My First Try at Photographing the International Space Station

The idea of being able to take a photograph of the International Space Station is enchanting. Here’s one of humanities’ greatest achievements, passing by very frequently and yet so far out of reach to those of us on the ground.

Taking photos of the ISS is perfectly possible from the ground, but it requires some preparation. First, you have to know how to find it. There are several smartphone apps and on-line sites that allow you to predict when and where the ISS will be visible from your location. I use ISS Spotter on an iPhone, which I find very handy.

Once you know where it is going to be you have to think about how to capture it. The ISS typically crosses a section of the sky at a rate of between 1 and 3 degrees per second. This doesn’t sound too fast, but when you realize that it’s about 100x faster than computerized telescope mounts move you get some idea of the challenge. Even a large consumer telescope on a computer mount just can’t keep up.

It IS possible to follow the ISS and other satellites using computerized telescope mounts, but they’re not off-the-shelf gear. An absolute master at this kind of photography is Thierry Legault, an engineer based in Paris, France. Thierry’s systems include modified mounts that can turn at the phenomenal speeds needed to track a satellite. Take a look at his images and his methods at: http://www.astrophoto.fr/

My equipment isn’t up to that sort of approach, but you don’t need to that way. Instead, I’ve tried mounting my 125mm Meade Terabeam Maksutov-Cassegrain telescope on a photographic tripod. This arrangement (see the photo) is easily carried in one hand. It depends on being able to use the finding device (in this case a Rigel Systems QuikFinder reflex sighting device) to follow the target. Using this simple set-up it’s possible to follow the target and take numerous photos or shoot video, and them examine the resulting images later for any that worked out. This is an approach related to “Lucky Imaging” that is commonly used in more sane corners of amateur astronomy.

ISS Hunting Rig

My ISS-hunting rig. I’ve mounted a Nikon dSLR camera at prime focus on a 125 mm Meade Terabeam Maksutov-Cassegrain telescope. This is then set up on a heavy-duty photography tripod. This telescope is equipped with a red-circle Rigel Systems QuikFinder (http://rigel.datacorner.com/rigelsys/quikfinder.html )

Of course I am using the term “sane” in a tongue-in-cheek manner here and mean no disrespect to those suffering from mental disabilities. It’s just the term that came to mind as I snapped away at the space station like a field gunner trying to shoot down an Sopwith Camel during the First World War.

There are a couple of very basic set-up steps that deserve every bit of attention before the pass begins.

First, ensure that your finding device is well-aligned with the telescope itself. You will not be looking through the telescope or camera to take these photos.  You’re flying blind, relying on the finder to set things up. You are adjusting the aim of the telescope throughout the entire pass. The steadier the better, but you still must keep moving to keep the ISS as close to the telescope’s centre of view as possible.

Second, focus is crucial. The ISS is tiny from earth – just a few arc-seconds across. Before the pass focus the telescope as carefully as possible on a star. This is a little easier said than done without having the telescope on a capable telescope mount. I used the moon and also very distant lights to try to focus the spot mac.

Jet 29 July 2017

While I was setting up to shoot the ISS I snapped this distant jet high over Lake Huron. Possibly 30 km or more away.

 

Keep in mind too that if you are using a dSLR your camera is going to shake like made when the mirror and shutter are activated. Every bit of extra motion is a problem. I think an ideal imager for this application would be a mirrorless camera with a full-frame sensor, but I’m not quipped with one of these.

For my first try I used a Nikon D800 camera on video mode. I started running the video before the ISS came into view, and simply kept the telescope pointed at it, moving as smoothly as I could, throughout the pass. Afterward I then exported all of the images using IrfanView, and threw out everything that wasn’t a recognizable image. In other words, nearly all of the resulting frames.

moon from the beach 29 July 2017

Just for the focus. I used the moon as a target to focus the telescope prior to the pass of the ISS on 29 July 2017 visible from the mouth of the Pine River. 

