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The NS Class 1600 is a type of B′B′ electric locomotive built by Alstom between 1980 and 1983 based on the SNCF Class BB 7200, and in use by the Dutch Railways since 1981. They were styled by the French industrial designer Paul Arzens. The Class 1600 was ordered in 1978, after several types of locomotives were tested in the 1970s.
The International Loadstar is a series of trucks that were produced by International Harvester from 1962 to 1978. [1] The first purpose-built medium-duty truck designed by the company, International slotted the Loadstar between its light-duty pickup trucks (initially the C-series, later the D-series) and the heavy-duty R-series.
All 1600 engines displace 1.6 L; 96.9 cu in (1,588 cc) with bore X stroke of 80 mm × 79 mm (3.15 in × 3.11 in) and have DOHC, 16 valves and MPI. Two variations were created: Two variations were created:
Video, by contrast, encodes images electronically, turning the images into analog or digital electronic signals for transmission or recording. [3] Video technology was first developed for mechanical television systems, which were quickly replaced by cathode-ray tube (CRT) television systems. Video was originally exclusively live technology ...
The history of scientific method considers changes in the methodology of scientific inquiry, not the history of science itself. The development of rules for scientific reasoning has not been straightforward; scientific method has been the subject of intense and recurring debate throughout the history of science, and eminent natural philosophers and scientists have argued for the primacy of ...
Raspberry Pi (/ p aɪ /) is a series of small single-board computers (SBCs) developed in the United Kingdom, originally limited to 32-bit with most later models 64-bit, with the Pico, before Pico 2, still 32-bit.
Gaia is a space observatory of the European Space Agency (ESA) that was launched in 2013 and is planned to operate until March 2025. The spacecraft is designed for astrometry: measuring the positions, distances and motions of stars with unprecedented precision, [5] [6] and the positions of exoplanets by measuring attributes about the stars they orbit such as their apparent magnitude and color. [7]