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Characterization of asteroid analogues by means of emission and reflectance spectroscopy in the 1- to 100-µm spectral range

Maturilli, Alessandro and Helbert, Jörn and Ferrari, Sabrina and Davidsson, B. and D’Amore, M. (2016) Characterization of asteroid analogues by means of emission and reflectance spectroscopy in the 1- to 100-µm spectral range. Earth, Planets and Space, 68 (1). Springer. DOI: 10.1186/s40623-016-0489-y ISSN 1343-8832

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Official URL: http://dx.doi.org/10.1186/s40623-016-0489-y

Abstract

The last decades have seen a large number of missions targeting small bodies in the solar system. NASA, ESA and JAXA sent missions to different solar system small bodies (SSSB), and the Japan mission Hayabusa returned samples from the surface of the S-type asteroid Itokawa. JAXA launched in 2014 a follow-up mission (Hayabusa2) to collect a sample from carbonaceous (C-type) asteroid 1999 JU3 asteroid and bring it back to Earth. The NASA’s OSIRIS-REx mission will launch in September 2016 to explore the carbonaceous asteroid Bennu. Despite an already existing rich collection of reflectance and emissivity spectral libraries for asteroid analogues, those are mostly based on measurements in air for a spectral range covering the visible to the medium infrared (approximately, from 0.4 to 25 µm). To characterize minerals, rocks and meteorites suitable for being surface analogues for asteroids and SSSB in general, spectroscopic measurements are needed for a wider spectral range and in vacuum, conditions that more closely resemble those found on asteroid surfaces. To fill this gap we acquired spectral measurements over a large spectral range (1–100 µm) for several meteorites and other analogues at the Planetary Emissivity Laboratory of the German Aerospace Center in Berlin. Those data provide more direct analogues for asteroid surfaces and expand our existing database of emissivity and reflectance measurements.

Item URL in elib:https://elib.dlr.de/109398/
Document Type:Article
Title:Characterization of asteroid analogues by means of emission and reflectance spectroscopy in the 1- to 100-µm spectral range
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Maturilli, AlessandroAlessandro.Maturilli (at) dlr.deUNSPECIFIED
Helbert, JörnJoern.Helbert (at) dlr.deUNSPECIFIED
Ferrari, Sabrinasabrina.ferrari (at) dlr.deUNSPECIFIED
Davidsson, B.department of physics and astronomy, uppsala university, box 516, 75120 uppsala, swedenUNSPECIFIED
D’Amore, M.mario.damore (at) dlr.deUNSPECIFIED
Date:13 June 2016
Journal or Publication Title:Earth, Planets and Space
Refereed publication:Yes
Open Access:Yes
Gold Open Access:Yes
In SCOPUS:Yes
In ISI Web of Science:No
Volume:68
DOI :10.1186/s40623-016-0489-y
Publisher:Springer
Series Name:Open
ISSN:1343-8832
Status:Published
Keywords:Asteroid analogue materials Emissivity measurements Reflectance measurements Infrared spectroscopy
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Project MASCOT (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Experimentelle Planetenphysik
Deposited By: Maturilli, Alessandro
Deposited On:15 Dec 2016 09:01
Last Modified:19 Apr 2018 05:03

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