BAA Lunar Section

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Lunar photography

Advisor: Bruce Kingsley


Introduction to lunar photography
by Peter Grego

Until the advent of photography in the mid-19th century, drawing the Moon at the eyepiece was the only way to capture the splendour of the lunar landscape. The arrival of CCD cameras and their increasing availability to amateur astronomers since the 1980s enabled lunar imaging to take its next great step - high resolution imaging that captures all the fine detail that the eye can see. Image processing and computer enhancement further refines images to bring out more detail, and our understanding of lunar topography is aided by placing features in fresh perspectives (such as creating alternative views based on 3D modeling or producing anaglyphs of the sort shown below).


The Moretus area on 2008 September 21, imaged and processed into a 3D anaglyph by Bruce Kingsley (requires red/blue glasses)

Conventional photography
The Moon is such a large, bright object, that any film camera pointed through a telescope can capture a lunar image. With luck and experimentation, pleasing images can be obtained by holding a camera up close to the eyepiece of an undriven telescope and clicking away. But this is very much a hit and miss approach - costly, too, if out of a whole roll of film you're only going to produce just one or two reasonably good shots!

There are a number of important guidelines that all successful conventional lunar photographers follow, but there is also a degree of art to it - the products of experience and intuition that can't be explained clearly in writing. For the very best results, a sturdy, driven equatorially mounted telescope is required, since even with exposures of fractions of a second, the Moon's drift through the field of view in an undriven instrument will produce a degree of image blurring. To obtain the sharpest image possible, a camera should be secured to the telescope so that it is in line with the optical axis and unable to wobble around.

Afocal photography with a fixed-lens camera
The techniques of afocal photography apply to both conventional and digital fixed lens cameras alike. However, the simplest and cheapest types of film camera don't have any means of focusing the image - they have a set focus range from several metres to infinity - nor can the exposure time be adjusted. In spite of their severe limitations such basic cameras are sufficient to capture a pleasing image if the Moon is first focused in the telescope eyepiece, and the camera is then positioned close to the eyepiece (but this has to be the right kind of eyepiece, as explained below). The photographer will usually have to fashion a makeshift adapter for the camera to fit onto the telescope, since the cheapest cameras won't be threaded to accept adapters or attachments. All amateur astronomers ought to have in their toolbox some blu-tack and electrical tape - adequate materials to temporarily fix a lightweight camera to a telescope.

Even though an eyepiece can give a large apparent field of view when viewed with the eye, vignetting can occur on the finished photograph - that's where the image of the Moon is surrounded by a dark circular border. The degree of vignetting depends on the size of the camera's fixed lens in relation to the eyepiece lens, the type of eyepiece used and the distance of the camera lens from the eyepiece. The main cause of vignetting is due to the camera lens being much larger than the eyepiece lens. In addition, the eye relief of an eyepiece affects the degree of vignetting, and very short eye relief eyepieces (usually short focal length eyepieces that give high magnification) are difficult to use afocally with a fixed lens camera because it is necessary to position both camera lens and eyepiece lens as closely as possible (so close that they are almost touching). Usually the result is highly unsatisfactory, with only a small central image surrounded by a dark border, like viewing through a long tunnel. Eyepieces that deliver small apparent fields of view also produce vignetting, so basic types like the Huygenian design are to be avoided.

Finally, make notes of your experiments! There's nothing more frustrating than running off a roll or two of lunar exposures, discovering several lunar images that appear to be perfect, only to scratch one's head and wonder exactly which eyepiece was used and what exposure employed.

Advanced lunar photography
The most popular camera used by lunar photographers is the 35 mm SLR (single lens reflex), a design that has been in common use since the 1960s. Some of the older and lower end SLRs are very basic in design, with exclusively manual controls. The more expensive SLRs have full electronic controls that can adjust every aspect of the camera's functions. A basic SLR is all that is required for lunar photography, and it can deliver just as good a lunar image as a camera ten times its price. The image entering the SLR is directed by an internal mirror into the viewfinder, allowing a direct view of the subject being photographed. When the shutter is released, the mirror flips up, allowing light to fall directly onto the film. The mechanical vibrations introduced by 'shutter slap' can affect the quality of the image, and the mirrors of some cameras can be locked into the 'up' position before the image is taken. To minimise vibration that might blur an image when pressing the shutter button, lunar photographers use a cable release, a function that can be controlled electronically on high-end SLRs.