Despite all of the make-shift arrangements, at the end of the day I did capture something with structure. Here are a couple of frames:

ISS 29 Aug 2017 from Pine River

I’ve seen some authors recommending this approach with telescopes on Dobson mounts. This makes a lot of sense too, as these mounts are intended to allow you to point the telescope by hand with ease. I will try to take more images of the ISS as time and opportunity permits. It’s a fascinating subject!

Copyright 2017 David Galbraith

 

 

Get ready for AstroCATS 2014: Canada’s Astronomy Trade Show!

The Royal Astronomical Society of Canada – Hamilton Centre is presenting the second annual Canadian Astronomy Trade Show, AstroCATS, on 3-4 May, 2014!

The web site for this exciting event is: http://www.astrocats.ca/

The big show will open at 10 AM on Saturday 3 May, and close at 6. On Sunday it opens again at 10 and closes at 4. AstroCATS 2014 will be held in the David Braley Athletic & Recreation Centre at Mohawk College, 135 Fennell Ave. West, Hamilton L9C 1E9.

Visit the web site to find lists of vendors, special speakers, and all of the exciting highlights planned for the show in May. Hope to see you there!

Supernova SN 2014J in Ursa Minor

On 22 January 2014, S. J. Fossey discovered a supernova, designated SN 2014J, in the Cigar Galaxy, Messier 82. It’s turned out to be the brightest of its type visible in the Northern Hemisphere in living memory. M82 is in Ursa Major, nice and high in the night sky for those of is in the Great White North! It is not visible to the unaided eye, clocking in at about Magnitude 11.5, but that’s well within the capability of a home telescope on a dark night to spot, and especially with a short exposure with a digital camera on a 4″ or 5″ telescope.

I wanted to see if I could take an image of the supernova from my livingroom couch, and so used a simple web form to request an image be taken by the MicroObservatory Network in Arizona. Anyone can use this free educational system, using the on-line forms at: http://mo-www.harvard.edu/MicroObservatory/

The simple icon-driven menu asks for subject, field of view, and exposure time. All the rest is automated. I sent the request in on 25 January, and on the afternoon of the 26th I received an email message from the system indicating that an image was ready. Here’s the result. The supernova is the bright star to the right of centre of the irregular galaxy.

SN2014J in M82 20140126

Supernova SN 2014J is visible between the hair lines along the right side of this image. The cloudy mass is the Cigar Galaxy, Messire 82, in Ursa Major. This is an uncropped image as provided by the MicroObservatory Network. See the text for description. Click on the image to see it scales a little better.

The fact that the galaxy is so far over to the right side of the frame is the result of errors in the on-line system. It amounts to perhaps a 10th of a degree or less, but that’s enough to put things way off of centre. Given that this is a free, public-access system, you can’t complain too much! I wish I had had access to a system like this as a child – this and other robotic telescope systems now available to the public would make for amazing science fair projects! I have an article in a forthcoming issue of the Hamilton Amateur Astronomer’s newsletter The Event Horizon on robotic observatories, which I find a very nice way of avoiding the cold outside conditions of astronomy in Canada in the winter. Yes, I’m a wimp, but I’m a warm wimp.

Copyright © 2014 David Allan Galbraith

Public Access Astronomy: the MicroObservatory Robotic Telescope Network

The MicroObservatory Robotic Telescope Network, operated by the Harvard-Smithsonian Center for Astrophysics OWN “Observing With NASA” program allows free, public access use of 6″ reflecting telescopes located at the Whipple Observatory in Amado, Arizona. If you are a teacher interested in introducing astronomy in a hands-on way, a parent wanting to show kids that they can also take astrophotos, or just interested in experiencing with Internet-based remote observatories, making use of this free system is well worth a try. This system has been in use for over a decade and is a lot of fun.

The network can be reached at: http://mo-www.cfa.harvard.edu/MicroObservatory/

Guest users can select from a pre-set menu of target objects. In December 2013 I tried shooting images of several deep space targets over successive nights. The 6″ reflectors (identified as Ed, Ben and Cecilia, Donald) are programmed with a simple web form. Once images are captured, users are sent an email message with instructions on how to retrieve the files. The files are all returned as 650 x 500 FITS files. The network also supplies MicroObservatoryImage, a free program based on Java that processes FITS files, including stacking RGB images, optimised for the small images the system produces.

