Harnessing the Power of Convolutional Neural Network for Exoplanet Discovery

None Gaurav, Sumit Gupta
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Abstract

The discovery of planets apart from Earth that can sustain lives has always been fascinating as well as challenging. Discussion around such planets, popularly termed as "Exoplanets" have been doing the rounds for quite some time now. These exoplanets are often considered to be "Earth-like" or "habitable" because they may have conditions that could potentially support life. This work focuses on how Deep Learning techniques can be useful in identifying potential exoplanets. To do so, astronomical data gathered by space telescopes such as Kepler and BRITE have been utilized. The method employed to detect exoplanets is Transit Photometry along with Convolutional Neural Network. The study highlights the limitations of small training datasets and suggests the use of data augmentation techniques to increase the size of the training dataset, and the transfer learning approach to improve the performance of the classification models. The research offers valuable insights into the nature and diversity of exoplanets and may open avenues for future discoveries. With a performance accuracy of 96.67%, the proposed approach showcases merit and hence can prove to be a harbinger in exploring planetary habitability in the colossal space.
利用卷积神经网络的力量发现系外行星
发现地球以外可以维持生命的行星一直是令人着迷的,也是具有挑战性的。关于这类行星的讨论,通常被称为“系外行星”,已经进行了相当长一段时间了。这些系外行星通常被认为是“类地”或“宜居”的,因为它们可能具有可能支持生命的条件。这项工作的重点是深度学习技术如何在识别潜在的系外行星方面发挥作用。为了做到这一点,利用了开普勒和BRITE等太空望远镜收集的天文数据。探测系外行星的方法是凌日光度法和卷积神经网络。该研究强调了小型训练数据集的局限性,并建议使用数据增强技术来增加训练数据集的大小,并使用迁移学习方法来提高分类模型的性能。这项研究为了解系外行星的性质和多样性提供了有价值的见解,并可能为未来的发现开辟道路。该方法的性能精度为96.67%,显示了其优点,因此可以被证明是在巨大空间中探索行星可居住性的先驱。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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