The most conspicuous feature is the extremely bright object right of centre, and it seemed highly likely on first inspection that this would be one of the planets, which for once meant that the timing of the photographs was extremely important. These timings are given in the Definitive Apollo Source Book.

The most obvious candidate for such a bright night sky object is Venus, and indeed that is exactly what it turned out to be.

The combined view is splendid for a couple of reasons. First of all it combines Venus, Mars and, hidden in the flare near the window frame, Saturn, all taken from a point many thousands of miles from Earth. It also shows just what an incredible view the astronauts had. As long as they could get rid of ambient light, they could see the universe laid before them.

As with other pictures featuring stars, the great distances between us and them mean that it doesn’t matter whether a photograph is taken on the moon or the Earth, the star patterns are the same.  However, because Mars and Venus are in the frame what we can definitively state is when it was taken.

The Stellarium view above is based on a time of midnight on the 27th, and if you care to overlay the two images, you’ll find it is a reasonable estimate, which it should be given that it matches what the official reports say. Make the image 12 hours earlier or later, however, and you get the two versions of the same scene shown below.

Although there is no information as to what direction to look in, the constellation shown is very recognisable to anyone in the southern Hemisphere, the Southern Cross.

There aren’t enough stars present, or even (to be fair) enough objects that we can be sure are stars, but it is only reasonable to present everything available. Make your own mind up.

Sadly, that’s all we have for Apollo 16’s stellar photography efforts. Another magazine (126) features the results of Gegenschein photography and another batch of Gum nebula images, but as yet this is unavailable.

What we do have to look at are several photographs of the lunar surface taken under illumination from Earthshine, and it would be a shame not to look at them. For the uninitiated, Earthshine works in the same way as moonshine does: light reflects from the Earth’s surface and illuminates the moon,. The effect can be seen around sunrise and sunset when, in the right conditions, the unlit portion of the lunar surface stands out against clearly the night sky.

The best images are on magazine 127, AS16-127-20018 & 19, shown below.

According to the reports these two photographs were taken at 20:22 and 20:24 respectively on 21/04/72 with an exposure time of 1/125 of a second. This is a remarkable shutter speed for a dark area, an is indication both of the amount of light given out by the Earth and the light capturing capability of the Zeiss lens.

The photographs themselves are of Riccioli crater and some smaller ones to the east of it. Riccioli is a crater near the western limb, and was definitely in the dark at the time it was pictured. The images below show the Stellarium view of the moon from Earth at the time of the photographs (approximate position marked by the white dot), and a terrestrial view of the same area photographed in 2004.

A perfect match. A similar version of the image is also available in this 1974 report, where it is mistakenly inverted! The Venus image also features in the report.

While the 35mm magazines don’t show any of the solar corona photographs, we do have some in the 70mm Hasselblad record on magazine 124. Two images sequences in this magazine show the corona and the stars around it, and the best examples of these are shown below, AS16-124-19985 (left) and AS16-124-19904 (right).

The first set was taken on revolution 38 (which commenced at 147:10) and the second set on revolution 47 (started at 165:08).

What can we see on them? Well, Stellarium shows us should be visible at a midpoint in time between the two sessions (middle, above).

The cluster of stars halfway down the right hand side are the Pleiades, while on the left the bright star just below the corona is Mothallah. At the top of the photograph above the corona is Menkar.

All the stars are where they should be for the time they were photographed, in a solar corona that could not be photographed from Earth.

The only other dim light photographs currently available are in a Hasselblad magazine (magazine TT), but it is unlikely that any stars will be identified because the feature shown is likely to be light reflecting in a water dump. This is discussed in the mission report, where they mention that a water dump was photographed ‘possibly’ (according to Charlie Duke) on 70mm film. It isn’t clear when the photographs were taken. The photographs below show one of these images (AS16-125-19932) in its original form (left) and enhanced (right).

What is worth pointing out here is that while the wider view of Riccioli is very similar to that of the Earth-based photograph, the view of the satellite craters is not - it shows an almost vertical view of them that is not possible from here.

The other Earthshine views are difficult to identify - even with image enhancements it is not possible with any certainty to pick out the surface features they show. The best that can be done is the one below, AS16-127-20014, taken a few moments after the Ricciolo overview photograph. The enhanced and rotated view (below left) is compared with an oblique Google Moon view (below right)  showing a Lunar Orbiter overlay.

The Stellarium view taken 12 hours earlier is on the left, 12 hours later on the right and both are superimposed on the Apollo image and made slightly transparent. The Apollo image has been darkened a little to make the glare around the window less prominent. No other changes have been made,

Venus and Mars are clearly in different positions while the stars remain fixed. Saturn’s much greater distance from us means that its movement is small enough to be undetectable over this time period. An astronomer would be able to tell you more accurately, but it will be many many years either side of this date in 1972 before these three planets share this configuration in this precise position in the sky.

The photographs were taken at the time it was claimed to have been taken, and they were taken in space.

Having settled that debating point, we can move on to looking at the other CSM attitude.

It’s debatable, but it is in the right place.

