Low Earth Orbit
Get Low Earth Orbit essential facts below. View Videos or join the Low Earth Orbit discussion. Add Low Earth Orbit to your PopFlock.com topic list for future reference or share this resource on social media.
Low 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.)

A low Earth orbit (LEO) is an Earth-centred orbit close to the Earth, often specified as an orbital period of 128 minutes or less (making 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, with an altitude never more than about one-third of the radius of the Earth.[2]

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

All crewed space stations to date have been in LEO. From 1968 to 1972 the Apollo program's lunar missions sent humans beyond LEO. Since the end of the Apollo program there have been no human spaceflights beyond LEO.

Defining characteristics

A large 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 an LEO Orbit because their highest altitude (or apogee) exceeds 2,000 km (1,242.7 mi). Sub-orbital objects can also reach the LEO region but are not in an 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

The mean orbital velocity needed to maintain a stable low Earth orbit is about 7.8 km/s (28,000 km/h; 17,000 mph), but reduces with increased orbital altitude. Calculated for circular orbit of 200 km (120 mi) it is 7.79 km/s (28,000 km/h; 17,400 mph), and for 1,500 km (930 mi) it is 7.12 km/s (25,600 km/h; 15,900 mph).[9] The delta-v needed to achieve low Earth orbit starts around 9.4 km/s. Atmospheric and gravity drag associated with launch typically adds 1.3-1.8 km/s (4,700-6,500 km/h; 2,900-4,000 mph) to the launch vehicle delta-v required to reach normal LEO orbital velocity of around 7.8 km/s (28,100 km/h; 17,400 mph).[10]

Orbitalaltitudes.jpg

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, by definition, in free fall, since there is no force holding it up. As a result objects in orbit, including people, experience a sense of weightlessness, even though they are not actually without weight.

Objects in LEO 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. Due to atmospheric drag, satellites do not usually orbit below 300 km (190 mi). Objects in LEO orbit Earth between the denser part of the atmosphere and below the inner Van Allen radiation belt.

Equatorial low Earth orbits (ELEO) are a subset of LEO. These orbits, with low inclination to the Equator, allow rapid revisit times of low-latitude places on Earth and have the lowest delta-v requirement (i.e., fuel spent) of any orbit, provided they have the direct (not retrograde) orientation with respect to the Earth's rotation. Orbits with a very high inclination angle to the equator are usually called polar orbits.

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 began to be seen in regulatory filings. These orbits, below about 450 km (280 mi) and referred to as "VLEO", require the use of novel technologies for orbit raising because they operate in orbits that would ordinarily decay too soon to be economically useful.[11][12]

Use of LEO

Roughly half an orbit of the ISS.

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

Unlike geosynchronous satellite, satellites in LEO have a small field of view, only able to observe and communicate with a fraction of the Earth at a time. This means that a network (or "constellation") of satellites is required in order to provide continuous coverage. Satellites in lower regions of LEO also suffer from fast orbital decay, requiring either periodic re-boosting to maintain a stable orbit, or launching replacement satellites when old ones re-enter.

Examples

  • The International Space Station is in a LEO about 400 km (250 mi) to 420 km (260 mi) above Earth's surface,[13] and needs re-boosting a few times a year due to orbital decay.
  • The Iridium telecom satellites orbit at about 780 km (480 mi).
  • Earth observation satellites, also known as remote sensing satellites, including spy satellites and other Earth imaging satellites, use LEO as they are able to see the surface of the Earth more clearly by being closer to it. A majority of artificial satellites are placed in LEO.[14] Satellites can also take advantage of consistent lighting of the surface below via Sun-synchronous LEO orbits at an altitude of about 800 km (500 mi) and near polar inclination. Envisat (2002-2012) is one example.
  • Gravimetry missions such as GOCE orbited at about 255 km (158 mi) to measure Earth's gravity field at highest sensitivity. The mission lifetime was limited because of atmospheric drag. GRACE and GRACE-FO were orbiting at about 500 km (310 mi).* The Hubble Space Telescope orbits at about 540 km (340 mi) above Earth.
  • The Chinese Tiangong-1 station was in orbit at about 355 kilometres (221 mi),[15] until its de-orbiting in 2018.
  • The Chinese Tiangong-2 station was in orbit at about 370 km (230 mi), until its de-orbiting in 2019.

