{ "viewingDirection": "left-to-right", "metadata": [ { "label": "Uniform Title", "value": "Aequatorium astronomicum" }, { "label": "Origin Place", "value": "Nuremberg" }, { "label": "Physical Location", "value": "Cambridge University Library" }, { "label": "Extent", "value": "Leaf height: 310 mm, width: 310 mm." }, { "label": "Funding", "value": "" }, { "label": "Abstract", "value": "
Johannes Schoener (1477-1547) was a priest and later a teacher of mathematics, who had a strong interest in astronomy and astrology. He assembled a printing shop in his house in Bamberg, where he oversaw each stage of the printing process, from setting the type and carving the woodblocks for illustration to binding the final product. He produced many valuable editions of previously unpublished works by many eminent astronomers of the fifteenth century, including Regiomontanus' De cometae magnitudine ... problemata XVI<\/i> (1531), as well as publishing his own works. He also made his own globes, which he issued alongside some of his printed books, and his cartographic work was influential to later map-makers such as Gemma Frisius and Gerard Mercator. In 1521 Schoener put his printing press to use for the publication of his Aequatorium astronomicum<\/i>, in which he employed movable paper disks to represent the movement of the planets. The reader was expected to cut out the templates provided by Schoener and assemble the parts to create a moveable paper instrument, from which planetary positions could be calculated in accordance with Ptolemaic cosmology. After Schoener's death in 1547, his son Andreas published his father's mathematical works under the title Opera mathematica<\/i> (1551); this copy of the Aequatorium astronomicum<\/i> is from the revised and enlarged second edition of the Opera mathematica<\/i>, published in 1561. This diagram shows how the equatorium models the theory of Saturn already discussed, and in particular how the threads that form part of the completed device can be used to show important astronomical parameters. For further explication, Schoener refers his readers to the works of Georg von Peuerbach and Jacques Lefèvre d'�taples.<\/p>" }, { "label": "Date of Creation", "value": "1561" }, { "label": "Title", "value": "Use of the equatorium for the theory of Saturn" }, { "label": "Material", "value": "paper" }, { "label": "Classmark", "value": "R*.2.8(C)" }, { "label": "Note(s)", "value": "
Links to other items:<\/p>
Further image from this edition: CUL R*.2.8(C) (Frame for the equatorium of Saturn)<\/a><\/p> Further image from this edition: CUL R*.2.8(C) (Frame for the equatorium of the eighth sphere)<\/a><\/p> Further image from this edition: CUL R*.2.8(C) (Motion of Saturn (side view))<\/a><\/p> Further image from this edition: CUL R*.2.8(C) (The motion in latitude of Saturn)<\/a><\/p> Further image from this edition: CUL R*.2.8(C) (Theory of Saturn and the circles of motion)<\/a><\/p>