title: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð¹ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð² Ð³Ð°Ð·Ð¾Ð²ÑÑ Ð»Ð¾Ð²ÑÑÐºÐ°Ñ Ð² ÑÐµÐ³Ð¾Ð»Ð¸ÑÐµ ÐÐ°ÑÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Modeling of possible biological activity in gas trap covers in the Martian regolith
Creators: name: ÐÑÐ·ÑÐµÐ²Ð°, ÐÐ¸Ð°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÐÐµÑÐ°Ð½
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ÐÐµÐ´ ÑÑÑ Ð¾Ð¹
ÐÐ°ÑÑ
Ð¶Ð¸Ð·Ð½Ñ Ð½Ð° ÐÐ°ÑÑÐµ
ÑÐºÑÑÑÐµÐ¼Ð¾ÑÐ¸Ð»Ñ
Ð¿ÐµÑÑ Ð»Ð¾ÑÐ°Ñ Ð½Ð°ÑÑÐ¸Ñ
Ð³Ð°Ð·Ð¾Ð²Ð°Ñ Ð»Ð¾Ð²ÑÑÐºÐ°
Ð¶Ð¸Ð´ÐºÐ¸Ðµ Ð¿Ð¾ÑÐ¾ÐºÐ¸ Ð½Ð° ÐÐ°ÑÑÐµ
Mars
life on Mars
extremophiles
sodium perchlorate
gas trap cover
RSL flows on Mars

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¶Ð¸Ð´ÐºÐ¾Ð³Ð¾ ÑÐ»Ð¾Ñ Ð² Ð¿Ð¾Ð´Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¼ ÑÐ»Ð¾Ðµ ÐÐ°ÑÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¼Ð¾Ð¶ÐµÑ Ð²ÑÑÑÑÐ¿Ð°ÑÑ Ð² ÑÐ¾Ð»Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° Ð±Ð¸Ð¾Ð³ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð½Ð° Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÐµ Ð¿Ð»Ð°Ð½ÐµÑÑ. ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° - Ð¿ÑÐ¾Ð²ÐµÑÐ¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ Ð²ÑÐ¶Ð¸Ð²Ð°ÐµÐ¼Ð¾ÑÑÑ Ð¼Ð¸ÐºÑÐ¾-Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð² Ð¶Ð¸Ð´ÐºÐ¸Ñ ÑÐ¾Ð»ÑÐ½ÑÑ ÑÐ°ÑÑÐ²Ð¾ÑÐ°Ñ (ÑÐ¾ÑÑÐ¾ÑÑÐ¸Ñ Ð¸Ð· Ð¿ÐµÑÑÐ»Ð¾ÑÐ°ÑÐ° Ð½Ð°ÑÑÐ¸Ñ Ð¸ Ð´Ð¸ÑÑÐ¸Ð»Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð²Ð¾Ð´Ñ) Ð² Ð¿Ð¾Ð´Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¼ ÑÐ»Ð¾Ðµ Ð³ÑÑÐ½ÑÐ° Ñ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð½ÑÐ¼Ð¸ Ðº Ð¼Ð°ÑÑÐ¸Ð°Ð½ÑÐºÐ¸Ð¼ ÑÑÐ»Ð¾Ð²Ð¸ÑÐ¼Ð¸ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ, Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð³Ð¸Ð¿Ð¾ÑÐµÐ·Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð° Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÐµ ÐÐ°ÑÑÐ° Ð² ÑÐ¾Ð´Ðµ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼ÐµÑÑÐ½ÑÑ Ð¼Ð¸ÐºÑÐ¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð² Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ Ð¿Ð¾Ð´Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÑ Â«Ð»Ð¾Ð²ÑÑÐºÐ°ÑÂ», ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿Ð¾Ð´Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÑ Ð³Ð°Ð·Ð¾Ð². Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÑÐ¸ÑÑ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ, ÑÑÐ¾ Ð¶Ð¸Ð´ÐºÐ¸Ðµ ÑÐ¾Ð»ÑÐ½ÑÐµ Ð¿Ð¾ÑÐ¾ÐºÐ¸ Ð½Ð° Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ ÐÐ°ÑÑÐ° Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ñ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð³Ð°Ð·Ð° Ð² Ð»ÐµÐ´ÑÐ½Ð¾Ð¹ Ð»Ð¾Ð²ÑÑÐºÐµ Ð¸ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ð¼ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸ÐµÐ¼ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð³Ð°Ð·Ð¾Ð²Ð¾Ð¹ Ð»Ð¾Ð²ÑÑÐºÐ¸ Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼ Ð²ÑÐ±ÑÐ¾ÑÐ¾Ð¼ Ð¸Ð· Ð½ÐµÐµ Ð¿Ð¾Ð´Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÑ Ð¶Ð¸Ð´ÐºÐ¸Ñ ÑÐ°ÑÑÐ²Ð¾ÑÐ¾Ð² Ð½Ð° Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÑ.
description: The given work is devoted to modeling the liquid layer in the subsurface layer of Mars, which can act as a possible source of methane in the atmosphere of the planet. The main objective of the experiment is to test the possible survival of microorganisms in liquid salt solutions (consisting of sodium perchlorate and distilled water) in a subsurface layer of soil with environmental conditions close to Martian; to consider the assumption that methane on the planet appears precisely during the life of local microorganisms in such subsurface "traps", which contain a large amount of subsurface gases. In this work it is also suggested that liquid salt flows on Mars may be caused by the accumulation of gas in the ice trap cover and the further destruction of this gas trap, followed by releasing of subsurface liquid solu-tions from it onto the planetâs surface.