Low Density Amorphous IceEdit
Low-Density Amorphous Ice (Low-Density Amorphous Ice) is a metastable, non-crystalline form of water ice that exists at cryogenic temperatures. As one of the family of amorphous ices, it contrasts with the well-ordered crystalline forms of ice and with the denser amorphous counterpart known as high-density amorphous ice. LDA is of particular interest in cryophysics and planetary science because its disordered structure preserves aspects of water’s hydrogen-bond network in a state far from crystalline order. The study of LDA helps illuminate how water behaves when cooled rapidly or when water molecules are deposited as a thin film under vacuum, conditions that are common in laboratory cryogenics and in space environments.
Formation and Structure - LDA can be prepared by rapid cooling or “hyperquenching” of liquid water droplets to cryogenic temperatures, as well as by vapor deposition of water onto a cold surface in vacuum at low temperatures. These methods prevent the water molecules from organizing into a crystalline lattice, yielding a glassy, disordered solid. See discussions of hyperquenching and vapor deposition for related preparation techniques. - The resulting structure is amorphous, meaning it lacks long-range translational order. Local hydrogen-bonding environments resemble those found in liquid water and in crystalline ice, but there is no repeating crystal lattice over large distances. Analytical techniques such as X-ray diffraction and infrared spectroscopy reveal broad, featureless signals characteristic of amorphous networks rather than sharp Bragg peaks of crystals.
Physical Properties - Density: LDA is a low-density form relative to other amorphous ices, with reported values around 0.93–0.94 g/cm^3 at cryogenic temperatures. This places it below high-density amorphous ice but above many crystalline ices, and it demonstrates the diversity of water’s amorphous forms. - Thermal behavior: As a glassy solid, LDA remains rigid at low temperatures. Upon heating, LDA may crystallize into more ordered ices (often stacking-disordered ice I or other crystalline forms) if given time and sufficient mobility. The exact crystallization pathway can depend on the preparation method and heating rate. - Spectroscopy and structure: Infrared and Raman spectroscopies show broad OH-stretch bands reflecting a wide distribution of hydrogen-bond lengths and angles. These spectral features, together with diffuse scattering in diffraction experiments, distinguish LDA from crystalline ices and from higher-density amorphous forms.
Phase Relationships and Polyamorphism - LDA is part of a broader discussion about polyamorphism in water—the existence of more than one amorphous solid state—alongside high-density amorphous ice (HDA) and very high-density amorphous ice (VHDA). In this framework, LDA and HDA represent distinct amorphous states with different densities and local structures. - The nature of transitions between amorphous ices (for example, LDA transforming into HDA under pressure) and the interpretation of such transitions are topics of ongoing scientific debate. Some experiments and simulations support a sharp, pressure-induced LDA↔HDA transition and align with a two-structure model of water, while others raise questions about sample history, preparation conditions, and the universality of such transitions. The dialogue reflects broader questions about how water organizes itself under extreme conditions and how to reconcile experimental results with theoretical models.
Relevance to Planetary Science and Astrophysics - Amorphous ices are believed to be common in the cold outer regions of the Solar System. On icy moons, comets, and interstellar grains, water vapor can condense as amorphous ice due to rapid deposition at very low temperatures. The presence and properties of LDA influence how volatile species are trapped and released, affecting models of surface chemistry, outgassing, and the evolution of icy bodies. - The behavior of LDA under irradiation, cosmic-ray processing, or heating by solar radiation informs ideas about the chemical inventory that might be delivered to other planets and moons, as well as the storage of simple molecules in dense molecular clouds. Discussions of these processes often reference the broader literature on interstellar ice and cosmic ice analogs.
Historical Origins and Key Debates - The discovery and characterization of LDA are closely associated with early cryogenic experiments led by researchers such as Ken-ichirō Mishima in the 1980s and 1990s. These experiments demonstrated that water can form a glassy, low-density solid that is distinct from crystalline ice and from denser amorphous forms. - A central scholarly debate concerns how best to interpret the relationship between amorphous ices and the hypothesized liquid states of water. Some researchers emphasize a "two-structure" perspective in which LDA and HDA reflect fundamentally different hydrogen-bond networks and relate to proposed liquid-liquid phase behavior in supercooled water. Others argue that the amorphous phases may reflect kinetic and thermodynamic factors specific to cryogenic preparation, rather than a direct analogue to liquid states. Experimental divergences, model dependence in simulations, and the sensitivity of amorphous samples to preparation history all contribute to the ongoing discussion.
Connections to Related Topics - For readers exploring the broader context of water’s solid forms, see water and ice to compare crystalline and amorphous states. - The study of LDA intersects with the physics of the glassy state, as well as with techniques like X-ray diffraction and infrared spectroscopy used to probe disordered materials. - The family of amorphous ices includes not only LDA but also high-density amorphous ice and very high-density amorphous ice, each representing different regions of the amorphous landscape in water.
See also - Water - Ice - amorphous ice - Low-Density Amorphous Ice - High-Density Amorphous Ice - Very High-Density Amorphous Ice - Ken-ichirō Mishima - Mishima (scientist)