Colección SciELO Chile

Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Búsqueda Publicación
Búsqueda por Tema Título, Abstract y Keywords



The high optical brightness of the BlueWalker 3 satellite
Indexado
WoS WOS:001106758000001
DOI 10.1038/S41586-023-06672-7
Año 2023
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


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.

Revista



Revista ISSN
Nature 0028-0836

Métricas Externas



PlumX Altmetric Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Disciplinas de Investigación



WOS
Multidisciplinary Sciences
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



Ord. Autor Género Institución - País
1 Nandakumar, Sangeetha - Universidad de Atacama - Chile
2 Eggl, Siegfried Hombre UNIV ILLINOIS - Estados Unidos
IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
3 Tregloan-Reed, Jeremy - Universidad de Atacama - Chile
IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
4 Adam, Christian - Universidad de Antofagasta - Chile
5 Anderson-Baldwin, Jasmine - UNIV AUCKLAND - Nueva Zelanda
6 Bannister, Michele T. - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Univ Canterbury - Nueva Zelanda
7 Battle, Adam - UNIV ARIZONA - Estados Unidos
8 Benkhaldoun, Zouhair Hombre IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Cadi Ayyad Univ - Marruecos
9 Campbell, Tanner - UNIV ARIZONA - Estados Unidos
10 Colque, J. P. - Universidad de Antofagasta - Chile
11 Damke, Guillermo - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
NSFs NOIRLab - Estados Unidos
12 Plauchu Frayn, Ilse - Univ Nacl Autonoma Mexico - México
13 Ghachoui, Mourad - Cadi Ayyad Univ - Marruecos
14 Guillen, Pedro F. - Univ Nacl Autonoma Mexico - México
15 Kaeouach, Aziz Ettahar - Oukaimeden Observ - Marruecos
16 Krantz, Harrison R. - UNIV ARIZONA - Estados Unidos
17 Langbroek, Marco - Delft Tech Univ - Países Bajos
18 Rattenbury, Nicholas - UNIV AUCKLAND - Nueva Zelanda
19 Reddy, Vishnu - UNIV ARIZONA - Estados Unidos
20 Ridden-Harper, Ryan - Univ Canterbury - Nueva Zelanda
21 Young, Brad - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
22 Unda-Sanzana, Eduardo - Universidad de Antofagasta - Chile
23 Watson, Alan M. - Univ Nacl Autonoma Mexico - México
24 Walker, Constance E. - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
NSFs NOIRLab - Estados Unidos
25 Barentine, John C. - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Dark Sky Consulting LLC - Estados Unidos
Univ Utah - Estados Unidos
26 Benvenuti, Piero - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Univ Padua - Italia
27 Di Vruno, Federico - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Jodrell Bank - Reino Unido
28 Peel, Mike W. - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
Inst Astrofis Canarias - España
UNIV LA LAGUNA - España
Imperial Coll London - Reino Unido
29 Rawls, Meredith L. - IAU Ctr Protect Dark & Quiet Sky Satellite Conste - Francia
UNIV WASHINGTON - Estados Unidos
30 Bassa, Cees - ASTRON Netherlands Inst Radio Astron - Países Bajos
31 Flores-Quintana, Catalina - Universidad Nacional Andrés Bello - Chile
Inst Milenio Astrofis MAS - Chile
32 Garcia, Pablo - Universidad Católica del Norte - Chile
CASSACA - China
33 Kim, Sam - Pontificia Universidad Católica de Chile - Chile
Max Planck Inst Astron - Alemania
34 Longa-Pena, Penelope A. Mujer Universidad de Antofagasta - Chile
35 Ortiz, Edgar - Universidad de Atacama - Chile
36 Otarola, Angel - European Southern Observ Chile Alonso de Cordova - Chile
37 Romero-Colmenares, Maria - Universidad de Atacama - Chile
38 Sanhueza, Pedro - NSFs NOIRLab - Estados Unidos
39 Siringo, Giorgio - European Southern Observ Chile Alonso de Cordova - Chile
Atacama Large Millimeter Array - Chile
40 Soto, Mario - Universidad de Atacama - Chile

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
CONACYT
Air Force Office of Scientific Research
University of Maryland
ESO-Government of Chile Joint Committee
ANID/FONDECYT
NASA Goddard Space Flight Center
IAU CPS SatHub
Rutherford Discovery Fellowships from New Zealand Government
Universidad Nacional Autonoma de Mexico (Grant CIC)
Universidad Nacional Autonoma de Mexico (Grant DGAPA/PAPIIT)
National Agency for Research and Development (ANID)/Scholarship Program/DOCTORADO BECAS NACIONAL CHILE

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
S.E. and C.E.W. acknowledge the support of the IAU CPS SatHub. S.E. acknowledges D. Stanley for his assistance with satellite ground track generation. J.T.-R. acknowledges financial support from ANID/FONDECYT (an Initiation in Research grant; Project Number 11220287), and this material is based upon work supported by the Air Force Office of Scientific Research (Award FA9550-22-1-0292). C.A. acknowledges the support of the Regional Fund granted by the ESO-Government of Chile Joint Committee. J.A.-B. and M.T.B. acknowledge F. Gunn and I. Bell-Butler for their support in the Otehiwai Mt. John observations. M.T.B. appreciates support from the Rutherford Discovery Fellowships from New Zealand Government funding, administered by the Royal Society Te Aparangi. J.P.C. and E.U-S. acknowledge the assistance of M. Rocchetto and S. Fossey to set up Ckoirama. H.R.K. acknowledges the Steward Observatory Mountain Operations staff for their support at the Mt. Lemmon SkyCenter facility. E.O acknowledges support from the National Agency for Research and Development (ANID)/Scholarship Program/DOCTORADO BECAS NACIONAL CHILE/2018-21190387. Some of the data used in this paper were acquired with the DDOTI instrument at the Observatorio Astronomico Nacional on the Sierra de San Pedro Martir, Baja California, Mexico. DDOTI is funded by CONACyT (Grants LN 232649, LN 260369, LN 271117 and 277901), the Universidad Nacional Autonoma de Mexico (Grants CIC and DGAPA/PAPIIT IG100414, IT102715, AG100317, IN109418, IG100820 and IN105921), the NASA Goddard Space Flight Center and the University of Maryland (Grant NNX17AK54G). DDOTI is operated and maintained by the Observatorio Astronomico Nacional and the Instituto de Astronomia of the Universidad Nacional Autonoma de Mexico. We acknowledge the contribution of N. Gehrels to the development of DDOTI. Part of this work is based on observations at Cerro Tololo Inter-American Observatory, National Science Foundation's NOIRLab, which is managed by the Association of Universities for Research in Astronomy under a cooperative agreement with the National Science Foundation. This research used data from the SMARTS 0.9 m telescope, which is operated as part of the SMARTS Consortium. We acknowledge the substantial time and effort required to carry out this observing campaign, which was voluntarily contributed.

Muestra la fuente de financiamiento declarada en la publicación.