‘A Paper That Speaks, a Radio That Writes’: I Volsci and the Impact of Radio on the Printed Word

2021 ◽  
pp. 408-432
Keyword(s):  
2007 ◽  
Vol 66 (2) ◽  
pp. 389-421 ◽  
Author(s):  
Tariq A Baloch

Although the transformative influence of the printed word is acknowledged in the history of the common law (I will focus primarily on law books), there is as yet no comprehensive study which looks at how the production and dissemination of that printed word was shaped by “communities of printers, booksellers, readers and (for want of a better word) censors”. Not only does this deprive us of a fascinating narrative on the history of the law book, but also, as a consequence, prevents us from tracking more accurately than before the impact of the printed word on legal development across the centuries. As only a book length study could provide a complete narrative on this history, the present article will focus on one part of this story, namely the impact of the practices of printers and booksellers (who were the most important members of the book trade and will therefore be collectively referred to as “the book trade”) on law book publishing in the eighteenth century.


Disruption ◽  
2021 ◽  
pp. 82-139
Author(s):  
David Potter

The chapter opens with a discussion of the social and political order of 15th-century Europe and the Catholic doctrine that provided the ideological core of the system. The next topic will be the development of a new technology, printing, which is crucial to the reform movement initiated by Martin Luther, who made unique use of the printed word to spread his ideas. The next topic is the political use of the Reform movement first in Germany, then in England and the Netherlands. The impact of the Reformation is the development of the nation state and the growth of reasoning based on science.


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


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