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The high optical brightness of the BlueWalker 3 satellite.
Nandakumar, Sangeetha; Eggl, Siegfried; Tregloan-Reed, Jeremy; Adam, Christian; Anderson-Baldwin, Jasmine; Bannister, Michele T; Battle, Adam; Benkhaldoun, Zouhair; Campbell, Tanner; Colque, J P; Damke, Guillermo; Plauchu Frayn, Ilse; Ghachoui, Mourad; Guillen, Pedro F; Kaeouach, Aziz Ettahar; Krantz, Harrison R; Langbroek, Marco; Rattenbury, Nicholas; Reddy, Vishnu; Ridden-Harper, Ryan; Young, Brad; Unda-Sanzana, Eduardo; Watson, Alan M; Walker, Constance E; Barentine, John C; Benvenuti, Piero; Di Vruno, Federico; Peel, Mike W; Rawls, Meredith L; Bassa, Cees; Flores-Quintana, Catalina; García, Pablo; Kim, Sam; Longa-Peña, Penélope; Ortiz, Edgar; Otarola, Ángel; Romero-Colmenares, María; Sanhueza, Pedro; Siringo, Giorgio; Soto, Mario.
Afiliación
  • Nandakumar S; Instituto de Investigación en Astronomía y Ciencias Planetarias, Universidad de Atacama, Copiapó, Chile. an.sangeetha@gmail.com.
  • Eggl S; Department of Aerospace Engineering/Department of Astronomy, University of Illinois at Urbana-Champaign, Champaign, IL, USA. eggl@illinois.edu.
  • Tregloan-Reed J; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France. eggl@illinois.edu.
  • Adam C; Instituto de Investigación en Astronomía y Ciencias Planetarias, Universidad de Atacama, Copiapó, Chile. jeremy.tregloan-reed@uda.cl.
  • Anderson-Baldwin J; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France. jeremy.tregloan-reed@uda.cl.
  • Bannister MT; Centro de Astronomía (CITEVA), Universidad de Antofagasta, Antofagasta, Chile.
  • Battle A; The University of Auckland, Auckland, New Zealand.
  • Benkhaldoun Z; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Campbell T; School of Physical and Chemical Sciences Te Kura Matu, University of Canterbury, Christchurch, New Zealand.
  • Colque JP; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Damke G; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Plauchu Frayn I; Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Marrakesh, Morocco.
  • Ghachoui M; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Guillen PF; Centro de Astronomía (CITEVA), Universidad de Antofagasta, Antofagasta, Chile.
  • Kaeouach AE; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Krantz HR; NSFs NOIRLab, Tucson, AZ, USA.
  • Langbroek M; Instituto de Astronomía, Universidad Nacional Autónoma de Méxic, Ensenada, Mexico.
  • Rattenbury N; Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Marrakesh, Morocco.
  • Reddy V; Instituto de Astronomía, Universidad Nacional Autónoma de Méxic, Ensenada, Mexico.
  • Ridden-Harper R; High Atlas Observatory, Oukaimeden Observatory, Oukaimeden, Morocco.
  • Young B; University of Arizona Steward Observatory, Tucson, AZ, USA.
  • Unda-Sanzana E; Faculty of Aerospace Engineering, Delft Technical University, Delft, The Netherlands.
  • Watson AM; The University of Auckland, Auckland, New Zealand.
  • Walker CE; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Barentine JC; School of Physical and Chemical Sciences Te Kura Matu, University of Canterbury, Christchurch, New Zealand.
  • Benvenuti P; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Di Vruno F; Centro de Astronomía (CITEVA), Universidad de Antofagasta, Antofagasta, Chile.
  • Peel MW; Instituto de Astronomiía, Universidad Nacional Autónoma de México, Mexico City, Mexico.
  • Rawls ML; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Bassa C; NSFs NOIRLab, Tucson, AZ, USA.
  • Flores-Quintana C; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • García P; Dark Sky Consulting, LLC, Tucson, AZ, USA.
  • Kim S; Consortium for Dark Sky Studies, University of Utah, Salt Lake City, UT, USA.
  • Longa-Peña P; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Ortiz E; Department of Astronomy, University of Padova, Padova, Italy.
  • Otarola Á; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Romero-Colmenares M; SKA Observatory, Jodrell Bank, Macclesfield, UK.
  • Sanhueza P; IAU Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference, Paris, France.
  • Siringo G; Instituto de Astrofísica de Canarias, La Laguna, Spain.
  • Soto M; Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain.
Nature ; 623(7989): 938-941, 2023 Nov.
Article en En | MEDLINE | ID: mdl-37783227
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.

Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Nature Año: 2023 Tipo del documento: Article País de afiliación: Chile

Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Nature Año: 2023 Tipo del documento: Article País de afiliación: Chile