The web site is well worth exploring, as there are several resources there of interest to teachers, especially.

Here are three images I captured with this system in December 2013. The images I was able to capture did suffer from several artifacts, including diffraction spikes, and “blooms” produced by very bright stars.

The Cab Nebula (Messier 1) imaged with one of the educational telescopes of the  MicroObservatory Robotic Telescope Network.

The Cab Nebula (Messier 1) imaged with one of the educational telescopes of the
MicroObservatory Robotic Telescope Network. Three images were taken, one each through a red, green, and blue filter, and then they were combined with the MicroObseervatoryImage software supplied by the network.

NGC5457, Messier 101, imaged with the MicroObservatory Robotic Telescope Network.

NGC5457, Messier 101, imaged with the MicroObservatory Robotic Telescope Network. This was taken as a single 60 second exposure, taken at 5:37 AM local time on 31 December 2013. The area imaged is approximately one degree of arc across.

orion1 retouched1

The Great Nebula in Orion (M42) imaged in three colours using the MicroObservatory system. The colour image was assembled as described above for the image of the Crab Nebula. This image is slightly retouched to reduce artefacts created by both diffraction effects (spikes) and also “blooms” or smears produced by very bright stars.

Copyright © 2014 David Allan Galbraith

Free Solar Observing Today at Royal Botanical Gardens

We’re going to hold Royal Botanical Gardens’ third “Solar Thursday” today (29 August 2013) from 12 noon to 1 PM, on the lawn area in front of the main visitor entrance to RBG Centre. Everyone’s welcome to join us for a view of the sun through special, safe telescopes.

If you have a solar telescope you are very welcome to join us in presenting the amazing spectacle of the sun to the public. We like to be “open for business” at 12 noon, so coming a little earlier to set up would be helpful. We have electrical power available if your telescope needs it. We start packing things up around 1 PM. RBG is located at 680 Plains Road West, Burlington, Ontario.

We will be looking through specially-equipped telescopes that filter the bright light from the sun. These filters make it safe to observe the sun’s surface. Remember:

No one should ever look directly at the sun without special, appropriate equipment. Permanent eye damage or blindness may result from inappropriate attempts to see the Sun, or the use of incorrect equipment. We will be using telescopes designed specifically for solar observation, or those equipped with filters specifically made for this purpose.

Once you’re familiar with the equipment and have things in focus, you will be able to take in the sights in just a few minutes! Some nice sunspots are visible today.

Katie

Visitors to Royal Botanical Gardens, 680 Plains Road West, Burlington, Ontario enjoying views of the sun live during RBG’s second “Solar Thursday” event, 15 August 2013.

Copyright © 2013 David Allan Galbraith

Enchanted by the Sun

This summer I’ve been delving into solar studies. Perhaps it’s like the proverbial goldfish not noticing the water that surrounds him, but I really hadn’t paid much attention to our nearest star. Last year I did start to take my own look at the sun, using solar filters on an old 80mm f15 refractor, and that was pretty interesting. Somehow the solar bug has really bit me this year.

I’ve added some equipment to Pine River Observatory this year, and that’s helped. In addition to my Meade ETX 125 Terabeam telescope, which I now have equipped with both a Kendrick Astro Mylar solar filter and a Baader Planetarium continuum filter, I picked up a Coronado 60 mm Solar Max II BF15 Hydrogen alpha telescope a couple of months ago. The upshot of all of that is that I can take a look – and am starting to photograph – the sun at two quite different wavelengths, corresponding to different structures on its surface.

There’s an interesting feedback loop here. As I’ve been able to see the sun for myself, and consider how to take photos, and even explain what can be seen through a telescope to others taking a look, I’ve found that my curiosity has risen. I’ve been reading more, seeking out a deeper understanding of what I’m seeing. That in turn has made my observations a little better, I think, and certainly has meant I’m doing a better job of interpreting for others.

