Khan Scope Centre AstroNotes Newsletter
The
Lunt LS152 H Solar H Alpha Telescope Finally arrives!
ᅠᅠᅠᅠᅠᅠᅠᅠᅠ
It was an exciting day on May 5th, when our first LS152mm Lunt H Alpha
Solar Telescope arrived! Being that the Sun was out, we got
the instrument out to test it immediately (Thundershowers were forecast )and
were treated to a few prominences
and a couple of flares right off the bat!
This instrument is a real a jaw dropper; we
really can'''t wait to see it in more action!! We expect to show one off at the
Starfest Astronomy convention in 2010, held in Mount Forest, Ontario,
so if you are able to attend, drop by our display and check it out!
This new refractor based telescope has a front aperture of 152mm with a
precision aligned doublet lens. An un-obstructed 60mm internal etalon that is
tuned with the new Pressure Tuner allows for views at <0.65 Angstrom band
pass.
Aperture: 152mm
Focal Length: 900mm
Band Pass: <0.65 Angstroms
Etalon Tuning: Doppler True Pressure Tuner
Blocking Filter: B1200 standard
Focuser: Starlight Feather Touch Focuser
Color: Pearl White with Black Anodized Accents
The LS152THa can be used in either a Ha or CaK mode. There is a removable
Hydrogen-alpha module that can be switch out with a CaK module.
Being the largest aperture Solar Telescope currently available, the LS152 is
sure to provide the most stunning balance of resolution and performance.
This package is perfect for the Intermediate to Advanced User.
If it''s image scale you''re after, the LS152 provides the largest and highest
resolution image size of any single etalon dedicated scope. The 100%
unobstructed system will perform to the highest level at both low and high
magnifications. Utilizing both advanced hi-contrast coatings, and the new
Doppler True Pressure Tuning system, the user will be able to experience crisp,
sharp, high magnification visual images, as well as utilize this system for high
end digital processes.
The system has an optional, interchangeable, CaK module allowing for the
research of multiple wavelengths thru the same platform.
This long awaited instrument, over 3 years in development, is for the serious
H-Alpha Enthusiast.ᅠ If that's you, then you will want to order one of
these
knock out instruments today! To order Toll Free, Call 1 800 580 7160
or local 416 783 4140 or email us at info@khanscope.com
or for details
click here
Just arrived....and New for
2010!ᅠ
- The Meade LT 8 ACF is a full featured, computer controlled 8"
telescope with Advanced Coma-Free (ACF) optics.
- The Meade LT 8" ACF telescope includes UHTC - Ultra High
Transmission Coatings for distortion-free, tack sharp images.
- AutoStar guides the telescope to 30,000 objects in its comprehensive
library, automatically.
- Level North and Easy-Align Technology makes all LT-8's easy to use - right
out of the box!
Now in Stock for immediate delivery! Only $1725 Complete
Package. but don't wait...order before it's too late!
To order Toll Free Call 1 800 580 7160 or local 416 783 4140 or email
info@khanscope.com
Celestron
Telescope Sale!
Save up to $1400 on a Celestron Schmidt-Cassegrain...!
It's not often that we can offer
savings like these on many
popular Celestron telescopes like these. If you have been on the fence
then now is the time to act. You can even trade in your existing
instrument
to take advantage of this Sale.
Right now, we are offering instant savings on select
Celestron Telescope models
and Optical Tube assemblies as well.
Don't Miss your chance to save $$$.
The Advanced Series of 6" to 11" go-to SCTS and
the Celestron CGEM Series.
And...the Celestron CGE Pro 9.25" to 14" go-to
Schmidt Cassegrains.
Finally, Savings on Celestron Optical Tube assemblies only
from 6" to 14".
This sale ends May 31st or while quantities last.
Click
here for all the details.......
New
for 2010!ᅠ
Mallincamᅠ VSS Colour Plus
Order Now!
Now
with Variable Shutter Speed!
The easiest way to Astro-image just got better!
Question: What makes the Mallincam VSS model different
from previous incarnations?
Answer: Simple! You can now control the Shutter speed of
the Camera. This makes it ideal
for planetary and Deep Sky imaging. Plus the fact that the Mallincam is
easy to use.
If you are doing any kind of public education, or just observing in a group, or
with family or friends,
then utilizing the Mallincam for Deep Sky observing, even in a light polluted
city like Toronto,
makes all the difference, in terms of details you will see on your PC or
Monitor, versus your telescope
eyepiece.
When in Toronto, we invite you to drop by our retail store,
where we have over 70 Telescopes on Display! We are open 7 days a week to serve
you better.
There are several restaraunts in the immediate neighbourhood and we are also
close to the Subway.
The TTC bus stops right outside our door!
Khan Scope Centre
www.khanscope.com
3243 Dufferin Street
Toronto, Ontario. Canada
M6A 2T2
Phone; 416 783 4140 Toll Free 1 800
580 7160
email: info@khanscope.com
Spring Retail Store
Hours 2010
Monday to Wed: 10am to 7pm
Thursday: 10am to 8pm
Friday: 10am to 7pm
Saturday: 10am to 7pm
Sunday: 11am to 6pm
Cassegrain Telescope Collimation Breakthrough! Our Friends at Hotech have finally come up with a Collimation Device to Accurately Collimate CT Telescopes.
That includes Maks, RC and SCT models made by various manufacturers.
