Tunguska event

Tunguska event

Location of the event in Siberia (modern map)
Event Explosion in forest area (10–15 Mtons TNT)
Time 30 June 1908
Place Podkamennaya Tunguska River in Siberia, Russian Empire
Effects Flattening 2,000 km2 (770 sq mi) of forest
Damage Devastation to local plants and animals
A few damaged buildings
Deaths 2 (unofficial)
Cause Probable air burst of small asteroid or comet
Coordinates 60°55′N 101°57′E / 60.917°N 101.950°E / 60.917; 101.950

The Tunguska event was a large explosion that occurred near the Stony Tunguska River, in Yeniseysk Governorate (now Krasnoyarsk Krai), Russia, on the morning of 30 June 1908 (N.S.).[1][2] The explosion over the sparsely populated Eastern Siberian Taiga flattened 2,000 km2 (770 sq mi) of forest yet caused no known human casualties. The explosion is generally attributed to the air burst of a meteoroid. It is classified as an impact event, even though no impact crater has been found; the object is thought to have disintegrated at an altitude of 5 to 10 kilometres (3 to 6 miles) rather than hit the surface of the Earth.[3]

The Tunguska event is the largest impact event on Earth in recorded history. Studies have yielded different estimates of the meteoroid's size, on the order of 60 to 190 metres (200 to 620 feet), depending on whether the body was a comet or a denser asteroid.[4]

Since the 1908 event, there have been an estimated 1,000 scholarly papers (most in Russian) published on the Tunguska explosion. In 2013, a team of researchers published analysis results of micro-samples from a peat bog near the center of the affected area showing fragments that may be of meteoritic origin.[5][6]

Early estimates of the energy of the air burst range from 10–15 megatons of TNT (42–63 PJ) to 30 megatons of TNT (130 PJ),[7] depending on the exact height of burst estimated when the scaling-laws from the effects of nuclear weapons are employed.[7][8] However, modern supercomputer calculations that include the effect of the object's momentum find that more of the energy was focused downward than would be the case from a nuclear explosion and estimate that the airburst had an energy range from 3 to 5 megatons of TNT (13 to 21 PJ).[8]

The 15 megaton (Mt) estimate represents an energy about 1,000 times greater than that of the atomic bomb dropped on Hiroshima, Japan — roughly equal to that of the United States' Castle Bravo (15.2 Mt) ground-based thermonuclear detonation on 1 March 1954, and about one-third that of the Soviet Union's Tsar Bomba explosion on October 30, 1961 (which, at 50 Mt, was the largest nuclear weapon ever detonated).[9]

It is estimated that the Tunguska explosion knocked down some 80 million trees over an area of 2,150 square kilometres (830 sq mi), and that the shock wave from the blast would have measured 5.0 on the Richter magnitude scale. An explosion of this magnitude would be capable of destroying a large metropolitan area,[10] but, due to the remoteness of the location, no human fatalities were officially documented. Several reports have indicated that two people may have died in the event, however these deaths remain unofficial.[11][12][13][14] This event has helped to spark discussion of asteroid impact avoidance.

Description

Trees knocked over by the Tunguska blast. Photograph from the Soviet Academy of Science 1927 expedition led by Leonid Kulik.

On 30 June 1908, at around 07:17 local time, Evenki natives and Russian settlers in the hills north-west of Lake Baikal observed a column of bluish light, nearly as bright as the Sun, moving across the sky. About ten minutes later, there was a flash and a sound similar to artillery fire. Eyewitnesses closer to the explosion reported that the source of the sound moved from the east to the north of them. The sounds were accompanied by a shock wave that knocked people off their feet and broke windows hundreds of kilometres away. The majority of witnesses reported only the sounds and tremors, and did not report seeing the explosion. Eyewitness accounts vary regarding the sequence and duration of the events.

The explosion registered at seismic stations across Eurasia. It is estimated that, in some places, the resulting shock wave was equivalent to an earthquake measuring 5.0 on the Richter magnitude scale.[15] It also produced fluctuations in atmospheric pressure strong enough to be detected in Great Britain. Over the next few days, night skies in Asia and Europe were aglow;[16] it has been theorized that this was due to light passing through high-altitude ice particles that had formed at extremely low temperatures—a phenomenon that many years later would be produced by space shuttles.[17][18] In the United States, the Smithsonian Astrophysical Observatory and the Mount Wilson Observatory observed a months-long decrease in atmospheric transparency due to an increase in suspended dust particles.

