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On the problem of the Tunguska meteorite material
O. G. Gladysheva, 2007. Solar System Research 41(4), 314–321.
Averages measurements of the presumed remnant material, finding it enriched in alkali and alkaline-earth elements and very heterogeneous, and estimates an upper density limit of 2.8 g/cm³ with disintegration into 10⁻⁷ to 10⁻³ m particles.
What it's used for here
The composition and density argument from microscopic remnants.
Our copy
Research copy, for editors and curators. The work is the publisher's, so readers are sent to it. We keep this copy so the citation can be checked if the page changes or goes.
doi.org · fetched 27 Oct 2026
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Cited by on this site 2 records
EVD
The 1908 Tunguska event
MYSThe mystery article
Cite it
Gladysheva, O. G. (2007). On the problem of the Tunguska meteorite material. Solar System Research 41(4), 314–321. https://doi.org/10.1134/S0038094607040041
@article{gladysheva2007material,
author = {Gladysheva, O. G.},
title = {On the problem of the Tunguska meteorite material},
journal = {Solar System Research 41(4), 314–321},
year = {2007},
doi = {10.1134/S0038094607040041},
url = {https://doi.org/10.1134/S0038094607040041}
}TY - JOUR TI - On the problem of the Tunguska meteorite material AU - Gladysheva, O. G. PY - 2007 JO - Solar System Research 41(4), 314–321 DO - 10.1134/S0038094607040041 UR - https://doi.org/10.1134/S0038094607040041 ER -
Gladysheva, O. G.. “On the problem of the Tunguska meteorite material.” Solar System Research 41(4), 314–321 (2007). https://doi.org/10.1134/S0038094607040041.