{"title":"Accuracy of Estimation of the Probability of Asteroid Collision with the Earth Based on Linear Stochastic Modeling of Parametric Uncertainty","authors":"V. A. Avdyushev, O. M. Syusina, V. A. Tamarov","doi":"10.1134/S0038094624602147","DOIUrl":null,"url":null,"abstract":"<p>This paper investigates the accuracy of probabilistic estimates of asteroid impacts with the Earth obtained by mapping over time the initial orbital uncertainty modeled by linear stochastic methods based on observational material. The accuracy of the estimated probabilities is established in comparison with the probabilities obtained using nonlinear stochastic methods. The example of test asteroids shows how linear methods can be inadequate under certain observational circumstances when applied for probabilistic assessment if the nonlinearity is extremely strong. The discrepancy between linear and nonlinear probability estimates sometimes reaches one or two orders of magnitude. In addition, nonlinear probability estimates may be zero even with very significant linear estimates; in other words, in the real absence of the risk of an asteroid colliding with the Earth, linear estimates will falsely indicate the danger of a catastrophe.</p>","PeriodicalId":778,"journal":{"name":"Solar System Research","volume":"59 6","pages":""},"PeriodicalIF":0.8000,"publicationDate":"2025-06-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar System Research","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0038094624602147","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This paper investigates the accuracy of probabilistic estimates of asteroid impacts with the Earth obtained by mapping over time the initial orbital uncertainty modeled by linear stochastic methods based on observational material. The accuracy of the estimated probabilities is established in comparison with the probabilities obtained using nonlinear stochastic methods. The example of test asteroids shows how linear methods can be inadequate under certain observational circumstances when applied for probabilistic assessment if the nonlinearity is extremely strong. The discrepancy between linear and nonlinear probability estimates sometimes reaches one or two orders of magnitude. In addition, nonlinear probability estimates may be zero even with very significant linear estimates; in other words, in the real absence of the risk of an asteroid colliding with the Earth, linear estimates will falsely indicate the danger of a catastrophe.
期刊介绍:
Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.