A Proposal for Enhancing Technosignature Search toward the Galactic Center

We discuss the possibility of enhancing intelligent life searches toward the Galactic center. From the clockwork orbital motions of stars around the Sgr A* black hole, we can determine the distance to the Galactic center at an exceptional accuracy, despite its remoteness ∼8.3 kpc. In addition, we ca...

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Main Author: Naoki Seto
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad2a48
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author Naoki Seto
author_facet Naoki Seto
author_sort Naoki Seto
collection DOAJ
description We discuss the possibility of enhancing intelligent life searches toward the Galactic center. From the clockwork orbital motions of stars around the Sgr A* black hole, we can determine the distance to the Galactic center at an exceptional accuracy, despite its remoteness ∼8.3 kpc. In addition, we can define precise reference epochs by selecting a prominent object such as the bright B-type star S2. These properties have a particular affinity for the coordinated signaling scheme that was hypothesized by Seto for systematically connecting intentional senders to searchers without a prior communication. If S2 is actually being used as a common reference clock, we can compress the search directions around the Galactic center by more than 2 orders of magnitude, with the scanning interval of ∼16 yr.
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spelling doaj.art-72e96963d8e34c56a19e740e024c1ae42024-03-21T09:01:28ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01964210510.3847/1538-4357/ad2a48A Proposal for Enhancing Technosignature Search toward the Galactic CenterNaoki Seto0https://orcid.org/0000-0001-6521-4235Department of Physics, Kyoto University , Kyoto 606-8502, Japan ; seto@tap.scphys.kyoto-u.ac.jpWe discuss the possibility of enhancing intelligent life searches toward the Galactic center. From the clockwork orbital motions of stars around the Sgr A* black hole, we can determine the distance to the Galactic center at an exceptional accuracy, despite its remoteness ∼8.3 kpc. In addition, we can define precise reference epochs by selecting a prominent object such as the bright B-type star S2. These properties have a particular affinity for the coordinated signaling scheme that was hypothesized by Seto for systematically connecting intentional senders to searchers without a prior communication. If S2 is actually being used as a common reference clock, we can compress the search directions around the Galactic center by more than 2 orders of magnitude, with the scanning interval of ∼16 yr.https://doi.org/10.3847/1538-4357/ad2a48Search for extraterrestrial intelligenceAstrobiologyGalactic center
spellingShingle Naoki Seto
A Proposal for Enhancing Technosignature Search toward the Galactic Center
The Astrophysical Journal
Search for extraterrestrial intelligence
Astrobiology
Galactic center
title A Proposal for Enhancing Technosignature Search toward the Galactic Center
title_full A Proposal for Enhancing Technosignature Search toward the Galactic Center
title_fullStr A Proposal for Enhancing Technosignature Search toward the Galactic Center
title_full_unstemmed A Proposal for Enhancing Technosignature Search toward the Galactic Center
title_short A Proposal for Enhancing Technosignature Search toward the Galactic Center
title_sort proposal for enhancing technosignature search toward the galactic center
topic Search for extraterrestrial intelligence
Astrobiology
Galactic center
url https://doi.org/10.3847/1538-4357/ad2a48
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