Space debris

The LEO environment is becoming congested with space debris because of the frequency of object launches. This has caused growing concern in recent years, since collisions at orbital velocities can easily be dangerous, and even deadly. Collisions can produce even more space debris in the process, creating a domino effect known as Kessler syndrome. The Combined Space Operations Center, part of United States Strategic Command (formerly the United States Space Command), tracks more than 8,500 objects larger than 10 cm in LEO.[16] There could be approximately one million very dangerous objects larger than 2 millimeters,[17] which are too small to be visible from Earth-based observatories, according to a limited Arecibo Observatory study.[18]

See also

Notes

  1. ^ Orbital periods and speeds are calculated using the relations 4?2R3 = T2GM and V2R = GM, where R, radius of orbit in metres; T, orbital period in seconds; V, orbital speed in m/s; G, gravitational constant, approximately ; M, mass of Earth, approximately .
  2. ^ Approximately 8.6 times (in radius and length) when the moon is nearest ( ÷ ) to 9.6 times when the moon is farthest ( ÷ ).

References

  1. ^ "Current Catalog Files". Retrieved 2018. LEO: Mean Motion > 11.25 & Eccentricity < 0.25
  2. ^ Sampaio, Jarbas; Wnuk, Edwin; Vilhena de Moraes, Rodolpho; Fernandes, Sandro (2014-01-01). "Resonant Orbital Dynamics in LEO Region: Space Debris in Focus". Mathematical Problems in Engineering. 2014: Figure 1: Histogram of the mean motion of the cataloged objects. doi:10.1155/2014/929810.
  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. 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. Retrieved .
  5. ^ "Frequently Asked Questions". FAA. Retrieved . LEO refers to orbits that are typically less than 2,400 km (1,491 mi) in altitude.
  6. ^ Campbell, Ashley (2015-07-10). "SCaN Glossary". NASA. Retrieved . 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. 2015-06-01. Retrieved . LEO is the first 100 to 200 miles (161 to 322 km) of space.CS1 maint: others (link)
  8. ^ Steele, Dylan (2016-05-03). "A Researcher's Guide to: Space Environmental Effects". NASA. p. 7. Retrieved . the low-Earth orbit (LEO) environment, defined as 200-1,000 km above Earth's surface
  9. ^ "LEO parameters". www.spaceacademy.net.au. Retrieved .
  10. ^ Swinerd, Graham (2008). How Spacecraft Fly. Praxis Publishing. pp. 103-104. ISBN 978-0387765723.
  11. ^ 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. (2020-08). "The Benefits of Very Low Earth Orbit for Earth Observation Missions". Progress in Aerospace Sciences. 117: 100619. arXiv:2007.07699. doi:10.1016/j.paerosci.2020.100619. Check date values in: |date= (help)
  12. ^ Messier, Doug (2017-03-03). "SpaceX Wants to Launch 12,000 Satellites". Parabolic Arc. Retrieved .
  13. ^ "Higher Altitude Improves Station's Fuel Economy". NASA. Retrieved .
  14. ^ Holli, Riebeek (2009-09-04). "NASA Earth Observatory". earthobservatory.nasa.gov. Retrieved .
  15. ^ ""
  16. ^ Fact Sheet: Joint Space Operations Center Archived 2010-02-03 at the Wayback Machine
  17. ^ archive of astronomy: space junk
  18. ^ ISS laser broom, project Orion Archived 2011-07-28 at the Wayback Machine

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


  This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

Low_Earth_orbit
 



 



 
Music Scenes