A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite

We report the detection of a burst of emission over a 695.5–1031.5 MHz bandwidth by the Australian Square Kilometre Array Pathfinder. The burst was localized through analysis of near-field time delays to the long-decommissioned Relay 2 satellite and exhibited a dispersion measure of 2.26 × 10 ^−5 pc...

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Main Authors: C. W. James, A. T. Deller, T. Dial, M. Glowacki, S. J. Tingay, K. W. Bannister, A. Bera, N. D. R. Bhat, R. D. Ekers, V. Gupta, A. Jaini, J. Morgan, J. N. Jahns-Schindler, R. M. Shannon, M. Sukhov, J. Tuthill, Z. Wang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/ade3d3
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author C. W. James
A. T. Deller
T. Dial
M. Glowacki
S. J. Tingay
K. W. Bannister
A. Bera
N. D. R. Bhat
R. D. Ekers
V. Gupta
A. Jaini
J. Morgan
J. N. Jahns-Schindler
R. M. Shannon
M. Sukhov
J. Tuthill
Z. Wang
author_facet C. W. James
A. T. Deller
T. Dial
M. Glowacki
S. J. Tingay
K. W. Bannister
A. Bera
N. D. R. Bhat
R. D. Ekers
V. Gupta
A. Jaini
J. Morgan
J. N. Jahns-Schindler
R. M. Shannon
M. Sukhov
J. Tuthill
Z. Wang
author_sort C. W. James
collection DOAJ
description We report the detection of a burst of emission over a 695.5–1031.5 MHz bandwidth by the Australian Square Kilometre Array Pathfinder. The burst was localized through analysis of near-field time delays to the long-decommissioned Relay 2 satellite and exhibited a dispersion measure of 2.26 × 10 ^−5 pc cm ^−3 —69.7 total electron content units, consistent with expectations for a single pass through the ionosphere. After coherent dedispersion, the burst was determined to be less than 30 ns in width, with an average flux density of at least 300 kJy. We consider an electrostatic discharge (ESD) or plasma discharge following a micrometeoroid impact to be plausible explanations for the burst. ESDs have previously been observed with the Arecibo radio telescope, but on 1000 times longer timescales. Our observation opens new possibilities for the remote sensing of ESD, which poses a serious threat to spacecraft, and reveals a new source of false events for observations of astrophysical transients.
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series The Astrophysical Journal Letters
spelling doaj-art-39c07d36f4e54f85ab5e07d8d2dc40ee2025-08-20T03:29:57ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019871L1610.3847/2041-8213/ade3d3A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 SatelliteC. W. James0https://orcid.org/0000-0002-6437-6176A. T. Deller1https://orcid.org/0000-0001-9434-3837T. Dial2https://orcid.org/0009-0004-1205-8805M. Glowacki3https://orcid.org/0000-0002-5067-8894S. J. Tingay4https://orcid.org/0000-0002-8195-7562K. W. Bannister5https://orcid.org/0000-0003-2149-0363A. Bera6https://orcid.org/0000-0002-2864-4110N. D. R. Bhat7https://orcid.org/0000-0002-8383-5059R. D. Ekers8https://orcid.org/0000-0002-3532-9928V. Gupta9https://orcid.org/0000-0001-9817-4938A. Jaini10https://orcid.org/0000-0002-8987-1544J. Morgan11https://orcid.org/0000-0001-9224-5483J. N. Jahns-Schindler12https://orcid.org/0000-0003-4193-6158R. M. Shannon13https://orcid.org/0000-0002-7285-6348M. Sukhov14https://orcid.org/0009-0004-6311-2859J. Tuthill15https://orcid.org/0000-0002-7551-2073Z. Wang16https://orcid.org/0000-0002-2066-9823International Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.auCentre for Astrophysics and Supercomputing, Swinburne University of Technology , John St., Hawthorn, VIC 3122, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , John St., Hawthorn, VIC 3122, AustraliaInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.au; Institute for Astronomy, University of Edinburgh , Royal Observatory, Edinburgh EH9 3HJ, UK; Inter-University Institute for Data Intensive Astronomy, Department of Astronomy, University of Cape Town , Cape Town, South AfricaInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.auAustralia Telescope National Facility , CSIRO, Space and Astronomy, P.O. Box 76, Epping, NSW 1710, Australia; Sydney Institute for Astronomy, School of Physics, University of Sydney , NSW 2006, AustraliaInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.auInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.auInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.au; Australia Telescope National Facility , CSIRO, Space and Astronomy, P.O. Box 76, Epping, NSW 1710, AustraliaAustralia Telescope National Facility , CSIRO, Space and Astronomy, P.O. Box 76, Epping, NSW 1710, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, AustraliaCSIRO Space and Astronomy , P.O. Box 1130, Bentley, WA 6102, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, Australia; ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) , Hawthorn, VIC 3122, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, Australia; ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) , Hawthorn, VIC 3122, AustraliaSchool of Science, Royal Melbourne Institute of Technology , Melbourne, VIC 3000, AustraliaAustralia Telescope National Facility , CSIRO, Space and Astronomy, P.O. Box 76, Epping, NSW 1710, AustraliaInternational Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102, Australia ; clancy.james@curtin.edu.auWe report the detection of a burst of emission over a 695.5–1031.5 MHz bandwidth by the Australian Square Kilometre Array Pathfinder. The burst was localized through analysis of near-field time delays to the long-decommissioned Relay 2 satellite and exhibited a dispersion measure of 2.26 × 10 ^−5 pc cm ^−3 —69.7 total electron content units, consistent with expectations for a single pass through the ionosphere. After coherent dedispersion, the burst was determined to be less than 30 ns in width, with an average flux density of at least 300 kJy. We consider an electrostatic discharge (ESD) or plasma discharge following a micrometeoroid impact to be plausible explanations for the burst. ESDs have previously been observed with the Arecibo radio telescope, but on 1000 times longer timescales. Our observation opens new possibilities for the remote sensing of ESD, which poses a serious threat to spacecraft, and reveals a new source of false events for observations of astrophysical transients.https://doi.org/10.3847/2041-8213/ade3d3Time domain astronomyRadio transient sourcesArtificial satellites
spellingShingle C. W. James
A. T. Deller
T. Dial
M. Glowacki
S. J. Tingay
K. W. Bannister
A. Bera
N. D. R. Bhat
R. D. Ekers
V. Gupta
A. Jaini
J. Morgan
J. N. Jahns-Schindler
R. M. Shannon
M. Sukhov
J. Tuthill
Z. Wang
A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
The Astrophysical Journal Letters
Time domain astronomy
Radio transient sources
Artificial satellites
title A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
title_full A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
title_fullStr A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
title_full_unstemmed A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
title_short A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite
title_sort nanosecond duration radio pulse originating from the defunct relay 2 satellite
topic Time domain astronomy
Radio transient sources
Artificial satellites
url https://doi.org/10.3847/2041-8213/ade3d3
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