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— CH. 1 · EARTH'S ORBITAL NEIGHBORHOOD —

Geocentric orbit

6 min listen · Ch. 1 of 5
5 sections
  • Geocentric orbit is the technical name for any path around Earth, whether traced by the Moon or by a human-made machine. By 1997, NASA estimated 2,465 artificial satellite payloads circled the planet. The Goddard Space Flight Center tracked 6,216 additional pieces of space debris alongside them. Together, those figures capture only a snapshot of a neighborhood that had been filling since the first rockets flew. Why does anything stay in orbit at all? Why are some satellites clustered barely above the atmosphere while others sit tens of thousands of kilometers away? And what eventually happens to a machine when its working life is over? Earth's Moon, the original resident of geocentric space, circles at an average altitude of 384,403 kilometers. That places it at the outermost edge of a system whose inner boundary barely clears the upper atmosphere.

  • Reaching a low Earth orbit requires a horizontal speed of about 7.8 kilometers per second. A spacecraft at that velocity finds Earth's surface curving away at the same rate it falls. The result is a continuous arc that never reaches the ground.

    The fastest crewed airplane speed ever recorded, excluding deorbiting spacecraft, was 2.2 kilometers per second. That record was set in 1967 by the North American X-15. The gap between 2.2 and 7.8 kilometers per second underscores how different atmospheric flight is from orbital flight.

    Reaching orbital velocity at 600 kilometers altitude demands about 36 megajoules per kilogram. That figure is six times the energy needed simply to climb to that altitude without any forward speed. Beyond orbital velocity lies one more threshold. At about 11.2 kilometers per second, Earth's gravity can no longer hold an object back. That boundary marks the outer edge of geocentric space.

  • At 160 kilometers above Earth's surface, a satellite completes one orbit in approximately 90 minutes. That altitude marks the lower boundary of low Earth orbit, a band stretching upward to 2,000 kilometers. Circular orbital speed at that lower boundary reaches about 8 kilometers per second.

    Medium Earth orbit begins at 2,000 kilometers and climbs to the geosynchronous altitude of 35,786 kilometers. Within that band sits the semi-synchronous orbit at approximately 20,200 kilometers, where one circuit takes roughly 12 hours. Geosynchronous orbit occupies that upper boundary, and its period equals exactly one sidereal day. A sidereal day lasts 23 hours, 56 minutes, and 4.091 seconds, slightly shorter than the 24-hour calendar day. At geosynchronous altitude, orbital speed drops to approximately 3 kilometers per second.

    A geosynchronous orbit with an inclination of exactly zero degrees is called geostationary. From the ground, a satellite in that position appears motionless, fixed at a single point in the sky. This orbit also carries a second name: the Clarke orbit, named after the writer Arthur C. Clarke.

    Highly elliptical orbits extend their apogee above 35,786 kilometers while dropping their perigee as low as about 1,000 kilometers. Satellites using these paths spend the majority of their time near apogee, gaining prolonged coverage of high-latitude regions.

    Satellites that outlive their usefulness are often moved into the graveyard orbit. This disposal zone sits a few hundred kilometers above geosynchronous altitude, keeping retired spacecraft clear of active ones.

  • A perfectly circular orbit has an eccentricity of exactly zero. Even a small deviation produces an ellipse, with a perigee closest to Earth and an apogee farthest from it. At higher eccentricities, orbits stretch into long ovals; above eccentricity 1, the path becomes hyperbolic and the object escapes Earth's gravity entirely.

    Walter Hohmann gave his name to a particular orbital maneuver: a two-impulse path that moves a spacecraft from one circular orbit to another. A variant called the geosynchronous transfer orbit applies the same principle to carry satellites from low Earth orbit up to geosynchronous altitude.

    The Molniya orbit combines a 63.4-degree inclination with a period of roughly half a sidereal day. A satellite in that configuration spends most of its time near apogee, hovering over a designated area of Earth. The Tundra orbit shares the 63.4-degree inclination but extends its period to a full sidereal day. Both designs cause satellites to spend most of their time over a single designated region of Earth.

