ISS Live Tracker & Overhead Pass Predictor

Track the International Space Station in real time, view orbital ground tracks, and calculate upcoming visible overhead passes.

Latitude 24.30° N
Longitude 76.80° W
Altitude 418.5 km
Orbital Speed 27,584 km/h
Ground Sub-Point North Atlantic

Equirectangular Orbital Projection

Inclination: 51.6° • Period: 92.6 mins

Visible Overhead Pass Predictions

Select your city to view upcoming high-elevation evening and dawn viewing windows.

Date & Time (Local) Max Elevation Duration Pass Trajectory Visual Brightness
Tonight, 20:42 78° (Direct Overhead) 5m 45s WSW to ENE -3.6 (Extremely Bright)
Tomorrow, 21:30 34° (High Horizon) 4m 10s W to NNE -2.1 (Bright)
Thursday, 19:54 62° (High Overhead) 6m 02s SW to ENE -3.4 (Very Bright)

Expedition Crew Currently in Orbit

Human astronauts and cosmonauts living and conducting science experiments aboard the station.

NASA (USA) Sunita Williams Expedition Commander
NASA (USA) Barry Wilmore Flight Engineer
NASA (USA) Matthew Dominick Flight Engineer (Crew-8)
Roscosmos (Russia) Oleg Kononenko Cosmonaut Commander

How the International Space Station Orbits the Earth

The International Space Station maintains a low Earth orbit (LEO) with an orbital inclination of 51.6 degrees to the equator, allowing supply spacecraft launched from both Cape Canaveral and Baikonur Cosmodrome to rendezvous efficiently.

16 Sunrises and Sunsets

Traveling at nearly 5 miles per second, the ISS completes one revolution around Earth every 92 minutes, experiencing day and night cycles 16 times per day.

Why Ground Tracks Shift West

As the ISS completes each 92-minute orbit, the Earth rotates beneath it eastward by approximately 22.5 degrees of longitude, shifting consecutive ground track waves westward.

Atmospheric Drag & Re-Boosts

Residual atmospheric particles gradually decay the station's altitude by roughly 100 meters per day, requiring periodic thruster re-boosts by docked Progress or Cygnus cargo ships.

About this tool

How to use it

  1. Observe the real-time telemetry dashboard updating the International Space Station's latitude, longitude, speed, and altitude every second.
  2. Track the orbital ground track path across the interactive 2D world projection map with day/night illumination.
  3. Select your city or enter geographic coordinates in the Overhead Pass Predictor to compute upcoming visible passes.
  4. Check maximum elevation angles (degrees above horizon), compass entry/exit headings, and expected duration.
  5. View the current Expedition crew manifest and docked spacecraft status.

Why it matters

The International Space Station orbits Earth every 92.6 minutes at 17,500 mph (28,000 km/h) at an altitude of approximately 420 km. Because it reflects sunlight brightly against a twilight sky, it is often visible to the naked eye as a fast-moving star with magnitude rivaling Venus. This tool allows stargazers and educators to track its exact orbital trajectory and predict prime backyard viewing passes.

When to use it

Use when planning evening or morning stargazing sessions to spot the ISS, tracking crew mission rotations, teaching orbital mechanics and satellite inclinations, or calculating overhead visibility windows.

Common questions

What does the ISS look like in the night sky?

To the naked eye, the ISS looks like an extremely bright, non-blinking star or steady white point of light moving swiftly across the sky over 3 to 6 minutes. It does not produce flashing strobe lights like an airplane.

Why is the ISS only visible at dawn or dusk?

The space station is visible from the ground when the observer is in twilight darkness while the station (hundreds of kilometers high) is illuminated by direct sunlight reflecting off its massive solar panel arrays.

What is maximum elevation and why does it matter?

Elevation is measured in degrees from the horizon (0°) to the zenith overhead (90°). Passes with maximum elevations above 40° are brighter, closer, and far easier to see than low-horizon passes obstructed by trees or buildings.

Does this tracker work offline?

Yes! The tracker incorporates high-fidelity Keplerian orbital propagation algorithms that compute continuous orbital positions, ground tracks, and pass predictions locally in your browser.