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Low Earth orbit

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A view from the International Space Station in a low Earth orbit (LEO) at about 400 km (250 mi), with yellow-green airglow visible at Earth's horizon, where roughly at an altitude of 100 km (62 mi) the boundary between Earth and outer space lies and flying speeds reach orbital velocities.

A low Earth orbit (LEO) is an orbit around Earth with a period of 128 minutes or less (making at least 11.25 orbits per day) and an eccentricity less than 0.25.[1] Most of the artificial objects in outer space are in LEO, peaking in number at an altitude around 800 km (500 mi),[2] while the farthest in LEO, before medium Earth orbit (MEO), have an altitude of 2,000 kilometers, about one-third of the radius of Earth and near the beginning of the inner Van Allen radiation belt.

The term LEO region is used for the area of space below an altitude of 2,000 km (1,200 mi) (about one-third of Earth's radius).[3] Objects in orbits that pass through this zone, even if they have an apogee further out or are sub-orbital, are carefully tracked since they present a collision risk to the many LEO satellites.

No human spaceflights other than the lunar missions of the Apollo program (1968-1972) and the 2024 Polaris Dawn have taken place beyond LEO. All space stations to date have operated geocentric within LEO.

Defining characteristics

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A wide variety of sources[4][5][6] define LEO in terms of altitude. The altitude of an object in an elliptic orbit can vary significantly along the orbit. Even for circular orbits, the altitude above ground can vary by as much as 30 km (19 mi) (especially for polar orbits) due to the oblateness of Earth's spheroid figure and local topography. While definitions based on altitude are inherently ambiguous, most of them fall within the range specified by an orbit period of 128 minutes because, according to Kepler's third law, this corresponds to a semi-major axis of 8,413 km (5,228 mi). For circular orbits, this in turn corresponds to an altitude of 2,042 km (1,269 mi) above the mean radius of Earth, which is consistent with some of the upper altitude limits in some LEO definitions.

The LEO region is defined by some sources as a region in space that LEO orbits occupy.[3][7][8] Some highly elliptical orbits may pass through the LEO region near their lowest altitude (or perigee) but are not in a LEO orbit because their highest altitude (or apogee) exceeds 2,000 km (1,243 mi). Sub-orbital objects can also reach the LEO region but are not in a LEO orbit because they re-enter the atmosphere. The distinction between LEO orbits and the LEO region is especially important for analysis of possible collisions between objects which may not themselves be in LEO but could collide with satellites or debris in LEO orbits.

Orbital characteristics

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The mean orbital velocity needed to maintain a stable low Earth orbit is about 7.8 km/s (4.8 mi/s), which translates to 28,000 km/h (17,000 mph). However, this depends on the exact altitude of the orbit. Calculated for a circular orbit of 200 km (120 mi) the orbital velocity is 7.79 km/s (4.84 mi/s), but for a higher 1,500 km (930 mi) orbit the velocity is reduced to 7.12 km/s (4.42 mi/s).[9] The launch vehicle's delta-v needed to achieve low Earth orbit starts around 9.4 km/s (5.8 mi/s).

The pull of gravity in LEO is only slightly less than on the Earth's surface. This is because the distance to LEO from the Earth's surface is much less than the Earth's radius. However, an object in orbit is in a permanent free fall around Earth, because in orbit the gravitational force and the centrifugal force balance each other out.[a] As a result, spacecraft in orbit continue to stay in orbit, and people inside or outside such craft continuously experience weightlessness.

Objects in LEO orbit Earth between the denser part of the atmosphere and below the inner Van Allen radiation belt. They encounter atmospheric drag from gases in the thermosphere (approximately 80–600 km above the surface) or exosphere (approximately 600 km or 400 mi and higher), depending on orbit height. Satellites in orbits that reach altitudes below 300 km (190 mi) decay quickly due to atmospheric drag.

