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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
Products
2027 products
2027 products
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$539.00
1. L-eXtreme F/2 Introduction
Optolong L-eXtreme F/2 is a dual-band (500.7 nm and 656.28 nm, FWHM=7 nm) narrowband pass filter that meets the requirements for transmission at continuously varying angles. Astronomically characterised spectral lines (OIII, Ha) as the main transmission wavelengths, the OIII and H-Alpha nebula emission lines pass accurately at f2 - f3.3 Focal Ratio. It's a product that Optolong has developed specifically for fast optical systems or fast focal ratio imaging systems. It has performed well on RASA, HyperStar, and other fast ratio telescopes.
Key Features:
♦Together with one-shot colour astronomical cameras, monochrome astronomical cameras, and Digital SLR cameras, you can fast and quickly obtain clear and detailed images of the deep sky;
♦Ideal for fast optical systems, like RASA, Hyperstar, and other fast focal ratio telescope users;
♦Recommended for using a fast optical system with a focal ratio from f2 to f3.3;
♦Anti-light pollution、better contrast、more details of the celestial bodies: This filter cuts out background light and noise beyond the target celestial bodies to get better details and contrast of the images. L-eXtreme F/2 can effectively block light pollution so that the images will not affected by unwanted lights and skylight of the background. You can quickly get satisfactory pictures in fast optical systems.
2. Spectrum and Characteristic
Based on the characteristics of celestial bodies’ emission lines and light pollution emission lines, the L-eXtreme F/2 retains the prominent nebula OIII and Ha colours while blocking most of the light pollution. Specifically designed and optimally calculated for the characteristics of a fast optical system, the L-eXtreme F2 always keeps both OIII and Ha bands having high transmittance, which helps users to capture nebulae emission lines in these bands more accurately and quickly and obtain better astrophotographic images.
How to read the chart?
▲The horizontal axis is the Wavelength in Nanometers(nm).
▲The vertical axis is transmission in %.
3. Coating Technology
·Multi-layers anti-reflection coating
·Non-cementing optical substrate coating
·Optolong filter adopts precision coating based on Ion-assisted deposition coating technology for durability and resistance to scratching, as well as stability on CWL(central wavelength) no deviation affected by temperature change.
·Planetary rotation system offers precision and homogeneity of coatings ensuring high value on transmission of pass-band and Optical density of off-band.
SKU: 14803
From $420.00
L-eXtreme is a two 7nm bandpass filter which can be used with one-shot color cameras like DSLR's (digital SLR), and monochrome CCD cameras, it is also more suited for fast systems. The convenience and cost effectiveness of this filter allows amateurs to image a rich emission nebulas, even in bright, light pollution skies. Optolong believes the design of L-eXtreme filter would be better choice for fast systems in competitive price. It isolates the H-Alpha, and Oxygen III nebula emission lines so that the contrast and signal-to-noise ratio between nebulae were maximized. For people who is living in very light polluted areas, or when the moon is out, the L-eXtreme will be a good filter.
Unlike the Optolong L-eNhance filter which is a tri-band (transmits Hb, Ha, and OIII), the L-eXtreme filter is dual band that passes Ha and OIII emission lines.The advantage of the L-eXtreme filter is that there is no transmission between the H-beta and OIII lines, as there is no nebula emission lines there. In this case, it isn't letting light pollution come through so that maximize nebulas signal and make the sky background darker while imaging. The L-eXtreme filter should better isolate the emission lines only and better protect from light pollution.
Hydrogen is the largest, the most primitive, the simplest, and the oldest element in the universe. Scientists consider that Hydrogen amounts to more than 90% of visible substance in space. Our sun is 5 billion years old, but so far hydrogen is still the key matter of nuclear fusion. While the sulfur element does not have much scientific significance, so keeping H and O is meaning for exploration of life.
Therefore, we highlight H-a, H-b, O3 and O2, and reduce the signal of sulfur.
Spectrum and Characteristics
- Sbustrate: B270
- Thickness: 1.85mm
- Tpeak: T>90%
- Blocking range: 300-1000nm
- Blcoking depth: light pollution line blocking >99%
- Surface quality: 60/40
- Transmitted Wavefront RMS: λ/4
$455.00
The Optolong L-Para is a dual narrowband 10nm light pollution filter, specifically designed to filter out unwanted mercury, sodium, and LED light pollution emissions and enhance the detection of nebulae emission lines with a transmittance rate of over 85% and a 10nm FWHM for both OIII (500.7nm) and H-Alpha (656.3nm). It offers superior contrast and anti-halo effects for capturing detailed and vibrant nebulae images.
Key Features:
Broad Compatibility:
A dual narrowband filter suitable for all telescope systems, adaptable to fast optics (focal ratios of F2, F2.8, F3.2, F4) as well as various standard/normal focal ratio telescopes.
Light Pollution Resistance:
Effectively cuts off emission lines from mercury lamps, sodium lamps, LEDs, and other light pollution sources, making it applicable to Bortle Scale1- 7 dark skies.
High Transmission Rate:
In systems with a focal ratio of F2 and above, the transmittance of nebula emission lines OIII and Ha exceed 85%, resulting in higher imaging efficiency.
Excellent Contrast:
The high transmittance of nebula emission lines (OIII & Ha) combined with deep cut-off of light pollution bands significantly improves image contrast and detail richness.
Anti-Halo Characteristics:
The design has undergone several round of optimizations and many times of repeated testing ,resulting in a marked improvement in anti-halo performance, enhancing the capture of bright stars.
Optolong L-Para is a brand new dual narrowband 10nm light pollution filter. The FWHM of L-Para is 10nm for OIII (500.7nm) and H-Alpha (656.3nm) respectively. The transmittance of nebulae emission lines at are both greater than 85% in system with focal ratios of F2 and above. It effectively filters out mercury lamp, sodium lamp, and LED light pollution emission lines. At the same time, it has excellent contrast and anti-halo characteristics, allowing you to capture detailed and vivid nebula images. L-Para is suitable for both normal optical systems and fast optical systems, such as RASA and Hyperstar systems. Even when light is incident at an oblique angle, it can still maintain high transmission rates to provide you with a clear and precise shooting experience.
