Open-Galileo

Earth orbit in real time

Track satellites around the living Earth

Open-Galileo combines a 3D globe, propagated satellite positions, searchable NORAD objects, simulated time, and a local sky view. Follow an orbit globally, then understand where the object appears above an observer on Earth.

How satellite tracking works

A satellite tracker starts with orbital elements that describe an object’s orbit at a reference time. Software propagates those elements forward to estimate position and velocity. Open-Galileo displays the result in an Earth-centered 3D scene and updates the simulation clock so users can compare live and accelerated motion.

The catalog identifies many objects with a NORAD catalog number. Search by common name or NORAD number, select an object, and inspect it relative to Earth. Because orbital elements age and atmospheric drag varies, displayed positions are estimates rather than navigational guarantees.

3D Earthorbit positions in an Earth-centered frame
NORAD IDssearchable catalog identifiers
Live timeor accelerated orbital simulation
From Earthconnect global orbit to the observer’s sky

How to use the Open-Galileo satellite map

  1. Launch the explorer and keep Globe selected.
  2. Use Layers to make sure Satellites are visible.
  3. Search a spacecraft name or NORAD catalog number.
  4. Select the object to inspect details and focus the globe.
  5. Pause, run live, or accelerate time to watch the orbit evolve.
  6. Save an object and home location to prepare for pass-alert features.

Low, medium, and geostationary orbit

Low Earth orbit

Low Earth orbit, or LEO, contains many Earth-observation spacecraft, crewed vehicles, and communications constellations. These satellites move quickly across the local sky and complete an orbit in roughly an hour and a half to a few hours, depending on altitude.

Medium Earth orbit

Medium Earth orbit includes navigation constellations. Their longer orbital periods and higher altitude provide broad coverage while still moving relative to an observer.

Geostationary orbit

A geostationary satellite orbits above the equator with a period matched to Earth’s rotation. From the ground it appears nearly fixed in one direction, making the orbit useful for communications and weather observation.

Why satellites become visible

Most visible satellites do not emit their own light. They reflect sunlight. A favorable pass occurs when the observer is in darkness or twilight while the spacecraft remains illuminated above Earth’s shadow. Brightness also depends on distance, orientation, size, surface material, and atmospheric clarity.

Aircraft can resemble satellites at first glance, but aircraft usually blink, show colored navigation lights, or change apparent speed. A satellite typically looks like a steady point moving smoothly across the stars. Very bright flashes can occur when reflective surfaces align with the observer.