Вісник Астрономічної школи, 2016, том 12, № 1, с. 14–26

https://doi.org/10.18372/2411-6602.12.1014
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Активність процесів на видимих поверхнях тіл Сонячної системи

Відьмаченко А.П.

Головна астрономічна обсерваторія НАН України

Реферат

Розглянуто фізичні процеси на поверхнях тіл Сонячної системи, які приводять до видимих змін їх відбивальних характеристик. Показано, що для кожного тіла у Сонячній системі є набір таких хімічних елементів та їх з'єднань, перетворення яких показує суттєву активність у такому значному діапазоні зміни температури від понад 700 К (для Меркурія) до 30 К для Плутона. Тобто всі об'єкти у Сонячній системі проявляють відчутну активність. Проте вони є дуже індивідуальними щодо набору і типу проціесів, які мають місце на кожному тілі Сонячної системи.

Ключові слова: процессы на поверхности; тела Солнечной системы; отражательные характеристики

Перелік посилань

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