It’s also been exciting to see that there’s a lot happening in terms of science and solar observation right now. Consider these three news items from the past month alone:

  • A new ground-based solar telescope (the New Solar Telescope or NST) at the Big Bear Observatory in California has just started to produce incredible images of the photosphere and sunspots – with a resolving power that approaches 30 miles on the sun’s surface (http://www.bbso.njit.edu/)
  • A new solar observatory satellite, Interface Region Imaging Spectrograph (IRIS) achieved “first light” in July, and is already transmitting wonderful images back to earth (http://iris.lmsal.com/)
  • NASA has updated information available on the progress of the present solar maximum. This event, every 11 years or so, is marked by a peak in sunspot numbers, and represents a reversal in the orientation of the sun’s magnetic field. The present solar maximum was anticipated for 20111 but it’s a little late. The magnetic flip is anticipated between now and November.

These are just examples of the activity around solar observations in the past little while. The more I’ve read, too, the more I want to find out. The sun is quite addictive! More postings to come.

sun aug 2013

The sun’s “surface,” or photosphere, photographed from Burlington, Ontario’s LaSalle Park Marina on the morning of Monday 5 August 2013. This image was captured using a Meade ETX 125 TB telescope equipped with a Kendrick Astro Mylar solar filter and a Baader Planetarium continuum filter. These filters produce a green image that highlights contrast around sunspots and solar granulations. The image is a mosaic of two shots taken with a Nikon D5100 at prime focus, as the image produced by the telescope is larger than the D5100’s APS-C-sized sensor. The image was processed with Paint.net, a free image processing program. Although we might think of the sun as a big ball of hot gas it’s structure is much more remarkable than that. At its core the density is enormous – a liter of the gasses would weight 150 kg. At the surface we can see, as in this photo, the density is less than 1% of that of our own atmosphere at ground level.

 

Copyright © 2013 David Allan Galbraith

 

Solar Thursdays at Royal Botanical Gardens Start This Week!

Would you like to take a look at the sun, just for fun? Are you going to visit Royal Botanical Gardens (http://www.rbg.ca) on Thursdays this summer, or just in the neighborhood? Introducing “Solar Thursdays” – a weekly one-hour chance for visitors to  directly see features on our nearest star, the Sun, at RBG.
Solar Thursdays are a chance to see the sun through specially-equipped telescopes. We’ll be set up from 12 noon – 1 PM in July and into August, weather permitting. Some clouds will be OK, but heavy clouds will mean cancellation. We’ll be on the lawn in front of the main entrance to RBG Centre. There’s also a chance that other local astronomers might join in and bring along their own solar-equipped ‘scopes, too! Our address is 680 Plains Road West, Burlington, Ontario. Parking is free. We hope you’ll visit RBG after your look at the sun.
On Thursday we’ll likely see sunspots and solar prominences.  We’ll also have a solar weather update on hand. This offering is free of charge, and is being presented by RBG staff on their lunch hour.
scope

Visit us on the front lawn of Royal Botanical Gardens Centre, 680 Plains Road West, Burlington, Ontario, for Solar Thursdays! Here a visitor takes a turn looking at the sun with a Coronado 60 mm Solar Max II BF15 H-alpha telescope.

We will be looking through specially-equipped telescopes that filter the bright light from the sun. These filters make it safe to observe the sun’s surface. Remember:

No one should ever look directly at the sun without special, appropriate equipment. Permanent eye damage or blindness may result from inappropriate attempts to see the Sun, or the use of incorrect equipment. We will be using telescopes designed specifically for solar observation, or those equipped with filters specifically made for this purpose.

Once you’re familiar with the equipment and have things in focus, you will be able to take in the sights in just a few minutes.

sun

The sun photographed on 23 July 2013 from the front lawn of Royal Botanical Gardens, by using eyepiece projection and a Sony pocket camera. Several prominences are visible in this view through a Coronado 60 mm Solar Max II BF15 telescope.

We hope to see you there!

