H2020Индивидуална стипендия2017–2019

D BIOME · Deep Biosignatures on Mars and Earth

„Хоризонт 2020“ — Действия „Мария Склодовска-Кюри“

Период
2017-10-01 → 2019-10-04
Финансиране от ЕС
183 455 €
Участници
1
Схема
MSCA-IF-EF-ST

Линиите свързват координатора с партньорите.

Накратко на български

Древни следи от живот в дълбоките слоеве на земната кора и скалите на Марс се анализират чрез търсене на биосигнатури. Това помага да се разбере как животът е оцелял под повърхността на двете планети без слънчева светлина.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

Deep Biosignatures on Mars and Earth

"This research addressed fundamental science questions about the distribution of life on Earth, the history of life on Earth, and the ongoing multi-billion dollar search for life on Mars. It has become clear in recent decades that living organisms thrive throughout the Earth's crust to depths of several kilometres. Many subsurface ecosystems are sustained by chemical reactions between water and basaltic rock and do not require sunlight or any input of organic matter from the surface. These same conditions could have supported life on Mars long after the surface became uninhabitable. Thus, there is considerable interest in how current and future Mars missions may identify the traces of ancient subsurface life preserved in rocks now exposed on the martian surface. At the same time, the realisation that a sizeable proportion of terrestrial life resides underground motivates questions about the role of deep life in the history of our own planet. Answering these questions requires us to identify robust evidence of ancient subsurface life in rocks, and to piece this evidence together into an integrated archive: a fossil record. Against this background, the present work was originally directed towards four main objectives: 1. To identify and describe ancient deep biosignatures (""fossils"") in both marine and terrestrial rocks on Earth, showing how their origin can be interpreted and confirmed, and extending the deep fossil record. 2. To determine experimentally whether ancient deep biosignatures in rocks on Mars could be detected by rover instruments if they are exist and are exposed on the surface, particularly using the European Space Agency’s ExoMars rover (now named Rosalind Franklin). 3. To simulate the crustal subsurface (~100–1000 m deep) experimentally and discover which environmental parameters most strongly affect the growth of microorganisms and the production of biosignatures in these conditions. 4. To model how the rock- and sediment-hosted deep biosphere has changed in size and activity over the history of the Earth, and show how an analogous biosphere could have done so if it ever existed on Mars. The main conclusions of the work were: 1. A fossil record of the deep biosphere exists but is more difficult than previously thought to distinguish from non-biological microscopic structures (pseudofossils). 2. Calcium sulfate veins, which are widespread on Mars, have the potential to yield organic residues and other chemical (isotopic) evidence of ancient subsurface life. 3. The biomass of life on Earth was dominated by subsurface organisms for at least two billion years. 4. Sediment-dwelling microbes may have played key roles in the preservation of fossils of early macro-organisms on Earth."

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

In recent decades, samples from mines and boreholes have revealed that our planet’s biosphere extends several miles downwards into the crust. Pores and fissures far below the seafloor and land surface are populated by vast numbers of microorganisms, with broad economic and scientific implications. These implications reach as far as Mars, whose subsurface has provided a potentially habitable environment for billions of years, protected from the hostile conditions at the surface. Although Earth's modern-day ""deep biosphere"" is now the subject of a major global research effort, almost nothing is known about its variation across geological time, which may have been considerable and highly consequential for planetary biogeochemistry. This project will combine state-of-the-art analyses of fossil and chemical traces of deep life (""deep biosignatures"") with experimental and modelling work to elucidate the abundance, activity and geological record of ancient subsurface life on Earth and its possible relevance for Mars. Dr McMahon’s research at the UK Centre for Astrobiology (School of Physics and Astronomy, University of Edinburgh) will be directed towards four main objectives, as follows:1. To identify and describe ancient deep biosignatures in both marine and terrestrial rocks on Earth, showing how their deep origin can be confirmed, and extending the deep fossil record.2. To conduct experiments to determine whether and how, if they exist, deep biosignatures could be detected in rocks on Mars by rover instruments—particularly those on the European ExoMars rover.3. To simulate experimentally the conditions deep below the surface of Earth and Mars and discover which environmental parameters most strongly affect the growth of relevant deep microorganisms and the production of biosignatures.4. To model how the deep biosphere has changed in size and activity over the history of the Earth, and how a deep biosphere on Mars, if it ever existed, could have done so.""

Оригинален текст от CORDIS (на английски).

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Данни: CORDIS, © Европейски съюз