Meteor air burst

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NASA visualization and narration of the Chelyabinsk meteor air burst.

A meteor air burst is a type of air burst in which a meteoroid explodes after entering a planetary body's atmosphere. This fate leads them to be called fireballs or bolides, with the brightest air bursts known as superbolides. Such meteoroids were originally asteroids and comets of a few to several tens of meters in diameter. This separates them from the much smaller and far more common "shooting stars", that usually burn up quickly upon atmospheric entry.

Contents

The most powerful meteor air burst in the modern era was the 1908 Tunguska event. During this event a stony meteoroid about 50–60 m (160–200 ft) in size [1] [2] :p. 178 exploded at an altitude of 5–10 km (16,000–33,000 ft) over a sparsely populated forest in Siberia. The resulting shock wave flattened an estimated 80 million trees over a 2,150 km2 (830 sq mi) area, and may have killed 3 people. [1] [3] [4] [5] [6]

Extremely bright fireballs traveling across the sky are often witnessed from a distance, such as the 1947 Sikhote-Alin meteor and the 2013 Chelyabinsk meteor, both over Russia. If the bolide is large enough fragments may survive, as from both such meteorites. Modern developments in infrasound detection by the Comprehensive Nuclear-Test-Ban Treaty Organization and infrared Defense Support Program satellite technology have increased the likelihood of detecting airbursts.

Explanation

Meteoroids enter the Earth's atmosphere from outer space traveling at speeds of at least 11 km/s (7 mi/s) and often much faster. Despite moving through the rarified upper reaches of Earth's atmosphere the immense speed at which a meteor travels rapidly compresses the air in its path. The meteoroid then experiences what is known as ram pressure. As the air in front of the meteoroid is compressed its temperature quickly rises. This is not due to friction, rather it is an adiabatic process, a consequence of many molecules and atoms being forced to occupy a smaller space. Ram pressure and the very high temperatures it causes are the reasons few meteoroids make it all the way to the ground. Most simply burn up or are ablated into tiny fragments. Larger or more solid meteorites may explode instead.

Airburst explosions

The use of the term explosion is somewhat loose in this context, and can be confusing. This confusion is exacerbated by the tendency for airburst energies to be expressed in terms of nuclear weapon yields, as when the Tunguska airburst is given a rating in megatons of TNT. Large meteoroids do not explode in the sense of chemical or nuclear explosives. Rather, at a critical moment in its atmospheric entry the enormous ram pressure experienced by the leading face of the meteoroid converts the body's immense momentum into a force blowing it apart over a nearly instantaneous span of time. [7] That is, the mass of the meteoroid suddenly ceases to move at orbital speeds when it breaks up. Conservation of energy implies much of this orbital velocity is converted into heat.

In essence, the meteoroid is ripped apart by its own speed. This occurs when fine tendrils of superheated air force their way into cracks and faults in the leading face's surface. Once this high pressure plasma gains entry to the meteoroid's interior it exerts tremendous force on the body's internal structure. This occurs because the superheated air now exerts its pressure over a much larger surface area, as when the wind suddenly fills a sail. This sudden rise in the force exerted on the meteoroid overwhelms the body's structural integrity and it begins to break up. The breakup of the meteoroid yields an even larger total surface area for the superheated air to act upon and a cycle of amplification rapidly occurs. This is the explosion, and it causes the meteoroid to disintegrate with hypersonic velocity, a speed comparable to that of explosive detonation. [7]

Frequency

The table from Earth Impact Effects Program (EIEP) estimates the average frequency of airbursts and their energy yield in kilotons (kt) or megatons (Mt) of TNT equivalent.

World map of bolide events (1994-2013) SmallAsteroidImpacts-Frequency-Bolide-20141114.jpg
World map of bolide events (1994–2013)
Stony asteroid impacts that generate an airburst [9]
Impactor
diameter
Kinetic energy atAirburst
altitude
Average
frequency
(years)
atmospheric
entry
airburst
4  m (13  ft )3 kt 0.75 kt42.5  km (139,000  ft )1.3
7 m (23 ft) 16 kt 5 kt36.3 km (119,000 ft)4.6
10 m (33 ft)47 kt 19 kt 31.9 km (105,000 ft)10
15 m (49 ft)159 kt 82 kt 26.4 km (87,000 ft)27
20 m (66 ft)376 kt 230 kt 22.4 km (73,000 ft)60
30 m (98 ft) 1.3 Mt 930 kt16.5 km (54,000 ft)185
50 m (160 ft)5.9 Mt5.2 Mt8.7 km (29,000 ft)764
70 m (230 ft)16 Mt 15.2 Mt 3.6 km (12,000 ft)1,900
Based on density of 2600 kg/m3, speed of 17 km/s, and an impact angle of 45°