From $260.00
Optolong L-Pro 1.25 inch is multi-bandpass filter which offers better color balance by maximizing the transmission band. The balanced transmission allows astrophotos to be taken with minimal color cast to broadband emission objects such as galaxies, reflection nebulae and globular star clusters.
Warning - Do not use this filter for solar purposes !
Optolong L-Pro (L-Professional) filter is designed to improve the visibility of various deepsky objects. By selectively reducing the transmission of wavelengths of light pollutants, specifically those produced by artificial lightings including mercury vapor lamps, both high & low pressure sodium vapor lights and the unwanted natural light caused by neutral oxygen emission in our atmosphere (i.e. skyglow). Together with the highly transparent in main nebula emission lines at OIII(496nm and 500nm), H-beta (486nm), NII(654nm and 658nm), H-alpha(656nm) as well as SII(672nm), the filter is suitable for enhancing the contrast and details for both visual and photograghic purpose at sub-rural area with heavy light pollution.
Optolong L-Pro is multi-bandpass filter which offers better color balance by maximizing the transmission band. The balanced transmission allows astrophotos to be taken with minimal color cast to broadband emission objects such as galaxies, reflection nebulae and globular star clusters. L-Pro is the best choice for light pollution suppression.
- Optical glass fine material
- Spectrum: 380-750nm
- Surface Quality: 60/40 (Refer to MIL-O-13830)
- Fine-optically polished to ensure accurate 1/4 wavefront and < 30 seconds parallelism over the both surfaces
- High transmission at major nebula emission lines (i.e. H-alpha 656nm, OIII 496nm&500nm, SII 672nm and H-beta 486nm).
- Precision off-band blocking, specifically the major emission lines of artificial light pollution (i.e. Na 589nm, Hg 435nm and 578nm).
$329.00
L-Quad Enhance Filter (L-QEF) is a quad bandpass light pollution suppression filter for colour cameras. It effectively suppresses the transmission of light pollution wavelengths, especially light pollution generated by artificial lighting (including mercury and sodium lamps), as well as the effects of natural skylight-induced effects on the shot, thus effectively enhancing the contrast and details of the celestial bodies, and making the objects more distinct and stereoscopic. This filter provides better color balance while improving resistance of light pollution. L-QEF can be used for both wide field astrophotography, such as the Milky Way in Summer and Winter, and deep sky objects such as nebulae, galaxies, star clusters, and so forth; It allows you to save a lot of time during the shooting process and get better results at the same time. The design of quad bandpass maximises the colour balance of nebulae, galaxies and other broadband spectral targets.
Key Features:
- Cuts out light pollution from mercury and sodium lamps and produces a nice broadband image with minimal colour cast;
- Signal-to-noise ratio (SNR);
- Near IR cut-off to 1000nm, reducing the effects of IR noise;
- L-QEF has more than 90% transmittance of the nebula emission lines at H-Beta/OIII/H-Alpha/SII, with cut-off depth from OD2 to OD4, thus providing a significant increase in resistance to light pollution. L-QEF is good for night sky from Bortel 1 to Bortel 7 levels; (Bortel 8, Bortel 9 environments shall not be recommended, kindly chose Optolong other narrow-band filters, 3nm, 7nm type of filters are available.);
- Suitable for wide range of deep sky targets: it covers most nebulae, galaxies, star clusters, reflected and emitted line signals astronomical objects with higher contrast and rich details while maintaining excellent colour balance. L-QEF is superior to other filters of the same type.
Spectrum and Characteristic
| Sbustrate | optical glass |
| Thickness | 1.85mm |
| FWHM | Quad bandpass filter |
| Blocking range | 300-1000nm |
| Blocking Depth | OD2-OD4 |
| Surface quality | 60/40 |
| Transmitted Wavefront RMS | λ/4 |
| Parallelism | 30s |
Based on the characteristics of celestial bodies’ emission lines and light pollution emission lines, L-Quad Enhance filter effectively reduces the impact of light pollution and suppresses the background light of astronomical objects, thus effectively enhancing the contrast and details of the celestial bodies. Using L-QEF filter can help you save a lot of time during the shooting process, yet obtaining incredible results.
$499.00
Optolong L-Synergy Dual Narrowband Filter
The Optolong L-Synergy filter is designed for astrophotographers using DSLR, color CMOS, or CCD cameras who want to achieve stunning narrowband results without switching to a monochrome system. By pairing traditional dual-narrowband (Ha & OIII) concepts with a unique “Ha & OIII + SII & OIII” approach, L-Synergy overcomes the usual limitations of colour cameras and makes Hubble-Palette–style imaging accessible to everyone.
With this filter, you can produce deep, high-contrast SHO-like images of emission nebulae using your existing colour camera—no additional SHO filters or monochrome upgrade required. It’s an affordable way to achieve professional-level results even under bright suburban skies.
Why Choose the L-Synergy Filter?
The L-Synergy is a dual 7 nm narrowband filter engineered for telescopes with an f/ratio of f/3.3 or slower. Years of optical refinement have produced a design that suppresses bright star halos while delivering extremely high transmission in the key emission bands.
-
Selective Narrowband Performance
Transmits only the OIII (500.7 nm) and SII (672.4 nm) nebula emission lines, rejecting unwanted wavelengths and light pollution. -
Exceptional Contrast and Signal-to-Noise
By isolating the oxygen and sulfur signals, the filter produces a darker background sky and dramatically improves contrast—especially valuable in heavily light-polluted environments. -
Light-Pollution Resistant
Filters out the vast majority of urban skyglow, allowing astrophotographers to capture clean, detailed nebula structure from almost any location.
Optical Design
L-Synergy is precision-engineered based on the spectral behaviour of emission nebulae and common light-pollution sources. Its carefully tuned passbands maintain consistently high transmission in both SII and OIII, ensuring accurate colour capture and high-quality data for processing.
