  We present a speculative exploration of the properties of a proposed new Dark
Matter (DM) candidate in a heretofore under-explored region of parameter space.
Our proposed ultra-cold candidatae has been a matter of speculation for some
time,and has recently been tentatively identified via direct-detection. While
unconventional, demonstrated existence of this DM candidate would have
wide-ranging implications for a range of fields, from particle cosmology to
exobiology and the Search for Extraterrestrial Life (SETI).
