22-EPN3-049: Retrieving multiple ice cores to study the link between the solar cycle and the cosmogenic tritium in precipitation

22-EPN3-049: Retrieving multiple ice cores covering the last 100 years to study the link between the solar cycle and the cosmogenic tritium in precipitation.

Visit by László Palcsu and Marjan Temovski (Institute for Nuclear Research, Hungary) to TA1.4 AU Greenland Kangerlussuaq Field Site (Greenland).
Dates of visit: 19-23 June 2023

Report Summary:

The objective of the mission was to retrieve multiple ice cores at the EGRIP site (75°37′N, 35°59′W, 2702 m a.s.l.) to study the natural as well as anthropogenic variation of tritium in the ice layers. We have studied the recent publications, which suggest lower snow accumulation rate than what we have previously thought. Therefore, we intended to drill more shallow cores. During five days at EGRIP (19-23 June 2023), we drilled five 24 m-long ice cores representing the last 100-110 years. The ice cores were cut into subsamples of 15 cm, and packed into plastic containers. One full core was collected. The bottom part (depth between 16.2 and 24.0 m) of the additional 4 cores was also collected to get more material for sensitive analysis of tritium by the 3He-ingrowth method.  Altogether 368 samples have been collected. Besides the cosmogenic tritium, stable isotopes of water, and Sr-Nd-Hf isotope signatures will be also analysed. To compare this latter to older ice (>10,000 years), we took ice samples at the ice margin in a location between the glaciers Isunnguata Sermia and Russell about 36 km from Kangerlussuaq, near Point 660. The ice there is supposed to be around 40,000 years old. We drilled a shallow core (~ 4 m), cut into 10 pieces, and stored in pre-cleaned plastic vessels. All of the ice samples have been already shipped to our laboratory in Hungary. The first analyses for stable isotopes, 137Cs around the Chernobyl event, and tritium around the bomb-peak have been already started.

Drilling down to 24 m in the clean area of the EGRIP site, Kangerlussuaq,
Drilling down to 24 m in the clean area of the EGRIP site, Kangerlussuaq, Greenland. Credit: László Palcsu.

Read full scientific report with kind permission by László Palcsu.


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22-EPN3-126: In-Situ observations in support for VERITAS Venus analogue airborne radar campaign at Holuhraun and Djyngasandur, Iceland

22-EPN3-126: In-Situ observations in support for VERITAS Venus analogue airborne radar campaign at Holuhraun and Djyngasandur, Iceland

Solmaz Adeli and Stephen Patrick Garland (German Aerospace Center (DLR), Germany) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 1-14 August 2023

The composition of lava fields on Venus and their alteration state is poorly understood. The Venus Emissivity Mapper (VEM)/VERITAS will observe the surface of Venus in the NIR range, which will allow studying the spectral characteristics of the Venusian surface, as well as the type of lava and likely alteration processes. To prepare for this mission, VERITAS organised a field campaign in Iceland in early August, 2023, which included in-situ NIR data acquisition by the DLR-Berlin team, enabled through this Europlanet funding. The main goals have been 1) to understand the in-situ NIR reflectance spectral response of Venus analogue material, 2) to acquire in-situ emittance of an active volcano in the NIR spectral range, 3) to collect samples to be analysed in the Planetary Spectroscopy Laboratory (PSL-DLR-Berlin) using reflectance and emittance spectroscopy methods, to create an emissivity spectral library, and 4) to compare the laboratory data with field measurements.

In order to collect a wide range of textures (from pahoehoe to a’a) and compositional variations of basaltic lava fields, in addition to different fumarolic deposits, the team visited and imaged the Holuhraun lava field, Askja lava field, and Fagradalsfjall area. These sites offer an age range from the altered 1960 Askja lava field to the 2023 eruption in Fagradalsfjall. The Askja and Holuhraun sites also offered variation in grain sizes and tefra and sand coverage, which affects the spectral behavior of the surface material in NIR. the team also collected about 60 kg of samples to be analysed in the Venus chamber of the PSL-DLR-Berlin.

