Determining Fireball Fates Using the α-β Criterion

As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analyzing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide information on positions and, with timing information, velocities. Ho...

Full description

Bibliographic Details
Main Authors: Sansom, Eleanor, Gritsevich, M., Devillepoix, Hadrien, Jansen-Sturgeon, Trent, Shober, Patrick, Bland, Phil, Towner, Martin, Cupak, Martin, Howie, Robert, Hartig, Benjamin
Format: Journal Article
Language:English
Published: IOP PUBLISHING LTD 2019
Subjects:
Online Access:http://purl.org/au-research/grants/arc/DP170102529
http://hdl.handle.net/20.500.11937/90264
_version_ 1848765359608299520
author Sansom, Eleanor
Gritsevich, M.
Devillepoix, Hadrien
Jansen-Sturgeon, Trent
Shober, Patrick
Bland, Phil
Towner, Martin
Cupak, Martin
Howie, Robert
Hartig, Benjamin
author_facet Sansom, Eleanor
Gritsevich, M.
Devillepoix, Hadrien
Jansen-Sturgeon, Trent
Shober, Patrick
Bland, Phil
Towner, Martin
Cupak, Martin
Howie, Robert
Hartig, Benjamin
author_sort Sansom, Eleanor
building Curtin Institutional Repository
collection Online Access
description As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analyzing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide information on positions and, with timing information, velocities. However, extending this pipeline to determine the terminal mass estimate of a meteoroid is a complex next step. Established methods typically require assumptions to be made of the physical meteoroid characteristics (such as shape and bulk density). To determine which meteoroids may have survived entry there are empirical criteria that use a fireball's final height and velocity - low and slow final parameters are likely the best candidates. We review the more elegant approach of the dimensionless coefficient method. Two parameters, α (ballistic coefficient) and β (mass loss), can be calculated for any event with some degree of deceleration, given only velocity and height information. α and β can be used to analytically describe a trajectory with the advantage that they are not mere fitting coefficients; they also represent the physical meteoroid properties. This approach can be applied to any fireball network as an initial identification of key events and determine on which to concentrate resources for more in-depth analyses. We used a set of 278 events observed by the Desert Fireball Network to show how visualization in an α-β diagram can quickly identify which fireballs are likely meteorite candidates.
first_indexed 2025-11-14T11:34:00Z
format Journal Article
id curtin-20.500.11937-90264
institution Curtin University Malaysia
institution_category Local University
language English
last_indexed 2025-11-14T11:34:00Z
publishDate 2019
publisher IOP PUBLISHING LTD
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-902642023-02-22T07:47:43Z Determining Fireball Fates Using the α-β Criterion Sansom, Eleanor Gritsevich, M. Devillepoix, Hadrien Jansen-Sturgeon, Trent Shober, Patrick Bland, Phil Towner, Martin Cupak, Martin Howie, Robert Hartig, Benjamin Science & Technology Physical Sciences Astronomy & Astrophysics Fireballs Meteors Bolides Meteoroids LOST CITY NETWORK METEORITES MASS VELOCITIES ATMOSPHERE INNISFREE EQUATIONS BOLIDES HEIGHT As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analyzing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide information on positions and, with timing information, velocities. However, extending this pipeline to determine the terminal mass estimate of a meteoroid is a complex next step. Established methods typically require assumptions to be made of the physical meteoroid characteristics (such as shape and bulk density). To determine which meteoroids may have survived entry there are empirical criteria that use a fireball's final height and velocity - low and slow final parameters are likely the best candidates. We review the more elegant approach of the dimensionless coefficient method. Two parameters, α (ballistic coefficient) and β (mass loss), can be calculated for any event with some degree of deceleration, given only velocity and height information. α and β can be used to analytically describe a trajectory with the advantage that they are not mere fitting coefficients; they also represent the physical meteoroid properties. This approach can be applied to any fireball network as an initial identification of key events and determine on which to concentrate resources for more in-depth analyses. We used a set of 278 events observed by the Desert Fireball Network to show how visualization in an α-β diagram can quickly identify which fireballs are likely meteorite candidates. 2019 Journal Article http://hdl.handle.net/20.500.11937/90264 10.3847/1538-4357/ab4516 English http://purl.org/au-research/grants/arc/DP170102529 IOP PUBLISHING LTD fulltext
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
Fireballs
Meteors
Bolides
Meteoroids
LOST CITY
NETWORK
METEORITES
MASS
VELOCITIES
ATMOSPHERE
INNISFREE
EQUATIONS
BOLIDES
HEIGHT
Sansom, Eleanor
Gritsevich, M.
Devillepoix, Hadrien
Jansen-Sturgeon, Trent
Shober, Patrick
Bland, Phil
Towner, Martin
Cupak, Martin
Howie, Robert
Hartig, Benjamin
Determining Fireball Fates Using the α-β Criterion
title Determining Fireball Fates Using the α-β Criterion
title_full Determining Fireball Fates Using the α-β Criterion
title_fullStr Determining Fireball Fates Using the α-β Criterion
title_full_unstemmed Determining Fireball Fates Using the α-β Criterion
title_short Determining Fireball Fates Using the α-β Criterion
title_sort determining fireball fates using the α-β criterion
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
Fireballs
Meteors
Bolides
Meteoroids
LOST CITY
NETWORK
METEORITES
MASS
VELOCITIES
ATMOSPHERE
INNISFREE
EQUATIONS
BOLIDES
HEIGHT
url http://purl.org/au-research/grants/arc/DP170102529
http://hdl.handle.net/20.500.11937/90264