Evidence for asteroid space weathering from the Sloan Digital Sky Survey

By D. Nesvorný, Robert Jedicke, R. Whiteley, Željko Ivezic´. 2005

230 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology

View Paper: https://www.semanticscholar.org/paper/bcb5bb7199afbc4db3c1cb190193596f1393b3b3

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Citations in the corpus

Yarkovsky/YORP chronology of asteroid families (2006, methodology): “This information is interesting within the context of our work, because Jedicke et al. (2004) and Nesvorný et al. (2005) related these mean values to the age of a family as an expression of the degree of space weathering.”
Asteroid family ages (2015, methodology): “In the literature we found only (Nesvorný et al., 2005) giving a consistent, but low accuracy, 2± 1 Gy.”
Size-frequency distributions of fragments from SPH/N-body simulations of asteroid impacts: Comparison with observed asteroid families (2007, background): “Observed SFDs of main-belt asteroid families (Nesvorný et al., 2005), plotted to the same scale as the modeled SFDs in Fig.”
LSST: From Science Drivers to Reference Design and Anticipated Data Products (2008, methodology): “26) and size; size distributions of asteroid families (Parker et al. 2008) and their correlations with age (Jedicke et al. 2004; Nesvorný et al. 2005); dynamical effects (Bottke et al. 2001); and studies of object shapes and spin states using light curve inversion techniques (Pravec & Harris 2000;…”
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, methodology): “We choose not to use a? defined by Ivezić et al. (2002) or the first Principal Component (PC1) defined by Nesvorný et al. (2005) used in other works. a? is the first principal component of the r’-i’ versus g’-r’ colors and PC1 is the first principal component of the measured fluxes of all five…”
The fossilized size distribution of the main asteroid belt (2003, methodology): “Note that this method has bee successfully used to identify the 5.8 Myr old Karin clu ter and many other main belt families(Nesvorný et al., 2002c, 2003, 2005; Nesvorný and Bottke, 2004).”
Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) (2019, methodology): “s depicted in Fig. 16. Boundary limits shown for the orbits of the terrestrial planets in Fig. 16c may illuminate the role that tidal resurfacing plays as a consequence of close planetary encounters (Nesvorný et al. 2005, 2010; Binzel et al., 2010). It is important to note these boundaries are not e”
Space weathering and the interpretation of asteroid reflectance spectra (2010, methodology): “Spectral slope (reddening and color index) has been used as a space weathering index (e.g., Hiroi and Sasaki, 2001; Jedicke et al., 2004; Marchi et al., 2005, 2006; Nesvorný et al., 2005; Lazzarin et al., 2006; Brunetto et al., 2006a; Fevig and Fink, 2007; Paolicchi et al., 2007; Moretti et al., 200”
Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion (2005, background): “These families have members that are too large to be dispersed by the Yarkovsky effect or ground away by comminution over several Gyr (Nesvorný and Bottke, 2004; Nesvorný et al., 2005).”
The Size Distributions of Asteroid Families in the SDSS Moving Object Catalog 4 (2008, methodology): “puzzled why a similar color-aided search by Nesvorný et al. (2005)”
NEAR-INFRARED SPECTROSCOPY OF TROJAN ASTEROIDS: EVIDENCE FOR TWO COMPOSITIONAL GROUPS (2008, background): “It is not clear, however, exactly how this process would be expressed on a primitive asteroid surface (e.g., Nesvorný et al. 2005; Lagerkvist et al. 2005; Lazzarin et al. 2006).”
The Compositional Structure of the Asteroid Belt (2015, background): “About 100,000 asteroids have measurements that tell us about their surface compositions (Ivezic et al., 2001, Szabo et al., 2004, Nesvorny et al., 2005, Carvano et al., 2010), providing a broader view of the Asteroid Belt than ever before.”
Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, background): “Dedicated studies based on spectroscopic observations showed both reddening [Lazzarin et al., 2006; Fornasier et al., 2016; Kaluna et al., 2016] and blueing [Nesvorný et al., 2005; Lantz et al., 2013] effects on spectral slopes.”