308 Polyxo:: ISO-SWS spectrum up to 26 micron

被引:17
作者
Dotto, E
Barucci, MA
Brucato, JR
Müller, TG
Carvano, J
机构
[1] INAF, Osservatorio Astron Roma, I-00040 Rome, Italy
[2] Observ Paris, LESIA, F-92195 Meudon, France
[3] INAF, Osservatorio Astron Capodimonte, I-80131 Naples, Italy
[4] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[5] CAA, MCT, Observ Nacl, BR-20921400 Rio De Janeiro, Brazil
关键词
minor planets; asteroids; radiation mechanisms : thermal; infrared : solar system; meteors; meteorites;
D O I
10.1051/0004-6361:20041638
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Infrared spectroscopic observations of the asteroid 308 Polyxo have been carried out by the Infrared Space Observatory (ISO) with the Short Wavelength Spectrometer (SWS) in the spectral region between 7 and 26 mum. The Standard Thermal Model and the Thermophysical Model have been applied to the obtained data in order to model the thermal continuum. Sub-solar and black-body temperatures also have been derived. The obtained spectrum has been compared with laboratory spectra of minerals and meteorites available in the literature. Moreover, we performed new measurements to obtain infrared spectra of the Tagish Lake meteorite, recognized as the best analog of primitive D-type asteroids. A tentative spectral similarity with the Ornans meteorite is suggested, while we cannot confirm, in the considered wavelength range, the analogy with the Tagish Lake meteorite.
引用
收藏
页码:1081 / U130
页数:6
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