The leaves and prices are falling this autumn!
You can find our colorful selection of special offers here in the shop. Get them now!
The offer is valid from September 23rd to November 28th, 2024 and only while supplies last!
The leaves and prices are falling this autumn!
You can find our colorful selection of special offers here in the shop. Get them now!
The offer is valid from September 23rd to November 28th, 2024 and only while supplies last!
The brand Celestron is known for its high-quality Schmidt-Cassegrain telescopes. These compact telescopes have a special glass plate on the front end which is exposed to the air and, therefore, is relatively susceptible to dewing up.
Celestron now offers a newly-developed range of accessories to solve this problem:
These sturdy caps have an internal velvet surround to protect against pesky scattered light as well as dew. As every cap comes with a compatible dust cap, they can also stay on the telescope tube once you have finished observing for the night. This is a big advantage for observatory telescopes.
The dew caps are available in all Celestron SC telescope sizes. You can find the entire range here in our shop.
This new solution to the issue of dew is especially innovative. With just a few flicks of the wrist, you can separate the holding ring from the plate and replace it with a new ring with integrated heating. Thanks to the integrated sensor, the temperature of the Schmidt plate is kept just below the dew point and, therefore, remains dry.
If you are purchasing a new Celestron telescope, we can complete the installation for you prior to despatch. You can find all models here in the shop.
A set of controls is required to supply power to the heating ring. This not only provides the required energy, but also keeps the heating element’s other sensors operating optimally. This saves energy and prevents the heating creating negative optical effects. You only heat as much as you need to!
Both the 2x dew cap smart controls and the 4x dew cap smart controls can also control heating elements produced by other manufacturers. Additionally, they function as a hub for additional accessories. This prevents there being a tangle of cables and allows your set-up to be powered and controlled by one device and one software.
All of Celestron’s dew prevention options can be found here in our shop.
Autoguiding is understood to refer to the automatic monitoring of the tracking of astronomical mounts. This monitoring is required for astrophotography in order to keep the targeted object steady on the camera’s sensor.
There are a multitude of cameras available for autoguiding, however they require a laptop or PC and suitable software. Now, standalone solutions are coming out which do not require these supports. The latest innovation in this field is the StarAid Revolution autoguiding camera. Tracking monitoring is extremely simple using this!
Plug & Guide: Connect the camera to your guide scope, connect it to your mount via the guide port, and voila! The camera kicks into action after around 30 seconds and sends corrective impulses to your mount’s motors.
But the StarAid Revolution can do even more: For example, polar alignment, the precise alignment of your mount with the Earth’s rotational axis. It is even possible to control the astronomical camera. An app is available for these additional options and also to monitor the tracking. In order to allow you to connect your smartphone to your autoguider, the StarAid Revolution creates its own WiFi network.
Revolution is a big word. Here, it really does apply!
With the PowerTank Lithium LT, Celestron is introducing a particularly light battery, which is especially suitable for smaller telescopes.
Modern telescope electronics react very sensitively to an incorrect voltage. Operating a telescope at too low a voltage can cause the motors to suffer at higher loads and even cause the electronics to fail. The PowerTank Lithium LT uses a built-in voltage regulator to ensure that it continually delivers at least 11.8 volts, until the battery is almost empty and shuts itself down.
Compared to a classic lead-acid battery, the PowerTank Lithium LT is smaller, lighter, more efficient and better for the environment. It offers better performance, a longer life and safer operation than other, cheaper lithium-ion batteries. It also offers automatic shutdown, reverse polarity protection and charge/discharge protection, as well as protection against overvoltage and short circuits.
We recommend the PowerTank Lithium LT for telescopes from the following series:
By the way: the battery also meets the current FAA regulations for hand luggage – ideal for travelling!
It should be easy, but sometimes it really is exasperating. How am I supposed to find a galaxy, a nebula in the sky, when there are hardly any reference points?
The solution: the Radiant finder. With three circles in divisions of a half, two and four degrees, you use a two-dimensional search device; this offers an invaluable advantage over a simple LED finder with a projected dot. Indeed, astronomers who started with point-finders have often needed years to develop the necessary system or routine so that they could find something easily.
