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Solar radiation pressure influence in motion of asteroids, including near-Earth objects. / Martyusheva, Alexandra; Oskina, Kristina; Petrov, Nikita; Polyakhova, Elena.

2015 International Conference on Mechanics - Seventh Polyakhov's Reading. ed. / A. A. Tikhonov. Institute of Electrical and Electronics Engineers Inc., 2015. 7106756 (2015 International Conference on Mechanics - Seventh Polyakhov's Reading).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review

Harvard

Martyusheva, A, Oskina, K, Petrov, N & Polyakhova, E 2015, Solar radiation pressure influence in motion of asteroids, including near-Earth objects. in AA Tikhonov (ed.), 2015 International Conference on Mechanics - Seventh Polyakhov's Reading., 7106756, 2015 International Conference on Mechanics - Seventh Polyakhov's Reading, Institute of Electrical and Electronics Engineers Inc., 2015 INTERNATIONAL CONFERENCE ON MECHANICS SEVENTH POLYAKHOV'S READING, Saint Petersburg, Russian Federation, 2/02/15. https://doi.org/10.1109/POLYAKHOV.2015.7106756

APA

Martyusheva, A., Oskina, K., Petrov, N., & Polyakhova, E. (2015). Solar radiation pressure influence in motion of asteroids, including near-Earth objects. In A. A. Tikhonov (Ed.), 2015 International Conference on Mechanics - Seventh Polyakhov's Reading [7106756] (2015 International Conference on Mechanics - Seventh Polyakhov's Reading). Institute of Electrical and Electronics Engineers Inc.. https://doi.org/10.1109/POLYAKHOV.2015.7106756

Vancouver

Martyusheva A, Oskina K, Petrov N, Polyakhova E. Solar radiation pressure influence in motion of asteroids, including near-Earth objects. In Tikhonov AA, editor, 2015 International Conference on Mechanics - Seventh Polyakhov's Reading. Institute of Electrical and Electronics Engineers Inc. 2015. 7106756. (2015 International Conference on Mechanics - Seventh Polyakhov's Reading). https://doi.org/10.1109/POLYAKHOV.2015.7106756

Author

Martyusheva, Alexandra ; Oskina, Kristina ; Petrov, Nikita ; Polyakhova, Elena. / Solar radiation pressure influence in motion of asteroids, including near-Earth objects. 2015 International Conference on Mechanics - Seventh Polyakhov's Reading. editor / A. A. Tikhonov. Institute of Electrical and Electronics Engineers Inc., 2015. (2015 International Conference on Mechanics - Seventh Polyakhov's Reading).

BibTeX

@inproceedings{4de664964e8f4875b8fc7c654e5b5e01,
title = "Solar radiation pressure influence in motion of asteroids, including near-Earth objects",
abstract = "The orbital evolution of several groups of relatively small asteroids (of about several hundreds meters in size) is investigated by numerical integration, with solar radiation pressure effects taken into account. Basic equations are written in the frame of the three-body problem (Sun-planet-asteroid) together with the Solar System planetary perturbations. Numerical integration was carried out to model objects with diverse physical properties and orbital parameters. Three resonance regions with Jupiter (2:1, 3:2, 1:1) and one region with the Earth (1:1) were considered. Initial conditions for integration were chosen to correspond to real relationships in asteroid belt. It was discovered that solar radiation pressure effects increase significantly with orbital eccentricity for a given asteroid orbit, no matter how strong all other perturbing actions are. Maximal variations of orbital elements occur near the above-mentioned resonance regions with planets. For example, the derived estimates show that the total variation of the distance between an asteroid's non-perturbed orbit and the orbit as perturbed by solar radiation pressure force is as high as 103 km over 100 years for Jupiter and (1-4)×103 km for the Earth (where solar radiation is more intensive). In terms of the actual asteroid hazard for the Earth, the estimated time until a hazardous close approach (of about the Earth one radius) is 10-10000 years when solar radiation pressure is taken into account.",
author = "Alexandra Martyusheva and Kristina Oskina and Nikita Petrov and Elena Polyakhova",
year = "2015",
month = may,
day = "13",
doi = "10.1109/POLYAKHOV.2015.7106756",
language = "English",
series = "2015 International Conference on Mechanics - Seventh Polyakhov's Reading",
publisher = "Institute of Electrical and Electronics Engineers Inc.",
editor = "Tikhonov, {A. A.}",
booktitle = "2015 International Conference on Mechanics - Seventh Polyakhov's Reading",
address = "United States",
note = "2015 INTERNATIONAL CONFERENCE ON MECHANICS SEVENTH POLYAKHOV'S READING : SEVENTH POLYAKHOV'S READING ; Conference date: 02-02-2015 Through 06-02-2015",
url = "http://pol2015.math.spbu.ru/en/, http://pol2015.math.spbu.ru/en/about/, http://pol2015.math.spbu.ru/",

