TS Optics Planetary HR 3.2mm 58° 1.25″ Eyepiece
The Planetary HR series from TS Optics was designed with one clear goal: to deliver an eyepiece that handles both detailed planetary observing and deep-sky exploration without any compromise in optical quality. The result is an eyepiece that performs equally well on the Moon and planets as it does on nebulae and distant galaxies. It also supports projection astrophotography with a digital SLR or compact camera.
Sharp, high-contrast views - night after night
The Planetary HR 3.2mm eyepiece stands out for its high contrast and image clarity. Fine details - whether the cloud bands on Jupiter or surface structures on the Moon - remain clearly visible even during long observing sessions, without causing excessive eye strain. Thanks to FMC (Fully Multi-Coated) anti-reflection coatings, the optics deliver reliable results on compact deep-sky objects too, where every photon counts.
Comfortable for eyeglass wearers
The 16mm eye relief is a practical advantage, particularly for observers who wear glasses. You do not need to press your eye close to the lens - the field of view remains full and comfortable. The 20mm exit lens diameter and soft rubber eyecup make it easy to find the correct viewing position quickly.
Where to use this eyepiece
Recommended applications:
- Observing the Moon and planets
- Nebulae and galaxies
- Compact deep-sky objects
- Projection astrophotography with a digital SLR or compact camera
Technical specifications
| Parameter |
Value |
| Focal length |
3.2mm |
| Field of view |
58° |
| Barrel diameter |
1.25″ |
| Eye relief |
16mm |
| Exit lens diameter |
20mm |
| Lens coating |
FMC (Fully Multi-Coated) |
Is this eyepiece right for you?
If you want sharp, high-contrast views of planets and the Moon, and also need an eyepiece that works well on compact deep-sky objects, the TS Optics Planetary HR 3.2mm is a strong choice. The generous eye relief makes it a practical option for observers who wear glasses. It fits any standard telescope with a 1.25″ focuser.