Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Zoe A. Landsman"'
Autor:
Stephanie G. Jarmak, Tracy M. Becker, Charles E. Woodward, Casey I. Honniball, Andrew S. Rivkin, Margaret M. McAdam, Zoe A. Landsman, Saverio Cambioni, Thomas G. Müller, Driss Takir, Kurt D. Retherford, Anicia Arredondo, Linda T. Elkins-Tanton
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 8, p 183 (2024)
Our understanding of solar system evolution is closely tied to interpretations of asteroid composition, particularly the M-class asteroids. These asteroids were initially thought to be the exposed cores of differentiated planetesimals, a hypothesis b
Externí odkaz:
https://doaj.org/article/26d1958e853a422d896c3071ddd03a57
Publikováno v:
Advances in Space Research. 71:5400-5412
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd5438b0dd11e0f3dd5600cc904cb60b
https://doi.org/10.1016/j.asr.2023.02.034
https://doi.org/10.1016/j.asr.2023.02.034
Autor:
Philip T. Metzger, Cody D. Schultz, Zoe A. Landsman, Makayla Peppin, Ryan L. Kobrick, Daniel T. Britt, Nina Orlovskaya
Publikováno v:
Advances in Space Research. 67:3308-3327
The Martian moon Phobos is the target of the upcoming JAXA Martian Moons eXploration (MMX) mission. There are currently no known samples of Phobos, so spacecraft hardware testing and scientific studies require Phobos regolith simulants. Here, we pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::86a0cc3fca3314b8a3dc32e70f40f6e9
https://doi.org/10.1016/j.asr.2021.01.024
https://doi.org/10.1016/j.asr.2021.01.024
Autor:
Daniela Lazzaro, D. Morate, J. de León, J. L. Rizos, Noemi Pinilla-Alonso, V. Lorenzi, H. Medeiros, Zoe A. Landsman, Marcel Popescu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:3866-3875
The main objective of this work is to compositionally analyse the visible to near-infrared spectra of a total of six V-type candidates identified using the MOVIS (Y-J) versus (J-Ks) colour–colour plot and located outside the Vesta collisional famil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::17775ed01d70d336519328af9dff52bb
https://doi.org/10.1093/mnras/stz2001
https://doi.org/10.1093/mnras/stz2001
Autor:
Philip T. Metzger, Yuxue Sun, Zoe A. Landsman, M. Peppin, Christian Sipe, C. D. Schultz, K. M. Cannon, Daniel T. Britt
Publikováno v:
Earth and Space 2021.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9c95b161f57906e3dafbb4eeec7f6b7b
https://doi.org/10.1061/9780784483374.018
https://doi.org/10.1061/9780784483374.018
Autor:
Daniel T. Britt, Zoe A. Landsman
The Exolith Lab at The University of Central Florida’s Center for Lunar and Asteroid Surface Science (CLASS) produces high-mineralogical fidelity asteroid and planetary regolith simulants (several are pictured in Figure 1). Regolith simulants are u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72ae212b323e7f8e724a0d0807d07c28
https://doi.org/10.5194/epsc2020-906
https://doi.org/10.5194/epsc2020-906
Autor:
Joshua P. Emery, Humberto Campins, Zoe A. Landsman, Dale P. Cruikshank, Josef Hanus, Lucy F. Lim
Publikováno v:
Icarus. 304:58-73
Asteroid (16) Psyche is a unique, metal-rich object belonging to the “M” taxonomic class. It may be a remnant protoplanet that has been stripped of most silicates by a hit-and-run collision. Because Psyche offers insight into the planetary format
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f9def30c3d83bf7f8a10ff48ed0c079f
https://doi.org/10.1016/j.icarus.2017.11.035
https://doi.org/10.1016/j.icarus.2017.11.035
Autor:
Vania Lorenzi, Humberto Campins, Zoe A. Landsman, Javier Licandro, Marco Delbo, V. Alí-Lagoa, Michael P. Lucas, Brian Burt, Francesca E. DeMeo, Kevin J. Walsh, J. de León, Noemi Pinilla-Alonso
Publikováno v:
Icarus. 274:231-248
The inner asteroid belt is an important source of near-Earth asteroids (NEAs). Dynamical studies of the inner asteroid belt have identified several families overlapping in proper orbital elements, including the Polana and Eulalia families that contai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1a33016f8776bcf37fb72fdda1555d5
https://doi.org/10.1016/j.icarus.2016.03.022
https://doi.org/10.1016/j.icarus.2016.03.022
Autor:
Zoe A. Landsman, Javier Licandro, Humberto Campins, Julie Ziffer PhD, Dale P. Cruikshank, Mário De Prá
Publikováno v:
Icarus. 269:62-74
Spectroscopic investigations of primitive asteroid families constrain family evolution and composition and conditions in the solar nebula, and reveal information about past and present distributions of volatiles in the solar system. Visible and near-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12f02afbe3c74c0991fac899c3f77ca9
https://doi.org/10.1016/j.icarus.2016.01.008
https://doi.org/10.1016/j.icarus.2016.01.008
Autor:
Vania Lorenzi, V. Alí-Lagoa, Zoe A. Landsman, Alberto Cellino, P. Bendjoya, Francesca E. DeMeo, J. Gayon-Markt, Javier Licandro, David Morate, Marco Delbo, Kevin J. Walsh, Humberto Campins, J. de León, Antonio Cabrera-Lavers, Paolo Tanga, Noemi Pinilla-Alonso
Publikováno v:
Icarus. 266:57-75
The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three collisional families of primitive asteroids (Erigone, Clarissa, and Sulamitis), and a low-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7dfded418d2abeca31a9d332c276f9ae
https://doi.org/10.1016/j.icarus.2015.11.014
https://doi.org/10.1016/j.icarus.2015.11.014