Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion
Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensi...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Perodios, E. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1992 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1992 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 192(1992), 2 vom: Juni, Seite 291-297 |
|---|---|
| Übergeordnetes Werk: |
volume:192 ; year:1992 ; number:2 ; month:06 ; pages:291-297 |
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| DOI / URN: |
10.1007/BF00684486 |
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| 520 | |a Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. | ||
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10.1007/BF00684486 doi (DE-627)OLC2066189480 (DE-He213)BF00684486-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Perodios, E. verfasserin aut Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion 1992 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1992 Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. Parameter Space Early Paper Mass Parameter Periodic Motion Parameter Region Markellos, V. V. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 192(1992), 2 vom: Juni, Seite 291-297 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:192 year:1992 number:2 month:06 pages:291-297 https://doi.org/10.1007/BF00684486 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 GBV_ILN_4700 AR 192 1992 2 06 291-297 |
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10.1007/BF00684486 doi (DE-627)OLC2066189480 (DE-He213)BF00684486-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Perodios, E. verfasserin aut Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion 1992 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1992 Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. Parameter Space Early Paper Mass Parameter Periodic Motion Parameter Region Markellos, V. V. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 192(1992), 2 vom: Juni, Seite 291-297 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:192 year:1992 number:2 month:06 pages:291-297 https://doi.org/10.1007/BF00684486 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 GBV_ILN_4700 AR 192 1992 2 06 291-297 |
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10.1007/BF00684486 doi (DE-627)OLC2066189480 (DE-He213)BF00684486-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Perodios, E. verfasserin aut Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion 1992 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1992 Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. Parameter Space Early Paper Mass Parameter Periodic Motion Parameter Region Markellos, V. V. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 192(1992), 2 vom: Juni, Seite 291-297 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:192 year:1992 number:2 month:06 pages:291-297 https://doi.org/10.1007/BF00684486 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 GBV_ILN_4700 AR 192 1992 2 06 291-297 |
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10.1007/BF00684486 doi (DE-627)OLC2066189480 (DE-He213)BF00684486-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Perodios, E. verfasserin aut Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion 1992 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1992 Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. Parameter Space Early Paper Mass Parameter Periodic Motion Parameter Region Markellos, V. V. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 192(1992), 2 vom: Juni, Seite 291-297 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:192 year:1992 number:2 month:06 pages:291-297 https://doi.org/10.1007/BF00684486 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 GBV_ILN_4700 AR 192 1992 2 06 291-297 |
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10.1007/BF00684486 doi (DE-627)OLC2066189480 (DE-He213)BF00684486-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Perodios, E. verfasserin aut Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion 1992 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1992 Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. Parameter Space Early Paper Mass Parameter Periodic Motion Parameter Region Markellos, V. V. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 192(1992), 2 vom: Juni, Seite 291-297 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:192 year:1992 number:2 month:06 pages:291-297 https://doi.org/10.1007/BF00684486 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 GBV_ILN_4700 AR 192 1992 2 06 291-297 |
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Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion |
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Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. © Kluwer Academic Publishers 1992 |
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Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. © Kluwer Academic Publishers 1992 |
| abstract_unstemmed |
Abstract The intervals of possible stability, on the μ-axis, of the basic families of three-dimensional periodie motions of the restricted three-body problem (determined in an earlier paper) are extended into regions of the μ-m3 parameter space of the general three-body problem. Sample three-dimensional periodic motions corresponding to these regions are computed and tested for stability. Six regions, corresponding to the vertical-critical orbitsl1v, m1v,m2v, andilv, survive this preliminary stability test-therefore, emerging as the mass parameters regions allowing the simplest types of stable low inclination three-dimensional motion of three massive bodies. © Kluwer Academic Publishers 1992 |
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| title_short |
Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion |
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Markellos, V. V. |
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