Zobrazeno 1 - 10
of 3 798
pro vyhledávání: '"G J Taylor"'
Publikováno v:
Journal of the Royal Asiatic Society of Great Britain and Ireland, 1897 Apr 01, 406-407.
Externí odkaz:
https://www.jstor.org/stable/25207863
Autor:
Bob Bermond
Publikováno v:
Clinical Psychology & Psychotherapy. 7:240-240
Autor:
David J. Stevenson
Publikováno v:
Science. 234:1016-1017
Autor:
G. J. Taylor, Briony Horgan, H. J. Melosh, Brandon C. Johnson, Timothy J. Bowling, J. Kendall, Paul G. Lucey
Publikováno v:
Geology. 45:1063-1066
Publikováno v:
Geochimica et Cosmochimica Acta. 134:275-288
The nakhlite group of martian meteorites found in the Antarctic contain varying abundances of both martian and terrestrial secondary alteration phases. The aim of this study was to use transmission electron microscopy (TEM) to compare martian and ter
Autor:
Sander Goossens, Paul G. Lucey, Erwan Mazarico, Y. Li, Frank G. Lemoine, Maria T. Zuber, Jeffrey C. Andrews-Hanna, Walter S. Kiefer, Colleen Milbury, James W. Head, G. J. Taylor, J. C. Jansen, Jason M. Soderblom
Publikováno v:
Icarus
Data from the Gravity Recovery and Interior Laboratory (GRAIL) mission have revealed that ∼98% of the power of the gravity signal of the Moon at high spherical harmonic degrees correlates with the topography. The remaining 2% of the signal, which c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9c8701ca22ebdd2118ba12502422d69
https://europepmc.org/articles/PMC7477950/
https://europepmc.org/articles/PMC7477950/
Publikováno v:
Earth and Planetary Science Letters. :84-92
Mars does not recycle crustal materials via plate tectonics. For this reason the magmatic water reservoir of the martian mantle has not been affected by surface processes, and the deuterium/hydrogen (D/H) ratio of this water should represent the orig
Autor:
Lydia J. Hallis, A. W. Needham, Kazuhide Nagashima, Gary R. Huss, G. J. Taylor, Ian A. Franchi, Monica M. Grady
Publikováno v:
Geochimica et Cosmochimica Acta. 97:105-119
Secondary alteration phases, such as carbonates, smectite clays and Fe-oxides, are found within the martian meteorites. If these meteorites were seen to fall, the assumption can be reasonably made that the secondary phases have a martian origin. Howe
Autor:
Lydia J. Hallis, G. J. Taylor
Publikováno v:
Meteoritics & Planetary Science. 46:1787-1803
– Petrological and geochemical analyses of Miller Range (MIL) 03346 indicate that this meteorite originated from the same augitic cumulate layer(s) as the nakhlite Martian meteorites, but underwent rapid cooling prior to complete crystallization. A
Publikováno v:
Earth and Planetary Science Letters. 308:107-114
The composition of Mercury's surface is poorly known, but the MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) mission has provided a wealth of new data from three flybys. In particular, MESSENGER Neutron Spectrometer (NS) ob