Published July 1, 2016 | Version v1
Journal article

Diamonds in space: a brief history and recent laboratory studies

  • 1. Institute of Atomic and Molecular Sciences, Academia Sinica, Taipei 106, Taiwan (China)

Description

Stardust grains exist in outer space. However, due to their low abundance, structural heterogeneities, and lack of distinct spectroscopic features, unambiguous identification of their chemical composition has been a challenge. Diamond is a notable exception because it is composed of carbon and has several unique physicochemical properties that make the identification possible. Here, we provide a brief review on how diamonds were discovered in space based on the remarkable spectral matching between laboratory spectra and astronomical observations of the infrared emission at 3.43 and 3.53 µm, followed by a discussion of fluorescent nanodiamond as a possible carrier for extended red emission at 600 — 800 nm. Recent evidence to support the latter suggestion is provided. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/728/6/062004

Additional details

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
728
Journal Issue
6
Journal Page Range
[8 p.]
ISSN
1742-6596

Conference

Title
Physics and chemistry of the late stages of stellar evolution
Acronym
11. Pacific Rim conference on stellar astrophysics
Dates
14-17 Dec 2015
Place
Hong Kong (China)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
48100373
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ABUNDANCE; ASTRONOMY; CHEMICAL COMPOSITION; COSMIC DUST; DIAMONDS; FLUORESCENCE; INFRARED SPECTRA; INTERSTELLAR GRAINS; SPACE
Descriptors DEC
CARBON; DUSTS; ELEMENTS; EMISSION; LUMINESCENCE; MINERALS; NONMETALS; PARTICLES; PHOTON EMISSION; SPECTRA