Assessment of “Meteor Airburst” Radiation in the Atmosphere of Venus

In addition to craters, radar-bright and dark spots are observed on the surface of Venus. Their formation is presumed to be caused by the effects of shock waves generated by “meteor airbursts.” One reason for the formation of dark spots, which correspond to a smoother surface, could be the melting and evaporation of the surface layer due to radiation from the shock wave. Direct calculations of the fragmentation and deceleration of asteroids with sizes of 0.6–1 km conducted in this work, along with assessments of the resulting radiation and its effect on the surface, have shown that within an area with a characteristic size of several tens of kilometers, the thickness of the evaporated/melted layer is several centimeters. The flow of the melt and the deposition of condensed vapors can significantly smooth the surface and affect its reflective properties.

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Publication Details

Journal
Solar System Research
Published
2025-12-01
DOI
https://doi.org/10.1134/s0038094625600751
Primary Topic
Planetary Science and Exploration
Type
article
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article

Assessment of “Meteor Airburst” Radiation in the Atmosphere of Venus

В. В. Шувалов, B. A. Ivanov
Solar System Research
Planetary Science and Exploration
article

Assessment of “Meteor Airburst” Radiation in the Atmosphere of Venus

В. В. Шувалов, B. A. Ivanov
article en

Abstract

In addition to craters, radar-bright and dark spots are observed on the surface of Venus. Their formation is presumed to be caused by the effects of shock waves generated by “meteor airbursts.” One reason for the formation of dark spots, which correspond to a smoother surface, could be the melting and evaporation of the surface layer due to radiation from the shock wave. Direct calculations of the fragmentation and deceleration of asteroids with sizes of 0.6–1 km conducted in this work, along with assessments of the resulting radiation and its effect on the surface, have shown that within an area with a characteristic size of several tens of kilometers, the thickness of the evaporated/melted layer is several centimeters. The flow of the melt and the deposition of condensed vapors can significantly smooth the surface and affect its reflective properties.

Solar System ResearchVol. 59(7)
Institute of Geosphere Dynamics (RU)
Openalex Percentile: Top 73%
Planetary Science and Exploration
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