{"product_id":"zwo-ff131-apo-flat-field-refractor-ota","title":"ZWO FF131 APO Flat-Field Refractor OTA","description":"\n\u003cp\u003eFor generations, a five-inch apochromatic refractor has been the instrument many observers work toward. It represents a wonderful balance of aperture, optical performance, and practicality. Large enough to reveal serious planetary and deep-sky detail, yet still manageable without the machinery and mounting requirements of a much larger instrument, a well-made five-inch refractor can be a telescope that stays with its owner for a very long time.\u003c\/p\u003e\n\n\u003cp\u003eThe ZWO FF131 APO brings that familiar appeal into the world of modern astrophotography. Its 131mm objective collects approximately three and a half times as much light as a 70mm refractor, while its 983mm focal length provides the image scale needed to explore smaller galaxies, planetary nebulae, globular clusters, and other objects that benefit from additional resolving power.\u003c\/p\u003e\n\n\u003cp\u003eBut there's something else that makes the FF131 particularly interesting. Its four-element apochromatic optical system is designed to provide a flat photographic field across a 44mm image circle. A separate field flattener isn't necessary, and the photographer doesn't have to experiment with a precise flattener-to-camera spacing to bring the corners into focus.\u003c\/p\u003e\n\n\u003cp\u003eAt f\/7.5, this isn't a short, fast refractor intended primarily for enormous regions of emission nebulosity. It's a telescope designed for the observer who wants to move in closer, look more carefully, and discover details that a smaller instrument may leave unresolved.\u003c\/p\u003e\n\n\u003ch3\u003eWhy a Five-Inch Refractor?\u003c\/h3\u003e\n\n\u003cp\u003eThere is a noticeable difference between observing through a small refractor and spending an evening with one having five inches of clear aperture. The larger objective gathers more light and has greater theoretical resolving power, two advantages that can make themselves apparent on the Moon, planets, double stars, and many deep-sky objects.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131's 131mm aperture collects approximately 3.5 times as much light as a 70mm refractor, assuming comparable optical transmission. Compared with the FF110, it gathers approximately 42% more light.\u003c\/p\u003e\n\n\u003cp\u003eThat increase doesn't mean an extended nebula will automatically photograph three and a half times faster. Photographic exposure speed for extended objects depends heavily on focal ratio and image sampling. The advantage of the larger aperture is that it supports greater image scale and potentially finer detail while still collecting enough light to make those smaller targets practical.\u003c\/p\u003e\n\n\u003cp\u003eIts resolving power is another consideration. All else being equal, a larger objective can distinguish finer details than a smaller one. Actual performance depends on optical quality, atmospheric seeing, thermal conditions, and accurate focus, but the additional aperture gives the FF131 more potential to work with.\u003c\/p\u003e\n\n\u003cp\u003eAt the eyepiece, that can mean a more satisfying view of Jupiter's cloud belts or the tightly packed stars of a globular cluster. At the camera, it can mean giving a galaxy more pixels across its spiral structure without relying quite so heavily on enlarging a smaller photograph afterward.\u003c\/p\u003e\n\n\u003cp\u003eFor many observers, this is the attraction of a five-inch apo. It's a serious optical instrument, but one that remains practical for an individual to own and use regularly.\u003c\/p\u003e\n\n\u003ch3\u003eNearly a Meter of Focal Length\u003c\/h3\u003e\n\n\u003cp\u003eThe FF131 has a native focal length of 983mm, just a little short of one meter. That's considerably longer than the 490mm focal length of the FF70, and even the FF110's 766mm.\u003c\/p\u003e\n\n\u003cp\u003eWith the same camera, the longer focal length makes an astronomical object appear larger on the sensor. This is especially helpful with galaxies that occupy relatively small areas of the sky.\u003c\/p\u003e\n\n\u003cp\u003eConsider the Whirlpool Galaxy, M51. A short refractor can photograph the galaxy and its companion, but the pair may occupy only a small portion of a wide field. At 983mm, the galaxies take up more of the sensor, providing additional opportunity to record their spiral structure when seeing and tracking permit.\u003c\/p\u003e\n\n\u003cp\u003eThe Black Eye Galaxy, M64, is another excellent example. Its bright central region is interrupted by a striking dark dust feature, and the additional image scale of the FF131 makes that feature a more prominent part of the photograph.\u003c\/p\u003e\n\n\u003cp\u003ePlanetary nebulae present an especially interesting challenge. The Ring Nebula in Lyra and the Owl Nebula in Ursa Major are both comparatively small objects. They don't require an enormous photographic field, but they reward accurate guiding, fine image sampling, and enough integration time to bring out their subtler structures.