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:

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 ( )

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



The Great Eclipse of 2017 is Just Around the Corner!

One of the grandest spectacles in astronomy is a total solar eclipse. On 21 August 2017 there’s going to be a stunning event, as the shadow of the moon sweeps over the continental USA from west to east. I’ve recently seen suggestions that this might be the most photographed event in history (to date) when it happens. I’ll be in there too, dear readers, making plans for many months about the chance to photograph this spectacle. The next one that will be visible over the North American continent will take place on 8 April 2014.

eclipse book cover

Alan Dyer’s ebook on the 21 August 2017 eclipse is highly recommended. You can get your own copy here: 

A total solar eclipse is, of course, a transient event in which the moon passes directly in front of the sun from the perspective of some location on earth. Because of the coincidence of the similar relative sizes of the sun and moon as viewed from earth, the moon can just about block out the central disk of the sun. A total eclipse, as the name suggests, brings the sun, moon, and earth into alignment. A partial solar eclipse consists of part of the sun’s disk being blocked.

The 21 August event will be a partial solar eclipse in southern Ontario. For observers in a band a few kilometers across running from the west to the east coast of the USA it will be total.

Preparation for watching an eclipse is a must. Not only should anyone wanting to take this in be prepared from the perspective of observation itself, safety is a crucial concern. Although the disk of the sun is blocked by the moon during these events, the sun is still producing a great deal of UV radiation from the corona, the tenuous outer layers of the sun’s atmosphere. Always wear appropriate eye protection during these events, or observe indirectly, such as with a pinhole camera you make make from a simple cardboard box. For safe eclipse observing ideas, see:

In preparation I’ve been sorting out gear, trying things, and reading up. I highly recommend Alan Dyer’s comprehensive e-book on photography of this specific event. I’m planning on using several cameras to capture different aspects of the eclipse. At least one will be running interval photos that can later be stacked to produce this sort of effect:

Solar Practice 2017

A three hour sequence of solar photographs taken at the home base of the Pine River Observatory, at Lurgan Beach, Ontario on 29 August 2017. A Nikon D7000 digital camera was set up to take photos every 30 seconds, and was equipped with a Mylar solar filter and a wide-angle lens. Every sixth resulting photo was then stacked with StarStaX. The last photo, with the sun in the trees, was taken without the solar filter. It forms a background for the otherwise rather dull individual photos of the sun.

Another camera will be set up with a long telephoto lens and a Mylar solar filter. I am not quite sure yet whether or not I will set up any camera on a telescope mount to track the sun – as this trip requires some travel, lugging such things around is always complicated.

If you are able to take images of the eclipse, consider submitting them to SkyNews Magazine, Canada’s own astronomy magazine. They’re holding a contest for the best solar eclipse photo: 

Safe observing!

Copyright 2017 David Galbraith


A New Year, a New Night-Time Photography Class!

I’m happy to report that Royal Botanical Gardens has asked me to lead another Night-Time Photography class! If we get sufficient response, we’ll start at 7 PM on the evening of Thursday 26 January 2017, at RBG’s Nature Interpretive Centre. The class will run for a total of four sessions, weekly.

The class will be a hands-on opportunity to take photos at night, with an emphasis on capturing beautiful images of the sky. We’ll cover equipment, celestial objects, post-photography processing, and more. This isn’t an astronomy class per se, but we will talk a bit about astronomy. By the end of the course I am hoping everyone will feel confident going out at night with their cameras and experimenting with capturing beautiful images.

We’ll try to end each two hour classroom experience with a quick dash outside to see be seen. Guidance will also be given on photo opportunities taking place between classes.

RBG’s public program calendar is available on-line at:

You can register on-line for any of the RBG programs at:

To find the Night-Time Photography course, just click 26 January 2017 on the calendar on the web site. Registration is limited to 20.

If you are planning to take the course, please contact me ahead of time for more information. It’s recommended that participants bring their digital cameras and tripods to the first class. Digital cameras should be able to be operated completely manually. A wide-angle lens is best for this sort of photography. Tripods should be very sturdy. I can make recommendations if anyone has any questions.



Night-Time Photography Cancelled

Unfortunately there haven’t been enough takers this year for the Night-Time Photography short course that Royal Botanical Gardens has asked me to present to go ahead. The course has been cancelled.

A stacked star-trails image captured

A stacked star-trails image captured along the shores of Lake Huron.

