How Can Spherical Trigonometry Help Calculate the Sun's Path?

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SUMMARY

This discussion focuses on using spherical trigonometry and calculus to accurately calculate the sun's path, particularly considering the Earth's axial tilt. The participants suggest that while a simple sine function may suffice for daily calculations, incorporating a secondary sine function with a yearly period is necessary for more precise modeling. They also recommend exploring alternative mathematical functions, such as raising the sine function to a power, to better fit the sun's trajectory. The conversation highlights the importance of considering both daily and yearly variations in solar position.

PREREQUISITES
  • Spherical trigonometry fundamentals
  • Basic calculus concepts
  • Understanding of sine and cosine functions
  • Knowledge of Earth's axial tilt and its effects on solar position
NEXT STEPS
  • Research spherical trigonometry applications in astronomy
  • Explore advanced sine function modeling techniques
  • Study the effects of Earth's axial tilt on solar calculations
  • Learn about observational astronomy methods for solar path analysis
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Astronomy students, mathematicians, and anyone interested in accurately modeling solar trajectories using advanced mathematical techniques.

alech4466
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Last semester in my astronomy class, we tried to find an equation that would fit the path of the sun based on measurements we took, but we realized that due to the change in the tilt of the earth, it wouldn't be a simple sine or cosine graph, and we dropped the subject. I was wondering if there is any simple way, using spherical trigonometry, calculus, or something to calculate the equation

Thanks in advance
 
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It really comes down to how accurate you want your equation to be, and over what scale of time. For the day-to-day, a sin function wouldn't be too bad (considering only the regions where it is daylight). To take into account the yearly oscillation of tilt, you would (I think) have to modulate your initial sin function (with a period of a day), with another smaller-amplitude sin function (with a period of a year).

If you looked at the situation in more detail (e.g. the geometry) you might find that simply 'sin' isn't the best function. Perhaps sin raised to some power would be better etc etc.

I'm sure the answer is readily available out there. Have you tried a google search? Hopefully an observational astronomer will chime in---I'm sure they have the specific answer.
 
I've done a google search, but I didn't find anything.

When we tried to find the equation, we tried just using a normal sine equation over the period of a day, not taking the oscillation of tilt into account

Thanks
 

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