Up until now, the only real way that we have been able to collimate an SCT has been with an actual Star test.
not much fun when its -20 outside!
Collimate Your Cassegrain Telescope
- Without using a star
- Indoor or outdoor - day or night
- Focus stays at final view setting
- Within focal distance from your telescope
- One-man operation
- Portable and simple to setup and use
- Works on CT, SCT, Maksutov, & RC
"This is a very clever device. By using three perfectly aligned laser beams it simulates the parallel rays coming from a distant star. The beams then pass through the telescope twice to amplify any error in the entire system making even small miscollimation errors readily seen and fixed. David'''s done his homework on this one, coming up with a very ingenious answer to daytime collimation of an SCT."
Craig Stark, Ph. D. Associate Professor of UCI and Founder of Stark Labs & PHD Guiding
Innovation brings Affortable and Portable Collimation into Reality
Since the invention of the Cassegrain Telescope in 1672 by the French sculptor Sieur Guillaume Cassegrain, the Cassegrain Telescope has evolved into various derivative designs such as the more popular Ritchey-Chr←tien, Dall-Kirkham, Schmidt-Cassegrain, and Maksutov-Cassegrain. The designs have gained their popularity because of their compact and simple to produce design. With different designs, star collimation is and has always been the only effective method to collimate for Cassegrain telescope owners.
Now, backyard astronomers have an alternative to achieve excellent collimation conveniently using the Advanced CT Laser Collimator. The Advanced CT Laser Collimator brings the collimating star to your telescope within arm reaching distance. With its short range capability, you can perform collimation indoors - day or night - without being subjected to weather conditions. And best of all, this new collimator utilizes a clear and simple-to-read, large target display for the telescope alignment diagnostic. This large target display is within a short focal distance of the telescope which allows you to collimate without guessing.
No Star Required to Collimate
In order to achieve an accurate star collimation, normally the amateur astronomer requires good seeing conditions with no cloud, no wind, stable temperature, no light pollution, a well-aligned telescope mount tracking system, telescope optical tube assemble (OTA) thermal equilibrium, and a good visible magnitude star. The visual quality of the referencing star is greatly affected by the prescribed factors most of which are all in Gods hand as you can see in the photo. Adjusting the collimation is guessing game where you move between front and the back of the telescope adjusting the corresponding alignment screw and holding your breath peeping through a high magnification eyepiece referencing the concentricity of the unstable defocused image. This can be an incredibly frustrating experience.
An artificial star can never simulate a real star because it is impossible to collimate with the telescope focus set at infinity. After artificial star collimation, you will need to adjust your focus back to infinity to view a real star by moving the primary mirror to a different position. The distance the primary mirror has been adjusted can accumulate mechanical tolerance errors. For some of the mass produced SCTs, the sticky baffle on the primary mirror focusing mechanism may also cause mirror-flop. If a mirror-flop has ocurred, it will affect the alignment position which in turn will render the collimation useless. Ideally, It is best to collimate your optics at the same viewing focusing position without major optical displacements to correspond to the final view setting. The Advanced CT Laser Collimator can accomplish this task without all the possible accumulated errors.
The large target display on the Advanced CT Laser Collimator brings you a clear visual queue of three projecting laser dots as the alignment reference at a very comfortable visual distance providing an accurate axial alignment error diagnostic. And during the entire collimation process, no major focusing is needed, thus minimizing the possible accumulated errors from the focusing adjustments. The referencing adjustments are made by bringing the three clearly discernable projected laser dots projected on the target, into a concentric ring. No more peeping through the eyepiece looking for a changing, ambigu star image. This alternative collimation method saves precious observing time by collimating the telescope and preparing the viewing programs at dusk or before dawn without the influences of the external environmental conditions.
Collimate Within Focal Distance From Your Telescope
The Advanced CT Laser Collimator does not require long focal distances to achieve high-accuracy collimation. Utilizing the installed flat mirror at the focal point (eyepiece location), the collimator lasers double-passes both your primary and secondary mirrors and magnifies the alignment errors to a higher accuracy level. In addition, it also cuts the collimating distance in half achieving near-field alignment process. The collimator is stationed within your telescope'''s focal length directly in front of your telescope. Setting up for collimation, you will be standing between the telescope and the collimator aiming both the telescope and the collimator at each other. Then you will adjust the secondary mirror knob to bring the returning lasers on the same track. This is a very convenient one-man operation.
At a Fraction of the Cost of Wavefront Interferometer Technology
The state-of-the-art advanced laser optical alignment technology used in the Advanced CT Laser Collimator achieves the same rough alignment function of a costly large aperture interferometer commonly use in high-energy labs at a fraction of its cost.
The Advanced CT Laser Collimator uses three collimated lasers, evenly spaced apart, to sample large aperture optical elements in your telescope. The three parallel laser beams completely simulate the light path (flat-wavefront) from a distant star and pass through the entire telescopes optical elements and reflect back to its target for a complete and accurate double-pass diagnostic reading of your telescope optical alignment. This innovative collimation technique and technology enables the amature astronomer to achieve far-field collimation as a near-field process.
Precision CNC Machined Panel and Components
This beautifully designed instrument is precision machined from a solid block of aero-space grade aluminum. It is then hardened and anodized to keep the entire mounted laser system thermally stable allowing you to achieve accurate collimation. The rigid, ultra thin profile, and light-weight design makes the unit portable and simple to setup and use.
Collimates All CT, SCT, Makustov, & RC Price: $555. |
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