The result: a powerful, easy-to-use narrowband solution that unlocks deep-sky imaging performance far beyond what typical colour cameras can achieve, giving more astrophotographers access to true SHO-style imaging.
From $500.00
It's about a 3nm dual band designed to drastically reduce the effect of light pollution, the 3nm isolates the nebulae's emissions into H-Alpha (red) and OIII (green-blue). It blocks light pollution, maximizes the signal from nebulae, and darkens the sky background. It also blocks artificial light from mercury vapor lamps, high and low pressure sodium vapor lights, and unwanted natural light caused by the emission of neutral oxygen in our atmosphere. Maximizes the transmission of the main emission lines of the nebula in OIII (496nm and 500nm) and H-alpha (656nm). Used with DSLR, color/MONO CMOS and CCD, however, this filter is not suitable for fast ratio systems.
The advantage of L-Ultimate is that it only passes through the emission lines OIII(500.7nm) and Ha(656.3nm), in which case all other light pollution emission lines are eliminated so that only the emission and reflection signals of the nebula are captured during imaging. Therefore, the sky background of the image is darker, and the contrast between the nebulae and the signal-to-noise ratio are improved to the greatest extent. In heavy light pollution areas, the product can also selectively filter light pollution and clutter signals through the emission lines of nebulae, and finally avoid the impact of light pollution on astrophotography.
It is different from the series of dual-narrowband L-eNhance and L-eXtreme in that L-Ultimate is a dual-3nm bandwidth filter that only passes through Ha and OIII emission lines. You will get a darker sky background, more contrast of the image and the suppression on stars. L-Ultimate has also been optimised in terms of halo performance, so that there is no obvious halo when shooting on a bright star object.
Features
| Substrate | optical glass |
| FWHM | OIII 3nm Ha 3nm |
| Blocking range | 300-1000nm |
| Blocking | >OD4 |
| Surface quality | 60/40 |
| Transmitted Wavefront RMS: | λ/4 |
| Parallelism | 30seconds |
$919.00
Optolong L2 Dual-Combo Filter Set
The Optolong L2 Dual-Combo Set includes two premium dual-narrowband filters, L-eXtreme and L-Synergy, designed for colour-camera astrophotography. Compatible with telescopes f/3.3 and slower, this set allows users to capture Hubble Palette deep-sky images without switching to a monochrome camera or buying a full three-filter SHO set. It provides professional-level narrowband imaging with minimal investment.
The L-eXtreme transmits OIII (500.7 nm) and Hα (656.3 nm), blocking unwanted light-pollution wavelengths to deliver bright nebula details with high contrast. Years of refinement optimise performance and reduce bright star halos.
The L-Synergy transmits OIII (500.7 nm) and SII (672.4 nm) with high efficiency while rejecting other wavelengths. It minimises light pollution effects and preserves nebula detail, producing clean data for processing.
The combination of these filters allows colour-camera users to achieve Hubble Palette imaging efficiently. It enhances nebula structure, improves contrast, and enables richer colour separation in light-polluted skies.
The filters are engineered to preserve the distinctive colours of nebulae while filtering out most light pollution. Their tuned transmission profiles ensure strong signal in the target emission lines and high signal-to-noise performance for detailed deep-sky images.
This set is ideal for astrophotographers using colour cameras who want professional-quality narrowband imaging with existing equipment.
From $400.00
Optolong LRGB filter set is designed for maximum contrast and with extremely high gradients for clear differentiation of colors. The LRGB filter set divides the spectrum into its components red, green, blue and luminance.
OIII emission overlaps on blue and green filters with maximum transmission to allow high efficiency and natural color imaging. Gap between green and red filters serves to block out the primary Sodium light pollution line at 589nm and improves color balance and separation.
- RGB, parfocal:1:1:1
- Creat images in their true original colors showing a wealth of natural detail;
- Steep bandpass filters to eliminate UV and IR interference;
- Include Luminance (UV/IR Cut), Red, Green, and Blue filters to reproduce the star's color
From $99.00
The UHC (Ultra High Contrast) broadband filter is designed to improve the visibility of various deepsky objects. By selectively reducing the transmission of wavelengths of light pollutants, specifically those produced by artificial lightings including mercury vapor lamps, both high & low pressure sodium vapor lights and the unwanted natural light caused by neutral oxygen emission in our atmosphere (i.e. skyglow). Together with the highly transparent in main nebula emission lines at OIII(496nm and 500nm), H-beta (486nm), NII(654nm and 658nm), H-alpha(656nm) as well as SII(672nm), the filter is suitable for enhancing the contrast and details for both visual and photograghic purpose at sub-rural area with heavy light pollution.
Main Use and Performance
Suitable for color CCD cameras and unmodified DSLRs.
UHC with narrower passband provides higher contrast than CLS. Thus it is more suitable for urban environment where you suffer from severe light pollution.
UHC has a substantial red passband and offer superb views for objects like the Orion Nebula (M42).
Light pollution filter do not eliminate the effects of light pollution or increase the object’s brightness. In many cases, they increase the contrast between nebula and night sky, not brightening the nebula.
WARNING: The filters of Optolong are not designed for sun observation. DO NOT LOOK AT THE SUN WITH OPTOLONG FILTER. You would be BLIND if you fail to observe the warning.
| Sbustrate | optical glass |
| Tave | >95% |
| Blocking range | 300-700nm |
| Blcoking depth | OD3, light pollution line blocking >99% |
| Surface quality | 60/40 (Refer to MIL-O-13830A, MIL-C-48497A) |
| Transmitted Wavefront RMS | ¼ λ |
| Parallelism | 30s |
From $80.00
Optolong UV/IR Cut filter is designed for ultraviolet and infrared wavelength blocking to improve sharpness of the image as most of the optics are designed for the visible spectrum, because it’s very difficult to create a lens with the same focal point for the visible and IR spectrum.
It is used on a digital camera and the video, which do not have an IR protection filter toward an image sensor or were remodeled. This is important because unfiltered CCD and CMOS sensors are extremely susceptible to UV and IR rays just outside the visible spectrum that can have a very negative impact on image quality.
