An orbital pass (or simply pass) is the period in which a spacecraft is above the local horizon, and thus available for line-of-sight communication with a given ground station, receiver, or relay satellite, or for visual sighting. The beginning of a pass is termed acquisition of signal (AOS); the end of a pass is termed loss of signal (LOS). ^[1] The point at which a spacecraft comes closest to a ground observer is the time of closest approach (TCA). ^[1]

Timing and duration

The timing and duration of passes depends on the characteristics of the orbit a satellite occupies, as well as the ground topography and any occulting objects on the ground (such as buildings), or in space (for planetary probes, or for spacecraft using relay satellites). ^[2] The longest duration ground pass will be experienced by an observer directly on the ground track of the satellite. ^[3] Path loss is greatest toward the start and end of a ground pass, ^[4] as is Doppler shifting for Earth-orbiting satellites. ^[5]

Satellites in geosynchronous orbit may be continuously visible from a single ground station, whereas satellites in low Earth orbit only offer short-duration ground passes ^[3] (although longer contacts may be made via relay satellite networks such as TDRSS). Satellite constellations, such as those of satellite navigation systems, may be designed so that a minimum subset of the constellation is always visible from any point on the Earth, thereby providing continuous coverage. ^[2]

Prediction and visibility

A number of web-based and mobile applications produce predictions of passes for known satellites. ^[6] In order to be observed with the naked eye, a spacecraft must reflect sunlight towards the observer; thus, naked-eye observations are generally restricted to twilight hours, during which the spacecraft is in sunlight but the observer is not. A satellite flare occurs when sunlight is reflected by flat surfaces on the spacecraft. The International Space Station, the largest artificial satellite of Earth, has a maximum apparent magnitude of –5.9, ^[7] brighter than the planet Venus. ^[8]

See also

• Ground track, the path on the surface of the Earth directly below a satellite
• Satellite revisit period, the time elapsed between observations of the same point on Earth by a satellite
• Satellite watching, as a hobby

References