When I do offer this three night course, the program is all about learning to take photographs of the night sky with a digital camera. Ideal equipment includes any digital SLR and wide-angle lens, tripod, and remote or cable release. Other digital cameras may be usable, but it will depend on whether you can take complete manual control over the camera. Functions like ISO rating, shutter speed, aperture, colour temperature and focus should all be able to be controlled manually to get the most of out night-time photography.

The Burlington Waterfront in December 2013, photographed early on e morning.

The Burlington Waterfront in December 2013, photographed early one morning.

We talk a little about telescopes, and there’s a chance to try out some telescope photography, too. However, this introductory program is intended to help you take beautiful images of landscapes and the sky at night, especially those with interesting skies and night-time city-scapes. Subjects covered include basic camera operations, composition, planning for photography at night, controlling long exposures, and computer software for various functions such as stacking star trail images.

The Burlington Waterfront and Pier before dawn.

The Burlington Waterfront and Pier before dawn.

Our first evening together is usually in a classroom. The subsequent meetings are outdoors. Locations are chosen depending on the weather and class interest. Excellent opportunities for interesting night-time photos are often to be had along the edges of Hamilton Harbour (such as at La Salle Park Marina) or along the Burlington waterfront.

Consellation Oroion rising over a surbab street in Burlington, Ontario, on the evening of 2013 March 26. Betelgeuse, the brightest star in Orion, is in the middle of the frame and about 1/8th of the way down from the top.

Constellation Orion rising over a suburban street in Burlington, Ontario, on the evening of 23 March 2013. Betelgeuse, the brightest star in Orion, is in the middle of the frame and about 1/8th of the way down from the top.


The moon photographed early on the morning of 29 August 2013.

The moon photographed early on the morning of 29 August 2013. Yes, this one was taken with a telescope.

I hope the program will be invited once again. I’ll post updates if that happens.

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:

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!

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:

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

Try Cell Phone Afocal Photography – Especially for Sidewalk Astronomy

There are a great many different ways to take a photograph of astronomical objects. If you are looking through a telescope at a bright object like the moon, it’s possible to take satisfying photos “on the fly” without even having to attach a camera to anything. It’s called afocal photography. It’s very well suited to public or “sidewalk” astronomy events where nearly everyone visiting will have their own camera of some sort.

Afocal photography is the process of shooting a photo with a camera simply by lining the camera up to the telescope (or microscope, or spotting scope, where this technique is sometimes called digiscoping) eyepiece. It does not require attaching the camera to the eyepiece (although there are ways of attaching the camera that makes things much easier. This post is about just trying it hand-held). There’s a nice introduction to afocal photography on Wikipedia (

I thought a demonstration might be fun, using a very ubiquitous and simple digital camera, that built into an iPhone 3GS. If you want to try this with any camera more advanced than that on an iPhone 3Gs, please make sure that you turn the flash off!

On the evening of Saturday 14 September 2013 the Hamilton Amateur Astronomers (  presented a public astronomy evening in the parking area of a visitor centre in Grimsby, Ontario. I went along with my little Meade 125mm Maksutov-Cassegrain telescope, an iPhone 3Gs, and also a Nikon D5100 body. I thought it might be nice to compare two photo methods: afocal (putting the iPhone over the telescope eyepiece) and prime focus (replacing the eyepiece with the camera all together) photography of the moon.

DAG_2722 800px

A public observing night put on by the Hamilton Amateur Astronomers on the evening of 14 September 2013 in Grimsby, Ontario. These events are terrific fun and a chance to see many different types of home telescopes in operation.

After setting up my telescope I was happy to have lots of members of the public come by and take a look at the moon through a wide-angle eyepiece. The Meade telescope has a focal length of 1,900 mm. With a wide-angle eyepiece of 28 mm focal length, the combination had a magnification of 67x (magnification, or “power,” in telescopes is calculated by the ration of the focal length of the tube divided by the focal length of the eyepiece).


My Meade Terabeam (TB) 125mm telescope set up for photography of the moon at the Grimsby public astronomy event. This compact little telescope is very versatile.

In between looks through the telescope, I held the iPhone’s camera over the eyepiece as “flat” as possible – in line with the long axis of the eyepiece, pretty much up against the rubber eye cup. Once I could see the bright light of the moon showing up on the iPhone screen, I moved the phone carefully around a few mm at a time until more and more of the moon showed up.

iPhone 1

A first afocal exposure of the moon taken with the camera built into an iPhone 3Gs. At least one crater is visible – a good, if humble, start!

