Does the Saros Cycle Provide Accurate Eclipse Predictions Across Time?

  • Context: Undergrad 
  • Thread starter Thread starter lewis198
  • Start date Start date
  • Tags Tags
    Cycle Time
Click For Summary

Discussion Overview

The discussion centers on the Saros cycle and its reliability for predicting eclipses over long periods, including thousands of years into the past or future. Participants explore the implications of Earth's changing rotation and orbital dynamics on eclipse timing and location.

Discussion Character

  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that while the Saros cycle period is approximately 6585⅓ days, the accuracy of eclipse predictions is affected by the variable rotation rate of the Earth, which is influenced by factors like volcanic eruptions and tidal forces from the moon.
  • There is a discussion about the predictability of the Earth's orbit and how it changes over time, with some arguing that these changes can lead to discrepancies in historical eclipse locations compared to records.
  • One participant questions the order of error in eclipse predictions, wondering if it is negligible compared to the Saros cycle period and if it is related to the n-body problem.
  • Another participant notes that while the timing of eclipses is relatively stable, the location is more variable due to the changing length of the day, which is affected by tidal friction and random geological events.
  • Some participants clarify that the Earth's mass does not decrease over time, and the distribution of mass, rather than total mass, is what influences rotation and eclipse predictions.
  • Post-glacial rebound is mentioned as a significant factor affecting the Earth's crust and its implications for measuring changes in the length of the day and the barycentre of the Earth.

Areas of Agreement / Disagreement

Participants express differing views on the effects of Earth's mass and rotation on eclipse predictions, with no consensus reached on the extent of these influences or the implications for the accuracy of the Saros cycle over time.

Contextual Notes

Participants highlight limitations in understanding the exact effects of various factors on eclipse predictions, including the unpredictability of geological events and the complexities of the n-body problem.

lewis198
Messages
95
Reaction score
0
Hey guys.
I was wondering, does the period of the Saros cycle stay the same across all time? for example, using the saros cycle could you accurately predict eclipse times thousands of years into the past or future?
 
Astronomy news on Phys.org
Depends how accurately you mean "stay the same". The rotation rate of the Earth (ie length of a day) is the most variable since every volcanc erruption, tidal wave or earthquake has an effect. It is also slowing at a predicatable rate due to tidal braking from the moon. The Earth's orbit is also changing reasonably predictably.

When looking at ancient eclipses we can predict when and where they occurred but the "where" often differs from historical records. This is the best way of studying historical changes in the Earht's rotation rate.
 
OK, so the decreasing mass of the Earth affects the location of the eclipse.
So the when would essentially be the same? If the error is residual, what kind of order are we looking at? the Saros Cycle period is approximately 6585⅓ days. If there is any error, is it <<6585.5 days? And would it be unsolvable because of the n-body problem? Is it negligible?
 
When the eclipse happens depends on the position of the Earth and moon in orbit. Although technically chaotic because they depend on every othe piece of mass in the solar system these are relatively stable over long periods. Over very long periods the length of the cycle will increase because the moon is dirifting away from earth, this will also eventually stop total eclipses since the moon will be too small to cover the sun.

The 'where' depends on the length of the day which changes much more quickly, both in a predictable manner due to tidal friction from the moon lengthening the day and from random events.
The day is predicted to increase by about 2.5 ms/century from the effect of the moon but historical eclipses allow us to calculate it at about 1.7 ms/centrury. The missing 0.8 ms/century comes from changes in the earth.

The mass of the Earth doesn't matter (and is in fact actually increasing as comets land on us) it is the distribution of mass. Like a spinning ice skater if mass moves out toward the surface the rotation slows down - this provides the main random unknown. The biggest cause is probably the crust rebounding after the weight of ice removed at the end of the last ice age!
 
An admittedly technical point, but the Earth's mass does not decrease over time - as noted by mgb. I also doubt the mass of ice on the surface of earth, melting or otherwise, is sufficient to influence plate tectonics.
 
Last edited:
Chronos said:
I also doubt the mass of ice on the surface of earth, melting or otherwise, is sufficient to influence plate tectonics.
"Post-glacial rebound" as it's called does have quite a large effect for northern europe. In the UK, Scotland has been rising since the weight of the ice was removed and London is sinking. This movement is at around the rate the sea level is rising - but unfortunately in the opposite direction.

This effect is large enough to have to be corrected for in Long Baseline interferometry between radio telescopes in Cambridge and other countries.
In addition the change in the length of the day and the barycentre of the Earth is continually monitored and corrections published. Although because these numbers are needed to accurately throw ICBMs around, the results are only published later when no-longer current.
After major seismic events a correction has to be hurridly calculated and published.
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
Replies
5
Views
996
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 1 ·
Replies
1
Views
5K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 14 ·
Replies
14
Views
11K
  • · Replies 87 ·
3
Replies
87
Views
11K
Replies
1
Views
2K