The star test is the ultimate method to test and collimate your telescopes. The most and
very much the only difficult part of doing the star test is that you need a star. Sadly, a real
star is not always available, and you really may not want to spend your precious
observation time doing star test even when it is available.  Of course, you will also need a
good tracking system for doing star test with the moving star. After all the troubles, due to
the turbulence, the real star may not even reveal the true quality of your telescopes or give
you a perfect collimation.

An artificial star will provide you an excellent alternative mean to do the star test anytime
and anywhere you want, without all the drawbacks of the real stars. However, the problem
with the artificial star is that you really need different size of artificial stars for different
telescopes of different apertures with different F/#, and even for the same telescopes but at
different distances, and under different lighting environment.

The innovative Hubble 5-star Artificial Stars is a perfect solution to this problem. It has 5
bright white LEDs with 5 precision pinholes (50/100/150/200/250 microns). It will enable
you to test practically all the telescopes of different apertures with different F/#, from any
reasonable distances needed, and under different lighting environment.

We are not suggesting that you should stop using any other methods or any collimating
tools you feel comfortable with. You can continue your current practice, but after that always
use the star test to validate or confirm your scope is indeed in perfect collimation; no other
method (except the star test) can guarantee a perfect collimation. If your scope is still not in
a perfect collimation after your current practice, you need to use the star test to fine-tune the
collimation to its perfection. However, if you do not have any other collimating tool yet, then
a star test with Hubble 5-star Artificial Stars alone will enable you to reach a perfect
collimation with your telescopes.

  • You can instantly find out which star is best for your particular telescope at that
    particular distance under that particular lighting environment by simply choosing the
    smallest possible star, but which still give you clear defocused image
  • You can even adjust the brightness of the stars by twisting the LED cap.
  • You can mask out any 4 of the 5 stars with a provided magnetic mask.


With Hubble 5-star Artificial Stars, telescopes are truly easy to test and collimate!

Special Introduction offers:
The single unit: $24.95 ($19.95 +$5 Shipped Worldwide)
(regular price $29.95)


The 2 unit pack: $46.40 (Shipped Worldwide)
(regular price $55.50)

(Shipped via HKPS airmail,  6-10 business days delivery)
  • Please make sure the cleanness of the mask, and use it only when needed to
    prevent the blockage of the pinholes.
  • The unit should be kept in a clean Ziploc bag when not used; separated from the
    magnetic mask.
  • It is powered by 3 AAA batteries (Not Included).

Please note that there is NO printed instruction in the package. You just need to insert 3
AAA battery cells, and turn it on.

Here are some very useful online helps on star test:

Telescope Collimation via Star Test by Thierry Legault
Basic Star Testing by Stephen Tonkin
Aberrator, an extremely useful star test simulator by Cor Berrevoets

A must have book by Harold Richard Suiter:
Star Testing Astronomical Telescopes, Second Edition
There is also a brief but excellent chapter on the star test in Richard Berry’s
Build Your Own Telescope
Copyright 2009, All Rights Reserved
Q1:  Is there a printed document for the Hubble 5-star Artificial Star(s)
There will be no printed document. But we will maintain this online FAQ up to date as a
brief document to the 5-star.  
Here is the printable version of this FAQ.
For complete and detailed instruction on the collimation and star test, please refer  the
must have book by Harold Richard Suiter,  
 Star Testing Astronomical Telescopes, Second
Edition

Q2: Where do you place the 5-star during the test?
The 5-star can just sit on a tripod top, on a table, or even on a rock; you only need to aim
the star roughly towards (no precision aiming needed) to your telescope; then aim your
telescope to the 5-star. The 5-star provides a very wide angle for a very easy usage.

Q3: Which of the 5 stars to use for the star test?
Choose the smallest possible star, but which still give you clear defocused image. You
may need to dim the stars with the new batteries by twisting the LED head cap. Basically
you change the brightness by adjusting the alignment among the LEDs and the pinholes.
It is time to change batteries if all stars are too dim to see clearly.

Q4: How far should the 5-star be placed from the telescope?
The 5-star should be placed in a distance to you scope about M times of the focal length;
M is 336*D/F^3, or 336*D/(F*F*F) for a Newtonian(May, 1991, Sky and Telescope, Roger
Sinnott), where D is the Clear Aperture  (in inches) and the F is the focal ratio. E.g., if your
scope is 10" F/5, then the M is 336 x 10 / 5^3 = 336 x 10 /(5 x 5 x 5) =26.88. So the 5-star
need to be M  x  D x F = 26.88 x 10 x 5 = 1344" away, or about 34 m away.  In general, a
minimum of 20 for the M is suggested by Suiter.

