Zobrazeno 1 - 10
of 41
pro vyhledávání: '"N A Sharkey"'
Autor:
Juan A. Sanchez, Vishnu Reddy, Audrey Thirouin, William F. Bottke, Theodore Kareta, Mario De Florio, Benjamin N. L. Sharkey, Adam Battle, David C. Cantillo, Neil Pearson
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 6, p 131 (2024)
The study of small (
Externí odkaz:
https://doaj.org/article/aa8087365a0d4940bf57bab4d6fb7d9b
Autor:
Benjamin N. L. Sharkey, Vishnu Reddy, Renu Malhotra, Audrey Thirouin, Olga Kuhn, Albert Conrad, Barry Rothberg, Juan A. Sanchez, David Thompson, Christian Veillet
Publikováno v:
Communications Earth & Environment, Vol 2, Iss 1, Pp 1-7 (2021)
The Earth’s most stable quasi-satellite, Kamoʻoalewa, displays an extremely red reflectance spectrum typical of space weathering of lunar-like silicate material which raises the possibility that it is formed of material originating from the Moon
Externí odkaz:
https://doaj.org/article/9dfc393c5a4e4f15944fe155380f22ca
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 11, p 223 (2023)
We collect near-infrared spectra (∼0.75–2.55 μ m) of four Jovian irregular satellites and visible spectra (∼0.32–1.00 μ m) of two Jovian irregular satellites, two Uranian irregular satellites, and four Neptune Trojans. We find close similar
Externí odkaz:
https://doaj.org/article/217e63aabc554fa984372a611edcd099
Autor:
David C. Cantillo, Vishnu Reddy, Adam Battle, Benjamin N. L. Sharkey, Neil C. Pearson, Tanner Campbell, Akash Satpathy, Mario De Florio, Roberto Furfaro, Juan Sanchez
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 9, p 177 (2023)
Carbonaceous chondrites are among the most important meteorite types and have played a vital role in deciphering the origin and evolution of our solar system. They have been linked to low-albedo C-type asteroids, but due to subdued absorption bands,
Externí odkaz:
https://doaj.org/article/8ab37fc351434db88f0099554a1e98e1
Autor:
Darryl Z. Seligman, Davide Farnocchia, Marco Micheli, David Vokrouhlický, Aster G. Taylor, Steven R. Chesley, Jennifer B. Bergner, Peter Vereš, Olivier R. Hainaut, Karen J. Meech, Maxime Devogele, Petr Pravec, Rob Matson, Sam Deen, David J. Tholen, Robert Weryk, Edgard G. Rivera-Valentín, Benjamin N. L. Sharkey
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 2, p 35 (2023)
We report statistically significant detections of nonradial, nongravitational accelerations based on astrometric data in the photometrically inactive objects 1998 KY _26 , 2005 VL _1 , 2016 NJ _33 , 2010 VL _65 , 2016 RH _120 , and 2010 RF _12 . The
Externí odkaz:
https://doaj.org/article/ba06458cd5d54af48e5e47af29efaa61
Autor:
Darryl Z. Seligman, Davide Farnocchia, Marco Micheli, David Vokrouhlický, Aster G. Taylor, Steven R. Chesley, Jennifer B. Bergner, Peter Vereš, Olivier R. Hainaut, Karen J. Meech, Maxime Devogele, Petr Pravec, Rob Matson, Sam Deen, David J. Tholen, Robert Weryk, Edgard G. Rivera-Valentín, Benjamin N. L. Sharkey
We report statistically significant detections of non-radial nongravitational accelerations based on astrometric data in the photometrically inactive objects 1998 KY$_{26}$, 2005 VL$_1$, 2016 NJ$_{33}$, 2010 VL$_{65}$, 2016 RH$_{120}$, and 2010 RF$_{
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0131bfd816a8e4b667300b02ddb44615
Autor:
Vishnu Reddy, William F. Bottke, David C. Cantillo, Adam Battle, Theodore Kareta, Benjamin N. L. Sharkey, Juan A. Sanchez, Neil Pearson
Metal-rich near-Earth asteroids (NEAs) represent a small fraction of the NEA population that is mostly dominated by S- and C-type asteroids. Because of this, their identification and study provide us with a unique opportunity to learn more about the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::560ac9637a120d557aef2ec8bb44d80f
http://arxiv.org/abs/2109.13950
http://arxiv.org/abs/2109.13950
Autor:
Richard J. Wainscoat, Rob Landis, Robert Weryk, Detlef Koschny, M. J. Brucker, Alessandra Springmann, Hong Kyu Moon, K. E. Fast, Jon D. Giorgini, Olivier Hainaut, Boris M. Shustov, Viqar Abbasi, Frank D. Ghigo, Michael S. P. Kelley, Donovan Mathias, Davide Farnocchia, Cassandra Lejoly, Lorien Wheeler, Paul W. Chodas, Theodore Kareta, Annika Gustafsson, Myung-Jin Kim, Robert S. McMillan, William Ryan, Martin A. Slade, Vishnu Reddy, James Bauer, Ravi Teja Nallapu, David Polishook, Jessie L. Dotson, James V. Scotti, John Noonan, Joseph S. Jao, Clement G. Lee, Haris Khan Niazi, Eileen V. Ryan, J. A. Larsen, Makoto Yoshikawa, T. A. Lister, Nicolas Erasmus, Michael W. Busch, Shantanu P. Naidu, Lindley S. Johnson, David G. Gilbank, Lawrence G. Snedeker, Young-Jun Choi, Rachel B. Fernandes, Walter M. Harris, Denis G. Laurin, Amber Bonsall, David Trilling, Alberto Quijano Vodniza, Benjamin N. L. Sharkey, Amanda A. Sickafoose, Lauren Schatz, Michael Mommert, Lance A. M. Benner, Marc A. Silva, Zarah Brown, Joseph R. Masiero, Marco Micheli, E. A. Kramer, Schelte J. Bus, David J. Tholen, Marina Brozovic, Cristina A. Thomas, John P. Faucher, Lindsay R. Slick, Nicholas Moskovitz
Publikováno v:
Icarus. 326:133-150
著者人数: 69名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 吉川, 真)
Number of authors: 69 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Yoshikaw
Number of authors: 69 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Yoshikaw
Autor:
Andrew S. Rivkin, Joshua P. Emery, Ellen S. Howell, Theodore Kareta, John W. Noonan, Matthew Richardson, Benjamin N. L. Sharkey, Amanda A. Sickafoose, Laura M. Woodney, Richard J. Cartwright, Sean Lindsay, Lucas T. Mcclure
Publikováno v:
The Planetary Science Journal. 3:153
We present evidence, via a large survey of 191 new spectra along with previously published spectra, of a divide in the 3 μm spectral properties of the low-albedo asteroid population. One group (“sharp types,” or STs, with band centers μm) has a
Nereid, Neptune's third largest satellite, lies in an irregular orbit and is the only outer satellite in the system (apart from Triton) that can be spectroscopically characterized with the current generation of Earth-based telescopes. We report our r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1881a0df9d3490daebaa5858cf74a6e
http://arxiv.org/abs/2106.12084
http://arxiv.org/abs/2106.12084