Main Use and Performance
Suitable for color CMOS and CCD cameras and modified DSLRs.
Use with monochrome CCD for astrophotography.
Available to assist in focusing.
Act as an outstanding dust shield, which prevents the possibility of dust settling on the lens during long time exposure.
WARNING: The filters of Optolong are not designed for sun observation. DO NOT LOOK AT THE SUN WITH OPTOLONG FILTER. You would be BLIND if you fail to observe the warning.
From $65.00
Adjust the brightness level of the Moon, Venus, and other bright objects with the Optolong Variable Polarizer. A standard Moon Filter is similar to a pair of sunglasses. They work fine, but sometimes the scene is too dark or too bright, and there’s not a lot you can do about it. A variable polarizing filter is much more flexible than a Moon filter. It allows you to set the percentage of attenuation by turning the top section of the two-piece filter. Simply attach the 2" threaded filter to a like-sized eyepiece or Astro accessory barrel, and then slowly rotate the top half of the filter—it turns 360°—to achieve the results you desire.
The Optolong Variable Polarizing Filter also works great to cut brightness when you are using your telescope for terrestrial observations or photography. If you have ever done photography through a SLR or DSLR camera, you may have already been introduced to the qualities of a polarizing filter, since it is a very popular accessory for polarizing the light and making the sky appear bluer. You will especially appreciate a polarizing filter when viewing over water or photographing a scene that includes a river or body of water. Simply turn the filter until you achieve the most glare-free results—you will really see the difference.
| 1.25 inch | 2 inch | |
| Brand | Optolong | Optolong |
| Type | Variable Polarizing | Variable Polarizing |
| Substrate Thickness | 2mm | 2mm |
| Clear Aperture | 26mm | 44mm |
| Surface Quality | 60/40 | 60/41 |
| Surface parallelism | 1/4λ | 1/4λ |
| Parallelism | 30" | 30" |
| Thread | M28.5*0.6 | M48*0.75 |
| Single Thread | Yes | Yes |
$219.00
This Orion Heating Band Large 9.25-12 inch telescopes is highly power efficient, drawing only 2.5 amps at maximum output.
Unlike competing dew-prevention systems, the Orion Dew Zapper Pro's heating bands have right-angle cable connections to reduce cable strain and provide a tighter fit. Hook-and-loop fasteners hold the bands snugly around your telescope and accessories. This heating band comes with a 6'-long cable that plugs into the control module via an RCA-type connector. Removable caps are included to protect any unused ports from exposure to the elements.
Don't let high humidity or dew dampen your spirits — or your optics. Buy the Orion Dew Zapper Pro today! Made in the U.S.A.
SKU: 03522
$169.00
This Orion Heating Band Medium 6-8 inch telescopes is highly power efficient, drawing only 1.69 amps at maximum output.
Unlike competing dew-prevention systems, the Orion Dew Zapper Pro's heating bands have right-angle cable connections to reduce cable strain and provide a tighter fit. Hook-and-loop fasteners hold the bands snugly around your telescope and accessories. This heating band comes with a 6'-long cable that plugs into the control module via an RCA-type connector. Removable caps are included to protect any unused ports from exposure to the elements.
Don't let high humidity or dew dampen your spirits — or your optics. Buy the Orion Dew Zapper Pro today! Made in the U.S.A.
$155.00
The Orion Illuminated Plossl 12.5 mm eyepiece is a vital addition to any astronomer's equipment collection thanks to its many useful applications.
Achieve precise alignment of computerized GoTo systems easily by using the relatively high-power 12.5 mm focal length eyepiece to accurately center alignment stars. The illuminated reticle enables you to precisely center alignment stars and objects in the telescope, thus increasing the accuracy of the GoTo system.
The 4-element Plossl design is also well suited for off-axis guiders, where light gathering is minimal, to help ensure tracking accuracy during guided astrophotography sessions. Use the 12.5 mm Illuminated Plossl with an off-axis guider (sold separately) to keep a guide star centered precisely to capture tack-sharp astrophotos.
A 4-element Plossl design with fully multi-coated lenses ensures bright views through the illuminated reticle eyepiece. Its 40° apparent field is ideal for multiple functions. The LED-illuminated double crossline reticle has adjustable focus and brightness. Three GP-189 batteries (included) are required for illuminator operation. Also compatible with three SR-54, SG-10, or equivalent button-cell batteries (not included). The Orion Illuminated Plossl 12.5 mm eyepiece features a 1.25" barrel diameter, compatible with 1.25" telescope focusers, or 2" focusers equipped with a step-down 1.25" adapter.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU: 08450
$29.00
The largest planet in our solar system is a joy to explore with a telescope, and the Orion Jupiter Map & Observing Guide is loaded with educational information and tips to help you get the most out of each and every view of Jupiter. With its bold equatorial cloud belts and swirling storms including the famous Great Red Spot, the planet Jupiter is an ideal telescopic target for beginners and experienced stargazers alike. The Orion Jupiter Map & Observing Guide is packed with observing tips, filter recommendations for viewing and imaging Jupiter, and features beautifully detailed images of the gas giant planet. Use it along with your telescope to identify Jovian atmospheric features including belts, zones, regions, and bright and dark features using official nomenclature.
Jupiter's four brightest moons; Io, Europa, Callisto and Ganymede, provide backyard astronomers with a different view each night as they orbit the gas giant planet in a celestial dance. The Jupiter Map & Observing Guide includes a list of helpful hints for observing Jupiter's Galilean moons, and features an illustrated selection of rare Jovian moon events from 2014 to 2020, making it easy to plan observing sessions so you don't miss any of these unique moon formations around the gas giant planet. This ideal tool for observing Jupiter even includes lists of all oppositions, conjunctions, and even asteroid flyby events from 2014 to 2020.
The Jupiter Map & Observing Guide measures 25.25" x 11" when fully unfolded, and folds up to 8.5" x 11". The tri-fold Jupiter Map & Observing Guide is plastic laminated for long-lasting durability as well as protection against dew, dirt, and the occasional coffee spill.
