Reflector · Primary and diagonal mirror

Newtonian reflectors: the simplest big telescope

Isaac Newton built the first working reflecting telescope in 1668 with a curved metal mirror and a small flat one. The design has barely changed: it is still the cheapest way to make a large, color-free telescope, and it sits inside every Dobsonian.

Curved primary mirror Eyepiece at the side of the tube Flat diagonal mirror Diagram not to scale
Light enters the open tube, reflects off the curved primary mirror, and a flat diagonal mirror sends it out the side to the eyepiece. No glass lens, so no color fringing.
First built
1668by Isaac Newton
Typical focal ratio
f/4 to f/5for imaging Newtonians
Central obstruction
20% to 35%of the aperture
Imaging 8-inch from
$925Sky-Watcher Quattro 200P
Color fringing
nonemirrors reflect all colors alike

A parabolic mirror and a flat diagonal

The primary mirror is ground to a paraboloid, the shape that brings parallel starlight to a single point. A flat secondary mirror, tilted at 45°, sits on a four-vane spider near the top of the tube and sends the light out the side. The vanes cause the four-pointed spikes on bright stars in Newtonian photographs.

Newtonians come on three kinds of mount: Dobsonian rocker boxes for visual use, equatorial mounts for tracking and imaging, and small altitude-azimuth mounts for beginner models.

Fast Newtonians trade a larger obstruction for wide, bright imaging fields

Imaging Newtonians run f/4 to f/5 with large secondary mirrors to cover a camera sensor fully; visual ones run f/5 to f/8 with smaller secondaries for higher contrast on planets. All fast Newtonians show coma, stars drawn into small comet shapes toward the edge of the field, which a coma corrector lens removes.

TelescopeApertureFocal lengthRatioObstructionResolvesWidest fieldMax power
StarSense Explorer DX 130AZ130 mm650 mmf/5.033%0.9"2.4°260x
Quattro 150P150 mm600 mmf/4.037%0.8"4.4°300x
Quattro 200P203 mm800 mmf/3.934%0.6"3.3°350x
Quattro 250P254 mm1,000 mmf/3.932%0.5"2.6°350x
Quattro 300P305 mm1,200 mmf/3.933%0.4"2.2°350x

Obstruction figures are approximate, as a share of the aperture's diameter. Widest true field uses the largest eyepiece the focuser takes: a 46 mm field stop for 2-inch focusers, 27 mm for 1.25-inch. Highest useful power is 2x per millimeter of aperture, capped at 350x by the air.

Current Newtonians from Sky-Watcher and Celestron

Sky-Watcher's Quattro line, made by Synta in China, dominates imaging Newtonians in the US; Celestron sells beginner Newtonians with phone-guided pointing.

ModelMakerApertureRatioUS priceNotes
StarSense Explorer LT 114AZCelestron114 mmf/8sold outEntry-level; phone-guided
StarSense Explorer DX 130AZCelestron130 mmf/5$500Phone-guided; alt-azimuth mount
Quattro 150PSky-Watcher150 mmf/4$665Tube only; imaging
Quattro 200PSky-Watcher203 mmf/4$925Tube only; imaging
Quattro 250PSky-Watcher254 mmf/4$1,325Tube only; imaging
Quattro 300PSky-Watcher305 mmf/4$1,995Tube only; needs a heavy mount

Prices are from US dealers in November 2026; tariffs on Chinese-made optics raised most prices in 2025.

Best for fast deep-sky imaging and big-aperture visual observing

Newtonians give the most aperture per dollar on an equatorial mount and are fast enough to image nebulae and galaxies in short exposures. Their costs are collimation, which must be checked often, an open tube that lets in dust and dew, and a large central obstruction that softens planetary contrast slightly. A Quattro 200P weighs about 20 lb and needs a mount rated for 30 lb or more, such as a Sky-Watcher EQ6-R or a ZWO AM5.