TY - JOUR
T1 - Search for an Alien Message to a Nearby Star
AU - Gillon, Michaël
AU - Burdanov, Artem
AU - Wright, Jason T.
N1 - Publisher Copyright:
© 2022. The Author(s). Published by the American Astronomical Society.
PY - 2022/11/1
Y1 - 2022/11/1
N2 - If alien probes have colonized the whole galaxy, they could have formed an efficient galactic-scale communication network by establishing direct gravitationally lensed links between neighboring systems. Under this scenario, observing the positions opposite the nearest ecliptic stars represents a promising artifact SETI strategy that could make it possible to “eavesdrop” on the emission of local probes to one of these stars. In this context, we present here a first attempt to detect optical messages emitted from the solar system to the ecliptic star Wolf 359, the third-nearest stellar system, based on observations gathered by the TRAPPIST-South and SPECULOOS-South robotic telescopes. While sensitive enough to detect constant emission with emitting power as small as a few watts, this search led to a null result. We note that the putative alien probes could be emitting “off-axis” and be located much closer to the Sun than the start of the “solar gravitational line” at 550 au. We performed a search for such an off-axis emitter in our data, whose result turned out negative too.
AB - If alien probes have colonized the whole galaxy, they could have formed an efficient galactic-scale communication network by establishing direct gravitationally lensed links between neighboring systems. Under this scenario, observing the positions opposite the nearest ecliptic stars represents a promising artifact SETI strategy that could make it possible to “eavesdrop” on the emission of local probes to one of these stars. In this context, we present here a first attempt to detect optical messages emitted from the solar system to the ecliptic star Wolf 359, the third-nearest stellar system, based on observations gathered by the TRAPPIST-South and SPECULOOS-South robotic telescopes. While sensitive enough to detect constant emission with emitting power as small as a few watts, this search led to a null result. We note that the putative alien probes could be emitting “off-axis” and be located much closer to the Sun than the start of the “solar gravitational line” at 550 au. We performed a search for such an off-axis emitter in our data, whose result turned out negative too.
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U2 - 10.3847/1538-3881/ac9610
DO - 10.3847/1538-3881/ac9610
M3 - Article
AN - SCOPUS:85141718099
SN - 0004-6256
VL - 164
JO - Astronomical Journal
JF - Astronomical Journal
IS - 5
M1 - 221
ER -