- Includes lists of all Jupiter oppositions, observable conjunctions from 2014 to 2020
- Features an illustrated selection of rare Jovian moon events from 2014 to 2020
- Plastic-laminated for durability, the Jupiter Map measures 25.25" x 11" when fully unfolded, and folds up to 8.5" x 11" for easy portability
$29.00
Have you ever wanted to explore Mars, the planet next door to our own? With this detailed Map, you finally can- as complete as it can be with our current knowledge of the Martian terrain, the Orion Mars Map and Observing guide will be of great aid in locating and identifying the many intriguing martian features there are to find on this planet. This useful tool is ideal for any amateur astronomer looking to get more out of their telescopic observations of Mars- the map not only identifies the classical albedo features observable through a telescope, it also identifies over 150 Martian Features using modern nomenclature. Throughout the tri-fold of the map and observation guide, you can find heaps of information on the dust clouds and storms, polar ice caps, and seasons of Mars. The guide also includes information on optimal filters recommended to help enhance visual views and photos of mars- and to top it all of, it contains a detailed list of all upcoming conjunction and opposition events
$29.00
Orion Moon Map 260 | Orion Telescopes and Binoculars Orion Moon Map 260 | Orion Telescopes and Binoculars
- The meticulously detailed Moon Map 260 is a must-have for any backyard astronomer
- Map identifies over 260 lunar features including craters, valleys, ancient lava flows, mountain ranges, all successful US and Soviet lunar mission landing sites, and more
- Conveniently laminated for protection against dew, dirt, and the elements
- Measures 25.25″ x 11″ when fully unfolded, and folds up to 8.5″ x 11″ for easy portability
- Includes both correct-image and reversed “mirror image” maps of the Moon for easy use with binoculars, unaided eyes, or any telescope
Orion Moon Map 260 | Orion Telescopes and Binoculars
The bright face of our planet’s Moon has been inspiring astronomers for centuries. Since the Moon is much closer to Earth than any other object in the night sky, views of its illuminated surface are amazingly detailed when observed through binoculars or a telescope. Intriguing craters, craggy mountains, and vast “seas” of ancient lava flows make for wonderful targets for backyard astronomers. With the affordable Orion Moon Map 260, you can easily identify, locate and learn about the many interesting features of Earth’s only natural satellite.
The Moon Map identifies over 260 of the most popular lunar surface features including craters, mountain ranges, valleys, rilles, “seas” and more. Each feature is cross-referenced in the MoonMap’s tables with its official name, size and a brief description. In addition to lunar landscape features, all successful spacecraft landing sites from US Apollo, Surveyor and Ranger Probe missions as well as Soviet Luna Probe missions are also clearly identified on the map.
We’ve designed the Orion MoonMap 260 with versatility in mind. Both a correct-image and reversed, or “mirror image” view of the Moon are included on the map, so it can be used when observing the Moon with unaided eyes, binoculars; or any refractor, reflector, or Cassegrain telescope. The map is conveniently laminated for use in almost any weather.
Using the Moon Map 260 is easy. Simply find the reference number of the lunar feature you wish to identify on the map, and then look up its name using the map’s numerical index. Conversely, if you wish to locate a specific named feature with your telescope or binoculars, use the map’s numerical index to find the lunar feature’s reference number, then locate the number and feature on the map. For ease of use, the reference numbers are roughly ordered from north to south (top to bottom).
The Orion MoonMap 260 measures 25.25″ x 11″ when fully unfolded, and folds up to 8.5″ x 11″. The tri-fold MoonMap 260 is plastic laminated for long-lasting durability as well as protection against dew, dirt, and the occasional coffee spill.
Whether you’re an experienced amateur astronomer or a novice just beginning to explore the night sky, the MoonMap 260 will help you make each moonlit night more memorable. It’s a must-have for any of our fellow “Luna”tics!
$109.00
Orion narrow dovetail plate (Vixen Style) is made of extruded, black anodized aluminum. With several holes and two long slots, this versatile plate is ideal for mounting telescope and guide scope tube rings, cameras, finder scopes, and other accessories.
Near the center of the plate are two counterbored through holes and two M6x1 threaded holes. Two long slots are also counterbored underneath so that the heads of standard socket head cap screws are recessed under the bottom surface of the plate.
Both the through holes and slots can accommodate 1/4"-20 socket head cap screws and some smaller sizes. The slots make it easy to accommodate the needed spacing between two tube rings for different telescope and guide scope configurations.
Two holes on each end of the plate have M6x1 threads also.
With the Orion narrow dovetail plate, you'll have a secure connection and perfect placement ? no matter what tube you're using to explore the universe!
$59.00
When placed over the front of a telescope, handy Orion PinPoint Telescope Focusing Masks make it easy to achieve quick and precise focusing without guesswork. Also known as Bahtinov masks, these focus aids feature a laser-cut slot pattern that produces a distinct, intersecting 3-line pattern once accurate focus is achieved in any type of telescope.
Orion PinPoint Focusing Masks will help astrophotographers save time and avoid frustrating, fuzzy results caused by slightly defocused exposures. With a PinPoint Mask installed on an imaging telescope, just focus on any bright star within or near the celestial object you want to photograph and adjust focus until the intersecting 3-line pattern is displayed indicating precise focus has been achieved. Wow, that was fast! Besides astrophotographic applications, PinPoint Focusing Masks are also useful for visual observations when fast, tack-sharp focusing is desired.
Precise focus is achieved when the middle spike is exactly centered in the "X" pattern.
Three Orion-exclusive adjustable rubber-sleeved pegs equipped with thumbscrews clamp onto the outside of your telescope tube or dew shield to hold the PinPoint Mask firmly in place. Orion PinPoint Focusing Masks are easy to install and remove so you can achieve precise focus and quickly start capturing astrophoto exposures.