Telephoto lens photography
Telephoto lunar photography has several advantages - the equipment is relatively lightweight and portable, allowing quick setup and access to the Moon from areas in the backyard that might not be possible with a bulky telescope and its mount. Used with fast film (with a higher ISO rating, hence shorter exposure times) the relatively low magnification of the Moon will not produce a great deal of image drift and blurring. Provided that the camera is stably supported (preferably on a tripod), very nice images of the whole Moon that show detail along the lunar terminator can be obtained with a 35 mm SLR using a telephoto lens with a focal length of 800 mm to 2,000 mm. To find the size of the lunar image on film, simply divide the focal length of the lens by 110. A 50 mm lens will give a tiny lunar image size of less than half a millimetre; an 800 mm lens will give an image more around 7 mm across, and a 2,000 mm lens will produce an image of 18 mm. A x2 teleconverter will effectively double the focal length of any telephoto lens, extending a 500 mm focal length into 1,000 mm, although the resulting image will be slightly dimmer and inferior to one taken with a 1,000 mm telephoto lens. However, the larger image size resulting from the use of a teleconverter will produce a far better image than a lab-enlarged image of the Moon taken with the same telephoto lens without the teleconverter, since the enlargement will be grainier and less distinct due to the limitations of the resolution of the film.

Prime focus photography
Using a T-adapter to attach the camera body to the telescope, the telescope effectively becomes a large telephoto lens. Using prime focus, a telescope with a focal length under 2,000mm can project the entire half-degree wide lunar disc onto a 35mm frame. Prime focus is the best method to capture a sequence of lunar phases. It is quite easy to focus the Moon through the camera's viewfinder, and exposure times must be judged according to the focal ratio of the telescope, the ISO (speed) of the film used and the Moon's phase.

Eyepiece projection
Prime focus photography is great for capturing the entire lunar disc, but for closer, higher magnification views, an eyepiece can project the image directly onto the film. Eyepiece projection adapters are available - these fit into the eyepiece holder, the eyepiece is inserted and the camera is fixed to the adapter. Standard Plössl eyepieces can be used to deliver nice crisp images with flat fields of view. Experiment with a variety of focal length eyepieces and bracket the exposure times to find the combination that suits your requirements.

Film types and exposure times
When beginning in lunar photography, generic 200 ISO colour film is ideal to experiment with, since it is cheap and widely available, although the quality will vary from brand to brand (and even in different batches of the same 'budget' brand). The ISO rating of a film denotes its 'speed' - the higher the ISO, the faster the film and less exposure time is required. The Moon is so bright that it is possible to use very slow film to capture it - even as slow as ISO 25. Slower films are less grainy and as a result can withstand higher enlargement than faster films without the grain showing through.
Formulae for calculating lunar exposures take into account the aperture and focal length of the lens/telescope, the camera f/stop employed, the film speed and the Moon's phase. The brightness of the Moon and hence the exposure time required is also affected by the Moon's altitude and the presence of cloud.

Digital cameras
Most digital cameras possess non-removable lenses, so the principles involved in photographing the Moon through them are identical to fixed-lens conventional film cameras and the afocal method (see above). Digital cameras are versatile, with a variety of functions that can be adjusted to suit the conditions, and images can be instantly reviewed on the camera's TFT screen to determine whether they are worth keeping. After manipulation with an image program on computer, the end results, on screen and in print, can be superb.

A digital camera's resolving power depends on the size of its CCD (charged coupled device) - a tiny electrical chip with an array of minute photosensitive squares (pixels), immediately behind the camera lens. Cameras with the highest pixel rating will capture the highest resolution single-shot images of the Moon. Digicams can store images in a range of resolutions - the lower the resolution, the smaller the image file and the more images can be stored in the camera. Digicams of 3 megapixels or higher can capture impressive single-shot views of the Moon, while images secured with high-end 8 megapixel (or higher) digicams can produce crisp images capable of being enlarged. Many digicams are capable of taking video clips which can be computer processed to produce high-resolution still images, overcoming the effects of poor seeing.
Focusing can be a problem with digicams, as their TFT screens are usually quite small, some measuring less than 4 cm (diagonally). First, focus the image with your eye through the telescope eyepiece and then attach the digicam to the eyepiece; use zoom to zero-in on the lunar terminator, where fine focusing will prove easiest. If your camera can be hooked up to a TV monitor, the larger image will be far easier to focus by.

The problems of image vignetting may be combated by using the zoom facility. If the edge of the field appears dark or hazy, an adjustment in zoom can remove it altogether. High degrees of zooming brings into play the camera's 'digital zoom' and should be avoided, as in this mode the image is usually of low resolution. It's better to enlarge a high resolution picture than to try to capture the same area zoomed in at low resolution.

Gauging exposure can prove troublesome. The camera's inbuilt autoexposure meter may overexpose the Moon, particularly if the whole Moon is being imaged and the Moon is not centred in the field of view. Autoexposure usually works best if there is a uniformly bright field, and your digicam will probably judge exposures well with lunar close-ups. Many digicams have exposure variation capabilities equivalent to two f/stops above and below the optimum, so use this if you're having problems with overexposure or underexposure. The type of light conditions selected can affect exposure too, so experiment with various combinations and note which ones appear to work best.

