Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Timothy J. Bowling"'
Publikováno v:
Icarus. 329:207-221
Over the past thirty years, spacecraft missions, Earth-based radar experiments, and telescopic observations have revolutionized our knowledge of Main Belt asteroids, near-Earth asteroids, and comet nuclei. As a result of this effort, we now possess h
Publikováno v:
Journal of Geophysical Research: Planets. 124:941-957
Autor:
Carol A. Raymond, Paul M. Schenk, Christopher T. Russell, Debra Buczkowski, Timothy J. Bowling, David A. Williams, Jennifer E.C. Scully, Adrian Neesemann, Julie Castillo-Rogez
Publikováno v:
Icarus. 320:7-23
Occator crater is one of the most recognizable features on Ceres because of its interior bright regions, which are called the Cerealia Facula and Vinalia Faculae. Here we use high-resolution images from Dawn (∼35 m/pixel) to create a detailed geolo
Autor:
Thomas M. Davison, Timothy J. Bowling, Julie Castillo-Rogez, Jennifer E.C. Scully, Simone Marchi, Brandon C. Johnson, Fred J. Ciesla
Publikováno v:
Icarus. 320:110-118
Occator crater is perhaps the most distinct surface feature observed by NASA's Dawn spacecraft on the Cerean surface. Contained within the crater are the highest albedo features on the planet, Cerealia Facula and Vinalia Faculae, and relatively smoot
Autor:
Debra Buczkowski, Timothy J. Bowling, Andrea Longobardo, Carol A. Raymond, P. M. Schenk, Andreas Nathues, C. Bu, Ralf Jaumann, Andrea Raponi, Nathan Stein, Adrian Neesemann, Jennifer E.C. Scully, Ottaviano Ruesch, Julie Castillo-Rogez, Lynnae C. Quick, Ernesto Palomba, Christopher T. Russell, E. C. Thomas
Publikováno v:
Icarus. 320:213-225
The distinctive bright regions within Occator crater are one of the most remarkable discoveries of the Dawn mission's exploration of Ceres. The central region is named Cerealia Facula and the additional regions in the eastern crater floor are named V
Autor:
Britney E. Schmidt, Timothy J. Bowling, Maria Cristina De Sanctis, Julie Castillo-Rogez, Frank Preusker, Carol A. Raymond, P. M. Schenk, Christopher T. Russell, Jennifer E.C. Scully, Debra Buczkowski, Ryan S. Park, Lynnae C. Quick, Hanna G. Sizemore
Publikováno v:
Icarus. 320:159-187
The prominent bright deposit Cerealia Facula, Ceres, coincides with the central depression (or central pit) of the recently formed 92 km-wide complex crater Occator. The central pit is 9–10 km wide and up to 1 km deep and is partially filled with a
Autor:
Timothy J. Bowling, Julie Castillo-Rogez, Hannah Kaplan, Naoyuki Yamashita, Mauro Ciarniello, Eleonora Ammannito, Simone Marchi, Vassilissa Vinogradoff, Christopher T. Russell, Ernesto Palomba, Andrea Raponi, Thomas H. Prettyman, M. C. De Sanctis, Carol A. Raymond
Publikováno v:
Nature Astronomy
Nature Astronomy, 2019, 3 (2), pp.140-145. ⟨10.1038/s41550-018-0656-0⟩
Nature Astronomy, Nature Publishing Group, 2019, 3 (2), pp.140-145. ⟨10.1038/s41550-018-0656-0⟩
Nature Astronomy, 2019, 3 (2), pp.140-145. ⟨10.1038/s41550-018-0656-0⟩
Nature Astronomy, Nature Publishing Group, 2019, 3 (2), pp.140-145. ⟨10.1038/s41550-018-0656-0⟩
The surface mineralogy of dwarf planet Ceres appears to be dominated by products of rock–fluid interactions, such as phyllosilicates—some of which are NH4-bearing—and carbonates1–3. Elemental concentrations derived from the inferred mineral m
Autor:
Simone Marchi, Timothy J. Bowling, Michael T. Bland, Carol A. Raymond, David A. Williams, F. Preusker, Julie Castillo-Rogez, Anton I. Ermakov, Ryan S. Park, Roger R. Fu, Christopher T. Russell
Publikováno v:
Geophysical Research Letters. 45:1297-1304
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
Iron meteorites provide a record of the thermal evolution of their parent bodies, with cooling rates inferred from the structures observed in the Widmanstätten pattern. Traditional planetesimal thermal models suggest that meteorite samples derived f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b49e9e9a11894e5a5986a7dabe91eb4
http://hdl.handle.net/10044/1/70047
http://hdl.handle.net/10044/1/70047