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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
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2026 products
2026 products
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$29.00
AUTHOR:
David Hawcock studied art in York, UK, majoring in graphic design. He opened a design studio in Bath specialising in children's books. He has designed and produced many successful pop-ups, which have sold hundreds of thousands of copies, including The Amazing Fold-Out Pop-Up Body in a Book and the Journal of Inventions: Leonardo Da Vinci.
$267.00
FUNCTIONAL PROTECTION FOR YOUR SPOTTING SCOPE
Innovative and perfectly tailored accessories not only enhance the capabilities and functionality of your SWAROVSKI OPTIK spotting scope, they also help to protect it. User-oriented concepts and design both play an important role.
SOC stay-on case 115 objective module
The perfect case for the 115 mm objective module. The close-fitting stay-on case protects the scope against impact even in demanding conditions.
$22.99
Diagrams drawn for the latitude of southern Australia, but including events visible from New Zealand and South Africa.
Written and illustrated by astronomical experts.
Content includes:
- Advice on where to start looking
- Easy-to-use star maps for each month with descriptions of what to see
- Special, detailed charts for positions of planets, minor planets and comets in 2026
- Seasonal charts
- Details of dark sky sites
- Details of objects and events you might see in 2026
- Diagrams of notable events visible from Australia, and some for New Zealand and South Africa
Conduct dozens of your own experiments with the 28 Piece Celestron Microscope Kit. Includes a metal bodied microscope with 3 objective lenses (100x, 600x, and 1200x). Examine the 5 prepared slides or create your own using the 7 blank slides and cover slips. Also includes fun accessories like a 2x magnifying glass, plastic scalpel, and more.
- Beginner set with metal bodied biological microscope
- Blow molded, rugged carry case for portability and protection
- 3 objective lenses for high power viewing - 100x, 600x, and 1200x
- 7 blank slides, 5 prepared specimen slides, and 7 slide cover slips and labels
- Multiple lab accessories to get you experimenting right away:
- Plastic scalpel
- Tweezers
- Pointer
- 2x magnifier
- Sea salt samples
$15.00
This V-Style Dove tail bar is designed for DSLR camera attachment.
Attach the yellow dovetail bar to the DSLR camera body using the supplied ¼” inch screw.
Like all tripods or camera mounting systems, do not over-tighten the ¼” inch screw to avoid possible damage to the camera body.
Loosen the side clamps on the Sky-Watcher Star Adventurer GTI mount head and slide the yellow bar with the camera body into the mount head. Tighten both mount clamps to secure the camera.
Again, please don’t over-tighten the mount clamps.
Able to support 3kg total weight.
Tools you’ll need:
A 4mm or 3/16th Inch Allen Key
$31.00
A Star Explodes is about the supernova of 1054 was one of the brightest supernova events recorded in history. And its remnant, the Crab Nebula, is still studied today.
Beginning at the moment of a supernova explosion thousands of years ago, this story travels forward in time to 1054, the year people around the world saw the
unparalleled light of an exploding star appear in Earth’s sky. The story then travels deep into space to see the remnant of this supernova—the Crab Nebula—followed by a continuing trip forward in time.
Taking a unique approach integrating astronomy, cultural history, and advances in technology, the book encourages readers to think about the world around them and their place in the universe.
Told in minimal, poetic text with stunning watercolor and ink illustrations, the book closes with an invitation for readers to imagine a time when they, too, might see the rare event of a supernova shining in the sky
The Accura 70mm Mini Telescope is a compact refractor engineered for both celestial and terrestrial viewing. Its 70mm objective and 300mm focal length deliver three distinct magnification levels (15x, 20x, and 50x), via interchangeable eyepieces (6mm, 12mm, 20mm), allowing you to balance field of view with detail depending on your target.
The included moon filter reduces glare during lunar observation, while the red dot finder scope accelerates target location.
At just 2kg with a lightweight aluminium tripod, it's genuinely portable for field sessions or backyard astronomy. Ideal for observers seeking a no-fuss instrument that handles both night-sky exploration and daytime long-range viewing without sacrificing optical quality.
Specs:
| Type | Refractor |
| Objective Diameter | 70mm |
| Focal Length | 300mm |
| Magnification | 15x, 20x, 50x |
| Eyepieces | 6mm, 12mm, 20mm |
| Tripod | Aluminium alloy |
| Package Dimensions | 465 x 220 x 115 mm |
| Package Weight | 2kg |
In The Box:
- Accura Mini 70 Relfector Telescope
- Tripod
- 5x24 Finderscope
- 45 degree correct Image attachement
- Moon filter
- 3 x eyepieces (H6mm, F12mm, H20mm)
- 1.5x Erecting Eyepiece
- Aluminium Alloy Tripod
- Attachment plate
- Screws
- User manual
The Accura Traveller 114 delivers serious light-gathering capability in a portable package. The 114mm Newtonian reflector collects enough light for detailed lunar observation and bright deep-sky objects, while tube is still compact enough for travel.
The included 2x Barlow lens effectively doubles your magnification range, pair it with the included 10mm eyepiece for 100x magnification on steady nights.
Setup takes minutes without tools, and the full-length metal tripod with accessory tray provides stable support. The included red-dot finder gets you on target quickly. Ideal for observers seeking aperture and portability without compromise.
Specs:
| Optical Design | Newtonian |
| Aperture | 114mm |
| Maximum Magnification | 100x |
| Focal Length | 500mm |
| Focal Ratio | f/4.4 |
| Eyepieces | 10mm & 25mm |
| Finderscope | Red-dot |
| Barlow Lens | 2x |
What's in the Box:
- Accura 114mm Reflecting Travel Telescope
- Findersope
- Barlow lens
- 2x Eyepieces
- Tripod
- Attachment plate & screws
- Soft carry case
The Accura Traveller 70mm refractor delivers impressive optical performance in a portable package. With a 700mm focal length and fully coated glass optics, it achieves up to 210x magnification, ideal for lunar detail, planetary observation, and deep-sky exploration.