Photos from the campaign can be found in the DLR Flickr Album: VERITAS – Expedition for NASA & ESA Missions to Venus:

VERITAS

22-EPN3-129: In-situ and laboratory spectroscopic characterisation of Icelandic lava flows

22-EPN3-129: In-situ and laboratory spectroscopic characterisation of Icelandic lava flows; an analogue of Venus – VERITAS mission preparation

Nils Mueller and Akin Domac (German Aerospace Center (DLR), Germany) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 1-7 August 2023

As part of collaborative field work of the VERITAS science team, Nils Mueller and Akin Domac visited several locations with partially sediment covered lava flows in the vicinity of Askja, Vatnajokull National Park, Iceland. This was done simultaneously with an airborne radar campaign by the German Aerospace Center {DLR. e.V.) acquiring synthetic aperture radar images at X- and S-band, the wavelengths of the radar instruments on the Venus orbiters VERITAS and Magellan, respectively. The objective of the field­work was to document the nature and extend of sediment cover on lava flows and how it affects scattering and roughness at radar wavelengths. This will improve the combined Magellan/VERITAS SAR image interpretation by providing in-situ data that can be tied to specific S and X band backscatter values. Another aspect is change detection as the same airborne radar collected data of the near pristine Holuhraun lava flow in 2015.

The field work data collected includes photos, notes, LIDAR scans of SxS m2 patches, and clast and sediment samples from the the surface and, if possible, from 20 cm depth. The initial observations show that parts of the Holuhraun lava flow have been significantly modified by aeolian sediments in the 8 years since the end of the eruption. These sediments affect the roughness on radar wavelengths but also radar backscatter via changes in composition, density, clast size, and water content. Whether the changes are notable in the radar images remains to be seen, as the interpretation is ongoing.

Photos from the campaign can be found in the DLR Flickr Album: VERITAS – Expedition for NASA & ESA Missions to Venus:

VERITAS

20-EPN2-071: Deposition of organic matter as a factor controlling microbial colonisation of analogue terrestrial surfaces

20-EPN2-071: Deposition of organic matter as a factor controlling microbial colonisation of analogue terrestrial surfaces

Tina Santl-Temkiv (Aarhus University, Denmark) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 29-30 June 2023

This project was designed to improve the understanding of biosignatures in analogue terrestrial surfaces, volcanic rocks, that result as a consequence of microbial colonisation and weathering. During the visit, the automatic medium-volume sampling system PNS DM — modified to run on batteries charged with solar panels — was assembled, tested, and calibrated in the laboratory of Matis.

Due to a delay in shipment of the solar panels, the installation of the system at the field site could not be performed but will be finalised by the host institution in the near future. As a part of the visit, the area of the Fagradalsfjall volcano was visited and the location where the sampling system will be installed was discussed. Once the sampler system will be installed in proximity of the Fagradalsfjall volcano crater, aerosol samples will be collected continuously for a year along with replicate rock samples in order to investigate the impact of aerosol deposition on rock microbial community assembly, using microbial, chemical and physical analysis. This will be performed in collaboration between the team of Prof. Viggó Þór Marteinsson and the team of Assoc. Prof. Tina Santl-Temkiv and will result in greatly improved understanding of colonisation, community assembly, and biosignature emergence in analogue terrestrial surfaces.

Read the full scientific report with kind permission by Tina Santl-Temkiv.

Banner image: Iceland’s Fagradalsfjall volcano. Credit: CC BY-SA 4.0 Mokslo Sriuba


22-EPN3-007: SeisChem – The influence of seismic events on fluid and gas chemistry at the Icelandic planetary field site

22-EPN3-007: SeisChem – The influence of seismic events on fluid and gas chemistry at the Icelandic planetary field site

Visit by John Edgar and Jon Telling (Newcastle University, UK) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 12-21 September 2023

Measurable H2 can be generated during active seismicity through the reaction of water with freshly created rock surfaces. Field measurements have shown that rock-water reactions during seismic events can also lead to significant changes in the pH and increase the concentration of H2O2 in geological fluids. Whilst prior studies have investigated locations representing felsic crust, a large proportion of the deep biosphere resides in basaltic terrains. H2O2 generated through rock-water reactions is greater in basaltic rocks and enhanced when temperatures exceed ~80 °C. Importantly, these elevated temperatures overlap the growth ranges of some hyperthermophilic microorganisms. The generation of H2O2 in these environments represents an understudied energetic window of opportunity for extant microbial life, and possibly for the origins of life on Earth.

This project sampled a seismically active hydrothermal area in Iceland where elevated temperatures were anticipated to lead to enhanced H2O2 generation from rock-water reactions.
The SeisChem team investigated the relationship between seismicity and the products of rock – water reactions in a geologically active hydrothermal system. The central objective of SeisChem was to bridge a knowledge gap between laboratory studies and field measurements by:

  • Sample fluid and gas in time series, recording in-situ H2O2 and ancillary geochemical data
  • Store and return samples to the laboratory for H2 (g) and major ion (aq) analyses
  • Compare and contrast field and laboratory data with local seismic activity.