It takes a little time and patience to line up the camera over the eyepiece, but in a few minutes I got the hang of it and started taking photos.


Getting closer! Nearly the whole moon is visible in this afocal shot, one of many taken to ensure a good one is captured.

After about a dozen images recorded, I captured one that I thought was pretty good.


A pretty satisfying image of the moon, one of about a dozen tried. Hand-held afocal photography is very much a trial-and-error process.

Some shops actually carry devices to hold cameras of various kinds (including cellphones) up against telescope or spotting scope eyepieces. These would be really helpful, especially if you wanted to take video or longer exposures. As it was, in this case I used the default camera app on the iPhone, allowing the camera and phone software to control exposure and focus.


The afocal image above, rotated, and flipped left-for-right. I’ve also adjusted the brightness, contrast, and sharpness very slightly. This compares very well to the image of the moon taken with a Nikon D5100 dSLR body at prime focus, below.

After taking a photo I was satisfied with, I put the iPhone away and set up the Nikon dSLR on the telescope, at prime focus. This is the place where the telescope makes its basic image without an eyepiece. With this 1,900 mm telescope image of the waning gibbous moon, about two or three days past first quarter, just barely fit onto the APS-C sized sensor on the Nikon D5100. I had to rotate the camera to get it onto the sensor.

DSC_0120 cr1 1200px

A photo of the moon taken a few minutes after the afocal iPhone images, by placing a Nikon D5100 dSLR body onto the same telescope at prime focus (replacing the eyepiece with the camera).

The iPhone afocal image compares pretty well with that from the dSLR once both are reduced down to the same size of image. The dSLR image is more detailed than the iPhone photo taken on the 14th, in part because of the much bigger (16 megapixel) sensor on the Nikon, and in part because of the wide-angle eyepiece used. Put side by side, sections of the images at their original resolution give a good idea of difference in resolution.

side by side

The southern part of the moon imaged with iPhone afocal photography (left) and with a Nikon D5100 at prime focus (right). Both images were converted to black and white, and then a strip 400 pixels wide by 800 pixels high was cropped out of each. The two images here are presented in their original resolutions for comparison. the large round crater with two smaller ones along its edge, toward the bottom of both images, is Clavius. The smaller, circular crater to the north, with a prominent central peak, is Tycho.

Afocal photography is a “quick and dirty” method, but it’s also a lot of fun. One effect you might notice with this method is chromatic aberration, even if you are using a telescope that is an apo-chromat or a reflector that is not itself subject to this problem. It may show up, even on focused images, as colour ghost images or fringes.

As I noted at the beginning, this process is particularly well-suited for public astronomy nights. Nearly everyone (well, lots of people, anyway) has a cell phone or pocket camera with them these days.  If you are inviting the public to try looking through a telescope at something bright like the moon, ask them if they’d like to try to make their own souvenir of the event, too – their own photo of the moon, on their own camera. A few of our guests in Grimsby took away their own photos through my telescope, and they were pretty excited. I’m sure these were sent to a bunch of their fiends by SMS before too many more minutes had passed.

Copyright © 2013 David Allan Galbraith

Stitching A Lunar Panorama

Astrophotography today is becoming more and more about taking a series of individual images and assembling them into something else. This can be done in two sorts of ways. Very often, astophotographers will take repeated shots of the same area of the sky, and then use software to “stack” them, which has the effect of greatly reducing noise in the final image. As many of the objects in space are extremely faint, long, noise-free images are necessary to find them at all.

It’s also possible to make images of large areas of the sky by taking individual photos and joining them together, or stitching them. This can be a very effective way of using small cameras to produce large, high-resolution images. Despite the trend in some circles of seeking ever-bigger sensors dSLR cameras, stitching means that small cameras – like a web cam – can be used to great effect.

On the night of 16 August 2013 I was doing some observing and photograph form my west-facing balcony in Hamilton, and decided to try to make a large portrait of the moon using a small camera. I tried imaging the moon with several different cameras that night. My telescope was my Meade 125 Terabeam Maksutov Cassegrain catadioptric telescope mounted on an EQ6Pro mount with Synscan. Because of my balcony’s situation, it’s impossible to do an actual polar alignment; I can’t see Polaris. I can get to within a degree or so, which is good enough for taking a few images of bright objects like the moon.

