Portrait of the Polana–Eulalia family complex: Surface homogeneity revealed from near-infrared spectroscopy

Portrait of the Polana–Eulalia family complex: Surface homogeneity revealed from near-infrared... •Comprehensive collection of NIR spectra of asteroids in the Polana/Eulalia families. •The 63 spectra are red with an average slope of S′ = 0.68 ± 0.68 %/1000 Å. •NIR spectroscopy cannot be used to separate members of these families or the background. •Spectroscopy of (495) Eulalia covering a whole rotation suggests surface homogeneity. •(495) Eulalia is red (S′= 0.91 ± 0.60 %/1000 Å) similar to the deMeo C-complex. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Icarus Elsevier

Portrait of the Polana–Eulalia family complex: Surface homogeneity revealed from near-infrared spectroscopy

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Publisher
Elsevier
Copyright
Copyright © 2016 Elsevier Inc.
ISSN
0019-1035
eISSN
1090-2643
D.O.I.
10.1016/j.icarus.2016.03.022
Publisher site
See Article on Publisher Site

Abstract

•Comprehensive collection of NIR spectra of asteroids in the Polana/Eulalia families. •The 63 spectra are red with an average slope of S′ = 0.68 ± 0.68 %/1000 Å. •NIR spectroscopy cannot be used to separate members of these families or the background. •Spectroscopy of (495) Eulalia covering a whole rotation suggests surface homogeneity. •(495) Eulalia is red (S′= 0.91 ± 0.60 %/1000 Å) similar to the deMeo C-complex.

Journal

IcarusElsevier

Published: Aug 1, 2016

References

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