Read the full scientific report with kind permission by John Edgar and Jon Telling.


22-EPN3-130: Biosignatures in Icelandic geothermal aerosols

22-EPN3-130: Biosignatures in Icelandic geothermal aerosols

Visit by Mark Fox-Powell and Ben Stephens (Open University, UK) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 23-31 August 2023

The aim of our project was to capture and study microscopic aerosols ejected from bubbling geothermal springs in Iceland, as an analogue for the formation of cryovolcanic plumes at icy moons such as Enceladus. This project built on a successful Europlanet-funded field campaign in 2022. Our objectives in 2023 were to (i) comprehensively map size-dependent aerosol fluxes with increasing distance and elevation from the springs; and (ii) to collect simultaneous samples for microbiological and elemental analyses at multiple downwind locations.

We focused our investigations on Olkelduhals hot springs, near Hverageroi, where a pool with circum-neutral pH supporting thick microbial streamers experiences constant moderate gas flux. Our data from 2022 showed that this spring is a prolific and constant source of aerosols. We found that downwind aerosol size distributions changed with distance and with elevation from the spring. Four complete aerosol sample sets were taken downwind of the spring; each requiring a full field day. A background (upwind) air sample was also taken. Comprehensive samples for geochemical and microbiological analyses were taken from the spring, along with the collection of volatile and semi-volatile organic compounds using thermal desorption tubes. The sample set will form the basis of a new PhD studentship, beginning in October 2023 at the Open University, which will investigate the chemical composition, biomass content and microbial diversity of aerosols, and the volatile profiles of geothermal gases. Our data will provide the first insights from natural analogues into the formation of aerosols within cryovolcanic plumes.


22-EPN3-116: Fault Scaling at Southwest Iceland

22-EPN3-116: Fault Scaling at Southwest Iceland

Visit by Işık Su Yazıcı (German Aerospace Center DLR, Germany) and Sebastian Sturm (University of Freiburg, Germany) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 02-10 August 2023

Fault population studies reveal the lithospheric stress and strength conditions. Geometric fault properties provide insights into mechanical and temporal evolution of fault systems, as well as past and future potential for seismic energy release. Understanding the displacement-length relationship of faults can also help to estimate the current seismicity level. Improved constraints on the current seismicity of Mars based on lnSight mission results, are the motivation for a renewed and detailed analysis of martian fault systems. Partly due to the limited number of reliable datasets, data on the relationships between fault displacement and length of extraterrestrial bodies are scarce. Using Digital Elevation Models (OEM) and corresponding orthoimages derived from High Resolution Stereo Camera (HRSC) data, we previously obtained information on the displacement distribution along faults and the maximum displacement (Dmax) at the Memnonia Fossae (MF) fault system on Mars.

The volcanic rifting zone in SW Iceland displays similar characteristics as MF. Specifically, the availability of airborne HRSC data (HRSC-AX) of an area characterized by widespread normal faults in the rift zone at Thingvellir, and well-exposed faults in Reykjanes, are exceptionally well-suited sites as analogues for the MF. Considering the scarcity of terrestrial analogue work complementing the analysis of planetary fault scaling, this field work helps to improve our understanding of fault scaling relationships: Our goal is to combine terrestrial remote sensing data (HRSC-AX) with ground truth to obtain a better basis for evaluating planetary fault scaling (which relies on remote sensing only).

Read the full scientific report with kind permission by Işık Su Yazıcı.

Examples of faults in SW Iceland.
Examples of faults in SW Iceland. Credit: Işık Su Yazıcı.

22-EPN3-061: Analogue Studies to Test the Scientific Potential of the First SERS Prototype Analysis

22-EPN3-061: Analogue Studies to Test the Scientific Potential of the First SERS Prototype Analysis

Marco Veneranda and Guillermo Lopez-Reyes (University of Valladolid, Spain) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 24-30 July 2023

Iceland provides access to a great variety of environments that are widely considered potential analogues of hydrothermal processes on Mars). Previous investigation revealed a wide variety of microbial communities proliferating at the water side of Krysuvik and Hveradalir hydrothermal systems. Although providing crucial information on the dynamics of extremophilic life, the lack of low altered mineralogical samples prevented from: 1) fully comprehend the hydrothermal weathering dynamics of the primary rock (extrusive Fe-rich basaltic lava), and 2) determine the relation between microbial proliferation and the degree of hydrothermal alteration of the hosting mineral substrate. 

