What we know: We know a solar day on Mars is how long it takes for the sun to make a complete "rotation" in the sky and return to the same point. Because the Sun is not a fixed point in the sky (due to the fact that Earth and Mars are rotating it) a solar day will differ from a sidereal day, which is how long it takes for a fixed point (typically a star) to reach its same location in the sky.
Image from: http://ottawa-rasc.ca/articles/earl_mike/Satellite_Tracking/Dishes/Satellite_Dishes.html
We also know from Kepler's Law: P2αa3
and from the problem: Pe=1year
ae=1AU
am=32AU
(where Pe and Pm is the rotation period of the Earth and Mars respectively and ae and am are the distance between the Sun and Earth and Mars respectively).
Solve:
From Kepler's Law we can set up the ratio: P2eP2m=a3ea3m
and isolate the rotation period of Mars: Pm=√P2ea3ma3e
plugging in the provided values give:Pm=√12⋅32313
which simplifies to: Pm=(32)32≈95Earthyears
when converting to days we get 95Earthyears⋅365days≈660daysinaMartianyear
But this is not enough, we want the difference between the two days in minutes per day, not the length of a Martian year. To find the difference we can use the fact that Mars traverses an entire orbit in a 660 days 360∘660days≈0.55∘day
to show that a sidereal day is about half a degree less than a solar day. Then we can convert to days per minute: 360∘660days⋅1hr15∘⋅60min1hr≈2minday
Conclusion: with the given values, the difference between sidereal and solar day is about 2 minutes. This means that Mars's sidereal day is 2 minutes shorter than its solar day.
Acknowledgements: Many thanks to Barra for working on this worksheet with me.
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ReplyDeleteVery nice job working this through. I particularly like how you converted 1.5 to a fraction. It's pretty cool that using an approximation as rough as you did actually works. The actual fraction is 32=5.22.8 .
By the by, to get well proportioned parenthesis the \left( \right is how to get them to scale with what is in the problem. e.g \left(\frac{\sqrt{e^{i \pi}}}{\frac{e^{i \theta} - \cos{\theta}}{\sin{\theta}}}\right) = 1 is (√eiπeiθ−cosθsinθ)=1
Fixed! Thank you, that trick was very useful in future blog posts.
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