Digicams can produce some vivid colours that bear no resemblance to the view through the eyepiece. Many digital photographers mute these tones in the processing, or decide to convert the images to black and white, which can appear much more pleasing to the eye than a multicoloured Moon. If your camera has the ability to photograph in black and white, give it a go - black and white images can appear much sharper than colour images, and the smaller image files take up less space in your camera's memory.

Camcorders
Although the Moon is not a dynamic world, its shadows appearing to creep at a snail's pace across the surface near the terminator, video footage of the Moon is fascinating to watch, and conveys a sense of being at the eyepiece far more than a still picture can ever do. Video captures the atmospheric shimmer as it momentarily distorts the view, and a sweep at high magnification along the terminator using the telescope's slow motion controls allows the viewer to experience what real observing is like. Camcorders are also ideal to record lunar eclipses and planetary occultations.

Camcorders are heavier than digicams, and the coupling between camcorder and eyepiece must be rigid. Adapters are available that slot into the eyepiece socket and hold the camcorder on an adjustable arm so that it can be brought up close to the telescope eyepiece and locked into position. Digital camcorders are the lightest and most versatile available, and their images can be edited on the computer.

Camcorder imaging uses the same afocal principles as conventional or digicam photography. The problems of eyepiece selection and vignetting are present, and their solutions are the same as with digital photography (above). With experience, it is possible to produce a wonderful tour of the Moon and its terminator, taking time to zoom in on interesting features. These make fantastic presentations at any astronomical society meeting - but think twice before showing all of your hard-won camcorder footage to visitors and relatives, as they may not appreciate half an hour of wandering around the crater-crowded southern uplands as much as you!

By downloading digital footage onto your computer, images can be grabbed individually (at low resolution) or digitally stacked to produce detailed, high resolution images. The same method is used to produce high resolution webcam images (explained below). It is essential, when embarking upon digital video editing, to have at least 5 gigabytes free on your computer's hard drive, as the process temporarily eats away at the available hard drive space. The resulting edited videos can be transferred to CD-ROM or DVD-ROM and then removed from your hard drive to free up more space.

Webcams
The use of webcams to capture high resolution lunar and planetary images has been growing in popularity since the early 1990s. Webcams are only a fraction of the cost of dedicated astronomical CCD cameras, they are lightweight and versatile - indeed, many experienced lunar and planetary imagers prefer webcams because their high frame rate allows ease of focusing and the opportunity to capture more images per unit of time. Any off-the-shelf webcam attached to a computer at one end and a telescope at the other can be used to image the Moon and the brighter planets.

Webcams are usually positioned at the telescope's prime focus in place of the eyepiece. Several makes have removable lenses into which can be screwed commercially available adapters, such as those for the Philips Vesta Pro, Philips ToUcam Pro and the Logitech QC 3000 Pro. CCDs are highly sensitive to infrared (IR) light, and the lens assembly contains an IR blocking filter. Without an IR filter, a perfectly clean focus through a refractor is not possible as IR is focused differently to visible light. IR blocking filters are however available, to place between the telescope and webcam, allowing only visible light to pass through to a sharp focus.

Although webcams are used at prime focus, the image of the Moon they produced is at quite a substantial magnification, and only the shortest focal length instruments will allow the whole Moon to be viewed in the field. The CCD chip itself is quite small, and only part of the image is being projected onto it. For example my short focal length (f/5) 80 mm refractor requires the use of a x2 focal reducer in order to fit the entire Moon into the field of view.

Since they don't have a viewfinder or a TFT screen, focusing a webcam can be a trying experience. There's no point focusing the Moon through the eyepiece and replacing the eyepiece with the webcam, as there will be a substantial difference in where the focal point lies. It is best to focus the webcam on the lunar terminator whilst having a clear view of the computer monitor, best done with a laptop in the field, next to the telescope. Even a slight knock can push the Moon out of the small field of view - this is where a really well-aligned finderscope comes in extremely useful! If your webcam is connected by wire to a computer indoors, focusing may entail some rushing to and fro until a good focus is achieved. Once a good focus has been found, carefully mark the position of the focuser tube with a chinagraph pencil so that you don't have to go through the whole process again the next time you want to do some imaging. Of course, the focus will need tweaking slightly each time you set up, since a fraction of a millimetre can be all the difference between an acceptable focus and a razor sharp one. Electric focusers are a highly desirable item in webcam imaging, and being able to adjust the focus at leisure from indoors at the computer can make a great deal of difference to your enjoyment and the quality of your images.

