 days = 360 degrees for Mars

The Attempt at a Solution



(360 degrees/ 687 days)x 365 day = 191 degrees for Mars sweeping.
That's cool. I get that.

It's the diametrically opposed part that I am having issues with comprehending. Yahoo answers gave a solution:

"Mars and the Sun are in opposition every T days where T is given by 1/T = 1/E - 1/M where E =365 days is the Earth year and M=687 days is the Mars year. This works out to T = 779 days, slightly more than 2 years. "

This works. But this formula seemed out of the blue to me. Where did they come up with this? Am I missing something really simple? (Probably...)

No need to solve the problem, it's on where they got that formula. Thank you very much.
 
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hi epicbattle! :smile:
epicbattle said:
1/T = 1/E - 1/M where E =365 days is the Earth year and M=687 days is the Mars year.

hint: angular speed = 2π/D radians per day …

and how do you find the relative angular speed of two bodies? :wink:
 
Ah hah, thank you.

[2pi/Days(Earth) - 2pi/Days(Mars)]*180/2pi degrees per day. The 2pi cancels leaving the formula. Thank you.

So .2311 degrees per day is relative angular velocity

So how often are they diametrically apart 180/.2311 which solves for 779 days. Thank you very much. I won't forget this.
 
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