As these two aspects are of key importance to understand the habitability potential of the ancient hydrothermal systems found on Mars, Marco Veneranda and Guillermo Lopez Reyes performed a new campaign of analysis to address these two topics. On one hand, the two researchers investigated the mineralogical composition of the two analogue sites by using a portable emulator of the RLS Raman spectrometer onboard the ESA/ExoMars rover. Afterwards, a novel device for the automated synthesis of SERS nanoemulsions was used to investigate the organic content of the hydrothermal waters. The obtained results were then used to select optimal geological and biological samples to be returned in the laboratory for further investigation. As a whole, this research project aims at supporting the RLS team in defining and optimizing the potential scientific outcome of the RLS instrument once it will be operated on the surface of Mars.

Read the full scientific report with kind permission by Marco Veneranda and Guillermo Lopez-Reyes.

Molecular analysis performed in-situ by using a portable Raman spectrometer at the hydrothermal areas of Krýsuvik and Hveradalir.
Molecular analysis performed in-situ by using a portable Raman spectrometer at the hydrothermal areas of Krýsuvik and Hveradalir. Credit: M Veneranda.

22-EPN3-011: Phototrophic Microorganisms in Cold Deserts of Iceland

22-EPN3-011: Phototrophic Microorganisms in Cold Deserts of Iceland – Ecology and Diversity of Potential Analogues

Visit by Daniel Remias (University of Salzburg, Austria) and Lenka Procházková (Charles University, Czech Republic) to TA1 – Iceland Field Sites, MATIS
Dates of visit: 07-13 July 2023

Geology and climate of inland regions at Iceland are ideal prerequisites for exploring microbial adaptation to cold and dry habitats. Bare terrestrial ground surfaces and high­altitude melting snowfields represent niches at the edge of life on Earth. Soil samples were harvested at altitudes from almost at sea level up to more than 1000 m. Additionally, red snow caused by cryoflora (snow algae) from permanent snow packs in the Kerlingarfjoll Mountains were collected, and photosynthetic uptake rates were measured in situ with labelled carbon (13C). Red snow was transported to the lab and the pigments extracted and the UV-protecting pigments characterized by HPLC.

The main aim of the project was the molecular characterisation of the phototrophic microbial community for evaluation of abundance and diversity of terrestrial and frozen habitats. Barren, desert­like sites were compared with vegetated ones. Microalgae marker DNA were extracted with dedicated kits for environmental soil samples.

This study aims to shed light on how photoautotrophic microbial life could work at Earth analogues with similar or even worse climatical or soil conditions. Finally, Icelandic terrestrial microalgae will be tested as potential analogues compared to other worlds like Mars or icy moons.

Read the full scientific report with kind permission by Daniel Remias and Lenka Procházková.

Image credit: Desert-like sampling site close to Sandfell Mt. Credit: D Remias.


1st  Europlanet Planetary Science Workshop in Bolivia 2024

1st  Europlanet Planetary Science  Workshop in Bolivia 2024

This workshop will be held during 4 days at the Institute for Geological and Environmental Research (Instituto de Investigaciones Geologicas y del Medio Ambiente UMSA) in La Paz, Bolivia. The purpose of the workshop is to provide tools for the processing and mapping of planetary surfaces, exploring different planets and analogous environments in Bolivia and Latin America.

Registration is now open!

Deadline for registrations is Friday 12 January.

Expert Exchanges – Call Now Open

Europlanet Expert Exchanges – Call Now Open

A new call has been launched for the Expert Exchange Programme, funded through Europlanet 2024 Research Infrastructure (RI), which aims to share expertise and best practice within the planetary community, and to prepare new facilities and services for integration into the RI.

Applications should be made before the next call deadline of 17 January 2024. Visits through this call should take place between 1 February and 15 May 2024.

The programme provides funding for short visits (up to one week).

Objectives for an Europlanet Expert Exchange might be:

  • To improve infrastructure facilities and services offered to the scientific community by Europlanet 2024 RI laboratories or institutes.
  • To provide training on theoretical or practical aspects of the laboratory/fieldwork required to plan a future TA application.
  • To foster cooperation between academia and industry (SMEs).
  • To support early career professionals to develop skills to use or manage RI facilities or services.
  • To widen participation from Under-Represented States in RI activities and services.
  • To support the inclusion of amateur communities in European planetary science campaigns.
  • To support engagement with wider society e.g. through the involvement of outreach providers, educators, journalists, artists etc.

For more details, see the Expert Exchange Call Page.

