2011 EO40

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2011 EO40
Discovery[1]
Discovered byRichard A. Kowalski
(Mount Lemmon Survey)
Discovery date10 March 2011
Designations
2011 EO40
Orbital characteristics[3][5]
Epoch 9 August 2022 (JD 2459800.5)
Uncertainty parameter 6
Aphelion2.5467 AU (380.98 Gm)
Perihelion0.76039 AU (113.753 Gm)
1.65356 AU (247.369 Gm)
Eccentricity0.54015
2.1264 yr (776.66 d)
169.9°
0° 27m 47.736s / day
Inclination3.3591°
50.249°
17.154°
Earth MOID0.0482051 AU (7.21138 Gm)
Jupiter MOID2.79322 AU (417.860 Gm)
Physical characteristics
Dimensions150–330 m[a][6]
21.5[3]

2011 EO40 is an asteroid, classified as a near-Earth object and a potentially hazardous asteroid of the Apollo group. It is a possible candidate for the parent body of the Chelyabinsk superbolide.[7][8][9]

Discovery, orbit and physical properties

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2011 EO40 was discovered by Richard A. Kowalski on 10 March 2011 while observing for the Mount Lemmon Survey.[1][10]

Its orbit is typical of Apollo asteroids and is characterized by significant eccentricity (0.54), low inclination (3.36º), and a semi-major axis of 1.65 AU.[10] Upon discovery, it was classified as an Earth crosser, a near-Earth asteroid (NEA) and a potentially hazardous asteroid (PHA) by the Minor Planet Center. It was listed on the Sentry Risk Table for less than one day.[11] Its orbit is in need of additional observations to determine if it is part of an asteroid family; as of October 2015 the orbit is determined using just twenty observations spanning an observation arc of 34 days.[3] 2011 EO40 has an absolute magnitude of 21.5,[3] which gives a characteristic diameter of about 200 metres (660 ft).[6]

Relationship to the Chelyabinsk superbolide

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Recent calculations indicate that this object is a plausible candidate to be the parent body of the Chelyabinsk superbolide, since its orbit is very similar to the computed, pre-impact path of the Chelyabinsk meteoroid.[7][8][9] It has relatively frequent close encounters with Venus, the EarthMoon system, and Mars. It had a close encounter with Earth on 28 January 2011 at 0.0953 AU (14,260,000 km; 8,860,000 mi),[3] and it will have a nominal Earth approach on 23 September 2025 at about 0.06 AU (9,000,000 km; 5,600,000 mi).[3] Asteroid 2011 EO40 experiences close approaches to the Earth–Moon system following a rather regular pattern, every 17 years approximately due to the combined action of multiple secular resonances.[8]

Visibility

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Future opposition windows are: 7 June 2016 at magnitude 24.5, and 28 May 2018 at magnitude 24.6. The best observation window will be on 2–23 September 2025.[3] Depending on the Earth approach distance (0.04–0.12 AU),[3] it should be brighter than magnitude 19.[12]

See also

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Notes

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  • ^ This is assuming an albedo of 0.20–0.04.

References

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  1. ^ a b Discovery MPEC
  2. ^ List Of Apollo Minor Planets
  3. ^ a b c d e f g h i Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  4. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  5. ^ NEODyS-2 on 2011 EO40 Retrieved 2013-07-31
  6. ^ a b Absolute-magnitude conversion table (H)
  7. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  8. ^ a b c Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  9. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  10. ^ a b MPC data on 2011 EO40
  11. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). (2.7e-07 = 1 in 3,704,000 chance)
  12. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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Lua error in Module:Authority_control at line 153: attempt to index field 'wikibase' (a nil value).