{"title":"Experimental analysis and machine learning-based recognition of multiscale solid particles moving in gas","authors":"I. Doroshchenko, I. Znamenskaya, N. Sysoev","doi":"10.1016/j.actaastro.2025.09.091","DOIUrl":null,"url":null,"abstract":"<div><div>The rapid growth of artificial objects in Earth orbit poses increasing risks to satellites, human missions, and the long-term sustainability of space operations. Uncontrolled collisions with such fragments can damage spacecraft, threaten human missions, and jeopardize the long-term safety of spaceflight operations. Detecting and characterizing small debris—particularly in the sub-millimeter to millimeter range—remains a major challenge as far as small particles size lies below the effective resolution of most ground-based radar and optical systems. To address this, we present an integrated experimental–computational framework that combines high-speed flow visualization with machine learning–based recognition. Shock tube experiments at rarified air flow velocities from 50 up to 900 m/s were used to reproduce conditions representative of particle motion. Particle dynamics were recorded using high-speed shadowgraphy and processed through two complementary pipelines: a contour-based algorithm extracting geometric parameters (width, height, area) together with average brightness relative to the background, and a YOLOv11 deep learning model trained on annotated datasets for real-time particle detection and trajectory reconstruction. The method enables automated generation of particle size distributions, brightness statistics, x–t diagrams, and velocity–time profiles for particles in the 10 μm–5 mm range. The novelty of this work lies in combining high-speed laboratory shadowgraphy with both classical computer vision and deep learning methods, enabling simultaneous extraction of geometric, optical, and kinematic particle characteristics with direct relevance to orbital debris studies. By linking controlled laboratory experiments with scalable computer vision tools, this approach provides a basis for studying fine-particle debris dynamics, validating flow models, and advancing space situational awareness capabilities for debris detection and mitigation.</div></div>","PeriodicalId":44971,"journal":{"name":"Acta Astronautica","volume":"238 ","pages":"Pages 1030-1039"},"PeriodicalIF":3.4000,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Astronautica","FirstCategoryId":"5","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S009457652500668X","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ENGINEERING, AEROSPACE","Score":null,"Total":0}
引用次数: 0
Abstract
The rapid growth of artificial objects in Earth orbit poses increasing risks to satellites, human missions, and the long-term sustainability of space operations. Uncontrolled collisions with such fragments can damage spacecraft, threaten human missions, and jeopardize the long-term safety of spaceflight operations. Detecting and characterizing small debris—particularly in the sub-millimeter to millimeter range—remains a major challenge as far as small particles size lies below the effective resolution of most ground-based radar and optical systems. To address this, we present an integrated experimental–computational framework that combines high-speed flow visualization with machine learning–based recognition. Shock tube experiments at rarified air flow velocities from 50 up to 900 m/s were used to reproduce conditions representative of particle motion. Particle dynamics were recorded using high-speed shadowgraphy and processed through two complementary pipelines: a contour-based algorithm extracting geometric parameters (width, height, area) together with average brightness relative to the background, and a YOLOv11 deep learning model trained on annotated datasets for real-time particle detection and trajectory reconstruction. The method enables automated generation of particle size distributions, brightness statistics, x–t diagrams, and velocity–time profiles for particles in the 10 μm–5 mm range. The novelty of this work lies in combining high-speed laboratory shadowgraphy with both classical computer vision and deep learning methods, enabling simultaneous extraction of geometric, optical, and kinematic particle characteristics with direct relevance to orbital debris studies. By linking controlled laboratory experiments with scalable computer vision tools, this approach provides a basis for studying fine-particle debris dynamics, validating flow models, and advancing space situational awareness capabilities for debris detection and mitigation.
期刊介绍:
Acta Astronautica is sponsored by the International Academy of Astronautics. Content is based on original contributions in all fields of basic, engineering, life and social space sciences and of space technology related to:
The peaceful scientific exploration of space,
Its exploitation for human welfare and progress,
Conception, design, development and operation of space-borne and Earth-based systems,
In addition to regular issues, the journal publishes selected proceedings of the annual International Astronautical Congress (IAC), transactions of the IAA and special issues on topics of current interest, such as microgravity, space station technology, geostationary orbits, and space economics. Other subject areas include satellite technology, space transportation and communications, space energy, power and propulsion, astrodynamics, extraterrestrial intelligence and Earth observations.