Join the 2024 GMAP Geology and Planetary Mapping Winter School!

Join the 2024 GMAP Geology and Planetary Mapping Winter School!

The GMAP Geology and Planetary Mapping Winter School is an exciting opportunity to delve into planetary geological mapping with guidance from experienced scientists. The Winter School is led by GMAP, Europlanet’s geological mapping activity.

Building upon earlier editions targeting Mars, the Moon, and Mercury, the 2024 Winter School will cover exemplary geologic mapping aspects on VenusIcy Satellites and Small Bodies.

The Winter School will be largely hands-on, with the inclusion of seminars and time for asynchronous interaction and individual/project mapping work. Topics covered include: Basemap resources, QGIS project creation, and practical experience of map crafting.

The school will run synchronously in the week 22-26 January 2024, and asynchronously on the Streavent platform for the following month (February 2024). As usual, materials will be freely available after the school, for interested parties, to learn individually at their own pace.

Each body of interest will be introduced, hands-on activities will be described, and participants will be guided through the task, i.e. individual completion of a small mapping area. At the end of each day, specific time slots are dedicated to seminars, which will provide insights, perspectives and additional knowledge on related topics.

After the synchronous and asynchronous phases of the School, no dedicated support will be provided, but any interested party is welcome to participate to the monthly GMAP calls, as well as to join the GMAP Discord server for discussion and support.

Find out more

Supporting UK and Hungarian Industry Collaborations

Supporting UK and Hungarian Industry Collaborations

Two overarching objectives of Europlanet are to foster industry-academic collaboration and to widen participation from under-represented states in Europe and around the world. Last week, there were opportunities to support both these aims at the UK Space Conference in Belfast and an event at the Hungarian Embassy in London.

At the UK Space Conference from 21-23 November, Europlanet shared a stand with the Hungarian Space Cluster (Hunspace). Over the course of the meeting, we met with many members of the UK and international community, in particular with early career researchers. We were particularly delighted to meet and take part in discussion sessions with the space clusters that represent the different space communities across the UK. Plenary sessions featured discussions on exploration of our Solar Sytem and the technical challenges involved.

On Friday 24 November, we were privileged to be hosted by the Hungarian Embassy in London for a meeting of the UK and Hungarian Space Communities. We were welcomed by Orsolya Ferencz, Ministerial Commissioner  Hungarian  Ministry of Foreign Affairs, and by the Hungarian Ambassador to London, Ferenc Kumin. Nigel Mason (Europlanet 2024 RI Coordinator) and Zsolt Fulop (Chair of the research infrastructure committee in Hungary) kicked off proceedings. Tomas Barzy (Admatis) gave an overview of the Hunspace cluster’s membership, remit and history. Presentations by Hungarian and UK space industry and organisations were followed by a round-table discussion. Many thanks to Gábor Takács-Carvalho and all the team at the Hungarian Embassy for their hospitality.

Full reports on both events will be published soon.

22-EPN3-060: A new apparatus for measuring the electrical charge of volcanic ash particles

22-EPN3-060: A new apparatus for measuring the electrical charge of volcanic ash particles

Visit by Allan Fries, University of Geneva (Switzerland), to TA2.4 Planetary Environment Facilities (PEF), AU (Denmark)
Dates of visit: 02-11 August 2023

Report summary: The electrical charge carried by volcanic ash particles is known to play a crucial role in the formation of aggregates, which modulate the atmospheric transport and deposition rate of volcanic ash. However, direct field measurements of these charges remain rare, and more investigations are required to better comprehend both charge generation and aggregation mechanisms. This study aimed at building and testing a portable device to quantify the charge of individual volcanic ash particles and aggregates using a Through-Type Faraday Cage (TTFC) connected to a charge amplifier circuit capable of detecting the very small voltages induced by charged particles entering the TTFC.

After building the apparatus, 187 tests were performed, using different quantities and types of particles, as well as varying the measurement technique. First results show that the newly built device is capable of measuring charges down to 0.1 pC and that measurements agree well with alternative estimations obtained by directly integrating the current generated in the TTFC over time.

Beside the charge, results also suggest that the device can be used to obtain the particle settling velocity, based on the duration of the voltage signal. Few additionnal tests are now required to detect smaller particles (i.e., smaller charges) and the instrument will then be used for field analysis and laboratory experiments.

Read the full scientific report, with kind permission from Allan Fries.


