{"title":"Maximizing the velocity deflection of asteroid Didymos using the Whale Optimization Algorithm","authors":"Iman Shafieenejad","doi":"10.1016/j.pss.2025.106075","DOIUrl":null,"url":null,"abstract":"<div><div>This study aims to optimize the velocity change of the Didymos asteroid using the Whale Optimization Algorithm (WOA). The deflection of asteroids that pose significant threats to Earth is a crucial aspect of upcoming space missions. In this research, a spacecraft is attached to the Didymos asteroid, utilizing its gravitational force as a perturbation to modify the asteroid's trajectory. The transfer of kinetic energy from the spacecraft to the asteroid induces a change in velocity (ΔV). The findings indicate that the most substantial impact on velocity occurs in the radial direction, showing divergent oscillatory behavior. The results suggest that the optimal point for significant velocity change is located shortly after the perihelion. At this point, WOA achieves the maximum velocity change. Additionally, the stability of the asteroid's deflection is investigated due to the nonlinear characteristics of the orbital motion equations. The optimal velocity change is identified as <span><math><mrow><mo>Δ</mo><msub><mi>V</mi><mrow><mi>t</mi><mi>o</mi><mi>t</mi><mi>a</mi><mi>l</mi></mrow></msub><mo>=</mo><mn>2.5139</mn><mo>×</mo><mn>1</mn><msup><mn>0</mn><mrow><mo>−</mo><mn>7</mn></mrow></msup><mrow><mo>(</mo><mfrac><mrow><mi>k</mi><mi>m</mi></mrow><mi>s</mi></mfrac><mo>)</mo></mrow></mrow></math></span> at <span><math><mrow><mo>Δ</mo><mi>t</mi><mo>=</mo><mn>27.657</mn><mrow><mo>(</mo><mi>h</mi><mo>)</mo></mrow></mrow></math></span>, occurring after the perihelion at <span><math><mrow><msub><mrow><mi>t</mi><mrow><mo>(</mo><mi>h</mi><mo>)</mo></mrow></mrow><mrow><mo>Δ</mo><msub><mi>V</mi><mi>max</mi></msub></mrow></msub></mrow></math></span>. This study introduces a novel optimization approach for asteroid deflection, emphasizing the nonlinear dynamics of orbital motion.</div></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"258 ","pages":"Article 106075"},"PeriodicalIF":1.8000,"publicationDate":"2025-02-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S003206332500042X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This study aims to optimize the velocity change of the Didymos asteroid using the Whale Optimization Algorithm (WOA). The deflection of asteroids that pose significant threats to Earth is a crucial aspect of upcoming space missions. In this research, a spacecraft is attached to the Didymos asteroid, utilizing its gravitational force as a perturbation to modify the asteroid's trajectory. The transfer of kinetic energy from the spacecraft to the asteroid induces a change in velocity (ΔV). The findings indicate that the most substantial impact on velocity occurs in the radial direction, showing divergent oscillatory behavior. The results suggest that the optimal point for significant velocity change is located shortly after the perihelion. At this point, WOA achieves the maximum velocity change. Additionally, the stability of the asteroid's deflection is investigated due to the nonlinear characteristics of the orbital motion equations. The optimal velocity change is identified as at , occurring after the perihelion at . This study introduces a novel optimization approach for asteroid deflection, emphasizing the nonlinear dynamics of orbital motion.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research