地球に異星信号が届いていた場合、なぜ私たちは観測できていないのか (If alien signals reached Earth, why haven’t we seen them?)

2026-02-16 スイス連邦工科大学ローザンヌ校(EPFL)

スイス連邦工科大学ローザンヌ校(EPFL)の研究者らは、地球外文明からの信号が地球に届いていても観測されない理由を理論的に検討した。電波信号は宇宙空間で拡散・減衰し、発信源が遠距離や短命な文明である場合、現在の観測技術では検出が極めて困難になる。また、文明の発信期間が宇宙時間尺度で短ければ、地球と同時期に存在する確率も低い。銀河内に多数の文明が存在しても、距離、時間的重なり、技術的制約が重なり合い「見えない」状況が生じ得るとし、フェルミのパラドックスに新たな定量的視点を与えている。

<関連情報>

技術的種族との未検出の過去の接触:テクノシグネチャー科学への影響 Undetected Past Contacts with Technological Species: Implications for Technosignature Science

Claudio Grimaldi
The Astronomical Journal  Published: 2026 February 16
DOI:10.3847/1538-3881/ae394b

地球に異星信号が届いていた場合、なぜ私たちは観測できていないのか (If alien signals reached Earth, why haven’t we seen them?)

Abstract

In the search for extraterrestrial intelligence (SETI), the highly incomplete sampling of the technosignature search space is often considered as a plausible explanation for the persistent lack of detections over six decades of searches. If correct, this would imply that technosignatures may already have reached Earth without being detected or correctly identified. Here, we explore this possibility using a Bayesian inference framework to estimate present-day detectability given n ≥ 1 undetected contacts over the past 65 yr—the period since the first SETI experiment. We show that achieving high detectability of technosignatures emitted within a few hundred light-years of Earth would require implausibly large n values, even exceeding the population of habitable planets within that range. More conservative estimates can be obtained only assuming that emitters are tightly clustered near Earth or that their population in the Milky Way has undergone a very recent and sudden boost. This tension is further exacerbated for short-lived technosignatures and persists whether they are omnidirectional, as in Dysonian megastructures, or directional, as in intentional communication attempts. These findings suggest that, if undetected past contacts from the Milky Way have indeed occurred, the best prospects of detection may lie in searches extending over several thousand light years, though only a few detectable technoemissions would be expected.

1701物理及び化学
ad
ad
Follow
ad
タイトルとURLをコピーしました