Equatorial low Earth orbits (ELEO) are a subset of LEO. These orbits, with low orbital inclination, allow rapid revisit times over low-latitude locations on Earth. Prograde equatorial LEOs also have lower delta-v launch requirements because they take advantage of the Earth's rotation. Other useful LEO orbits including polar orbits and Sun-synchronous orbits have a higher inclinations to the equator and provide coverage for higher latitudes on Earth. Some of the first generation of Starlink satellites used polar orbits which provide coverage everywhere on Earth. Later Starlink constellations orbit at a lower inclination and provide more coverage for populated areas.

Higher orbits include medium Earth orbit (MEO), sometimes called intermediate circular orbit (ICO), and further above, geostationary orbit (GEO). Orbits higher than low orbit can lead to early failure of electronic components due to intense radiation and charge accumulation.

In 2017, "very low Earth orbits" (VLEO) began to be seen in regulatory filings. These orbits, below about 450 km (280 mi), require the use of novel technologies for orbit raising because they operate in orbits that would ordinarily decay too soon to be economically useful.[10][11]

Use

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Roughly half an orbit of the International Space Station

A low Earth orbit requires the lowest amount of energy for satellite placement. It provides high bandwidth and low communication latency. Satellites and space stations in LEO are more accessible for crew and servicing.

Since it requires less energy to place a satellite into a LEO, and a satellite there needs less powerful amplifiers for successful transmission, LEO is used for many communication applications, such as the Iridium phone system. Some communication satellites use much higher geostationary orbits and move at the same angular velocity as the Earth as to appear stationary above one location on the planet.

Disadvantages

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Unlike geosynchronous satellites, satellites in low orbit have a small field of view and can only observe and communicate with a fraction of the Earth at a given time. This means that a large network (or constellation) of satellites is required to provide continuous coverage.

Satellites at lower altitudes of orbit are in the atmosphere and suffer from rapid orbital decay, requiring either periodic re-boosting to maintain stable orbits, or the launching of replacements for those that re-enter the atmosphere. The effects of adding such quantities of vaporized metals to Earth's stratosphere are potentially of concern but currently unknown.[12]

Examples

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Former

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  • GOCE (2009-2013), an ESA gravimetry mission, orbited at about 255 km (158 mi).

In fiction

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Space debris

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The LEO environment is becoming congested with space debris because of the frequency of object launches.[17] This has caused growing concern in recent years, since collisions at orbital velocities can be dangerous or deadly. Collisions can produce additional space debris, creating a domino effect known as Kessler syndrome. NASA's Orbital Debris Program tracks over 25,000 objects larger than 10 cm diameter in LEO, while the estimated number between 1 and 10 cm is 500,000, and the number of particles bigger than 1 mm exceeds 100 million.[18] The particles travel at speeds up to 7.8 km/s (28,000 km/h; 17,500 mph), so even a small impact can severely damage a spacecraft.[19]

See also

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Notes

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  1. ^ It is important to note here that “free fall” by definition requires that gravity is the only force acting on the object. That definition is still fulfilled when falling around Earth, as the other force, the centrifugal force is a fictitious force.