Events

Before the 20th century

While airbursts undoubtedly happened prior to the 20th century, reliable reports of such are sparse. A possible example is the Qingyang event of 1490, which had an unknown energy yield but was reportedly powerful enough to cause 10,000 deaths. [10] Modern researchers are sceptical about the figure, but had the Tunguska event occurred over a highly populous district, it might have caused a similar level of destruction. [10] There has also been unofficial speculations that the mysterious 1626 Wanggongchang Explosion in the Ming dynasty capital Beijing, which reportedly killed 20,000 people and was long blamed onto potential mishandling of black gunpowder stored at the local armoury, might actually be a Tunguska-like impact event/air burst that coincidentally happened over a gunpowder factory.[ citation needed ]

A study published in 2020 claimed that on 22 August 1888, a meteorite killed a man and left another paralyzed in Sulaymaniyah, Iraq, as reported by the local governor to Sultan Abdul Hamid II of the Ottoman Empire. [11]

After 1901

Depending on the estimate, there were only 3–4 known airbursts in the years 1901–2000 with energy yield greater than 80 kilotons (in 1908, 1930?, 1932?, and 1963), roughly consistent with the estimate of the EIEP table. However, the 1963 event may have not been a meteor, but instead a nuclear test. Most values for the 1930 Curuçá River event put it well below 1 megaton, comparable to the Chelyabinsk meteor and Kamchatka superbolide. [12] [13] [14] The Comprehensive Nuclear-Test-Ban Treaty Organization and modern technology has improved multiple detection of airbursts with energy yield 1–2 kilotons every year within the last decade. [15]

The first airburst of the 21st century with yield greater than 100 kilotons came from the 2013 Chelyabinsk meteor, which had an estimated diameter of 20 metres.

