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Amegacryometeor is a very large chunk ofice which, despite sharing many textural, hydro-chemical, and isotopic features found in largehailstones, is formed under unusual atmospheric conditions which clearly differ from those of thecumulonimbus cloud scenario (i.e. clear-sky conditions). They are sometimes called huge hailstones, but do not need to form underthunderstorm conditions unlike hailstorms. Jesús Martínez-Frías, a planetarygeologist andastrobiologist at Institute of Geosciences (Spanish:Instituto de Geociencias,IGEO) in theSpanish National Research Council (Spanish:Consejo Superior de Investigaciones Científicas,CSIC)[1] inMadrid, pioneered research into megacryometeors.
More than 50 megacryometeors have been recorded since the year 2000. They vary in mass between 0.5 kilograms (1.1 lb) to several tens of kilograms. One inBrazil weighed in at more than 50 kilograms (110 lb).[2]Chunks about 2 m (6 ft 7 in) in size also fell in Scotland on 13 August 1849.[3]
The process that creates megacryometeors is not completely understood yet, mainly with respect to the atmospheric dynamics necessary to produce them. They may have a similar mechanism of formation that leads to the production of hailstones.[4] Scientific studies show that their composition matches normal troposphericrainwater for the areas in which they fall. In addition, megacryometeors also display textural variations of the ice surface and hydro-chemical and isotopic heterogeneity in its composition, which gives potential evidence to a complex formation process in the loweratmosphere.[5][6][7] It is known that they do not form from airplane toilet leakage because the large chunks of ice that occasionally do fall from airliners are distinctly blue due to thedisinfectant used by them (hence their common name of "blue ice").
Some have speculated that these ice chunks must have fallen from aircraft fuselages[4] after plain water ice accumulating on those aircraft through normal atmospheric conditions has simply broken loose. However, similar events also occurred prior to the invention of aircraft.[8][9] Studies indicate that the metrological fluctuations intropopause, associated with hydration of the lowerstratosphere and stratospheric cooling, can be related to their formation.[5] A detailed micro-Raman spectroscopic study made it possible to place the formation of the megacryometeors within a particular range of temperatures: −10 to −20 °C (14 to −4 °F).[10] They are sometimes confused withmeteors because they can leave smallimpact craters, though they form in theatmosphere and not fromouter space.
