The G Search for Extraterrestrial Civilizations with Large Energy Supplies
Arnold (2005), Forgan (2013), and Korpela et al. (2015) noted that planet-sized artificial structures could be discovered with Kepler as they transit their host star.
We present a general discussion of transiting megastructures, and enumerate ten potential ways their anomalous silhouettes, orbits, and transmission properties would distinguish them from exoplanets. We also enumerate the natural sources of such signatures.
Several anomalous objects, such as KIC 12557548 and CoRoT-29, have variability in depth consistent with Arnold’s prediction and/or an asymmetric shape consistent with Forgan’s model. Since well motivated physical models have so far provided natural explanations for these signals, the ETI hypothesis is not warranted for these objects, but they still serve as useful examples of how nonstandard transit signatures might be identified and interpreted in a SETI context. Boyajian et al. 2015 recently announced KIC 8462852, an object with a bizarre light curve consistent with a “swarm” of megastructures. We suggest this is an outstanding SETI target.
We develop the normalized information content statistic M to quantify the information content in a signal embedded in a discrete series of bounded measurements, such as variable transit depths, and show that it can be used to distinguish among constant sources, interstellar beacons, and naturally stochastic or artificial, information-rich signals. We apply this formalism to KIC 12557548 and a specific form of beacon suggested by Arnold to illustrate its utility.
The ? Search for Extraterrestrial Civilizations with Large Energy Supplies. IV. The Signatures and Information Content of Transiting Megastructures
Jason T. Wright, Kimberly M. S. Cartier, Ming Zhao, Daniel Jontof-Hutter, Eric B. Ford
(Submitted on 15 Oct 2015)
Comments: 25 pages, 10 figures. Submitted to ApJ
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:1510.04606 [astro-ph.EP] (or arXiv:1510.04606v1 [astro-ph.EP] for this version)
Submission history
From: Kimberly Cartier
[v1] Thu, 15 Oct 2015 16:18:57 GMT (11692kb,D)
http://arxiv.org/abs/1510.04606