Each Orion PinPoint Focusing Mask can fit a range of telescope tube diameters. For example, this 118-153mm ID Orion PinPoint Focusing Mask will fit telescope tubes with an outer diameter ranging from 118mm to 153mm (4.64" to 6.02").
Made of laser-cut black plastic. Flat for easy storage and transport.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU:40007
$65.00
When placed over the front of a telescope, handy Orion PinPoint Telescope Focusing Masks make it easy to achieve quick and precise focusing without guesswork. Also known as Bahtinov masks, these focus aids feature a laser-cut slot pattern that produces a distinct, intersecting 3-line pattern once accurate focus is achieved in any type of telescope.
Orion PinPoint Focusing Masks will help astrophotographers save time and avoid frustrating, fuzzy results caused by slightly defocused exposures. With a PinPoint Mask installed on an imaging telescope, just focus on any bright star within or near the celestial object you want to photograph and adjust focus until the intersecting 3-line pattern is displayed indicating precise focus has been achieved. Wow, that was fast! Besides astrophotographic applications, PinPoint Focusing Masks are also useful for visual observations when fast, tack-sharp focusing is desired.
Precise focus is achieved when the middle spike is exactly centered in the "X" pattern.
Three Orion-exclusive adjustable rubber-sleeved pegs equipped with thumbscrews clamp onto the outside of your telescope tube or dew shield to hold the PinPoint Mask firmly in place. Orion PinPoint Focusing Masks are easy to install and remove so you can achieve precise focus and quickly start capturing astrophoto exposures.
Each Orion PinPoint Focusing Mask can fit a range of telescope tube diameters. For example, this 138-173mm ID Orion PinPoint Focusing Mask will fit telescope tubes with an outer diameter ranging from 138mm to 173mm (5.43" to 6.81").
Made of laser-cut black plastic. Flat for easy storage and transport.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU:40008
$69.00
When placed over the front of a telescope, handy Orion PinPoint Telescope Focusing Masks make it easy to achieve quick and precise focusing without guesswork. Also known as Bahtinov masks, these focus aids feature a laser-cut slot pattern that produces a distinct, intersecting 3-line pattern once accurate focus is achieved in any type of telescope.
Orion PinPoint Focusing Masks will help astrophotographers save time and avoid frustrating, fuzzy results caused by slightly defocused exposures. With a PinPoint Mask installed on an imaging telescope, just focus on any bright star within or near the celestial object you want to photograph and adjust focus until the intersecting 3-line pattern is displayed indicating precise focus has been achieved. Wow, that was fast! Besides astrophotographic applications, PinPoint Focusing Masks are also useful for visual observations when fast, tack-sharp focusing is desired.
Precise focus is achieved when the middle spike is exactly centered in the "X" pattern.
Three Orion-exclusive adjustable rubber-sleeved pegs equipped with thumbscrews clamp onto the outside of your telescope tube or dew shield to hold the PinPoint Mask firmly in place. Orion PinPoint Focusing Masks are easy to install and remove so you can achieve precise focus and quickly start capturing astrophoto exposures.
Each Orion PinPoint Focusing Mask can fit a range of telescope tube diameters. For example, this 158-193mm ID Orion PinPoint Focusing Mask will fit telescope tubes with an outer diameter ranging from 158mm to 193mm (6.22" to 7.59").
Made of laser-cut black plastic. Flat for easy storage and transport.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU:40009
$75.00
When placed over the front of a telescope, handy Orion PinPoint Telescope Focusing Masks make it easy to achieve quick and precise focusing without guesswork. Also known as Bahtinov masks, these focus aids feature a laser-cut slot pattern that produces a distinct, intersecting 3-line pattern once accurate focus is achieved in any type of telescope.
Orion PinPoint Focusing Masks will help astrophotographers save time and avoid frustrating, fuzzy results caused by slightly defocused exposures. With a PinPoint Mask installed on an imaging telescope, just focus on any bright star within or near the celestial object you want to photograph and adjust focus until the intersecting 3-line pattern is displayed indicating precise focus has been achieved. Wow, that was fast! Besides astrophotographic applications, PinPoint Focusing Masks are also useful for visual observations when fast, tack-sharp focusing is desired.
Precise focus is achieved when the middle spike is exactly centered in the "X" pattern.
Three Orion-exclusive adjustable rubber-sleeved pegs equipped with thumbscrews clamp onto the outside of your telescope tube or dew shield to hold the PinPoint Mask firmly in place. Orion PinPoint Focusing Masks are easy to install and remove so you can achieve precise focus and quickly start capturing astrophoto exposures.
Each Orion PinPoint Focusing Mask can fit a range of telescope tube diameters. For example, this 178-213mm ID Orion PinPoint Focusing Mask will fit telescope tubes with an outer diameter ranging from 178mm to 213mm (7.0" to 8.38").
Made of laser-cut black plastic. Flat for easy storage and transport.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU:40010
$49.00
When placed over the front of a telescope, handy Orion PinPoint Telescope Focusing Masks make it easy to achieve quick and precise focusing without guesswork. Also known as Bahtinov masks, these focus aids feature a laser-cut slot pattern that produces a distinct, intersecting 3-line pattern once accurate focus is achieved in any type of telescope.
Orion PinPoint Focusing Masks will help astrophotographers save time and avoid frustrating, fuzzy results caused by slightly defocused exposures. With a PinPoint Mask installed on an imaging telescope, just focus on any bright star within or near the celestial object you want to photograph and adjust focus until the intersecting 3-line pattern is displayed indicating precise focus has been achieved. Wow, that was fast! Besides astrophotographic applications, PinPoint Focusing Masks are also useful for visual observations when fast, tack-sharp focusing is desired.
Precise focus is achieved when the middle spike is exactly centered in the "X" pattern.
Three Orion-exclusive adjustable rubber-sleeved pegs equipped with thumbscrews clamp onto the outside of your telescope tube or dew shield to hold the PinPoint Mask firmly in place. Orion PinPoint Focusing Masks are easy to install and remove so you can achieve precise focus and quickly start capturing astrophoto exposures.
