| Issue |
A&A
Volume 572, December 2014
|
|
|---|---|---|
| Article Number | A106 | |
| Number of page(s) | 16 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201424064 | |
| Published online | 04 December 2014 | |
Online material
Appendix A: Asteroid spectra vs. meteorites spectra
The closest spectral matches between the reflectance spectra of the asteroids analyzed in our article and the laboratory spectra of different meteorites. Additional details related to meteorite samples are given in Table 3.
 |
Fig. A.1
Reflectance spectrum of (2201) Oljato and the closest three matches resulting from meteorite comparison: a) H6 ordinary chondrite Dwaleni (Sample ID: TB-TJM-073); b) L6 ordinary chondrite L’Aigle (Sample ID: TB-TJM-141); c) H6 ordinary chondrite Dwaleni (Sample ID: MB-CMP-003-D). |
| Open with DEXTER | |
 |
Fig. A.2
Reflectance spectrum of (4183) Cuno and the closest three matches resulting from meteorite comparison: a) LL6 ordinary chondrite Bandong (Sample ID: TB-TJM-067); b) LL6 ordinary chondrite Karatu (Sample ID: TB-TJM-077); c) L6 ordinary chondrite Wethersfield/1971 (Sample ID: TB-TJM-144). |
| Open with DEXTER | |
 |
Fig. A.3
Reflectance spectrum of (4486) Mithra and the closest three matches resulting from meteorite comparison: a) L6 ordinary chondrite Kunashak (Sample ID: TB-TJM-139); b) L6 ordinary chondrite Colby (Wisconsin) (Sample ID: MR-MJG-057); c) H5 ordinary chondrite Nuevo Mercurio (Sample ID: MH-FPF-053-D). |
| Open with DEXTER | |
 |
Fig. A.4
Reflectance spectrum of (5143) Heracles and the closest three matches resulting from meteorite comparison: a) LL6 ordinary chondrite Bandong (Sample ID: TB-TJM-067); b) L6 ordinary chondrite Colby (Wisconsin) (Sample ID: MR-MJG-057); c) LL6 ordinary chondrite Jelica (Sample ID: MR-MJG-072). |
| Open with DEXTER | |
 |
Fig. A.5
Reflectance spectrum of (6063) Jason (spectrum obtained on September 21, 2013) and the closest three matches resulting from meteorite comparison: a) LL5 ordinary chondrite Paragould (Sample ID: MB-CMP-002-L); b) L5 ordinary chondrite Mabwe-Khoywa (Sample ID: TB-TJM-107); c) L6 ordinary chondrite Gifu (Sample ID: MH-JFB-022). |
| Open with DEXTER | |
 |
Fig. A.6
Reflectance spectrum of (6063) Jason (spectrum obtained on October 21, 2013) and the closest three matches resulting from meteorite comparison: a) L6 ordinary chondrite Colby (Wisconsin) (Sample ID: MR-MJG-057); b) LL4 ordinary chondrite Y74442 (Sample ID: MB-TXH-086-A); c) L5 ordinary chondrite Farmington (Sample ID: MH-CMP-003). |
| Open with DEXTER | |
 |
Fig. A.7
Reflectance spectrum of (269690) 1996 RG3 (spectrum obtained on September 21, 2013) and the closest three matches resulting from meteorite comparison: a) CI Unusual carbonaceous chondrite Y-82162,79 <125 um (Sample ID: MB-CMP-019-1); b) CM2 carbonaceous chondrite Murchison heated at 900C (Sample ID: MB-TXH-064-F); c) CM2 carbonaceous chondrite LEW90500,45 (Sample ID: MC-RPB-002). |
| Open with DEXTER | |
Appendix B: The parameters of some of the spectra available in the literature
Comparison between several visible spectra available in the literature for the NEAs studied in this paper.
© ESO, 2014
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