The included 3x Barlow lens and eyepieces (25mm, 10mm) provide flexible magnification options, while the red dot finder scope ensures quick target acquisition.
The 45° erect prism diagonal keeps views upright for terrestrial use. Lightweight aluminium tripod and carry case make transport effortless. Quick setup means more time observing. A capable choice for amateur astronomers seeking versatility without bulk.
Specs:
| Magification | 28X, 84X, 70X, 210X |
| Optical design | Refractor |
| Aperture | 70mm |
| Focal length | 700mm |
| Eyepiece | K25mm, K10mm |
| Barlow lens | 3X |
| Finder scope | red dot |
| Diagonal | 45 ° erect prism diagonal |
| Resolution | ≤ 3.1 |
| Viewing angle | 2 ° 24 |
| Tripod | Aluminum alloy tripod |
What's in the Box:
- 70mm Travel Telescope,
- Soft Carry Case,
- Correcting Prism,
- 2x Eyepieces,
- 3x Barlow Lens,
- Tripod, Mount,
- Red Dot Finder
Have you ever observed the night sky with astronomy binoculars?
These affordable Acuter binoculars offer a large 80mm aperture optics for collecting the fine details of star cluster, nebulae and even distant galaxies millions of light years away.
Away from city lights under a dark sky, you'll never forget the experience of scanning the star clouds and dust lanes in our home galaxy, the Milky Way.
They mount on any photographic tripod to ensure steady viewing for extended periods. An adjustable balance point positions them perfectly.
While ideal for astronomy, their high magnification also makes them a great choice for whale watching from the shoreline, wildlife viewing or taking in distant views.
Details:
- Aperture: 80mm
- Magnification: 20x
- Case included: Yes
- Tripod Mount: Standard .25" photographic
New Solar Telescope
- Telescope Focal Length: 400mm (f/10)
- Crayford Focuser (Rotatable)
- 45mm Dovetail Bar with 1/4-20 tripod threads (side mounted)
- Supplied with Universal Smartphone Adaptor
The Acuter Elite Phoenix 40 Solar Telescope is a Solar H-Alpha telescope for narrow-band observation and photography of the Sun. This instrument makes it possible to explore extraordinary solar surface dynamics that go far beyond what a white light solar filter can show.
Phenomena such as solar protuberances, active spots, flares, granulations, plasma filaments and more finally become observable and photographable with excellent sharpness and resolution. Hydrogen Alpha (Ha) solar telescopes are specialized instruments for observing the Sun at a specific wavelength of light, 656.3 nm, corresponding to the red line of the Balmer series in the hydrogen emission spectrum. This wavelength is critical for studying solar phenomena such as protuberances, filaments, sunspots and flares.
Unlike standard white-light telescopes, which capture the full solar spectrum, Ha telescopes offer a specific window into the activities of the chromosphere, the layer of the solar atmosphere located just above the photosphere. Compact and Portable: The metal optical tube makes the Acuter Phoenix 40mm solar telescope ideal for travel, while the rugged design ensures uncompromising durability.
Perfect for experienced observers and enthusiasts who wish to explore and admire the Sun’s surface in detail. Perfect for astrophotography enthusiasts and observers of the Sun.
ISO Certified Safety: This telescope complies with ISO 12312-2:2015, ensuring maximum protection for the eye during solar observation.
When viewing the Sun in the narrow H-alpha bandwidth, the observer is rewarded with thrilling, awe-inspiring real-time views of our nearest star in it’s full fiery majesty, seething with activity, revealing exciting details such as solar flares, prominences, spicules, surface granularity & sun spots
Supplied with a universal smartphone camera adaptor to take photos using your smartphone to keep a photographic record of your observations. Also supplied with a regular Star Diagonal & Red Dot Finder – the telescope can be used for normal astronomical observations as an 80/400 achromatic refractor telescope with the etalon removed
- Suitable for CCD cameras with 1.25″ adaptor and backfocus of 55mm or less
- Sky-Watcher SolarQuest Solar Go-To/Tracking Mount Recommended
- Safety Compliance Certification: ISO12312-2:2015
- OTA Length: 412mm
- OTA Weight: 2kg
- Magnifications (with eyepiece supplied): x25-x80
- Eyepiece Supplied (1.25″): 5-16mm Zoom
- Telescope Focal Length: 400mm (f/10)
- Front Etalon: Diameter: 40mm, Bandwidth: <0.6 Angstrom
- Tuning method: Pressure tuning
- Exit opening 8mm
- 8mm Block Filter
- 90° (1.25″) Diagonal (Rotatable)
- Safe Solar Finder
- Crayford Focuser (Rotatable)
- 45mm Dovetail Bar with 1/4-20 tripod threads (side mounted)
- Supplied with Universal Smartphone Adaptor
$89.00
Annals of the Deep Sky - Vol 1 A Survey of Galactic and Extragalactic Objects by Jeff Kanipe and Dennis Webb
“At last: the sky guide we’ve been waiting for! Annals of the Deep Sky melds through-the-eyepiece observing with up-to-date 21st century astrophysics. Its highly readable format should appeal to observers and non-observers alike. .....
358Pages 158 illustrations, softbound.
Covers Andromeda, Antlia, Apus, and Aquarius plus Introductions to Basic Astronomy and Astrophysics.
$119.00
Annals of the Deep Sky Vol 10 explores the constellations of Draco, Equuleus, Eridanus and Fornax, each with a bounty of fascinating stars and nonstellar objects. Draco contains numerous double stars, such as the wide pair Nu Draconis, two fifth-magnitude stars that look alike but are nonetheless very different. One of Draco’s most popular deep-sky objects is the Cat’s Eye Nebula (NGC 6543), the first planetary nebula to be decoded spectroscopically, by William Huggins in 1910. Modest Equuleus can at least boast the spiral galaxy NGC 7040, discovered by Mark Walrod Harrington in 1882. We include a brief, but strange, backstory of Harrington. Eridanus, too, may be a small constellation but it contains the intriguing galactic group associated with NGC 1723 and a “lopsided” galaxy, NGC 1637. Fornax is replete with interesting galaxies, including NGC 1097 with its peculiar nucleus, the shell system NGC 1344, and the “three-ringed” galaxy NGC 1326. And don’t neglect S Fornacis, an odd sun that occasionally exhibits superflares.
