What magnification does the included eyepiece give?
The 28mm eyepiece gives 96x (2700mm / 28mm). The highest useful magnification is 420x and the lowest is 67x.
Does the Mak need collimating?
Instead of a separate secondary mirror, the Mak has a secondary spot of reflective coating applied to the inside of the corrector plate, so it does not need the occasional collimation a Schmidt-Cassegrain does; the spot is also significantly smaller than a Schmidt-Cassegrain secondary, which gives the Mak its signature high-contrast views.
Why does the Mak take longer to cool down?
The larger, heavier Maksutov corrector plate takes longer to cool down and adjust to ambient air temperature than a Schmidt-Cassegrain corrector of the same aperture.
Can I use 2" accessories?
Yes. The 2" visual back and 2" star diagonal (with a 1.25" adapter) take the included 28mm 2" eyepiece, and the tube accommodates larger 2" accessories such as 2" Barlow lenses, Celestron's 2" eyepiece and filter kit, and larger wide-field eyepieces.
Can I polar align the CGEM II if I can't see the celestial pole?
Yes. All-Star Polar Alignment lets you polar align accurately using any bright star, even when the celestial pole cannot be seen. After a two-star alignment with at least one calibration star, you slew to a bright star from the Named Star list, ideally high in the sky and near the meridian, and choose Polar Align, then Align Mount. The mount syncs on the star and slews to where it should be if accurately polar aligned, and you center it with the mount's latitude and azimuth adjustments, not the hand control's direction buttons.
How does Permanent PEC work?
Periodic Error Correction improves tracking by reducing the amplitude of the worm errors. It works in three steps: the mount indexes its worm gear, you guide with an autoguider for at least 10 minutes (one full worm revolution) while it records your corrections, and then you play them back. The mount retains the recording, and PEC is for advanced astrophotography and still needs careful guiding.
Will the CGEM II track past the meridian?
The CGEM II tracks well past the meridian for uninterrupted imaging through the best part of the sky. The R.A. slew limits can be set anywhere from 40° above level to 20° below, so the mount can keep tracking past the meridian without flipping, or stop before an imaging cable runs out of length, and the Meridian setting (Favor Current, Favor West, Favor East or Disable) chooses which side of the mount the tube stays on. The CGEM II images through the meridian without needing a meridian flip until the object is a full 20° past it.
How do I balance the telescope on the CGEM II?
To balance in R.A., loosen the R.A. lock lever with the counterweight bar horizontal and move the counterweight until the telescope stays put; in Dec, loosen the DEC clutch with the tube level and slide the tube in the saddle. Celestron's tip for imaging is a very slight imbalance, toward the counterweight side when the tube is west of the mount and toward the tube when it is east, so the worm gear always pushes against a slight load.
What power does the CGEM II need?
Power is 12V DC at 3.2 amps. The supplied car battery adapter plugs into a car's cigarette lighter outlet or a portable power supply, or you can use one of Celestron's optional AC to DC adapters; use only adapters Celestron supplies, as others may damage the electronics and void the warranty.
Can I control the CGEM II from a computer?
The hand control's USB port connects to a computer for point-and-click slewing from software and for firmware updates; updating the hand control with Celestron Firmware Manager may resolve some problems. The mount's software is Starry Night Special Edition and the SkyPortal app.