Intermediate-thrust arcs and their optimality in a central, time-invariant force field
dc.creator | Archenti, Aníbal R. | |
dc.creator | Vinh, Nguyen X. | |
dc.date | 1973 | |
dc.date | 2021-08-20T19:16:04Z | |
dc.date.accessioned | 2023-07-15T02:44:13Z | |
dc.date.available | 2023-07-15T02:44:13Z | |
dc.identifier | http://sedici.unlp.edu.ar/handle/10915/123097 | |
dc.identifier | issn:0022-3239 | |
dc.identifier | issn:1573-2878 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7463082 | |
dc.description | This paper presents the general equations of the intermediate-thrust arcs in a general, time-invariant, central force field. Two families of planar arcs, namely, the family of Lawden's spirals in the equatorial plane of an oblate planet and the family of intermediate-thrust arcs in a gravitational field of the form μ/r<sup>n</sup>, have been considered in detail. The Kelley-Contensou condition has been used to test their optimality condition. It is shown that, in the first case, there exist portions of the arcs at a finite distance satisfying the condition, while, in the second case, the entire family satisfies the condition for n ≥ 3. Hence, in a perturbed Newtonian gravitational force field, the intermediate-thrust arcs, under certain favorable conditions, can be part of an optimal trajectory. | |
dc.description | Facultad de Ingeniería | |
dc.format | application/pdf | |
dc.format | 293-304 | |
dc.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
dc.subject | Ingeniería | |
dc.subject | Ingeniería Aeronáutica | |
dc.subject | Optimality Condition | |
dc.subject | Force Field | |
dc.subject | Favorable Condition | |
dc.subject | General Equation | |
dc.subject | Gravitational Field | |
dc.title | Intermediate-thrust arcs and their optimality in a central, time-invariant force field | |
dc.type | Articulo | |
dc.type | Articulo |