Evidence found in legal and literary texts from early modern England undermines and complicates any notions of a monolithic, stable ideal of female conduct. Loreen L. Giese's study of over 5000 important folios of court depositions contemporary with Shakespeare's plays demonstrates the complex ways those plays participate in and comment upon their culture, rather than stand apart from it. The depositions from the Consistory Court of London for 1586-1611 and the texts of Shakespeare's dramas represent two different kinds of evidence of how courtship and marriage, and the roles available to women within those processes, were perceived, represented, and contested. Whether in the courtroom or on the stage, these texts show that women often enjoyed autonomous roles: they were both suitors and objects of suits, givers as well as receivers of gifts. Thus, both the court records and the plays themselves present women as agents who are capable of challenging the roles traditionally assigned to them in courtship and marriage, so that rather than genders being wholly determinative, the evidence shows that it also allowed space for agency.

Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth's environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort is not merely an academic exercise for a few specialists interested in the solar dust cloud. Since this same cloud exclusively allows direct in-situ acess to investigate extraterrestrial dust particles over a wide range of sizes and materials, it provides valuable information for realistic treatment of dust phenomena in other remote cosmic regions such as in dense molecular clouds, circumstellar dust shells, and even protostellar or protoplanetary systems.