Zobrazeno 1 - 10
of 30
pro vyhledávání: '"G. J. Consolmagno"'
Autor:
Turrini, D., Combe, J. -P., McCord, T. B., Oklay, N., Vincent, J. -B, Prettyman, T. H., McSween, H. Y., SJ, G. J. Consolmagno, De Sanctis, M. C., Corre, L. Le, Longobardo, A., Palomba, E., Russell, C. T.
The Dawn spacecraft observed the presence of dark material, which in turn proved to be associated with OH and H-rich material, on the surface of Vesta. The source of this dark material has been identified with the low albedo asteroids, but it is stil
Externí odkaz:
http://arxiv.org/abs/1401.6152
Publikováno v:
Meteoritics & Planetary Science. 54:2729-2743
We have developed the first database of asteroid regolith properties: fifty asteroids so far, to aid space resource utilisation workers. The physical parameters: grain density, grain size, near surface bulk density and porosity are provided of a coll
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::60bf29860aea1b25a4dabc8262e13251
https://doi.org/10.5194/epsc2020-939
https://doi.org/10.5194/epsc2020-939
Publikováno v:
Meteoritics & Planetary Science. 55
Publikováno v:
Geochemistry. 78:269-298
The physical properties of the stone meteorites provide important clues to understanding the formation and physical evolution of material in the Solar protoplanetary disk as well providing indications of the properties of their asteroidal parent bodi
Publikováno v:
Icarus. 280:328-339
The survival of asteroid Vesta during the violent early history of the Solar System is a pivotal constraint on theories of planetary formation. Particularly important from this perspective is the amount of olivine excavated from the vestan mantle by
Publikováno v:
Turrini, D.; Svetsov, V.; Consolmagno, G.; Sirono, S.; Jutzi, Martin (2018). The late accretion and erosion of Vesta’s crust recorded by eucrites and diogenites as an astrochemical window into the formation of Jupiter and the early evolution of the Solar System. Icarus, 311, pp. 224-241. Elsevier 10.1016/j.icarus.2018.04.004
For decades the limited thickness of Vesta's basaltic crust, revealed by the link between the asteroid and the howardite-eucrite-diogenite family of meteorites, and its survival to collisional erosion offered an important constraint for the study of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18371db97347a30b7fcfe1844a442638
Autor:
Ellen S. Howell, Daniel T. Britt, M. W. Schaefer, G. J. Consolmagno, Robert J. Macke, Michael C. Nolan, Bradley E. Schaefer
Publikováno v:
Planetary and Space Science. 87:146-156
Meteorite heat capacity (specific heat) is an essential parameter in modeling many aspects of the orbital and internal evolution of small solar system bodies, and can be a tool for characterization of the material in a meteorite itself. We have devis
Publikováno v:
Meteoritics & Planetary Science. 47:319-329
– In our ongoing survey of meteorite physical properties, we have to date measured the thermal conductivity for seventeen stony meteorites at temperatures ranging from 5 K to 300 K. Here, we report new results for nine ordinary chondrites, one enst
Publikováno v:
Meteoritics & Planetary Science. 46:311-326
– As part of a large-scale survey of meteorite bulk and grain densities, porosities, and magnetic susceptibilities, we measured these properties for 174 stones from 106 achondritic meteorites. These include four lunar meteorites, 15 stones from 10