Testar Australia is a technical assistant dealer for Avalon Instruments. Our staff has been trained at the Avalon Instruments factory to provide assistance, repairs and maintenance on their products.
The Avalon M-ZERO LHQ is the same light, strong and innovative mount as the M-ZERO, but with extended latitude range adjustment down to 0°. Four range degrees are available :
- 0° - 15°
- 15° - 45°
- 30° - 55°
- 55° - 70°
The M-ZERO has been designed to revolutionize the world of portable astronomy. The unique and innovative design, the light weight and small dimensions, greater versatility and high quality make the M-Zero the perfect portable mount.
NOTE: the Alt/Az configuration is not available in the M-Zero LHQ mount.
Double Telescope Setup
With the Dual-DEC system, you can install a second telescope on the opposite side of the declination axis. Considering this capability it is possible to use a great range of optics starting from a small refractor up to a double setup with a total weight of 12-13 kg. Avalon offers a vast range of accessories that can be connected with the Dual-DEC system such as Vixen saddles, Losmandy Saddles or the X-Guider.
Meridian flip, something of the past.
As for the Linear, the motion transmission technology is based on pulley-tooth belt without play while its geometry makes the imaging easy at the meridian without having to wait for the object to cross the meridian. It works particularly well for objects such as the Andromeda Galaxy, M27 or M33 that reaches a maximum elevation of just a few degrees above the horizon, capturing that time is limited and it should not be wasted on the meridian flip routine.
Why using counterweights if the mount itself can be a large counterweight? That is the concept behind the Avalon M-Zero mount: shift all the mount mechanism on the counterweight side and reduce the dead weight to be carried. The declination axis can be quickly balanced like in an equatorial mount, while for the RA axis there is a small 0.5kg counterweight that can be placed in different positions.
The M-Zero total weight is only 12 kg with the tripod (included) and in terms of lightness and transportability, it ranks at the top of the lightest mounts with capacity up to 8/10 kg.
No gears for high guiding performance
Different from other mounts, the Avalon M-Zero has such a low guiding RMS error that it makes astrophotography possible with telescopes with focal length up to 2m such as the Schmidt Cassegrain 8" f/10.
The majority of telescope mounts employ a worm drive gear system. This system however may produce a poor guiding performance due to mechanical errors in gears such as periodic error, rough gear surfaces and a play between gears (backlash).
- Periodic error: it is caused by the eccentricity of the worm gear in right ascension which has to turn constantly in order to compensate the Earth's rotation. While the guiding system tries to reduce the periodic error, it will never disappear completely due to its short period and its high amplitude. As a result, the tracking accuracy in right ascension will be always poorer than in declination. The Avalon fully belt driven system produces a periodic error with such a long period that your guiding system will always be capable to correct it and therefore delivering high performance guiging results.
- Gears roughness: gears are made of metal and while the grease reduces friction and wear, rough spots on the gear surfaces generate sudden tracking movements (spikes). When a guiding graph shows a sudden spike, your photo is most likely ruined or the stars in your photo will look ovalized. The effect is similar to wind gusts that do ruin your shots. Avalon does not use gears so the guiding performance is strikingly high!
- Backlash: in mounts driven by gears, backlash is caused by a gap between the gear teeth and it causes a play and consequently a delay in the guiding responsiveness. Some mounts allow a backlash compensation, producing a quick acceleration of the gears until the gear teeth touch and then transmit the rotation. However, the backlash varies along different points of the worm drive and generally also increases overtime. Avalon and its fast reverse technology produce an immediate guiding response as the system employs pulleys that do not suffer of backlash.
Pulleys and toothed belts, zero backlash!
This choice has allowed to obtain several advantages: a very steady motion without play (no backlash) or sudden peaks, which are factors of paramount relevance for long guided exposures and during high magnification visual observations. These features are of particular relevance especially for the declination axis motor which can now quickly reverse the motion without breaks to recover the plays: hence the mount name FAST REVERSE. The toothed belts used in the M-Zero have the structure made of special material with steel strands to avoid any deformation, elongation and stress, much better than those used in the automotive engine distribution system (which are generally made of rubber with nylon strands). Comparing the service time for the automotive toothed belts, which is around 100.000 km, assuming a medium regime of 2.000 rpm and thermal stress from 0 to 90°C in a few minutes, we can assure that the life cycle of the m-Uno toothed belts will be extremely long!
It is important to point out that in the gear-worm systems the motion transmission has only one tangent point of contact; any error on each of the two components will sooner or later result in a tracking error.
In the pulley-toothed belt system, no direct contact occurs and the motion is transmitted by the belt, engaging from 50% to 90% of the girth surface. Consequently, any eventual error present is averaged among the cogs and greatly reduces the tracking error.
No wear, no friction!
No wear since no relevant friction occurs. In fact, all the pulleys and the axes rotate on roller bearings allow to reduce the total friction almost to zero.
Another significant advantage of very low friction is that the risks of motor slipping during GOTO operation is virtually nil.
On the contrary, it is well known how difficult it is to regulate the coupling between gear and worm in conventional mounts. If the coupling is tight, the motors can get stuck with consequent loss of the position, if the coupling is too loose the play increases.
On the other hand, the absence of significant play in the M-uno makes the initial calibration quick and easy.
No lubrication, no maintenance!
Since there are no gears, there is no need for periodical lubrication of the internal components and therefore the maintenance is much reduced and limited to the external cleaning.
it can be performed using the polar scope mounted on the RA body that can be rotated (as shown in the picture below) to the upper position for a comfortable adjustment of the Polar Alignment.
The standard kit includes:
2. Support stand provided of scope fixing knobs and dovetail attack with fixing grip knob.
3. Illuminator cap provided of red LED and connection cable to the StarGO.
Single arm fork equatorial mount
8 kg for imaging (13 kg with double scope setup), 10 kg in visual mode
10.1 kg (12 kg with tripod)
Four stages belts drive system
CNC anodized aluminum
|StarGO GoTo Control System with WiFi|
|SkyWatcher polar scope (optionally Losmandy model)|
|2 years (5 years for the belts)|
- Single Fork Equatorial mount,
- Vixen Style dovetail saddle
- Mini counterweight bar
- 0.5kg kg counterweight
- Tripod T-Pod 90