The webcam manufacturer's own software is used to record image sequences as AVI files from the webcam to the computer. The image download rate will vary with the type of equipment used. Using an older USB-1 camera of 640 x 480 resolution, the rate should be limited to a maximum of 5 frames per second to avoid lossy compression. Much higher rates of up to 30 fps with no compression are possible with USB2 enabled high-end webcams. The image can be adjusted to produce the best balance of exposure, brightness, contrast and colour, but often the Moon can be successfully imaged in full auto mode in short bursts. As with digicam imaging, the use of black and white (greyscale) can simplify matters, especially if you're using a short focal length achromat prone to producing a degree of false colour.
Image editing software, such as the freeware Astrostack, is then used to extract individual images from the AVI. A well-aligned and smoothly operating equatorial mount is essential to good webcam imaging, as a misaligned mount will produce image drift even in short capture sequences - this produces problems when attempting to align and stack the images. AVI files are chopped into individual BMP frames by the processing software, and each BMP can be checked visually (a laborious process) or by the software itself for quality. The best images are stacked and combined to remove noise (improving the signal to noise ratio) and eliminate artifacts. The stacked image is then processed to bring out detail, unsharp masking being one of the most useful tools for achieving a clean-cut image. Beware of applying too much image processing - spurious artifacts can, and do, arise as a result of overzealous manipulation, and fine tonal detail can be obliterated.

 
Beginning lunar imaging
Introductory notes by Maurice Collins

I have recently been contacted by someone who is interested in getting into lunar imaging, so I have been thinking about how I started, and giving him some tips. I thought may be worth sharing with a wider audience also in case there is anyone out there who may be under the impression that it is something way too difficult or expensive for them to do.

Firstly, do you have any sort of still digital camera that you use for family photos, holidays etc? Even a mobile phone camera will work. If you do have a digital camera and a good eye relief eyepiece of fairly long focal length, you are all set to make a start. To begin with, a 25 mm to 17 mm eyepiece works well, but you can use up to the limit of your telescope as long as the camera can see through it.

To take images, simply point the camera through the eyepiece, holding it by hand. To find the Moon with the camera lens, which can be a bit tricky, back off a bit until you see the bright spot of the Moon’s image on the cameras LCD screen, then bring it down closer, but never actually touching the two lenses together (though no harm seems to be done if they do briefly touch). Put one finger on the side of the eyepiece to steady the camera in place. It does not cause as much vibration as you would expect and helps keep the Moon in the field of view while taking the photo.

Next, focus the telescope, as the focus of your eye at the eyepiece is different to what the camera sees — for me it is a reasonably large change of telescope focus. Then use the camera’s zoom function (either digital or optical zoom is okay) to frame out the black eyepiece field stop that vignettes the image so that you only see the lunar surface on the LCD of the camera, or at least only the edges of the frame showing black. Gently press the shutter while holding your breath so as not to giggle anything. Oh yes, and remember to disable the flash! And voila, you should get a very nice image of the whole disk or part of the Moon. If it looks too bright and saturated, or too dim and grainy, check the EV settings on the camera and go up or down a couple of settings to see what works best for that phase of Moon.

Take lots of shots. Some will be blurry, some will be sharp, and the more you have the better you will get a good one out of it. You can then process the images on your computer to reduce the size to sharpen it and run the other image processing functions over it to get it looking good. Sometimes the images look better in grayscale, sometimes the good ones look nice in color.
The technique described above is the easy way into lunar astrophotography. If your camera has an AVI movie mode, you are even one step up and can just record a video sequence which you can then stack using a program like Registax to get really sharp images that you can mosaic together if you like. This works for planets too. This way, I recently obtained a really nice shot of the crescent Mercury showing its phase. You can even use a video camera, and convert the camera files to AVI and then do the stacking. I have only used this for a lunar eclipse and thin crescent Moon but it works, though a bit more work is involved.

The next step up (and easier way) is with the a modified webcam or astronomical CCD camera such as the Meade LPI (Lunar and Planetary Imager). No eyepieces are needed, just the camera at prime focus and you can add a Barlow lens if you wish to increase the image scale.

Think simple, and it usually works. Also if someone says to you: “You can’t do it that way!” ask “why not?” Break the rules (if there are any hard and fast ‘rules’) and experiment to see if it works. You don’t you need brackets and fancy CCD cameras to do lunar astrophotography. If you have them, all the better, but if you don’t, lunar imaging is still something you can do.
I now use the Meade LPI to do my lunar imaging, and much of it is done remotely, but it wasn’t too long ago that I was using the simplest methods outlined here to take pictures of the Moon, so before I forget my beginnings I thought it worth sharing with others. I hope this helps someone in getting started who would otherwise not think of trying it, using gear they may already have around home.