Vision in the ultraviolet

Sensitivity to ultraviolet light (UV) is achieved by photoreceptors in the eye that contain a class of visual pigments maximally sensitive to light at wavelengths <400 nm. It is widespread in the animal kingdom where it is used for mate choice, communication and foraging for food. UV sensitivity is not, however, a constant feature of the visual system, and in many vertebrate species, the UV-sensitive (UVS) pigment is replaced by a violet-sensitive (VS) pigment with maximal sensitivity between 410 and 435 nm. The role of protonation of the Schiff base-chromophore linkage and the mechanism for tuning of pigments into the UV is discussed in detail. Amino acid sequence analysis of vertebrate VS/UVS pigments indicates that the ancestral pigment was UVS, with loss of UV sensitivity occurring separately in mammals, amphibia and birds, and subsequently regained by a single amino acid substitution in certain bird species. In contrast, no loss of UV sensitivity has occurred in the UVS pigments of insects.     

The spatial arrangement of cones in the primate fovea.

The retinae of Old World primates contain three classes of light-sensitive cone, which exhibit peak absorption in different spectral regions. But how are the different types of cone arranged in the hexagonal mosaic of the fovea? This question has often been answered with artists' impressions, but never with direct measurements. Staining for antibodies specific to the short-wave photopigment has revealed a sparse, semiregular array of cones; but nothing is known about the arrangement of the more numerous long- and middle-wave cones. Are they randomly distributed, with chance aggregations of one type, as Hartridge postulated in these columns nearly 50 years ago? Or do they exhibit a regular alteration, recalling the systematic mosaics seen in some non-mammalian species? Or, conversely, is there positive clumping of particular cone types, as might be expected if local patches of cones were descended from a single precursor cell? We have made direct microspectrophotometric measurements of patches of foveal retina from Old World monkeys, and report here that the distribution of long- and middle-wave cones is locally random. These two cone types are present in almost equal numbers, and not in the ratio of 2:1 that has been postulated for the human fovea.     

地球在碰撞中运行

对太阳系的探测表明,陨石撞击是行星表面的形成及日后演变的一个重要进程。例如,月亮表面满是陨痕累累的高地及低洼的、布满熔岩的盆地。遍布陨石坑的高地表明,最初的月球外壳及盆地是38亿年以前、月球形成最后阶段中所发生的巨大碰撞的结果。这些盆地是由直径为10～50公里的物体撞击出来的,后来,陨石坑为大熔岩所填充,就成了现在大家所熟知的平坦的玄武岩平原,即月球海。地球表面一定也曾发生过类似的碰撞。这些巨大的碰撞可能是地壳由早先的模样演变成现今海洋和大陆板