The study delves into the composition of sea foam collected from Rhode Island beaches, analyzing its amphiphilic components through Folch extraction to concentrate organic compounds. By identifying hemoglycin polymer amide molecules, previously characterized in meteorites, stromatolites, and now sea foam, the research offers insights into the extraterrestrial origin of certain compounds in Earth's oceans. Through MALDI mass spectrometry, a specific m/z sequence was revealed in the sea foam samples, indicating a unique composition distinct to this environment. The presence of hemoglycin in sea foam raises questions about its role in the foam's structure. The study suggests that hemoglycin's ability to form vesicles and lattice structures could contribute to the stability and lightness of sea foam, allowing it to maintain its structure even as water drains from it. Furthermore, the analysis proposes a water-splitting reaction cycle that involves hydrogen production, shedding light on a potential mechanism for the foam's buoyancy and resistance to detachment. Overall, the research highlights the complex interplay between organic compounds, cosmic dust, and marine environments, offering a new perspective on the formation and resilience of sea foam. By linking meteoritic polymer amide to sea foam composition, the study provides valuable insights into the intricate processes shaping Earth's oceans and potentially influencing global ecosystems.