Selected eyewitness reports

Testimony of S. Semenov, as recorded by Leonid Kulik's expedition in 1930:[19]

At breakfast time I was sitting by the house at Vanavara Trading Post [65 kilometres/40 miles south of the explosion], facing north. [...] I suddenly saw that directly to the north, over Onkoul's Tunguska Road, the sky split in two and fire appeared high and wide over the forest [as Semenov showed, about 50 degrees up—expedition note]. The split in the sky grew larger, and the entire northern side was covered with fire. At that moment I became so hot that I couldn't bear it as if my shirt was on fire; from the northern side, where the fire was, came strong heat. I wanted to tear off my shirt and throw it down, but then the sky shut closed, and a strong thump sounded, and I was thrown a few meters. I lost my senses for a moment, but then my wife ran out and led me to the house. After that such noise came, as if rocks were falling or cannons were firing, the earth shook, and when I was on the ground, I pressed my head down, fearing rocks would smash it. When the sky opened up, hot wind raced between the houses, like from cannons, which left traces in the ground like pathways, and it damaged some crops. Later we saw that many windows were shattered, and in the barn, a part of the iron lock snapped.

Testimony of Chuchan of Shanyagir tribe, as recorded by I. M. Suslov in 1926:[20]

We had a hut by the river with my brother Chekaren. We were sleeping. Suddenly we both woke up at the same time. Somebody shoved us. We heard whistling and felt strong wind. Chekaren said, 'Can you hear all those birds flying overhead?' We were both in the hut, couldn't see what was going on outside. Suddenly, I got shoved again, this time so hard I fell into the fire. I got scared. Chekaren got scared too. We started crying out for father, mother, brother, but no one answered. There was noise beyond the hut, we could hear trees falling down. Chekaren and I got out of our sleeping bags and wanted to run out, but then the thunder struck. This was the first thunder. The Earth began to move and rock, the wind hit our hut and knocked it over. My body was pushed down by sticks, but my head was in the clear. Then I saw a wonder: trees were falling, the branches were on fire, it became mighty bright, how can I say this, as if there was a second sun, my eyes were hurting, I even closed them. It was like what the Russians call lightning. And immediately there was a loud thunderclap. This was the second thunder. The morning was sunny, there were no clouds, our Sun was shining brightly as usual, and suddenly there came a second one!

Chekaren and I had some difficulty getting out from under the remains of our hut. Then we saw that above, but in a different place, there was another flash, and loud thunder came. This was the third thunder strike. Wind came again, knocked us off our feet, struck the fallen trees.

We looked at the fallen trees, watched the tree tops get snapped off, watched the fires. Suddenly Chekaren yelled "Look up" and pointed with his hand. I looked there and saw another flash, and it made another thunder. But the noise was less than before. This was the fourth strike, like normal thunder.

Now I remember well there was also one more thunder strike, but it was small, and somewhere far away, where the Sun goes to sleep.

Sibir newspaper, 2 July 1908:[21]

On the 17th of June,[22] around 9 a.m. in the morning, we observed an unusual natural occurrence. In the north Karelinski village [200 verst (213 km (132 mi)) north of Kirensk] the peasants saw to the northwest, rather high above the horizon, some strangely bright (impossible to look at) bluish-white heavenly body, which for 10 minutes moved downwards. The body appeared as a "pipe", i.e., a cylinder. The sky was cloudless, only a small dark cloud was observed in the general direction of the bright body. It was hot and dry. As the body neared the ground (forest), the bright body seemed to smudge, and then turned into a giant billow of black smoke, and a loud knocking (not thunder) was heard as if large stones were falling, or artillery was fired. All buildings shook. At the same time the cloud began emitting flames of uncertain shapes. All villagers were stricken with panic and took to the streets, women cried, thinking it was the end of the world.

The author of these lines was meantime in the forest about 6 versts [6.4 km] north of Kirensk and heard to the north east some kind of artillery barrage, that repeated in intervals of 15 minutes at least 10 times. In Kirensk in a few buildings in the walls facing north-east window glass shook.

Siberian Life newspaper, 27 July 1908:[23]

When the meteorite fell, strong tremors in the ground were observed, and near the Lovat village of the Kansk uezd two strong explosions were heard, as if from large-caliber artillery.

Krasnoyaretz newspaper, 13 July 1908:[24]

Kezhemskoe village. On the 17th an unusual atmospheric event was observed. At 7:43 the noise akin to a strong wind was heard. Immediately afterward a horrific thump sounded, followed by an earthquake that literally shook the buildings as if they were hit by a large log or a heavy rock. The first thump was followed by a second, and then a third. Then the interval between the first and the third thumps was accompanied by an unusual underground rattle, similar to a railway upon which dozens of trains are traveling at the same time. Afterward, for 5 to 6 minutes an exact likeness of artillery fire was heard: 50 to 60 salvoes in short, equal intervals, which got progressively weaker. After 1.5–2 minutes after one of the "barrages" six more thumps were heard, like cannon firing, but individual, loud and accompanied by tremors.