The moon was lovely that night. After a few minutes of general moongazing, I mounted a Nikon D800 body on the telescope at prime focus, and was able to capture images of the whole moon’s face in one shot.


A photo of the moon taken on the evening of 16 August 2013 from an apartment balcony in Hamilton, Ontario, using a Nikon D800 camera on a 125mm Maksutov Cassegrain catadipotric telescope.

I then changed the camera, replacing the big dSLR with a little imager sold specifically for lunar and planetary imaging, a Celestron NexImage 5. This little camera looks like a miniature hockey puck about 2″ across. Inside is a 5 megapixel colour image sensor, which attaches to a computer via a USB cable. In contrast to the very expensive Nikon camera, the NexImage 5 retails for under $200. Because the pixels are quite small compared to the dSLR, it is able to record images of much higher resolution on subjects like the moon, for a given magnification. It is able to do a variety of things, including recording AVI video files that can be used in the stacking process.

Lunar tile

One image captured by the NexImage 5 camera, including the famous craters Tycho and Clavius.

I decided to try making an image of the moon using single exposures with the NexImage 5. I set up the telescope to point at an area along the terminator of the moon, took a single image with the camera, and then manually moved the telescope so that it was pointing to an area that overlapped the first image by about 30 percent. In this fashion I worked my way across the entire surface of the moon, taking 41 individual images.

Having the pictures recorded was just the first step. The camera software had recorded the pictures as bitmap files (*.bmp), and so I used a free image processing software to convert them from bitmap to JPG files. I then used another free software package called Autostitch (downloaded free for personal use at: to automatically bring all of the JPGs together, align them, and blend them together. I ran the program first on about a dozen overlapping tiles to see if it would work at all: Autostitch is designed for landscape photos – not moonscapes!

pano1 800px

A section of the lunar panorama made by using Autostitch to put together a dozen individual tiles.

Autostitch performed better than I could have hoped on my lunar frames! I re-ran the program using the whole set of 41 tiles, and in moments had my portrait of the moon in high resolution.


The moon, stitched together from 41 individual frames using Autostitch.

The final stage in assembling the image was to fill in the grey areas that were not actually captured by the imager.  I used another free software package, Paint.NET (not as capable as Photoshop but a whole lot less expensive!) to adjust contrast and brightness a bit, and paint in the grey areas with black. The results would be even better if each of the tiles had been prepared by the stacking process, which can result in dramatic improvements in such images. For now, I’m happy with yet another photo of the moon!


The final composite image of the moon, captured on 16 August 2013.

Copyright © 2013 David Allan Galbraith

Can Astrophotography be Considered Art?

The debate as to whether photography can be an art – or whether (at least some) photographs are art – has been long standing, and in some circles doesn’t end. The fact that there is some kind of equipment involved, and a process that wasn’t available in Renaissance Times to the great masters, seems to be a sticking point for some. For those that only consider art to be a handicraft executed with traditional materials, astrophotography must seem like arcane technical fiddling resulting in – what? A picture of the moon or stars? How is that art?

That there are now about a trillion photographs per year being taken around the world, most of them with cell phones, doesn’t help resolve anything, I suppose. Then again, art is not about a set kind of process or a formulaic end product. It can’t be. Otherwise, the skillful application of a paint bush to the side of a barn is art just as is the Mona Lisa.

Defining what is and isn’t art isn’t a matter of technology applied. At least in my mind, art is a process of communication in which thought and creativity are combined to express something of meaning. This is of course very open-ended, but in my experience there’s little more specific that can be brought together in one short definition that fits the range of artistic expression I see around me. Art isn’t just about a defined product, because that removes the receptive mind of the person experiencing the art from the equation, too. The receptive, critical mind of the observer/audience is as important to defining art as is the creative, skillful, intent of the artist.

This is nearly as vague as stating that “art is what an artist does or makes,” but even this second idea isn’t all that far off the mark. Who is an artist? Is someone who has great technical skill but does not apply any critical thought to their work, or who never puts that work into the sphere of a receptive audience, an artist? I’m not sure, of course. An interesting case in point is that of the late American street photographer Vivian Maier, who is being recognized as an amazing artist, but only after others found her work and popularized it. Was she an artist? A hobbyist? An obsessive-compulsive photo-snapper hoarder?

