{"title":"WISE探测到盖亚-2MASS选择的恒星周围的戴森球/结构了吗?","authors":"Andrew W. Blain","doi":"arxiv-2409.11447","DOIUrl":null,"url":null,"abstract":"Soon after the release of the WISE all-sky catalogue of 500 million\nmid-infrared (IR) objects, suggestions were made that it could be used to\nsearch for extrasolar devices constructed by an advanced civilization to\nconvert a significant fraction of their host star's luminosity into useful\nwork: \"technostructures\", \"megastructures\" or \"Dyson spheres/structures\",\nhereafter DSMs, whose inevitable waste heat would be seen by WISE at mid-IR\nwavelengths. However, a trawl of several million potentially-habitable\nGaia-detected stars for mid-IR-excess signatures is fraught with danger, due to\nboth noise from such a large sample and, more importantly, confusion with the\nemission from dusty background galaxies. In light of a recent claim of seven\npotential DSMs in MNRAS, a brief rebuttal appeared on arXiv. Further to this\nresponse, the relevance of WISE-detected galaxies is discussed in more detail,\nleading to a seemingly tight limit on the number and lifetime of DSMs, and\nindeed intelligent worlds, in the ~600-pc-radius region patrolled by Gaia.\nHowever, the detectability of DSMs is questioned: a DSM might extinguish its\nstar at optical/near-IR wavelengths, and thus either not appear or appear\nanomalously faint in a stellar catalogue. Moreover, a civilization advanced\nenough to construct a DSM is likely to be advanced enough to use\ncountermeasures to mask its presence from us.","PeriodicalId":501348,"journal":{"name":"arXiv - PHYS - Popular Physics","volume":"12 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Did WISE detect Dyson Spheres/Structures around Gaia-2MASS-selected stars?\",\"authors\":\"Andrew W. Blain\",\"doi\":\"arxiv-2409.11447\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Soon after the release of the WISE all-sky catalogue of 500 million\\nmid-infrared (IR) objects, suggestions were made that it could be used to\\nsearch for extrasolar devices constructed by an advanced civilization to\\nconvert a significant fraction of their host star's luminosity into useful\\nwork: \\\"technostructures\\\", \\\"megastructures\\\" or \\\"Dyson spheres/structures\\\",\\nhereafter DSMs, whose inevitable waste heat would be seen by WISE at mid-IR\\nwavelengths. However, a trawl of several million potentially-habitable\\nGaia-detected stars for mid-IR-excess signatures is fraught with danger, due to\\nboth noise from such a large sample and, more importantly, confusion with the\\nemission from dusty background galaxies. In light of a recent claim of seven\\npotential DSMs in MNRAS, a brief rebuttal appeared on arXiv. Further to this\\nresponse, the relevance of WISE-detected galaxies is discussed in more detail,\\nleading to a seemingly tight limit on the number and lifetime of DSMs, and\\nindeed intelligent worlds, in the ~600-pc-radius region patrolled by Gaia.\\nHowever, the detectability of DSMs is questioned: a DSM might extinguish its\\nstar at optical/near-IR wavelengths, and thus either not appear or appear\\nanomalously faint in a stellar catalogue. Moreover, a civilization advanced\\nenough to construct a DSM is likely to be advanced enough to use\\ncountermeasures to mask its presence from us.\",\"PeriodicalId\":501348,\"journal\":{\"name\":\"arXiv - PHYS - Popular Physics\",\"volume\":\"12 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Popular Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.11447\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Popular Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11447","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
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.