Annals of the Deep Sky is a comprehensive reference that guides amateur and semipro astronomers into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisals of prominent stars and celestial objects.
$119.00
By Jeff Kanipe
Product information: Softbound, 6 by 9 inches, 432 pages, first published 2024, colour.
Annals of the Deep Sky is a comprehensive reference that guides amateur and semipro astronomers into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisals of prominent stars and celestial objects.
In Volume 11, we delve into the celestial smorgasbord found in the constellations Gemini, Grus, Hercules, Horologium, and Hydra. Featured objects include the open cluster M35 in Gemini, as well as the strange case of NGC 2371-72, one of the most unusual examples of a planetary nebula. The southern constellation Grus contains IC 5148, a large planetary nebula with an unusual inner-tube-like morphology, as well as the grand design, multi-armed spiral galaxy NGC 7424, which contains a number of enigmatic radio and X-ray sources. Hercules hosts the great globular clusters M13 and M92, of course, and imagers will want to target Abell 2151, the rich Hercules Cluster that links up with the Great Wall of galaxies. Horologium contains the remarkable star Gliese 1061, a solar neighbour harbouring a planetary system. And don’t forget to check out the globular cluster NGC 1261 and the stunning Seyfert galaxy NGC 1433. Finally, Hydra’s showcase object is the Southern Pinwheel Galaxy, M83; other attractions include the face-on multiarm spiral galaxy NGC 2835 and the spectacular pair NGC 3314A and B — two entwined galaxies with different orientations.
$119.00
By Jeff Kanipe
Product information: Softbound, 6 by 9 inches, 432 pages, first published 2024, colour.
Annals of the Deep Sky is a comprehensive reference that guides amateur and semipro astronomers into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisals of prominent stars and celestial objects.
In volume 12 of Annals of the Deep Sky, explore the realms of Hydrus, Indus, Lacerta, Leo, Leo Minor, Lepus, Libra, and Lupus. Featured objects in Hydrus include NGC 602, a young version of the Orion Nebula, and NGC 1466, a bright, rich globular cluster. In Indus, the galaxy pair NGC 6935/6937 presents very different spiral-type morphologies. Lacerta harbors BL Lacertae, the prototype of a class of active galactic nuclei.
Leo includes the famous Leo Triplet and the striking pair M95 and M96, and Leo Minor includes the two interacting systems of Arp 107 and NGC 3395/3396. Lepus has R Leporis, the symbiotic star SS Leporis, and an incipient planetary nebula. Libra includes the Algol-type variable Delta Librae, HD 140283, and NGC 5728, a triple-ringed Seyfert 2 galaxy.
Finally, Lupus hosts the Lupus Clouds, among the nearest low-mass star-forming regions; IC 4406, an edge-on planetary nebula; and NGC 5643, a grand design spiral galaxy with complex inner structure.
$89.00
Annals of the Deep Sky - Vol. 2 : A Survey of Galactic and Extragalactic Objects by Jeff Kanipe and Dennis Webb
“At last: the sky guide we’ve been waiting for! Annals of the Deep Sky melds through-the-eyepiece observing with up-to-date 21st century astrophysics. Its highly readable format should appeal to observers and non-observers alike. .....
344pages , 244 illustrations, softbound.
Covers Aquila, Ara, Aries, Auriga, Boötes, Caelum plus a 72-page Essential Terminology Glossary.
$89.00
Annals of the Deep Sky - Vol. 3 : A Survey of Galactic and Extragalactic Objects by Jeff Kanipe and Dennis Webb
“At last: the sky guide we’ve been waiting for! Annals of the Deep Sky melds through-the-eyepiece observing with up-to-date 21st century astrophysics. Its highly readable format should appeal to observers and non-observers alike. .....
344pages, 199 illustrations, softbound.
Covers Cameloparadalis, Cancer, Canes Venatici, Canis Major plus Worlds of Discovery: The Search for Exoplanets.
$89.00
Annals of the Deep Sky - Vol 4 : A Survey of Galactic and Extragalactic Objects by Jeff Kanipe and Dennis Webb
“At last: the sky guide we’ve been waiting for! Annals of the Deep Sky melds through-the-eyepiece observing with up-to-date 21st century astrophysics. Its highly readable format should appeal to observers and non-observers alike. .....
358 pages, 158 illustrations, softbound.
Covers Canis Minor, Capricornus, Carina, and Cassiopeia.
The newest handbook for Deep-Sky observers.
Annals of the Deep Sky - Vol 4: Foreward
We are happy and proud to present volume four of Annals of the Deep Sky, in which we continue our survey of prominent stars and deep-sky objects in all 88 constellations. With this volume, we are approaching a quarter of the way to completion, though, speaking realistically, we know we have only just begun.... Among the numerous reviews, online discussion boards, and remarks from star party attendees, we’ve not heard one discouraging word. Most gratifying was the reader who likened receiving a new volume to embarking on a journey of exploration.
Readers may not be aware of this, but our labors on this series have taken us on an exciting journey as well. If you dig deeply into almost any subject you come across interesting tid-bits sooner or later, but when the subject is the universe, one never ceases to be amazed. For us, it is a constant state of being. Each day we come across some eye-opening perspective that allows us to depict the celestial objects we profile as real, physical entities, not abstractions removed across vast gulfs of space.
We strive to present stars, nebulae, and galaxies as objects you can pick up and examine as you would an interesting shell or piece of driftwood on the beach, except that we also relate how the shell or driftwood got there, why it has its unique shape, and what form it will take over time. Our discoveries are your discoveries, as is our surprise and astonishment.
