Some things special about NEAs: Geometric and environmental effects on the optical signatures of hydration

• Published in: Icarus (New York, N.Y. 1962) Vol. 333; pp. 415 - 428
• Main Authors: Potin, S., Beck, P., Schmitt, B., Moynier, F.
• Format: Journal Article
• Language: English
• Published: Elsevier Inc 15.11.2019; Elsevier
• Subjects: Astrophysics; Earth and Planetary Astrophysics; Sciences of the Universe; Reflectance spectra measurements; Mukundpura CM2 chondrite; carbonaceous chondrite
• ISSN: 0019-1035; 1090-2643
• DOI: 10.1016/j.icarus.2019.06.026

Here were report on a laboratory study aiming to reproduce specificities of near-Earth Asteroid. We study how the elevated surface temperature, their surface roughness (rock or regolith), as well as observation geometry can affect the absorption features detected on asteroids. For that purpose, we selected a recent carbonaceous chondrite fall, the Mukundpura CM2 chondrite which fell in India in June 2017. Bidirectional reflectance spectroscopy was performed to analyze the effect of the geometrical configuration (incidence, emergence and azimuth angle) on the measurement. Our results show that reflectance spectra obtained under warm environment (NEA-like) tends to show shallower absorption bands compared to low-temperature conditions (MBA-like), but still detectable in our experiments under laboratory timescales. Irreversible alteration of the sample because of the warm environment (from room temperature to 250 °C) has been detected as an increase of the spectral slope and a decrease of the band depths (at 0.7 μm, 0.9 μm and 2.7 μm). Comparing the meteoritic chip and the powdered sample, we found that surface texture strongly affects the shape of the reflectance spectra of meteorites and thus of asteroids, where a dust-covered surface presents deeper absorption features. We found that all spectral parameters, such as the reflectance value, spectral slope and possible absorption bands are affected by the geometry of measurement. We observed the disappearance of the 0.7 μm absorption feature at phase angle larger than 120°, but the 3 μm band remains detectable on all measured spectra. •Reflectance spectroscopy of surfaces strongly depends on the viewing geometry.•Slope, absorption bands and photometry are affected by the geometry.•Warm meteorites present shallower absorption bands than in cold environment.•Irreversible alteration of the spectra are met at high temperature.•Dust-covered samples present deeper absorption bands than raw surface.