Stargazer's Atlas Astronomy Tools & Reference
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Eyepieces & Optics

Barlow Lens

A diverging lens that multiplies the effective focal length of everything behind it.

Technical line drawing of a barlow lens

Specifications

Magnification factor1.5×, 2×, 2.5×, 3×
Elements2 (achromatic) to 3 (apochromatic)
Barrel1.25″ or 2″
Optical length added≈ 100 – 150 mm
CoatingsFully multi-coated
Weight90 – 350 g

Observing parameters

Effective focal ratiotelescope f/ratio × Barlow factor
Magnificationtelescope focal length × factor ÷ eyepiece focal length
Exit pupildivided by the Barlow factor
Practical ceilingavoid exceeding 2× aperture in mm total magnification
Best used withplanetary 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

ObservingImaging
Planet Lunar

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

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