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131's 983mm focal length puts these objects at a useful scale for a refractor, although the very smallest planetary nebulae will still benefit from longer effective focal lengths and exceptional atmospheric conditions.\u003c\/p\u003e\n\n\u003cp\u003eAnd, of course, the FF131 can still photograph larger subjects. The Dumbbell Nebula, Crescent Nebula, and many globular clusters fit comfortably within its field. Nearly a meter of focal length does not mean that the telescope becomes useful only for tiny objects.\u003c\/p\u003e\n\n\u003ch3\u003eFour-Element Apochromatic Optics\u003c\/h3\u003e\n\n\u003cp\u003eThe FF131 uses a fully air-spaced, four-element apochromatic optical system incorporating one element made from extra-low dispersion, or ED, glass.\u003c\/p\u003e\n\n\u003cp\u003eRefractor optics must overcome the tendency of different wavelengths of light to focus at different distances. Blue light is refracted more strongly than red light, so an ordinary lens may produce colored fringes around bright objects rather than bringing the visible spectrum to a common focus.\u003c\/p\u003e\n\n\u003cp\u003eBy carefully combining lens elements of different optical properties, an apochromatic design greatly reduces this chromatic aberration. The result is better color correction and improved image definition, particularly on stars, planets, and other subjects where unwanted color is readily apparent.\u003c\/p\u003e\n\n\u003cp\u003eZWO doesn't specify the exact ED glass formulation used in the FF131. The important consideration is the performance of the complete four-element system, rather than assuming that the designation of any one glass element determines the quality of the telescope.\u003c\/p\u003e\n\n\u003cp\u003eThe four elements serve another purpose as well. They are designed to correct field curvature, allowing the FF131 to produce a flat photographic image without requiring an additional field flattener.\u003c\/p\u003e\n\n\u003cp\u003eThis is a meaningful convenience. A conventional refractor typically forms its sharpest image on a slightly curved surface, while the image sensor in a camera is flat. A separate field flattener corrects the problem, but usually requires the sensor to be positioned at a particular distance behind the flattener.\u003c\/p\u003e\n\n\u003cp\u003eAdding a filter wheel, off-axis guider, or different camera can complicate that spacing. It may even require replacing several adapters with others of slightly different lengths.\u003c\/p\u003e\n\n\u003cp\u003eWith the FF131, field flattening is built into the telescope. As long as the camera can reach focus within the available mechanical range, there is no separate flattener correction distance to maintain.\u003c\/p\u003e\n\n\u003cp\u003eThis doesn't remove the need for accurate mechanical alignment. Camera tilt, flexure, or a loose adapter can still affect the stars near the corners. But having the optical field corrected within the telescope eliminates one common source of frustration.\u003c\/p\u003e\n\n\u003ch3\u003eA Flat Field for Full-Frame Cameras\u003c\/h3\u003e\n\n\u003cp\u003eZWO specifies a 44mm image circle for the FF131, large enough to cover the approximately 43.3mm diagonal of a standard full-frame photographic sensor.\u003c\/p\u003e\n\n\u003cp\u003eWith a 36mm x 24mm full-frame camera, the 983mm focal length provides a field approximately 2.1 degrees wide and 1.4 degrees high.\u003c\/p\u003e\n\n\u003cp\u003eThat's a useful amount of sky for many galaxies and smaller nebulae. There's enough room to include the surrounding star field without making a reasonably compact subject look lost in an enormous photograph.\u003c\/p\u003e\n\n\u003cp\u003eAn APS-C camera, depending on its exact sensor dimensions, records a smaller field of approximately 1.4 degrees by 0.9 degrees. That can be particularly attractive for globular clusters, compact galaxies, and other targets where a tighter composition is desirable.\u003c\/p\u003e\n\n\u003cp\u003eA full-frame camera isn't required to enjoy the FF131. In fact, a smaller sensor can be a sensible choice when your primary interest is photographing compact objects.\u003c\/p\u003e\n\n\u003cp\u003eThe manufacturer's 44mm image-circle specification describes the intended optical coverage. A full-frame imaging system still needs properly sized filters and adapters, good camera alignment, and adequate mechanical support. Restrictive openings or camera tilt can affect corner illumination and star shapes even when the telescope itself has a flat focal field.\u003c\/p\u003e\n\n\u003ch3\u003eChoosing the Right Camera and Image Scale\u003c\/h3\u003e\n\n\u003cp\u003eAt nearly a meter of focal length, the FF131 deserves a little thought when selecting a camera.\u003c\/p\u003e\n\n\u003cp\u003eA camera with 3.76-micron pixels provides an image scale of approximately 0.79 arcseconds per pixel at the FF131's native focal length. That's relatively fine sampling, which can be useful when atmospheric seeing is good and the mount is guiding accurately.