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A temporary satellite is an object which has been captured by the gravitational field of a planet and thus has become the planet's
natural satellite A natural satellite is, in the most common usage, an astronomical body that orbits a planet, dwarf planet, or small Solar System body (or sometimes another natural satellite). Natural satellites are often colloquially referred to as ''moo ...
, but, unlike
irregular moon In astronomy, an irregular moon, irregular satellite or irregular natural satellite is a natural satellite following a distant, inclined, and often eccentric and retrograde orbit. They have been captured by their parent planet, unlike regular s ...
s of the larger outer planets of the
Solar System The Solar System Capitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Solar ...
, will eventually either leave its orbit around the planet or collide with the planet. The only observed examples are , a temporary satellite of
Earth Earth is the third planet from the Sun and the only astronomical object known to harbor life. While large volumes of water can be found throughout the Solar System, only Earth sustains liquid surface water. About 71% of Earth's surfa ...
for twelve months from July 2006 to July 2007, and , which was discovered in 2020. Some defunct space probes or rockets have also been observed on temporary satellite orbits. In astrophysics, a temporary satellite is any body that enters the
Hill sphere The Hill sphere of an astronomical body is the region in which it dominates the attraction of satellites. To be retained by a planet, a moon must have an orbit that lies within the planet's Hill sphere. That moon would, in turn, have a Hill sph ...
of a planet at a sufficiently low velocity such that it becomes gravitationally bound to the planet for some period of time.


Capture of asteroids

The dynamics of the capture of asteroids by Earth was explored in simulations conducted on a supercomputer, with results published in 2012. Of 10 million virtual
near-Earth asteroids A near-Earth object (NEO) is any small Solar System body whose orbit brings it into proximity with Earth. By convention, a Solar System body is a NEO if its closest approach to the Sun (perihelion) is less than 1.3 astronomical units (AU). ...
, 18,000 have been temporarily captured. Earth has at least one temporary satellite across at any given time, but they are too faint to detect by current surveys. According to the simulations, temporary satellites are typically caught and released when they pass one of two gravitational equilibrium points of the Sun and the planet along the line connecting the two, the L1 and L2
Lagrangian point In celestial mechanics, the Lagrange points (; also Lagrangian points or libration points) are points of equilibrium for small-mass objects under the influence of two massive orbiting bodies. Mathematically, this involves the solution of ...
s. The captured asteroids typically have orbits very similar to the planet's (
co-orbital configuration In astronomy, a co-orbital configuration is a configuration of two or more astronomical objects (such as asteroids, moons, or planets) orbiting at the same, or very similar, distance from their primary, i.e. they are in a 1:1 mean-motion resona ...
) and are captured most often when the planet is closest to the Sun (in the case of the Earth, in January) or furthest from the Sun (Earth: in July). In strict sense, only bodies that complete a full orbit around a planet are considered temporary satellites, also called temporarily captured orbiters (TCO). However, asteroids not in a tight co-orbital configuration with a planet can be temporarily captured for less than a full orbit; such objects have been named temporarily-captured fly-bys (TCF). In a 2017 follow-up to the 2012 simulation study which also considered an improved model of near-Earth asteroid populations, 40% of captured objects were TCF. The combined number of TCO/TCF was found to be smaller than in the previous study, the maximum size of objects which can be expected to be orbiting Earth at any given moment was . In another 2017 study based on simulations with one million virtual co-orbital asteroids, 0.36% have been temporarily captured.


Examples

, two objects have been observed at the time when they were temporary satellites: and 2020 CD3. According to orbital calculations, on its solar orbit, passes Earth at low speed every 20 to 21 years, at which point it can become a temporary satellite again. , there is one confirmed example of a temporarily captured asteroid that didn't complete a full orbit, . This asteroid was observed for a month after its discovery in November 1991, then again in April 1992, after which it wasn't seen until May 2017. After the recovery, orbital calculations confirmed that was a temporary satellite of Earth in February 1992. Another temporary capture episode was experienced by that may become a full mini-moon in December 2051.


Artificial objects on temporary satellite orbits

The Earth can also temporarily capture defunct space probes or rockets travelling on solar orbits, in which case astronomers cannot always immediately determine whether the object is artificial or natural. The possibility of an artificial origin has been considered for both and . The artificial origin has been confirmed in other cases. In September 2002, astronomers found an object designated
J002E3 J002E3 is an object in space discovered on September 3, 2002, by amateur astronomer Bill Yeung. Initially thought to be an asteroid, it has since been tentatively identified as the S-IVB third stage of the Apollo 12 Saturn V rocket (designat ...
. The object was on a temporary satellite orbit around Earth, leaving for a solar orbit in June 2003. Calculations showed that it was also on a solar orbit before 2002, but was close to Earth in 1971. J002E3 was identified as the third stage of the Saturn V rocket that carried
Apollo 12 Apollo 12 (November 14–24, 1969) was the sixth crewed flight in the United States Apollo program and the second to land on the Moon. It was launched on November 14, 1969, by NASA from the Kennedy Space Center, Florida. Commander Charles ...
to the Moon. In 2006, an object designated
6Q0B44E 6Q0B44E, sometimes abbreviated to B44E, is a small object, probably an item of space debris, that is currently orbiting Earth outside the orbit of the Moon as of November 2018. Discovery 6Q0B44E was first observed by Catalina Sky Survey researche ...
was discovered on a temporary satellite orbit, later its artificial nature was confirmed, but its identity is unknown. Another confirmed artificial temporary satellite with unidentified origin is .


See also

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Near-Earth object A near-Earth object (NEO) is any small Solar System body whose orbit brings it into proximity with Earth. By convention, a Solar System body is a NEO if its closest approach to the Sun (perihelion) is less than 1.3  astronomical units (AU) ...
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Horseshoe orbit In celestial mechanics, a horseshoe orbit is a type of co-orbital motion of a small orbiting body relative to a larger orbiting body. The osculating (instantaneous) orbital period of the smaller body remains very near that of the larger body, a ...
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Quasi-satellite A quasi-satellite is an object in a specific type of co-orbital configuration (1:1 orbital resonance) with a planet (or dwarf planet) where the object stays close to that planet over many orbital periods. A quasi-satellite's orbit around the Sun ...
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EQUULEUS Equuleus ( ) is a constellation of stars that are visible in the night sky. Its name is Latin for "little horse", a foal. Located just north of the celestial equator, it was one of the 48 constellations listed by the 2nd century astronomer Ptolem ...


References

{{reflist Moons