{"title":"The current impact rate on the regular satellites of Jupiter, Saturn, and Uranus","authors":"R. Brasser, E. W. Wong, S. C. Werner","doi":"10.1051/0004-6361/202453433","DOIUrl":null,"url":null,"abstract":"<i>Context.<i/> The impact and cratering rates onto the regular satellites of the giant planets are subject to great uncertainties.<i>Aims.<i/> We aim to compute the impact rates for objects with a diameter <i>D<i/><sub>i<sub/> > 1 km onto the regular satellites of Jupiter, Saturn, and Uranus using dynamical simulations of the evolution of the outer Solar System coupled with the best estimates of the current population of objects beyond Neptune, and their size-frequency distribution.<i>Methods.<i/> We analyse the last 3.5 billion years of evolution of the outer Solar System from our database of simulations and combine this with observational constraints of the population beyond Neptune to compute the flux of objects entering the Centaur region. The initial conditions of these simulations resemble the current population. We obtain an improved estimate of the impact probability of a Centaur with the satellites from enacting simulations of planetesimals flying past the satellites on hyperbolic orbits, which agree with literature precedents.<i>Results.<i/> Our impact rate of objects <i>D<i/><sub>i<sub/> > 1 km with Jupiter is 0.001 yr<sup>−1<sup/>, which is 3–6 times lower than previous estimates. Both our impact probabilities with the satellites scaled to the giant planets and leakage rate of objects from beyond Neptune into the Centaur region are consistent with earlier literature estimates. However, our absolute impact probabilities with the giant planets are lower. We attribute this difference to whether the impact probabilities are computed over the whole age of the Solar System including planet migration, or over a shorter interval closer to the present.<i>Conclusions.<i/> Our lower impact rate compared to earlier literature estimates is due to basing our results on the flux of objects coming in from beyond Neptune rather than relying on the current observed impact rate with Jupiter. We stress the importance of clearly stating all parameters and assumptions in future studies to enable meaningful comparisons.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"94 1","pages":""},"PeriodicalIF":5.8000,"publicationDate":"2025-03-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202453433","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Context. The impact and cratering rates onto the regular satellites of the giant planets are subject to great uncertainties.Aims. We aim to compute the impact rates for objects with a diameter Di > 1 km onto the regular satellites of Jupiter, Saturn, and Uranus using dynamical simulations of the evolution of the outer Solar System coupled with the best estimates of the current population of objects beyond Neptune, and their size-frequency distribution.Methods. We analyse the last 3.5 billion years of evolution of the outer Solar System from our database of simulations and combine this with observational constraints of the population beyond Neptune to compute the flux of objects entering the Centaur region. The initial conditions of these simulations resemble the current population. We obtain an improved estimate of the impact probability of a Centaur with the satellites from enacting simulations of planetesimals flying past the satellites on hyperbolic orbits, which agree with literature precedents.Results. Our impact rate of objects Di > 1 km with Jupiter is 0.001 yr−1, which is 3–6 times lower than previous estimates. Both our impact probabilities with the satellites scaled to the giant planets and leakage rate of objects from beyond Neptune into the Centaur region are consistent with earlier literature estimates. However, our absolute impact probabilities with the giant planets are lower. We attribute this difference to whether the impact probabilities are computed over the whole age of the Solar System including planet migration, or over a shorter interval closer to the present.Conclusions. Our lower impact rate compared to earlier literature estimates is due to basing our results on the flux of objects coming in from beyond Neptune rather than relying on the current observed impact rate with Jupiter. We stress the importance of clearly stating all parameters and assumptions in future studies to enable meaningful comparisons.
上下文。对巨行星的常规卫星的撞击和撞击率存在很大的不确定性。我们的目标是利用外太阳系演化的动力学模拟,结合目前海王星外天体数量的最佳估计,以及它们的大小-频率分布,计算直径为1000公里的天体对木星、土星和天王星的常规卫星的撞击率。我们从模拟数据库中分析了最近35亿年外太阳系的演变,并将其与海王星以外的人口的观测限制相结合,计算了进入半人马座区域的物体的通量。这些模拟的初始条件类似于当前的人口。我们通过模拟星子在双曲线轨道上飞过卫星的过程,得到了半人马座与卫星碰撞概率的改进估计,与文献先例一致。我们的天体撞击木星的概率为0.001 yr - 1,比之前的估计低3-6倍。我们的卫星与巨行星的碰撞概率和海王星以外的物体进入半人马座区域的泄漏率都与早期的文献估计一致。然而,我们与巨行星相撞的绝对概率较低。我们将这种差异归因于撞击概率是在包括行星迁移在内的整个太阳系年龄内计算的,还是在更接近现在的更短的间隔内计算的。与早期的文献估计相比,我们的撞击率较低,是因为我们的结果是基于来自海王星以外的物体的通量,而不是依赖于目前观测到的木星撞击率。我们强调在未来的研究中明确说明所有参数和假设的重要性,以便进行有意义的比较。
期刊介绍:
Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.