2010/03/18
The First Light of Herschel Wedge
Goodbye my C5
2010/02/13
Small 60mm China made refractor and reflection
At a first glance, the finish of C60 is bad, however the design is good. It has an extension tube and the eyepiece holder is even equipped with compression ring! One just needs to screw the extension tube into the end of the focuser and it works for webcam.
The handcraft is by no mean good! So what about the optics? I used Nagler 2-4mm and 3-6mm zoom in both C60 and FS60C. The big problem of the C60 is that chromatic aberration in any magnification is pronounced, especially when viewing high contrast objects. In fact I tried to use Baader Planetarium 8-24mm zoom to test the low magnification performance of it, the problem persisted. Another bad design of the C60 is that the inner tube of the focuser is very long and the inner diameter is smaller than 60mm. I guess this makes the effective aperture of C60 smaller! Look at the attached photo. On the other hand, the chromatic aberration in FS60C is very small. One can detects it when the magnification is very high, say larger then 355/2.5=142X. Of course this is a rough figure. The result may vary from different viewing conditions. My subjective opinion about the maximum acceptable magnification of both scope are:
C60: 220/2=110X
FS60C: 355/3x2.5=296X
Beyond the above magnifications, the contrast would be too low.
I used to use 5-point scale to rank telescope. If I keep on use this scale, I must give the C60 negative score! However I found that I was spoiled by those ED/APOs! I have several refractors. Some are achromatic and some are EDs or so-called APOs. After I got the ED/APOs, all my achromatic refractors are sitting in the store room and gather no more photons. I do most of the visual observations and imaging with ED/APO refractors. I never seriously look back the achromatic refractors again. Until this test, my instant feeling was that I bought garbage! Then I dug out my Meade ETX70. Although the finish is good compared with C60, the chromatic aberration is very bad. I do remember I was once satisfied with these achromatic refractors. Now I say they are garbage! I was really spoiled by those ED/APOs! In most of the time when I do optical testing of those ED/APOs, I deliberately push the magnification to limit, point to bright and high contrast objects and do rigorous star tests etc. Radically fault picking the scopes. Sometimes the differences can be only be identified by experienced telescope users. In fact if one is not doing a side by side test, I doubt the results are reliable. I asked myself is it the way to promote astronomy. I can say virtually all the telescopes we used nowadays are much better than the one used by Galileo 400 years ago. His achievement in astronomy was tremendous! I reckon that always talk about prestigious telescopes may not be the way to promote astronomy because the price of those prestigious scopes are too high in some sense. We should introduce more good value scopes, for example Sky-watcher Mak 127, Celestron Nexstar 4SE or even binoculars, to the public. These good value scopes once lead me to the world of astronomy. Anyway, in terms of optics, test result is follow (10-point scale):
C60: 4 (Moderate blue and red aberration, but more contrast than ETX70)
Mead ETX70:5 (Severe violet aberration, but sharper than C60)
Takahashi FS60C: 8 (Sharp, high contrast, by all mean winner in this test)
2010/01/29
LS35T Sent for Repair
2009/11/20
Equinox 66 Vs Tak FS60C
I went to David’s school at about 5:00pm yesterday. We setup all the scopes quickly. David’s students were good helpers and little judges. I guess they are trained to be experienced telescope users. The main disc was Equinox 66ED Vs Tak FS60C. However, there was another super star TMB 80/480. The main concern was the chromatic aberration. We selected some white light sources from distant buildings. In addition, we luckily found some really small bright spots which can be treated as point source. So we did “star test” as well. However, one should be reminded that these artificial objects were much brighter than Sirius and even Venus. Using these artificial sources was extremely harsh to telescopes.
At the first sign, both scopes are strongly built. I like both focusers, although Tak FS60C got no dual speed, it is firm and solid. While the Equinox’s dual speed focuser makes focusing easier. We used the Nagler 2-4mm zoom and Nagler 3-6mm zoom. Ordinary diagonals used were used. For comparison purpose we set the magnifications of Equinox and Tak to 400/3 = 133X and 360/3 = 120X respectively. Despite low contrast, both scopes didn’t breakdown even at 2mm eyepiece focal length. The trends of CA of both scopes were similar. There were some violet in front of the focus and some green behind the focus. However the degree of CA was different. The CA of Tak FS60C was very small. The CA of Equinox was small. Both scopes gave good “star test” results. All the diffraction rings were symmetrical. However the pattern in front of the focus and behind the focus in the case of Tak FS60C was a bit better. We repeated all the comparisons by swapping the Nagler 2-4mm zoom and Nagler 3-6mm zoom, the results were the same, which means the differences were not from the eyepieces, but the scopes. Anyway, the difference in CA was not big in fact. So what really make the difference in this comparison? Resolution!!! David and I found that the resolution tells the difference. Tak FS60C gave shaper images.
