First published in 1793, this concise monograph is a valuable early manual for the computation of cometary movement.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Preface 1. General view of the method 2. On the motion of the point of intersection of the radius vector and cord 3. On the comparison of the parabolic cord with the space which answers to the mean velocity of the earth in the same time 4. Of the reduction of the second longitude of the comet 5. On the proportion of the three curtate distances of the comet from the earth 6. Of the graphical declination of the orbit of the earth 7. Of the numerical quantities to be prepared for the construction or computation of the comet's orbit 8. Determination of the distances of the comet from the earth and the sun 9. Determination of the elements of the orbit from the determined distances 10. Determination of the place of the comet from the earth and sun 11. Determination of the distances of the comet from the earth and sun 12. Determination of the comet's orbit 13. Determination of the place of the comet 14. Application of the graphical method to the comet of 1769 15. Application of the distances found 16. Determination of the place of the comet, for another given time 17. Application of the trigonometrical method to the comet of 1769 18. Determination of the elements of the orbit of the comet of 1769 Example of the graphical operation for the orbit of the comet of 1769 Example of the trigonometrical operation for the orbit of the comet of 1769 Conclusion La Place's general method for determining the orbits of comets Determination of the two elements of the orbit Application of La Place's method of finding the approximate perihelion distance Application of La Place's method for correcting the orbit of a comet, to the comet of 1769 Explanation and use of the tables Tables Appendix Plates.
Preface 1. General view of the method 2. On the motion of the point of intersection of the radius vector and cord 3. On the comparison of the parabolic cord with the space which answers to the mean velocity of the earth in the same time 4. Of the reduction of the second longitude of the comet 5. On the proportion of the three curtate distances of the comet from the earth 6. Of the graphical declination of the orbit of the earth 7. Of the numerical quantities to be prepared for the construction or computation of the comet's orbit 8. Determination of the distances of the comet from the earth and the sun 9. Determination of the elements of the orbit from the determined distances 10. Determination of the place of the comet from the earth and sun 11. Determination of the distances of the comet from the earth and sun 12. Determination of the comet's orbit 13. Determination of the place of the comet 14. Application of the graphical method to the comet of 1769 15. Application of the distances found 16. Determination of the place of the comet, for another given time 17. Application of the trigonometrical method to the comet of 1769 18. Determination of the elements of the orbit of the comet of 1769 Example of the graphical operation for the orbit of the comet of 1769 Example of the trigonometrical operation for the orbit of the comet of 1769 Conclusion La Place's general method for determining the orbits of comets Determination of the two elements of the orbit Application of La Place's method of finding the approximate perihelion distance Application of La Place's method for correcting the orbit of a comet, to the comet of 1769 Explanation and use of the tables Tables Appendix Plates.
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