This volume spotlights four constellations: Canis Minor, Capricornus, Carina and Cassiopeia.
Canis Minor
Canis Minor is not often at the top of anyone’s observing list, but like its bigger brother, Canis Major, it contains a prominent first-magnitude star, Procyon, with a white dwarf companion nearly hidden in the primary’s glare. The orbit of Procyon B itself is nearly circular, but the periastron and the apastron junctures are rather extreme, ranging from a minimum distance of 9 AU to a maximum of 21AU. Given that apastron occurs sometime around the year 2027, now is a good time to begin looking for Procyon B.
Procyon has been studied using the rapidly developing technique of asteroseismology, the analysis of stellar oscillations....Starlight tells us much about a star’s temperature and chemical makeup, but asteroseismology allows us to view the star from the inside out. A running theme in the Galactic section of Canis Minor isthe number of asterisms and suspect star clusters to be found within its bounds. NGC 2394 is one of these. Although most research suggests it is not a real cluster, other studies contradict this conclusion....
Capricornus
Capricornus is another low-profile constellation, but it does contain Dabih (β Capricorni) that forms a quadruple system definitely worth telescopic scrutiny. Without doubt, the jewel of the Sea Goat is the globular cluster M30, an old object with an extremely dense core and radiating star chains. It is thought that the central density may exceed a million stars per cubic parsec, making it one of the highest-density environments in the Galaxy. Life forms living on a planet in such a locale would never know a night sky, except, perhaps, under rare conditions, reminding us of Isaac Asimov’s science fiction short story, “Nightfall.”
For the galaxy enthusiast, Capricornus also features a double galaxy, NGC 6907 and NGC6908. The larger system, NGC6907, is an easy find, but see if you can spot its companion, “hidden” in the other’s easternmost spiral arm.
Carina
Our next starry fare is Carina, the Keel, formerly known as Argo Navis. What can we say about this sprawling and incredibly bountiful constellation? Dennis has deemed it our masterpiece, and truth be told, there is no shortage of celestial marvels to chronicle and illustrate. We think it safe to say (as much as modesty allows) that our review of the uncanny, volatile star Eta Carinae is one of the more comprehensive available in the popular literature today. Given its enduring observational history and abundance of cutting-edge research, it is deserving of its own book length treatment. Be sure to check out our three-dimensional presentation of the curious bipolar nebula encompassing this star, called the Homunculus, as well as the star’s laser emission and light echoes from the “Great Eruption” in the 1840s.
Of course, there are numerous other objects to explore in Carina, not the least of which is the Carina Nebula (NGC 3372), which lies just east of the dark, hourglass-shaped Keyhole Nebula; NGC 2516, also known as the Southern Beehive; the planetary NGC 2867 with its hot Wolf-Rayet central star; and the extremely rich globular cluster NGC 2808. The southern regionof Carina, away from the Milky Way, also harbors a number of fascinating galaxies, including the pair IC 2554 and NGC 3136B, NGC 3136, a bright elliptical with some internal structure, and, for imagers, an intriguing face-on spiral, NGC 3059.
Cassiopeia
Given its location immersed in the northern Milky Way, Cassiopeia features myriad stars and nonstellar objects of all kinds. Among the former, we offer Caph (β Cassiopeiae), the brightest member of the class of Delta Scuti stars, four Mira-type variables, the triple star Iota (ι) Cassiopeiae, and the massive binary AO Cassiopeiae. Of the latter selection, we include the young planetary nebula IC 289, the bright open clusters M52 and M103, and the extensive star-forming region (with associated star cluster) IC 1805.
In the northern part of the constellation, we find two satellites of the Andromeda Galaxy, the dwarf ellipticals NGC 185 and NGC 147. Those with an abiding interest in the history and on going research into the supernovae remnants Tycho’s Star (SN 1572) and Cassiopeia A will find plenty to mull over, as well as a sidebar on the eccentric Tycho himself. If each volume is truly like a journey of exploration, we hope you think of us as travel guides, pointing out the most interesting aspects of the astr onomical sights we encounter. We are all at the beginning of an adventure without comparison, and without end.
$89.00
Annals of the Deep Sky Vol 5 : A Survey of Galactic and Extragalactic Objects by Jeff Kanipe and Dennis Webb,
Volume 5 explores three very rich, and very different, constellations. Centaurus features a detailed overview of the Alpha Centauri system, descriptions of the Scorpius-Centaurus Association (the nearest OB affiliation to the Sun), and the stunning Omega Centauri globular cluster (NGC 5l39). Some time is also spent probing the many levels of the mysterious Centaurus A galaxy (NGC 5128), with its bizarre mixture of spiral and elliptical morphologies.
Cepheus may look dim to the unaided eye, but this constellation hosts some truly beautiful and beguiling objects. These include the star-forming region IC 1396 with its centerpiece, the Elephant Trunk Nebula (see cover image). We take a stroll down the Milky Way to visit several fine star clusters, some still associated with nebulosity, and other star-forming hotbeds.
Finally, Cetus leads us into a largely extragalactic realm where we find the nearby dwarf irregular IC l6l3, the edge-on spiral NGC 1055, and one of the brightest and nearest Seyfert 2 galaxies, M77. But the stars Mira and Tau Ceti are also on the itinerary, both of which have their stories to tell: one of a complex circumstellar environment, the other of possible extraterrestrial life.
We cannot visit these celestial marvels in our own hyperdrive spacecraft (yet), but Annals of the Deep Sky is the next best thing. Turn to page 1 and let it fly you across the universe.
$89.00
The Annals of the Deep Sky Vol 6: A Survey of Galactic and Extragalactic Objects is a comprehensive reference that guides astronomy enthusiasts into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects in both the Northern and Southern hemisphere skies, including rarely observed objects and other celestial exotica. Incorporating the most recent findings in astrophysics and cosmology, deep historical context, and captivating illustrations and images, Annals provides readers with in-depth profiles of celestial objects beyond the solar system. The mission of every Annals volume is to guide observers on their own astronomical journey of exploration, whether it be at the eyepiece or from the comfort of a favorite chair on a rainy night. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisal of prominent celestial objects.
