and straightforward at first look, but it is actually very time consuming if you don’t have a lot of experience with it. You are strongly suggested to do a lot of homework before trying it out. It is also suggested that you work with people who have had a lot of experience -- at least for the first couple of nights.

With DEC Drift Method, you monitor the drift of each star which tells you how far away you are from the celestial pole.

To perform a DEC drift, you should first perform the steps previously mentioned (Find Polaris and Find NCP).

You need to pick two bright stars to do the DEC drift. One should be close to the eastern horizon and the other due south near the meridian. Both stars should be near the celestial equator (i.e., 0° declination). Monitor the drift of each star one at a time and in DEC only.

While monitoring the star on the meridian, any misalignment in the east-west direction is revealed. While monitoring a star near the east/west horizon, any misalignment in the north-south direction is revealed. It is helpful to have an illuminated eyepiece to help you recognize any drift. To fine tune the alignment, a Barlow lens is recommended since it increases the magnification and reveals any drift faster. When looking due south, insert the diagonal so the eyepiece points straight up. Insert the cross hair eyepiece and align the cross hairs so that one is parallel to the declination axis and the other is parallel to the right ascension axis. Move your telescope manually in R.A. and DEC to check parallelism.

Choose your star near where the celestial equator and the meridian meet. The star should be approximately within half an hour of the meridian and within five degrees of the celestial equator. Center the star in the field of your telescope and monitor the drift in declination.

If the star drifts south, the polar axis is too far east. If the star drifts north, the polar axis is too far west.

Make the appropriate adjustments to the polar axis to eliminate any drift. Once you have eliminated all of the drift, move to the star near the eastern horizon. The star should be 20 degrees above the horizon and within five degrees of the celestial equator.

If the star drifts south, the polar axis is too low.

If the star drifts north, the polar axis is too high.

The two stars in the front of the bowl of the Big Dipper point to Polaris, which is less than one degree from the true (north) celestial pole. Cassiopeia, the “W” shaped constellation, is on the opposite side of the pole from the Big Dipper. The North Celestial Pole (N.C.P.) is marked by the “+” sign.

Again, make the appropriate adjustments to the polar axis to eliminate any drift. Unfortunately, the latter adjustments interact with the prior adjustments ever so slightly.

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iOptron PR EQ manual

PR EQ specifications

The iOptron PR EQ series represents a significant step forward in equatorial mounting technology, engineered for both amateur astronomers and seasoned astrophotographers. With precision and innovation at its core, the PR EQ series boasts a host of features that make it a standout choice for celestial observation and imaging.

One of the main features of the iOptron PR EQ is its advanced GoTo tracking system. This system utilizes a sophisticated database that includes over 200,000 celestial objects, allowing users to effortlessly locate and track stars, planets, and deep-sky phenomena with just a few keystrokes. The built-in GPS module further enhances user experience, automatically aligning the mount with ease and ensuring accurate tracking no matter where you are.

The mount is designed with portability in mind, weighing in at a manageable level yet providing robust stability. This balance between weight and strength makes the PR EQ particularly appealing for those who wish to transport their equipment for field observations. The user-friendly setup process means that even novice astronomers can get up and running quickly.

In terms of construction, the PR EQ features high-quality materials that ensure durability and longevity. The precision machined metal components and advanced gear systems provide smooth movement and steady tracking, essential for capturing high-quality images through telescopes. The load capacity of the mount supports a range of optical tubes, allowing versatility in equipment choice.

Another highlight is the innovative SmartStar technology integrated within the mount. This technology ensures an optimal user experience by providing real-time feedback during setup and alignment, making adjustments automatically when necessary to maintain precision tracking. Additionally, the PR EQ supports various control methods, including hand controller operation and smartphone connectivity, offering users the flexibility to operate the mount according to their preference.

The iOptron PR EQ series is also designed for astrophotography enthusiasts, featuring features like autoguiding compatibility. This allows for extended exposure times without the risk of star trails, making it an ideal choice for capturing intricate celestial images.

In summary, the iOptron PR EQ is a powerful and versatile equatorial mount that combines advanced technology with user-friendly features. Its accurate tracking, sturdy construction, and smart capabilities make it an excellent investment for anyone looking to delve deeper into the wonders of the night sky. Whether for casual stargazing or serious astrophotography, the PR EQ stands out as a reliable companion for celestial exploration.