Machine Learning for a new era of data-driven planetary science

The Europlanet 2024 Research Infrastructure (RI) project looks at the many ways Machine Learning (ML) is revolutionising planetary science. The advent of Machine Learning (ML) has enabled a new approach, known as data-driven science. Using the wealth of datasets and streams available, ML can explore the data to find a pattern or commonality. Out of these initial steps comes a hypothesis that can be tested through data analysis, which, again, hopefully leads to a new understanding. Clustering or fusing datasets, moreover, can reveal connections that are not recognisable in the individual datasets.

The Europlanet 2024 Research Infrastructure is a €10m project, funded by the European Commission’s Horizon 2020 programme, that supports the planetary science community. The project’s core activities are to provide access to facilities, field sites, and data services.

However, Europlanet also provides investment through ‘Joint Research Activities’ that combine the expertise of multiple partners to create the new infrastructure and services needed to carry out world-leading planetary research. Since 2020, the project has developed ML tools to handle complex planetary science data more efficiently and provide opportunities to combine and visualise multiple diverse datasets. This programme has been further enhanced through a collaboration with a second Horizon 2020 project, EXPLORE, which is developing applications for the exploitation of galactic, stellar and lunar data, and provides a platform for deploying and testing ML tools and services.

Further, Europlanet’s ML-powered tools are based on scientific cases proposed by the community that address key challenges in planetary research. From these proposals, seven cases were chosen to follow up initially during the project, and further cases have been added over time. All the tools are open-source, ready-to-use, and highly customisable, enabling other researchers to freely deploy and adapt them for their own research scenarios.

Lastly, it should be noted that, by developing ML tools tailored to data-driven planetary science, Europlanet has cemented collaborations, started to build new user communities and developed services that are already resulting in publications. While the planetary science community could be seen as late to the party in adopting ML, interest is now high. This couldn’t be more timely – with flagship missions to Mercury and Jupiter soon adding to the deluge of data streams, the era of data-driven science is only just beginning.

Europlanet 2024 RI and EXPLORE have received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreements No. 871149 and No. 101004214, respectively.

Please follow the link here to read to entire article.

22-EPN3-061: CO2 Ice Crystals Formation Under Conditions in the Martian Polar Regions

22-EPN3-061: CO2 Ice Crystals Formation Under Conditions in the Martian Polar Regions: Influence of Substrate Properties and Temperature Gradient

Visit by Ganna Portyankina, DLR (Germany), to TA2.4 Planetary Environment Facilities (PEF), AU (Denmark)
Dates of visit: 30 April – 01 October 2023 (two visits)

Report summary: The main goal of most recent tests conducted at the Planetary Environment Facilities at Aarhus University was to condense CO2 from the chamber’s atmosphere under Martian conditions onto a specially designed set of different surface materials (martian regolith simulant, glass beads of various sizes, dust). We investigated ranges of temperatures and pressures and observed the texture of the created CO2 ice. Our goal was to determine if CO2 deposits over regolith/glass beads/dust differently compared to brushed aluminium. We have observed that various properties of substrate did not considerably alter the deposition morphologies of CO2 observed in our previous work. Most importantly, we find that under conditions usual for Martian polar areas in fall and winter, CO2 ice always deposits as a translucent slab.  Under deviating conditions, i.e. colder temperatures and lower pressures, CO2crystals assume different shapes including opaque slab and highly porous multi-crystalline. Such CO2crystalline morphologies require further investigations, because of their relevance to icy satellite surfaces as well as CO2 cloud formation.

Read the full scientific report, with kind permission from Ganna Portyankina.


1st Europlanet Latin America Planetary Science Workshop

1st Europlanet Latin America Planetary Science Workshop: Connecting Earth with Other Planets

The next event in the Europlanet Workshop Series will be the 1st Europlanet Latin America Planetary Science Workshop, which will take place from 31 October-03 November 2023 at the University of Buenos Aires, Argentina. The workshop will be held in the hybrid mode.

Who is for?

Post-graduated students, researchers, early career and professionals interested in planetary science, planetary surface and astrobiology.

Programme

The programme for the workshop can be found here.

Fee

The workshop is free of charge but places are limited!

Registration

Registration opens on 01/08/2023 and closes on 27/09/2023. It is compulsory and must be accompanied by a letter of interest and a brief curriculum vitae (max 1 page). You will receive via email confirmation of your acceptance. Participation in the workshop includes all coffee and lunch breaks.

Number of participants

35 people will be admitted in-person and up to 100 online.

Language

English or Spanish

Deliverables

Attendees (both in-person and online) will be issued, on request, with a certificate of attendance. The materials of topics presented at the 1st Latin America Planetary Science Workshop – Connecting Earth with other Planets will be available.

