2014 AA

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2014 AA was a small Apollo near-Earth asteroid roughly 2–4 meters in diameter that struck Earth on 2 January 2014. It was discovered on 1 January 2014 by Richard Kowalski at the Mount Lemmon Survey at an apparent magnitude of 19 using a 1.52-meter (60 in) reflecting telescope at Mount Lemmon Observatory. 2014 AA was only observed over a short observation arc of about 70 minutes, and entered Earth's atmosphere about 21 hours after discovery. Nonetheless, it remains one of only a few asteroids observed before impact (see Asteroid impact prediction).

2014 AA
2014 AA imaged by the Catalina Sky Survey in January 2014. The asteroid was around one lunar distance from Earth at that time.
Discovery
Discovered byRichard Kowalski
Mount Lemmon Survey (G96)
Discovery date1 January 2014
Designations
MPC designation
2014 AA
Minor planet category
  • Apollo
  • NEO
Orbital characteristics
Epoch 1 January 2014 (JD 2456658.5)
Uncertainty parameter 9
Observation arc~70 minutes
Aphelion1.4080 AU (210.63 Gm) (Q)
Perihelion0.9163 AU (137.08 Gm) (q)
Semi-major axis
1.1623 AU (173.88 Gm) (a)
Eccentricity0.2116 (e)
Orbital period (sidereal)
1.25 yr (457.26 d)
Mean anomaly
324.1460° (M)
Mean motion
0° 47m 14.244s / day (n)
Inclination1.4156° (i)
Longitude of ascending node
101.6086° (Ω)
Time of perihelion
15 February 2014 (would have been)
Argument of perihelion
52.3393° (ω)
Earth MOID4.54412×10−7 AU (67.9791 km)
Jupiter MOID3.58092 AU (535.698 Gm)
Physical characteristics
Dimensions~3 meters (10 ft)
Mass~4×104 kg (assumed)
Absolute magnitude (H)
30.9

Entry

Using a poorly determined orbit, the JPL Small-Body Database listed a 3-sigma solution with impact occurring around 2 January 2014 02:33 UT ± 1 hour and 5 minutes. The Minor Planet Center listed impact as occurring around 2 January 2014 05:00 UT ± 10 hours. Independent calculations by Bill Gray, the Minor Planet Center and Steve Chesley at the Jet Propulsion Laboratory verified that impact was virtually certain. It entered the atmosphere going about 11.7 km/s with respect to Earth.

The impactor would have been roughly the size of 2008 TC3, which exploded above the Nubian Desert in Sudan on 7 October 2008. Calculations by Chesley suggest the impactor fell somewhere on an arc extending from Central America to East Africa, with a best-fit location just off the coast of West Africa. Calculations by Pasquale Tricarico using the nominal orbit show that 2014 AA entered Earth's shadow cone approximately 40 minutes before entering the atmosphere.

Infrasound was detected by three stations of the Comprehensive Nuclear-Test-Ban Treaty Organization. Peter Brown and Petrus Jenniskens located weak signals from infrasound stations in Bolivia, Brazil and Bermuda. 2014 AA entered Earth's atmosphere around 03:06 ± 5 min UT, 3,000 km from Caracas, Venezuela, far from any landmass. No ships or planes reported witnessing the event. A recalculation of the impact parameters of this meteor based on infrasound recordings puts it in the Atlantic Ocean about 1900 km (1030 nautical miles) east of Port of Spain in Trinidad, at a longitude of impact of nearly 44º west and a latitude of 11º north, the impact time being 2456659.618 JD UTC. Extensive numerical simulations indicate that, prior to impact, 2014 AA was subjected to a number of secular resonances and it may have followed a path similar to those of the NEOs 2011 GJ3, 2011 JV10, 2012 DJ54, and 2013 NJ4; NEOs in this transient group experience close encounters with the Earth-Moon system at perihelion and Mars at aphelion and could be a dynamical family.

Other discoveries

Kowalski previously discovered 2008 TC3, the first asteroid discovered before Earth's impact, using the same telescope in October 2008. There are about a billion near-Earth objects in the size range of 2014 AA, and impacts of comparably-sized objects occur several times each year.

Several years later, 2018 LA was also discovered by the Mount Lemmon Survey, and ended up impacting Earth in southern Botswana in June 2018.

See also

  • Asteroid impact prediction
  • 2008 TC3
  • WT1190F
  • 2018 LA
  • 2019 MO
  • 2022 EB5
  • 2022 WJ1

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