DateGeneral:Specific LocationCoordinatesEnergy
(TNT equivalent)
Height of explosionNotes
1908, Jun 30Russia: 60 kilometres (37 mi) W-NW of Vanavara [16] near Tunguska River 60°53′09″N101°53′40″E / 60.88583°N 101.89444°E / 60.88583; 101.89444 15,000 kilotonnes of TNT (63,000 TJ)8.5 km (5.3 mi) Tunguska event (Largest witnessed meteor airburst to date)
1919, Nov 26United States: southern Michigan and northern Indiana 42°N86°W / 42°N 86°W / 42; -86 Known as the 1919 Michigan Event. A gigantic meteor was seen approaching from the east. A brilliant flash of light, thunder, and an earthquake lasting three minutes were reported. Damage to property over a large area as well as to telegraph, telephone and electrical systems. [17]
1927, Jul 13United States: Illinois 38°12′N89°41′W / 38.200°N 89.683°W / 38.200; -89.683 20 km (12 mi)Tilden meteor. From more than a hundred miles it appeared like "a piece falling off the sun." Then it exploded. [18]
1930, Aug 13 South America: Curuçá River, Brazil 5°11′S71°38′W / 5.183°S 71.633°W / -5.183; -71.633 100 kilotonnes of TNT (420 TJ)?Also known as the 1930 Curuçá River event or "Brazilian Tunguska". [19] Hypothesised to be generated by three meteor fragments. An astrobleme of 1 km was found on the ground, but may be related to an older feature. [19] [20] [21] [22] [23]
1932, Dec 8 Europe: Arroyomolinos de León, Spain 38°01′00″N6°25′00″W / 38.01667°N 6.41667°W / 38.01667; -6.41667 190 kilotonnes of TNT (790 TJ)?15.7 km (9.8 mi)Assumed to be produced by an 18-meter object and connected to the December delta-Arietids meteor shower. [24]
1935, Dec 12 Guyana: near Maumauktpautau which is 24 km south of Marudi Mountain, south of the Rupununi region. 2°00′N59°10′W / 2.000°N 59.167°W / 2.000; -59.167 An exceptionally large meteor fall woke witnesses with a terrific roar, concussion and brilliant illumination. Shortly after a region of devastated forest perhaps ten miles by five was located, where trees large and small had been pushed over. The view must have been obtained from the top of Maumauktpautau. Other reports say that trees had been broken or twisted off 25 ft above their bases. An elongated damaged area more than 20 miles in extent was reported seen from an aircraft. [25] A 1937 report says a 30-mile Path Cut By Meteor in Jungle and that the meteor fell, some ten miles from a place named Camshock. [26] The only place near there was Davidson's cottage high on the side of Marudi Mountain.
1941, Apr 9Russia: Ural Mountains, Katav-Ivanovo district of Chelyabinsk ru:Катавский болид (Katavsky bolide). Residents saw a fireball flying at a high speed in the dark sky, followed by roaring like the sound of a speeding steam locomotive. Fragments were left as a result of the event.[ citation needed ]
1947, Feb 12Russia: Sikhote-Alin Mountains in eastern Siberia 46°09′36″N134°39′12″E / 46.16000°N 134.65333°E / 46.16000; 134.65333 10 kilotonnes of TNT (42 TJ) Sikhote-Alin bolide. The largest meteorite fall of recent times with total mass of fragments at 23 tons. [27] A bright flash and a deafening sound were observed for 300 km. Estimated explosive yield of 10 kt equivalent. [28]
1948, Feb 18United States: Norton County, Kansas 39°41′N99°52′W / 39.683°N 99.867°W / 39.683; -99.867 Norton County bolide. One of the 5 largest meteorite falls of the 20th century, with more than 1 ton of fragments collected. [29] A brilliant fireball appeared in the sky. Then there was a loud explosion as the meteor broke apart. [30]
1959, Nov 24 Asia: Azerbaijan 38°56′N48°15′E / 38.933°N 48.250°E / 38.933; 48.250 Yardymly bolide. A bright object that illuminated the area for almost 3,000 square km before it shattered into pieces with a thunderous noise. [31] [32]
