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Low Earth orbit Wiki2Web Clarity Challenge

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Study Guide: Understanding Low Earth Orbit (LEO): Concepts and Characteristics

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Understanding Low Earth Orbit (LEO): Concepts and Characteristics Study Guide

Defining Low Earth Orbit (LEO)

A Low Earth Orbit (LEO) is strictly defined by an orbital period of exactly 128 minutes and an eccentricity of 0.25.

Answer: False

Explanation: The definition of Low Earth Orbit (LEO) specifies an orbital period of 128 minutes or less, not exactly 128 minutes. Similarly, the eccentricity must be less than 0.25.

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The region generally considered Low Earth Orbit (LEO) extends up to an altitude of approximately 2,000 kilometers above the Earth's surface.

Answer: True

Explanation: The Low Earth Orbit (LEO) region is generally defined as extending up to an altitude of approximately 2,000 kilometers above the Earth's surface.

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The Kármán line, often considered the boundary between Earth and space, is located well below the typical altitude range of LEO.

Answer: False

Explanation: The Kármán line, at approximately 100 kilometers altitude, is considered the boundary between Earth and space and lies within the lower reaches of the Low Earth Orbit (LEO) region.

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An orbital period of 128 minutes corresponds to a semi-major axis of approximately 8,413 kilometers, according to Kepler's third law.

Answer: True

Explanation: According to Kepler's third law, an orbital period of 128 minutes corresponds to a semi-major axis of approximately 8,413 kilometers.

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The LEO region is defined as an object's specific path around the Earth meeting certain orbital parameters.

Answer: False

Explanation: The LEO region refers to a zone in space up to 2,000 km altitude, whereas a LEO orbit describes an object's specific path meeting orbital criteria. Objects not in a LEO orbit can still enter the LEO region.

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Which of the following best defines the orbital period criterion for Low Earth Orbit (LEO)?

Answer: An orbital period of 128 minutes or less.

Explanation: A low Earth orbit (LEO) is characterized by an orbital period of 128 minutes or less.

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What is the typical upper altitude limit defining the Low Earth Orbit (LEO) region?

Answer: 2,000 kilometers

Explanation: The LEO region is generally considered to extend up to an altitude of approximately 2,000 kilometers above the Earth's surface.

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The Kármán line, often considered the boundary between Earth and space, is situated at approximately what altitude?

Answer: 100 kilometers

Explanation: The Kármán line, widely recognized as the boundary between Earth's atmosphere and outer space, is situated at an approximate altitude of 100 kilometers.

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Orbital Dynamics and Physics

Objects in LEO experience significantly less gravitational pull than objects on Earth's surface, which is the primary reason they remain in orbit.

Answer: False

Explanation: The gravitational pull in LEO is only slightly diminished compared to Earth's surface. Objects remain in orbit due to a continuous state of free fall, balancing gravitational force with their orbital velocity, not solely due to reduced gravity.

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Weightlessness experienced by astronauts in LEO is caused by the complete absence of gravitational force at that altitude.

Answer: False

Explanation: Weightlessness in LEO is a result of continuous free fall, where the spacecraft and its occupants are constantly falling around the Earth. Gravitational force is still present and is essential for maintaining the orbit.

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Satellites orbiting below approximately 300 km in LEO are unlikely to be significantly affected by atmospheric drag.

Answer: False

Explanation: Satellites orbiting below approximately 300 kilometers in LEO are subject to significant atmospheric drag from the thermosphere and exosphere, which can lead to rapid orbital decay.

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Orbits higher than LEO generally expose electronic components to less intense radiation compared to LEO.

Answer: False

Explanation: Orbits situated higher than Low Earth Orbit can expose electronic components to more intense radiation, potentially leading to component failure and charge accumulation issues.

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The oblateness of Earth's shape is one factor that can cause variations in an object's altitude, even in seemingly circular orbits.

Answer: True

Explanation: The oblateness of Earth's shape, along with other factors like local topography, can cause variations in an object's altitude even in orbits that appear circular.

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The mean orbital velocity required for a stable LEO is approximately 7.8 kilometers per hour.

Answer: False

Explanation: The mean orbital velocity required for a stable LEO is approximately 7.8 kilometers per second, not per hour. This equates to roughly 28,000 kilometers per hour.

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Orbital velocity increases as altitude increases within LEO.

Answer: False

Explanation: Orbital velocity decreases as altitude increases within LEO. Satellites at lower altitudes require higher velocities to maintain orbit.

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Objects in LEO are in a continuous state of free fall, which is why they remain in orbit.