About the CA of Equinox 120ED, it was reported in Cloudy Nights that if one stops down an Equinox 120ED to 110mm, it was virtually color free. So I tested this idea in Equinox 66ED. Since I could not find a compass this morning, I used a cap to draw a circle. The diameter of the stopper was then 58.5mm. There was still CA exists and showed a bit improvement in violet. I couldn’t see improvement in green.
Well, the final verdict cannot be made. The reason is that in real sky observations, stars are much dimmer that artificial lights. The observed CA in very bright artificial lights may not be detectable by human eyes in the case of real stars, so further test is needed.
2009/11/10
DIY Bi-scope Platform
Weight of Bi-scope Platform
A Quick Observation
2009/10/27
Lunar Image Taken with Equinox 66ED
2009/10/26
Equipment Testing: Equinox 66ED
2009/10/19
Equipment Testing: Meade 8 ACF, APM/TMB 80/600 & Equinox 66ED
The long waited Meade 8” SCT AFC was finally settled! The order has been delayed for many times and I’ve disappointingly waited for half years. Finally I got an offer from a local stargazer who bought this telescope in a special offer given by the local dealer half years ago. The reason that he sold this M8 was that he got another extremely cheap LX200 offer. The M8 ACF he sold to me was very new. It has been used in field, Pak Tam Chung, for once only. I was lucky enough to get it because another stargazer told me about this and I responded fast enough to it, or the chance would go! It is very hard to get a used M8 ACF in Hong Kong. Although he sold me at the same price he paid half years ago, it was still a good price and it healed my pain at once! Last night, the sky condition was so so. The transparency was ok, but the seeing was bad. With clouds running around, I could hardly catch a few moments to look at Jupiter. Nothing could be concluded, but the M8 worked. The maximum magnification I tried was 2000/9 = 222X.
Another encounter was the trial of the APM/TMB 80/600 APO. I went to the Sky-watcher dealer and replaced the long tripod with a short tripod for the EQ3Pro. Sky-watcher is certainly a homely-made like manufacturer. Their product specifications change from time to time and even their dealer doesn’t know it! Their product specifications can be modified according to requests! This is odd, but flexible right! I am an efficient guy. I know the dealer got a used APM/TBM 80/600. It would be nice if I can have a look at it before it was sold to somebody else. I deliberately arranged the tripod replacement and the glance of the APM/TBM APO in one go. Ha Ha! In fact the main course was the APO… Well, it was daytime, I did the terrestrial observations only. The first eyepiece I tried on the APM/TMB 80/600 was 25mm Aspheric Orthoscopic. When you look through the eyepiece, the feeling was WOW! The image was so sharp and the contrast was so high. The image was sharp to the edge of the field. This telescope was the best I’ve ever seen for terrestrial observation! I cannot imagine what will happen if I use the APM/TBM 203 to do terrestrial observations! The color tone was warm. The Aspheric Orthoscopic gave good eye relief and the field was reasonably wide. The viewing was so pleasing and comfortable. When I put the 16mm TBM Super Monocentric, which is supposed to be a top planetary eyepiece, the off-axis image was a bit blur. However, the image around the principal axis was extremely sharp and of very high contrast. The color of the Mono was not as warm as Orthoscopic. I didn’t have the chance to compare these two eyepieces on viewing stars side by side that day. I couldn’t comment which one was better for stargazing. It would be nice to do it later. Finally I tried the 13mm Ethos. There is no need to mention about its field of view. The viewing was very comfortable. The image was sharp and the contrast was high. I couldn’t tell the difference in sharpness between Aspheric Orthoscopic and Ethos. Both are very good eyepieces, which need longer observation and being tested to differentiate. Again I was in a rush to go! So try again next time.