1963, Aug 3 Indian Ocean: about 1100 km west of the Prince Edward Islands 51°S24°E / 51°S 24°E / -51; 24 540–1,990 kilotonnes of TNT (2,300–8,300 TJ)The Prince Edward Islands bolide was detected infrasonically about 1,100 km (680 mi) W-SW from the Prince Edward Islands off the coast of South Africa by a U.S. Government instrument network for detecting atmospheric explosions. [33] The event "did not have independent confirmation from other techniques. It remains possible that this event was not a bolide but rather another source.". [34] Washington DC Nov 1963 "Despite those earlier denials, the Defense Department now concedes that a mysterious explosion in the Antarctic last August could have been a secret nuclear blast." [35]
1965, Mar 31Canada: Revelstoke, British Columbia 51°06′N117°36′W / 51.1°N 117.6°W / 51.1; -117.6 40–140 kilotonnes of TNT (170–590 TJ)13 km (8 mi)Revelstoke bolide. It exploded brilliantly and detonations were heard up to 130 km away. [36] About 1 g of meteorite found. Sometimes placed in SE Canada on May 31. [37] [34]
1966, Sep 17Canada: Lake Huron, Michigan, Ontario 0.6 kilotonnes of TNT (2.5 TJ)13 km (8 mi)The Kincardine fireball. [33] A brilliant meteor illuminated the whole of SW Ontario. [38]
1967, Feb 5Canada: Vilna, Alberta 0.6 kilotonnes of TNT (2.5 TJ)13 km (8 mi)Vilna bolide. Photographed. [39] Its detonation was also clearly recorded by the seismograph of the Univ. of Alberta. [40] Two very small fragments < 1 g found and stored by the university. [41]
1969, Feb 8Mexico: Chihuahua 26°58′N110°19′W / 26.967°N 110.317°W / 26.967; -110.317 Allende bolide. The 3rd largest meteorite fall of the 20th century. A huge, brilliant fireball lit the sky and ground for hundreds of miles. It exploded and broke up. About 2 tons of fragments were later found. [42]
1972, Apr 14 Indian Ocean 13°S78°E / 13°S 78°E / -13; 78 14 kilotonnes of TNT (59 TJ)Infrasound detection. [43]
1976, Mar 8Asia: Jilin Province in China 43°42′N126°12′E / 43.700°N 126.200°E / 43.700; 126.200 Jilin bolide. The 2nd largest meteorite fall of the 20th century (after the Sikhote-Alin event). A fireball larger than the full moon was seen. There were several explosions then a violent breakup. [44] It yielded a piece at 1770 kg, more than twice the Chelyabinsk meteorite (654 kg), and total fragments collected was about 4 tons. [45]
1984, Feb 26 Russia: Chulym, Krasnoyarsk region 57°42′N85°06′E / 57.7°N 85.1°E / 57.7; 85.1 11 kilotonnes of TNT (46 TJ)Chulym bolide explosion [46]
1984, Apr 3 Africa: Nigeria 11°29′N11°39′E / 11.483°N 11.650°E / 11.483; 11.650 Gujba bolide. A bright object was witnessed then an explosion was heard. More than 100 kg of fragments were found. [47]
1988, Apr 15 [48] Southeast Asia: Banda Sea 4°06′S124°18′E / 4.1°S 124.3°E / -4.1; 124.3 14 kilotonnes of TNT (59 TJ)
1993, Jan 19 Europe: Lugo, Italy 44°30′N11°54′E / 44.5°N 11.9°E / 44.5; 11.9 10 kilotonnes of TNT (42 TJ)30 kmSuperbolide airburst caused by the breakup of a low density meteoroid traveling at approximately 26 km/s. [49]
1994, Jan 18 Europe: Cando, Spain 42°50′34.8″N8°51′40.4″W / 42.843000°N 8.861222°W / 42.843000; -8.861222 Much less than 1 kilotonne of TNT (4.2 TJ)Cando event. An unexplained ground explosion at 7:15 UTC. Topsoil and large trees were thrown tens of metres away. No fragments found and there are problems with the trajectory. It might not be an impact event. [50]
1994, Feb 1 Pacific Ocean: near the Marshall Islands 2°36′N164°06′E / 2.6°N 164.1°E / 2.6; 164.1 11 kilotonnes of TNT (46 TJ)21–34 km (13–21 mi)Marshall Islands fireball (about 9 ± 5 meters in diameter). Two fragments exploded at 34 km and 21 km of altitude. This impact was observed by space-based sensors both in infrared (by the DOD) and visible wavelength (by the DOE). [51]
