Johann Bode developed a so-called law of planetary distances best known as Bode’s Law. The story of the discovery of Juno in 1804 by Karl Harding tells how Juno fit into that scheme and is examined as it relates to the philosopher Georg Hegel’s 1801 thesis that there could be no planets between Mars and Jupiter. By 1804 that gap was not only filled but had three residents: Ceres, Pallas and Juno! When Juno was discovered no one could have imagined its study would call into question Newton’s law of gravity, or be the impetus for developing the mathematics of the fast Fourier transform by Carl Gauss. Clifford Cunningham, a dedicated scholar, opens to scrutiny this critical moment of astronomical discovery, continuing the story of asteroid begun in earlier volumes of this series. The fascinating issues raised by the discovery of Juno take us on an extraordinary journey. The revelation of the existence of this new class of celestial bodies transformed our understanding of the Solar System, the implications of which are thoroughly discussed in terms of Romantic Era science, philosophy, poetry, mathematics and astronomy. The account given here is based on both English and foreign correspondence and scientific papers, most of which are translated for the first time.
... Brewster Pallas 2 1802/Apr. 2 284–295 Pearson Ceres 3 1802/May 12 53–62 Piazzi Ceres 2 1802/May 2 20–22 Walker Ceres, Pallas 2 1802/May 2 48–55 Pearson Ceres 2 1802/May 2 56–60 Zach Ceres 1 1802/May 1 13 366 Walker Pallas 1 1802/May ...
Victor Knorre, 'The Asteroids', Pearson's Magazine, X (1900). William Fitzgerald, 'Sir Howard Grubb', Strand Magazine, XII (1896), 5 p. 373. Dan F. Seeson, 'The Minor Planets', British Space Fiction Magazine, 6 II/4 (1955), pp. 30–35.
The discovery of Uranus generated great interest in Bode's law3. The law predicts that there should be a planet between the orbits of Mars and Jupiter, and Bode advocated for a search for this missing planet.
Based on extensive primary sources, many never previously translated into English, this is the definitive account of the origins of Ceres as it went from being classified as a new planet to reclassification as the first of a previously ...
... and proposed that these bodies should be termed asteroids rather than planets, much to Piazzi's annoyance; the discovery of Juno by Harding in 1804, and of Vesta by Olbers in 1807; and indeed the role of Bode's Law (or better, ...
The first asteroid, Ceres, was discovered in 1801, and three others (Pallas, Juno and Vesta) were found between 1801 and ... They based their search on Bode's law (actually first described by J. Titius of Wittemberg, but popularized by ...
The Law was confirmed! ... When Karl Ludwig Harding (1765–1834) found Juno in 1804 and Olbers found Vesta in 1807, this explanation seemed valid ... Neptune and Other Problems AFTER the discovery of the minor 18 THE TITIUS—BODE LAW ...
A reader's guide to the narrative and lyric poetry of Thomas Lovell Beddoes, 18. Newcastle upon Tyne: Cambridge Scholars Publishing. Lofland, J. 1828. The harp of Delaware; or, the miscellaneous poems of the Milford Bard, 65.
Corrispondenza Astronomica fra Giuseppe Piazzi e Barnaba Oriani. Milan: Univ. of Hoepli. Cajori, F. (1897). ... Clark, R. N. (1990). Visual astronomy of the deep sky. Cambridge: Cambridge University Press. Clerke, A. (1901).
They detected a giant luminous arc around the cluster of galaxies, Abell 370; the arc is 500000 light- years long and 25 000 light-years wide. The effect is due to the light from a background galaxy being bent in the gravitational field ...