I borrowed the Equinox 66ED from the dealer for a short period of time. I tried it in daytime recently. A first look at this little scope, it inherited the beauty build of Equinox series. I have tried Equinox 80ED and 120ED, now the 66ED. The only Equinox I didn’t try is the 100ED. Well, the optic of this scope was good. I used Skywatcher eyepieces and Tele Vue 2.5X and 5X Powermates in the entire testing. For daytime terrestrial observation, if the magnification was below or equal to 400/5 = 80, the color, sharpness and contrast are very good. It doesn’t mean it will breakdown when the magnification goes beyond 80, but will not be too promising to use it for birding or other terrestrial observations as the contrast and the brightness are low. I tried to boost the magnification to 400/8*2.5 = 125X and 400/15*5 = 133X respectively. I was able to see the price tag of a fruit store. I guess the characters’ size was about 5cm and the store was about 1.5km apart. A quick estimated resolution to achieve such an observation is 5X10^-2/1.5X10^3 = 3.3X10^-5. The Rayleigh resolution, theoretical maximum, is 1.2X550X10^-9/66X10^-3 = 1.0X10^-5. It is not bad right! However, if it is used for stargazing, the magnification can be boosted further since the background is much darker. It all depends on what celestial objects you are going to watch. For the 200X, I tried in different settings, 400/2 = 200X and 400/5X2.5 = 200X. The 400/2 = 200X gave a slightly better performance in terms of sharpness and contrast. At such magnification, the contrast was very low. However, the image didn’t breakdown completely. One could still see some details. The corresponding magnification per inch is above 70X. It is a good figure already. I owned a small achromatic refractor, Meade ETX 80. Its optical performance cannot be compared with Equinox 66ED in terms of chromatic aberration and resolution. To be fair, the price of ETX70 was just a few hundred. Although optically it is a loser, it is a best buy.
2009/09/26
Top equipment, but hazy sky!
At a first glance, the tube material was robust lightweight polymer. Both 100mm/F800mm and 130mm/F1200mm can be mounted on EQ3Pro. I forgot to carry both APOs and got a feeling of how heavy they were, but they should not belong to heavy class. Everything was strongly and nicely built. The base and the bracket of the finder scope were quite unique. I would not say it is stylish, but the design concept was neither Japanese nor Chinese, but German. The Feather Touch focuser was solid. Well back to the main dish, optical performance. Both APOs delivered high contrast images. I tried another 12” Newtonian last night. The Newtonian deliver brighter images, but it contrast was far below than that of APOs at similar magnifications. We boosted the magnifications to 288X and ~500X for 100mm/F800mm and 130mm/F1200mm respectively. These mean we pushed the limit to 72X/inch (288X) and 96X/inch (500X) respectively. The 100mm/F800mm was able to handle 72X/inch. Although the Jupiter image was breakdown under 96X/inch for the 130mm/F1200mm, one could still see some color fringes of Jupiter. That was not a flat images disc of Jupiter.
Last night there were two points I especially want to mention, the chromatic aberration and the resolution of the surfaces the Jupiter’s satellites. When I used the APOs to observe the Jupiter, the north pole of the Jupiter was a bit bluish. The dealer said it was due to atmospheric chromatic aberration, not the chromatic aberration of the APO. Here comes the question! Is the dealer telling the truth? To me, this is a physics question. If the optics got no or low astigmatism, the chromatic aberration should be cylindrical symmetric. There should be false color around the star, not just appearance in certain direction. My conclusion is that the bluish color at the north pole of Jupiter was caused by atmospheric aberration. One can do some experiments to verify this. Use the same telescope to observe the same object and see if the position of the aberration changes with time. About the resolution of the surface of the Jupiter’s satellites, moon surface, we saw all four satellites, IO, Europa, Callisto and Ganymede. The dealer and I were not sure about the moon surfaces were revealed or they were just Airy discs. As the magnitude of those satellites were small, probably larger than 5. When I observed the satellites by the 100mm/F800mm APO, it seemed that I saw the 1st order diffraction ring, but I was not sure. But it was possible that it was Airy disc. When we used the 130mm/F1200mm APO, the image of the satellite improved a bit. The hazy sky kept on discourages us whole night. It seemed that the 130mm/F1200mm APO gave a more solid image. However, it was illusion or fact. We need to wait for the sky. But it is highly possible that these two APOs will be delivered to new owners. So what can I do! Ha! Ha! Use theory to justify it! As these two APOs were claimed to be diffraction limited, we can do some calculations and see if it is possible to see the moon surface.
The visual angles in arc second of the satellites are:
IO 1.2”
Europa 1”
Callisto 1.6”
Ganymede 1.7”
By using the Rayleigh Criteria, we can calculate the theoretical limit of the resolution of the telescope.
R = 1.2 L/D where R is the resolution, L is the wavelength and D is the diameter.
The resolution calculated is in radian, we can convert it back to degree easily. In order to get a feeling of how good is the optics, I assume the average wavelength of visible light to be 550nm. After some simple calculations, for diffraction limited optics, the resolution of different diameter in arc second is given below:
100mm 1.36”
130mm 1.05”
203mm 0.67”
It means that 100mm APO is not able to resolve the Jupiter’s moon surface. The image was just an Airy disc. The 130mm APO can barely resolve the Jupiter’s moon surface. The 203mm APO can resolve Jupiter’s moon surface. This is a simple discussion, meaning that if the optics is diffraction limited, it is possible to resolve it. On the other hands, the practical optic is not possible to go beyond the theoretical limit.

