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Up Abstract I. Purpose II. Background III. Orbits IV. Period Determination V. Methods VI. Kepler's Laws VII. Observing Suggestions VIII. Data Gathering IX. Data Processing X. Observer's Data Results XI. Other Quad-A Results XII. Conclusions XIII. Attachments
This Project Jupiter Report
was prepared by
Mizar Consulting
Eugene A. Lanning
130 Hillside Terrace
Nebraska City, NE
68410-3740
ealanni@alltel.net
Member of AAAA
AAAA
The American Association
of Amateur Astronomers
P.O. Box 7981
Dallas, TX
75209-0981
e-Mail:
aaaa@astromax.com
www.AstroMax.com
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Project
Jupiter
IV. Period
Determinations
A. Why
The orbital period of a satellite/moon or planet is a fundamental
parameter that is used to describe the relation of one object to
another. The orbit period is a quantifiable parameter that may be
precisely transmitted to others.
B. Predictions of positions
Because the orbital period may be determined with a high degree of
accuracy – how much accuracy is dependent on the skill of the observer,
the amount of time devoted to the task and the quality and type of
equipment available – future positions of the object observed may be
made with good confidence. This predictive capability is expected to be
examined in a future AAAA project, to derive interesting conclusions.
C. The Period and its Relation to the Mass of the Planet
When the period of an orbiting body is known, then Kepler’s Third Law
(more later) and Newton’s Law of Gravitation may be combined to enable
one to calculate the mass of the body being orbited. Part of Project
Jupiter is to perform those calculations.
D. What about other Planets?
While Project Jupiter is designed around the planet Jupiter, the
technique is general to orbiting bodies
(6) . Its application to any
planet that has a satellite (including Earth) will yield corresponding
information about the planet being orbited. The application to some
planets may be limited by the ability of the telescope to resolve the
satellite-planet spacing, or be constrained by the limiting magnitude of
the telescope system in use.
6 The model does have to be
significantly upgraded to be used on moons whose orbits are significantly
inclined to the Earth’s orbit, i.e., those moons that do not orbit nearly
in the plane of the ecliptic. |
[Home] [Abstract] [I. Purpose] [II. Background] [III. Orbits] [IV. Period Determination] [V. Methods] [VI. Kepler's Laws] [VII. Observing Suggestions] [VIII. Data Gathering] [IX. Data Processing] [X. Observer's Data Results] [XI. Other Quad-A Results] [XII. Conclusions] [XIII. Attachments]
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