Back Orbita meya terrestre AN مدار أرضي متوسط Arabic Средна околоземна орбита Bulgarian Òrbita terrestre mitjana Catalan Mittlere Erdumlaufbahn German Órbita circular intermedia Spanish مدار میانی زمین Persian Orbite terrestre moyenne French מסלול לווייני בינוני HE मध्य भू कक्षा Hindi

Medium Earth orbit

Orbit size comparison of GPS, GLONASS, Galileo, BeiDou-2, and Iridium constellations, the International Space Station, the Hubble Space Telescope, and geostationary orbit (and its graveyard orbit), with the Van Allen radiation belts and the Earth to scale.[a]
The Moon's orbit is around 9 times as large as geostationary orbit.[b] (In the SVG file, hover over an orbit or its label to highlight it; click to load its article.)
To-scale diagram of low, medium, and high Earth orbits

A medium Earth orbit (MEO) is an Earth-centered orbit with an altitude above a low Earth orbit (LEO) and below a high Earth orbit (HEO) – between 2,000 and 35,786 km (1,243 and 22,236 mi) above sea level.[1]

The boundary between MEO and LEO is an arbitrary altitude chosen by accepted convention, whereas the boundary between MEO and HEO is the particular altitude of a geosynchronous orbit, in which a satellite takes 24 hours to circle the Earth, the same period as the Earth’s own rotation. All satellites in MEO have an orbital period of less than 24 hours, with the minimum period (for a circular orbit at the lowest MEO altitude) about 2 hours.[2]

Satellites in MEO orbits are perturbed by solar radiation pressure, which is the dominating non-gravitational perturbing force.[3] Other perturbing forces include: Earth's albedo, navigation antenna thrust, and thermal effects related to heat re-radiation.

The MEO region includes the two zones of energetic charged particles above the equator known as the Van Allen radiation belts, which can damage satellites’ electronic systems without special shielding.[4]

A medium Earth orbit is sometimes called mid Earth orbit[1] or intermediate circular orbit (ICO).[2]


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  1. ^ a b Catalog of Earth Satellite Orbits. NASA Earth Observatory. 4 September 2009. Accessed 2 May 2021.
  2. ^ a b "Definitions of geocentric orbits from the Goddard Space Flight Center". User support guide: platforms. NASA Goddard Space Flight Center. Archived from the original on 27 May 2010. Retrieved 8 July 2012.
  3. ^ Bury, Grzegorz; Sośnica, Krzysztof; Zajdel, Radosław; Strugarek, Dariusz (February 2020). "Toward the 1-cm Galileo orbits: challenges in modeling of perturbing forces". Journal of Geodesy. 94 (2): 16. Bibcode:2020JGeod..94...16B. doi:10.1007/s00190-020-01342-2.
  4. ^ "Popular Orbits 101". Aerospace Security. 26 October 2020. Accessed 2 May 2021.

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