The sky, at the first sight, appeared to be clear. There was no wind and no clouds. Upon closer inspection to the north, i.e. where most of the thumps were heard, a kind of an ashen cloud was seen near the horizon, which kept getting smaller and more transparent and possibly by around 2–3 p.m. completely disappeared.

Trajectory Models of The Tunguska Fireball
Tunguska’s trajectory and the locations of five villages projected onto a plane normal to the Earth’s surface and passing through the fireball’s approach path. The scale is given by an adopted beginning height of 100 km. Three zenith angles ZR of the apparent radiant are assumed and the trajectories plotted by the solid, dashed, and dotted lines, respectively. The parenthesized data are the distances of the locations from the plane of projection: a plus sign indicates the location is south-south west of the plane; a minus sign, north-north east of it. The transliteration of the village names in this figure and the text is consistent with that of Paper I and differs somewhat from the transliteration in the current world atlases.

Investigations

The first recorded expedition arrived at the scene more than a decade after the event. In 1921, the Russian mineralogist Leonid Kulik, visiting the Podkamennaya Tunguska River basin as part of a survey for the Soviet Academy of Sciences, deduced from local accounts that the explosion had been caused by a giant meteorite impact. He persuaded the Soviet government to fund an expedition to the Tunguska region, based on the prospect of meteoric iron that could be salvaged to aid Soviet industry. Kulik's party eventually undertook an expedition in 1927.

Photograph from Kulik's 1929 expedition taken near the Hushmo River

Upon arrival, Kulik made arrangements with the local Evenki hunters to guide his party to the impact site. Reaching the explosion site was an extremely arduous task. Upon reaching an area just south of the site, the superstitious Evenki hunters would go no farther, fearing what they called the Valleymen. Kulik had to return to the nearby village, and his party was delayed for several days while they sought new guides.

The spectacle that confronted Kulik as he stood on a ridge overlooking the devastated area was overwhelming. To the explorers' surprise, they found no crater. There was instead around ground zero a vast zone (8 kilometres[5.0 mi] across) of trees scorched and devoid of branches, but standing upright. The trees farther away had been partly scorched and knocked down in a direction away from the centre. Much later, in the 1960s, it was established that the zone of levelled forest occupied an area of some 2,150 square kilometres (830 sq mi), its shape resembling a gigantic spread-eagled butterfly with a "wingspan" of 70 kilometres (43 mi) and a "body length" of 55 kilometres (34 mi).[25] Upon closer examination, Kulik located holes that he erroneously concluded were meteorite holes; he did not have the means at that time to excavate the holes.

During the next ten years there were three more expeditions to the area. Kulik found several dozens of little "pothole" bogs, each some 10 to 50 metres (33 to 164 ft) in diameter, that he thought might be meteoric craters. After a laborious exercise in draining one of these bogs (the so-called "Suslov's crater", 32 metres[105 ft] in diameter), he found an old stump on the bottom, ruling out the possibility that it was a meteoric crater. In 1938, Kulik arranged for an aerial photographic survey of the area[26] covering the central part of the leveled forest (some 250 square kilometres[97 sq mi]).[27] The negatives of these aerial photographs (1,500 negatives, each 18 by 18 centimetres[7.1 by 7.1 in]) were burned in 1975 by order of Yevgeny Krinov, then Chairman of the Committee on Meteorites of the USSR Academy of Sciences, as part of an initiative to dispose of hazardous nitrate film.[27] Positive prints were preserved for further study in the Russian city of Tomsk.[28]

Expeditions sent to the area in the 1950s and 1960s found microscopic silicate and magnetite spheres in siftings of the soil. Similar spheres were predicted to exist in the felled trees, although they could not be detected by contemporary means. Later expeditions did identify such spheres in the resin of the trees. Chemical analysis showed that the spheres contained high proportions of nickel relative to iron, which is also found in meteorites, leading to the conclusion they were of extraterrestrial origin. The concentration of the spheres in different regions of the soil was also found to be consistent with the expected distribution of debris from a meteoroid air burst.[29] Later studies of the spheres found unusual ratios of numerous other metals relative to the surrounding environment, which was taken as further evidence of their extraterrestrial origin.[30]

Chemical analysis of peat bogs from the area also revealed numerous anomalies considered consistent with an impact event. The isotopic signatures of stable carbon, hydrogen, and nitrogen isotopes at the layer of the bogs corresponding to 1908 were found to be inconsistent with the isotopic ratios measured in the adjacent layers, and this abnormality was not found in bogs located outside the area. The region of the bogs showing these anomalous signatures also contains an unusually high proportion of iridium, similar to the iridium layer found in the Cretaceous–Paleogene boundary. These unusual proportions are believed to result from debris from the falling body that deposited in the bogs. The nitrogen is believed to have been deposited as acid rain, a suspected fallout from the explosion.[30][31][32]

Researcher John Anfinogenov has suggested that a boulder found at the event site, known as John's stone, is a remnant of the meteorite.[33]

Earth impactor model

Asteroid air burst

The leading scientific explanation for the explosion is the air burst of an asteroid 6–10 km (4–6 mi) above Earth's surface.

