Next Pass FAQs
How do you determine a visible pass?
The station must be sunlit while your observing point is in darkness or twilight. We compute solar elevation for both you and the ISS at each second of a pass.
What defines pass quality?
Higher maximum elevation, longer duration, and brighter (more negative) magnitude values increase quality; we label the best combinations as “Great Pass!”
Why are there no visible passes right now?
All passes in the next several days may occur in daylight. Try again in a few days; the timing of evening and dawn passes shifts earlier daily.
How accurate are the times?
Predictions generally match official sources within seconds. Atmospheric drag and orbital adjustments can introduce small shifts; re-check close to viewing time.
What should I look for?
The ISS appears as a bright, fast-moving white point with steady brightness (no flashing). It rises in the indicated start direction, peaks near max elevation, then fades toward the end direction.