Diamonds as the key to unravel the origin of Earth's water
This project aims to determine Earth's primordial deuterium-to-hydrogen ratio using ancient diamonds to uncover the origin of Earth's water and implications for planetary habitability.
Projectdetails
Introduction
The origin of Earth's water is still an unsolved mystery in Earth Sciences. Yet, answering this question is paramount in order to validate planetary accretion models and determine the conditions for life-sustainable planets to form.
Importance of D/H Ratio
Comparing Earth's original deuterium-to-hydrogen ratio (D/H) with those of Solar system objects such as meteorites, comets, and the solar nebula can constrain the provenance of water. However, while D/H is precisely determined for extra-terrestrial objects, the exact value for Earth is not known. This uncertainty arises from the fact that Earth's primordial D/H has been lost since its formation due to surface and mantle geological processes.
Challenges in Current Estimates
Current estimates from mantle-derived lavas are challenged by the ability of these samples to retain pristine values. This indicates the need for a pristine reservoir that has remained unaffected over geological time to be found.
Role of Diamonds
Diamonds from the Earth's mantle may be key as they contain trace amounts of hydrogen and are inert and robust time capsules able to survive over several billion years.
Project Goals
The overarching goal of this project is to determine Earth's primordial D/H by investigating the hydrogen content and isotopic composition of a unique set of worldwide, natural diamonds dating from 3.5 to 0.09 billion years ago. This will be achieved using newly-developed, high-precision, and high-efficiency isotope ratio mass spectrometry.
Methodology
The isotopic data will be complemented by atomistic state-of-the-art ab initio simulations to understand the atomic and diffusion behavior of hydrogen in natural diamonds.
Long-term Implications
The new results will be fundamental to pinpoint Earth's water origin, with long-term implications for understanding planet habitability. In a time when international space agencies are actively searching for potentially habitable planets and extra-terrestrial life, this new knowledge will be crucial for understanding the geological and biological evolution of planets in our Solar System and beyond.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.499.758 |
Totale projectbegroting | € 1.499.758 |
Tijdlijn
Startdatum | 1-1-2023 |
Einddatum | 31-12-2027 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- UNIVERSITA DEGLI STUDI DI PADOVApenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
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Atmospheric tracing of Earth's evolutionProject ATTRACTE aims to enhance understanding of Earth's atmospheric evolution by analyzing paleo-atmospheric gases and integrating data into models for insights on habitability and exoplanetary geology. | ERC Starting... | € 2.499.125 | 2023 | Details |
Hydrogen and deuterium survey of minor bodies: transformative science with a purpose-built CubeSatThe project aims to develop a miniature UV space telescope using CubeSats to detect hydrogen and deuterium around comets and asteroids, enhancing our understanding of water's origin on Earth. | ERC Consolid... | € 3.000.000 | 2023 | Details |
A Primitive solar Atmosphere around The young Earth?The APATE project aims to investigate the isotopic composition of neon in Earth's mantle to assess the origins of a primordial H2/He-rich atmosphere and its implications for Earth's composition. | ERC Advanced... | € 2.784.505 | 2023 | Details |
New isotope tracers of rocky planet forming environmentsThis project aims to uncover the origins and evolution of precursor materials for terrestrial planets by analyzing chondrules in meteorites using advanced isotopic and imaging techniques. | ERC Consolid... | € 1.970.878 | 2024 | Details |
The role of silica in the dawn of life on our planet
The PROTOS project aims to simulate Hadean conditions through laboratory experiments to uncover the role of silica in early Earth's organic chemistry and the origin of life.
Atmospheric tracing of Earth's evolution
Project ATTRACTE aims to enhance understanding of Earth's atmospheric evolution by analyzing paleo-atmospheric gases and integrating data into models for insights on habitability and exoplanetary geology.
Hydrogen and deuterium survey of minor bodies: transformative science with a purpose-built CubeSat
The project aims to develop a miniature UV space telescope using CubeSats to detect hydrogen and deuterium around comets and asteroids, enhancing our understanding of water's origin on Earth.
A Primitive solar Atmosphere around The young Earth?
The APATE project aims to investigate the isotopic composition of neon in Earth's mantle to assess the origins of a primordial H2/He-rich atmosphere and its implications for Earth's composition.
New isotope tracers of rocky planet forming environments
This project aims to uncover the origins and evolution of precursor materials for terrestrial planets by analyzing chondrules in meteorites using advanced isotopic and imaging techniques.