\u003c\/p\u003e\n\n\u003cp\u003eOn nights when the stars are blurred by several arcseconds of atmospheric turbulence, however, recording them at such a fine scale won't necessarily reveal additional detail. The camera may simply be spreading the same blurred information across more pixels.\u003c\/p\u003e\n\n\u003cp\u003eA camera with pixels in the 4.6- to 5-micron range records approximately 0.97 to 1.05 arcseconds per pixel. Those are also useful sampling scales for a telescope of this focal length.\u003c\/p\u003e\n\n\u003cp\u003eAnother option is to use 2x2 binning with a smaller-pixel camera. When supported by the camera and software, this combines groups of four neighboring pixels into a larger effective pixel. For a camera with 3.76-micron pixels, the resulting sampling is approximately 1.58 arcseconds per effective pixel.\u003c\/p\u003e\n\n\u003cp\u003eBinning sacrifices spatial sampling in exchange for fewer, larger image samples. It can improve the usefulness of the data in some imaging situations, although any signal-to-noise improvement depends on the particular camera and whether binning is performed in hardware or software. Modern CMOS cameras don't all behave like older CCD cameras in this respect.\u003c\/p\u003e\n\n\u003cp\u003eThere's no single pixel size that is automatically best for everyone. Your seeing conditions, guiding accuracy, camera sensor, and preferred subjects all matter.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131 provides enough image scale to make that choice meaningful, particularly if your goal is to photograph galaxies and other objects containing relatively fine structure.\u003c\/p\u003e\n\n\u003ch3\u003eA Focuser Built for a Full Imaging Train\u003c\/h3\u003e\n\n\u003cp\u003eA telescope of this size is likely to carry more than a small camera threaded directly onto the back. A cooled astronomical camera, filter wheel, off-axis guider, and several adapters can create a substantial imaging assembly.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131 uses a 3\" rack-and-pinion focuser with dual-speed adjustment. The larger mechanism provides substantial mechanical support, while the 10:1 fine-focus control allows the small adjustments needed when approaching critical focus.\u003c\/p\u003e\n\n\u003cp\u003eThat's especially important when imaging at approximately 0.8 arcseconds per pixel. A small focus error that might be less obvious in a very wide-field photograph can soften fine stellar and galactic detail at this image scale.\u003c\/p\u003e\n\n\u003cp\u003eThe focuser incorporates a 360-degree camera rotator, allowing the camera to be positioned for the most attractive composition without loosening the optical tube in its mounting rings.\u003c\/p\u003e\n\n\u003cp\u003eThat may not seem particularly important until you're trying to place two galaxies diagonally across the sensor or keep an elongated nebula comfortably within the field. A small rotation can produce a much more satisfactory photograph.\u003c\/p\u003e\n\n\u003cp\u003eOnce the camera is positioned, secure the rotator and check focus again before beginning the exposure sequence.\u003c\/p\u003e\n\n\u003cp\u003eThe focuser is also designed to accept a compatible ZWO EAF electronic focuser. Motorized focusing is especially useful on long imaging nights, allowing compatible software to refocus when temperature changes or when different filters are selected.\u003c\/p\u003e\n\n\u003ch3\u003eRear Connections and Camera Spacing\u003c\/h3\u003e\n\n\u003cp\u003eThe FF131 has a large M78x1 rear interface and includes a 55mm extension, along with adapters providing M54x0.75 and M48x0.75 connections.\u003c\/p\u003e\n\n\u003cp\u003eA four-section photography extension assembly is included, with a thread for a standard mounted 2\" astronomical filter. This provides flexibility when connecting different camera arrangements.\u003c\/p\u003e\n\n\u003cp\u003eBecause the FF131 is natively flat, you don't have to reproduce a particular distance between a separate field flattener and the camera sensor. But the camera still must be positioned where the telescope's focuser can bring it to focus.\u003c\/p\u003e\n\n\u003cp\u003eZWO specifies an imaging focus range of 42mm to 73mm measured from the designated M54-to-M48 adapter shoulder. The corresponding M54 connection uses a range of 60mm to 91mm, measured from its different reference point.\u003c\/p\u003e\n\n\u003cp\u003eThese figures describe the available focusing arrangement, not an optical correction spacing that must be matched exactly.\u003c\/p\u003e\n\n\u003cp\u003eBefore purchasing additional adapters, add up the mechanical lengths of your camera, filter wheel, off-axis guider, and any spacers. Also account for the distance from the camera's mounting face to its sensor.\u003c\/p\u003e\n\n\u003cp\u003eIf the assembly extends too far behind the telescope, the focuser may not have enough inward travel to reach focus. If the arrangement is unusually short, additional extension may be necessary.\u003c\/p\u003e\n\n\u003cp\u003eIt's a straightforward problem to solve when the measurements are known in advance, and a frustrating one to discover only after you've carried a 20-pound telescope into the backyard on the first clear night.