1997, Oct 10 United States: Las Cruces, New Mexico; El Paso, Texas 31°59′N106°50′W / 31.983°N 106.833°W / 31.983; -106.833 0.3 kilotonnes of TNT (1.3 TJ)16–24 km (10–15 mi)An airburst detected in El Paso and Las Cruces. The fireball traveled S-SE before disintegrating 10–15 miles above the surface with a loud explosion, traveling around 30,000 MPH. Luminosity is described only as "a very bright flash of light, bright orange-red, similar to a distant sunset". [52]
1997, Dec 9 Europe: 150 km south of Nuuk, Greenland 62°54′N50°06′W / 62.900°N 50.100°W / 62.900; -50.100 0.1 kilotonnes of TNT (0.42 TJ)25 km (16 mi)One airburst at 46 km, three more breakups detected between 25 and 30 km. No remains found so far. Yield only based on luminosity, i.e. the total energy might have been considerably larger. [53]
1998, June 20Asia: Kunya-Urgench in Turkmenistan 42°15′N59°12′E / 42.250°N 59.200°E / 42.250; 59.200 Kunya-Urgench bolide. One of the 5 largest meteorite falls of the 20th century, with more than 1 ton of fragments collected. [54] A large bolide brightened the sky, and a loud whistling then a crashing noise was heard. [55] [56]
1999, Nov 8 Europe: Northern Germany1.5 kilotonnes of TNT (6.3 TJ)Detected by the Deelen Infrasound Array in the Netherlands [57]
2000, Jan 18Canada: Yukon, BC 60°43′N135°03′W / 60.717°N 135.050°W / 60.717; -135.050 1.7 kilotonnes of TNT (7.1 TJ) [58] 30 km Tagish Lake bolide. One airburst at ~08:00, fragments recovered. [59]
2001, Apr 23 Pacific Ocean; west of California 28°00′N133°36′W / 28°N 133.6°W / 28; -133.6 2–9 kilotonnes of TNT (8.4–37.7 TJ)29 kmInfrasound detection. [60] Meteor estimated to be 2–3 metres in diameter. [61] Occurred 1,800 km west from the Scripps detector in San Diego.
2002, Jun 6 Mediterranean Sea: 230 km N-NE of Benghazi, Libya 34°N21°E / 34°N 21°E / 34; 21 12–26 kilotonnes of TNT (50–109 TJ) [58] [62] [63] 2002 Eastern Mediterranean event
2002, Sep 25Russia: Vitim River, near Bodaybo, Irkutsk Oblast 58°16′N113°27′E / 58.27°N 113.45°E / 58.27; 113.45 0.2–2 kilotonnes of TNT (0.84–8.37 TJ)30 kmVitim event or Bodaybo event [64]
2003, Mar 26United States: Park Forest, Illinois 41°29′N87°41′W / 41.483°N 87.683°W / 41.483; -87.683 0.5 kilotonnes of TNT (2.1 TJ) [33] Park Forest bolide. Residents in Illinois and neighboring states witnessed a bright meteor exploding overhead. [65]
2003, Sep 27 [15] Asia: Kendrapara in India 21°00′N86°36′E / 21°N 86.6°E / 21; 86.6 4.6 kilotonnes of TNT (19 TJ)26 km (16 mi)The Kendrapara bolide is notable as it may have caused injuries. [66] [67] A bright light then a loud noise that shattered windows. One part of the fireball fell in a village and may have set a hut on fire, injuring two people. [68]
2004, Sep 3 Antarctic Ocean: north of Queen Maud Land 69°S27°E / 69°S 27°E / -69; 27 12 kilotonnes of TNT (50 TJ)28–30 km (17–19 mi)Asteroid 7–10 meters in diameter. Coordinates are for dust trail observed after event by NASA's Aqua satellite and LIDAR in Davis Station. Event was also observed by military satellites and infrasound stations. [69]
2004, Oct 7 Indian Ocean 27°18′S71°30′E / 27.3°S 71.5°E / -27.3; 71.5 10–20 kilotonnes of TNT (42–84 TJ)Infrasound detection [60]
2005Start of JPL Fireball and Bolide Reports. [15] (Dates in yellow are not in the Jet Propulsion Laboratory reports.)
2005, Jan 1 [15] Africa: Libya 32°42′N12°24′E / 32.7°N 12.4°E / 32.7; 12.4 1.2 kilotonnes of TNT (5.0 TJ)31.8 km (19.8 mi)Largest for 2005.
2006, Apr 4 [15] Atlantic Ocean 26°36′N26°36′W / 26.6°N 26.6°W / 26.6; -26.6 5 kilotonnes of TNT (21 TJ)25 km (16 mi)
2006, Dec 9 [15] Africa: Egypt 26°12′N26°00′E / 26.2°N 26.0°E / 26.2; 26.0 10–20 kilotonnes of TNT (42–84 TJ)26.5 km (16.5 mi)Infrasound detection [60]
