| Issue |
A&A
Volume 535, November 2011
|
|
|---|---|---|
| Article Number | A15 | |
| Number of page(s) | 15 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201117118 | |
| Published online | 25 October 2011 | |
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 meteorites samples are given in Table 3.
 |
Fig. A.1
Reflectance spectrum of (1917) Cuyo and the closest match resulting from meteorite comparison – H3-4 ordinary chondrite Dhajala. |
| Open with DEXTER | |
 |
Fig. A.2
Reflectance spectrum of (5620) Jasonwheeler and the closest three matches resulting from meteorite comparison: a) CM2 carbonaceous chondrite Mighei/Meghei; b) CM2 carbonaceous chondrite Cold Bokkeveld; c) CM2 carbonaceous chondrite ALH84029. |
| Open with DEXTER | |
 |
Fig. A.3
Reflectance spectrum of (8567) 1996 HW1 and the closest match resulting from the meteorite comparison – LL4 ordinary chondrite Hamlet. |
| Open with DEXTER | |
 |
Fig. A.4
Reflectance spectrum of (16960) 1998 QS52 and the closest three matches resulting from a meteorite comparison: a) L4 ordinary chondrite Saratov; b) L5 ordinary chondrite Homestead; c) LL4 ordinary chondrite Hamlet. |
| Open with DEXTER | |
 |
Fig. A.5
Reflectance spectrum of (188452) 2004 HE62 and the closest three matches resulting from meteorite comparison: a) L6 ordinary chondrite La Criolla; b) LL6 ordinary chondrite Cherokee Springs; c) L6 ordinary chondrite Wold Cottage. |
| Open with DEXTER | |
 |
Fig. A.6
Reflectance spectrum of (188452) 2004 HE62 and the closest three matches resulting from meteorite comparison: a) L4 ordinary chondrite Saratov; b) L5 ordinary chondrite Mirzapur; c) L4 ordinary chondrite Rio Negro. |
| Open with DEXTER | |
Appendix B: De-reddened asteroid spectra vs meteorites spectra
The closest spectral matches between the de-reddened spectra of the S-type asteroids analyzed in our article and the laboratory spectra of different meteorites. Additional details related to meteorites samples are given in Table 3.
 |
Fig. B.1
De-reddened spectrum of (1917) Cuyo and the closest three matches resulting from meteorite comparison: a) H6 ordinary chondrite Lancon; b) H5 ordinary chondrite Collescipoli; c) H5 ordinary chondrite Ehole. |
| Open with DEXTER | |
 |
Fig. B.2
De-reddened spectrum of (8567) 1996 HW1 and the closest three matches resulting from meteorite comparison: a) LL6 ordinary chondrite Cherokee Springs; b) L3-6 ordinary chondrite Hedjaz; c) LL6 ordinary chondrite Ensisheim. |
| Open with DEXTER | |
 |
Fig. B.3
De-reddened spectrum of (16960) 1998 QS52 and the closest two matches resulting from meteorite comparison: a) LL4 ordinary chondrite Hamlet; b) H4 ordinary chondrite Gruneberg. |
| Open with DEXTER | |
 |
Fig. B.4
De-reddened spectrum of (188452) 2004 HE62 and the closest three matches resulting from meteorite comparison: a) H6 ordinary chondrite Nanjemoy; b) H5 ordinary chondrite Olmedilla de Alarcon; c) H5 ordinary chondrite MAC88119.9. |
| Open with DEXTER | |
 |
Fig. B.5
De-reddened spectrum of 2010 TD54 and the closest three matches resulting from meteorite comparison: a) H4 ordinary chondrite Gruneberg; b) H6 ordinary chondrite Queen’s Mercy; c) H4 ordinary chondrite Ochansk. |
| Open with DEXTER | |
© ESO, 2011
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