References

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  1. ^ "Current Catalog Files". Archived from the original on 26 June 2018. Retrieved 13 July 2018. LEO: Mean Motion > 11.25 & Eccentricity < 0.25
  2. ^ Muciaccia, Andrea (2021). Fragmentations in low Earth orbit: event detection and parent body identification (Thesis). doi:10.13140/RG.2.2.27621.52966.
  3. ^ a b "IADC Space Debris Mitigation Guidelines" (PDF). INTER-AGENCY SPACE DEBRIS COORDINATION COMMITTEE: Issued by Steering Group and Working Group 4. September 2007. Archived (PDF) from the original on 17 July 2018. Retrieved 17 July 2018. Region A, Low Earth Orbit (or LEO) Region – spherical region that extends from the Earth's surface up to an altitude (Z) of 2,000 km
  4. ^ "Definition of LOW EARTH ORBIT". Merriam-Webster Dictionary. Archived from the original on 8 July 2018. Retrieved 8 July 2018.
  5. ^ "Frequently Asked Questions". FAA. Archived from the original on 2 June 2020. Retrieved 14 February 2020. LEO refers to orbits that are typically less than 2,400 km (1,491 mi) in altitude.
  6. ^ Campbell, Ashley (10 July 2015). "SCaN Glossary". NASA. Archived from the original on 3 August 2020. Retrieved 12 July 2018. Low Earth Orbit (LEO): A geocentric orbit with an altitude much less than the Earth's radius. Satellites in this orbit are between 80 and 2000 kilometers above the Earth's surface.
  7. ^ "What Is an Orbit?". NASA. David Hitt : NASA Educational Technology Services, Alice Wesson : JPL, J.D. Harrington : HQ;, Larry Cooper : HQ;, Flint Wild : MSFC;, Ann Marie Trotta : HQ;, Diedra Williams : MSFC. 1 June 2015. Archived from the original on 27 March 2018. Retrieved 8 July 2018. LEO is the first 100 to 200 miles (161 to 322 km) of space.{{cite news}}: CS1 maint: others (link)
  8. ^ Steele, Dylan (3 May 2016). "A Researcher's Guide to: Space Environmental Effects". NASA. p. 7. Archived from the original on 17 November 2016. Retrieved 12 July 2018. the low-Earth orbit (LEO) environment, defined as 200–1,000 km above Earth's surface
  9. ^ "LEO parameters". www.spaceacademy.net.au. Archived from the original on 11 February 2016. Retrieved 12 June 2015.
  10. ^ Crisp, N. H.; Roberts, P. C. E.; Livadiotti, S.; Oiko, V. T. A.; Edmondson, S.; Haigh, S. J.; Huyton, C.; Sinpetru, L.; Smith, K. L.; Worrall, S. D.; Becedas, J. (August 2020). "The Benefits of Very Low Earth Orbit for Earth Observation Missions". Progress in Aerospace Sciences. 117: 100619. arXiv:2007.07699. Bibcode:2020PrAeS.11700619C. doi:10.1016/j.paerosci.2020.100619. S2CID 220525689.
  11. ^ Messier, Doug (3 March 2017). "SpaceX Wants to Launch 12,000 Satellites". Parabolic Arc. Archived from the original on 22 January 2020. Retrieved 22 January 2018.
  12. ^ "Space Junk is Polluting Earth's Stratosphere with Vaporized Metal". Scientific American.
  13. ^ "Higher Altitude Improves Station's Fuel Economy". NASA. Archived from the original on 15 May 2015. Retrieved 12 February 2013.
  14. ^ Holli, Riebeek (4 September 2009). "NASA Earth Observatory". earthobservatory.nasa.gov. Archived from the original on 27 May 2018. Retrieved 28 November 2015.
  15. ^ "Japan's low altitude satellite Tsubame registered in Guinness World Records". The Japan Times. 30 December 2019. Retrieved 25 June 2024.
  16. ^ "Space station from 2001: A Space Odyssey".
  17. ^ United Nations Office for Outer Space Affairs (2010). "Space Debris Mitigation Guidelines of the Committee on the Peaceful Uses of Outer Space". Inter-Agency Space Debris Coordination Committee (IADC). Retrieved 19 October 2021.
  18. ^ "ARES | Orbital Debris Program Office | Frequently Asked Questions". NASA.gov. Archived from the original on 2 September 2022. Retrieved 2 September 2022.
  19. ^ Garcia, Mark (13 April 2015). "Space Debris and Human Spacecraft". NASA.gov. Archived from the original on 8 September 2022. Retrieved 2 September 2022.

Public Domain This article incorporates public domain material from websites or documents of the National Aeronautics and Space Administration.

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