LABORATORY STUDY OF SILICATES AND APPLICATION TO COMETARY DUST

被引：2

作者：

BLANCO, A

OROFINO, V

MARTINO, M

FONTI, S

STEPHENS, JR

机构：

[1] Dipartimento di Fisica dell'Università, Lecce, 73100

[2] Istituto di Fisica Sperimentale, IUN, Napoli, 80133

[3] Los Alamos National Laboratory, Los Alamos, 87545, NM

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS | 1992年 / 15卷 / 06期

关键词：

Interplanetary space; Interstellar matter and nebulae; Laboratory techniques;

D O I：

10.1007/BF02506700

中图分类号：

学科分类号：

摘要：

The mass absorption coefficients of some glassy and crystalline silicates of astrophysical relevance have been measured. We produced and characterized also synthetic silicates of olivine type since this material is considered one of the most likely components of cometary dust grains. The experimental data are used to fit the emission feature observed in the Comet Halley spectrum between 8 and 13 mum. Satisfactory results are obtained by using synthetic olivine mixed with a small amount (5%) of crystalline grains.

引用

页码：1091 / 1096

页数：6

共 14 条

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