Towards a definition of a meteor cluster

Context. As of today, there is no official definition of a meteor cluster. It is usually identified as a large number of meteors sharing a similar radiant and velocity, all occurring within a few seconds. Only eight clusters have been reported so far, from single-camera or camera network observations. However, a cluster may be observed by several distant networks and remain unnoticed simply because each network is recording a small portion of the cluster. Aims. We aim to provide an overview of meteor clusters to help define what constitutes a cluster by potentially adding more to the already identified ones and determining their common parameters. Methods. A search for new clusters was performed in publicly available International Astronomical Union meteor databases with the DBSCAN algorithm. Then, a statistical significance method was applied to derive the most promising cluster candidates. However, the method still lacks a way to debias the atmospheric area surveyed by the cameras due to a lack of publicly available data. Results. A set of 16 statistically significant potential clusters is identified, involving four to seven fragments. The 90th percentile includes a duration of 8 seconds, a velocity difference of 2.2 km/s, and a radiant spread of nearly 4 degrees. The velocity difference may arise from the method used for orbit computation. Conclusions. Meteor clusters might be more frequent than currently reported. However, we recommend that future meteor orbit databases also include a way to estimate the surveyed area by the cameras involved in the detection. This would strengthen the veracity of the 16 identified cluster candidates and ultimately allow scientists to fully debias the number of clusters, and hence derive the physical lifetime expectancy of meteoroids, which is often overlooked due to the focus on collisional lifetime estimates only. We also recommend that any future cluster observation report include the expected number of random occurrences and consider the event to be real if this value is below 0.1.

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-04-04
DOI
https://doi.org/10.1051/0004-6361/202452445/pdf
Primary Topic
Mycorrhizal Fungi and Plant Interactions
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Towards a definition of a meteor cluster

Springer Link (Chiba Institute of Technology)
Mycorrhizal Fungi and Plant Interactions
article

Towards a definition of a meteor cluster

article en

Abstract

Context. As of today, there is no official definition of a meteor cluster. It is usually identified as a large number of meteors sharing a similar radiant and velocity, all occurring within a few seconds. Only eight clusters have been reported so far, from single-camera or camera network observations. However, a cluster may be observed by several distant networks and remain unnoticed simply because each network is recording a small portion of the cluster. Aims. We aim to provide an overview of meteor clusters to help define what constitutes a cluster by potentially adding more to the already identified ones and determining their common parameters. Methods. A search for new clusters was performed in publicly available International Astronomical Union meteor databases with the DBSCAN algorithm. Then, a statistical significance method was applied to derive the most promising cluster candidates. However, the method still lacks a way to debias the atmospheric area surveyed by the cameras due to a lack of publicly available data. Results. A set of 16 statistically significant potential clusters is identified, involving four to seven fragments. The 90th percentile includes a duration of 8 seconds, a velocity difference of 2.2 km/s, and a radiant spread of nearly 4 degrees. The velocity difference may arise from the method used for orbit computation. Conclusions. Meteor clusters might be more frequent than currently reported. However, we recommend that future meteor orbit databases also include a way to estimate the surveyed area by the cameras involved in the detection. This would strengthen the veracity of the 16 identified cluster candidates and ultimately allow scientists to fully debias the number of clusters, and hence derive the physical lifetime expectancy of meteoroids, which is often overlooked due to the focus on collisional lifetime estimates only. We also recommend that any future cluster observation report include the expected number of random occurrences and consider the event to be real if this value is below 0.1.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 54%
Mycorrhizal Fungi and Plant Interactions
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Towards a definition of a meteor cluster · Springer Link (Chiba Institute of Technology) (2025) | TGRS Research Map | TGRS