Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Sean S. Lindsay"'
Autor:
Vishnu Reddy, Cristina A. Thomas, Sean S. Lindsay, Eric M. MacLennan, Noemi Pinilla-Alonso, Richard Cartwright, Michael P. Lucas, Juan A. Sanchez, Joshua P. Emery, V. Lorenzi
Publikováno v:
Icarus. 322:227-250
Spectral observations of asteroid family members provide valuable information regarding parent body interiors, the origin and source regions of near-Earth asteroids, and the link between meteorites and their parent bodies. Asteroids of the Hungaria f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fe149ee5768f31dad2d412f6f89726de
https://doi.org/10.1016/j.icarus.2018.12.010
https://doi.org/10.1016/j.icarus.2018.12.010
Autor:
Lucas T. McClure, Sean S. Lindsay
Publikováno v:
Icarus. 379:114944
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f2a5b1c032209a092260f9f1d4b15c9c
https://doi.org/10.1016/j.icarus.2022.114944
https://doi.org/10.1016/j.icarus.2022.114944
Autor:
Lucas T. McClure, Sean S. Lindsay
Publikováno v:
Icarus. 379:114907
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40b1a0721c06292ed575c2b51354ae38
https://doi.org/10.1016/j.icarus.2022.114907
https://doi.org/10.1016/j.icarus.2022.114907
Autor:
Marcell Tessenyi, Neil Bowles, Giorgio Savini, Sean S. Lindsay, Billy Edwards, Giovanna Tinetti, C. Arena
Twinkle is an upcoming 0.45-m space-based telescope equipped with a visible and two near-infrared spectrometers covering the spectral range 0.4 to 4.5 μm with a resolving power R ∼ 250 (λ 2.42 μm). We explore Twinkle’s capabilities for small b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bda096c1b52e000feb03ac2c0def2afa
https://ora.ox.ac.uk/objects/uuid:b2669fe2-e372-46be-a191-0eb168fd1ce4
https://ora.ox.ac.uk/objects/uuid:b2669fe2-e372-46be-a191-0eb168fd1ce4
Autor:
Vishnu Reddy, Sean S. Lindsay, Cristina A. Thomas, Juan A. Sanchez, Adriana M. Mitchell, N. A. H. Frere
The surface composition of S-type asteroids can be determined using band parameters extracted from their near-infrared (NIR) spectra (0.7-2.50 $\mu$m) along with spectral calibrations derived from laboratory samples. In the past, these empirical equa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82aaa43c18b581b771b552d814cc3f7e
Publikováno v:
Icarus. 291:268-287
The Hungaria asteroids remain as survivors of late giant planet migration that destabilized a now extinct inner portion of the primordial asteroid belt and left in its wake the current resonance structure of the Main Belt. In this scenario, the Hunga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::610258346e8d9e85cd8f6c86afe061f3
https://doi.org/10.1016/j.icarus.2016.11.002
https://doi.org/10.1016/j.icarus.2016.11.002
Autor:
Marcell Tessenyi, Sean S. Lindsay, C. Arena, Neil Bowles, Billy Edwards, Giovanna Tinetti, Giorgio Savini
Remote-sensing observations of Solar System objects with a space telescope offer a key method of understanding celestial bodies and contributing to planetary formation and evolution theories. The capabilities of Twinkle, a space telescope in a low Ea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cd7424140783392f781ca6d7696eaf1
Publikováno v:
Meteoritics & Planetary Science. 51:806-817
Near-infrared reflectance spectra of S-type asteroids contain two absorptions at 1 and 2 μm (band I and II) that are diagnostic of mineralogy. A parameterization of these two bands is frequently employed to determine the mineralogy of S(IV) asteroid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::21e51a0b3a739cbfd5ab7bac0681fd9f
https://doi.org/10.1111/maps.12611
https://doi.org/10.1111/maps.12611
Publikováno v:
Icarus, 247, 0, pp. 53-70
Icarus, 247, 53-70
Icarus, 247, 53-70
We provide a taxonomic and compositional characterization of Multiple Asteroid Systems (MASs) located in the main belt (MB) using visible and near-infrared (0.45-2.5 um) spectral data of 42 MB MASs. The mineralogical analysis is applied to determine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3887da6d4a48bc88eb3bc6d95d924c9b
https://doi.org/10.1016/j.icarus.2014.08.040
https://doi.org/10.1016/j.icarus.2014.08.040
Potentially hazardous asteroids (PHAs) represent a unique opportunity for physical characterization during their close approaches to Earth. The proximity of these asteroids makes them accessible for sample-return and manned missions, but could also r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c7b907dc9f89eb0019d2863154ac8a56
http://arxiv.org/abs/1507.01008
http://arxiv.org/abs/1507.01008