Covers; Chamaeleon, Circinus, Columba, Coma Berenices and Corona Australis.
ISBN: 978-1942675112
$89.00
The Annals of the Deep Sky Vol 7: A Survey of Galactic and Extragalactic Objects is a comprehensive reference that guides astronomy enthusiasts into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects in both the Northern and Southern hemisphere skies, including rarely observed objects and other celestial exotica. Incorporating the most recent findings in astrophysics and cosmology, deep historical context, and captivating illustrations and images, Annals provides readers with in-depth profiles of celestial objects beyond the solar system. The mission of every Annals volume is to guide observers on their own astronomical journey of exploration, whether it be at the eyepiece or from the comfort of a favorite chair on a rainy night. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisal of prominent celestial objects.
Covers; Corona Borealis, Corvus, Crater and Crux.
ISBN: 978-1942675136
$89.00
Annals of the Deep Sky Vol 8: A Survey of Galactic and Extragalactic Objects by Jeff Kanipe.
The Annals of the Deep Sky: A Survey of Galactic and Extragalactic Objects is a comprehensive reference that guides astronomy enthusiasts into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects in both the Northern and Southern hemisphere skies, including rarely observed objects and other celestial exotica. Incorporating the most recent findings in astrophysics and cosmology, deep historical context, and captivating illustrations and images, Annals provides readers with in-depth profiles of celestial objects beyond the solar system. The mission of every Annals volume is to guide observers on their own astronomical journey of exploration, whether it be at the eyepiece or from the comfort of a favorite chair on a rainy night. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisal of prominent celestial objects. We cannot visit these celestial marvels in our own hyperdrive spacecraft (yet), but Annals of the Deep Sky is the next best thing. Turn to page 1 and let it fly you across the universe.
Annals sorts the night sky into Galactic objects (those within the Milky Way) and extragalactic objects beyond our galaxy. Each chapter begins with an overall description of the pertinent constellation, its mythology if any, visibility, and overall appearance. From here, we move on to the building blocks of the Milky Way: stars in all their many forms, bright and dark nebulae, molecular clouds, star-forming regions, planetary nebulae, star clusters of every kind, and even the occasional telescopic asterism. Then, through the Milky Way framed by each constellation, we peer out into extragalactic space.
Volume 8 explores three of the most fascinating constellations in the night sky.
Cygnus is extremely rich, particularly in nebulae. Featured objects include popular favorites such as Chi Cygni, which has one of the largest visual amplitudes among Mira-class stars; P Cygni, a supernova in the making; the North America and Pelican nebulae; NGC 6888, the Crescent Nebula; and the radio galaxy Cygnus A.
Delphinus include the nova, HR Delphini; the bright globular clusters NGC 6394 and NGC 7006; and the galaxy groups of NGC 6928 and NGC 6956.
Dorado leads us into the wonders of the southern sky beginning with the close binary Alpha Doradus; R Doradus, known for having the largest apparent diameter of any star in the sky except the Sun; and the beautiful face-on spiral galaxy, NGC 1566.
$119.00
Annals of the Deep Sky - Vol 9 is a comprehensive reference that guides amateur and semipro astronomers into every mind-boggling corner of the observational universe. Each volume presents extensive descriptions of prominent stars and deep-sky objects. No other popular work in astronomy provides the comprehensive historical background and astrophysical appraisals of prominent stars and celestial objects.
This volume is dedicated to the Milky Way’s nearest and largest satellite galaxies, the Magellanic Clouds. Throughout history they have been the subject of awe and wonder, catching the eye of Indigenous peoples of Australia and New Zealand, 16th century mariners, and astronomy’s pioneer observers such as Nicolas-Louis de Lacaille, James Dunlop, and John Herschel. In the late 19th and early 20th centuries, northern astronomers began traveling to the Southern Hemisphere to photograph, map out, and study the celestial constituents of what they referred to as Nubecula Major and Nubecula Minor. This book presents not only a thorough historical account of the clouds dating back 40,000 years, but also how astronomers’ ideas of the Clouds have changed over the decades — particularly on the Clouds’ origins, interactions with the Milky Way, and the quizzical aspects of star formation posed by their many unusual clusters and H II regions. Come discover the observational richness and astrophysical conundrums that are the Magellanic Clouds, true treasure islands lying just beyond our Galactic shores.
Annals of the Deep Sky - Vol 9 also includes two special fold-out maps for exploring the Magellanic Clouds in more detail, one showing the Large Magellanic Cloud and the other the Small Magellanic Cloud plus extra detail on the Tarantula Nebula, the star-forming region also known as 30 Doradus.
Author Jeff Kanipe has released the latest edition of this great series and for those of us in the South we are blessed. Volume 9 covers the Magellanic Clouds. Definitely will be in my Library of Southern Hemisphere books, can’t wait.
SKU:WBANN9
$649.00
ALP-T Dual Band 5nm Filter is best suited for optics f-ratios slower than f/3.6, the standard Antlia ALP-T Dual Band filter is highly recommended. Meanwhile, if you seek the best possible performance with any optics faster than f/2.2, the highspeed version is the best choice.
The Antlia ALP-T dual band 5nm series filter is a dual line-pass filter that was designed to be used primarily with one-shot color (OSC) cameras such as DSLR's and astronomical OSC cameras. It can also be used as a narrowband filter for monochrome cameras to save imaging time. The advanced multi-coatings on our ALP-T ultra dual-band filter effectively isolate the red Ha and the blue-green OIII lines light from emission nebulae, with almost total suppression of optical density (OD) 4.5 on unwanted wavelengths from light pollution, moonlight, and airglow. The result is that our ALP-T dual band 5nm filter creates a superior signal-to-noise ratio and better contrast in your images.
