The \textit{Principia} and comets (Q5890301)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: The \textit{Principia} and comets |
scientific article; zbMATH DE number 1642093
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | The \textit{Principia} and comets |
scientific article; zbMATH DE number 1642093 |
Statements
16 January 2002
0 references
The \textit{Principia} and comets (English)
0 references
The author stresses that Newton's law of gravitation indicated that any conic section was a permissible orbit for any celestial body, comets included. The comet of 1680 was one of the keys to his discovery. Its orbit was found to be essentially parabolic and the Principia showed, for the first time, how its orbital parameters could be calculated. The Principia can be regarded in part as a textbook on comets. Newton discusses their luminosity variation, tail formation, periodicity, mass, supposed influence on Earth, and role as a fuel for stars. NEWLINENEWLINENEWLINENewton's approach to orbital calculation was used to find the path and perihelion passage time of Halley's comet at its first expected return in 1758/59. The success of this calculation had a considerable effect on the standing of Newton at that time.
0 references
0.9157450795173644
0 references
0.8128359317779541
0 references
0.7397474646568298
0 references
0.7368287444114685
0 references
0.7115591764450073
0 references