Eyepieces & Optics
Barlow Lens
A diverging lens that multiplies the effective focal length of everything behind it.
Specifications
| Magnification factor | 1.5×, 2×, 2.5×, 3× |
|---|---|
| Elements | 2 (achromatic) to 3 (apochromatic) |
| Barrel | 1.25″ or 2″ |
| Optical length added | ≈ 100 – 150 mm |
| Coatings | Fully multi-coated |
| Weight | 90 – 350 g |
Observing parameters
| Effective focal ratio | telescope f/ratio × Barlow factor |
|---|---|
| Magnification | telescope focal length × factor ÷ eyepiece focal length |
| Exit pupil | divided by the Barlow factor |
| Practical ceiling | avoid exceeding 2× aperture in mm total magnification |
| Best used with | planetary and lunar, split doubles |
Overview
A Barlow sits between the focuser and the eyepiece and spreads the light cone so that it comes to focus further back, effectively lengthening the telescope. A 2× Barlow doubles the magnification of every eyepiece you own, which is the cheapest way to get a high-power set.
It also increases eye relief relative to a native short eyepiece, so a 2× Barlow with a 20 mm Plössl behaves like a 10 mm with comfortable viewing. The trade is slightly reduced transmission and a longer, more top-heavy stack.
Quality matters more than multiplier: a cheap 3× or 5× Barlow is usually a way to produce a dim, mushy image. Stick to 1.5×, 2× or 2.5× from a reputable maker, and prefer an apochromatic (ED) design for imaging.
Where it fits
Practical notes
- A Barlow plus a mid-length eyepiece beats a very short eyepiece for eye relief every time.
- Be realism about the seeing: doubling magnification on a turbulent night doubles the mush.
- For imaging, an apo (ED) Barlow avoids the colour fringing a cheap achromat introduces.
- A 2″ Barlow lets you use long-focal-length 2″ eyepieces at higher power without vignetting.
Pairs with
- Plössl eyepiece
- Wide-Field Eyepiece
- Star Diagonal
- CMOS Camera