Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Nico Schmedemann"'
Autor:
Maximilian P. Reitze, Iris Weber, Andreas Morlok, Harald Hiesinger, Jan Hendrik Pasckert, Nico Schmedemann, Karin E. Bauch, Aleksandra N. Stojic, Jörn Helbert
Publikováno v:
Earth and Space Science, Vol 10, Iss 6, Pp n/a-n/a (2023)
Abstract The MErcury Radiometer and Thermal Infrared Spectrometer instrument onboard the BepiColombo spacecraft is designed to investigate Mercury’s surface in the mid‐infrared (mid‐IR). Based on MESSENGER data and modeling, Mercury is thought
Externí odkaz:
https://doaj.org/article/99d9bc26e9f442fba90d3093afede99c
Autor:
Jan Hendrik Pasckert, Nico Schmedemann, Andreas Nathues, Harald Hiesinger, Carolyn H. van der Bogert
Publikováno v:
Icarus
In this study we investigated the previously observed young resurfacing absolute model ages at the floor of Occator crater on dwarf planet Ceres on the basis of Dawn data. These young resurfacing absolute model ages have been interpreted to represent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f394f4a89f48d67136dfe56186716884
https://hdl.handle.net/21.11116/0000-000C-AADB-E
https://hdl.handle.net/21.11116/0000-000C-AADB-E
Autor:
Thomas Frueh, Harald Hiesinger, Carolyn H. van der Bogert, Jaclyn D. Clark, Thomas R Watters, Nico Schmedemann
The lithosphere of the Moon has been deformed by tectonic processes for at least 4 billion years, resulting in a variety of tectonic surface features. Extensional large lunar graben formed during an early phase of net thermal expansion before 3.6 Ga.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ff3355275fa2bfee74f8f17adbd324e
https://doi.org/10.1002/essoar.10513004.2
https://doi.org/10.1002/essoar.10513004.2
Introduction: The Multi-Temporal Database of Planetary Image Data (MUTED) is a comprehensive web-tool to identify and to access orbital images of Mars, Moon, and Mercury. The database is available at https:\\muted.wwu.de and provides various tools fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c0ee5d22093dfa2433a68353e720d120
https://doi.org/10.5194/epsc2022-428
https://doi.org/10.5194/epsc2022-428
Autor:
Stefan Wiedeking, Anja Lentz, Jan Hendrik Pasckert, Jan Raack, Nico Schmedemann, Harald Hiesinger
Publikováno v:
Icarus. 389:115267
Autor:
Namitha Rose Baby, Katrin Stephan, Roland Wagner, Thomas Kenkmann, Nico Schmedemann, Ernst Hauber
The formation of Ganymede’s light or bright tectonically resurfaced terrain and its possible interaction with a subsurface ocean has been made one of the top goals of the upcoming JUICE mission [1]. We therefore investigate the currently available
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::93260662526a3c7e2f965e89a7a8c698
https://doi.org/10.5194/egusphere-egu22-5168
https://doi.org/10.5194/egusphere-egu22-5168
Autor:
Aleksandra N. Stojic, Juulia-Gabrielle Moreau, Tomas Kohout, Antti Penttilä, Andreas Morlok, Iris Weber, Maximilian P. Reitze, Harald Hiesinger, Nico Schmedemann, Argo Joeleht, Karin E. Bauch, Jan-Hendrik Pasckert, Jörn Helbert
Introduction: Mercury’s surface is exposed to a multitude of surface altering effects that have a significant influence on its optical properties. Impact events – small or large, are one of the major surface-altering agents. Inferred from hypothe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1560858f991e0063202a980f4080067b
https://elib.dlr.de/191327/
https://elib.dlr.de/191327/
Autor:
Marine Desjardins, Ernst Hauber, Tilman Bucher, Matthias Geßner, Harald Hiesinger, Nico Schmedemann, Andreas Johnsson, Fabian Ellermann, Cynthia Sassenroth, Jörg Brauchle, Susan Conway, Axel Noblet
The mid-latitudes of Mars host a large amount of buried ice deposits [1], which bear a record on the very Late Amazonian climate evolution (~107 to 108 yr.) [2] and are a possible resource for future exploration [3]. The reconstruction of the history
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47603498452c045a7eeb57ca4b9f1ac9
https://doi.org/10.5194/epsc2022-1035
https://doi.org/10.5194/epsc2022-1035
Autor:
Andreas Morlok, Christian Renggli, Bernard Charlier, Olivier Namur, Stephan Klemme, Maximilian Reitze, Iris Weber, Aleksandra N. Stojic, Karin Bauch, Nico Schmedemann, Jan-Hendrik Pasckert, Harald Hiesinger, Jörn Helbert
Introduction: The IRIS (Infrared and Raman for Interplanetary Spectroscopy) laboratory generates mid-infrared spectra for the ESA/JAXA BepiColombo mission to Mercury. Onboard is a mid-infrared spectrometer (MERTIS-Mercury Radiometer and Thermal Infra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffb1cf25c26b3b00334fe4e41c71edc2
https://doi.org/10.5194/epsc2022-876
https://doi.org/10.5194/epsc2022-876
Autor:
Carol A. Raymond, Jian-Yang Li, C. M. Pieters, H. Hiesinger, Guneshwar Thangjam, Julie C. Castillo-Rogez, Andreas Nathues, Jan Hendrik Pasckert, Nico Schmedemann, Ottaviano Ruesch, Edward A. Cloutis, L. Le Corre, Kurt Mengel, Vishnu Reddy, Michael J. Hoffmann, David A. Williams
Publikováno v:
Nature Astronomy. 4:794-801
NASA’s Dawn mission revealed a partially differentiated Ceres that has experienced cryovolcanic activity throughout its history up to the recent past. The Occator impact crater, which formed ~22 Myr ago, displays bright deposits (faculae) across it