Copyright © 2013 David Allan Galbraith

Remote Astrophotography: Taking It On-Line

Since the time of Galileo four hundred years ago, astronomers have used telescopes to see the sky. Since 1839 people have tried to take photographs through telescopes. Now, anyone with an internet connection – and a credit card – can take their own photos through professional-grade telescopes.

It’s called remote astrophotography, and I’ve been getting interested in giving this a try. I haven’t done so yet myself, mostly because I don’t have a good home internet connection yet. This seems to be a good reason to get one, and I hope to report back later this winter with some results of my own. In the mean time, I thought I’d report here on this intriguing idea.

A variety of companies are now operating telescopes in places with good conditions for astronomy and offering them up on-line, with equipment and software that allows paying users to control them remotely. What’s more, these set-ups are designed for astrophotography. The telescopes are equipped with specialized CCD cameras designed for astrophotography. The lure of remote astrophotography is not just being able to use these telescopes to see on-line. They can take amazing photographs and deliver them to your home computer.

Costs for this service range from an annual subscription of around $150 at SLOOH Space Camera (http://www.slooh.com/slooh-home.php) to a fee per use running up to $100/hr at LightBuckets (http://www.lightbuckets.com/index.php), MyTelescope.com (http://www.mytelescope.com/index.html), or iTelescope (http://www.itelescope.net/). There are likely others out there, too.

A NASA image of M51 and NGC5194.

A NASA image of M51 and NGC5194. M51, a magnificent spiral also called the Whirlpool Galaxy, is on the left. It is interacting with M51b or NGC5194, the dwarf galaxy on the right.  They are located south of Canis Major, in the constellation Canes Venatici. These galaxies are well within the scope of amateurs to image. An astrophotograph of these galaxies taken by amateur astronomer Martin Pugh won the 2012 Astronomy Photography of the Year Award. (See this link for the contest: http://www.universetoday.com/97469/the-universe-shines-for-astronomy-photographer-of-the-year-winners/)

In some cases, users have to download specialized software like CCDCommander (http://ccdcommander.com/) that gives users complete control from their desktops, and even allows pre-programming of the functions of the telescope.

There are several reasons why remote astrophotography is very attractive. One of the most important from an image quality perspective is that the telescopes involved can be set up in remote locations with excellent dark skies and clear weather, such as in Arizona or even Chile. Users don’t have to make a trek to those locations to take advantage of the conditions. Another big consideration is cost. The camera, telescope, mount, and observatory systems set up by these companies can easily be worth $15,000 to $20,000 each or more. Renting some time on these set-ups is a lot more attractive than having to buy hundreds of kilos of very pricey kit. Furthermore, the remote telescopes are set up and maintained by experts. Even if money was no object, there’s a very long technical learning curve to really be proficient with big ‘scopes – years in many cases. Renting sidesteps all of that and can give you excellent results in hours, not years.

Remote astrophotography is not limited to by-the-hour rentals, either. Some people who are able to purchase their own telescopes chose to have them installed at remote locations for the same reasons as these rentals are located there: better sky conditions than at home. Clearly an expensive proposition, these private observatories have the potential to allow for many hundreds of hours of observing and photography that would be impossible under any circumstances other than moving to a dark sky location. Some people are able to take up that option, too.

Where To Go From Here?

While I’ve been interested in astronomy for over forty years, it’s only in the past year and a bit that I’ve returned to that interest in any sort of “serious” way as an amateur. I’ve been poking around at various telescope shops, getting to know some other amateurs in my area, and taking a lot of nightscape photos. I’ve even started taking a few photos of the moon and Jupiter with the equipment I have. Now what?

The sky is a big place. A simple calculation gives you an idea of just HOW big it is – and I’m not talking about how deep it is in time/distance. Consider first the moon. The moon is pretty big. It has a surface area about the same size as the continent of Africa, although we only can see about half of it from Earth of course. With the existing small telescopes I have I can make out features perhaps 5 km across if the lighting is right. The surface of the moon is about 38,000,000 km^2 (km^2 means “kilometer-squared or square kilometers) so if I can see half of it (in total) that’s about 19,000,000 km^2. A crater 5 km across has a surface area of about 19.6 km^s – so that little crater is just about 1/100,000 of the visible face of the moon. The whole visible surface is a lot of territory (or lunatory) to consider. Of course, it might be better to consider the visible disk of the moon, not the near hemisphere for a comparison like this. A disk with the radius of the moon would have a surface area of about 9,500,000 km^2, so the ratio would be about 50,000 craters-worth of area to explore. Still a lot! A purist would try this with angles but the answer would be the same as the disk area sketch.

