Discovering faint and high apparent motion rate near-Earth asteroids using a deep learning program

Author:

Wang Franklin12ORCID,Ge Jian3,Willis Kevin1

Affiliation:

1. Science Talent Training Center , Gainesville, FL 32606, USA

2. Palo Alto Senior High School , 50 Embarcadero Road, CA 94301, USA

3. Division of Optical Astronomical Instrumentation, Shanghai Astronomical Observatory , 80 Nandan Road, Shanghai 200030, China

Abstract

ABSTRACT Although many near-Earth objects have been found by ground-based telescopes, some fast-moving ones, especially those near detection limits, have been missed by observatories. We developed a convolutional neural network for detecting faint fast-moving near-Earth objects. It was trained with artificial streaks generated from simulations and was able to find these asteroid streaks with an accuracy of 98.7 per cent and a false positive rate of 0.02 per cent on simulated data. This program was used to search image data from the Zwicky Transient Facility (ZTF) in four nights in 2019, and it identified six previously undiscovered asteroids. The visual magnitudes of our detections range from ∼19.0 to 20.3 and motion rates range from ∼6.8 to 24 deg d−1, which is very faint compared to other ZTF detections moving at similar motion rates. Our asteroids are also ∼1–51 m diameter in size and ∼5–60 lunar distances away at close approach, assuming their albedo values follow the albedo distribution function of known asteroids. The use of a purely simulated data set to train our model enables the program to gain sensitivity in detecting faint and fast-moving objects while still being able to recover nearly all discoveries made by previously designed neural networks which used real detections to train neural networks. Our approach can be adopted by any observatory for detecting fast-moving asteroid streaks.

Funder

National Science Foundation

Stockholm University

University of Maryland

University of Washington

Deutsches Elektronen-Synchrotron

Humboldt University

Lawrence Berkeley National Laboratory

International Astronomical Union

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Machine Learning-Based Space Risk Management: Asteroid and Solar Flare Prediction;2024 IEEE 3rd International Conference on Electrical Power and Energy Systems (ICEPES);2024-06-21

2. ICC-BiFormer: A Deep-Learning Model for Near-Earth Asteroid Detection via Image Compression and Local Feature Extraction;Electronics;2024-05-28

3. Classification of Potentially Hazardous Asteroids Using Artificial Neural Networks and Over Sampling Techniques;2023 Global Conference on Information Technologies and Communications (GCITC);2023-12-01

4. Euclid: Identification of asteroid streaks in simulated images using deep learning;Astronomy & Astrophysics;2023-11

5. Representing Source Movement in Sequences of Telescopic Images Based on Contrastive Learning for Asteroid Detection;2023 27th International Computer Science and Engineering Conference (ICSEC);2023-09-14

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3