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Cosmic Dust
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High Quality Content by WIKIPEDIA articles! Cosmic dust is a type of dust composed of particles in space which are a few molecules to 0.1 mm in size. Cosmic dust can be further distinguished by its astronomical location; for example: intergalactic dust, interstellar dust (potentially concentrated in a nebula), interplanetary dust (such as in a circumstellar disk) and circumplanetary dust (such as in a planetary ring). In our own Solar System, interplanetary dust causes the zodiacal light. Sources include comet dust, asteroidal dust, dust from the Kuiper belt, and interstellar dust passing through our solar system. The terminology has no specific application for describing materials found on the planet Earth, other than in the most general sense that all elements with an atomic mass higher than hydrogen are believed to be formed in the core of stars via stellar nucleosynthesis and supernova events. As such all elements that exist can be indiscriminately considered to be a form of "cosmic dust".
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786130250607
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Sprache Englisch
- Genre Physik & Astronomie
- Größe H220mm x B150mm x T8mm
- Jahr 2009
- EAN 9786130250607
- Format Kartonierter Einband
- ISBN 978-613-0-25060-7
- Titel Cosmic Dust
- Untertitel Dust, Molecule, Outer space, Interstellar medium, Nebula, Circumstellar disk, Planetary ring, Solar System, Zodiacal light, Asteroid belt, Kuiper belt, Stellar nucleosynthesis, Supernova
- Gewicht 207g
- Herausgeber Alphascript Publishing
- Anzahl Seiten 128
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