Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry

Andrey K. Murtazov

doi:doi:10.11648/j.ajmp.20130206.12

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Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry

Andrey K. Murtazov

Published in American Journal of Modern Physics (Volume 2, Issue 6)

Received: 29 August 2013 Accepted: Published: 20 October 2013

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Abstract

The reverse problem of the Solar system atmosphereless body and satellite photometry is the determination of their shapes, dimensions, and reflective properties based on the observed light curves. In general, the solution of the problem is not unambiguous. To disambiguate it, the author used the physical simulation method for obtaining satellite surface spectral indicatrices. This paper describes spectral characteristics of some space object surfaces which make it possible to identify them by photometric and spectral observation results.

Published in	American Journal of Modern Physics (Volume 2, Issue 6)
DOI	10.11648/j.ajmp.20130206.12
Page(s)	282-286
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Solar System, Atmosphereless Bodies, Photometry Reverse Problem, Physical Simulation, Surface Optical Properties

References

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[2]	M.A. Barucci, M. Fulchignoni, R. Salvatori, "Asteroid Photometry Simulated in the Laboratory: Phase Functions of Some Meteorites Used as Irregular Asteroid Models" Lunar and Planet. Sciences, Vol. 15, pp. 35-36 (1984).
[3]	V.M. Grigorevsky, S.Ya. Kolesnik, "Light reflection from regularity specular-surface space objects" Solar System Research, Vol. 12, pp. 107-119 (1978).
[4]	B.H. Hapke, "A Theoretical Photometric Function for the Lunar Surface" Journal of Geophysical Research, Vol. 68, pp. 4571-4586 (1963).
[5]	G.N. Kolesnichenko, A.V. Mironov, A.A. Vasjunin, S.V. Loginov, "Application of multispectral photometric data for recognition problem of space objects" Information-measuring and control systems, Radiotekhnika, Vol. 8, n. 5, pp. 86-92 (2010).
[6]	N.I. Koshkin, "Laboratory modeling of asteroids’ light curves" Solar System Research, Vol. 22, pp. 159-166 (1988).
[7]	V.I. Kuryshev, A.K. Murtazov, S.I. Vereshchyagin, "Modeling of astronomical objects photometric characteristics" USSR higher school proceedings. Instrument engineering, Vol. 28, pp. 81-85 (1985).
[8]	M.S. Mattews, "The Asteroid Conference in Tucson" Sky and Telescope, Vol. 42. pp. 22-24 (1971).
[9]	A.P. Mosin, "Solar light regular reflection by regular-surface convex body" Astronomical Circular, n. 1459, pp. 3-5 (1986).
[10]	A.K. Murtazov, "Laboratory photometry of bright diffuse cylinders" USSR higher school proceedings. Physics, Deposit manuscript, № 6178, 8 pp. (1983).
[11]	A.K. Murtazov, "Optical properties of artificial space objects and technogenic space debris" Near-Earth astronomy and the problems of investigations of small bodies in the Solar system. Collected Papers, Мoscow. Kosmosinform, pp. 262-268 (2000).
[12]	A.K. Murtazov, "Ecology of circumterrestrial space" Moscow, Fizmatlit, 304 pp. (2004).
[13]	A.K. Murtazov, "Direct photometric problem of optical monitoring of objects in circumterrestrial space" Russian Physics Journal, NY, Springer, Vol. 49, n. 11. pp. 1224-1229 (2006).
[14]	P. Oetking, "Photometric Studies of Diffuse Reflecting Surfaces with Applications to the Brightness of the Moon" Journal of Geophysical Research, Vol. 71, pp. 2505-2513 (1966).

