Determining the size of craters on the surfaces of atmosphereless bodies in Solar system with ground-based methods
Вісник астрономічної школи
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Title |
Determining the size of craters on the surfaces of atmosphereless bodies in Solar system with ground-based methods
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Creator |
Klianchin A.I.
Prokof'eva-Mikchailovskaya V.V. |
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Date |
2013
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Source |
Astronomical School’s Report, 2013, Volume 9, Issue 2, P. 111-114
2411-6602 |
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Identifier |
http://astro.nau.edu.ua/papers/AstSR_2013_Vol_9_Iss_2_P_111.pdf
10.18372/2411-6602.09.2111 |
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Language |
ru
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Description |
A new method of determining the size of craters on the surfaces of atmosphereless bodies of the Solar system, called spectral-frequency method (SFM), was developed at the Crimean Astrophysical Observatory by V. V. Prokofieva-Mikhaylovska, N. A. Rublevsky in collaboration with V. V. Busarev from SAI (MSU). SFM of studying color- or lightcurves of asteroids allows to obtain information about the size of details on their surfaces with ground-based tools. Visibility of craters is explained with the inverse coherent scattering of solar radiation on the regolith ejected during bodies collisions.
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Publisher |
National Aviation University
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Format |
application/pdf
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