Sun elevation for ISS visibility

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  • Thread starter Thread starter Cristiano
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SUMMARY

The discussion focuses on calculating the Sun elevation as viewed from the International Space Station (ISS) to determine visibility. A specific case is presented where the ISS has a magnitude of -3.8 and a Sun elevation of -19.9 degrees. The participants highlight the impact of atmospheric refraction on visibility calculations and inquire about the lowest Sun elevation necessary for the ISS to remain outside the Earth's shadow. The need for formulas to perform these calculations is emphasized.

PREREQUISITES
  • Understanding of orbital mechanics related to the ISS
  • Knowledge of atmospheric refraction effects
  • Familiarity with astronomical magnitude scales
  • Basic proficiency in trigonometric calculations for elevation angles
NEXT STEPS
  • Research the formulas for calculating Sun elevation from the ISS
  • Explore the effects of atmospheric refraction on astronomical observations
  • Learn about the visibility conditions of satellites in low Earth orbit
  • Investigate the relationship between ISS altitude and Earth's shadow geometry
USEFUL FOR

Astronomers, satellite tracking enthusiasts, and anyone interested in the visibility of the ISS and related astronomical phenomena.

Cristiano
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I use several web sites to search the visible passes of the ISS over a given location.
Then I calculate the Sun elevation as seen from the ISS and I get surprisingly low elevations; for example, I get ISS magnitude= -3.8 and Sun elevation at the ISS= -19.9 deg.
I suppose that the atmospheric refraction is very high, but what's the lowest Sun elevation to consider the ISS outside the Earth's shadow?

Thank you
 
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You can look up the ISS height and the radius of Earth and calculate it yourself.

-19.9 is just at the edge of visibility.
 
Please, would you post the formulas?
 

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