Some photographers have rejected the idea that they are artists. One of the greatest living photographic masters, Sebastião Salgado, is a Brazilian photographer whose work is considered as social documentaries. He has stated that he doesn’t think he makes anything new, but instead picks up things around him to tell stories. Yet, when I see his work I am moved, and his work has the qualities I identify as art: great creativity, expression of ideas and passion, and technical mastery. For me, an artist must bring some measure of all of these things together, regardless of the medium being used. I call Salgado an artist even if he is reluctant to do so.

“I don’t know art but I know if I like it,” or perhaps more honestly, “I don’t know how to define art, but I know it if I see it” might be closer to the mark. And perhaps more honest, too.

I am certainly prepared to dispense with the question of whether a photograph can be considered as art. More than anything else, it depends on who is looking at it. One point in favour of the proposition that astrophography can be an art was provided in 2012, when an art museum in the USA put on an exhibit of astrophotographs as art. This step – of having a curated exhibit at a museum – is one of the only widely-recognized measures of whether something that may previously be considered “not art” suddenly makes the jump into the “art” sphere.

“Starstruck: The Fine Art of Astrophotography” ( was an exhibit at the Bates College Museum of Art (Lewiston, Maine, USA), on exhibit from 8 June 2012 through 15 December 2012. This is the first instance of which I am aware that an art museum has taken on astrophotography specifically as art.

Others have approached the question, too. Russell Corman considered on his blog whether astrophotography is art or science (, and describes what he does as a “very technical art.” ( Interestingly, I would argue against amateur astrophography for creative purposes as being science. For me, science isn’t just the application of technology for some activity. Science, like art, is a process that results in interaction with a community, and with the communication of scientific results in a way that the community understands and recognizes. It may be educational, fascinating, and highly technical, but if an activity doesn’t put results into a peer-reviewed journal, for me it’s not exactly “science” either. There certainly can be amateur scientists (Darwin was one), just as there can be amateur artists (most, in fact, are, by definition: someone who does what they do for the love of it, not because it’s a regular 9-5 job). It’s not whether or not you work for some “sciencey” institution that designates you as a scientist – it’s whether you apply the critical thought process of science to a problem that interests you and then disseminate the results so that others can learn what you have learned.

I expect that this question will remain an open one, and that’s encouraging and exciting. I don’t consider all astrophotographs as art any more than I’d identify all photocopies as art. However, could a photocopier be used by an artist as part of her work? Certainly. Could a camera and telescope be used by an artist to create an image that was thought-provoking and moving? Yes. Can it be considered art? Show me and we’ll discuss it. The precedent of the Starstruck museum exhibit opens the door in a serious manner. An examination of some of the images that were included in the exhibit is, perhaps, an indication of where the art is to be found in astrophotography. Some of the images available in the on-line material about the exhibit were in fact taken by NASA spacecraft. They were selected and prepared for the exhibit by artists, using a variety of processes and final media. The show also included images considered historically significant that were created for documentary purposes.

I recall my dear, late mother’s view of art, too, when I approach questions like this. For her, art was something that represented something she recognized. She loved Pablo Picasso’s early works, but hated his cubism. She even kept a print of his Harlequin on her bedroom wall, not knowing who had done the work until I pointed it out to her. If a work wasn’t a skillful, draftsman-like rendering of something she recognized (and liked), my mom wouldn’t give it the time of day.  For her – and for everyone, in reality – the determinant of whether something is considered as art depends on a complex set of cultural expectations and filters. Recognizing that we all have those sorts of filters is an important first step to asking a more difficult question: is my own set of filters keeping me from seeing what others might be seeing? I think that’s where art has one of its strongest roles in society, and it’s where an artist’s contribution is most vital. Bringing things forward that others may not see. In that sense, some astrophotography is art indeed.

Copyright © 2013 David Allan Galbraith

View Nova Delphinus 2013 – A Limited Time Opportunity

nova and nebula

Nova Delphinus 2013 (left) and planetary nebula NGC 6905 (right), cropped at full scale from the same photograph taken on the evening of 24 August 2013. While I’m generally pleased with the images I took that evening, there is evidence of some problems on this 30 second exposure – the pulled out stars should all be points. More details follow below.

Although a lot has been made of two comets passing through our skies in 2013, August has given us an unpredictable and much rarer astronomical event: a nova, visible to the naked eye. Nova Delphinus 2013 has proven to be the brightest nova in five yeas – definitely worth a look. Novas are fleeting, however. There isn’t much time.