The Antlia ALP-T Dual Band filter enables the capture of the two main emission nebulae bands at the same time, whilst suppressing unwanted light pollution. It enables you to capture cleaner data and reduces the post-processing efforts to isolate faint details from the background light pollution.
Application and Performance:
Designed especially for optics, slower than f/3.6
Engineered specifically for use with DSLR, CMOS, and CCD color cameras
Suppression of optical density (OD) 4.5 on unwanted wavelengths adds signal-to-noise
Extremely steep bandpass edges minimize internal reflections
Ideal flat-top and moderate bandpass reducing spectrum downshifts
Ion Gun Assisted Deposition coating technology on the double-sided polished substrate making it the most consistent and accurate light pollution suppression filter
Designed to suppress artificial lighting from Bortle scale 1 to Bortle scale 8
Near IR (NIR) is blocked up to 1050nm
Technical Specifications:
| Hydrogen-alpha | Oxygen III | |
| FWHM | 5nm | 5nm |
| CWL (Central Wavelength) | 657.8nm | 502.2nm |
| Peak Transmission | 88% | 82% |
| Blocking | ≥OD4.5 @ 300-1050nm | |
| Filter Thickness | 2mm+/-0.05mm | |
Filter Ring:
2'' (M48*0.75)
Ultra-thin filter cell to minimize vignetting by maximize possible clear aperture
Black Anodized Finish
Laser Engraving No Fading
Spectrum Curve:
Not Recommended:
Solar imaging
Night visual observation
Not Permitted:
DO NOT LOOK AT THE SUN WITH THIS FILTER
Serious eye damage will result if you fail to observe the warning
$689.00
Antlia ALP-T Dual Band 5nm Highspeed Filters are optimized to work with high-speed imaging systems by shifting slightly the passband and center wavelength. Using these highspeed filters between optics f/2.2 and f/3.6 shows much stronger and more contrasted in nebulae imaging compared to the standard version, if you seek the best possible performance with any optics faster than f/2.2, the highspeed version is the best choice.
But keep in mind, the blue shift data by the computer simulation indicates narrowband filter shifts its bandwidth to shorter wavelengths with faster optics than f/2, transmission at the emission wavelength may decrease perhaps 15%-20%. Although the Antlia ALP-T highspeed filter has similar transmission rates reduction in the H-a and OIII when the filter is used on fast optics, based on current standard version users’ data, it is evident that the filter still has the high performance of increase in emission nebula contrast and minimized halo.
The highspeed version price is the same as the standard filters and double benefits for the high-speed optics users. Worth mentioning is that Antlia inspected and measured products piece by piece with one of Agilent Cary’s professional spectrophotometer, resolution/slit width is up to 0.2nm, which make us provide highly reliable and consistent products to you.
The Antlia ALP-T dual band 5nm series filter is a dual line-pass filter that was designed to be used primarily with one-shot color (OSC) cameras such as DSLR's and astronomical OSC cameras. It can also be used as a narrowband filter for monochrome cameras to save imaging time. The advanced multi-coatings on our ALP-T ultra dual band filter effectively isolate the red Ha and the blue-green OIII lines light from emission nebulae, with almost total suppression of optical density (OD)4.5 on unwanted wavelengths from light pollution, moonlight, and airglow. The result is that our ALP-T dual band 5nm filter creates a superior signal-to-noise ratio and better contrast in your images.
The filter enables the capture of the two main emission nebulae bands at the same time, whilst suppressing unwanted light pollution. It enables you to capture cleaner data and reduces the post-processing efforts to isolate faint details from the background light pollution.
Application and Performance:
Designed especially for fast astronomy optics, in particular f-ratios f/2.2 to f/3.6
Engineered specifically for use with DSLR, CMOS, and CCD color cameras
Suppression of optical density (OD)4.5 on unwanted wavelengths adds signal-to-noise
Extremely steep bandpass edges minimize internal reflections
Ideal flat-top and moderate bandpass reducing spectrum down shifts
Ion Gun Assisted Deposition coating technology on the double-sided polished substrate making it the most consistent and accurate light pollution suppression filter
Designed to suppress artificial lighting from Bortle scale 1 to Bortle scale 8
Near IR (NIR) is blocked up to 1050nm
Technical Specifications:
| Hydrogen-alpha | Oxygen III | |
| FWHM | 5nm | 5nm |
| CWL (Central Wavelength) | 657.8nm | 502.2nm |
| Peak Transmission | 88% | 82% |
| Blocking | ≥OD4.5 @ 300-1050nm | |
| Filter Thickness | 2mm+/-0.05mm | |
Filter Ring:
2'' (M48*0.75)
Ultra-thin filter cell to minimize vignetting by maximize possible clear aperture
Black Anodized Finish
Laser Engraving No Fading
Spectrum Curve:
Not Recommended:
Solar imaging
Night visual observation
Not Permitted:
DO NOT LOOK AT THE SUN WITH THIS FILTER
Serious eye damage will result if you fail to observe the warning
From $520.00
The Antlia LRGB-V Pro series filters are designed for monochrome cameras that use both CCD and CMOS sensors. Suitable sensors include KAF/KAI sensors, Sony IMX sensors, GSENSE and other sensor manufacturers. The LRGB-V Pro set is designed to approximately equalize the RGB response from the flux of red-sensitive CCD detectors. The result is that you achieve 1:1:1 equalized RGB exposures with the benefit of simplified post processing and reduced imaging time. New LRGB-V Pro series filters feature a carefully designed spectral gap between the green and red channels to minimize the effect of light pollution and to provide high transmittance of useful frequencies. The filters’ design maximizes the capture of details from fainter galaxies and nebulae emissions. The LRGB-V Pro series filters guarantee the high transmission of the OIII band in both the B and G filters (OIII signal >95% in blue and green). The bandwidth of the B channel is narrowed for the purpose of improving the blue channel overflow (haloing) around the star due to B channel overexposure. Antlia LRGB-V Pro series filters block the emission line around 589nm by the design of wide gap between G and R filters, which suppresses much of the light pollution from high pressure sodium and mercury street lamps and results in a more natural color balance. The uniformity in substrate thickness delivers good parfocal performance across all Antlia filters.
