类地行星预测器:机器学习方法

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Jeanne Davoult, Romain Eltschinger, Yann Alibert
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引用次数: 0

摘要

上下文。目前,寻找质量和平衡温度与地球相似的行星是在太阳系外寻找宜居环境的第一步,最终是在宇宙中寻找生命。未来的任务,如行星凌日和恒星振荡或大型系外行星干涉仪,将开始探测和描述这些小而冷的行星,为它们投入大量的观测时间。这项工作的目的是预测哪些恒星最有可能拥有一颗类地行星(ELP),以避免盲目搜索,最小化探测时间,从而最大化探测次数。利用之前关于ELP存在与其系统属性之间相关性的研究,我们训练了一个随机森林来识别和分类系统为“托管ELP”或“不托管ELP”。随机森林在由Bern模型导出的合成行星系统种群上进行训练和测试,然后应用于实际观测系统。在机器学习(ML)模型上进行的测试得出的精度分数高达0.99,这表明该模型识别出的99%具有elp的系统至少具有一个elp。在已被测试的少数几个实际观测到的系统中,有8个被选为具有高概率承载ELP的系统,对这些系统稳定性的快速研究证实,在这些系统中存在一颗类地行星将使它们保持稳定。在机器学习模型上进行的测试获得了出色的结果,证明了它能够识别来自Bern模型的种群中有或没有elp的系统的典型架构。如果我们假设Bern模型充分描述了真实系统的结构,那么在寻找类地行星的过程中,这样的工具将被证明是不可或缺的。类似的方法可以应用于其他行星系统形成模型,以验证这些预测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Earth-like planet predictor: A machine learning approach
Context. Searching for planets analogous to Earth in terms of mass and equilibrium temperature is currently the first step in the quest for habitable conditions outside our Solar System and, ultimately, the search for life in the universe. Future missions such as PLAnetary Transits and Oscillations of stars or Large Interferometer For Exoplanets will begin to detect and characterise these small, cold planets, dedicating significant observation time to them.Aims. The aim of this work is to predict which stars are most likely to host an Earth-like planet (ELP) to avoid blind searches, minimises detection times, and thus maximises the number of detections.Methods. Using a previous study on correlations between the presence of an ELP and the properties of its system, we trained a Random Forest to recognise and classify systems as ‘hosting an ELP’ or ‘not hosting an ELP’. The Random Forest was trained and tested on populations of synthetic planetary systems derived from the Bern model, and then applied to real observed systems.Results. The tests conducted on the machine learning (ML) model yield precision scores of up to 0.99, indicating that 99% of the systems identified by the model as having ELPs possess at least one. Among the few real observed systems that have been tested, eight have been selected as having a high probability of hosting an ELP, and a quick study of the stability of these systems confirms that the presence of an Earth-like planet within them would leave them stable.Conclusions. The excellent results obtained from the tests conducted on the ML model demonstrate its ability to recognise the typical architectures of systems with or without ELPs within populations derived from the Bern model. If we assume that the Bern model adequately describes the architecture of real systems, then such a tool can prove indispensable in the search for Earth-like planets. A similar approach could be applied to other planetary system formation models to validate those predictions.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
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.
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