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The quest to understand interstellar sulfur and metal chemistry through synergetic laboratory and radio telescope observations

Project description

Written in (between) the stars

The number of stars in the universe has been compared to the number of grains of sand on all the beaches on Earth. However, unlike sand, the stars are distantly spaced. Filling the spaces is the interstellar medium (ISM), consisting of about 99 % gas and 1 % dust. Understanding the physical properties and chemical behaviours of the constituents of the ISM is of critical importance to our understanding of star and galaxy formation and evolution, planet formation and the origins of life. However, relatively little is known about the structure and evolution of the ISM in large part due to the very low abundance of constituents. The EU-funded AstroSsearch project plans to increase our knowledge regarding the gaps between the stars with a combination of laboratory experiments and astronomy observations.

Objective

The fellowship AstroSsearch addresses open questions related to the abundance of sulfur and metals in the interstellar medium. While some species have been detected in astronomical environments, their abundance and complexity is quite low, thereby preventing a full understanding of the chemistry occurring in these environments. We will attack this problem with a synergic approach exploiting new laboratory microwave spectroscopy developments and radio astronomy observations. The key objectives include the generation of high-resolution rotational spectra of previously undetected sulfur/metal containing compounds and ions by mating broadband (chirped-pulse Fourier transform) microwave spectroscopy techniques with electrical discharge and laser ablation sources. Additionally, a novel discharge source will be developed in which the chemistry can be controlled to reveal likely reaction pathways that produce the observed species. This will allow for the postulation of viable astronomical formation mechanisms. The expected results are:
(1) Development of a new controlled reactive chemistry source that can be paired with laser ablation.
(2) High-resolution, rotational spectra of complex sulfur and metal containing species leading to their unambiguous identification in interstellar environments and their inclusion in theoretical models.
(3) Elucidation of viable reaction pathways in astronomical environments for targeted and detected species and the insertion of these pathways into existing models.
These results will facilitate radio astronomy detections, expanding our comprehension of astronomical chemistry. The synergy of laboratory spectroscopy and observational astrophysics will bring together all facets of the multidisciplinary field of astrochemistry, broadening our understanding of the chemistry that is occurring in interstellar and circumstellar environments and shedding light on the chemical complexity of the universe.

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Programme(s)

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Topic(s)

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MSCA-IF - Marie Skłodowska-Curie Individual Fellowships (IF)

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Call for proposal

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(opens in new window) H2020-MSCA-IF-2019

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Coordinator

UNIVERSIDAD DE VALLADOLID
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 172 932,48
Address
PLAZA SANTA CRUZ 8 PALACIO DE SANTA CRUZ
47002 VALLADOLID
Spain

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Region
Centro (ES) Castilla y León Valladolid
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 172 932,48
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