Each Orion PinPoint Focusing Mask can fit a range of telescope tube diameters. For example, this 58-83mm ID Orion PinPoint Focusing Mask will fit telescope tubes with an outer diameter ranging from 58mm to 83mm (2.28" to 3.27").
Made of laser-cut black plastic. Flat for easy storage and transport.
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only.
SKU:40004
$29.00
The affordable Orion Saturn Map & Observing Guide is a wonderful tool for backyard astronomers of all skill levels who want to enrich their observations and understanding of this unique gas giant planet and its spectacular ring system. We've packed the tri-fold Saturn Map & Observing Guide with beautiful images and useful tips to help you get the most out of each view of Saturn. With this Map & Observing Guide at your side, you'll learn interesting information about Saturn's many moons, its extensive ring system, ring tilt cycle, and more. The Map will help you learn to identify light and dark atmospheric features of Saturn using official nomenclature. You'll appreciate the thorough list of recommended filters to help enhance visual views and astrophotos of Saturn, and the detailed list of all upcoming conjunctions and oppositions of Saturn from 2014 through 2020 will help you plan ahead to catch these interesting events.
The Saturn Map & Observing Guide measures 25.25" x 11" when fully unfolded, and folds up to 8.5" x 11". The tri-fold Saturn Map & Observing Guide is plastic laminated for long-lasting durability as well as protection against dew, dirt, and the occasional coffee spill.
- Includes lists of all Saturn oppositions, observable conjunctions from 2014 to 2020
- Lists best filters for visual observation and astrophotography of Saturn
- Plastic-laminated for durability, the Saturn Map measures 25.25" x 11" when fully unfolded, and folds up to 8.5" x 11" for easy portability
Born and raised in remote Broken Hill, Trevor Barry left school after year ten to work in the mines. Years later, a single glimpse of Saturn through a colleague's telescope knocked Trevor's world completely off its axis, turning his whole life upside down.
With his newfound passion and armed with decades of outback know-how, Trevor set about building an observatory in his backyard using bits and pieces from his shed, a second-hand washing machine motor, rainwater tank parts and an old catamaran wire. It took some canny negotiations with his wife, Cheryl, 'the Gorgeous and Adorable', whose prized garden took a battering - especially when he decided to add a second storey - but before long Trevor was not just gazing at the stars but capturing extraordinary images of the planets.
Over the years, Trevor's love affair with Saturn, 'the ringed jewel of the solar system', only grew more passionate, and in his early fifties he did a degree in astronomy, topping his class.
When he recorded a massive storm on Saturn from his backyard observatory, he alerted NASA. The world's greatest space agency took note and invited Trevor to contribute to its interplanetary research - leading to opportunities far beyond Broken Hill and even Trevor's wildest dreams.
Today, when he's not tending the greens at his local bowls club, Trevor can usually be found in his backyard, collecting data for international research projects. His work is held in high regard by professional astronomers, and his observations are published in peer-reviewed scientific journals around the world.
About Trevor
Trevor Barry has called Broken Hill home his whole life. At 17, he started work in the local mines and built a good life there, married to his high school sweetheart, Cheryl, the Gorgeous and Adorable. But then Trevor fell in love again - not with Cheryl, but with a planet: Saturn. Just one look through a telescope changed his life forever. First he built his own telescope, and then an observatory - until finally, at 51, Trevor decided to gaze at the stars full time and enrolled at university to study astronomy. He now collects data vital to NASA research and is renowned for his extraordinary photographs of the planets.
$5,910.00
The Helium ME400 Red Tripod is ideal for portable Paramount use and is available for the Paramount MEII and ME6 models:
- Provides a stable platform for all your equipment
- Helium ME400 has a maximum payload capacity of 180 kg when the legs are fully extended, or up to 227 kg capacity when the legs are fully retracted
- Allows eyepiece placement at a convenient height with an adjustable height range Helium ME400 from 61cm to 100 cm.
- The ultra-portable and lightweight design weighs in at 14kg
Helium MX400 Features
- Simple and intelligent mechanics permit the legs to be expanded or collapsed in seconds and produce exceptional stability at all heights
- The top plate rotates 360 degrees for hassle-free polar alignment in azimuth.
- A wide range of coarse leveling adjustments can accommodate gently sloping surfaces.
- Fine-level adjustments help achieve the optimal level
- Swiveling feet can be fit with spikes or other third-party commercial tripod feet based on your observing site (grass, wood, concrete, gravel, etc.)
- Built-in bubble level helps quickly get the top plate horizontal.
- The 6061 aluminum tripod legs are red anodized with black anodized aluminum structural components (top plate, feet, etc.)
- Large tray between the legs conveniently stows your eyepieces and other equipment
- Legs accept many off-the-shelf tripod feet (including spikes, and wide rubber pads) to optimize coupling to the observing surface
The result of these innovative features is an exceptionally stable and readily portable imaging platform that can be quickly set up on any surface, leveled and aligned with the celestial pole, and easily taken down each night.
$1,799.00
The Paramount ME II Large Dovetail is an optional accessory that enables the Paramount ME II’s Versa-Plate to accept optical tube assemblies that use the Planewave Instrument dovetails (including PlaneWave Instruments and Officina Stellare telescopes).
The large dovetail is rated to carry 108 kg.
Total additional weight is 1.5kg
This unit is included in the Multi OTA Mounting Kit
$4,500.00
The Multi-OTA Mounting Kit includes:
- Paramount ME II Versa-Plate Spacers
- Paramount ME II Large Dovetail Rails
- One Side-by-Side Adaptor plate
When the Paramount ME II Versa-Plate is rotated to the wide orientation, these components can be used to attach two or more ring-mounted optical tube assemblies.
From $36,350.00
Introducing the new Paramount ME Series 6 observatory workhorse.
The Paramount ME Series 6 represents the latest in gear-driven GEM performance.
Its new features include a state-of-the-art MKS 6000 telescope control system that lets you connect via USB C, Ethernet, and Wi-Fi. Its two-port USB 2.0 hub is conveniently located on the instrument panel
The Paramount ME Series 6 remains an observatory favorite among professional and advanced-amateur astronomers.
