I'm trying to find data on the heliocentric velocities of planets in our solar system and was directed to Mathematica's AstronomicalData in a previous topic. Unfortunately I cannot find any x,y and z velocity components and was hoping someone might be able to point me in the right direction.
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asked May 24 '13 at 18:07
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An approximation (speed is in m/s and Position in m):
AstronomicalData["Mars", {"Speed", {2019, 3, 1, 0, 0, 0}}] Normalize @@
Differences[ AstronomicalData[ "Mars", {"Position", {2019, 3, 1, 0, 0, #}}] & /@ {0, 1}]
(*
{-22373.4, 8780.75, 734.403}
*)
answered May 24 '13 at 21:07
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1$\begingroup$ +1 Consider a central difference instead: it should be more accurate. It makes a substantial difference, by the way: it affects the third sig. fig. in your example, because it reflects the net planetary acceleration during the course of 12 hours. $\endgroup$ – whuber May 24 '13 at 22:18
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$\begingroup$ @whuber Perhaps I'm wrong, but I think I'm taking one second differences, not one day. Even within 10 seconds, there aren't appreciable speed changes (as expected, of course) $\endgroup$ – Dr. belisarius May 25 '13 at 4:44
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1$\begingroup$ Central difference:
{1, -1}.(AstronomicalData["Mars", {"Position", DatePlus[{2019, 3, 3}, {#, "Second"}]}] & /@ {1, -1}/2). Normalize and multiply with the speed afterwards. :) $\endgroup$ – J. M. is away♦ May 25 '13 at 9:48 -
$\begingroup$ Would something like this not work as well? v = ((AstronomicalData[ "Mars", {"Position", {2013, 1, 1, 1, 1, 1.01}}] - AstronomicalData["Mars", {"Position", {2013, 1, 1, 1, 1,1}}]))/0.01 $\endgroup$ – InquisitiveInquirer May 25 '13 at 12:08
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1$\begingroup$ @J.M.
Normalize[{1, -1}.(AstronomicalData[ "Mars", {"Position", DatePlus[{2019, 3, 1}, {#, "Second"}]}] & /@ {1, -1}/ 2)] AstronomicalData["Mars", {"Speed", {2019, 3, 1, 0, 0, 0}}]gives the same result as mine. That's why I don't understand whuber's comment. I'm forgetting something, surely $\endgroup$ – Dr. belisarius May 25 '13 at 14:24
