Venus' non-relativistic contribution to Mercury's precession

In summary: This is known as the precession of perihelion and is a well-known phenomenon in orbital mechanics.In summary, Mercury has an eccentric orbit that brings it closer to the Sun at its perihelion and farther away at its aphelion. Venus, on the other hand, has a nearly circular orbit. When Mercury is approaching its aphelion, it can come close to Venus if they are in similar parts of their orbits. However, Venus's gravitational pull does not change the shape of Mercury's orbit, but it does cause its perihelion to precess or shift gradually in the direction of its motion. This precession is caused by the combined gravitational pull of all the planets, with Venus having the strongest effect due
  • #1
Eugene
4
1
TL;DR Summary
why does the orbit rotate as oppose to not rotate and just change its shape
Mercury's orbit is rather eccentric, its perigee brings it much nearer to the sun than its apogee. Venus by contrast has practically a circular orbit. When Mercury is approaching apogee, it can get close to venus if it is in the similar part of its orbit. At this point, Mercury's precession advances the most. but why does this venus gravitational pull cause mercury's orbit to rotate(its elliptical orbit maintains the same shape) as opposed to changing (elongating) Mercury's orbit?
 
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  • #2
The gravitational pull of Venus does not cause Mercury's orbit to rotate (in the sense of changing its orientation). It causes the perihelion of Mercury—the point at which it is closest to the Sun—to precess, or gradually shift in the direction of motion. The precession of Mercury's perihelion is caused by the combined gravitational pull of all the other planets, but Venus has the strongest effect due to its proximity to Mercury.The elliptical shape of Mercury's orbit is determined primarily by the mass of the Sun and the distance between Mercury and the Sun. The gravitational pull of Venus will not change this shape, but it will cause the perihelion to precess. This precession causes Mercury to move slightly faster when it is closer to the Sun, and slightly slower when it is farther away, resulting in a slight change in its orbital period.
 

FAQ: Venus' non-relativistic contribution to Mercury's precession

What is Venus' non-relativistic contribution to Mercury's precession?

Venus' non-relativistic contribution to Mercury's precession refers to the effect that Venus' gravitational pull has on Mercury's orbit, causing it to shift slightly over time.

How does Venus' non-relativistic contribution affect Mercury's precession?

Venus' non-relativistic contribution causes Mercury's orbit to precess, or rotate, slightly over time. This means that the point at which Mercury is closest to the Sun (perihelion) shifts slightly with each orbit.

Why is Venus' non-relativistic contribution important to study?

Studying Venus' non-relativistic contribution to Mercury's precession allows scientists to better understand the complex interactions between planets in our solar system. It also helps us to make more accurate predictions about Mercury's orbit and the long-term stability of our solar system.

How is Venus' non-relativistic contribution different from its relativistic contribution?

Venus' non-relativistic contribution is the effect of its gravitational pull on Mercury's orbit without taking into account the effects of Einstein's theory of general relativity. Venus' relativistic contribution, on the other hand, includes the effects of general relativity and is a much smaller factor in Mercury's precession.

Can Venus' non-relativistic contribution be measured?

Yes, Venus' non-relativistic contribution to Mercury's precession can be measured using precise observations of Mercury's orbit over time. By tracking the slight shifts in Mercury's perihelion, scientists can determine the exact amount of influence that Venus has on Mercury's orbit.

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