Telescopes & Mounts
Equatorial Mount
One axis pointed at the pole, so tracking a star needs only one motor.
Specifications
| Payload capacity | 5 – 60 kg (imaging ≈ half the visual rating) |
|---|---|
| Tracking rates | Sidereal, lunar, solar |
| Periodic error | ±5 to ±20 arcsec (uncorrected) |
| GoTo database | Typically 40,000 – 100,000 objects |
| Power | 12 V DC, 1 – 5 A while slewing |
| Mount head weight | 4.5 – 25 kg |
Observing parameters
| Polar alignment accuracy | ≤ 5 arcmin for visual, ≤ 1 arcmin for guided imaging |
|---|---|
| Unguided exposure limit | 30 – 120 s (depends on periodic error and focal length) |
| Guided exposure limit | limited by seeing, not the mount |
| Slew speed | 2°/s to 5°/s |
| Image scale limit | ≈ 1–2 arcsec/px before guiding is mandatory |
Overview
An equatorial mount tilts its polar axis to align with Earth's rotation axis. Once that axis is aligned, the sky's daily motion becomes a single rotation about a single axis, which means one motor driven at sidereal rate keeps a target centred. It also means the field does not rotate — essential for long-exposure imaging.
The price is setup complexity. The mount must be polar aligned before tracking is useful, the telescope swings into awkward positions as it tracks, and payload weight ratings are optimistic — for imaging, aim for a mount rated at roughly double your actual payload.
Below roughly 8 kg of payload, a good alt-azimuth mount with tracking is less trouble. Above it, or for any long-exposure imaging, an equatorial mount is not optional.
Where it fits
Practical notes
- Balance in both axes with the full imaging load attached, with the tube roughly where it will be during the session.
- Do a drift alignment if you plan unguided exposures longer than a minute — a polar scope alone rarely gets you under 2 arcmin.
- Never loosen the clutch with the counterweights off; the tube will slam round and can bend the shaft.
- For imaging, halve the manufacturer's payload figure. A mount at 100% of rating will not guide well.