£113.02

Springer - Composition and Origin of Cometary Materials

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Description

Explore the fundamental building blocks of our solar system with this scientific volume from the ISSI Space Sciences Series. Comet nuclei represent the most primitive bodies in existence, having formed far from the early Sun. Because their material properties have changed very little since their creation, they offer a direct window into the chemical and thermodynamic conditions of the original solar nebula. This book brings together insights from leading cometary experts to examine the composition and structure of these celestial bodies. The content provides a detailed review of scientific conclusions drawn from in situ measurements taken during the Comet Halley mission. Additionally, it incorporates remote sensing observations from the bright comets Hale-Bopp and Hyakutake. This collection serves as a vital resource for researchers and students studying the origins of our solar system through the lens of cometary science.

Key Features

Provides deep insights into the primitive nature of comet nuclei and their role in solar system history.

Includes expert reviews based on direct in situ measurements from the Comet Halley mission.

Covers remote sensing observation data from the notable bright comets Hale-Bopp and Hyakutake.

Analyzes the chemical and thermodynamic conditions of the early solar nebula.

Part of the professional Space Sciences Series of ISSI for academic and research use.

Product Specifications

Format
hardcover
Domain
Amazon UK
Release Date
31 January 2000
Listed Since
15 December 2006

Barcode

No barcode data available

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