Implications of temperature-dependent near-IR spectral properties of common minerals and meteorites for remote sensing of asteroids

J. L. Hinrichs, P. G. Lucey, M. S. Robinson, A. Meibom, A. N. Krot

Research output: Contribution to journalArticle

28 Scopus citations

Abstract

Remote sensing analysis of common mafic silicates on bodies like asteroid 433 Eros may be in error unless temperature effects are considered. In this paper, spectral sensitivity to temperature as a function of wavelength from 0.4 to 2.5 microns is quantified using new measurements of reflectance spectra of olivine and two ordinary chondrites. The new data were obtained at higher temperature resolution and with greater accuracy than previous measurements. We use a simple thermal model to show that the temperature difference between terrestrial ambient conditions and those prevailing on main belt asteroids, as well as the temperature variations expected on the surfaces of individual asteroids during observations by spacecraft, are large enough to cause easily detectable spectral differences. Therefore, interpretations of asteroid spectra using spectra of minerals and meteorites obtained at terrestrial ambient conditions are suspect.

Original languageEnglish (US)
Pages (from-to)1661-1664
Number of pages4
JournalGeophysical Research Letters
Volume26
Issue number12
DOIs
StatePublished - Jun 15 1999
Externally publishedYes

    Fingerprint

ASJC Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

Cite this