Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Namitha Rose Baby"'
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 9, p 162 (2023)
The stratigraphy of the largest natural satellite of our solar system, Ganymede, is investigated using available global mosaic (basemap) and high-resolution images. We are focusing on the reconstruction of the formation and tectonic evolution of sele
Externí odkaz:
https://doaj.org/article/2d22e267c9ab4219abdcf3b47493237c
Polygonal impact craters (PIC) are impact craters that have at least one straight rim segment in planform [1-8]. Among all impact craters, PICs represent a small percentage. They exist on both rocky and icy planetary bodies [9]. To our knowledge no s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::69e3e9f184c3ab0f787af7b359fa7a5d
https://doi.org/10.5194/egusphere-egu23-354
https://doi.org/10.5194/egusphere-egu23-354
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:
Namitha Rose Baby, Katrin Stephan, Roland Wagner, Thomas Kenkmann, Geoffrey Collins, Ernst Hauber, Ralf Jaumann
Introduction The formation of Ganymede’s light terrain and its possible interaction with a subsurface ocean, have made its investigation one of the top goals of the upcoming JUICE mission [1, 2]. In this study we present a detailed stratigraphic an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45798ab343d6edba06d25ef4278eabfc
https://doi.org/10.5194/epsc2022-1016
https://doi.org/10.5194/epsc2022-1016
Two major terrain units dominate Ganymede’s surface: 1) the ancient heavily cratered dark terrain and 2) the tectonically resurfaced bright or light terrain (Collins et al., 2013). Previous studies suggest that the dark material is a relatively thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c110cc43184ea9c3f0335dc24da2db63
https://doi.org/10.5194/epsc2021-589
https://doi.org/10.5194/epsc2021-589
The Jovian satellite Ganymede experienced a pronounced period of tectonic resurfacing forming the extended bright or light terrain the so-called Sulci, which cover about 2/3 of Ganymede’s surface (Pappalardo et al., 2004 and references therein). It
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b726a268fb48203282051e7b638ef917
https://doi.org/10.5194/epsc2021-352
https://doi.org/10.5194/epsc2021-352