Answer: True

Explanation: Objects in LEO remain in orbit because they are in a continuous state of free fall, where their sideways velocity balances the gravitational pull, preventing them from falling to Earth.

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Satellites in lower LEO altitudes require less frequent re-boosting due to reduced atmospheric drag.

Answer: False

Explanation: Satellites in lower LEO altitudes experience greater atmospheric drag, leading to more rapid orbital decay and thus requiring *more* frequent re-boosting, not less.

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What is the approximate mean orbital velocity required to maintain a stable Low Earth Orbit?

Answer: 7.8 kilometers per second

Explanation: The mean orbital velocity needed to maintain a stable Low Earth Orbit is approximately 7.8 kilometers per second.

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Why do objects remain in orbit around the Earth in LEO, despite the presence of gravity?

Answer: Objects are in a continuous state of free fall, balancing gravitational pull with their sideways velocity.

Explanation: Objects remain in orbit because they are in a continuous state of free fall, where their sideways velocity perfectly balances the gravitational pull, preventing them from falling to Earth.

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What atmospheric layer do satellites in LEO, particularly those below 600 km, interact with, causing atmospheric drag?

Answer: The Thermosphere or Exosphere

Explanation: Satellites in LEO, especially below 600 km, encounter atmospheric drag from gases in the thermosphere or the exosphere.

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What significant challenge do satellites in lower LEO altitudes face?

Answer: Rapid orbital decay due to significant atmospheric drag.

Explanation: Satellites in lower LEO altitudes face rapid orbital decay due to significant atmospheric drag.

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Which of the following is NOT a factor mentioned that can cause the altitude of an object in orbit to vary?

Answer: The gravitational pull of the Moon

Explanation: Factors mentioned that can cause altitude variation include Earth's oblateness, local topography, and altitude variation above ground for polar orbits. The gravitational pull of the Moon is not listed as a cause in the provided data.

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How does the orbital velocity of a satellite change as its altitude increases within LEO?

Answer: It decreases.

Explanation: Orbital velocity decreases as altitude increases within LEO. Satellites at lower altitudes require higher velocities to maintain orbit.

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LEO Applications and Missions

All space stations launched and operated to date have been located within Medium Earth Orbit (MEO).

Answer: False

Explanation: All space stations that have been launched and operated thus far have been situated within Low Earth Orbit (LEO), not Medium Earth Orbit (MEO).

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A significant disadvantage of LEO satellites for global coverage is their wide field of view, allowing a single satellite to see most of the Earth.

Answer: False

Explanation: A significant disadvantage of LEO satellites for global coverage is their relatively small field of view, necessitating a constellation of many satellites for continuous coverage.

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The International Space Station (ISS) orbits at an altitude of roughly 400 kilometers and requires periodic re-boosting due to orbital decay.

Answer: True

Explanation: The International Space Station (ISS) orbits at an altitude of approximately 400 to 420 kilometers and requires periodic re-boosting maneuvers to counteract orbital decay.

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Earth observation satellites are often placed in LEO because their higher altitude provides better resolution for imaging.

Answer: False

Explanation: Earth observation satellites are often placed in LEO because their proximity to Earth allows for clearer images and data capture, not because a higher altitude provides better resolution.

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The Hubble Space Telescope orbits at an altitude significantly higher than the International Space Station.

Answer: True

Explanation: The Hubble Space Telescope orbits at an altitude of approximately 540 kilometers, which is higher than the International Space Station's orbital altitude of roughly 400-420 kilometers.

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The Chinese Tiangong space station orbits at altitudes between 340 and 450 kilometers.

Answer: True

Explanation: The Chinese Tiangong space station maintains an orbit at altitudes ranging between 340 and 450 kilometers.

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The Japanese satellite Tsubame holds the record for the lowest altitude achieved by an Earth observation satellite, orbiting at approximately 167.4 kilometers.

Answer: True

Explanation: The Japanese satellite Tsubame achieved a record for the lowest altitude for an Earth observation satellite, orbiting at approximately 167.4 kilometers.

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The European Space Agency's (ESA) GOCE mission orbited at a very low altitude of approximately 255 kilometers.

Answer: True

Explanation: The European Space Agency's (ESA) gravimetry mission GOCE operated at a very low altitude of approximately 255 kilometers.

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In the film *2001: A Space Odyssey*, the fictional Earth transit station 'Space Station V' was depicted orbiting at approximately 300 kilometers above Earth.

Answer: True

Explanation: The fictional 'Space Station V' in the film *2001: A Space Odyssey* was depicted orbiting at approximately 300 kilometers above Earth.

