Tunguska cosmic body of 1908: is it from planet Mars?; Arxiv.org

Podrobná bibliografie
Parent link:Arxiv.org.— 2014.— Earth and Planetary Astrophysics
Další autoři: Anfinogenov J., Budaeva L., Kuznetsov D., Anfinogenova Ya. J. Yana Jonovna
Shrnutí:Title screen
The aim of the study was to discover remnants of the 1908 Tunguska meteorite. Mainobjective of the field studies was identification of exotic rocks, furrows, and penetration funnels reported by the first eyewitnesses, residents of the area with severe forest destruction. Main methods included decoding of aerial survey photographs, systematic survey of the epicenter area of the Tunguska explosion, exloratory excavations of the objects of interest, reconstruction studies of exotic boulder by using its splinters, mineralogical and spectral analysis of specimens, experimental attempt of plasma-induced reproduction of the fusion crust on specimen. The authors present results on discovery of penetration funnel-like structures; exotic boulder (known as John's Stone)) with its shear-fractured splinters and fresh furrow in the permafrost; several splinters with glassy coatings; evidence of high-speed John's Stone deceleration in the permafrost; and clear consistency in geometry of spacial arrangements of all splinters, furrows, cleaved pebbles according to data of reconstruction studies. John's Stone is composed of highly silicified gravelite sandstone (98.5% SiO2) with grain size of 0.5 to 1.5 cm. Outer surface of several splinters showed continuous glassy coating similar to shiny fusion crust reminiscent of freshly applied enamel. Plasma-induced heating of John's Stone specimen led to its explosivedisintegration; residue presented with whitish semi-transparent pumice-like grains andirregularly shaped fused particles. Overall, our data suggest that John's Stone is Tunguskameteorite candidate. Recent discoveries of sedimentary rocks, lithified gravelite sandstone, clay, and quartz on Mars provide rationale for search and identification of silica-rich Martian meteorites of sedimentary origin.
Jazyk:angličtina
Vydáno: 2014
Témata:
On-line přístup:http://arxiv.org/abs/1401.6391
Médium: MixedMaterials Elektronický zdroj Kapitola
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=639017

MARC

LEADER 00000naa0a2200000 4500
001 639017
005 20250212113547.0
035 |a (RuTPU)RU\TPU\network\3414 
090 |a 639017 
100 |a 20150218d2014 k||y0rusy50 ba 
101 0 |a eng 
102 |a US 
135 |a drcn ---uucaa 
181 0 |a i  
182 0 |a b 
200 1 |a Tunguska cosmic body of 1908: is it from planet Mars?  |f J. Anfinogenov [et al.] 
203 |a Text  |c electronic 
300 |a Title screen 
320 |a [References.: 27 tit.] 
330 |a The aim of the study was to discover remnants of the 1908 Tunguska meteorite. Mainobjective of the field studies was identification of exotic rocks, furrows, and penetration funnels reported by the first eyewitnesses, residents of the area with severe forest destruction. Main methods included decoding of aerial survey photographs, systematic survey of the epicenter area of the Tunguska explosion, exloratory excavations of the objects of interest, reconstruction studies of exotic boulder by using its splinters, mineralogical and spectral analysis of specimens, experimental attempt of plasma-induced reproduction of the fusion crust on specimen. The authors present results on discovery of penetration funnel-like structures; exotic boulder (known as John's Stone)) with its shear-fractured splinters and fresh furrow in the permafrost; several splinters with glassy coatings; evidence of high-speed John's Stone deceleration in the permafrost; and clear consistency in geometry of spacial arrangements of all splinters, furrows, cleaved pebbles according to data of reconstruction studies. John's Stone is composed of highly silicified gravelite sandstone (98.5% SiO2) with grain size of 0.5 to 1.5 cm. Outer surface of several splinters showed continuous glassy coating similar to shiny fusion crust reminiscent of freshly applied enamel. Plasma-induced heating of John's Stone specimen led to its explosivedisintegration; residue presented with whitish semi-transparent pumice-like grains andirregularly shaped fused particles. Overall, our data suggest that John's Stone is Tunguskameteorite candidate. Recent discoveries of sedimentary rocks, lithified gravelite sandstone, clay, and quartz on Mars provide rationale for search and identification of silica-rich Martian meteorites of sedimentary origin. 
463 |t Arxiv.org  |v Earth and Planetary Astrophysics  |d 2014 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
701 1 |a Anfinogenov  |b J. 
701 1 |a Budaeva  |b L. 
701 1 |a Kuznetsov  |b D. 
701 1 |a Anfinogenova  |b Ya. J.  |c medic  |c Lecturer of Tomsk Polytechnic University, Doctor of medical sciences  |f 1970-  |g Yana Jonovna  |3 (RuTPU)RU\TPU\pers\33592 
801 2 |a RU  |b 63413507  |c 20150317  |g RCR 
856 4 |u http://arxiv.org/abs/1401.6391 
942 |c CF