Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders
The reflectance of a particulate surface depends on the phase angle at which it is observed. This is true for laboratory measurements on powders of natural materials as well as remote observations of Solar System surfaces. Here, we measured the dependences of reflectance spectra with phase angles, o...
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ftdatacite:10.48550/arxiv.2009.10496 2023-05-15T18:30:06+02:00 Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders Beck, Pierre Schmitt, Bernard Potin, Sandra Pommerol, Antoine Brissaud, Olivier 2020 https://dx.doi.org/10.48550/arxiv.2009.10496 https://arxiv.org/abs/2009.10496 unknown arXiv https://dx.doi.org/10.1016/j.icarus.2020.114066 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Earth and Planetary Astrophysics astro-ph.EP FOS Physical sciences article-journal Article ScholarlyArticle Text 2020 ftdatacite https://doi.org/10.48550/arxiv.2009.10496 https://doi.org/10.1016/j.icarus.2020.114066 2022-03-10T15:11:07Z The reflectance of a particulate surface depends on the phase angle at which it is observed. This is true for laboratory measurements on powders of natural materials as well as remote observations of Solar System surfaces. Here, we measured the dependences of reflectance spectra with phase angles, of a suite of 72 meteorites in the 400-2600 nm range. The 10-30° phase angle range is investigated in order to study the contribution of Shadow Hiding Opposition Effect to the phase behavior. The behavior is then extrapolated to phase angle of 0° using a polynomial fit, in order to provide grounds for comparison across meteorite groups (enabling to remove the contribution of shadows to reflectance) as well as to provide equivalent albedo values that should be comparable to geometric albedo values derived for small bodies. We find a general behavior of increasing strength of the SHOE with lower reflectance values (whether between samples or for a given samples with absorption features). This trend provides a first order way to correct any reflectance spectra of meteorite powders measured under standard conditions (g=30) from the contribution of shadows. The g=0 degre calculated reflectance and equivalent albedos are then compared to typical values of albedos for main-belt asteroids. This reveals that among carbonaceous chondrites only Tagish Lake group, CI, and CM chondrites have equivalent albedo compatible with C- and D-type asteroids. On the other hand equivalent albedo derived with CO, CR and CK chondrites are compatible with L- and K-type asteroids. The equivalent albedo derived for ordinary chondrites is related to petrographic types, with low-grade petrographic type (type 3.6 and less) being generally darker that higher petrographic types. This works provides a framework for further understanding of the asteroids meteorite linkage when combining with colors and spectroscopy. Article in Journal/Newspaper Tagish DataCite Metadata Store (German National Library of Science and Technology) Tagish ENVELOPE(-134.272,-134.272,60.313,60.313) Tagish Lake ENVELOPE(-134.233,-134.233,59.717,59.717) |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Earth and Planetary Astrophysics astro-ph.EP FOS Physical sciences |
spellingShingle |
Earth and Planetary Astrophysics astro-ph.EP FOS Physical sciences Beck, Pierre Schmitt, Bernard Potin, Sandra Pommerol, Antoine Brissaud, Olivier Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
topic_facet |
Earth and Planetary Astrophysics astro-ph.EP FOS Physical sciences |
description |
The reflectance of a particulate surface depends on the phase angle at which it is observed. This is true for laboratory measurements on powders of natural materials as well as remote observations of Solar System surfaces. Here, we measured the dependences of reflectance spectra with phase angles, of a suite of 72 meteorites in the 400-2600 nm range. The 10-30° phase angle range is investigated in order to study the contribution of Shadow Hiding Opposition Effect to the phase behavior. The behavior is then extrapolated to phase angle of 0° using a polynomial fit, in order to provide grounds for comparison across meteorite groups (enabling to remove the contribution of shadows to reflectance) as well as to provide equivalent albedo values that should be comparable to geometric albedo values derived for small bodies. We find a general behavior of increasing strength of the SHOE with lower reflectance values (whether between samples or for a given samples with absorption features). This trend provides a first order way to correct any reflectance spectra of meteorite powders measured under standard conditions (g=30) from the contribution of shadows. The g=0 degre calculated reflectance and equivalent albedos are then compared to typical values of albedos for main-belt asteroids. This reveals that among carbonaceous chondrites only Tagish Lake group, CI, and CM chondrites have equivalent albedo compatible with C- and D-type asteroids. On the other hand equivalent albedo derived with CO, CR and CK chondrites are compatible with L- and K-type asteroids. The equivalent albedo derived for ordinary chondrites is related to petrographic types, with low-grade petrographic type (type 3.6 and less) being generally darker that higher petrographic types. This works provides a framework for further understanding of the asteroids meteorite linkage when combining with colors and spectroscopy. |
format |
Article in Journal/Newspaper |
author |
Beck, Pierre Schmitt, Bernard Potin, Sandra Pommerol, Antoine Brissaud, Olivier |
author_facet |
Beck, Pierre Schmitt, Bernard Potin, Sandra Pommerol, Antoine Brissaud, Olivier |
author_sort |
Beck, Pierre |
title |
Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
title_short |
Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
title_full |
Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
title_fullStr |
Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
title_full_unstemmed |
Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
title_sort |
low-phase spectral reflectance and equivalent geometric albedo of meteorites powders |
publisher |
arXiv |
publishDate |
2020 |
url |
https://dx.doi.org/10.48550/arxiv.2009.10496 https://arxiv.org/abs/2009.10496 |
long_lat |
ENVELOPE(-134.272,-134.272,60.313,60.313) ENVELOPE(-134.233,-134.233,59.717,59.717) |
geographic |
Tagish Tagish Lake |
geographic_facet |
Tagish Tagish Lake |
genre |
Tagish |
genre_facet |
Tagish |
op_relation |
https://dx.doi.org/10.1016/j.icarus.2020.114066 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.2009.10496 https://doi.org/10.1016/j.icarus.2020.114066 |
_version_ |
1766213586422595584 |