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What is a primary advantage of using Low Earth Orbit (LEO) for communication satellites?

Answer: Offers high bandwidth with low communication latency.

Explanation: LEO offers high bandwidth with low communication latency, making it advantageous for many communication applications.

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The International Space Station (ISS) orbits at an altitude of approximately 400-420 km and experiences orbital decay of about how much per month?

Answer: 2 kilometers

Explanation: The International Space Station (ISS) experiences orbital decay of about 2 kilometers per month.

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Why are Earth observation and remote sensing satellites frequently placed in LEO?

Answer: Because their proximity allows for clearer images and data capture.

Explanation: Earth observation and remote sensing satellites are frequently placed in LEO because their proximity to the Earth's surface allows for clearer images and data capture.

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What is the approximate altitude of the Hubble Space Telescope?

Answer: 540 kilometers

Explanation: The Hubble Space Telescope orbits the Earth at an altitude of approximately 540 kilometers.

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Which of the following is an example of a satellite internet constellation utilizing Low Earth Orbit?

Answer: Iridium

Explanation: The Iridium satellite constellation operates in Low Earth Orbit, fitting the criteria for a satellite internet constellation.

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What is the approximate altitude of the Chinese Tiangong space station?

Answer: Between 340 and 450 km

Explanation: The Chinese Tiangong space station orbits the Earth at altitudes between 340 and 450 kilometers.

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What is the primary reason that providing continuous global coverage requires a large constellation of satellites in LEO?

Answer: LEO satellites have a relatively small field of view.

Explanation: LEO satellites have a relatively small field of view, meaning a large constellation is required to achieve continuous global coverage.

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Orbital Hazards and Debris

Kessler syndrome describes a scenario where space debris in LEO is easily cleared by atmospheric drag.

Answer: False

Explanation: Kessler syndrome describes a scenario where cascading collisions in LEO generate debris, increasing the probability of further collisions and potentially rendering the orbit unusable, rather than being easily cleared by atmospheric drag.

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NASA's Orbital Debris Program tracks over 25,000 objects larger than 10 cm in Low Earth Orbit.

Answer: True

Explanation: According to NASA's Orbital Debris Program, over 25,000 objects larger than 10 centimeters are actively tracked in Low Earth Orbit.

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Even small particles of space debris are not dangerous in LEO due to the low orbital velocities.

Answer: False

Explanation: Even small particles of space debris are highly dangerous in LEO due to the extremely high orbital velocities, which impart significant kinetic energy upon impact.

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Where is the highest concentration of artificial objects in space typically found within the LEO region?

Answer: Around 800 kilometers (500 miles).

Explanation: The majority of artificial objects in space are found in LEO, with the highest concentration typically occurring around an altitude of 800 kilometers (500 miles).

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What theoretical scenario describes cascading collisions in LEO due to high object density, potentially rendering the orbit unusable?

Answer: The Kessler Syndrome

Explanation: The Kessler Syndrome is a theoretical scenario where the density of objects in LEO leads to cascading collisions, generating debris that increases the probability of further collisions and potentially renders the orbit unusable.

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Why are collisions involving space debris in LEO particularly dangerous?

Answer: Debris travels at extremely high speeds, possessing significant kinetic energy.

Explanation: Collisions involving space debris in LEO are particularly dangerous because the debris travels at extremely high speeds, possessing significant kinetic energy that can cause severe damage.

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According to NASA's Orbital Debris Program, how many objects larger than 10 cm are tracked in LEO?

Answer: Over 25,000

Explanation: NASA's Orbital Debris Program tracks over 25,000 objects larger than 10 centimeters in diameter within Low Earth Orbit.

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What is the estimated number of space debris particles in LEO between 1 and 10 cm in size?

Answer: Approximately 500,000

Explanation: It is estimated that there are approximately 500,000 particles of space debris in LEO between 1 and 10 cm in size.

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Launch and Maintenance

The delta-v requirement for launching into LEO is typically around 9.4 kilometers per second.

Answer: True

Explanation: The delta-v, representing the change in velocity a rocket must achieve, needed to reach Low Earth Orbit typically starts around 9.4 kilometers per second.

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What does delta-v represent in the context of rocket launches to LEO?

Answer: The change in velocity a rocket must achieve.

Explanation: Delta-v represents the change in velocity a rocket must achieve to reach its target orbit, such as Low Earth Orbit.

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Beyond LEO: Historical Missions

Which historical human spaceflight program is mentioned as having ventured beyond Low Earth Orbit?

Answer: The Apollo program

Explanation: Historically, only the lunar missions of the Apollo program have traveled beyond Low Earth Orbit.

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