2007, Sep 28 Europe: Northern Ostrobothnia, Finland 40 km (25 mi)Bolide that was observed as far as northern Lapland. [70] Meteoritic material was suspected to have landed southeast of Oulu but none has been found.[ citation needed ]
2008, Oct 7 [15] Africa: Nubian Desert, Sudan 20°48′00″N32°12′00″E / 20.80000°N 32.20000°E / 20.80000; 32.20000 1–2.1 kilotonnes of TNT (4.2–8.8 TJ)37 km (23 mi) 2008 TC3, the first asteroid detected before impacting Earth. Fragment has been named as Almahata Sitta meteorite. [71] In JPL as 1 kt. [15]
2008, Nov 20 [15] Canada: Saskatchewan 53°06′N109°54′W / 53.1°N 109.9°W / 53.1; -109.9 0.4 kilotonnes of TNT (1.7 TJ)28.2 km (17.5 mi) Buzzard Coulee bolide. Five times as bright as the full moon and broke apart before impact. [72] Over 41 kg of fragments collected. [73]
2009, Feb 7 [15] Russia: Tyumen Oblast 56°36′N69°48′E / 56.6°N 69.8°E / 56.6; 69.8 3.5 kilotonnes of TNT (15 TJ)40 km (25 mi)
2009, Oct 8 [15] Asia: coastal region in South Sulawesi, Indonesia 04°30′00″S120°00′00″E / 4.50000°S 120.00000°E / -4.50000; 120.00000 31–50 kilotonnes of TNT (130–210 TJ)25 km (16 mi) 2009 Sulawesi superbolide. No meteoritic material found (most likely fell into the ocean). [74] Occurred ~03:00 UTC; ~11:00 local time. [74]
2009, Nov 21 [15] Africa: South Africa / Zimbabwe 22°00′S29°12′E / 22.0°S 29.2°E / -22.0; 29.2 18 kilotonnes of TNT (75 TJ)38 km (24 mi)Impacted going 32.1 km/s (19.9 mi/s). [15] There were 56 witnesses of the bolide and two seismic recorder detections. [75] [76]
2010, July 6 [15] Pacific Ocean: NE of New Zealand 34°06′S174°30′W / 34.1°S 174.5°W / -34.1; -174.5 14 kilotonnes of TNT (59 TJ)26 km (16 mi)
2010, Sep 3 [15] Pacific Ocean 61°00′S146°42′E / 61.0°S 146.7°E / -61.0; 146.7 3.8 kilotonnes of TNT (16 TJ)33.3 km (20.7 mi)
2010, Dec 25 [15] Pacific Ocean: east of Japan 38°00′N158°00′E / 38.0°N 158.0°E / 38.0; 158.0 33 kilotonnes of TNT (140 TJ)26 km (16 mi)
2011, May 25 [15] Africa: Cameroon 4°06′N14°00′E / 4.1°N 14.0°E / 4.1; 14.0 4.8 kilotonnes of TNT (20 TJ)59 km (37 mi)
2012, Apr 22United States: California and Nevada [77] 37°6′N120°5′W / 37.100°N 120.083°W / 37.100; -120.083 4 kilotonnes of TNT (17 TJ) [78] [79] [ citation needed ]30–47 km [78] Sutter's Mill meteorite. Numerous fragments from object recovered. (Not in JPL reports.)
2013, Jan 25 [15] Canada: Quebec 60°18′N64°36′W / 60.3°N 64.6°W / 60.3; -64.6 6.9 kilotonnes of TNT (29 TJ)
2013, Feb 15 [15] Russia: Chebarkul 54°30′N61°30′E / 54.500°N 61.500°E / 54.500; 61.500 500 kilotonnes of TNT (2,100 TJ) [80] Estimated 30–50 km [81] Chelyabinsk meteor, about ~20 meters in diameter. [82] Largest meteor airburst known since Tunguska in 1908. More than a ton of fragments found, one large piece called the Chelyabinsk meteorite.
2013, Apr 21 [15] South America: Argentina 28°06′S64°36′W / 28.1°S 64.6°W / -28.1; -64.6 2.5 kilotonnes of TNT (10 TJ)40.7 km (25.3 mi)The bolide was captured on video at a Los Tekis rock concert. [83]
2013, Apr 30 [15] Atlantic Ocean: SW of the Azores 35°30′N30°42′W / 35.5°N 30.7°W / 35.5; -30.7 10 kilotonnes of TNT (42 TJ)21.2 km (13.2 mi)Asteroid impact at a low 12.1 km/s
2013, Oct 12 [15] Atlantic Ocean 19°06′S25°00′W / 19.1°S 25.0°W / -19.1; -25.0 3.5 kilotonnes of TNT (15 TJ)22 km (14 mi)
2013, Nov 26Canada: heard in Montreal, Ottawa, and New York 0.10 kilotonnes of TNT (0.42 TJ) [84] Montreal bolide. [85] [86] [87] [88]
2014, Jan 8 [15] Pacific Ocean; north of Papua New Guinea 1°18′S147°36′E / 1.3°S 147.6°E / -1.3; 147.6 0.11 kilotonnes of TNT (0.46 TJ)18.7 kmPotentially interstellar originating from an unbound hyperbolic orbit based on an eccentricity of 2.4, an inclination of 10°, and a speed of 43.8 km/s when outside of the Solar System. [89] This would make it notably faster than ʻOumuamua which was 26.3 km/s when outside the Solar System. The meteor is estimated to have been 0.9 meters in diameter.
