A family of stacked central configurations in the planar five-body problem
We study planar central configurations of the five-body problem where three bodies, m 1 , m 2 and m 3 , are collinear and ordered from left to right, while the other two, m 4 and m 5 , are placed symmetrically with respect to the line containing the three collinear bodies. We prove that when the col...
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| Vydáno v: | Celestial mechanics and dynamical astronomy Ročník 129; číslo 3; s. 321 - 328 |
|---|---|
| Hlavní autoři: | , , |
| Médium: | Journal Article Publikace |
| Jazyk: | angličtina |
| Vydáno: |
Dordrecht
Springer Netherlands
01.11.2017
Springer Nature B.V |
| Témata: | |
| ISSN: | 0923-2958, 1572-9478 |
| On-line přístup: | Získat plný text |
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| Shrnutí: | We study planar central configurations of the five-body problem where three bodies,
m
1
,
m
2
and
m
3
, are collinear and ordered from left to right, while the other two,
m
4
and
m
5
, are placed symmetrically with respect to the line containing the three collinear bodies. We prove that when the collinear bodies form an Euler central configuration of the three-body problem with
m
1
=
m
3
, there exists a new family, missed by Gidea and Llibre (Celest Mech Dyn Astron 106:89–107,
2010
), of stacked five-body central configuration where the segments
m
4
m
5
and
m
1
m
3
do not intersect. |
|---|---|
| Bibliografie: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ISSN: | 0923-2958 1572-9478 |
| DOI: | 10.1007/s10569-017-9782-8 |