Meteoroids enter Earth's atmosphere from outer space every day, travelling at a speed of at least 11 km/s (7 mi/s). The heat generated by compression of air in front of the body (ram pressure) as it travels through the atmosphere is immense and most meteoroids burn up or explode before they reach the ground. Since the second half of the 20th century, close monitoring of Earth's atmosphere has led to the discovery that such asteroid air bursts occur rather frequently. A stony asteroid of about 10 m (33 ft) in diameter can produce an explosion of around 20 kilotons, similar to that of the Fat Man bomb dropped on Nagasaki, and data released by the US Air Force's Defense Support Program indicate that such explosions occur high in the upper atmosphere more than once a year. Tunguska-like megaton-range events are much rarer. Eugene Shoemaker estimated that such events occur about once every 300 years.[34][35]

Blast patterns

The explosion's effect on the trees near the hypocentre of the explosion was replicated during atmospheric nuclear tests in the 1950s and 1960s, and was similar to the effects of the conventional Operation Blowdown. These effects are caused by the blast wave produced by large explosions. The trees directly below the explosion are stripped as the blast wave moves vertically downward, while trees farther away are knocked over because the blast wave is travelling closer to horizontal when it reaches them.

Soviet experiments performed in the mid-1960s, with model forests (made of matches on wire stakes) and small explosive charges slid downward on wires, produced butterfly-shaped blast patterns strikingly similar to the pattern found at the Tunguska site. The experiments suggested that the object had approached at an angle of roughly 30 degrees from the ground and 115 degrees from north and had exploded in mid-air.[36]

Asteroid or comet

In 1930, the British astronomer F.J.W. Whipple suggested that the Tunguska body was a small comet. A comet is composed of dust and volatiles, such as water ice and frozen gases, and could have been completely vaporised by the impact with Earth's atmosphere, leaving no obvious traces. The comet hypothesis was further supported by the glowing skies (or "skyglows" or "bright nights") observed across Europe for several evenings after the impact, possibly explained by dust and ice that had been dispersed from the comet's tail across the upper atmosphere.[7] The cometary hypothesis gained a general acceptance amongst Soviet Tunguska investigators by the 1960s.[7]

In 1978, Slovak astronomer Ľubor Kresák suggested that the body was a fragment of Comet Encke. This is a periodic comet with an extremely short period of 3 years that stays entirely within the orbit of Jupiter. It is also responsible for the Beta Taurids, an annual meteor shower with a maximum activity around 28–29 June. The Tunguska event coincided with the peak activity of that shower,[37] and the approximate trajectory of the Tunguska object is consistent with what would be expected from a fragment of Comet Encke.[7] It is now known that bodies of this kind explode at frequent intervals tens to hundreds of kilometres above the ground. Military satellites have been observing these explosions for decades.[38]

In 1983, astronomer Zdeněk Sekanina published a paper criticising the comet hypothesis. He pointed out that a body composed of cometary material, travelling through the atmosphere along such a shallow trajectory, ought to have disintegrated, whereas the Tunguska body apparently remained intact into the lower atmosphere. Sekanina argued that the evidence pointed to a dense, rocky object, probably of asteroidal origin. This hypothesis was further boosted in 2001, when Farinella, Foschini, et al. released a study calculating the probabilities based on orbital modelling extracted form the atmospheric trajectories of the Tunguska object. They concluded with a probability of 83% that the object moved on an asteroidal path originating from the asteroid belt, rather than on a cometary one (probability of 17%).[1]

Proponents of the comet hypothesis have suggested that the object was an extinct comet with a stony mantle that allowed it to penetrate the atmosphere.

The chief difficulty in the asteroid hypothesis is that a stony object should have produced a large crater where it struck the ground, but no such crater has been found. It has been hypothesised that the passage of the asteroid through the atmosphere caused pressures and temperatures to build up to a point where the asteroid abruptly disintegrated in a huge explosion. The destruction would have to have been so complete that no remnants of substantial size survived, and the material scattered into the upper atmosphere during the explosion would have caused the skyglows. Models published in 1993 suggested that the stony body would have been about 60 metres (200 ft) across, with physical properties somewhere between an ordinary chondrite and a carbonaceous chondrite. Typical carbonaceous chondrite substance tends to be dissolved with water rather quickly unless it is frozen.[39]

Christopher Chyba and others have proposed a process whereby a stony meteorite could have exhibited the behaviour of the Tunguska impactor. Their models show that when the forces opposing a body's descent become greater than the cohesive force holding it together, it blows apart, releasing nearly all its energy at once. The result is no crater, with damage distributed over a fairly wide radius, and all of the damage resulting from the thermal energy released in the blast.

