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Minimum orbit intersection distance

Measure of close approach in astronomy

Minimum orbit intersection distance

Summary

Measure of close approach in astronomy

The orbit of [[(4953) 1990 MU]], which, with a MOID of 0.0263 AU, is classified as a potentially hazardous object

Minimum orbit intersection distance (MOID) is a measure used in astronomy to assess potential close approaches and collision risks between astronomical objects. It is defined as the distance between the closest points of the osculating orbits of two bodies. Of greatest interest is the risk of a collision with Earth. Earth MOID is often listed on comet and asteroid databases such as the JPL Small-Body Database. MOID values are also defined with respect to other bodies as well: Jupiter MOID, Venus MOID and so on.

An object is classified as a potentially hazardous object (PHO) – that is, posing a possible risk to Earth – if, among other conditions, its Earth MOID is less than 0.05 AU. For more massive bodies than Earth, there is a potentially notable close approach with a larger MOID; for instance, Jupiter MOIDs less than 1 AU are considered noteworthy since Jupiter is the most massive planet.

A low MOID does not mean that a collision is inevitable as the planets frequently perturb the orbit of small bodies. It is also necessary that the two bodies reach that point in their orbits at the same time before the smaller body is perturbed into a different orbit with a different MOID value. Two objects gravitationally locked in orbital resonance may never approach one another. Numerical integrations become increasingly divergent as trajectories are projected further forward in time, especially beyond times where the smaller body is repeatedly perturbed by other planets. MOID has the convenience that it is obtained directly from the orbital elements of the body and no numerical integration into the future is used.

The only object that has ever been rated at 4 on the Torino Scale (since downgraded), the Aten asteroid (99942) Apophis, has an Earth MOID of 0.00026 AU. This is not the smallest Earth MOID in the catalogues; many bodies with a small Earth MOID are not classed as PHO's because the objects are less than roughly 140 meters in diameter (or absolute magnitude, H 22). Earth MOID values are generally more practical for asteroids less than 140 meters in diameter as those asteroids are very dim and often have a short observation arc with a poorly determined orbit. As of September 2023, there have been seven objects detected and their Earth-MOID calculated before the Earth impact. The first two objects that were detected and had their Earth-MOID calculated before Earth impact were the small asteroids and 2014 AA. 2014 AA is listed with a MOID of 0.00000045 AU, and is the second smallest MOID calculated for an Apollo asteroid after with an Earth-MOID of 0.00000039 AU.

ObjectEarth MOID
(AU)Size (m)
(approximate)(H)
0.000076 AU30021.1
0.000107 AU32019.8
0.000131 AU26020.4
0.000148 AU18021.5
0.000153 AU130017.9
0.000177 AU17021.7
0.000179 AU49019.4
0.000187 AU21021.2
0.000238 AU69519.3
0.000252 AU20021.3
99942 Apophis0.000257 AU37019.7
0.000261 AU130017.2
0.000305 AU70417.0
162173 Ryugu0.000315 AU89619.6
0.000321 AU230016.1
0.000335 AU50018.8
0.000368 AU15021.4
ObjectEpochEarth MOID
(AU)
3D/Biela18320.0005 AU
109P/Swift-Tuttle19950.0009 AU
55P/Tempel–Tuttle19980.0085 AU
255P/Levy20070.0088 AU
15P/Finlay20150.0092 AU
73P–BW20220.0093 AU
252P/LINEAR20160.0122 AU
460P/PanSTARRS20160.0163 AU
289P/Blanpain20190.0165 AU
21P/Giacobini–Zinner20170.0179 AU
ObjectEarth MOID
(Asteróide)
6 Hebe0.975 AU
7 Iris0.850 AU
8 Flora0.873 AU
12 Victoria0.824 AU
18 Melpomene0.811 AU
84 Klio0.798 AU
228 Agathe0.657 AU

References

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|archive-url=https://web.archive.org/web/20190528050554/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2016FG60 |archive-date=2019-05-28 |url-status=live

References

  1. [https://solarsystem.nasa.gov/basics/chapter1-3 Basics of Space Flight: The Solar System, p. 3], NASA Science, retrieved 14 May 2009 (from JPL site), [https://web.archive.org/web/20210917185720/https://solarsystem.nasa.gov/basics/chapter1-3/ archived] 17 September 2021.
  2. Bruce Koehn, "[http://www.lowell.edu/users/elgb/moid.html Minimum Orbital Intersection Distance]", Lowell Observatory, retrieved online 14 May 2009, [https://web.archive.org/web/20150715151635/https://lowell.edu/users/elgb/moid.html archived] 15 July 2015.
  3. Brian G. Marsden, [http://www.cfa.harvard.edu/iau/pressinfo/100PHAs.html "Press Information Sheet:Potentially Hazardous Asteroids"], Harvard-Smithsonian Center for Astrophysics, retrieved online 3 May 2009, [https://web.archive.org/web/20091122010157/http://www.cfa.harvard.edu/iau/pressinfo/100PHAs.html archived] 22 November 2009.
  4. [https://newton.spacedys.com/neodys/index.php?pc=4.5 List of Prior Impacts], NEODyS, retrieved 23 September 2023.
  5. [https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2014AA JPL SBDB: 2014 AA] (Earth impactor on 1 January 2014)
  6. [https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2020QY2 JPL SBDB: 2020 QY2] (Near-Earth asteroid roughly 2–meters in diameter)
  7. [https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?des=73P-BW JPL SBDB: 73P-BW] (Short-lived comet fragment)
  8. Prado, Antônio F. B. A.. (2013-10-17). "Mapeamento de órbitas em torno do asteróide 2001SN263". SBMAC.
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