Why is it difficult to measure the perihelion advance of the planet Venus? Help

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Measuring the perihelion advance of Venus is challenging primarily due to its nearly circular orbit, which makes the perihelion location less distinct. The small rate of advance, approximately 8 seconds of arc per century, complicates accurate measurement. Perturbations from other planets significantly influence Venus' orbit, necessitating their elimination for precise calculations. Additionally, the curvature of spacetime near the Sun plays a role, but the dominant factor remains gravitational interactions with other celestial bodies. Overall, achieving accurate measurements involves addressing both orbital geometry and external perturbations.
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Why is it difficult to measure the perihelion advance of the planet Venus? Please help me answer this question in details...Thank you~ :smile:
 
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kiwikiwi79 said:
Why is it difficult to measure the perihelion advance of the planet Venus? Please help me answer this question in details...Thank you~ :smile:
Venus' orbit is practically circular so the perihelion location is less distinct. Venus' orbital plane in inclined more than 3 degress to the plane of the Earth's orbit. I don't know if that makes it more difficult to measure. The main reason is probably that the rate of advance is so small. Mercury's perihelion advance is about 10 minutes/century. Venus' is about 8 seconds of arc per century.

AM
 
The curvature of space time closer to the sun is also a factor, right?
 
pinkie said:
The curvature of space time closer to the sun is also a factor, right?

If you're talking only about GR corrections, then yes, but the dominant source of perihelion advance in planetary orbits is perturbations from other planets.
 
Andrew Mason said:
Venus' orbit is practically circular so the perihelion location is less distinct. Venus' is about 8 seconds of arc per century. AM
So, it would appear to be a matter of precision of either measurement or calculation, and a matter of the geometry of the orbit (almost circular). I imagine the perturbations in the orbit due to other planets are on the order of a few seconds of arc.
 
KiwiKiwi,
The best way to measure the perhelion advance of any of the solar system planets is to first eliminate the peturbations of the other planets, then calculate the length of advance as opposed to the angular advance.
For Mercury the angular advance is about 43 seconds of arc, less for Venus and even more so for the earth; if we work with the length of advance instead (the length of the arc subtended by the angle of advance) it is the same for all planets and is approximately 27833.859 metres.
This length is determined only by the mass of the sun, G, and the velocity of light. Since this length is the same for all the planets in their orbits after the corrections for orbital ellipticity are removed we really ought to say that the perhelion advance is the same for all planets regardless of their distance from the sun.
 
i don't know weather this helps but maybe it could have some thing to do with the fact Venus is in retrograde?
 
i don't know weather this helps but maybe it could have some thing to do with the fact Venus is retrograde?
 
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