Three-dimensional numerical modelling of the Tunguska impact done by Utyuzhnikov and Rudenko in 2008[40] supports the comet hypothesis. According to their results, the comet matter dispersed in the atmosphere, while the destruction of the forest was caused by the shock wave.

During the 1990s, Italian researchers, coordinated by the physicist Giuseppe Longo from University of Bologna, extracted resin from the core of the trees in the area of impact to examine trapped particles that were present during the 1908 event. They found high levels of material commonly found in rocky asteroids and rarely found in comets.[41][42]

Kelly et al. (2009) contend that the impact was caused by a comet because of the sightings of noctilucent clouds following the impact, a phenomenon caused by massive amounts of water vapor in the upper atmosphere. They compared the noctilucent cloud phenomenon to the exhaust plume from NASA's Endeavour space shuttle.[43][44]

In 2010, an expedition led by Vladimir Alexeev with scientists from the Troitsk Innovation and Nuclear Research Institute (TRINITY) used ground penetrating radar to examine the Suslov crater at the Tunguska site. What they found was that the crater was created by the violent impact of a celestial body. The layers of the crater consisted of modern permafrost on top, older damaged layers underneath, and finally, deep below, fragments of the celestial body were discovered. Preliminary analysis showed that it was a huge piece of ice that shattered on impact, which seem to support the theory that a comet caused the cataclysm.[45] In contrast, in 2013, analysis of fragments from the Tunguska site by a joint US-European team was consistent with an iron meteorite.[46]

Lake Cheko

In June 2007, scientists from the University of Bologna identified a lake in the Tunguska region as a possible impact crater from the event. They do not dispute that the Tunguska body exploded in mid-air but believe that a ten-metre fragment survived the explosion and struck the ground. Lake Cheko is a small, bowl-shaped lake approximately 8 km (5.0 mi) north-northwest of the hypocentre.[47] The hypothesis has been disputed by other impact crater specialists.[48] A 1961 investigation had dismissed a modern origin of Lake Cheko, saying that the presence of metres-thick silt deposits at the lake's bed suggests an age of at least 5,000 years,[29] but more recent research suggests that only a metre or so of the sediment layer on the lake bed is "normal lacustrine sedimentation", a depth indicating a much younger lake of about 100 years.[49] Acoustic-echo soundings of the lake floor provide support for the hypothesis that the lake was formed by the Tunguska event. The soundings revealed a conical shape for the lake bed, which is consistent with an impact crater.[50] Magnetic readings indicate a possible metre-sized chunk of rock below the lake's deepest point that may be a fragment of the colliding body.[50] Finally, the lake's long axis points to the hypocentre of the Tunguska explosion, about 7.0 km (4.3 mi) away.[50] Work is still being done at Lake Cheko to determine its origins.[51]

The main points of the study are that

Cheko, a small lake located in Siberia close to the hypocentre of the 1908 Tunguska explosion, might fill a crater left by the impact of a fragment of a cosmic body. Sediment cores from the lake's bottom were studied to support or reject this hypothesis. A 175-centimetre (69 in)-long core, collected near the center of the lake, consists of an upper c. 1 m (39 in)-thick sequence of lacustrine deposits overlaying coarser chaotic material. 210Pb and 137Cs indicate that the transition from lower to upper sequence occurred close to the time of the Tunguska event. Pollen analysis reveals that remains of aquatic plants are abundant in the top post-1908 sequence but are absent in the lower pre-1908 portion of the core. These results, including organic C, N and δ13C data, suggest that Lake Cheko formed at the time of the Tunguska event.[52]

In 2017, however, new research by Russian Scientists points to a disproval of the theory. They used soil research to prove that the lake is 280 years old or even much older; in any case clearly older than the Tunguska Events.[53]

Geophysical hypotheses

The scientific consensus is that the explosion was caused by the impact of a small asteroid, however there are a few dissenters. Astrophysicist Wolfgang Kundt has proposed that the Tunguska event was caused by the release and subsequent explosion of 10 million tons of natural gas from within Earth's crust.[54][55][56][57][58] The basic idea is that natural gas leaked out of the crust and then rose to its equal-density height in the atmosphere; from there, it drifted downwind, in a sort of wick, which eventually found an ignition source such as lightning. Once the gas was ignited, the fire streaked along the wick, and then down to the source of the leak in the ground, whereupon there was the explosion.

The similar verneshot hypothesis has also been proposed as a possible cause of the Tunguska event.[59][60][61] Other research has supported a geophysical mechanism for the event.[62][63][64]

Similar events

Tunguska event is not the only example of a great unobserved explosion event. For example, the 1930 Curuçá River event in Brazil was an explosion of a superbolide that left no clear evidence of an impact crater. Modern developments in infrasound detection by the Comprehensive Nuclear-Test-Ban Treaty Organization and infrared DSP satellite technology have reduced the likelihood of undetected airbursts.

