1991
DOI: 10.2514/3.20690
|View full text |Cite
|
Sign up to set email alerts
|

Orbital motion under continuous radial thrust

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

0
25
0

Year Published

2000
2000
2024
2024

Publication Types

Select...
5
2

Relationship

0
7

Authors

Journals

citations
Cited by 44 publications
(25 citation statements)
references
References 2 publications
0
25
0
Order By: Relevance
“…In particular, he provided analytic solutions to the constant radial thrust problem, hereafter referred to as the Tsien problem. A comprehensive analysis of the problem is presented by Battin (1987) and Boltz (1991). It is found that there exists a limit value of the constant thrust that leads to a limit circular orbit.…”
Section: Introductionmentioning
confidence: 99%
“…In particular, he provided analytic solutions to the constant radial thrust problem, hereafter referred to as the Tsien problem. A comprehensive analysis of the problem is presented by Battin (1987) and Boltz (1991). It is found that there exists a limit value of the constant thrust that leads to a limit circular orbit.…”
Section: Introductionmentioning
confidence: 99%
“…The motion of a constant mass spacecraft under a radial thrust inversely proportional to the square of the distance from the primary body has been studied by Boltz (1991), and then further investigated by McInnes (2003) and Yamakawa (2006). From a practical point of view, a pure radial thrust can be obtained with a passive control by means of a sail having a slightly conical form, and whose apex is directed sunward (McInnes, 2003;Mengali and Quarta, 2005b).…”
Section: Introductionmentioning
confidence: 99%
“…A comprehensive analysis of the problem was presented by Battin [3], Boltz [4], and latter work by other authors [5,6,7,8] has provided further insight to the problem. The Tsien problem is integrable and admits closed-form solutions in terms of standard elliptic integrals: the radial time evolution depends on the incomplete elliptic integrals of the first and second kinds, and the orbit evolution is known to depend on the incomplete elliptic integral of the third kind [6].…”
Section: Introductionmentioning
confidence: 99%