Author
Listed:
- Sangeetha Nandakumar
(Universidad de Atacama)
- Siegfried Eggl
(University of Illinois at Urbana–Champaign
IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference)
- Jeremy Tregloan-Reed
(Universidad de Atacama
IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference)
- Christian Adam
(Universidad de Antofagasta)
- Jasmine Anderson-Baldwin
(The University of Auckland)
- Michele T. Bannister
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
University of Canterbury)
- Adam Battle
(University of Arizona)
- Zouhair Benkhaldoun
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
Cadi Ayyad University)
- Tanner Campbell
(University of Arizona)
- J. P. Colque
(Universidad de Antofagasta)
- Guillermo Damke
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
NSFs NOIRLab)
- Ilse Plauchu Frayn
(Universidad Nacional Autónoma de Méxic)
- Mourad Ghachoui
(Cadi Ayyad University)
- Pedro F. Guillen
(Universidad Nacional Autónoma de Méxic)
- Aziz Ettahar Kaeouach
(Oukaimeden Observatory)
- Harrison R. Krantz
(University of Arizona Steward Observatory)
- Marco Langbroek
(Delft Technical University)
- Nicholas Rattenbury
(The University of Auckland)
- Vishnu Reddy
(University of Arizona)
- Ryan Ridden-Harper
(University of Canterbury)
- Brad Young
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference)
- Eduardo Unda-Sanzana
(Universidad de Antofagasta)
- Alan M. Watson
(Universidad Nacional Autónoma de México)
- Constance E. Walker
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
NSFs NOIRLab)
- John C. Barentine
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
Dark Sky Consulting, LLC
University of Utah)
- Piero Benvenuti
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
University of Padova)
- Federico Vruno
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
Jodrell Bank)
- Mike W. Peel
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
Instituto de Astrofı́sica de Canarias
Universidad de La Laguna
Imperial College London)
- Meredith L. Rawls
(IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference
University of Washington)
- Cees Bassa
(ASTRON Netherlands Institute for Radio Astronomy)
- Catalina Flores-Quintana
(Universidad Andrés Bello
Instituto Milenio de Astrofísica MAS)
- Pablo García
(Universidad Católica del Norte
National Astronomical Observatories, CAS)
- Sam Kim
(Pontificia Universidad Católica de Chile
Max-Planck-Institut für Astronomie)
- Penélope Longa-Peña
(Universidad de Antofagasta)
- Edgar Ortiz
(Universidad de Atacama)
- Ángel Otarola
(European Southern Observatory (Chile) Alonso de Córdova)
- María Romero-Colmenares
(Universidad de Atacama)
- Pedro Sanhueza
(NSFs NOIRLab)
- Giorgio Siringo
(European Southern Observatory (Chile) Alonso de Córdova
Alonso de Córdova)
- Mario Soto
(Universidad de Atacama)
Abstract
Large constellations of bright artificial satellites in low Earth orbit pose significant challenges to ground-based astronomy1. Current orbiting constellation satellites have brightnesses between apparent magnitudes 4 and 6, whereas in the near-infrared Ks band, they can reach magnitude 2 (ref. 2). Satellite operators, astronomers and other users of the night sky are working on brightness mitigation strategies3,4. Radio emissions induce further potential risk to ground-based radio telescopes that also need to be evaluated. Here we report the outcome of an international optical observation campaign of a prototype constellation satellite, AST SpaceMobile’s BlueWalker 3. BlueWalker 3 features a 64.3 m2 phased-array antenna as well as a launch vehicle adaptor (LVA)5. The peak brightness of the satellite reached an apparent magnitude of 0.4. This made the new satellite one of the brightest objects in the night sky. Additionally, the LVA reached an apparent V-band magnitude of 5.5, four times brighter than the current International Astronomical Union recommendation of magnitude 7 (refs. 3,6); it jettisoned on 10 November 2022 (Universal Time), and its orbital ephemeris was not publicly released until 4 days later. The expected build-out of constellations with hundreds of thousands of new bright objects1 will make active satellite tracking and avoidance strategies a necessity for ground-based telescopes.
Suggested Citation
Sangeetha Nandakumar & Siegfried Eggl & Jeremy Tregloan-Reed & Christian Adam & Jasmine Anderson-Baldwin & Michele T. Bannister & Adam Battle & Zouhair Benkhaldoun & Tanner Campbell & J. P. Colque & G, 2023.
"The high optical brightness of the BlueWalker 3 satellite,"
Nature, Nature, vol. 623(7989), pages 938-941, November.
Handle:
RePEc:nat:nature:v:623:y:2023:i:7989:d:10.1038_s41586-023-06672-7
DOI: 10.1038/s41586-023-06672-7
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