2020
DOI: 10.1007/s10569-020-9955-8
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Interplanetary gravity-assist fuel-optimal trajectory optimization with planetary and Solar radiation pressure perturbations

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Cited by 4 publications
(4 citation statements)
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“…In an Ephemeris model, it is essential to take into account perturbing accelerations resulting from: 1) 𝓕 : solar radiation pressure, 2) 𝓕 : oblateness impacts of celestial bodies, and 3) 𝓕 : other celestial bodies of the Solar System. The disturbing accelerations are conceptualized as [28] ( ) where 𝒓 and πœ‡ show the position vector and the gravitational constant of a planet, πœ•π‘§ πœ•π’“ ⁄ = [0 0 1] , πœ‘ represents the planet-centric latitude, 𝜎 is a constant flight loading (𝜎=π‘š 𝐴 ⁄ where 𝐴 is the unit area), 𝜎 * is determined as 1.53 (gm -2 ), 𝛽 and 𝒓 signify the solar radiation pressure and the spacecraft position vector, in the Heliocentric Equatorial Reference Frame (HERF). The dynamics system is modeled as follows [28]:…”
Section: System Descriptionmentioning
confidence: 99%
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“…In an Ephemeris model, it is essential to take into account perturbing accelerations resulting from: 1) 𝓕 : solar radiation pressure, 2) 𝓕 : oblateness impacts of celestial bodies, and 3) 𝓕 : other celestial bodies of the Solar System. The disturbing accelerations are conceptualized as [28] ( ) where 𝒓 and πœ‡ show the position vector and the gravitational constant of a planet, πœ•π‘§ πœ•π’“ ⁄ = [0 0 1] , πœ‘ represents the planet-centric latitude, 𝜎 is a constant flight loading (𝜎=π‘š 𝐴 ⁄ where 𝐴 is the unit area), 𝜎 * is determined as 1.53 (gm -2 ), 𝛽 and 𝒓 signify the solar radiation pressure and the spacecraft position vector, in the Heliocentric Equatorial Reference Frame (HERF). The dynamics system is modeled as follows [28]:…”
Section: System Descriptionmentioning
confidence: 99%
“…The first aspect of this study concerns the design of an optimal Earth-to-Mars mission, which involves identifying launch windows and minimizing fuel consumption while considering various factors and constraints [24][25][26][27][28][29]. A low-thrust trajectory mission from Earth to Mars is analyzed, taking into account gravitational perturbations due to all planets in the Solar System, solar radiation pressure, and non-spherical perturbations of all planets.…”
Section: Introductionmentioning
confidence: 99%
“…The FTS payload measures wind velocity and direction, assisting in the study of geological weather circulation in Mars' atmosphere and determining suitable locations for wind power plant construction and climate study on Mars. The THz payload is for water vapor detection in Mars' atmosphere, delivering a study on Martian atmospheric properties [50].…”
Section: Introductionmentioning
confidence: 99%
“…Some alternative methods tackle this challenge by initializing co-states through particle swarm optimization (PSO) [21,30], optimal auxiliary unconstrained solutions [31], and the adjoint variable method [32]. Subsequent refinements by Jiang et al [30] and Saghamanesh and Baoyin [21,[33][34][35][36] have further improved this approach using various effective-practical techniques.…”
Section: Introductionmentioning
confidence: 99%