Why does Mercury have an elliptical orbit?

In summary, the planets in our solar system follow elliptical orbits, with Mercury having the most noticeable precession due to the curvature of spacetime caused by the presence of the sun. This precession can be explained by General Relativity, while Newtonian physics can only account for about 92% of it. All planets follow geodesic paths in spacetime, and attempts to discredit GR's ability to explain these orbits are false.
  • #1
TimeRip496
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Why is mercury obit elliptical? Is it because of the curvature of spacetime caused by the presence of sun such that the mercury moves in that orbit otherwise known as geodesics? However what about the other planets like Earth that orbits in a circular orbit? Is is just that that is their geodesics and attempt to explain such orbits through the curvature of spacetime is impossible due to the our inability to percieve the 4 dimensional spacetime?
 
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  • #2
You may be confusing elliptical orbits and precession.
Elliptical orbits are the standard solution for planetary motion in good old classical Newtonian physics, and all the planets follow at least slightly elliptical orbits - that's what you get if you solve the equations of motion for a ##1/r^2## force.

General relativity says that the Newtonian ##1/r^2## force law isn't exactly correct, and if you use GR to calculate the orbits you'll find that they are elliptical as Newton and Kepler said centuries ago, but also that the ellipses precess very slightly. This precession is most noticeable for Mercury because it is closest to the sun, the forces are greater, and the deviation from the classical non-precessing ellipse is greater.

All the planets are following geodesic paths through spacetime according to GR.
 
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  • #3
TimeRip496 said:
Is is just that that is their geodesics and attempt to explain such orbits through the curvature of spacetime is impossible due to the our inability to percieve the 4 dimensional spacetime?

No. There is a view on some crackpot sites that GR cannot describe the elliptical precessing orbits of planets. This is not true, and it is in fact Newton's theory which cannot describe the above.

The exact of solution of the ellipse like orbits uses the Weierstrass P function ##\wp##.

https://en.wikipedia.org/wiki/Weierstrass's_elliptic_functions
 
  • #4
Mentz114 said:
This is not true, and it is in fact Newton's theory which cannot describe the above.

Technically, Newton can describe about 92% of the perihelion advance. It's only that last 8% that needs GR.

Nugatory said:
all the planets follow at least slightly elliptical orbits

Back when Pluto was a planet, it had a larger eccentricity than Mercury. (I guess it still does!) The asteroids 2 Pallas and 3 Juno also have larger eccentricities.
 
  • #5
Vanadium 50 said:
Technically, Newton can describe about 92% of the perihelion advance. It's only that last 8% that needs GR.
True.
To be more specific, the Newtonian solutions are conic sections which do not include precession at all. Obviously introducing perturbations and applying Newtonian theory can account for most of the precession. GR explains the so called anomalous precession.
 

1. What is an elliptical orbit?

An elliptical orbit is a type of orbit in which the path of the object follows an ellipse, rather than a perfect circle. This means that the distance between the object and the body it is orbiting around varies throughout its orbit.

2. How does Mercury's orbit differ from other planets?

Mercury's orbit is different from other planets because it is the most elliptical, or elongated, of all the planets in our solar system. Its eccentricity, or measure of how elongated an ellipse is, is 0.21, compared to Earth's eccentricity of 0.017.

3. What causes Mercury's elliptical orbit?

The elliptical orbit of Mercury is caused by the gravitational pull of the Sun and other planets in our solar system. The closer an object is to the Sun, the stronger the Sun's gravitational pull is, causing the orbit to become more elliptical.

4. How does Mercury's elliptical orbit affect its distance from the Sun?

Because Mercury's orbit is elliptical, its distance from the Sun varies throughout its orbit. At its closest point, called perihelion, Mercury is about 29 million miles away from the Sun. At its farthest point, called aphelion, it is about 43 million miles away.

5. What are the implications of Mercury's elliptical orbit?

Mercury's elliptical orbit has several implications, including its effect on the planet's temperature. When Mercury is at perihelion, it receives about 2.5 times more solar radiation than when it is at aphelion. This causes extreme temperature variations on the planet's surface, with highs reaching over 800 degrees Fahrenheit and lows dropping below -290 degrees Fahrenheit.

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