2014, Feb 18 [15] South America: Argentina 32°48′S61°30′W / 32.8°S 61.5°W / -32.8; -61.5 0.1 kilotonnes of TNT (0.42 TJ)Even though this was a low-energy event, there were reports of windows and buildings shaking. [90]
2014, Aug 23 [15] Antarctic Ocean 61°42′S132°36′E / 61.7°S 132.6°E / -61.7; 132.6 7.6 kilotonnes of TNT (32 TJ)22.2 km (13.8 mi)
2015, Jul 4 [15] China 38°36′N103°06′E / 38.6°N 103.1°E / 38.6; 103.1 0.18 kilotonnes of TNT (0.75 TJ)46.3 km (28.8 mi)Head-on collision at 49 km/s (180,000 km/h). Fastest collision in the CNEOS Fireball and Bolide database.
2015, Sep 7 [15] Asia: Bangkok, Thailand 14°30′N98°54′E / 14.5°N 98.9°E / 14.5; 98.9 3.9 kilotonnes of TNT (16 TJ)29.3 km (18.2 mi)The 2015 Thailand meteor daylight bolide around 08:40 local time (UTC+7). Caught on at least 9 videos of dash and helmet cams online [91] [92]
2015, Nov 13 [15] Asia: India 16°00′N124°18′E / 16.0°N 124.3°E / 16.0; 124.3 0.3 kilotonnes of TNT (1.3 TJ)28.0 km (17.4 mi)Komar Gaon bolide. A daylight meteor accompanied by almost a minute of sonic booms. [93]
2015, Dec 12 [15] Asia: eastern Turkey 39°06′N40°12′E / 39.1°N 40.2°E / 39.1; 40.2 0.13 kilotonnes of TNT (0.54 TJ)39.8 km (24.7 mi)Sariçiçek meteorite. A bright fireball was seen and then heard as it exploded over a Turkish village. [94] More than 15 kg of fragments were found and villagers made an est. $300,000 selling the space rocks. [95]
2016, Feb 6 [15] Atlantic Ocean: NW of Tristan da Cunha island 30°24′S25°30′W / 30.4°S 25.5°W / -30.4; -25.5 13 kilotonnes of TNT (54 TJ)31 km (19 mi)Largest fireball for 2016. [96]
2016, May 17United States: NE coast 44°24′N71°12′W / 44.4°N 71.2°W / 44.4; -71.2 Many eyewitnesses, and some heard a sonic boom. [97]
2017, Nov 16Europe: Inari, Finland 69°06′N28°36′E / 69.1°N 28.6°E / 69.1; 28.6 20–91 kmA meteoroid weighing a few hundred kg exploded in an airburst and dropped tens of kg of meteorites into a remote area of Finnish Lapland. [98] The resulting shockwave was felt on the surface. [99] The event was detected by 7 infrasound stations. [100]
2017, Dec 15 [15] Russia: Kamchatka 60°12′N170°00′E / 60.2°N 170.0°E / 60.2; 170.0 6.4 kilotonnes of TNT (27 TJ)20 km (12 mi)The asteroid likely had a diameter of 2–5 meters prior to impact. But because it happened in a remote area in Kamchatka, there were likely no eyewitnesses. The event was detected at 11 CTBTO infrasound stations. [101]
2018, Jan 22 [15] Atlantic Ocean: off Senegal's coast 14°00′N17°24′W / 14.0°N 17.4°W / 14.0; -17.4 0.11 kilotonnes of TNT (0.46 TJ)Not related to ATLAS detected object A106fgF that had an impact track well south of Senegal.
2018, Jun 21 [15] Russia: Kursk Oblast 52°48′N38°06′E / 52.8°N 38.1°E / 52.8; 38.1 2.8 kilotonnes of TNT (12 TJ)27.2 km (16.9 mi)Loud sonic booms were reported [102] as well as fragments found. [103]
2018, Dec 18 [15] Bering Sea, near Kamchatka, Russia 56°54′N172°24′E / 56.9°N 172.4°E / 56.9; 172.4 173 kilotonnes of TNT (720 TJ)25.6 km (15.9 mi) Kamchatka superbolide asteroid (~10 meters in diameter) impacting at a fast 32 km/s. Largest airburst since Chelyabinsk. [104]
2019, Feb 18 [15] Africa: Zambia 15°30′S25°18′E / 15.5°S 25.3°E / -15.5; 25.3 4.2 kilotonnes of TNT (18 TJ)26 km (16 mi)
2019, June 22 [15] Caribbean Sea 14°54′N66°12′W / 14.9°N 66.2°W / 14.9; -66.2 6 kilotonnes of TNT (25 TJ)25 km (16 mi) 2019 MO (~3 meters in diameter) seen by ATLAS 12 hours before impact.
2020, December 22 [15] Qinghai province, China 31°54′N96°12′E / 31.9°N 96.2°E / 31.9; 96.2 9.5 kilotonnes of TNT (40 TJ)35.5 km (22.1 mi)Asteroid (~8 meters in diameter) impacting at a relatively slow 13.6 km/s. Largest known impact since 2018 December 18.
  After 2005, but not in JPL reports.

