The Scientific Investigation of Unidentified Aerial Phenomena (UAP) Using Multimodal Ground-Based Observatories

Author:

Watters Wesley Andrés12,Loeb Abraham23,Laukien Frank24,Cloete Richard25ORCID,Delacroix Alex26,Dobroshinsky Sergei2,Horvath Benjamin2,Kelderman Ezra2,Little Sarah27,Masson Eric2,Mead Andrew2,Randall Mitch28,Schultz Forrest29,Szenher Matthew2,Vervelidou Foteini210,White Abigail25,Ahlström Angelique2,Cleland Carol211,Dockal Spencer12,Donahue Natasha212,Elowitz Mark2,Ezell Carson2,Gersznowicz Alex2,Gold Nicholas2,Hercz Michael G.2,Keto Eric25,Knuth Kevin H.213,Lux Anthony2,Melnick Gary J.25,Moro-Martín Amaya21415,Martin-Torres Javier21617,Ribes Daniel Llusa2,Sail Paul2,Teodorani Massimo2,Tedesco John Joseph2,Tedesco Gerald Thomas2,Tu Michelle12,Zorzano Maria-Paz218

Affiliation:

1. Whitin Observatory, Department of Astronomy, Wellesley College, 106 Central St. Wellesley, MA, USA 02481

2. Galileo Project, 60 Garden Street, Cambridge, MA, USA 02138

3. Department of Astronomy, Harvard University, 60 Garden Street, Cambridge, MA, USA 02138

4. Department of Chemistry and Chemical Biology, Harvard University, 12 Oxford Street Cambridge, MA, USA 02138

5. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA, USA 02138

6. Caltech Optical Observatory, Pasadena, CA, USA 91125

7. Scientific Coalition for UAP Studies, Fort Myers, FL, USA 33913

8. Ascendant AI, Boulder, CO, USA 80304

9. Atlas Lens Co., Glendale, CA, USA 91201

10. Department of Earth, Atmospheric, & Planetary Sciences, Massachusetts Institute of Technology Cambridge, MA, USA 02139

11. Department of Philosophy, Center for the Study of Origins, University of Colorado Boulder Boulder, CO, USA 80309

12. Athabasca University, Centre for Science, 1 University Dr., Athabasca, AB, Canada T9S 3A3

13. Department of Physics, State University of New York at Albany 1400 Washington Avenue, Albany, NY, USA 12222

14. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, USA 21218

15. Department of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles Street Baltimore, MD, USA 21218

16. Department of Planetary Sciences, School of Geosciences, University of Aberdeen Meston Building, Aberdeen, Scotland, UK AB24 3UE

17. Instituto Andaluz de Ciencias de la Tierra (UGR-CSIC), Av. de las Palmeras 4, 18100 Armilla, Granada, Spain

18. Centro de Astrobiología (CSIC-INTA), Madrid, Spain

Abstract

Unidentified Aerial Phenomena (UAP) have resisted explanation and have received little formal scientific attention for 75 years. A primary objective of the Galileo Project is to build an integrated software and instrumentation system designed to conduct a multimodal census of aerial phenomena and to recognize anomalies. Here we present key motivations for the study of UAP and address historical objections to this research. We describe an approach for highlighting outlier events in the high-dimensional parameter space of our census measurements. We provide a detailed roadmap for deciding measurement requirements, as well as a science traceability matrix (STM) for connecting sought-after physical parameters to observables and instrument requirements. We also discuss potential strategies for deciding where to locate instruments for development, testing, and final deployment. Our instrument package is multimodal and multispectral, consisting of (1) wide-field cameras in multiple bands for targeting and tracking of aerial objects and deriving their positions and kinematics using triangulation; (2) narrow-field instruments including cameras for characterizing morphology, spectra, polarimetry, and photometry; (3) passive multistatic arrays of antennas and receivers for radar-derived range and kinematics; (4) radio spectrum analyzers to measure radio and microwave emissions; (5) microphones for sampling acoustic emissions in the infrasonic through ultrasonic frequency bands; and (6) environmental sensors for characterizing ambient conditions (temperature, pressure, humidity, and wind velocity), as well as quasistatic electric and magnetic fields, and energetic particles. The use of multispectral instruments and multiple sensor modalities will help to ensure that artifacts are recognized and that true detections are corroborated and verifiable. Data processing pipelines are being developed that apply state-of-the-art techniques for multi-sensor data fusion, hypothesis tracking, semi-supervised classification, and outlier detection.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Instrumentation

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