Search for aqueously altered materials on asteroids

被引：30

作者：

Barucci, MA ^{[1
]}

Doressoundiram, A

Fulchignoni, M

Florczak, M

Lazzarin, M

Angeli, C

Lazzaro, D

机构：

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

[2] CNPq, ON, Dept Astrofis, BR-20921 Rio De Janeiro, Brazil

[3] CEFET, Dept Fis, BR-8000 Curitiba, Parana, Brazil

[4] Dipartimento Astron, I-35122 Padua, Italy

来源：

ICARUS | 1998年 / 132卷 / 02期

关键词：

D O I：

10.1006/icar.1998.5889

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The analysis of visible and near-infrared reflectance spectra of C-class objects has revealed the presence of features that appear to indicate a history of aqueous alteration on their surfaces. This result can provide constraints on our understanding of the early Solar System. We have recorded spectra covering 0.48-0.92 mu m for 29 C-class objects with orbital semimajor axes between 2.3 and 3.6 AU, About 70% of the observed objects show features produced as the result of aqueous alteration processes. (C) 1998 Academic Press.

引用

页码：388 / 396

页数：9

共 17 条

[1] Water ice in primitive asteroids? [J].