\u003c\/p\u003e\n\n\u003ch3\u003eMounting a Five-Inch Refractor\u003c\/h3\u003e\n\n\u003cp\u003eThe FF131 is a substantial telescope. The optical tube alone weighs approximately 17.4 pounds, increasing to about 20.7 pounds when the supplied mounting rings, carry handle, and dovetail plate are installed.\u003c\/p\u003e\n\n\u003cp\u003eWith the dew shield retracted, its overall length is approximately 34.6\" in the visual configuration and 37.0\" with the photographic extension assembly. Extend the dew shield and photographic accessories, and the length can reach approximately 40.4\".\u003c\/p\u003e\n\n\u003cp\u003eThose dimensions matter when choosing a mount.\u003c\/p\u003e\n\n\u003cp\u003eA long refractor places different demands on a mounting system than a short optical tube weighing the same amount. The length gives wind and mechanical vibration more leverage, while a substantial camera assembly at the rear can shift the balance point noticeably.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131 deserves a capable equatorial or strain-wave mount with comfortable capacity for the complete imaging system. Accurate tracking, stiffness, tripod or pier stability, and wind resistance are just as important as the manufacturer's published maximum payload number.\u003c\/p\u003e\n\n\u003cp\u003eZWO offers the telescope in packages with its larger astronomical mounts, but the appropriate configuration depends on your actual camera and accessory load. Follow the mount manufacturer's instructions concerning counterweights, balancing, and allowable payloads.\u003c\/p\u003e\n\n\u003cp\u003eThe supplied detachable mounting rings and carry handle make the FF131 easier to install and remove. A 300mm dovetail mounting plate provides a useful adjustment range for positioning the optical tube in the mount saddle.\u003c\/p\u003e\n\n\u003cp\u003eThe dew shield retracts to reduce the overall length during storage and transportation, while internal baffling and anti-reflection treatment help control unwanted stray light during observing and photography.\u003c\/p\u003e\n\n\u003cp\u003eThe FF131 is portable, but it's not the sort of telescope most owners will casually pick up with one hand for a ten-minute look at the Moon. It's better suited to a thoughtfully assembled observing system, whether that means a sturdy tripod brought outside for a session or a permanent installation on a pier.\u003c\/p\u003e\n\n\u003ch3\u003eA Five-Inch Apo at the Eyepiece\u003c\/h3\u003e\n\n\u003cp\u003eFor all its photographic features, the FF131 is still a 131mm apochromatic refractor, and that makes it an appealing visual instrument as well.\u003c\/p\u003e\n\n\u003cp\u003eJupiter offers a wealth of changing detail. Its major cloud belts are relatively easy to observe, while more delicate structures, disturbances, and festoons become possible targets when the planet is high in a steady sky.\u003c\/p\u003e\n\n\u003cp\u003eWatching the shadow of a Galilean moon cross Jupiter's cloud tops is especially rewarding. These events can unfold over an evening, and the contrast between a moon's dark shadow and the bright planet makes them memorable through a good refractor.\u003c\/p\u003e\n\n\u003cp\u003eSaturn is another natural target. The rings, atmospheric banding, and some of the brighter moons are within reach, although the visibility of details such as the Cassini Division changes with the opening angle of the rings and the steadiness of the atmosphere.\u003c\/p\u003e\n\n\u003cp\u003eThe Moon may be the finest subject of all. At this aperture, the terminator reveals an extraordinary amount of topography. Crater walls, mountain peaks, ridges, and delicate shadows can keep an observer occupied for hours. On nights of exceptional seeing, small craterlets and other subtle features become worthwhile challenges.\u003c\/p\u003e\n\n\u003cp\u003eDouble stars provide another opportunity to appreciate the aperture and color correction. Attractive pairs such as Albireo are easy showpieces, while tighter pairs place greater demands on optical resolution, focusing, and atmospheric conditions.\u003c\/p\u003e\n\n\u003cp\u003eOn deep-sky objects, the additional light gathered by the FF131 makes a difference over smaller refractors. Bright globular clusters begin to show more individual stars, while open clusters, nebulae, and galaxies benefit from the greater aperture, especially at a dark observing site.\u003c\/p\u003e\n\n\u003cp\u003eAperture doesn't change the brightness of the sky or eliminate light pollution, of course. But a well-corrected five-inch refractor offers a satisfying combination of contrast, resolution, and versatility for visual astronomy.\u003c\/p\u003e\n\n\u003cp\u003eA compatible star diagonal and eyepieces are required for visual use and are sold separately.\u003c\/p\u003e\n\n\u003ch3\u003eWhat Owners Say on Cloudy Nights\u003c\/h3\u003e\n\n\u003cp\u003eAs a relatively recent addition to ZWO's flat-field refractor family, the FF131 doesn't yet have the extensive collection of long-term owner reports associated with more established telescope designs. Some early reports, however, are worth reading.