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ISS Pass Time Predictor

Calculate when the International Space Station will be visible from your location.

Tested tool guide Tested browser tools Checked August 16, 2026

What ISS Pass Time Predictor does and how it behaves

The International Space Station circles Earth every 92 minutes at about 7.66 km/s, and at its best it is the brightest moving object in the night sky - brighter than any star. Give this tool your location and it predicts the passes ahead: when to go outside, how high the station will climb, which direction to look, and how bright it will be. The one thing that surprises nearly everyone: the ISS is not visible every night, and each pass lasts only a few minutes.

How the result is produced

1

From orbital elements to a pass list

The station's orbit is described by a snapshot of its position and motion, called orbital elements. Propagating those elements forward produces the ground track - where the station will be at every moment. A pass is any interval in which that track rises above a minimum elevation above your horizon. The tool then keeps only the passes where the station is lit by the sun while your sky is dark enough to see it.

2

Why visibility comes in waves

Whether a pass is visible depends on the beta angle - the angle between the station's orbital plane and the sun. When the angle is small, the station dips into Earth's shadow each orbit, so visible passes are brief and low, near dawn and dusk. When it is large, the station stays sunlit for whole orbits and can sail overhead after dark. The angle cycles over about two months, so passes arrive in runs of nights, then a lull.

Good uses

  • Checking tonight's sky: you enter your location, scan the next 24 hours, and pick the pass that climbs highest to drag the family outside for a five-minute look.
  • Planning a photograph: a high pass can be captured as a clean streak across a fixed frame, and you need the exact start time and the compass direction the station appears from to aim the camera and preset focus.
  • Confirming a sighting: a bright, silent point of light glides across the sky, and you check whether a predicted pass matches the time, duration, and direction you saw - separating the ISS from a plane or another satellite.

Limits and checks

  • Fresh data matters: orbital elements age quickly, and the station is periodically reboosted or maneuvered to dodge debris. A prediction built from stale elements can be minutes off or miss a pass entirely, so recheck close to the date you plan to observe.
  • Listed does not mean seen: a pass in twilight can be washed out, and one that barely clears the minimum elevation can be hidden behind houses, trees, or horizon haze. The station is above the horizon for only four to six minutes, so a cloudy minute is a missed pass.
  • Read the directions correctly: the rise and set points are compass bearings, and the maximum elevation happens near the middle of the pass. Staring at the peak direction when the pass begins will miss it, and brightness is quoted in magnitudes, where a smaller number means a brighter object.

Common questions

Why does the tool show no visible passes for days, then several nights in a row?

That is normal, not an error. ISS visibility runs in cycles set by the beta angle - the tilt between the station's orbit and the sun. When the geometry keeps the station in Earth's shadow during your night, nothing is visible. A week or two later the angle shifts and passes return, sometimes two or three in one night.

It crossed the sky in a few minutes without blinking - was that really the ISS?

Almost certainly. The ISS takes four to six minutes to cross the sky, shows a steady light, and makes no sound, while aircraft blink, linger, and can turn. If the time and direction match a predicted pass from your location, that confirms it. A handful of other satellites are nearly as bright, but the ISS is by far the most common explanation.

References and verification

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