APM 100mm/F800mm

APM 130mm/F1200mm

Newtonian 305mm/F8.5
2009/09/23
Equinox 120ED and DBK21

Jupiter, Equinox 120ED, TV 5X, DBK 21
2009/08/15
Equipment Review
Tele Vue 2.5X and 5X Powermates
Unbranded 127mm F750m Refractor
2009/08/02
Sidewalk Astronomy and Telescopes Watching
After I walked around for a while in Tin Shui Wai, I decided to go to have my own star gazing. I rang my friend Lewis and our destination was Lung Ha Wan. We arrived at Lung Ha Wan at about 10:30pm. But the favorable location was occupied by some midnight divers! Gee! We wanted to try a new location, but it was just being occupied by others! Anyway, Lewis and I looked around and see if it was a good location for star gazing. But sky was very hazy and we could only see the Vega, the Jupiter and the moon. As there were no favorable car parks, we decided to go to good old Pak Tam Chung.
When we arrived Pak Tam Chung, there were no star gazers! I was fooled by those posts in the forum. Maybe everyone went to Tin Shui Wai. Well! We two lonely twins stated to setup our scopes and practice. The sky condition became very bad. When we arrived we could see the blurred moon, the fading Vega, the dim Polaris and Perhaps the bright Jupiter. I tried to setup the HEQ5Pro as quickly as possible. At the point I wanted to do the polar alignment, the Polaris was gone! So I used the compass to solve it. Unexpectedly the alignment done was quite good. The tracking of Jupiter was good. We shot the Jupiter with different imaging device, D90, 450D, SPC900NC and LPI. Both D90 and 450D have life-view which was very useful in focusing. But all the photos taken by D90 were unsatisfactory! We don’t know clearly why D90 failed. Maybe it was because of the flip mirror of D90 in the life-view mode flips before the release of the shutter, while 450D not. The small vibrations of flipping the mirror caused the burred images. As a Nikon user, I need to figure it out! This needs another investigation. My second task was to align the NexStar 4SE mount. It just couldn’t track the sun probably during the recent solar eclipse. I believe that ex-owner didn’t get it alignment in 2-star alignment or 3-star alignment once. According to the manual, one needs to get NexStar alignment once with at least 2-star alignment once before it works properly. However the noxious clouds covered the sky. You know! Finally I gave up and went to have dessert in Sai Kung. Today I tried to process my photos. I still don’t know how to use Registax. The photos shown were just click-click-click product.




2009/07/18
PTC’s Starry Night: Equipment Testing
2009/07/07
My new LS35THaDX




Shortly after the launch of LS35T, people found that it was not webcam focusable. It was basically the optical tube or the focuser tube was too long. Lunt didn’t give resolution for the first batch of LS35T, but will rectify the upcoming LS35T. Since the modification is very simple, either make a shorter optical tube or a shorter focus tube will make it works. Maybe this is a cheap solution that to let the local dealer to make the modification rather than ship back all the scopes and modify those scopes by Lunt.
The reason I bought the first batch of LS35T was that it was not simply a deluxe package, LS35THaDX. The lens of the first batch of LS35T was made by Carl Zeiss. I was told due to the mass production problem; Carl Zeiss could not meet the Lunt’s specification with a reasonable low cost. So the upcoming LS35T will not use Carl Zeiss lens anymore. In addition, the blocking filter of this special batch was B600 instead of B400. So I treat this special Carl Zeiss batch or prototype as a collection.
Well about the performance, today we got a beautiful sunny day, I tested the LS35T. Recently the sun is very claim. I was very lucky that I saw two sunspots and one prominence. The locations of the two sunspots were around 4:00 to 5:00 and the location of the prominence was around 12:00. I could see the details of the sun disc. Since I don’t have PST experience, I can only compare the LS35T with LS100T and LS100F. It is not a serious comparison because I only have limited experience of LS100T and LS100F. At the moment, I am not able to produce any photos because I am too green in astrophotography. Getting the sun in focus in daytime is another challenge. Anyway, the image produced by LS35T is bright. Although the 35mm aperture is small, the solar disc is bright and uniform. I was told by a Solarmax user that Lunt’s image is very uniform and no observable ghost image is found. Don’t expect you can see the filaments at once unless you are using larger aperture or double-stack systems. You need to stare at the solar disc and inspect it carefully. However, once you get use to it, it is obvious! The details of solar disc can be improved by fine tuning the Etalon. This is what I have done today. I will try my best to take some photos soon!
As it is a low end product, it cannot be compared with my friend's LS100THaDS. However, I am sure you will not regret to buy one! It is affordable and handy. But the bad news is that the local dealer only got four special Carl Zeiss version LS35T. He will ship one to China and keep one for himself. The other two were bought by another stargazer and me yesterday. So all the scopes gone!