}

RIS

TY - GEN

T1 - Solar radiation pressure influence in motion of asteroids, including near-Earth objects

AU - Martyusheva, Alexandra

AU - Oskina, Kristina

AU - Petrov, Nikita

AU - Polyakhova, Elena

N1 - Conference code: 7

PY - 2015/5/13

Y1 - 2015/5/13

N2 - The orbital evolution of several groups of relatively small asteroids (of about several hundreds meters in size) is investigated by numerical integration, with solar radiation pressure effects taken into account. Basic equations are written in the frame of the three-body problem (Sun-planet-asteroid) together with the Solar System planetary perturbations. Numerical integration was carried out to model objects with diverse physical properties and orbital parameters. Three resonance regions with Jupiter (2:1, 3:2, 1:1) and one region with the Earth (1:1) were considered. Initial conditions for integration were chosen to correspond to real relationships in asteroid belt. It was discovered that solar radiation pressure effects increase significantly with orbital eccentricity for a given asteroid orbit, no matter how strong all other perturbing actions are. Maximal variations of orbital elements occur near the above-mentioned resonance regions with planets. For example, the derived estimates show that the total variation of the distance between an asteroid's non-perturbed orbit and the orbit as perturbed by solar radiation pressure force is as high as 103 km over 100 years for Jupiter and (1-4)×103 km for the Earth (where solar radiation is more intensive). In terms of the actual asteroid hazard for the Earth, the estimated time until a hazardous close approach (of about the Earth one radius) is 10-10000 years when solar radiation pressure is taken into account.

AB - The orbital evolution of several groups of relatively small asteroids (of about several hundreds meters in size) is investigated by numerical integration, with solar radiation pressure effects taken into account. Basic equations are written in the frame of the three-body problem (Sun-planet-asteroid) together with the Solar System planetary perturbations. Numerical integration was carried out to model objects with diverse physical properties and orbital parameters. Three resonance regions with Jupiter (2:1, 3:2, 1:1) and one region with the Earth (1:1) were considered. Initial conditions for integration were chosen to correspond to real relationships in asteroid belt. It was discovered that solar radiation pressure effects increase significantly with orbital eccentricity for a given asteroid orbit, no matter how strong all other perturbing actions are. Maximal variations of orbital elements occur near the above-mentioned resonance regions with planets. For example, the derived estimates show that the total variation of the distance between an asteroid's non-perturbed orbit and the orbit as perturbed by solar radiation pressure force is as high as 103 km over 100 years for Jupiter and (1-4)×103 km for the Earth (where solar radiation is more intensive). In terms of the actual asteroid hazard for the Earth, the estimated time until a hazardous close approach (of about the Earth one radius) is 10-10000 years when solar radiation pressure is taken into account.

UR - http://www.scopus.com/inward/record.url?scp=84938271576&partnerID=8YFLogxK

U2 - 10.1109/POLYAKHOV.2015.7106756

DO - 10.1109/POLYAKHOV.2015.7106756

M3 - Conference contribution

AN - SCOPUS:84938271576

T3 - 2015 International Conference on Mechanics - Seventh Polyakhov's Reading

BT - 2015 International Conference on Mechanics - Seventh Polyakhov's Reading

A2 - Tikhonov, A. A.

PB - Institute of Electrical and Electronics Engineers Inc.

T2 - 2015 INTERNATIONAL CONFERENCE ON MECHANICS SEVENTH POLYAKHOV'S READING

Y2 - 2 February 2015 through 6 February 2015

ER -

ID: 48585741