\u003c\/p\u003e\n\n\u003cp\u003eIn August 2026, a Cloudy Nights member described receiving his FF131 to replace a smaller triplet refractor for galaxy photography. He planned to use it primarily for smaller and medium-sized galaxies, initially with a ZWO ASI533MC Pro and later with an ASI2600MC Pro.\u003c\/p\u003e\n\n\u003cp\u003eAfter his first imaging sessions, he reported that the stars appeared round across the corners of his ASI2600's APS-C sensor, with no obvious color fringing or camera tilt in his test images. He subsequently posted a photograph made at the telescope's native 983mm focal length and expressed satisfaction with the result.\u003c\/p\u003e\n\n\u003cp\u003eHe also noted that the telescope's larger aperture and focal length were a good match for the atmospheric seeing conditions he normally experiences. That is an important point. Buying more optical resolution than your skies can regularly support doesn't always translate into better finished photographs.\u003c\/p\u003e\n\n\u003cp\u003eThese are the observations of one owner rather than a comprehensive optical test, and performance across a full-frame sensor would require additional evaluation. Still, the report provides useful perspective on why an experienced astrophotographer might choose a five-inch, native-flat-field refractor instead of moving to an even larger or more expensive instrument.\u003c\/p\u003e\n\n\u003cp\u003eIt's a practical reminder that choosing a telescope is as much about matching equipment to your skies and the subjects you enjoy as it is about buying the largest aperture you can afford.\u003c\/p\u003e\n\n\u003ch3\u003eUnder the Night Sky\u003c\/h3\u003e\n\n\u003cp\u003eThe FF131's nearly one-meter focal length makes it particularly enjoyable when the evening sky fills with galaxies during spring.\u003c\/p\u003e\n\n\u003cp\u003eThe Whirlpool Galaxy, M51, is one of the most rewarding subjects in this part of the sky. Its recognizable spiral arms and interacting companion make an excellent photographic project, especially when several hours of exposures can be collected under steady conditions.\u003c\/p\u003e\n\n\u003cp\u003eThe Black Eye Galaxy, M64, in Coma Berenices offers a more compact but equally interesting challenge. Its dark dust feature stands out against the bright galactic core, and the surrounding galaxy benefits from careful exposure and processing.\u003c\/p\u003e\n\n\u003cp\u003eThe Great Globular Cluster in Hercules, M13, becomes favorably placed later in spring and summer. At the FF131's image scale, it offers an opportunity to record thousands of stars surrounding a densely packed central region. Careful focus and exposure are particularly important if you want the cluster to look like a collection of individual stars rather than one overly bright patch.\u003c\/p\u003e\n\n\u003cp\u003eSummer also brings the Ring Nebula, M57, in Lyra. Its bright ring is an excellent subject for a telescope of this focal length, while the much fainter outer halo presents a challenging long-integration project. The halo is significantly fainter than the familiar central ring, so specialized filtering and substantial exposure time can be helpful.\u003c\/p\u003e\n\n\u003cp\u003eThe Crescent Nebula in Cygnus provides a larger target, with an intricate shell of emission surrounding its central region. It is particularly interesting through narrowband filters, where the contrast between glowing gas and the background sky becomes much easier to record.\u003c\/p\u003e\n\n\u003cp\u003eIn autumn, the Bubble Nebula, NGC 7635, offers another attractive target. The curved boundary of the bubble is surrounded by glowing hydrogen gas, and the nearby cluster M52 can be included in wider compositions when the camera's field permits.\u003c\/p\u003e\n\n\u003cp\u003eWinter provides the Owl Nebula's planetary-nebula cousins, including the Eskimo Nebula in Gemini, while spring brings the Owl Nebula itself in Ursa Major. The Owl's two darker internal regions give the nebula its familiar appearance, and the FF131's focal length helps make them a meaningful part of the image.\u003c\/p\u003e\n\n\u003cp\u003eAt the eyepiece, there's always something worthwhile to investigate. Jupiter's changing atmosphere, Saturn's rings, the lunar terminator, and close double stars provide excellent opportunities to enjoy the telescope without attaching a camera.\u003c\/p\u003e\n\n\u003ch3\u003eObserving Tip: Balance the Complete Telescope\u003c\/h3\u003e\n\n\u003cp\u003eA long refractor with a heavy camera attached doesn't balance quite like a small optical tube with a lightweight eyepiece.\u003c\/p\u003e\n\n\u003cp\u003eBefore beginning an imaging session, assemble the FF131 with the camera, filter wheel, guider, electronic focuser, and other accessories you'll actually use. Extend the dew shield to its observing position, secure all connections, and check the balance according to your mount manufacturer's instructions.