Simonia, Irakli და Nabiyev, Shaig (2015) Nano-metric Dust Particles as a Hardly Detectable Component of the Interplanetary Dust Cloud. Journal of Astrophysics and Astronomy, 36 (3). С. 409-419.
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The present work introduces of existence of a hardly detectable component of the interplanetary dust cloud and demonstrates that such a component is a dust formation consisting of the dust particles of nano-metric dimensions. This work describes the main physical properties of such a kind of nano-dust,and its possible chemical and mineralogical peculiarities proposes new explanations related to reddening of the dynamically cold transneptunian objects on account of scattering their light by nano-dust of the hardly detectable component of the interplanetary dust cloud. We propose the relation for the coefficient of absorption by the nano-dust and provide result of the statistical analysis of the TNO color index-orbital inclinations. We also present a critical assessment of the proposed hypothesis.
| ობიექტის ტიპი: | სტატია |
|---|---|
| თემატიკა: | Q Science > QB Astronomy Q Science > QC Physics |
| ქვეგანყოფილება: | Faculties/Schools > School of Natural Sciences and Engineering |
| განმათავსებელი მომხმარებელი: | Irakli Simonia |
| განთავსების თარიღი: | 23 მაისი 2016 10:31 |
| ბოლო ცვლილება: | 23 მაისი 2016 10:31 |
| URI: | http://eprints.iliauni.edu.ge/id/eprint/4665 |
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