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Andrey K. Murtazov. (2013). Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. American Journal of Modern Physics, 2(6), 282-286. https://doi.org/10.11648/j.ajmp.20130206.12

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ACS Style

Andrey K. Murtazov. Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. Am. J. Mod. Phys. 2013, 2(6), 282-286. doi: 10.11648/j.ajmp.20130206.12

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AMA Style

Andrey K. Murtazov. Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. Am J Mod Phys. 2013;2(6):282-286. doi: 10.11648/j.ajmp.20130206.12

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@article{10.11648/j.ajmp.20130206.12,
  author = {Andrey K. Murtazov},
  title = {Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry},
  journal = {American Journal of Modern Physics},
  volume = {2},
  number = {6},
  pages = {282-286},
  doi = {10.11648/j.ajmp.20130206.12},
  url = {https://doi.org/10.11648/j.ajmp.20130206.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajmp.20130206.12},
  abstract = {The reverse problem of the Solar system atmosphereless body and satellite photometry is the determination of their shapes, dimensions, and reflective properties based on the observed light curves. In general, the solution of the problem is not unambiguous. To disambiguate it, the author used the physical simulation method for obtaining satellite surface spectral indicatrices. This paper describes spectral characteristics of some space object surfaces which make it possible to identify them by photometric and spectral observation results.},
 year = {2013}
}

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TY  - JOUR
T1  - Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry
AU  - Andrey K. Murtazov
Y1  - 2013/10/20
PY  - 2013
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JF  - American Journal of Modern Physics
JO  - American Journal of Modern Physics
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PB  - Science Publishing Group
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AB  - The reverse problem of the Solar system atmosphereless body and satellite photometry is the determination of their shapes, dimensions, and reflective properties based on the observed light curves. In general, the solution of the problem is not unambiguous. To disambiguate it, the author used the physical simulation method for obtaining satellite surface spectral indicatrices. This paper describes spectral characteristics of some space object surfaces which make it possible to identify them by photometric and spectral observation results.
VL  - 2
IS  - 6
ER  -

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Author Information

Andrey K. Murtazov

Astronomical observatory, Ryazan State University, Ryazan, Russia

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APA Style

Andrey K. Murtazov. (2013). Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. American Journal of Modern Physics, 2(6), 282-286. https://doi.org/10.11648/j.ajmp.20130206.12

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ACS Style

Andrey K. Murtazov. Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. Am. J. Mod. Phys. 2013, 2(6), 282-286. doi: 10.11648/j.ajmp.20130206.12

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AMA Style

Andrey K. Murtazov. Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry. Am J Mod Phys. 2013;2(6):282-286. doi: 10.11648/j.ajmp.20130206.12

Copy | Download

@article{10.11648/j.ajmp.20130206.12,
  author = {Andrey K. Murtazov},
  title = {Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry},
  journal = {American Journal of Modern Physics},
  volume = {2},
  number = {6},
  pages = {282-286},
  doi = {10.11648/j.ajmp.20130206.12},
  url = {https://doi.org/10.11648/j.ajmp.20130206.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajmp.20130206.12},
  abstract = {The reverse problem of the Solar system atmosphereless body and satellite photometry is the determination of their shapes, dimensions, and reflective properties based on the observed light curves. In general, the solution of the problem is not unambiguous. To disambiguate it, the author used the physical simulation method for obtaining satellite surface spectral indicatrices. This paper describes spectral characteristics of some space object surfaces which make it possible to identify them by photometric and spectral observation results.},
 year = {2013}
}

Copy | Download

TY  - JOUR
T1  - Physical Simulation of Space Objects’ Spectral Characteristics for Solving the Reverse Problem of their Photometry
AU  - Andrey K. Murtazov
Y1  - 2013/10/20
PY  - 2013
N1  - https://doi.org/10.11648/j.ajmp.20130206.12
DO  - 10.11648/j.ajmp.20130206.12
T2  - American Journal of Modern Physics
JF  - American Journal of Modern Physics
JO  - American Journal of Modern Physics
SP  - 282
EP  - 286
PB  - Science Publishing Group
SN  - 2326-8891
UR  - https://doi.org/10.11648/j.ajmp.20130206.12
AB  - The reverse problem of the Solar system atmosphereless body and satellite photometry is the determination of their shapes, dimensions, and reflective properties based on the observed light curves. In general, the solution of the problem is not unambiguous. To disambiguate it, the author used the physical simulation method for obtaining satellite surface spectral indicatrices. This paper describes spectral characteristics of some space object surfaces which make it possible to identify them by photometric and spectral observation results.
VL  - 2
IS  - 6
ER  -

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