The thing is, the moon is actually SMALL compared to the visible celestial sphere. Our eyes are drawn to the moon at night, but the reality is that it’s only about a half a degree across. The whole celestial sphere, encompassing 360°, has an area of approximately 41,253 °^2 (according to a Wikipedia entry on the angular area of the celestial sphere). The moon’s disk as an angle is about 0.2 °^2 – so it would take 206,000 moons to fill up the visible area of the sky! (The sun as virtually the same angular diameter as the moon – that’s why we can have such stunning total solar eclipses – so the same thing holds. The sun, so dominant in our sky, covers only about 1/200,000 of the visible celestial sphere. From the surface of the earth only about half of the celestial sphere is visible as the sky, and the sun is about 1/100,000 of it).

The moon photographed from Hamilton, Ontario, on 2012 12 19 2125 EDT with an 80mm refractor and Nikon D5100 at prime focus.

The moon photographed from Hamilton, Ontario, on 2012 12 19 2125 EDT with an 80mm refractor and Nikon D5100 at prime focus. Relatively simple equipment can take nice photos – but if you are interested in going further, what’s the next step?

The sky, then, has room for 200,000 moon-faces, and my little telescopes can show me details 1/100,000 of the moon’s surface. It’s overwhelming – and full of rich detail. From massive galaxies to wispy nebulas and sparkling star clusters, space beyond our little solar system is one of the richest treasures in nature. How luck we are that we can actually see it! If our solar system was within a more complex part of space we might not have as good a view as we do. Then again, it’s a fair bet that the more “interesting” places in space are far more risky too. Our fair wee planet has had less than five billion years of life so far, and only a few major boo-boos (like the asteroid impact that killed the dinosaurs – Ooops!).

So, back to the point of this ramble. As a (re)budding amateur astronomer, where do I start? I’m faced with this question because I’m looking seriously at upgrading some of my equipment, and different telescopes do different things. Do I make use of my existing optics and improve my ability to point and shoot, with a better mount and camera? Do I invest in a better optical tube (the actual “telescope” part)?

To some degree a telescope is a telescope. There are some basic characteristics everyone needs to consider when they are thinking about this kind of thing. One of the most important is portability. Like a lot of people, I live in a small apartment; I don’t have a garage or basement for storing large pieces of kit, and I don’t have my own space for a shed or observatory. So, compact and rugged is good. I’m also watching my budget (gulp). And, of paramount importance to me, I want to embark on something of a path in learning astronomy, not just grabbing at big telescopes because they’re cool! (and they are cool, and I’m a telescope geek).

I’m thinking I’ll start in the neighborhood this year, seeing what I can see – and photographing what I can photograph close to home in the “planetary” range – the sun, moon, and planets. This narrows things a bit, and is also a good choice for an urban dweller. Despite light pollution in cities, our own solar system is still quite observable from our sidewalks and parks because the objects are so bright. The existing ‘scopes I have – an old 80 mm refractor and a 130 mm “starter” Newtonian reflector – will do for now. What I need to do is to consider in the short term is what’s under the telescope and what’s attached to it.

Telescope mounts are important and perhaps underappreciated parts of the whole “system.” A heavy, capable mount makes viewing anything much easier. A lightweight mount only has the advantage of light weight. Small mounts shake. If you adjust a small telescope on a light mount it can take five or ten seconds or more for the resulting vibration in the camera to dampen out. So, I’ll be paying attention to mounts.

