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Important Deadlines and News

Upcoming deadlines / important events
Application deadline: 2020-01-06
Research assistant (PhD student/praedoc) reference code: OREOcube-Exocube

Deadline for application: 2020-01-17
AIAS-COFUND Marie Skłodowska-Curie Fellowships

Deadline for Registration and abstract submission: 2020-06-30
Fifth Network of Researchers on the Chemical Evolution of Life (NoR CEL) Conference

Abstract submission deadine: 2020-01-15
Biennial European Astrobiology Conference (BEACON)

Registration deadline: 2020-01-30
Introductory Astrobiology Course RED'20

Poster abstract submission deadline: 2020-05-25
Molecular Origins of Life, Munich (MOM) conference

Registration and accommodation booking deadline: 2020-02-01
Biennial European Astrobiology Conference (BEACON)

Registration deadline: 2020-06-21
Molecular Origins of Life, Munich (MOM) conference

EANA2020
EANA2020 will take place in Bologna (IT) from 1 to 4 September.
Details will be provided in January.

Added 6 Dec 2019
NASA Astrobiology Program FAQs
The NASA Astrobiology Program has announced a new programmatic infrastructure. Known as Research Coordination Networks (RCNs), and first deployed as the Nexus for Exoplanet System Science (NExSS), RCNs bring together researchers who are funded from a variety of sources into interdisciplinary, topically-focused research groups. By early 2020, the NASA Astrobiology Program will have activated five RCNs -- four new ones plus NExSS -- each organized around a key research topic identified in the 2015 Astrobiology Strategy: prebiotic chemistry and the early Earth; early metabolism, evolution, and complexity; life detection on other worlds; habitable worlds (initially focused on ocean worlds); and exoplanet system science.

This document contains answers to Frequently Asked Questions about the Astrobiology Program organized by topical areas.

Added 9 Nov 2018

Monthly research highlight (-> More highlights)

Thogersen et al. (2019): Light on windy nights on Mars: A study of saltation-mediated ionization of argon in a Mars-like atmosphere

Icarus 2019, 332, 14-18, DOI:10.1016/j.icarus.2019.06.025

Link to paper

Laboratory experiments show that sand grain saltation in a Mars-like environment can result in the ionization of argon. This suggests that saltation can be a mechanism for the destruction of methane (CH4) on Mars given the ionization energy of argon is higher than the energy required to ionize methane to a reactive cation. The ionization energy is also higher than the energy to dissociate methane to highly reactive species like CH3, CH2, and CH. The feasibility of capturing the resulting emission glow on a windy Martian night is discussed.
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