Zobrazeno 1 - 10
of 102
pro vyhledávání: '"Ana-Catalina Plesa"'
Autor:
Fabian Klenner, Mickael Baqué, Kristina Beblo-Vranesevic, Janine Bönigk, Marc S. Boxberg, Bernd Dachwald, Ilya Digel, Andreas Elsaesser, Clemens Espe, Oliver Funke, Ernst Hauber, Dirk Heinen, Florence Hofmann, Lucía Hortal Sánchez, Nozair Khawaja, Maryse Napoleoni, Ana-Catalina Plesa, Frank Postberg, Autun Purser, Tina Rückriemen-Bez, Susanne Schröder, Dirk Schulze-Makuch, Stephan Ulamec, Jean-Pierre Paul de Vera
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Icy bodies with subsurface oceans are a prime target for astrobiology investigations, with an increasing number of scientists participating in the planning, development, and realization of space missions to these worlds. Within Germany, the Ocean Wor
Externí odkaz:
https://doaj.org/article/a4dcc670ff044b54b53e2757f3279be7
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 11, Pp n/a-n/a (2023)
Abstract The composition of basaltic melts in equilibrium with the mantle can be determined for several Martian meteorites and in‐situ rover analyses. We use the melting model MAGMARS to reproduce these primary melts and estimate the bulk compositi
Externí odkaz:
https://doaj.org/article/d6c497ebc7884773b52365ad6bfe3fa1
Autor:
Chi Yan, Ankit Barik, Sabine Stanley, Jason S.-Y. Leung, Anna Mittelholz, Catherine L. Johnson, Ana-Catalina Plesa, Attilio Rivoldini
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 1, p 11 (2023)
Magnetic field observations from the MGS, MAVEN, and InSight missions reveal that a dynamo was active in Mars’s early history. One unique feature of Mars’s magnetic crustal field is its hemispheric dichotomy, where magnetic fields in the southern
Externí odkaz:
https://doaj.org/article/f4762010f0fb412aa9e0512b60f7e7e3
Publikováno v:
Nature Communications, Vol 8, Iss 1, Pp 1-10 (2017)
Mantle partial melting produced the volcanic crust of Mercury. Here, the authors numerically model the formation of post-impact melt sheets and find that mantle convection was weak at around 3.7–3.8 Ga and that the melt sheets of Caloris and Rembra
Externí odkaz:
https://doaj.org/article/e27fd91a775f48b69b28f3fc0362253d
The astrobiological potential of the Jovian moon Europa has long been acknowledged [1]. Europa’s surface, icy shell, likely salty ocean, and silicate mantle play a key role in determining Europa’s habitability. In particular, the icy shell may ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9fe585315159836da526397943cfe799
https://doi.org/10.5194/egusphere-egu23-6803
https://doi.org/10.5194/egusphere-egu23-6803
The dense atmosphere of Venus and the planet’s young surface, dominated by volcanic features, bear witness to its past and potentially ongoing volcanic activity. While unique among the terrestrial planets of our Solar System, Venus is likely simila
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d787065430dad451514fcbc0909ba7bb
https://doi.org/10.5194/egusphere-egu23-8996
https://doi.org/10.5194/egusphere-egu23-8996
Autor:
Iris van Zelst, Julia Maia, Moritz Spühler, Ana-Catalina Plesa, Raphaël F. Garcia, Richard Ghail, Anna J. P. Gülcher, Anna Horleston, Taichi Kawamura, Sara Klaasen, Philippe Lognonné, Csilla Orgel, Mark Panning, Leah Sabbeth, Krystyna Smolinksi
With the selection of multiple missions to Venus by NASA and ESA planned to launch in the coming decade, we will greatly improve our understanding of Venus as a planet. However, the selected missions cannot tell us anything about the seismicity on Ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e35e1e7b136b52d134ae952933bcf3b
https://doi.org/10.5194/egusphere-egu23-9086
https://doi.org/10.5194/egusphere-egu23-9086
Autor:
Brigitte Knapmeyer-Endrun, Jiaqi Li, Doyeon Kim, Ana-Catalina Plesa, Scott McLennan, Ernst Hauber, Rakshit Joshi, Jing Shi, Caroline Beghein, Mark Wieczorek, Mark P. Panning, Philippe Lognonne, W. Bruce Banerdt
Analysis of data from the seismometer SEIS on NASA’s InSight mission has by now provided a wealth of information on the crustal structure of Mars, both beneath the lander and at other locations on the planet. Here, we collect the P- and S-wave velo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cff160a8bacf3f18ffd8ed4d8662fea6
https://doi.org/10.5194/egusphere-egu23-15069
https://doi.org/10.5194/egusphere-egu23-15069
Autor:
Doyeon Kim, Simon Stähler, Christian Boehm, Ved Lekic, Domenico Giardini, Savas Ceylan, John Clinton, Paul Davis, Cecilia Duran, Amir Khan, Brigitte Knapmeyer-Endrun, Ross Maguire, Mark Panning, Ana-Catalina Plesa, Nicholas Schmerr, Mark Wieczorek, Géraldine Zenhäusern, Philippe Lognonné, William Banerdt
After more than 4 Earth years of operation on the martian surface monitoring the planet’s ground vibrations, the InSight’s seismometer is now retired. Throughout the mission, analyses of body waves from marsquakes and impacts have led to importan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f7448d6530ba60c3e02f3857c9b27e6
https://doi.org/10.5194/egusphere-egu23-12524
https://doi.org/10.5194/egusphere-egu23-12524
There is a growing consensus that Venus is seismically active, although its level of seismicity could be very different from that of Earth due to the lack of plate tectonics. Here, we estimate upper and lower bounds on the expected annual seismicity
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::051f3bcccf223c9d1e85b8e95df4607e
https://doi.org/10.31223/x5dq0c
https://doi.org/10.31223/x5dq0c