According to, Nova Delphinus 2013 was discovered on 14 August 2013 by Koichi Itagaki in Japan. Prior to brightening more than 100,000 times in its explosion, the star was a dim little 17th magnitude. It became as bright as 4th magnitude in the days since it was first spotted, and is now fading a bit. Over the coming days and weeks it will fade completely.

I set out on the evening of 24 August from our cottage in Bruce County to see if I could see it. Novas are exploding stars, and the initial flash doesn’t last too long. First, I had to find out the coordinates of this transient object.

The nova is located in the constellation Delphinus, the Dolphin, not too far from the “tip” of another constellation, the arrow, Sagita. The astronomical coordinates are RA. 20 h 23′ 31″, Dec. +20° 46′.

Some near-by land marks help, too:

  • Altair (α Aquilae), at 0.9 Magnitude, in Aquila, is the nearest very bright star.
  • Sualicin (α Delphini), 3.6 Magnitude, in the held of the dolphin, Delphinus, is the nearest named star.
  • A little blue planetary nebula, “The Blue Flash Nebula,” NGC 6905 is so close that it will appear in the same field of view through a wide-angle eyepiece. The 12th magnitude nebula is located at RA 20h 23m 02.52, Dec+20° 08’57.2″

A wide-angle chart of the area of Nova Delphinus 2013, rendered with the freeware planetarium program Cartes du Ciel. This chart covers about 30° of the sky. The nova and the planetary nebula NGC 6905 are so close together that I’ve just indicated the nebula here.


A narrow-angle drawing of the areas of Nova Delphinus 2013, prepared with Cartes du Ciel. This chart covers about 5°. The nova sits just within the boundaries of the constellation Delphinus (indicated by the faint purple lines).

As it will appear in most telescope mount “go to ” databases, finding NGC 6905 is a great way to get to the area of the nova quickly.

I set out to a gravel parking area near the Bruce Botanical Food Garden on the east side of Ripley, Ontario, at 8:30 PM on the evening of Saturday 24 August 2013 to see if I could spot the nova. I had found this site the night before, and it proved reasonably quiet, and fairly dark, although there are some near-by houses a few hundred yards away.

Some high clouds made the night of the 24th a little disappointing, and with moonrise set for 9:55 PM I knew I had to work fairly fast. I admit that I had trouble finding the nova with binoculars. I could see a fairly rich star field between Delphinus and Sagita, but really couldn’t decide if I was seeing my target or not.

I reverted to the aid of SynScan on my EQ6Pro mount to save the day, and wasn’t disappointed – eventually. I did found the nova, but only on photographs after the fact. Looking through a 28mm eyepiece on an 8” Newtonian, I couldn’t be sure at all what I was seeing. So, I re-reverted to imaging.

I set up a Nikon D800 body on the telescope, focused on a faint star using live view, and took a series of 30 second exposures at ISO 800. The nova turned out to be the brightest star in the frame, as expected. Actually, I spotted NGC 6905 first! The little blue ball was a charming sight on the photographs, and really stood out. I also have another admission, about NGC 6905. I didn’t know it was in the area of the nova until I saw my photos. At first I thought it was likely an artifact, but a quick check of the area on charts confirmed that in fact it was a planetary nebula, known as the Blue Flash Nebula. NGC 6905 is well worth a look on its own. It’s considered as a very lice planetary, and was discovered by William Herschel in 1782. This was another first for me – my first image of a planetary nebula. An added bonus for a night of nova hunting! The nova itself registered as a bright white star, bright enough to show faint diffraction spikes from the telescope’s secondary mirror spider.


Nova Delphinus 2013 (left) and the Blue Flash Nebula, NGC 6905 (right), photographed on the evening of 24 August 2013 at 9:51 PM EDT, from the east side of Ripley, Ontario. North is approximately toward the left. The single 30 second photograph was taken through a SkyWatcher 8” imaging Newtonian telescope with a coma corrector, and a Nikon D800 body, set to ISO 800, on an EQ6Pro mount. This copy has been reduced down in resolution and cropped from the original frame. The two smaller images at the head of the post are from the same frame, without reduction in resolution.

If weather and conditions permit, I recommend having a look for Nova Delphinus 2013. In the coming nights the moon will be rising later each night, and dropping in brightness, so this is a great time to try, while the nova is still bright. For southern Ontario Delphinus is nice and high in the sky after sunset. No reason not to go have a hunt for a truly rare sight!

Copyright © 2013 David Allan Galbraith