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Observations and theoretical analysis of lightcurves of natural satellites of planets. / Devyatkin, A.V.; Gorshanov, D.L.; Gritsuk, A. N.; Mel'nikov, A. V.; Sidorov, M. Yu; Shevchenko, I. I.

в: Solar System Research, Том 36, № 3, 01.12.2002, стр. 248-259.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Devyatkin, AV, Gorshanov, DL, Gritsuk, AN, Mel'nikov, AV, Sidorov, MY & Shevchenko, II 2002, 'Observations and theoretical analysis of lightcurves of natural satellites of planets', Solar System Research, Том. 36, № 3, стр. 248-259. https://doi.org/10.1023/A:1015849332450

APA

Devyatkin, A. V., Gorshanov, D. L., Gritsuk, A. N., Mel'nikov, A. V., Sidorov, M. Y., & Shevchenko, I. I. (2002). Observations and theoretical analysis of lightcurves of natural satellites of planets. Solar System Research, 36(3), 248-259. https://doi.org/10.1023/A:1015849332450

Vancouver

Devyatkin AV, Gorshanov DL, Gritsuk AN, Mel'nikov AV, Sidorov MY, Shevchenko II. Observations and theoretical analysis of lightcurves of natural satellites of planets. Solar System Research. 2002 Дек. 1;36(3):248-259. https://doi.org/10.1023/A:1015849332450

Author

Devyatkin, A.V. ; Gorshanov, D.L. ; Gritsuk, A. N. ; Mel'nikov, A. V. ; Sidorov, M. Yu ; Shevchenko, I. I. / Observations and theoretical analysis of lightcurves of natural satellites of planets. в: Solar System Research. 2002 ; Том 36, № 3. стр. 248-259.

BibTeX

@article{d46f30963cd14de6b9271ec1f0137f65,
title = "Observations and theoretical analysis of lightcurves of natural satellites of planets",
abstract = "We present the results of photometric observations of Saturn's seventh satellite Hyperion and four other planetary satellites: Saturn's moon Phoebe and three Jovian satellites Himalia, Elara, and Pasiphae. The observations have been conducted from September, 1999 to March, 2000, and during September-October, 2000. Analysis of periodic variations in Hyperion's lightcurve was performed. The lightcurve was modeled using the software package developed for calculating the rotational dynamics of a satellite. Our data generally indicate that over the period of observations Hyperion was in the chaotic mode of rotation.",
author = "A.V. Devyatkin and D.L. Gorshanov and Gritsuk, {A. N.} and Mel'nikov, {A. V.} and Sidorov, {M. Yu} and Shevchenko, {I. I.}",
year = "2002",
month = dec,
day = "1",
doi = "10.1023/A:1015849332450",
language = "English",
volume = "36",
pages = "248--259",
journal = "Solar System Research",
issn = "0038-0946",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Observations and theoretical analysis of lightcurves of natural satellites of planets

AU - Devyatkin, A.V.

AU - Gorshanov, D.L.

AU - Gritsuk, A. N.

AU - Mel'nikov, A. V.

AU - Sidorov, M. Yu

AU - Shevchenko, I. I.

PY - 2002/12/1

Y1 - 2002/12/1

N2 - We present the results of photometric observations of Saturn's seventh satellite Hyperion and four other planetary satellites: Saturn's moon Phoebe and three Jovian satellites Himalia, Elara, and Pasiphae. The observations have been conducted from September, 1999 to March, 2000, and during September-October, 2000. Analysis of periodic variations in Hyperion's lightcurve was performed. The lightcurve was modeled using the software package developed for calculating the rotational dynamics of a satellite. Our data generally indicate that over the period of observations Hyperion was in the chaotic mode of rotation.

AB - We present the results of photometric observations of Saturn's seventh satellite Hyperion and four other planetary satellites: Saturn's moon Phoebe and three Jovian satellites Himalia, Elara, and Pasiphae. The observations have been conducted from September, 1999 to March, 2000, and during September-October, 2000. Analysis of periodic variations in Hyperion's lightcurve was performed. The lightcurve was modeled using the software package developed for calculating the rotational dynamics of a satellite. Our data generally indicate that over the period of observations Hyperion was in the chaotic mode of rotation.

UR - http://www.scopus.com/inward/record.url?scp=0036283802&partnerID=8YFLogxK

U2 - 10.1023/A:1015849332450

DO - 10.1023/A:1015849332450

M3 - Article

AN - SCOPUS:0036283802

VL - 36

SP - 248

EP - 259

JO - Solar System Research

JF - Solar System Research

SN - 0038-0946

IS - 3

ER -

ID: 45989551