geolmsuВЕСТНИК МОСКОВСКОГО УНИВЕРСИТЕТА. СЕРИЯ 4. ГЕОЛОГИЯMoscow University Bulletin. Series 4. Geology0579-9406Издательский Дом МГУ10.55959/MSU0579-9406-4-2023-63-2-3-13geolmsu-573Research ArticleСтатьиГенетические типы грязевого вулканизма в районах Cydonia и Acidalia на МарсеGenetic types of mud volcanism in the Cydonia and Acidalia regions of MarsЧуЦ.ChuJ.

Цзюнь Чу

Москва

Chu Jun

Moscow

vladimirchujun@yandex.ruИвановМ. А.IvanovM. A.

Михаил Арсеньевич Иванов

Москва

Mikhail A. Ivanov

Moscow

mikhail_ivanov@brown.eduНикишинА. М.NikishinA. M.

Анатолий Михайлович Никишин

Москва

Anatoly M. Nikishin

Moscow

amnikishin@gmail.comМосковский государственный университет имени М. В. ЛомоносоваРоссияLomonosov Moscow State UniversityRussian FederationИнститут геохимии и аналитической химии им. В. И. Вернадского РАНРоссияVernadsky Institute of Geochemistry and Analytical ChemistryRussian Federation20230706202302313Copyright © Чу Ц., Иванов М.А., Никишин А.М., 20232023Чу Ц., Иванов М.А., Никишин А.М.Chu J., Ivanov M.A., Nikishin A.M.Данная работа распространяется под лицензией Creative Commons Attribution 4.0.This work is licensed under a Creative Commons Attribution 4.0 License.https://vestnik.geol.msu.ru/jour/article/view/573

Малые конусообразные структуры широко распространены на северных равнинах Марса. Они обычно интерпретируются как грязевые вулканы из-за их близкого морфологического сходства с грязевыми вулканами Земли (например, в Азербайджане и около Азовского моря). Если такая интерпретация верна, то малые конусы могут служить свидетельством существования обширного подповерхностного грязевого источника, который, в свою очередь, мог быть образован донными отложениями крупного водного резервуара (океана), существовавшего на северных равнинах Марса в прошлые эпохи геологической истории этой планеты. По сравнению с грязевыми вулканами Земли, морфология малых конусов на Марсе меняется в более широком диапазоне, что может быть связано с большим разнообразием механизмов формирования марсианских холмов. В данном исследовании мы изучали морфологию малых холмов в областях Cydonia и восточная Acidalia, которые расположены вблизи дихотомической границы в пределах северных равнин Марса и установили, что существуют 5типов холмов, морфология которых, вероятно, характеризует особенности водо-грязевого резервуара.

Small cone/mound-shaped structures are widespread on the northern plains of Mars. They are usually interpreted as mud volcanoes because of their close morphological resemblance to mud volcanoes on Earth (for example, in Azerbaijan and near the Sea of Azov). If this interpretation is correct, the small cones/mounds could be evidence of the existence of an extensive subsurface mud source, which, in turn, could be formed by the bottom sediments of a large water reservoir (ocean) that existed on the northern plains of Mars in the past eras of this planet’s geological history. Compared to mud volcanoes on Earth, the morphology of small cones/mounds on Mars varies over a wider range and, which may be due to a greater variety of mechanisms of formation of Martian cones/ mounds. In this study, we studied the morphology of small hills in the Cydonia and eastern Acidalia regions, which are located near the dichotomous boundary within the northern plains of Mars and found that there are 5types of cones/mounds, whose morphology probably characterizes the water-mud reservoir features.

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The authors declare that there are no conflicts of interest present.