Asteroids 2867 Steins and 21 Lutetia: surface composition from far infrared observations with the Spitzer space telescope

被引：65

作者：

Barucci, M. A. ^{[1
]}

Fornasier, S. ^{[1
,2
]}

Dotto, E. ^{[3
]}

Lamy, P. L. ^{[4
]}

Jorda, L. ^{[4
]}

Groussin, O. ^{[4
]}

Brucato, J. R. ^{[5
]}

Carvano, J. ^{[6
]}

Alvarez-Candal, A. ^{[1
]}

Cruikshank, D. ^{[7
]}

Fulchignoni, A. ^{[1
,2
]}

机构：

[1] Observ Paris, LESIA, F-92195 Meudon, France

[2] Univ Pairs Dierot, Paris 07, France

[3] Osserv Astron Roma, INAF, I-00040 Rome, Italy

[4] Lab Astrophys Marseille, F-13376 Marseille 12, France

[5] Osserv Astron Capodimonte, INAF, I-80131 Naples, Italy

[6] Observ Natl COAA, BR-20921400 Rio De Janeiro, Brazil

[7] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2008年 / 477卷 / 02期

关键词：

minor planets; asteroids; techniques : spectroscopic; methods : observational;

D O I：

10.1051/0004-6361:20078085

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Aims. The aim of this paper is to investigate the surface composition of the two asteroids 21 Lutetia and 2867 Steins, targets of the Rosetta space mission. Methods. We observed the two asteroids through their full rotational periods with the Infrared Spectrograph of the Spitzer Space Telescope to investigate the surface properties. The analysis of their thermal emission spectra was carried out to detect emissivity features that diagnose the surface composition. Results. For both asteroids, the Christiansen peak, the Reststrahlen, and the Transparency features were detected. The thermal emissivity shows a clear analogy to carbonaceous chondrite meteorites, in particular to the CO-CV types for 21 Lutetia, while for 2867 Steins, already suggested as belonging to the E-type asteroids, the similarity to the enstatite achondrite meteorite is confirmed.

引用

页码：665 / 670

页数：6

共 31 条

[1] Rosetta asteroid targets: 2867 Steins and 21 Lutetia [J].