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List of Mars-crossing minor planets

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Theorbit ofMars (yellow band; varies between 1.381 and 1.666 AU) displayed with 6 theoretically possible orbits for anasteroid (red line). The orbit of a Mars-crosser is displayed in the bottom row on the right. In generic terms, a Mars-crosser has a smallerperihelion and a largeraphelion compared to Mars.
Special cases include inner-grazers (top row, in the middle) and outer-grazers (bottom row, in the middle), which do not completely cross the orbital band described by Mars. The other three diagrams describe aco-orbital configuration (top row, on the right) where the asteroid's orbit is contained within the orbital band of Mars, as well as anear-Earth asteroid such as anAmor asteroid (top row, on the left) and amain-belt asteroid, for example of theHungaria family, which orbits are contained completely either inside or outside the orbit of Mars, respectively.

AMars-crossing asteroid (MCA, alsoMars-crosser,MC) is anasteroid whoseorbit crosses that ofMars. Some Mars-crossersnumbered below 100000 are listed here. They include the two numberedMars trojans5261 Eureka and(101429) 1998 VF31.

Many databases, for instance theJPL Small-Body Database (JPL SBDB), only list asteroids with aperihelion greater than 1.3AU as Mars-crossers. An asteroid with a perihelion less than this is classed as anear-Earth object even though it is crossing the orbit of Mars as well as crossing (or coming near to) that of Earth. Nevertheless, these objects are listed on this page. A grazer is an object with a perihelion below the aphelion of Mars (1.67 AU) but above the Martian perihelion (1.38 AU).[1] The JPL SBDB lists 13,500 Mars-crossing asteroids. Only 18 MCAs are brighter thanabsolute magnitude (H) 12.5,[2] which typically makes these asteroids with H<12.5 more than 13 km in diameter depending on thealbedo. The smallest known MCAs have an absolute magnitude (H) of around 24 and are typically less than 100 meters in diameter. There are over 21,600 known Mars-crossers[3] of which only 5751 have received a MPC number.

Earth having more gravity and surface area than Mars attracts more impactors than Mars. Earth isimpacted about 20 times more than the Moon,[4] and Mars only gets impacted about 3 to 5 times more than theMoon.[5]

Co-orbital

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L4 (leading cloud):

L5 (trailing cloud):

Candidates

Inner grazers

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Inner grazers that are alsoEarth-crossers or grazers

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Mars-crossers that are alsoEarth-crossers or grazers

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These objects are not catalogued as Mars-crossers in databases such as theJet Propulsion Laboratory's onlineSmall-body Database Browser. Instead, they are categorized asNear Earth Objects (NEOs).

Outer grazers

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Mars-crossers

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See also

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References

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  1. ^"Mars crosser", Encyclopædia Britannica, (2009),retrieved online May 3, 2009.
  2. ^"JPL Small-Body Database Search Engine: orbital class (MCA) and H < 12.5 (mag)". JPL Solar System Dynamics. Retrieved2015-05-12.
  3. ^"JPL Small-Body Database Search Engine: orbital class (MCA)". JPL Solar System Dynamics. Retrieved25 September 2021.
  4. ^NASA's Moon Data Sheds Light on Earth’s Asteroid Impact History
  5. ^How often does Mars get whacked?
  6. ^6386 Keithnoll at the JPL Small-Body Database Browser

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