A smaller air burst occurred over a populated area in Russia on 15 February 2013, at Chelyabinsk in the Ural district of Russia. The exploding meteoroid was an asteroid that measured about 17 to 20 metres across, with an estimated initial mass of 11,000 tonnes, and inflicted over 1,200 injuries, mainly from broken glass falling from windows shattered by its shock wave.[65]

See also

References

Notes

  1. 1 2 Farinella, Paolo; Foschini, L.; Froeschlé, Christiane; Gonczi, R.; Jopek, T. J.; Longo, G.; Michel, Patrick (2001). "Probable asteroidal origin of the Tunguska Cosmic Body" (PDF). Astronomy & Astrophysics. 377 (3): 1081–1097. Bibcode:2001A&A...377.1081F. doi:10.1051/0004-6361:20011054. Retrieved 1 September 2015.
  2. ↑ Trayner, C (1994). "Perplexities of the Tunguska meteorite". The Observatory. 114: 227–231. Bibcode:1994Obs...114..227T.
  3. ↑ Nemiroff, R.; Bonnell, J., eds. (14 November 2007). "Tunguska: The Largest Recent Impact Event". Astronomy Picture of the Day. NASA. Retrieved 12 September 2011.
  4. ↑ Lyne, J. E.; Tauber, M. (1995). "Origin of the Tunguska Event". Nature. 375: 638–639. Bibcode:1995Natur.375..638L. doi:10.1038/375638a0.
  5. ↑ Peplow, Mark (10 June 2013). "Rock samples suggest meteor caused Tunguska blast". Nature News.
  6. ↑ Kvasnytsya, Victor; R. Wirth; L. Dobrzhinetskaya; J. Matzel; B. Jacobsen; I. Hutcheon; R. Tappero; M. Kovalyukh (2013). "New evidence of meteoritic origin of the Tunguska cosmic body". Planet. Space Sci. 84: 131–140. Bibcode:2013P&SS...84..131K. doi:10.1016/j.pss.2013.05.003.
  7. 1 2 3 4 5 Shoemaker, Eugene (1983). "Asteroid and Comet Bombardment of the Earth". Annual Review of Earth and Planetary Sciences. US Geological Survey, Flagstaff, Arizona: Annual Review of Earth and Planetary Sciences. 11 (1): 461–494. Bibcode:1983AREPS..11..461S. doi:10.1146/annurev.ea.11.050183.002333.
  8. 1 2 "Sandia supercomputers offer new explanation of Tunguska disaster". Sandia National Laboratories. 17 December 2007. Retrieved 22 December 2007.
  9. ↑ Verma (2005), p 1.
  10. ↑ Longo, Giuseppe (2007). "18: The Tunguska event". In Bobrowsky, Peter T.; Rickman, Hans. Comet/Asteroid Impacts and Human Society, An Interdisciplinary Approach (PDF). Berlin Heidelberg New York: Springer-Verlag. pp. 303–330. ISBN 978-3-540-32709-7. Archived from the original (PDF) on 14 October 2013.
  11. ↑ Gritzner, C. "Human Casualties in Impact Events". SAO/NASA Astrophysics Data System (ADS). Retrieved 20 July 2017.
  12. ↑ Jay, Paul. "The Tunguska event". CBC News. Retrieved 20 July 2017.
  13. ↑ Coppins, Philip. "The Tunguska explosion: an unexpected loud bang and explosion". philipcoppins.com. Retrieved 20 July 2017.
  14. ↑ "Reported Deaths and Injuries from Meteorite Impact". delong.typepad.com. Retrieved 20 July 2017.
  15. ↑ Traynor, Chris (1997). "The Tunguska Event". Journal of the British Astronomical Association. 107 (3).
  16. ↑ Watson, Nigel. "The Tunguska Event". History Today 58.1 (July 2008): 7. MAS Ultra-School Edition. EBSCO. 10 February 2009
  17. ↑ Cornell University (24 June 2009). Space Shuttle Science Shows How 1908 Tunguska Explosion Was Caused By A Comet.
  18. ↑ Kelley, M. C.; Seyler, C. E.; Larsen, M. F. (2009). "Two-dimensional Turbulence, Space Shuttle Plume Transport in the Thermosphere, and a Possible Relation to the Great Siberian Impact Event". Geophys. Res. Lett. 36. Bibcode:2009GeoRL..3614103K. doi:10.1029/2009GL038362.
  19. ↑ N. V. Vasiliev, A. F. Kovalevsky, S. A. Razin, L. E. Epiktetova (1981). Eyewitness accounts of Tunguska (Crash)., Section 6, Item 4
  20. ↑ Vasiliev, Section 5
  21. ↑ Vasiliev, Section 1, Item 2
  22. ↑ Gregorian calendar: 30 June
  23. ↑ Vasiliev, Section 1, Item 3
