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Rio 2.0: revising the Rio scale for SETI detections

Authors :
Duncan Forgan
Eric J. Korpela
Elisabeth Piotelat
Jill Tarter
Jason T. Wright
Iván Almár
Andrew Siemion
SUPA School of Physics and Astronomy [University of St Andrews]
University of St Andrews [Scotland]-Scottish Universities Physics Alliance (SUPA)
Center for Exoplanets and Habitable World (CEHW)
Pennsylvania State University (Penn State)
Penn State System-Penn State System
Breakthrough Listen Laboratory
SETI Institute
Space Sciences Laboratory [Berkeley] (SSL)
University of California [Berkeley]
University of California-University of California
Department of Astronomy [Berkeley]
Radboud university [Nijmegen]
Konkoly Observatory
Research Centre for Astronomy and Earth Sciences [Budapest]
Hungarian Academy of Sciences (MTA)-Hungarian Academy of Sciences (MTA)
Laboratoire d'Informatique pour la Mécanique et les Sciences de l'Ingénieur (LIMSI)
Université Paris Saclay (COmUE)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université - UFR d'Ingénierie (UFR 919)
Sorbonne Université (SU)-Sorbonne Université (SU)-Université Paris-Saclay-Université Paris-Sud - Paris 11 (UP11)
European Research Council
University of St Andrews. School of Physics and Astronomy
University of St Andrews. St Andrews Centre for Exoplanet Science
Source :
International Journal of Astrobiology, International Journal of Astrobiology, Cambridge University Press (CUP), 2018, pp.1-9. ⟨10.1017/S1473550418000162⟩
Publication Year :
2018
Publisher :
Cambridge University Press (CUP), 2018.

Abstract

DHF gratefully acknowledges support from the ECOGAL project, grant agreement 291227, funded by the European Research Council under ERC-2011-ADG. The Center for Exoplanets and Habitable Worlds is supported by the Pennsylvania State University, the Eberly College of Science, and the Pennsylvania Space Grant Consortium. The Rio scale is a tool for communicating the significance of a signal to the general public. It assigns scores to signals detected in searches for extraterrestrial intelligence (SETI), which characterizes both the consequences of a signal and the probability the signal is truly from ETI, in an easily digestible format for laypeople to interpret. In the 17 years since its construction, the number of groups actively conducting searches for evidence of intelligent life beyond the Earth has increased significantly, and theoretical work has established a new suite of observables that are capable of revealing the presence of ETI in a range of astronomical observations. In this paper, we revise the Rio scale, with the aim of (i) achieving consensus across academic disciplines on a scheme for classifying signals potentially indicating the existence of advanced extraterrestrial life, (ii) supplying a pedagogical tool to help inform the public about the process scientists go through to develop an understanding of a signal and (iii) providing a means of calibrating the expectations of the world at large when signals are discussed in the media. We also present (and encourage the SETI community to adopt) a single set of consistent terminology for discussing signals. Postprint

Details

ISSN :
14753006 and 14735504
Volume :
18
Database :
OpenAIRE
Journal :
International Journal of Astrobiology
Accession number :
edsair.doi.dedup.....7be2fa13516cc706f8dd481cdaf345ae