Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Giovanna Serventi"'
Autor:
Cristian Carli, Sabrina Ferrari, Alessandro Maturilli, Giovanna Serventi, Maria Sgavetti, Arianna Secchiari, Alessandra Montanini, Jörn Helbert
Publikováno v:
Minerals, Vol 14, Iss 1, p 62 (2024)
Exploration of Mercury will continue in the near future with ESA/JAXA’s BepiColombo mission, which will increase the number and the type of datasets, and it will take advantage of the results from NASA’s MESSENGER (MErcury Surface, Space ENvirome
Externí odkaz:
https://doaj.org/article/3662e4646e6446d18716b49638bc9904
Publikováno v:
Minerals, Vol 13, Iss 6, p 764 (2023)
The presence of minerals formed under the occurrence of liquid water during the first billion years on Mars was a key discovery, but there is still a large number of open issues that make the study of these mineral deposits a main focus of remote sen
Externí odkaz:
https://doaj.org/article/1376b1d8c2464d45be02d895f8d2b54b
Autor:
Nicolas Bott, Rosario Brunetto, Alain Doressoundiram, Cristian Carli, Fabrizio Capaccioni, Yves Langevin, Davide Perna, François Poulet, Giovanna Serventi, Maria Sgavetti, Francesco Vetere, Diego Perugini, Cristina Pauselli, Ferenc Borondics, Christophe Sandt
Publikováno v:
Minerals, Vol 13, Iss 2, p 250 (2023)
Mercury’s peculiar orbit around the Sun (3:2 spin–orbit resonance) and lack of atmosphere result in one the widest temperature ranges experienced at the surface of a planetary body in the solar system. Temperature variations affect the physical a
Externí odkaz:
https://doaj.org/article/666f4dad5b0847e2a10d6ca84a2129cc
Publikováno v:
Minerals; Volume 13; Issue 6; Pages: 764
The presence of minerals formed under the occurrence of liquid water during the first billion years on Mars was a key discovery, but there is still a large number of open issues that make the study of these mineral deposits a main focus of remote sen
Publikováno v:
Planetary and Space Science. 209:105361
Mars has a relatively tenuous atmosphere, the remote-sensed spectral data of the surface are affected by the presence of the atmosphere. In particular the water and CO2 absorption of the atmosphere are in the same spectral region as water, OH− and
Publikováno v:
Icarus. 272:1-15
Spectroscopic measurements were carried out at Inaf-IAPS Istituto Nazionale di Astrofisica, Roma. EMPA analyses have been performed at Dipartimento di Geoscienze, Padova. E4 end-member has been kindly provided by Dr. Sabrina Ferrari, Department of Ge
Autor:
Andrea Orlando, Maria Sgavetti, Daniele Borrini, Giovanna Serventi, Cristian Carli, Giovanni Pratesi
Publikováno v:
Publons
Plagioclase feldspars are rock-forming minerals which can be detected in the VNIR reflectance spectroscopy due to the presence of low amount of iron in their crystal lattice. Nevertheless the correlation between the spectral properties and the plagio
Autor:
Giovanna Serventi, Loredana Pompilio, Giuditta Tampella, C. Tellini, Fulvio Franchi, Maria Sgavetti, Giuseppe Pedrazzi, Cristian Carli
Publikováno v:
Icarus (N.Y.N.Y. 1962) 245 (2015): 184–197. doi:10.1016/j.icarus.2014.09.027
info:cnr-pdr/source/autori:Sgavetti, Maria; Serventi, Giovanna; Tampella, Giuditta; Pedrazzi, Giuseppe; Carli, Cristian; Pompilio, Loredana; Franchi, Fulvio; Tellini, Claudio/titolo:Spectral reflectance characteristics of the Hamar Laghdad hydrothermal sequence, Morocco: Implications for the methane origin on Mars/doi:10.1016%2Fj.icarus.2014.09.027/rivista:Icarus (N.Y.N.Y. 1962)/anno:2015/pagina_da:184/pagina_a:197/intervallo_pagine:184–197/volume:245
info:cnr-pdr/source/autori:Sgavetti, Maria; Serventi, Giovanna; Tampella, Giuditta; Pedrazzi, Giuseppe; Carli, Cristian; Pompilio, Loredana; Franchi, Fulvio; Tellini, Claudio/titolo:Spectral reflectance characteristics of the Hamar Laghdad hydrothermal sequence, Morocco: Implications for the methane origin on Mars/doi:10.1016%2Fj.icarus.2014.09.027/rivista:Icarus (N.Y.N.Y. 1962)/anno:2015/pagina_da:184/pagina_a:197/intervallo_pagine:184–197/volume:245
We analyze and discuss reflectance spectra of carbonate rocks from the Hamar Laghdad area (Morocco), where evidences of interactions with hydrothermal, and, in some cases, methane enriched fluids derived from underlying volcanoclastic rocks, are repo
Autor:
Cristian Carli, Giovanna Serventi
The lunar surface consists of a regolith layer that covers the underlying bedrocks, and is generally char- acterized by particulates < 1 cm. Lunar soil is the fine fraction of the regolith, and is generally between 60 and 80 μm. Sizes < 10 μm, acco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13979995d87c1150e3dc2e5dfb4f9c6f
http://hdl.handle.net/20.500.12386/27418
http://hdl.handle.net/20.500.12386/27418
Publikováno v:
Geological Society, London, Special Publications. 401:139-158