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How Long is a Planet Stationary?
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A stationary planet is a planet that is turning retrograde or is turning direct. For a moment, the planet stops and changes direction. The planet is completely stationary for only a moment. How close to this exact moment when a planet changes direction can we consider the planet to be stationary?
Another way of stating this is that a stationary planet is not actually stationary! Perhaps for a fraction of a second it is actually stationary. How slow must the planet be in order to be considered stationary?
One tradition is to consider a planet stationary within about a day of the moment that its direction changed from direct to retrograde or from retrograde to direct. However, Mercury speeds up rapidly from the moment it is stationary and reaches its maximum speed in about 2 months whereas Mars, for example, speeds up much more slowly and takes over a year to reach its maximum speed. Mercury is like a race car that takes off from the starting line much more quickly than other planets. Therefore, it seems more reasonable to consider Mercury stationary for a shorter period of time than other planets.
An alternative to considering a planet stationary for some fixed period of time such as a day, is to consider the planet stationary when its speed is below some fraction of either its average speed or maximum speed. In this video, we show how basing the time period that the planet is stationary on its maximum speed produces results that intuitively make more sense than basing the timer period that the planet is stationary on its average speed.
Another possibility is to consider the duration of time between planetary stations and an alternative formula for determining the time period that is stationary is given in which the time between planetary stations for a planet is taken into account.
Also shown in this video are options in the Kepler 8 and Sirius 2.0 software for specifying when a planet is considered to be stationary and also options for how to have this indicated in a chart wheel.
Although the details presented in this tutorial video may be a bit tedious, these are important considerations because until now it has not been clear when we should consider a planet stationary and at last we have some clear guidelines for understanding what options are reasonable.
Another way of stating this is that a stationary planet is not actually stationary! Perhaps for a fraction of a second it is actually stationary. How slow must the planet be in order to be considered stationary?
One tradition is to consider a planet stationary within about a day of the moment that its direction changed from direct to retrograde or from retrograde to direct. However, Mercury speeds up rapidly from the moment it is stationary and reaches its maximum speed in about 2 months whereas Mars, for example, speeds up much more slowly and takes over a year to reach its maximum speed. Mercury is like a race car that takes off from the starting line much more quickly than other planets. Therefore, it seems more reasonable to consider Mercury stationary for a shorter period of time than other planets.
An alternative to considering a planet stationary for some fixed period of time such as a day, is to consider the planet stationary when its speed is below some fraction of either its average speed or maximum speed. In this video, we show how basing the time period that the planet is stationary on its maximum speed produces results that intuitively make more sense than basing the timer period that the planet is stationary on its average speed.
Another possibility is to consider the duration of time between planetary stations and an alternative formula for determining the time period that is stationary is given in which the time between planetary stations for a planet is taken into account.
Also shown in this video are options in the Kepler 8 and Sirius 2.0 software for specifying when a planet is considered to be stationary and also options for how to have this indicated in a chart wheel.
Although the details presented in this tutorial video may be a bit tedious, these are important considerations because until now it has not been clear when we should consider a planet stationary and at last we have some clear guidelines for understanding what options are reasonable.
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