The idea of easily finding objects differs fundamentally from actual practice, but why is this?
Well, because at the beginning, you still need some practice to transfer that which you see on the star chart to the sky. For example, how do I find the famous Owl Nebula M97? How can I visualise that in the sky?
Now there is a helpful solution to this: The Radiant Special Lineal
This makes it easier to find objects in the sky. You just place the transparent tool onto your star atlas and you can then find out how far, and in which directions, you need to move the circles in the sky. For example, place the centre of the circle on the lower-right star, Merak in the Big Dipper. Point roughly towards the 3.6 mag bright star, x UMa, and move Merak to the edge of the outer circle – M97 will already be in the centre. You can then do the same with your telescope in the evening.
It is like painting by numbers in the sky!
BONUS: Exclusively for Radiant purchasers
From now on, when you purchase a Radiant finder, you will also be given the special lineal with Radiant circles. This helpful tool is not available separately, you can only get it as a free bonus when you buy a Radiant finder.
Would you like to be able to find objects more easily? You can find the Radiant Finder with an Astro Lineal here!
In the coming weeks Venus, our “sister planet”, will become a good object for observing. The planet is a bright, easily detectable object in the morning or evening sky, but it is usually located very close to the horizon with corresponding atmospheric disturbance and rather short observing times. This will improve from around the end of January, when Venus will become progressively brighter and visible for longer in the evening sky. Then the planet will be found easily with the naked eye immediately after sunset and can be observed for almost four hours.
Even good binoculars, such as the Omegon Nightstar are suitable for observing. In telescopes with an aperture from around 90mm, Venus can already be identified as a small disc. Just like the Moon, the planet exhibits different phases, although details of the surface remain hidden owing to its very dense atmosphere. The cloud structures can be distinguished very well with telescopes from 130mm aperture. The use of a suitable filter (violet, dark blue, blue) is recommended to improve the contrast.
Venus is the second innermost planet in our solar system and is a similar size to Earth. Its atmosphere consists of carbon dioxide, nitrogen, sulphur dioxide and various noble gases. This composition, combined with its proximity to the Sun, makes our neighbouring planet a hostile and mysterious world. As it orbits the Sun, Venus rotates backwards, that is in exactly the opposite direction to our Earth. Therefore on Venus the Sun rises in the west and sets in the east. After the Moon, the planet is the brightest object, but, just like Mercury it is only visible in the morning or evening sky – hence it is also given the designation “morning-” or “evening star”.
From mid-January, Venus dominates our evening sky immediately after sunset on the southwestern horizon. Between then and the end of March it changes its position from about 25° to 46° and reaches a brightness of -4.7mag by the end of April. During this period it moves towards the western horizon and passes through the constellations Aquarius, Pisces and Aries. In April it reaches Taurus and can even be found close to the Pleiades (M45) at the beginning of April.
From January to May it’s best to track Venus using a star chart.
Have fun observing Venus in 2020!
The SkyGuider Pro is a very light mount on which you can set up a camera with interchangeable lenses or a small telescope. This approach allows longer exposure times and so you can create fascinating wide-angle shots of the night sky.
The SkyGuider Pro is now also available as a set together with the iPolar electronic polar finder, which has been built into the mount. With this accessory, you can easily and very precisely polar-align your mount.
The electronic finder has a built-in camera. This shows the position of the northern celestial pole and the location that the polar axis of the mount is pointing at, on your laptop. Simply bring the two points together by turning the adjustment screws for the azimuth and altitude axes of the mount – and you’re done!
The location of the celestial north pole differs somewhat from the location of the Pole Star. The electronics calculate the exact position using the date and time. Thanks to the sensitivity of the camera and the large field of view, this so-called polar alignment is successful even when the mount has been only roughly positioned. This also works in the southern hemisphere and even takes into account atmospheric refraction at low latitudes!
If want to do without iPolar, you can of course still purchase the SkyGuider Pro mount without the electronic polar finder here.
You can rely on PlaneWave Instruments’ professional CPWI software if you want to control your Celestron telescope via a laptop or PC.
