Question re: Planets Facing Each Other

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This discussion focuses on the mathematical determination of alignment between two points on different planets, specifically Point 1 on Earth (Planet A) and Point 2 on Mercury (Planet B). The user inquires about the feasibility of predicting when a laser beam from Earth can hit a specific target on Mercury, considering the planets' rotations and orbits. The conversation highlights the complexities of planetary motion and the unpredictability of rotation rates, emphasizing the need for precise calculations to ascertain alignment times.

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JorgeMedinero
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It may be that this question makes assumptions that are themselves invalid -- I am less than an amateur. But here goes.

Is there any easy way to determine how often Point 1 on Planet A and Point 2 on Planet B will align? That is, if at Time X you could draw a straight, unobstructed vector from Point 1 to Point 2, is there a simple equation for figuring out when the same vector will connect the same two points. Is there any assurance it will occur again?

Here is the thought experiment:

Thank you for the welcome!

Let us say that the vector is relative to the planetary surface -- imagine that I have a laser device (on Earth, Planet A) that shoots a perfectly straight, instantaneous beam (I know, impossible per Einstein). The device is fixed in place, angle, and so forth, save for the fact that the Earth rotates and orbits and so forth. The laser has a targeting scope.

It is located at Point 1. At Time X Mercury comes into my targeting scope and I fire, burning a spot at Point 2 on Mercury's surface.

Astronauts then travel to Mercury. They put a bullseye at Point 2. My question is whether there will ever be a Time Y at which my laser can shoot the bullseye, and if so, how it can be predicted.

---

Alternatively, is there any easy way to determine how often *any* unobstructed vector can be drawn from Point 1 to Point 2? In this case, the laser device can be re-aimed, but cannot be moved.
 
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The rotation rate (ie. length of a day) of planets is fairly constant but its value is random in that it depends on the precise arragement of particles at their creation - there is no law to predict the rotation rate from the mass or position of the planet.

The rotation rate of venus for instance was only measured once it was possible to detect mountains under the constant clouds using radar, the rotation rate of Jupiter is very easy to measure because you can watch the red spot go round.
 

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