On-axis Absolute Encoders vs. Motor-based Encoders.
Paramount's equipped with on-axis absolute encoders know where they are at all times. Paramount's with incremental encoders (or motor-based encoders) know only how far they have moved since they were initialized using a nightly process called homing.
The crucial additional difference is that the on-axis absolute encoders are fitted directly to the mount axes themselves, bypassing the worm drives. Paramount's with incremental encoders are fitted to the worms instead, which means that with incremental encoders alone, periodic errors in the worm drive show up in the tracking. These mounts must be calibrated and corrected using a process called periodic error correction (PEC), which measures and records the repeatable gear train errors and removes them. (TheSky features advanced, multi-harmonic PE detection and PEC calibration that minimizes periodic error in mounts with incremental encoders.)
For mounts with incremental encoders, homing re-zeros the encoders when precise sensors on each of the axes are reached. From then on, the incremental encoders are in effect delivering absolute readings.
However, the crucial additional difference remains, namely that the incremental encoder system is behind the worm drive, and periodic error correction is still required to get the best out of the RA tracking.
High-resolution on-axis absolute encoder technology is significantly more expensive than incremental encoders.
Are on-axis absolute encoders right for me ?
The short answer is, “it depends.”
Gear-driven Paramounts equipped with on-axis absolute encoders do not have periodic error, require no mechanical initialization (or homing), and the number of TPoint pointing samples needed for precision calibration is reduced.
These advantages expedite nightly setup, negate one-time periodic error training, and shorten the calibration process require to achieve spectacular pointing and tracking performance. However, the Paramount worm gear's uncorrected periodic error is low (below 7 arc seconds peak to peak), and, after a one-time PE training, periodic error correction (PEC) generally make it negligible. The Paramount without on-axis absolute encoders requires a nightly Find Home process that usually takes a minute or less to complete.
So, at least with Paramounts, periodic error is effectively in the noise, and homing straightforward.
What about pointing and tracking?
Without on-axis absolute encoders, Paramounts routinely produce 5-to-10-minute unguided exposures; many have reported 20 minutes. Also without on-axis absolute encoders, Paramount’s produce all-sky pointing accuracies at or below 30 arcseconds RMS (usually less than 15 arcseconds on fixed mirror telescopes).
Paramount’s exceptional software makes the above performance possible. TheSky Professional edition, in conjunction with TPoint™ and ProTrack™ the mount’s position is continually updated in both axes to correct system-wide pointing and tracking errors caused by tube flexure, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders and/or worm gears, and more.
On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior pointing and tracking.
So are on-axis absolute encoders right for you? Perhaps if you want to enjoy the conveniences mentioned above. And for many, that’s enough. With that said, the optional on-axis 26-bit Renishaw absolute encoders with 0.02 arc second precision are the finest available and they operate in temperatures between +80°C and –40°C.
Hardware Specifications
- 109 kg instrument capacity; 218 kg maximum payload capacity (instruments + counterweights)
- All sky pointing accuracies at or below 30 arcseconds RMS
- Unibody mount design weighs 38 kg without counterweights or counterweight shaft
- Maximum seven (7) arcseconds peak-to-peak periodic error before correction
- After a one-time training, periodic error is 1 arcsecond, peak-to-peak or less
- Optional 26-bit Renishaw encoders eliminate periodic error and the need for homing; operates in temps as low as –40° C
- If you skip encoders now and later decide you want them, they can be retrofitted on the Paramounts ME Series 6
- As there’s some confusion about what encoders can and cannot do, there’s an FAQ below that elaborates on that and whether they’re right for you
- Its encoder cables are located inside the mount to help prevent snags.
- All electronics and through-the-mount cables are housed inside the mount with ample room for additional cables
- Its state-of-the-art MKS 6000 telescope control system (TCS) lets you connect via USB C, Ethernet, and Wi-Fi
- Two-port USB 2.0 hub located on instrument panel
- Included Versa-Plate™ conveniently accepts most telescopes
- 48V DC power supply and PC-to-mount USB and Ethernet cables included
- Two 14 kg counterweights included. You may need more if your imaging system weighs more than 28 kg.
- Belt-driven gears with spring loaded worm gears produce virtually zero backlash
- Durable and fade-resistant red powder coating and black anodized finish; components are aluminum
- Clutch-free design helps maintain its TPoint™ assisted pointing accuracy
- AutoHome™ homing capability ensures the mount always knows its orientation (after performing an initializing process called “homing” that typically takes less than a minute)
- Calibrated azimuth and elevation polar alignment adjustments speed polar alignment
Software Specifications
- Paramount’s unequaled pointing and tracking wouldn’t be possible without its TPoint™ and ProTrack™ software.
- By employing TPoint’s calibration and telescope modeling tools, you’ll enjoy all sky pointing accuracies at or below 30 arcseconds RMS. Nothing outperforms that
- Operating in conjunction with TPoint ™, ProTrack™ continuously updates the mount’s position across both axes to correct system-wide tracking errors including tube flexures, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders, and more.
- On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior tracking.
- Without encoders, the Paramount ME Series 6 can deliver uncommonly long unguided exposures (one customer reported 20 minutes).
- For more information about what encoders can and cannot do, please see the FAQ below.
- All the included software is integrated into a single, easy-to-use, application consisting of TheSky™ Professional, TPoint™, Cameras+, Domes, Multi-OS+, and Weather modules.
- You can control all your astrophotography-related cameras and devices with this one app.
- It runs on macOS™, Windows™, Ubuntu™, and Linux (x86_64 and ARM64 architectures).
- Regardless of the operating system you run it on, it appears and operates identically. You can even switch between operating systems and its license allows up to six computers. Why paint yourself or your institution into a corner?
- Absent ProTrack™ which is unique to Paramount, the included software is sold separately as TheSky™ Universal Bundle and represents a US$1,095 value.
SKU: SB10616
Optional Black Anodised mounts available on request
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