This software is not only intuitive to use, but also lets you maximise the GoTo accuracy of your Celestron mount.
CPWI Telescope Control software is now compatible with all modern Celestron mounts, including:
You can download the software for free here on celestron.com!
Some special features of CPWI software include:
System requirements: Windows 7, 8 or 10 operating system, with USB 2.0 or 3.0 connection, 15MB hard disk space and 64MB RAM. Screen resolution of 1024×768 or higher is recommended.
Diamonds really are astronomers’ best friends – at least since the Baader Diamond Steeltrack focuser has been available. It uses real diamonds in its drive system!
In contrast to conventional Crayford or rack-and-pinion focusers, the Diamond Steeltrack’s micronized drive system guarantees entirely backlash-free operation, is completely non-slip and torsion-free – and has a vertical load capacity of 6 kilograms!
There are Diamond Steeltrack focusers available for Schmidt-Cassegrain telescopes, Newtonian telescopes and refractors.
The Steeldrive II motorized focuser drive with hand-held controller is now available:
The Steeldrive II motorized focuser drive permits automated focusing of a telescope via computer, as well as precise and vibration-free focusing using the buttons on the hand-held controller.
A good focuser considerably enhances observing pleasure and is essential for high-end astrophotography. The Steeltrack focuser is currently the best possible solution available!
CEM series mounts from iOptron are already widely used in the US and are becoming increasingly well known in Europe too. The CEM25P mount for portable astrophotography with Newtonian telescopes of up to 6 inches aperture and the CEM60 mount for use in observatories have proved particularly popular.
With their new CEM40 and CEM40-EC with encoders, iOptron now provides a middle range mount capable of carrying loads of up to 18 kilograms. The CEM40 is hence ideally suited for astrophotography with telescopes of up to 8 inches (200 millimetres) in aperture.
The abbreviation CEM stands for centre-balance equatorial mount, i.e. for equatorial mounts which are supported at their centre of gravity. This design ensures an excellent relation between weight and carrying capacity. The CEM40 weighs only 7 kilograms and yet can carry OTAs up to 2.5 times heavier. The amazing carrying capacity of CEM mounts has been constantly reaffirmed by our customers – especially regarding the CEM25P.
The CEM40 comes equipped with an electronic pole finder, known as ‘iPolar’. A laptop is required to operate this however, so the CEM40 is particularly suitable for astrophotographers who already use a laptop for their camera. iPolar and built-in GPS provide easy and accurate alignment and GoTo computer control initialization.
The encoders installed in the CEM40-EC version ensure very high GoTo accuracy and allow worm gear permanent periodic error correction – a problem that all mounts suffer from. The CEM40-EC does away with the need for guiding with your astrophotography.
The CEM family now covers a wide range of load carrying capacities, offering a suitable model for every budget!
Luminescent emission nebulae, supernova remnants and planetary nebulae are all particularly beautiful objects pertaining to the night sky. This applies both to the simple process of visual observation, as well as to astrophotography. Nature illuminates such nebulae in specific spectral colours: the red light of hydrogen, the blue-green light of oxygen ions and also in the colours of sulphur and nitrogen ions. Nebula filters enable these colours to pass through whilst blocking the diffused light of the natural luminance of the sky and of light pollution. The result is a marked increase in contrast.
With the Nebula Booster NB1, the filter specialists IDAS are introducing a new, very high-performing filter of this type onto the market, and one that is not overly expensive! As the transmission curve shows, the filter has high transmission and is permeable for all relevant spectral lines, with a surprisingly narrow passband: A real nebula intensifier!
The filter is ideal for photographing large nebula regions since it enables the typical colours of these objects to pass and blocks the disruptive skyglow. The filter quickly and completely cuts off near infrared up to 1100 nanometres. This is important since cameras are sensitive to this range, but telescopic lenses are optimised for the visible spectral range and are faulty in the infrared range.
The Nebula Booster NB1 is available with two versions which cover both of the common filter thread sizes and can be screw-fitted to the housings of eyepieces or cameras.