Carte du monde de Kepler's Tabulae Rudolphinae, quibus astronomicae scientiæ, temporum longinquitate collapsae restauratio continetur. Les tables Rudolphine se composent d'un catalogue d'étoiles et des planètes de tableaux publiés en 1627 en utilisant les données de Tycho Brah

• Contributeur: Science History Images / Alamy Banque D'Images
• ID de l’image: G15JY2
• Taille du fichier: 25 MB (1,1 MB Téléchargement compressé)
• Autorisations: Modèle - non | Propriété - non
• Dimensions: 3855 x 2265 px | 32,6 x 19,2 cm | 12,9 x 7,6 inches | 300dpi
• Photographe: Photo Researchers

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Cette image peut avoir des imperfections car il s’agit d’une image historique ou de reportage.

Map of the world from Kepler's Tabulae Rudolphinae, quibus astronomicae scientiae, temporum longinquitate collapsae restauratio continetur. The Rudolphine Tables consist of a star catalogue and planetary tables published in 1627 using data from Tycho Brahe's observations. Johannes Kepler (1571-1630) was a German mathematician, astronomer and astrologer. A key figure in the 17th century scientific revolution, he is best known for his works Astronomia nova, Harmonices Mundi, and Epitome Astronomiae Copernicanae. These works also provided one of the foundations for Isaac Newton's theory of universal gravitation. Kepler devised the three fundamental laws of planetary motion. These laws were based on detailed observations of the planets made by Tycho Brahe and himself. Kepler's first law states that the planets orbit the Sun in elliptical paths, with the Sun at one focus of the ellipse. The second law states that the closer a planet comes to the Sun, the faster it moves. Kepler's third law states that the ratio of the cube of a planet's mean distance from the Sun to the square of its orbital period is a constant.

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