  24. ↑ Vasiliev, Section 1, Item 5
  25. ↑ Boyarkina, A. P., Demin, D. V., Zotkin, I. T., Fast, W. G. "Estimation of the blast wave of the Tunguska meteorite from the forest destruction". Meteoritika, Vol. 24, 1964, pp. 112–128 (in Russian).
  26. ↑ Longo G. "The 1938 aerophotosurvey". Retrieved 3 January 2008.
  27. 1 2 See: Bronshten (2000), p. 56.
  28. ↑ Rubtsov (2009), p. 59
  29. 1 2 Florenskiy, K P (1963). "Preliminary results from the 1961 combined Tunguska meteorite expedition". Meteoritica. 13. Retrieved 26 June 2007.
  30. 1 2 Kolesnikov et al. "Finding of probable Tunguska Cosmic Body material: isotopic anomalies of carbon and hydrogen in peat", Planetary and Space Science, Volume 47, Issues 6–7, 1 June 1999, Pages 905–916
  31. ↑ Hou et al. "Discovery of iridium and other element anomalies near the 1908 Tunguska explosion site", Planetary and Space Science, Volume 46, Issues 2–3, February–March 1998, Pages 179–188
  32. ↑ Kolesnikov et al. "Isotopic anomaly in peat nitrogen is a probable trace of acid rains caused by 1908 Tunguska bolide", Planetary and Space Science, Volume 46, Issues 2–3, February–March 1998, Pages 163–167
  33. ↑ Anfinogenov, John; et al. (15 November 2014). "John’s Stone: A possible fragment of the 1908 Tunguska meteorite". Icarus. 245: 139–147. Bibcode:2014Icar..243..139A. doi:10.1016/j.icarus.2014.09.006.
  34. ↑ Wiley, John P., Jr. (January 1995). "Phenomena, Comment & Notes". Smithsonian.
  35. ↑ Subject: "Three Minutes to Impact", To: Cambridge-Conference@..., Date sent: Mon, 10 February 1997 23:04:24 -0600 (CST), From: pib@...
  36. ↑ Siberian Apocalypse on IMDb
  37. ↑ "The Tunguska object—A fragment of Comet Encke". Astronomical Institutes of Czechoslovakia. 29 (3). 1978. Bibcode:1978BAICz..29..129K.
  38. ↑ Nemtchinov, I.V.; Jacobs, C.; Tagliaferri, E. (1997). "Analysis of Satellite Observations of Large Meteoroid Impacts". Annals of the New York Academy of Sciences. 822 (1 Near–Earth Ob): 303–317. Bibcode:1997NYASA.822..303N. doi:10.1111/j.1749-6632.1997.tb48348.x.
  39. ↑ "Arctic Asteroid!". Science at NASA.
  40. ↑ Utyuzhnikov, S. V. and Rudenko, D. V. "An adaptive moving mesh method with application to nontstationary hypersonic flows in the atmosphere" Proceedings of the Institution of Mechanical Engineers, Part G, J. of Aerospace Engineering, 2008, 222 (5): 661–671
  41. ↑ Longo, G.; Serra, R.; Cecchini, S.; Galli, M. (1994). "Search for microremnants of the Tunguska Cosmic Body". Planetary and Space Science. UK: Elsevier Science Ltd. 42 (2): 163–177. Bibcode:1994P&SS...42..163L. doi:10.1016/0032-0633(94)90028-0.
  42. ↑ Serra, R.; Cecchini, S.; Galli, M.; Longo, G. (1994). "Experimental hints on the fragmentation of the Tunguska cosmic body". Planetary and Space Science. UK: Elsevier Science Ltd. 42 (9): 777–783. Bibcode:1994P&SS...42..777S. doi:10.1016/0032-0633(94)90120-1.
  43. ↑ Kelly, M.C.; C. E. Seyler; M. F. Larsen (22 June 2009). "Two-dimensional turbulence, space shuttle plume transport in the thermosphere, and a possible relation to the Great Siberian Impact Event". Geophysical Research Letters (Published online 22 July 2009). 36 (14): L14103. Bibcode:2009GeoRL..3614103K. doi:10.1029/2009GL038362. Retrieved 25 June 2009.
  44. ↑ Ju, Anne (24 June 2009). "A mystery solved: Space shuttle shows 1908 Tunguska explosion was caused by comet". Cornell Chronicle. Cornell University. Retrieved 25 June 2009.
  45. ↑ "Mystery of Tunguska meteorite solved". Pravda. 25 October 2010. Retrieved 17 February 2013.
  46. ↑ "Meteoroid, not comet, explains the 1908 Tunguska fireball". DiscoverMagazine.com blog. July 1, 2013.
  47. ↑ "A possible impact crater for the 1908 Tunguska Event", Department of Physics, University of Bologna