\u003c\/p\u003e\n\n\u003cp\u003eOn a conventional equatorial mount, shifting the telescope along the saddle may be necessary to obtain the proper balance in declination. A substantial camera at the rear often moves the center of gravity farther back than expected.\u003c\/p\u003e\n\n\u003cp\u003eStrain-wave mounts may have different balancing requirements from conventional equatorial mounts. Some are designed to operate without traditional counterweights within specified limits, so follow the instructions for the particular mount rather than assuming every system should balance in exactly the same way.\u003c\/p\u003e\n\n\u003cp\u003eOnce you have found a suitable position, a small removable reference mark on the dovetail can make repeat setups easier. Avoid making permanent marks on the telescope tube.\u003c\/p\u003e\n\n\u003cp\u003eCheck the arrangement again whenever you change cameras or add a substantial accessory. And don't release clutches or loosen mounting hardware unless the telescope is properly supported. A 20-pound refractor and several pounds of camera equipment deserve a little respect.\u003c\/p\u003e\n\n\u003cp\u003eOnce the balance is correct, give the optics time to approach the outdoor temperature, focus carefully, and check guiding before beginning a long sequence of exposures. At 983mm focal length, careful preparation can make a noticeable difference in the finished photograph.\u003c\/p\u003e\n\n\u003ch3\u003eFAQ\u003c\/h3\u003e\n\u003cdl\u003e\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eShould I choose the FF131 or FF110 APO?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eThe FF131 gathers approximately 42% more light than the FF110 and provides a longer 983mm focal length, compared with the FF110's 766mm. That makes it attractive for smaller galaxies, globular clusters, and planetary nebulae. The FF110 is lighter, easier to mount, and provides a wider field for medium-sized targets.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eDoes the FF131 require a separate field flattener?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eNo. Its four-element apochromatic optical system is designed to provide a natively flat field across a 44mm image circle. No separate field flattener or fixed flattener-to-camera correction spacing is required.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eCan the FF131 illuminate a full-frame camera?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eYes. ZWO specifies a 44mm image circle, sufficient to cover a conventional full-frame sensor. Camera tilt, adapter openings, and filter dimensions still matter when trying to obtain the best performance across the entire field.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eWhat back-focus distance is required?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eThe FF131 does not require one fixed correction spacing. ZWO specifies an imaging focus range of 42–73mm from the designated M48 interface and 60–91mm from the corresponding M54 interface. These are different mechanical reference points, so use the measurement appropriate to your adapter arrangement.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eWhat camera pixel size works best?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eWith 3.76-micron pixels, the image scale is approximately 0.79 arcseconds per pixel, useful for finer sampling when seeing and guiding are good. Pixels around 4.6–5 microns provide roughly one arcsecond per pixel. The best choice depends on your seeing, camera sensor, and intended subjects. Binning may provide additional flexibility with suitable cameras.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eWhat mount should I use?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eThe FF131 weighs approximately 20.7 pounds with the included mounting rings, handle, and dovetail, before adding camera equipment. Use a capable equatorial or strain-wave mount with adequate payload capacity, stiffness, and tracking accuracy. Consider the complete imaging weight and the telescope's length when choosing a mount.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eCan the FF131 be used visually?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eYes. With a suitable star diagonal and eyepieces, the FF131 can be used for observing the Moon, planets, double stars, star clusters, and brighter galaxies and nebulae. Visual accessories are sold separately.\u003c\/dd\u003e\n\n\u003cdt style=\"font-weight: bold; margin-top: 14px;\"\u003eIs an electronic focuser available?\u003c\/dt\u003e\n\u003cdd style=\"margin: 4px 0 12px 20px;\"\u003eYes. The FF131 can accept a compatible ZWO EAF electronic focuser with appropriate mounting hardware. Electronic focusing is useful for maintaining accurate focus as the nighttime temperature changes.