WISE探测到盖亚-2MASS选择的恒星周围的戴森球/结构了吗?

Andrew W. Blain
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引用次数: 0

摘要

在包含 5 亿个中红外(IR)天体的 WISE 全天空天体目录发布后不久,就有人提出可以利用它来搜寻由先进文明建造的太阳系外装置,以便将其宿主恒星光度的很大一部分转化为有用的工作:这些装置包括 "技术结构"、"巨型结构 "或 "戴森球/结构"(以下简称 "DSM")。然而,从几百万颗可能适合居住的盖亚探测到的恒星中寻找中红外超标信号是充满危险的,因为如此大的样本会产生噪声,更重要的是,会与尘埃背景星系的辐射混淆。鉴于《英国国家科学院院刊》(MNRAS)最近声称有七个潜在的 DSM,我们在 arXiv 上发表了一篇简短的反驳文章。然而,DSM的可探测性受到了质疑:DSM可能会在光学/近红外波长下熄灭其恒星,从而在恒星目录中不出现或显得异常暗淡。此外,先进到足以建造 DSM 的文明也很可能先进到足以使用反制措施来掩盖它的存在。
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Did WISE detect Dyson Spheres/Structures around Gaia-2MASS-selected stars?
Soon after the release of the WISE all-sky catalogue of 500 million mid-infrared (IR) objects, suggestions were made that it could be used to search for extrasolar devices constructed by an advanced civilization to convert a significant fraction of their host star's luminosity into useful work: "technostructures", "megastructures" or "Dyson spheres/structures", hereafter DSMs, whose inevitable waste heat would be seen by WISE at mid-IR wavelengths. However, a trawl of several million potentially-habitable Gaia-detected stars for mid-IR-excess signatures is fraught with danger, due to both noise from such a large sample and, more importantly, confusion with the emission from dusty background galaxies. In light of a recent claim of seven potential DSMs in MNRAS, a brief rebuttal appeared on arXiv. Further to this response, the relevance of WISE-detected galaxies is discussed in more detail, leading to a seemingly tight limit on the number and lifetime of DSMs, and indeed intelligent worlds, in the ~600-pc-radius region patrolled by Gaia. However, the detectability of DSMs is questioned: a DSM might extinguish its star at optical/near-IR wavelengths, and thus either not appear or appear anomalously faint in a stellar catalogue. Moreover, a civilization advanced enough to construct a DSM is likely to be advanced enough to use countermeasures to mask its presence from us.
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