Matches in SemOpenAlex for { <https://semopenalex.org/work/W4206476803> ?p ?o ?g. }
Showing items 1 to 80 of
80
with 100 items per page.
- W4206476803 abstract "<p>Through numerical modeling, Nesvorny et al. (2008) showed that asteroids can migrate due to Yarkovsky drift and resonances to outside of the boundaries of the Vesta family. In particular, they found that objects which end up in the scattered resonances region (so-called Cell I, defined by orbital elements 2.2 AU < a < 2.3 AU, 0.05 < e < 0.2, 0 < i deg < 10 deg) typically have retrograde rotations and thermal parameters that maximize Yarkovsky drift rates. These autors also showed, that asteroids migrating to the low inclination region (Cell II defined by 2.32 AU < a < 2.48 AU, 0.05 < e < 0.2, 2 deg < i < 6 deg) should be predominantly prograde rotators.</p> <p>We performe photometric observations and determine spins and shapes of V-type objects in Cell I and Cell II in order to characterize the dynamical properties of these asteroids more accurately. The results of dynamical modelling show that some asteroids may have migrated to their current location from the Vesta family within ~2 Gy. There are objects, however, whose origin in another parent body may also be plausible. This may support the hypothesis that the number of differentiated basaltic objects in the inner and middle Main Belt should be much higher than previously assumed. We will present preliminary results for the first ~10 asteroids in Cell I and Cell II.</p>" @default.
- W4206476803 created "2022-01-25" @default.
- W4206476803 creator A5000221671 @default.
- W4206476803 creator A5001383991 @default.
- W4206476803 creator A5003545794 @default.
- W4206476803 creator A5011855204 @default.
- W4206476803 creator A5021052882 @default.
- W4206476803 creator A5021129086 @default.
- W4206476803 creator A5031990929 @default.
- W4206476803 creator A5044236061 @default.
- W4206476803 creator A5047920062 @default.
- W4206476803 creator A5049066796 @default.
- W4206476803 creator A5051909942 @default.
- W4206476803 creator A5057149885 @default.
- W4206476803 creator A5058461055 @default.
- W4206476803 creator A5061781693 @default.
- W4206476803 creator A5065959955 @default.
- W4206476803 creator A5067002435 @default.
- W4206476803 creator A5072342531 @default.
- W4206476803 creator A5076153800 @default.
- W4206476803 creator A5076441851 @default.
- W4206476803 creator A5085646687 @default.
- W4206476803 date "2021-07-21" @default.
- W4206476803 modified "2023-10-06" @default.
- W4206476803 title "Shape models and dynamical properties of basaltic asteroids outside the dynamical Vesta family" @default.
- W4206476803 doi "https://doi.org/10.5194/epsc2021-217" @default.
- W4206476803 hasPublicationYear "2021" @default.
- W4206476803 type Work @default.
- W4206476803 citedByCount "0" @default.
- W4206476803 crossrefType "posted-content" @default.
- W4206476803 hasAuthorship W4206476803A5000221671 @default.
- W4206476803 hasAuthorship W4206476803A5001383991 @default.
- W4206476803 hasAuthorship W4206476803A5003545794 @default.
- W4206476803 hasAuthorship W4206476803A5011855204 @default.
- W4206476803 hasAuthorship W4206476803A5021052882 @default.
- W4206476803 hasAuthorship W4206476803A5021129086 @default.
- W4206476803 hasAuthorship W4206476803A5031990929 @default.
- W4206476803 hasAuthorship W4206476803A5044236061 @default.
- W4206476803 hasAuthorship W4206476803A5047920062 @default.
- W4206476803 hasAuthorship W4206476803A5049066796 @default.
- W4206476803 hasAuthorship W4206476803A5051909942 @default.
- W4206476803 hasAuthorship W4206476803A5057149885 @default.
- W4206476803 hasAuthorship W4206476803A5058461055 @default.
- W4206476803 hasAuthorship W4206476803A5061781693 @default.
- W4206476803 hasAuthorship W4206476803A5065959955 @default.
- W4206476803 hasAuthorship W4206476803A5067002435 @default.
- W4206476803 hasAuthorship W4206476803A5072342531 @default.
- W4206476803 hasAuthorship W4206476803A5076153800 @default.
- W4206476803 hasAuthorship W4206476803A5076441851 @default.
- W4206476803 hasAuthorship W4206476803A5085646687 @default.
- W4206476803 hasConcept C121332964 @default.
- W4206476803 hasConcept C1276947 @default.
- W4206476803 hasConcept C26873012 @default.
- W4206476803 hasConcept C2778870898 @default.
- W4206476803 hasConcept C2779700264 @default.
- W4206476803 hasConcept C44870925 @default.
- W4206476803 hasConcept C58142911 @default.
- W4206476803 hasConceptScore W4206476803C121332964 @default.
- W4206476803 hasConceptScore W4206476803C1276947 @default.
- W4206476803 hasConceptScore W4206476803C26873012 @default.
- W4206476803 hasConceptScore W4206476803C2778870898 @default.
- W4206476803 hasConceptScore W4206476803C2779700264 @default.
- W4206476803 hasConceptScore W4206476803C44870925 @default.
- W4206476803 hasConceptScore W4206476803C58142911 @default.
- W4206476803 hasLocation W42064768031 @default.
- W4206476803 hasOpenAccess W4206476803 @default.
- W4206476803 hasPrimaryLocation W42064768031 @default.
- W4206476803 hasRelatedWork W1488639739 @default.
- W4206476803 hasRelatedWork W1649066097 @default.
- W4206476803 hasRelatedWork W2010133960 @default.
- W4206476803 hasRelatedWork W2010201075 @default.
- W4206476803 hasRelatedWork W2050942819 @default.
- W4206476803 hasRelatedWork W3103114574 @default.
- W4206476803 hasRelatedWork W3117068793 @default.
- W4206476803 hasRelatedWork W3145073591 @default.
- W4206476803 hasRelatedWork W4287546530 @default.
- W4206476803 hasRelatedWork W4294945464 @default.
- W4206476803 isParatext "false" @default.
- W4206476803 isRetracted "false" @default.
- W4206476803 workType "article" @default.