Highlight of LRGB-V Pro series set
1. Premium coating technology and finely polished substrate Our quality selection processes are optimized to ensure highly homogeneous glass-substrates. Our application of advanced optical coating technology and double-sided precision polishing achieves both consistent parfocal and optical performance across all filters. 2. Maximized colour balance and contrast for each of the three RGB channels and excellent S/N performance Dozens of coating layers are deposited on both sides of the glass substrate that enables LRGB-V Pro filters to achieve a high SNR. The Anti reflection coatings and carefully designed spectral gaps minimize unwanted light scatter and maximize useful signal data for each filter channel.
3. Tighter star profiles and halo reduction The cut-off rate of LRGB-V Pro series set is designed in high level to minimize halos around brighter stars and reduce star bloat. Our careful design of the blue channel transmission characteristics targets the problem of blue star bloating.
Application and Performance:
1. Designed for monochrome CCD and CMOS cameras
2. Great imaging colors for celestial objects, galaxies, star clusters and nebulae
3. AR anti-reflection film design for secondary reflection and star halo reduction
4. R-Filter provides maximum transmission of H-alpha and S II emission
5. B/G overlap doubles the energy in the OIII line
6. Balanced RGB-design offer 1:1:1 exposure times for most telescope optical systems
7. All Antlia LRGB-V Pro filters are edge blackened to eliminate internal reflections from stray light
8. The substrate thickness of each of the four LRGB filers is maintained to tight tolerances
9. Not recommended for Solar observing and imaging
10. Not recommended for visual observation
Important Note: When using any parfocal filters, the user may still experience focus shifts between filters during long imaging sessions. It is important to remember that temperature shifts will change the length of the optical path due to the differential contraction between the telescope tube and the glass optical elements. It is recommended that the photographers check focus either manually or automatically in software every 1 to 2 hours. In cases where the telescope has been brought from a warm environment to outside, more frequent focus checks are required until the equipment has stabilized nearer to ambient temperature.
Technical Specifications:
Basic Substrate: optical substrate
Filter Thickness: 2mm+/-0.05mm for 1.25’’
Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)
Transmitted Wavefront: Lambda/4 or better.
Parallelism: less than 30 arcsec
Single / Non-glued substrate
$679.00
Antlia OIII 3nm Pro narrowband filter optimizes the FWHM (full width half maximum) to 3nm bandpass. As the bandwidth becomes narrower, the 3nm Pro narrowband filters enhance the contrast of emission targets by lowering the unwanted background signal. Antlia OIII 3nm Pro filters are designed to deliver 85% transmission at the 500.7nm line which provides you with the maximum signal and well-defined nebulae structures.
Conventional broader narrowband filters cause a heavy loss in transmission due to the strong Center Wavelength (CWL) shift. We guarantee T>85% within 1nm range of the center bandwidth, which means that the 3nm Pro narrowband filter can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blueshift data shows that Antlia 3nm Pro filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meet the requirements of fast optics like Hyperstar and RASA.
The out-of-band blocking specification is rated OD5 (0.001%) which delivers an excellent SNR(signal-to-noise ratio) and effective cut-off rate to minimize interference from other wavelengths. Improved sharp cut-off astrophotography 3nm Pro filters are designed to minimize halos around bright stars.
Application and Performance:
High transmittance and smallest bandwidth to maximize contrast
Steep spectral profile minimizes halos around bright stars
A single substrate to eliminate internal reflections
Narrowband Objects: OIII Emission Nebulae, Planetary, Wolf Rayet Nebulae and Supernova Remnants
Use in light polluted areas and dark sites
Extends imaging time when the moon is up
Antlia narrowband Pro filters can be used down to F/3 systems with slight loss of signal
All Antlia Narrowband filters are edge blackened to eliminate internal reflections from stray light
Superior optical reliability reduces post image processing
This filter is not suited to deep sky objects that do not contain OIII emissions.
Technical Specifications:
Basic Substrate: optical substrate
Filter Thickness: 2mm+/-0.05mm for 2'' mounted
FWHM (Full width at half maximum): 3nm
CWL (Central Wavelength): 500.7nm
Peak Transmission: >85%
Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm
Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)
Transmitted Wavefront: Lambda/4 or better.
Parallelism: less than 30 arcsec
Single / Non-glued substrate
Warranty: 3-years against delamination
DO NOT LOOK AT THE SUN WITH ANTLIA FILTERS.
When we design filters for astronomy imaging systems, we look at how they will work together with optical systems, carefully designing the blocking and bandpass parameters to achieve an optimum result. The out-of-band blocking rate is a very important performance index since it is designed to sharply attenuate off-band wavelengths. The result is that the Antlia OIII 3nm Pro filter delivers excellent contrast with extremely dark backgrounds whilst delivering a high transmission of the OIII signal. Such filters are more difficult to produce to a consistently high standard.
Each filter is individually tested and scanned to ensure that the quality meets the high-performance parameters. The end result is a filter that achieves excellent contrast but with a higher production cost. We believe the price-to-performance ratio compares more favorably than similar premium filters in the market.
SKU: ANTLIAOIII3nm2
From $1,310.00
The Antlia 3nm Pro Ultra Narrowband filter set includes the following items:
- Antlia H-Alpha 3nm filter
- Antlia OIII 3nm filter
- Antlia SII 3nm filter
Antlia SHO Pro narrowband filter optimizes the FWHM (full width half maximum) to 3nm bandpass. As the bandwidth becomes narrower, the 3nm Pro narrowband filters enhance contrast of emission targets by lowering the unwanted background signal. Antlia SHO 3nm Pro filter is designed to deliver 88% transmission at the 671.6nm line which provides you with the maximum signal and well defined nebulae structures.