    A polar orbit passes above or nearly above both poles on each revolution, requiring an inclination of 90 degrees or very close to it. This crossing pattern ensures the satellite eventually covers every part of Earth's surface. The sun-synchronous orbit pairs altitude and inclination so that the satellite crosses any given point at the same local solar time on every pass. That consistency makes it useful for imaging, spy, and weather satellites.

    More than 160 satellites have gathered at the two libration points, located at 105 degrees west and 75 degrees east. Spacecraft whose perigee dips into low Earth orbit, however, face a force no mission planner can work around: atmospheric drag.

  • More than 16,291 objects launched into Earth orbit have already re-entered the atmosphere. Atmospheric drag is the mechanism at work. It steadily reduces the altitude of any spacecraft whose path passes through the upper reaches of the atmosphere. How quickly drag acts depends on the satellite's cross-sectional area and mass, and on how dense the upper atmosphere happens to be.

    Below about 300 kilometers, the pace of orbital decay quickens sharply, and satellite lifetimes shrink to days. At 180 kilometers, the remaining lifespan is measured in hours, after which the spacecraft vaporizes in the atmosphere. An object arriving from outside Earth's gravity well with sufficient speed traces a capture trajectory, accelerating as it swings around the planet. Without an engine to slow it into a stable orbit, it departs along an escape trajectory and does not return.

Common questions

What is a geocentric orbit?

A geocentric orbit is any path around Earth taken by a natural or artificial object, including the Moon and human-made satellites. By 1997, NASA estimated 2,465 artificial satellite payloads were in geocentric orbits, alongside 6,216 pieces of space debris tracked by the Goddard Space Flight Center.

What speed does a satellite need to maintain a geocentric low Earth orbit?

A satellite in low Earth orbit must travel at about 7.8 kilometers per second horizontally. At that speed, Earth's surface curves away beneath the spacecraft at the same rate it falls, creating a continuous loop around the planet.

What is the difference between a geostationary and a geosynchronous geocentric orbit?

A geosynchronous orbit matches Earth's rotation period, completing one circuit every sidereal day (23 hours, 56 minutes, and 4.091 seconds) at an altitude of 35,786 kilometers. A geostationary orbit is a geosynchronous orbit with an inclination of exactly zero degrees, causing the satellite to appear fixed at a single point in the sky from the ground.

Who is the Clarke geocentric orbit named after, and at what altitude does it sit?

The Clarke orbit is named after the writer Arthur C. Clarke. It refers to geostationary orbit at 35,786 kilometers altitude, where a satellite with zero inclination appears motionless in the sky as seen from the ground.

How long can a satellite survive in geocentric orbit before re-entering the atmosphere?

Below about 300 kilometers, orbital decay is rapid and satellite lifetimes shrink to days. At 180 kilometers, only hours remain before the spacecraft vaporizes during re-entry.

What are the key characteristics of the Molniya geocentric orbit?

The Molniya orbit is a highly elliptical geocentric orbit with an inclination of 63.4 degrees and a period of roughly half a sidereal day, or about 12 hours. A satellite in this orbit spends most of its time near apogee, providing extended coverage over a designated area of Earth.

All sources

10 references cited across the entry

  1. 1Satellite Situation Report, 1997NASA Goddard Space Flight Center — 2000-02-01
  2. 2Getting to Low Earth OrbitJames V. H. Hill — April 1999
  3. 3X-15 WalkaroundLinda Shiner — Air & Space Magazine — November 1, 2007
  4. 4100 lbs to Low Earth Orbit (LEO): Small-Payload Launch OptionsP. Dimotakis et al. — The Mitre Corporation — October 1999
  5. 5Atmospheric Science and EnvironmentS. N. Ghosh — Allied Publishers — 2000
  6. 6Satellite Lifetimes and Solar ActivityJohn Kennewell et al. — Commonwealth of Australia Bureau of Weather, Space Weather Branch — 2011
  7. 7Earth Fact SheetDavid R. Williams — NASA — November 17, 2010
  8. 8Jonathan's Space ReportJonathan McDowell — 24 May 1998