Origin of John’s Stone: A quartzitic boulder from the site of the 1908 Tunguska (Siberia) explosion; Icarus; Vol. 258

Bibliografiske detaljer
Parent link:Icarus: Scientific Journal
Vol. 258.— 2015.— [P. 297-308]
Institution som forfatter: Национальный исследовательский Томский политехнический университет (ТПУ) Физико-технический институт (ФТИ) Кафедра иностранных языков физико-технического института (ИЯФТ)
Andre forfattere: Bonatti E. Enrico, Breger D. Dee, Tommaso D.R. Di Rocco, Fulvio F. Franchi, Luca G. Gasperini, Polonia A. Alina, Anfinogenov J. John, Anfinogenova Ya. J. Yana Jonovna
Summary:Title screen
An exotic meter-size quartzitic boulder known as John’s Stone was found by John Anfinogenov in 1972 buried in permafrost close to the epicenter of the 1908 Tunguska blast in a region of Siberia dominated by Permian–Triassic Siberian Trap basalts. The boulder is made almost entirely of well-cemented quartz grains, mostly around 100 µm in size; it contains zones with coarser or finer grain sizes. Rare zircon and rutile crystals are scattered within the quartz matrix. Quartz is often dissected by strain lamellae. The rock contains abundant scattered internal vugs rimmed by euhedral quartz crystals. We cannot exclude that John’s Stone is a fragment of a Permian granite-derived sandstone unit. However, based on structure, mineralogy and chemistry the quartzitic boulder may have originated due to silica deposition from hydrothermal solutions that had reacted with basaltic rocks. Anfinogenov et?al. (Anfinogenov, J. et?al. [2014]. Icarus 243, 139–147) interpreted features observed in the permafrost at the base of the boulder as indicating it impacted from above, suggesting the boulder may be a meteorite, possibly of martian origin, given the reported presence on Mars of silica-rich deposits. Triple oxygen isotope ratios determined on two samples of the quartzite reveal a terrestrial rather than a martian meteorites composition. Oxygen isotope data suggest also that the precipitation of SiO2 could have occurred in equilibrium with hydrothermal water (d18Ow ˜ -19.5‰) at the temperature of about 50 °C. The thermal event that generated the quartzite may be related either to the century-old Tunguska Event, or, more probably, to Permian–Triassic Siberian Traps magmatism, although an extraterrestrial origin cannot be completely ruled out.
Режим доступа: по договору с организацией-держателем ресурса
Sprog:engelsk
Udgivet: 2015
Fag:
Online adgang:http://dx.doi.org/10.1016/j.icarus.2015.06.018
Format: Electronisk Book Chapter
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=643884

MARC

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200 1 |a Origin of John’s Stone: A quartzitic boulder from the site of the 1908 Tunguska (Siberia) explosion  |f E. Bonatti [et al.] 
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300 |a Title screen 
330 |a An exotic meter-size quartzitic boulder known as John’s Stone was found by John Anfinogenov in 1972 buried in permafrost close to the epicenter of the 1908 Tunguska blast in a region of Siberia dominated by Permian–Triassic Siberian Trap basalts. The boulder is made almost entirely of well-cemented quartz grains, mostly around 100 µm in size; it contains zones with coarser or finer grain sizes. Rare zircon and rutile crystals are scattered within the quartz matrix. Quartz is often dissected by strain lamellae. The rock contains abundant scattered internal vugs rimmed by euhedral quartz crystals. We cannot exclude that John’s Stone is a fragment of a Permian granite-derived sandstone unit. However, based on structure, mineralogy and chemistry the quartzitic boulder may have originated due to silica deposition from hydrothermal solutions that had reacted with basaltic rocks. Anfinogenov et?al. (Anfinogenov, J. et?al. [2014]. Icarus 243, 139–147) interpreted features observed in the permafrost at the base of the boulder as indicating it impacted from above, suggesting the boulder may be a meteorite, possibly of martian origin, given the reported presence on Mars of silica-rich deposits. Triple oxygen isotope ratios determined on two samples of the quartzite reveal a terrestrial rather than a martian meteorites composition. Oxygen isotope data suggest also that the precipitation of SiO2 could have occurred in equilibrium with hydrothermal water (d18Ow ˜ -19.5‰) at the temperature of about 50 °C. The thermal event that generated the quartzite may be related either to the century-old Tunguska Event, or, more probably, to Permian–Triassic Siberian Traps magmatism, although an extraterrestrial origin cannot be completely ruled out. 
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463 |t Vol. 258  |v [P. 297-308]  |d 2015 
610 1 |a электронный ресурс 
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701 1 |a Bonatti  |b E.  |g Enrico 
701 1 |a Breger  |b D.  |g Dee 
701 1 |a Tommaso  |b D.R.  |g Di Rocco 
701 1 |a Fulvio  |b F.  |g Franchi 
701 1 |a Luca  |b G.  |g Gasperini 
701 1 |a Polonia  |b A.  |g Alina 
701 1 |a Anfinogenov  |b J.  |g John 
701 1 |a Anfinogenova  |b Ya. J.  |c Linguist  |c Lecturer of Tomsk Polytechnic University, Doctor of medical sciences  |f 1970-  |g Yana Jonovna  |3 (RuTPU)RU\TPU\pers\33592 
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