Conventional broader narrowband filters cause a heavy loss in transmission due to the strong (Center Wavelength (CWL)-shift. We guarantee T>88% within 1nm range of the center bandwidth,which means that the 3nm Pro narrowband filter can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data show that Antlia 3nm Pro filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meets the requirements of fast optics like Hyperstar and RASA.
The out of band blocking specification is rated OD5 (0.001%) which delivers an excellent SNR(signal to noise ratio) and effective cut-off rate to minimize interference from other wavelengths. Improved sharp cut-off astrophotography 3nm Pro filters are designed to minimize halos around bright stars.
Application and Performance:
- High transmittance and smallest bandwidth to maximize contrast
- Steep spectral profile minimizes halos around bright stars
- A single substrate to eliminate internal reflections
- Narrowband Objects: Emission Nebulae, Planetary, Wolf Rayet Nebulae and Supernova Remnants
- Use in light polluted areas and dark sites
- Extends imaging time when the moon is up
- Antlia narrowband Pro filters can be used down to F/3 systems with slight loss of signal
- All Antlia Narrowband filters are edge blackened to eliminate internal reflections from stray light
- Superior optical reliability reduces post image processing
$679.00
Antlia SII 3nm Pro narrowband filter optimizes the FWHM (full-width half maximum) to 3nm bandpass. As the bandwidth becomes narrower, the 3nm Pro narrowband filters enhance the contrast of emission targets by lowering the unwanted background signal. Antlia SII 3nm Pro filter is designed to deliver 88% transmission at the 671.6nm line which provides you with the maximum signal and well-defined nebulae structures.
Conventional broader narrowband filters cause a heavy loss in transmission due to the strong (Center Wavelength (CWL)-shift. We guarantee T>88% within 1nm range of the center bandwidth, which means that the 3nm Pro narrowband filter can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data show that Antlia SII 3nm Pro filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meet the requirements of fast optics like Hyperstar and RASA.
The out-of-band blocking specification is rated OD5 (0.001%) which delivers an excellent SNR(signal-to-noise ratio) and effective cut-off rate to minimize interference from other wavelengths. Improved sharp cut-off astrophotography 3nm Pro filters are designed to minimize halos around bright stars.
Application and Performance:
High transmittance and smallest bandwidth to maximize contrast
A steep spectral profile minimizes halos around bright stars
A single substrate to eliminate internal reflections
Narrowband Objects: SII Emission Nebulae, Planetary, Wolf-Rayet Nebulae and Supernova Remnants
Use in light-polluted areas and dark sites
Extend imaging time when the moon is up
All Antlia narrowband Pro filters can be used down to F/3 with a slight loss of signal
All Antlia Narrowband filters are edge-blackened to eliminate internal reflections from stray light
Superior optical reliability reduces post-image processing
This filter is not suited to deep-sky objects that do not contain SII emissions.
Technical Specifications:
Basic Substrate: Schott optical substrate
Filter Thickness:2mm+/-0.05mm for 2'' mounted
FWHM (Full width at half maximum): 3nm
CWL (Central Wavelength): 671.6nm
Peak Transmission: >88%
Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm
Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)
Transmitted Wavefront: Lambda/4 or better.
Parallelism: less than 30 arcsec
Single / Non-glued substrate
Warranty: 3 years against delamination
SKU: ANTLIASii3nm2
$95.00
V2 model now available!
The BG-58 astronomy flashlight v2 model now turns onto the red COB light low setting first, offering a soft red glow without cycling through any white lights interfering with your night vision.
Other new improvements include the 60% increase in battery capacity, now supporting a long 72 hour runtime on low with reduced LCD brightness for improved astro night vision support.
Designed for astronomers, the BG-58 red light astronomy torch offers two lighting outputs, a single white LED flashlight and dual coloured red or white COB light output.
Both the flashlight and COB light incorporates full brightness adjustment control with LCD digital display, ideal for astronomers and night vision support.
Also, The BG-58 comes integrated with an adjustable stand and two separate magnets to assist with placement for that perfect light direction.
Powered by a high capacity 4000mA lithium battery, recharging is super fast via the modern USB-C input, USB power output is also supported to help charge your smart phone or other USB devices such as drones or cameras.
BG-58 is inspired from the star 58 Orionis (Betelgeuse), a red supergiant from the Orion constellation and is approximately 760 times bigger than our sun. Betelgeuse is the 10th brightest star in the sky and the second brightest in Orion.
Features
Dual colour COB light with red and white light output
Adjustable brightness from 1 - 100% for optimal brightness control
Red light 1000 Kelvin output, the ideal colour to support your vision at night
USB power output, allowing you to charge or run other USB devices
Dual magnets and hook support options for complete light direction control
Power bank with USB output
LCD Battery level and output power indicator
Specifications
Flashlight maximum Lumens: 300
Flashlight colour temperature: 6000 Kelvin
Flashlight LED wattage: 5 Watt
COB light maximum lumens: 350
COB light colour temperaure (white): 6000 Kelvin
COB light colour temperaure (red): 1000 Kelvin
COB light wattage: 6 Watt
Operating temperature: 0 - 50
IP Rating: 42
Dimension (mm): 190 x 59 x 30
Weight: 260 grams
Included in the box:
x1 Flashlight
x1 USB-C 1.0m cable
x1 USB-C to Micro adapter
x1 Velcro cable support strap
Runtime
Flashlight
8 hours - High
72 hours - Low
COB light white
8 hours - Maximum
72 hours - Low
COB light red
8 hours - Maximum
72 hours - Low
Charge time:
5 - 6 hours
USB output:
3 hours @5 Watts
Battery Information
Battery Type: 18650
Battery size: 2000 mAh, 3.7V (x2)
Battery capacity: 4000 mAh @3.7V, 14.8 Wh
Battery chemistry: Lithium ion NMC
Connections
USB input: Type C, 5.0 Vdc, 1.0A, 5.0W
USB output: Type A, 5.0 Vdc, 1.0A, 5.0W
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