More about the Europlanet Workshop Series

More about Europlanet Global Collaboration and Integration Development

Issue 5 of the Europlanet Magazine is out now!

Issue 5 of the Europlanet Magazine is out now!

In this issue:

Cover of the Europlanet Magazine Issue 5
Cover of the Europlanet Magazine Issue 5

In Focus

round up of news from Europlanet and the planetary community, including

ESA’s JUICE Mission – Making History on its Way to Jupiter

Athena Coustenis (CNRS/Observatoire de Paris, Meudon, France), member of the JUICE Science Working Team and Co-I of the JANUS camera, describes the emotional journey to the launchpad and beyond for Europe’s new mission to explore the icy moons of Jupiter

Planetary Perspectives – A Planetary Scientist Turned Asteroid Miner

This edition’s ‘Planetary Perspectives’ interview with Dr Lauri Siltala has been contributed by J D Prasanna Deshapriya, Hans Huybrighs, Peter McArdle, and Ottaviano Rüsch of the Europlanet Early Career (EPEC) Future Research Working Group. It is the latest in a series of conversations by EPEC, ‘Industry or Academia?’, which aim to gather insights from people who have had success in both sectors. 

Policy Engagement on the Menu 

Members of the Europlanet Policy and Industry Team and Executive Board reflect on recent activities by Europlanet to engage with policy makers

A Guide to Live-Streaming Astronomy Events 

Claudia Mignone (INAF), Anne Buckle and Graham Jones (timeanddate.com) and Helen Usher (Open University) share tips for a new era of astronomy live-streaming

Developing Labs for Research that is Out of this World

Gareth Davies (Vrije Universiteit Amsterdam, Netherlands) describes how investment from the European Commission has supported Europlanet’s development of state-of-the-art facilities for planetary science – and other fields of research, such as cultural heritage.

Life Beyond Us: Showcasing Astrobiology through Science Fiction Stories 

Julie Nováková (European Astrobiology Institute, Czech Republic), co-editor of the ‘Life Beyond Us’ anthology, describes this new collection of 27 science fiction stories by award-winning authors and 27 essays by scientists. 

AbGradEPEC 2023 

After a three-year wait to hold the AbGradEPEC meeting for early career astrobiologists, former AbGradE President, Ruth-Sophie Taubner, and current President, Silvana Pinna, share highlights of the event. 

Fourth Fireball Forum

Günter Kargl and Manuel Scherf (Space Research Institute, Austrian Academy of Sciences) describe the outcomes of a series of workshops on fireball detection organised through the Europlanet 2024 Research Infrastructure (RI) project. 

SPIDER

The SPIDER Space Weather Service supports studies of BepiColombo flybys at Venus and Mercury.

CommKit

Thibaut Roger (Europlanet Communications Team/Universität Bern) explores the use of games and play-related formats for research and science communication. 

The Last Word
Nigel Mason (President, Europlanet Society) reflects on efforts to build a more collaborative European space science community.

Europlanet Summer School 2023 is Underway

Europlanet Summer School 2023 is Underway

The Europlanet Summer School 2023 is being hosted by Vilnius University’s Moletai Astronomical Observatory (MAO) in Lithuania from 8-18 August.

For the first time, the School is taking place in hybrid format, with 20 participants from 10 countries attending on site and up to 30 people following online. The participants include early careers (right the way from high-school to BSc, MSc, PhD and postdoc) and amateur astronomers.

During the School, participants will gain hands-on experience observing with MAO’s 1.65m and 35/51cm-telescopes (weather permitting!) and training in analysing exoplanet transits, stellar spectra, atmospheric parameters and variability data. The programme includes training modules in communication skills and engaging with schools, as well as lectures on space and ground-based observations and machine learning.

Deividas Dudulis (high-school student and astrophotographer), who is participating in the Summer School, will be posting photos here.

Investigating Venus via Volcanic Iceland

Investigating Venus via Volcanic Iceland

Solmaz Adeli and Nils Müller are travelling to Iceland this summer to carry out two research projects in support of upcoming missions to Venus.  Their visit, from 31 July – 14 August, is partly funded through Europlanet’s Transnational Access programme and the trip is part of a larger, international campaign organised by NASA‘s Jet Propulsion Laboratory (JPL) and the German Aerospace Centre, DLR.

Volcanic field sites in Iceland can be used as planetary analogues for Venus, since their resemblance to terrains and environments on Venus enable a better understanding of the processes that shape the venusian surface, and also provide an opportunity to test out instrumentation.

