Короны-источники молодого вулканизма на Венере: топографические особенности и оценки продуктивности

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Abstract

Выполненное нами исследование пространственной и генетической связи корон и лопастных равнин позволяет сделать два важных вывода. 1) Около 17% всех вулканических корон Венеры являются источниками молодых лав, образующих лопастные равнины Атлийского периода (короны-источники). Малая доля корон-источников в общей популяции корон отражает снижение темпа формирования мантийных диапиров. 2) Площадь лопастных равнин, связанных с той или иной короной, и площадь самой короны связаны отрицательной корреляцией. Такие соотношения допускают существование только двух моделей завершающих стадий эволюции мантийных диапиров. Проанализировав обе эти модели, мы предполагаем, что в течение Атлийского периода геологической истории Венеры либо существовала единая зона нейтральной плавучести, либо подошва литосферы располагалась примерно на одном уровне.

About the authors

Е. Н. Гусева

Институт геохимии и аналитической химии им. В.И. Вернадского РАН

Author for correspondence.
Email: guseva-evgeniya@yandex.ru
Russian Federation, Москва

М. А. Иванов

Институт геохимии и аналитической химии им. В.И. Вернадского РАН

Email: guseva-evgeniya@yandex.ru
Russian Federation, Москва

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