That’s it for the visible spectrum, but meanwhile on the lunar surface they were setting up a telescope to look at stars in the far ultra-violet spectrum, and this is dealt with in the next section.

Apollo Index Low Light Photography Index Apollo 14
Apollo 15
Apollo 16 UV Apollo 17

The report used above also helpfully points out that Venus is in shot in some of the frames, and it can be identified flashing by in the top right corner of this sequence of images from the remainder of the Zodiacal light frames.

As in the previous example, it is evident that the stars are being photographed from a moving vehicle - the vehicle in question being the Apollo 16 CSM.

The next star photographs from Apollo 16 are to be found in magazine 129. Most of the images are identified as ‘unused frames’, but there are several that contain useful images of an experiment designed to assess the impact of spacecraft emissions (from eg gas venting, urine dumps, particles from thruster burns) on photography, with a view to working round any problems in the future Skylab missions. The photographs, taken when the crew were well on their way home between 23:24 on 26/04/72 and 00:54 on the 27th, were done in 2 attitudes.

The first attitude is best illustrated by AS16-129-20071 and 20075, which can be combined to produce a wider view, as shown below:

Before seeing if we can locate what these photographs are showing, it’s worth discussing what’s in them.

Believe it or not, they all show roughly the same view. The two clearest ones on the top and bottom right show pretty much the same region of sky, and this can be determined by picking out the three stars in a line (the central one of which is Adhara) in the upper left quadrant.

These same three stars can also be seen in the bottom left image, which shows them as star trails.

Star trails are common in photographs taken from Earth thanks to its rotation under the view the camera is observing. The most spectacular images are those where the camera has centred on a pole star, around which all the stars apparently rotate from our viewpoint. The further away from the pole star, which appears as a fixed point, the more pronounced the elongation of the trail. In the northern sky this is Polaris, in the south it is Sigma Octantis.

In our photograph, we have a similar focal point that is not moving, while the other stars are shown as trails the further away they are from that point.

Is that focal point the north or south celestial pole?

Not to put too fine a point on it: No, it is some distance from it. Using Stellarium it is possible to obtain views of the sky, and we can use these as a comparison with our Apollo 16 photos to see where they actually are..

The report linked to above tells us not just when the photographs were taken, but of which part of the sky. It gives the image boundaries as between 7h35m Right Ascension (RA) and -330 (a co-ordinate system used in astronomy) and 6h10m RA, -150. By pointing Stellarium at this part of the sky it is a very quick task to identify one of the brighter stars, Sirius, cut in half and lurking at the upper left margin of AS16-127-20022. Once we have this identified it’s relatively easy to pick out others. The Apollo and Stellarium views are shown below.

So there we are, Apollo 16 takes a photograph of stars, which is a big kick in the nuts for everyone who says they didn’t.

They also took it when not pointing at the celestial pole, which means that the movement in the two other photographs (taken over 4 minutes rather than 1) is from the window mounted camera rather than the stars themselves. In other words it wasn’t from a camera stuck on the ground.

The next set of star photographs in magazine 127 are listed as showing ‘Zodiacal light’. This is light from our sun scattered by cosmic dust, It is very faint and therefore difficult to photograph. A large number of frames were exposed attempting to photograph the phenomenon on 21/04/72 either side of 21:00. As with the Gum nebula photographs there is mixed quality, but it is possible to make out some clear star patterns. The best views are in AS16-27-20004. Several frames after 20004 show trails, and as will be demonstrated these are definitely part of the same sequence.

First of all let’s see where 20004 is. The report above gives co-ordinates of between 3h30m 350 and 2h05 250

If we look around that area we indeed find a match:

Like the previous missions, Apollo 16’s low light level photography had several aims.

Photographs were to be taken of the Gum nebula, of Gegenschein regions, of the lunar surface under Earthshine, and to see what influence venting from spacecraft had on the quality of photographs in preparation for the future Skylab mission.

A number of magazines were exposed with the camera either hand held or secured on a bracket in the window behind a specially rigged blind. Cabin lights were usually turned off to minimise ambient light intrusion. Command Module pilot Mattingly stated in the mission report that he turned off all the lights even when not required to just to be on the safe side. CSM rotation was also minimised,

Magazines 128 and 130 were used for calibration purposes and are not available online. Magazines 127 and 129 are available here. Magazine 126 is yet to be found. Most of the images were taken using a Nikon F, but some were taken using the Hasselblads. The 16mm DAC was also used, but magazine HH has not been found online yet.

This report contains details of what can be found in the magazines, and the preliminary science report discusses the experiments. More information can be found in this report and the mission report.

What can we see in them? The frames in the report linked to above are discussed in reverse order, and we’ll stick with that to make life simpler.

The first batch of images are of the Gum nebula. This nebula is a diffuse structure occupying a large amount of the southern sky and emits very little light, making it hard to study from Earth. Using a range of filters and exposure times, the region was photographed on 21/04/72 and around 18:45 GMT while the spacecraft was on the lunar far side. The frames covering this period are AS16-127-20021-4, and they are shown below.

Apollo 16 Low light photography

And here is Venus, marked by the red cross hairs, compared with AS16-27-20007: