@inbook {901316,
	title = {On the Habitability of Our Universe},
	booktitle = {Consolidation of Fine Tuning},
	year = {2016},
	pages = {51},
	publisher = {Oxford University},
	organization = {Oxford University},
	abstract = {<p>Is life most likely to emerge at the present cosmic time near a star like the Sun? We consider the habitability of the Universe throughout cosmic history, and conservatively restrict our attention to the context of {\textquotedblleft}life as we know it{\textquotedblright} and the standard cosmological model, ΛCDM. The habitable cosmic epoch started shortly after the first stars formed, about 30 Myr after the Big Bang, and will end about 10 Tyr from now, when all stars will die. We review the formation history of habitable planets and find that unless habitability around low mass stars is suppressed, life is most likely to exist near \~{} 0.1M stars ten trillion years from now. Spectroscopic searches for biosignatures in the atmospheres of transiting Earth-mass\&nbsp;planets around low mass stars will determine whether present-day life is indeed premature or typical from a cosmic perspective.</p>},
	url = {http://arxiv.org/pdf/1606.08926.pdf},
	author = {Loeb, Abraham},
	editor = {Sloan, D}
}
