Originally posted by wizofoz Matt, I have yet to venture out in the dark with it, but I recently got the O-GPS1 - inspired mainly by this thread. I understand that it moves the sensor in the camera. I understand it uses GPS data to work out where the camera is located with respect to what it is pointed at, and then moves the sensor to compensate for the earths' rotation.
No doubt some with more experience can give us more information. I'm keen to learn as well.
Well, you have actually mentioned the essentials yourself, but here's a bit more elaborate explanation:
If you know
your 1)compass heading (Azimuth) and 2) the height above the horizon (Altitude) at which your lens is pointing and 3) your geographical co-ordinates plus 4) the date and time,
then
it is straightforward to calculate the declination and right ascension (R.A.) of the point/star at which you lens is pointing.
Further
Knowing the declination and R.A. of a star, you can also calculate the angular speed and direction at which the star will be moving across the sky at a given date and time.
Finally
Knowing the focal length of your lens and the inclination of your caméra, you can convert that to the linear speed and direction at which the image of your star will be moving across the camera sensor plane.
All of these data sets are compiled and processed in the camera firmware.
The ingenious trick
of the Astrotracer function is then to use the shake reduction actuators in the camera body to move the sensor to counteract the travelling of the star's image during exposure. You might say that the sensor is moved in such a manner that it works
as if the camera was mounted on an equatorial mount. A very clever exploitation of the Pentax in-body Shake Reduction mechanism indeed!
Obviously there are limits as to how much the sensor may be moved and thus, how long exposure times one can have at a given declination and a given focal length. Also, the accuracy of the (true geographical - not magnetic) compass reading is quite critical for the calculations which further limits the accuracy that one may reasonably expect.