Note: For sorting purposes, location is given in "general:specific" format. For example, "Europe: Spain". This table contains a chronological list of events with a large yield at least 3 kilotons since 2005, with earlier or smaller events included if widely covered in the media.

Airbursts per year

As of January 2020, the number of airbursts each year since 2005, as reported in the JPL Fireball and Bolide Reports are: [15]

YearNumber of
airbursts
201942
201839
201726
201629
201543
201433
201320
201231
201123
201032
200925
200827
200721
200632
200538

See also

Related Research Articles

<span class="mw-page-title-main">Meteorite</span> Solid debris from outer space that hits a planetary surface

A meteorite is a rock that originated in outer space and has fallen to the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.

<span class="mw-page-title-main">Tunguska event</span> 1908 meteor air burst explosion in Siberia

The Tunguska event was a large explosion of between 3 and 50 megatons that occurred near the Podkamennaya Tunguska River in Yeniseysk Governorate, Russia, on the morning of 30 June 1908. The explosion over the sparsely populated East Siberian taiga flattened an estimated 80 million trees over an area of 2,150 km2 (830 sq mi) of forest, and eyewitness accounts suggest up to three people may have died. The explosion is generally attributed to a meteor air burst, the atmospheric explosion of a stony asteroid about 50–60 metres wide. The asteroid approached from the east-south-east, probably with a relatively high speed of about 27 km/s (60,000 mph). Though the incident is classified as an impact event, the object is thought to have exploded at an altitude of 5 to 10 kilometres rather than hitting the Earth's surface, leaving no impact crater.

<span class="mw-page-title-main">Meteoroid</span> Sand- to boulder-sized particle of debris in the Solar System

A meteoroid is a small rocky or metallic body in outer space. Meteoroids are distinguished as objects significantly smaller than asteroids, ranging in size from grains to objects up to a meter wide. Objects smaller than meteoroids are classified as micrometeoroids or space dust. Many are fragments from comets or asteroids, whereas others are collision impact debris ejected from bodies such as the Moon or Mars.

<span class="mw-page-title-main">Impact event</span> Collision of two astronomical objects

An impact event is a collision between astronomical objects causing measurable effects. Impact events have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, as the impacting body is usually traveling at several kilometres a second, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.

<span class="mw-page-title-main">Bolide</span> Extremely bright meteor

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<span class="mw-page-title-main">Sikhote-Alin meteorite</span> 1947 meteorite impact in southeastern Russia

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<span class="mw-page-title-main">Libyan desert glass</span> Desert glass found in Libya and Egypt

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<span class="mw-page-title-main">Tagish Lake (meteorite)</span> Stony meteorite

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<span class="mw-page-title-main">Peter Jenniskens</span> Dutch astronomer

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The Great Daylight Fireball was an Earth-grazing fireball that passed within 57 kilometres of Earth's surface at 20:29 UTC on August 10, 1972. It entered Earth's atmosphere at a speed of 15 kilometres per second (9.3 mi/s) in daylight over Utah, United States and passed northwards leaving the atmosphere over Alberta, Canada. It was seen by many people and recorded on film and by space-borne sensors. An eyewitness to the event, located in Missoula, Montana, saw the object pass directly overhead and heard a double sonic boom. The smoke trail lingered in the atmosphere for several minutes.

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<span class="mw-page-title-main">Earth-grazing fireball</span> Meteoroid that enters Earths atmosphere and leaves again

An Earth-grazing fireball is a fireball, a very bright meteor that enters Earth’s atmosphere and leaves again. Some fragments may impact Earth as meteorites, if the meteor starts to break up or explodes in mid-air. These phenomena are then called Earth-grazing meteor processions and bolides. Famous examples of Earth-grazers are the 1972 Great Daylight Fireball and the Meteor Procession of July 20, 1860.

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<span class="mw-page-title-main">Chelyabinsk meteor</span> Near-Earth asteroid that fell over Russia in 2013

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Further reading