  48. ↑ Paul, Rincon (27 June 2007). "Team makes Tunguska crater claim". BBC.
  49. ↑ Gasperini, L.; Bonatti, Enrico; Longo, Giuseppe (April 2008). "Reply—Lake Cheko and the Tunguska Event: impact or non-impact?". Terra Nova. 20 (2): 169–172. doi:10.1111/j.1365-3121.2008.00792.x. Retrieved 27 May 2008.
  50. 1 2 3 Gasperini, L.; et al. (June 2008). "The Tunguska Mystery". Scientific American: 80–86. Retrieved 8 June 2008.
  51. ↑ "Crater From 1908 Russian Space Impact Found, Team Says". NationalGeographic.com. 28 October 2010. Retrieved 12 September 2011.
  52. ↑ Gasperini, Luca; Bonatti, Enrico; Albertazzi, Sonia; Forlani, Luisa; Accorsi, Carla A.; Longo, Giuseppe; Ravaioli, Mariangela; Alvisi, Francesca; Polonia, Alina; Sacchetti, Fabio (December 2009). "Sediments from Lake Cheko (Siberia), a possible impact crater for the 1908 Tunguska Event". Terra Nova. pp. 489–494. doi:10.1111/j.1365-3121.2009.00906.x.
  53. ↑ "Tunguska Event: Russian Scientists Debunk Meteorite Theory". Sputnik News. 2017-01-18. Retrieved 2017-01-19.
  54. ↑ Kundt, W (2001). "The 1908 Tunguska catastrophe" (PDF). Current Science. 81: 399–407.
  55. ↑ Jones, N. (7 September 2002). "Did blast from below destroy Tunguska?". New Scientist. 2359: 14..
  56. ↑ Kundt, W. (2007). "Tunguska (1908) and its relevance for comet/asteroid impact statistics". In Bobrowsky, P. T.; Rickman, H. Comet/Asteroid Impacts and Human Society. Springer. pp. 331–339..
  57. ↑ "100 years on, mystery shrouds massive 'cosmic impact' in Russia", Agence France-Presse, 29 June 2008.
  58. ↑ Choi, Charles Q., "Massive Tunguska Blast Still Unsolved 100 Years Later", Fox News, 4 July 2008.
  59. ↑ Phipps Morgan, J.; Reston, T. J.; Ranero, C. R. (2004). "Contemporaneous mass extinctions, continental flood basalts, and 'impact signals': are mantle plume-induced lithospheric gas explosions the causal link?" (PDF). Earth and Planetary Science Letters. 217: 263–284. Bibcode:2004E&PSL.217..263P. doi:10.1016/s0012-821x(03)00602-2..
  60. ↑ Vannucchi, P.; Morgan, J. P.; Della Lunga, D.; Andronicos, C. L.; Morgan, W. J. (2015). "Direct evidence of ancient shock metamorphism at the site of the 1908 Tunguska event". Earth and Planetary Science Letters. 409: 168–174. Bibcode:2015E&PSL.409..168V. doi:10.1016/j.epsl.2014.11.001..
  61. ↑ Burghardt, David (22 July 2009). "A century later scientists still at odds on Tunguska Event explanation". RIA Novosti..
  62. ↑ Ol'khovatov, A. Yu. (2003). "Geophysical circumstances of the 1908 Tunguska Event in Siberia, Russia" (PDF). Earth, Moon, and Planets. 93: 163–173. Bibcode:2003EM&P...93..163O. doi:10.1023/B:MOON.0000047474.85788.01..
  63. ↑ Sklublov G. T., Marin Yu. B., Skublov S. G., Bidyukov B. F., Logunova L. N., Gembitsky V. V., Nechaeva E. S. (2010), "Geological and mineralogical-geochemical peculiarities of loose sediments and primary rocks in epicenter of Tunguskaya catastrophe in 1908", Proceedings of the Russian Mineralogical Society, 139(1): 111–135 [in Russian, with English abstract].
  64. ↑ Skublov G. T., Marin Yu. B., Skublov S. G., Logunova L. N., Nechaeva E. S., Savichev A. A. (2011), "Mineralogical-geochemical features of primary rocks, loose sediments and catastrophic mosses in the Northern Swamp area (region of the Tunguska catastrophe in 1908)", Proceedings of the Russian Mineralogical Society, 140(3): 120–138 [in Russian with English abstract].
  65. ↑ Shurmina, Natalia; Kuzmin, Andrey. "Meteorite hits central Russia, more than 500 people hurt". Reuters. Archived from the original on 15 February 2013. Retrieved 15 February 2013.

Bibliography

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