Spike-shaped structures are produced by light-driven ablation in very different contexts. Penitentes 1-4 m high are common on Andean glaciers, where their formation changes glacier dynamics and hydrology. Laser ablation can produce cones 10-100 µm high with a variety of proposed applications in materials science. We report the first laboratory generation of centimeter-scale snow and ice penitentes. Systematically varying conditions allows identification of the essential parameters controlling the formation of ablation structures. We demonstrate that penitente initiation and coarsening requires cold temperatures, so that ablation leads to sublimation rather than melting. Once penitentes have formed, further growth of height can occur by melting. The penitentes intially appear as small structures (3 mm high) and grow by coarsening to 1-5 cm high. Our results are an important step towards understanding and controlling ablation morphologies.PACS numbers: 89.75. Kd,81.16.Rf,92.40.Rm,92.40.Sn, Penitentes 1-4 m high are found on glaciers in high mountain regions; laser ablation of materials can produce similar structures 10-100 µm high (Fig. 1). These structures are initiated by the same underlying physics: ablation caused by direct and reflected radiation. When radiation illuminates a surface, small surface depressions receive more reflected light than high points, leading to greater ablation in troughs and surface instability [1,2,3]. Penitente formation alters glacial energy balances and therefore affects local water runoff and flooding, feedback in climate dynamics, and paleo-climatic reconstruction [4,5]. In materials science, surface micropatterning via laser ablation can produce problematic surface roughness [6,7], but also has several proposed applications, including improved solar cells and electron-field emitters [8,9].Here we report the first laboratory generation of snow penitentes 1-5 cm high (Fig. 1). We characterize lab penitente formation and measure penitente coarsening. The lab setting allows controlled environmental conditions, and we can measure the evolution of lab penitentes visually in real time. Our experiments provide a model system for studying ablation morphologies.Penitentes occur on high-altitude snowfields exposed to intense sunlight, particularly in South America [10]. Expeditions studying penitentes have invoked the importance of sunlight [4,5,10,11] and cold, dry conditions (dew point below 0 o C), where melting is disfavored and ablation proceeds by sublimation [5,10]. Concentrated reflections and protection from wind increase penitente growth; higher temperature and humidity in the troughs of penitentes allows melting in the troughs [10]. This effect accelerates penitente growth, because sublimation of ice at 0 o C requires 7.8 times more energy than melting an equivalent volume, while the sublimating surface is evaporatively cooled, further lowering the surface temperature. Thus initiation of penitente growth requires a low dew point, but melting can occur during later height growth....