Iceland's Fagradalsfjall volcano
Iceland’s Fagradalsfjall volcano erupting in 2021. Credit: CC BY-SA 4.0 Mokslo Sriuba
3-D perspective view of Sapas Mons on Venus, with lava flows in the foreground. Credit: NASA/JPL

Solmaz, of the DLR Institute of Planetary Research, is leading a project that uses field sites on Iceland to help characterise the composition and origin of the major geologic terrains on the venusian surface, one of the main objectives of the NASA VERITAS and ESA EnVision missions. Her team will use a prototype of the VEM instrument, which will fly on-board VERITAS, to characterise lava flows in the Reykjanes peninsula, which range from very fresh terrains to areas that have been altered over time. “Very fresh” in this case even means that, by coincidence, the team will be able to measure hot lava that is currently erupting from the active Fagradalsfjall volcano since 10 July this year. The red-glowing lava rocks of the Litli-Hrútur eruption cone have about the same temperature as the surface of Venus, which is a 470 degree Celsius hothouse day and night. The team will also collect samples and take them back to the PSL laboratories at DLR-Berlin for analysis in the Venus emissivity chamber

This project will increase our understanding of the spectral emissivity data that will be obtained by the VERITAS and EnVision missions, and be an opportunity to calibrate field data taken by the prototype VEM instrument

Nils, a postoc at the Freie Universität Berlin, is leading a project to better understand volcanic activity on Venus by investigating the infrared signal of active eruptions and searching for new lava flows. The Dyngjusandur sand sheet (a cold sand desert) and the fissure-fed lava flows, Holuhraun and Thorvaldshraun, are excellent analogues on Iceland to prepare for these studies because these recent lava flows at the sites are sufficiently large and intense to be detectable on Venus.

An issue that complicates the quantitative study of volcanic activity on Venus is the unexpectedly low reflected radar signal from Venusian lava flows, which suggests that detection of active  flows may be difficult because they might quickly form uninterrupted crusts, obscuring the hot lava. It is, however, possible that wind-bourne sediments are partly responsible for these low radar reflections. The Iceland volcanic sites are very well-suited to study how sediments modify the radar signal of lava flows, so the study may give new insights into radar data collected at Venus.

The team aims to acquire airborne radar data, similar to the VERITAS radar data, and carry out field work simultaneously with the flight campaign. This ‘ground-truth’ data will include information on sediment coverage and humidity, which will help to interpret and add value to the radar data.

Uli Koehler, from the DLR Institute of Planetary Research, will be travelling with the expedition team and reporting on the campaign. For updates on their progress, see the DLR blog and follow the social media channels of DLR:

Image: CC BY-SA 4.0 Mokslo Sriuba

21-EPN-FT1-012: Zebra dolomites revised

21-EPN-FT1-012: Zebra dolomites revised: clumped isotope analysis as a tool to assess recrystallisation and dolomite cementation in overpressured settings

Visit by Swennen Rudy, KU Leuven (Belgium), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 22-26 May 2023.

Report Summary: Zebra dolomites are marked by an alternation of millimeter thick dark colored, as recrystallised interpreted bands and white cement bands. Disruption of the banding is manifested by displacements that gradually increases and subsequently deceases before disappearing. This disruption also occurs at intracrystalline scale with crystal rehealing features as observable under cathodoluminescence. This disruption of the zebra dolomites is explained by dolomitization in relation to overpressured fluid flow.  

In the framework of the Europlanet project zebra dolomite samples from 3 deep Belgian boreholes (Soumagne, Soiron and Bolland) were selected for clumped isotope analysis.  The aim was to sample and analyse the dark fine crystalline and white coarse dolomite cements separately to infer the original (re)crystallization temperature.  The following research questions were raised: i) is there a systematic difference in deduced temperature between the dark and white dolomite bands.  If so then this could help to better constrain the recrystallisation and cementation.  This would allow to assess the potential resetting of the original clumped isotope signature of the dark bands due to recrystallisation; ii) if the cement phases display uniform temperatures then this temperature can be compared with the minimum crystallization temperature deduced from primary fluid inclusion microthermometry [1]. The discrepancy between both temperatures, which links to the pressure correction, normally allows to quantify the overpressure of the system; iii) based on deduced crystallization temperature and δ18OPDB, the δ18OSMOW of the fluid can be assessed, allowing to constrain the origin of the dolomitizing fluids, certainly when combined with Sr isotope analysis.