Set Home Posit.
Each of the above Mount Parameters are discussed in detail below: 
5.3.10.2.1  Tracking Speed 
 This menu item allows you to set the speed and method used to track objects in the sky.  
You can select any of the following tracking speeds: 
  
Sidereal 
  
Lunar 
  
Solar 
  
Adaptive King 
  
None/Terrestrial 
  
Closed Loop 
  
Comet/User Def. 
Train Tracking 
 Calculate Rates 
 Activate 
"Sidereal" speed causes the telescope to track in right ascension (RA) at the rate of the 
Earth's rotation.  It is therefore an accurate tracking rate for stars and other deep space 
objects. 
"Lunar" speed causes the telescope to track the right ascension component of the lunar 
trajectory.  Since the Moon has a non circular orbit and moves in both RA and Dec. 
relative to Earth, "Lunar" tracking speed is calculated for the apparent movement of the 
Moon within the next hour. Especially if the Moon is near the horizon, reselecting Lunar 
tracking speed a while later will result in a slightly different tracking speed because 
refraction and parallax play a large role.  
"Solar" speed is very close to sidereal speed, but slightly more accurate for observing the 
Sun.  It is, however, so close, that visual observers of the Sun can usually use sidereal 
speed without difficulty.  As with   Lunar   tracking,   Solar   speed takes into account the 
changes caused by the elliptic orbit of the Earth, and adapts the tracking rate accordingly. 
"Adaptive King" speed is an enhancement of the fixed King Rate.  Its purpose is to take 
refraction into account when observing near the horizon, thereby adapting the tracking 
rate for the apparent change in an object 
s position.  See Chapter 3, section 3.3.1.2 of this 
manual for a more complete explanation. 
"None/Terrestrial" stops all telescope tracking.  It can be used for terrestrial observing, or 
when it is desirable to stop the telescope from moving without powering Gemini off. 
"Closed Loop" tracking is a tool for keeping an object centered in the field of view (1) 
when the mount is not accurately polar aligned or (2) when an object moves slowly with 
respect to the background sky, and its coordinates are downloaded cyclically.  Gemini 
Gemini Users Manual 
5  
6






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