The above distance is for the real star test, for the collimation purpose; about 70% of
above distance is good enough.

As long as you have enough back focus to focus on the close by object,  you will be
surprised how close you can get for the collimation. You may need to add one or two
focuser extension tubes.

Q5: How to perform the collimation with the 5-star?
First you should check if the scope is in rough collimation by observing a strongly
defocused star image (about 10 wavelets, or move focuser in or out until seeing about
5-10 rings). All rings and shadows should be concentric; if not, please perform the
collimation according to the instruction of the telescope until all rings and shadows are
concentric. You should do this at a magnification of 25X of your scope’s diameter (in
inches).

Coma due to misalignment of a 10" F/8 scope:
Then you need to do a fine and final collimation by observing the focused 50 microns
star image, the famous Airy disk with a magnification of at least 50X of your scope’s
diameter (in inches). Use a 2X, or 3X Barlow lens if necessary.  You should see an
uniform, complete, and concentric Airy disk and diffraction rings if the scope is in
perfect collimation. Follow the same procedure to do minor adjustment on your scope
until you reach a perfect collimation.

This is the final judgment of the collimation of your telescopes and all other
collimation tools and methods! Due to the seeing limit, you will be most likely unable
to do this with a real star!  Actually with a real star, most likely you will be unable  to
see the Airy disk!
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-IT WORKS

-The best $20 astronomical investment I have ever made.

-My SCT was collimated better than it's ever been that night, and, I did the
collimation in broad daylight.

-Wow, it really works, even at 86 ft. I just have to keep direct sunlight off
the artificial star so there's enough contrast to see the "airy disc" and
you're good to go. I can't wait to see it against the stars tonight, my scope
was pretty decently (and quite noticeably) out of collimation. Now I feel it's
pretty darn spot on.

-I first made sure the focuser was properly aligned.  I then used a barlow laser
to make sure both secondary and primary were aligned. Then using the
artificial star, I tweaked the primary. I had to move two knobs each about 1/8th
of a turn at most. I then locked the mirror with the locking screws, and pointed
up at polaris. It was pretty darn spot on…

I measured the holes of both (units) using a scanning electron microscope
at work... The microscope can reliably measure down to less than 10
nanometers (0.01 micrometers). Considering a single 50 micron laser
drilled hole in stainless steel disc (unmounted and no LEDs) can run $40-
50 from commercial suppliers here in the US, this is a fantastic bargain!
Thanks very much.

-Your 5-Star Artificial Star is GREAT! I've never had an easier time collimating my
SCT. Thanks for a great product.

Great product, good price! I wish I had bought this sooner!!
Q5: How to perform the star test with the 5-star?
Choose an appropriate star for your scope (Q2). After making sure the scope is in
perfect collimation(
Q4), follow the normal Star Test procedure to perform the test.
Please make sure all cells are inserted in the right direction, spring with the
negtive end. You may try to reinsert the cells to make sure all are in good
contact.

Q7: How was the Hubble Space Telescope tested once it had been
launched into the space?
The star test was used extensively and exclusively for the diagnosis and
verification for the Hubble Space Telescope in the space.

Referring to the last image attached (The imaging performance of the Hubble
Space Telescope, by C.J. Burrows et al, Astrophysical Journal, March, 1991),
"The left two columns (note that the first and third columns in the first two
rows are not clear enough to be visible) show observed images of bright
stars at two different scales, while the right columns show correspond
models. The top two rows show images taken on each side of the nominal
focus position. These images clearly demonstrate the presence of spherical
aberration. Instead of a uniformly illuminated pupil image, the inner or outer
edges are brighter"
Here is a description (F. Roddier, C.Roddier, Appl. Opt. 32, 1993) on how
the star test was conducted on the Hubble Space Telescope (HST) , “we
requested that the highly defocused images be taken in flight by HST so
exact amount of spherical aberration. Because defocusing the imaging
also defocus the telescope tracking system (a kind of off-axis auto
guider), it was not possible to obtain images sufficiently defocused for
the method to apply. However, defocused images recorded by the HST
are not blurred by the atmosphere and can be taken through narrow-
band filter. In this case the wave-front information is still preserved and
can be recovered by using phase-retrieval algorithm”