In Earth's atmosphere, the ratio of 3He to 4He is 1.343(13)×10−6.[5] However, the isotopic abundance of helium varies greatly depending on its origin. In the Local Interstellar Cloud, the proportion of 3He to 4He is 1.62(29)×10−4,[6] which is ~121 times higher than in Earth's atmosphere. Rocks from Earth's crust have isotope ratios varying by as much as a factor of ten; this is used in geology to investigate the origin of rocks and the composition of the Earth's mantle.[7] The different formation processes of the two stable isotopes of helium produce the differing isotope abundances.
Equal mixtures of liquid 3He and 4He below 0.8 K separate into two immiscible phases due to differences in quantum statistics: 4He atoms are bosons while 3He atoms are fermions.[8]Dilution refrigerators take advantage of the immiscibility of these two isotopes to achieve temperatures of a few millikelvin.
A mix of the two isotopes spontaneously separates into 3He-rich and 4He-rich regions.[9] Phase separation also exists in ultracold gas systems.[10] It has been shown experimentally in a two-component ultracold Fermi gas case.[11][12] The phase separation can compete with other phenomena as vortex lattice formation or an exotic Fulde–Ferrell–Larkin–Ovchinnikov phase.[13]