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Behavior of metal-containing species during entries of meteoroids into atmospheres of Mars, Jupiter, and Titan
Вісник астрономічної школи
View Archive Info| Field | Value | |
| Title |
Behavior of metal-containing species during entries of meteoroids into atmospheres of Mars, Jupiter, and Titan
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| Creator |
Berezhnoy A.A.
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| Date |
2011
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| Source |
Astronomical School’s Report, 2011, Volume 7, Issue 1, P. 11-15
2411-6602 |
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| Identifier |
http://astro.nau.edu.ua/papers/AstSR_2011_Vol_7_Iss_1_P_11.pdf
10.18372/2411-6602.07.1011 |
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| Language |
en
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| Description |
Chemical composition of impact-produced clouds during meteor events on Mars, Jupiter, and Titan is studied. The intensities of brightest atomic lines of meteoroid origin of Martian and Titan's bolides are comparable to that of Earth's bolides because in all these atmospheres abundances of metal monoxides, atoms and ions are comparable while the electronic density is determined by the matter of meteoroid origin. The most intensive lines in visible spectra of Martian and Titan's meteors are lines of atoms and ions of Na, Fe, Mg, and Ca. In spectra of Jupiter's superbolides the intensity of lines of atoms is higher than that of ions.
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| Publisher |
National Aviation University
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| Format |
application/pdf
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