\u003c\/dd\u003e\n\u003c\/dl\u003e\n\n\u003ch3\u003eWhat's Included\u003c\/h3\u003e\n\u003cul\u003e\n\u003cli\u003eZWO FF131 APO 131mm f\/7.5 flat-field apochromatic refractor optical tube\u003c\/li\u003e\n\u003cli\u003eDetachable mounting rings with carry handle\u003c\/li\u003e\n\u003cli\u003e300mm dovetail mounting plate\u003c\/li\u003e\n\u003cli\u003eFour-section photography extension tube with mounted 2\" filter thread\u003c\/li\u003e\n\u003cli\u003eM78x1 55mm extension adapter\u003c\/li\u003e\n\u003cli\u003eM78x1 to M54x0.75 threaded adapter\u003c\/li\u003e\n\u003cli\u003eM54x0.75 to M54x0.75 threaded adapter\u003c\/li\u003e\n\u003cli\u003eM54x0.75 to M48x0.75 threaded adapter\u003c\/li\u003e\n\u003cli\u003eManufacturer-supplied visual connection adapters\u003c\/li\u003e\n\u003cli\u003eUser manual\u003c\/li\u003e\n\u003cli\u003eInspection certificate\u003c\/li\u003e\n\u003cli\u003eWarranty card\u003c\/li\u003e\n\u003c\/ul\u003e\n\n\u003cp\u003e\u003cem\u003eEquatorial mount, imaging camera, electronic focuser, guide equipment, filters, star diagonal, and eyepieces are sold separately.\u003c\/em\u003e\u003c\/p\u003e\n\n\u003ch3\u003eOptional Accessories\u003c\/h3\u003e\n\n\u003cp\u003e\u003cstrong\u003eZWO Electronic Automatic Focuser (EAF):\u003c\/strong\u003e Provides motorized focusing and can help maintain accurate focus during long imaging sessions when used with compatible control equipment.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eZWO Off-Axis Guider and Guide Camera:\u003c\/strong\u003e Allows guiding through the main telescope's optical path, an attractive arrangement for longer focal-length photography where differential flexure can become more noticeable.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eElectronic Filter Wheel or Filter Drawer:\u003c\/strong\u003e Makes it easier to switch between broadband and narrowband filters when photographing different kinds of astronomical objects.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eMounted 2\" Astronomical Filters:\u003c\/strong\u003e The photographic extension assembly includes a compatible M48 filter thread. If using an off-axis guider, consider the location of narrowband filters so the guide camera receives enough starlight.\u003c\/p\u003e\n\n\u003cp\u003e\u003cstrong\u003eStar Diagonal and Eyepieces:\u003c\/strong\u003e Allow the FF131 to serve as a substantial visual refractor for observing the Moon, planets, double stars, and deep-sky objects.\u003c\/p\u003e\n\n\u003ch3\u003eFinal Thoughts\u003c\/h3\u003e\n\n\u003cp\u003eThere's something enduring about a five-inch apochromatic refractor. It is large enough to be taken seriously as both a visual and photographic instrument, yet still small enough that a dedicated observer can enjoy it without the infrastructure required by a truly enormous telescope.\u003c\/p\u003e\n\n\u003cp\u003eThe ZWO FF131 APO brings that tradition into modern astrophotography with a four-element optical system designed to provide a flat photographic field without a separate field flattener. Its 131mm aperture offers a meaningful increase in light-gathering ability and resolving power, while the 983mm focal length gives smaller galaxies, globular clusters, and planetary nebulae more prominence on the camera sensor.\u003c\/p\u003e\n\n\u003cp\u003eThe substantial 3\" focuser, integrated camera rotator, large rear threaded connections, and included photographic extension system make it a practical foundation for a serious imaging arrangement.\u003c\/p\u003e\n\n\u003cp\u003eIt isn't a telescope to purchase without considering the rest of your equipment. The longer focal length demands accurate guiding, the additional weight and length call for a stable mount, and the larger optical system benefits from time to adjust to nighttime temperatures. Those considerations come with moving into this aperture class, and they're worth understanding before making the investment.\u003c\/p\u003e\n\n\u003cp\u003eSomeone who primarily enjoys photographing enormous nebulae may still be happier with a shorter refractor. Someone concentrating exclusively on the tiniest galaxies may eventually want even more focal length. But for an observer who wants a substantial apochromatic refractor capable of rewarding both visual observation and detailed deep-sky photography, the FF131 offers a very appealing combination.\u003c\/p\u003e\n\n\u003cp\u003eAnd when spring comes around and the galaxies begin climbing into the evening sky again, there's a special satisfaction in having a telescope that encourages you to look a little closer.\u003c\/p\u003e\n\n\u003ch2\u003eTech Details:\u003c\/h2\u003e\n\u003ctable style=\"width:100%; border-collapse: collapse;\"\u003e\u003ctbody\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eManufacturer\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eZWO\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eModel\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eFF131 APO\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eTelescope Type\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eFlat-field apochromatic refractor\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eOptical Design\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eFour-element, fully air-spaced apochromatic optical system with integrated field flattening\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eED Glass\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eOne extra-low dispersion element; specific glass type not