B Enlarging Planetary Orbits: Evidence of the Solar System's Evolution?

AI Thread Summary
Evidence suggests that planetary orbits can change over time due to gravitational influences, with a long-term trend of outward movement as the Sun loses mass. However, these changes are often overshadowed by short-term variations. Historical data indicates significant orbital adjustments in the early solar system, particularly with Jupiter. Current observations show that Earth's orbit has increased on average in the short term but decreased over a longer timeline. Overall, the dynamics of planetary orbits reflect complex interactions and evolutionary trends within the solar system.
Sanborn Chase
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Is there any evidence of the enlargement of planetary orbits over time? Are the planets moving further from the sun?
 
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The orbits change their semi-major axis all the time, in both directions, based on the gravitational influence of other objects. There is a long-term trend outwards as the Sun loses mass, but over timescales we can observe this is completely drowned by the short-term variations.
 
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Thanks for your response, mfb. It's a great help.
 
To add to mfb's reply, here are two tables which give how orbital elements change with time.
The first is over the time period of 1800AD-2050AD:
https://ssd.jpl.nasa.gov/txt/p_elem_t1.txt

and the second for the time period of 3000BC-3000AD
https://ssd.jpl.nasa.gov/txt/p_elem_t2.txt

Note that in the first column (a), which gives the average orbital distance in AU and the change in AU per century, the Earth's orbit (EM bary), increases on average over the shorter time scale, but decreases on average over the longer time scale.
 
Thanks, Guys.
 
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