We report the first observation of nitrous oxide (N2O) clathrate hydrate (CH) under ultrahigh vacuum (UHV) conditions using infrared spectroscopy. While nucleation of CHs from water and guest molecules either spontaneously or in the presence of promoters is well-established under high-pressure conditions, their occurrence under cryogenic UHV remains less understood, particularly in multiguest systems. In this study, binary and ternary ice mixtures of N2O, ethylene oxide (ETO), dimethyl ether (DME), tetrahydrofuran (THF), and H2O were investigated via thermal annealing at 130 K. The binary N2O-H2O system showed no signs of hydrate formation after 50 h of annealing, whereas the addition of ETO, DME, or THF led to immediate CH formation under identical conditions. This demonstrates a clear promoter-assisted heterogeneous nucleation mechanism. In situ reflection absorption infrared (RAIR) spectroscopy confirms that ETO facilitates the formation of structure I hydrates, incorporating both ETO and N2O in the cages, while DME and THF promote larger-cage CHs. Density functional theory calculations support experimental RAIR results, which predict stronger host-guest interactions and blue shifts for small cages and weaker shifts for large cages. These findings offer new mechanistic insights into multiguest hydrate nucleation and establish N2O CH formation under UHV as a relevant process in cryogenic and astrochemical environments.