published\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eAperture\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e131mm (5.16\")\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFocal Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e983mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003ef\/7.5\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eImage Circle\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e44mm; designed for full-frame sensors\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eSeparate Field Flattener Required\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eNo; native flat-field optical design\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFull-Frame Field of View\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 2.1° x 1.4° with a 36mm x 24mm sensor\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eImage Scale with 3.76-Micron Pixels\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 0.79 arcseconds per pixel\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFocuser\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e3\" rack-and-pinion, dual-speed with 10:1 fine adjustment\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eCamera Rotator\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eBuilt-in 360° rear rotator\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eM48 Imaging Focus Range\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e42–73mm from specified M48 photographic interface\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eM54 Imaging Focus Range\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e60–91mm from specified M54 photographic interface\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003e1.25\" Visual Optical Path Range\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e100–131mm from the eyepiece-holder end\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003e2\" Visual Optical Path Range\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 110–142mm from the eyepiece-holder end\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eRear Thread Interfaces\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eM78x1, M54x0.75 and M48x0.75 with included adapters\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eM78 Extension\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e55mm extension adapter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003ePhotographic Extension Assembly\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eFour-section assembly with M48\/M54 adapters\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFilter Connection\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eM48x0.75 thread for mounted 2\" astronomical filters\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eDew Shield\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eRetractable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eVisual Configuration Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 34.6\" retracted; 37.9\" with dew shield extended\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003ePhotographic Configuration Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 37.0\" retracted; 40.4\" with dew shield extended\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eBare Optical Tube Weight\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 17.4 lb\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eWeight with Mounting Hardware\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eApproximately 20.7 lb with rings, handle, and dovetail\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eDovetail Plate Length\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003e300mm (11.8\"); confirm saddle-profile compatibility\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eMounting Rings\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eQuick-release clamshell-style rings with carry handle\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eFinder Mounting\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eFinder-mounting positions on handle and focuser assembly\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #f0f4f8;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eElectronic Focuser Compatibility\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eCompatible ZWO EAF with appropriate mounting hardware\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr style=\"background-color: #ffffff;\"\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc; font-weight: bold; width: 50%;\"\u003eVisual Observing\u003c\/td\u003e\n\u003ctd style=\"padding: 10px 14px; border: 1px solid #cccccc;\"\u003eSupported with suitable 1.25\" or 2\" visual accessories\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\u003c\/table\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":67754149707849,"sku":"ZWOFF131","price":1999.0,"currency_code":"USD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0573\/7974\/9961\/files\/FF130APO1_1296x_064d8830-4425-4fba-af85-91f327d91a3e.webp?v=1792513332","url":"https:\/\/astronomics.com\/products\/zwo-ff131-apo-flat-field-refractor-ota","provider":"Astronomics","version":"1.0","type":"link"}