Diamonds in space: a brief history and recent laboratory studies
Creators
- 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/10.1088/1742-6596/728/6/062004Additional details
Identifiers
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