Cameras are at the other end of the process. There are some things I can do with my dSLR cameras, but the best images today are actually being taken with cameras that are much simpler than a dSLR but are designed to be used with a telescope – and a computer. Derived essentially from webcams, most cameras that work brilliantly for planetary photography by amateurs have small-seeming sensors – often less than a megapixel. They are also specialized in two other ways. They often have a built-in cooler, to help control internal camera noise – and they are often monochrome. Yes, black and white. You can do a lot in black and white, and you can get colour images by taking a series of monochrome images through coloured filters. The image files (often actually captured as short video segments in AVI format) are then processed with some ingenious computer software to create stunning, sharp images. So, I’ll also be looking at a small, specialized camera designed for planetary imaging. By starting with a camera and a sturdier mount, I can get going and will consider upgrading the optics a little later.

I’m also sure that there will be lots of opportunities to peek out past our solar system in the coming year. I’m going to be making visits to observatories, star parties, and other events to soak in more of deep space – and of course to be able to make reports here at Pine River Observatory! And I’ll be spending time under the night sky doing wide-field photography and just wandering around the stallar back-yard with binoculars and a good star guide. There are many lifetimes of space out there to enjoy.

© 2012, David Allan Galbraith

First Light Through an Old Bargain

When a telescope is first put to use it’s traditional to call the first observations made through it, or the first images taken with it, as “first light.” It’s perhaps a bit of a cheat to consider photos of the photosphere of the sun that I took on 1 January 2013 as “first light” through one of my telescopes, but as I’ve been making repairs on it since I picked it up in December I felt a certain sense of occasion on New Years Day when I was able to set it up “for real” for the first time.

Set-up for balcony solar photographs.

Set-up for balcony solar photographs. My balcony faces WSW – good for some afternoon sungazing.

I have an affection for old optical equipment. As evidence I can readily point to my Hasselblad and large format film cameras, still used on occasion. For some months I had noticed an older refracting telescope – complete with a mount and wooden tripod in a big wooden box – on the floor of a local telescope shop. In early December it was on sale for $100, and suddenly found a new home at Pine River Observatory. Well, in my living room. Same thing, really.

So, I started fiddling about with the old telescope a few weeks ago, and quickly discovered why it was such a bargain. In addition to several bends where bends shouldn’t be in the fine adjustment gears on the mount, and a couple of other minor issues, the biggest problem with the telescope was that the collar that holds the eyepiece or other fittings in the focuser was in fact pretty badly damaged. It had been knocked around (I suspect it had been actually pulled or knocked out of the telescope by force at one point) and was being held into the telescope with aluminum duct tape! With a bit of perseverance, cleaning out, and re-bending, the collar is now looking much better, is equipped with new thumb screws, and is firmly epoxied into place – permanently.

The specifics are that it’s an 80 mm achromatic refractor, f/15 (or, put another way, it has a focal length of 1200 mm), and it’s labelled with the brand name “Polaroscope.” So far I haven’t been able to find out too much about this brand. It was likely made in Japan, possibly by a company called Eikow or Towa, and similar ‘scopes may have been sold under various trademarks. It may be as old as 1960.

Even though the repairs have been made, it’s still January in Ontario, and this winter so far has been very cloudy. However, on New Years Day there was a great deal of very welcome sun, and I was able to set up the old telescope in a fairly heavy-duty mount for a little solar imaging (Shortly after getting the telescope I did play around a little with taking photos of the moon with it, but this was with the camera held to the tube with duct tape). Equipped with a mylar solar filter over the objective and a Nikon D5100 dSLR at prime focus, I was pretty pleased with the $100 bargain ‘scope.

The results were worth waiting for, as several large sunspots came into view this afternoon. I have several more subjects planned for this telescope, including Jupiter and the Galilean moons, when the weather will be accommodating at the right time.

The sun's photosphere photographed 1t 1400 EDT, 1 January 2013 from Hamilton, Ontario.

The sun’s photosphere photographed at 1400 EDT, 1 January 2013 from Hamilton, Ontario.

Note:

As I’m now back to work five days a week, following a very nice holiday for Christmas and the New Year celebrations, I don’t think it will be very realistic for me to be posting daily blog entries. In January I am hoping to average one or two postings a week. Just so everyone knows.