The Search for Extraterrestrial Intelligence in Earth's Solar Transit Zone
Ren\'e Heller (1), Ralph E. Pudritz (2,3,4,5) ((1) Max Planck, Institute for Solar System Research, G\"ottingen (GER), (2) Origins, Institute, McMaster U, Hamilton ON (CAN), (3) Department of Physics and, Astronomy, McMaster U, Hamilton ON (CAN), (4) Max Planck Institute for

TL;DR
This paper investigates Earth's transit zone as a target for SETI, identifying potential extraterrestrial observers who could detect Earth and proposing observational strategies for detecting alien signals.
Contribution
It models Earth's transit zone, estimates the number of potential target stars, and highlights the ETZ as an optimal region for SETI efforts using current and upcoming telescopes.
Findings
Approximately 10^5 K and G dwarf stars are in Earth's transit zone.
GAIA can identify all G dwarfs in the ETZ within five years.
The ETZ is an ideal region for targeted SETI searches.
Abstract
Over the past few years, astronomers have detected thousands of planets and candidate planets by observing their periodic transits in front of their host stars. Related methods might soon allow studies of the chemical imprints of life in extrasolar planetary atmospheres. Here, we address the reciprocal question, namely, from where is Earth detectable by extrasolar observers using similar methods. We explore Earth's transit zone (ETZ), the projection of a band around Earth's ecliptic onto the celestial plane, where observers can detect Earth transits across the Sun. The ETZ is between and wide due to the non-circular Earth orbit. The restricted ETZ (rETZ), where Earth transits the Sun less than 0.5 solar radii from its center, is ~ wide. We first compile a target list of 45 K and 37 G dwarf stars inside the rETZ and within 1 kiloparsec (3260…
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