Orbital Images

OK, so, the conspiracy theorists two main lines of argument are pretty much trashed by the preceding sections. They often claim that the landing sites were created on Earth using imagery from earlier probes. We have pretty much demonstrated that this is not true. Of course they will make up some more nonsense about the real images being hidden in a secret vault somewhere, but this is (not to put too fine a point on it) bullshit.

The simple fact of the matter is that the Lunar Orbiter views are good, but they are not good enough, and once the Apollo missions began orbiting the moon these became the primary source for photographs of the landing sites. Apollo photographs are the only source for some areas, and it’s pretty stupid to claim that Apollo photographs were used to fake Apollo missions.

The conspiracy loons will also claim that the Apollo hardware and the astronaut footpath and vehicle trails have been somehow Photoshopped into the LRO views. Well, in order for this to be true not only do they have to have manipulated images of the mission evidence, they also have to fake every  single crater and rock, because we have so far established that any crater or rock over (say) a couple of feet across pictured in an Apollo photograph or video can also be picked out in the LRO view. Not just one LRO view, but several, because most of the landing sites have several different views taken at different times in the lunar day.

We can hammer this point home even more by picking other images from Apollo missions, this time from orbit, and seeing how the details compare with LRO and LO views.

In each case I will pick the smallest possible Apollo photograph (in terms of the areal extent that it covers). I’ll also pick areas that are not visible vertically from Earth - craters on the lunar limb or far side, so that the only way they could have been acquired is by actually having a photographer there.

As it’s a very good place the start, we’ll start at the beginning, Apollo 8. The image I have chosen to use is AS08-14-2402. The image itself is shown below (left), and next to it (centre)is its location on the lunar surface as depicted on Google Moon (see my Apollo Moon files). Apart from it covering a very small area of the moon (the image is about 20 km wide), the other good reason for choosing this view is that the Hasselblad magazine from which it is taken contains  several Earthrise sequences that can be dated very exactly thanks to the existence of contemporary satellite photographs(see here), dates that coincide remarkably well with the launch of a large Saturn V from Florida!

To make life even more interesting, I’m going to zoom in to the Apollo photograph and pick a very small area to work on, and that area is outlined in red. It covers an area roughly 500m wide.

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The photograph covers part of Korolev crater, a much larger feature on the lunar far side (and therefore not visible from Earth). As the lunar far side was first imaged by the then Soviet Union, many craters in that hemisphere are named after Soviet scientists, politicians and other luminaries.

The crater was imaged by Lunar Orbiter 1, and a high resolution image of it can found here.

It is shown on the right above, with the area covered by the entire Apollo image outlined in red.

So, what does the area outlined in red on the Apollo image look like when compared with the LRO depiction of the same area (taken from a screenshot on this site) and the LO photograph?

Strike one for Apollo there I think. While the Apollo orbital image is not as clear as the LRO’s much better camera, the major craters are still visible. The LO1 image, on the other hand, has resolved into just light and shade, and absolutely no detail is rendered.

We can even go one better on this mission. India’s Chandrayaan passed over the same area in 2009 on orbit 885 of its mapping mission. The Terrain Mapping Camera (TMC) captured the same area. In order to get the same image I’ve used you’ll need to register, so there is no link provided, but you have all the information you need there to do it. I’ve used the full sized TIFF image (originally 5Gb) to get this view.

Let’s have a look at the same broad region and then the area examined from the Apollo 8 image, I’ve added an animation to show that it’s the same spot!

So, let’s see how Benedict looks when we compare it with the view from the LRO and LO1.

On this occasion, the medium resolution image does a good job of identifying the broad outline of the craters, and even picks out some quite small features (see right).

It would have been interesting to see how a high resolution version of this crater would have fared, but again it doesn’t exist - the high resolution versions were done on the central portions of the medium resolution images, and these craters are on the edges of all the images in which they feature (that I have found at least).

Now let’s see how the selected portion of these craters compare from the various sources. The Apollo image is below left, the LRO below centre, and the LO is below right.

The figure below shows the comparison of the LRO view (left), Apollo (centre) and LO4 (right).

Thanks to the use of a high resolution LO4 photograph, the 4 larger craters can just be made out (see the red arrows), but as before the finer details are lost.

By contrast the Apollo view shows many of the much smaller craters visible in the LRO, demonstrating once again that Apollo photographs, even when taken from orbit, show much more detail than was available at the time to people planning the missions. The only way this could have been possible was to actually have the photographers where they were always claimed to be, and not in a studio on Earth.

Apollo 13 did take photos from orbit around the moon, but not ones that show any great detail, so the next photograph we choose is from Apollo 14, AS14-72-9997. Once again we don’t have a high resolution Apollo image to use. The photograph shows an area 15 km wide just north of Ganskiy crater on the far side. We just miss out on a high resolution LO2 image, so we have to make do with a medium resolution one.

I’ve zoomed in on a small area of the Apollo view, and we’ll see how this compared with LRO & LO2.

Again the LO2 image, despite being only a medium resolution, does a respectable job of picking out the broad details, but the Apollo view (centre) shows much more, and more importantly more features that can be seen on the LRO view.

Moving on to Apollo 15, I’ve selected a photo that shows a crater that is just about visible from Earth, but only from the side, as it can be found on the lunar limb. The photograph is of a small crater north-west of La Perouse, and is of interest because it is partially filled with landslide debris.

The image in question is AS15-81-10906. Once again we originally only had a low resolution view to use but the Flickr archive furnished a higher quality scan. The image covers an area 15 km wide. We’ll look at just the crater, which is just over 3 km wide. A high resolution view of the crater does exist from LO4, but unfortunately it is from quite a high altitude, so that while the crater is easily identifiable, the detail is low.

This time, the Quickmap site does not give a good image of this crater (too much is in shadow), so I’ve found a different one (from image M152383525LR) that shows more of the landslide area inside it. Japan’s Kaguya view is on the far right.

So, how do the Apollo (centre left), LO image (centre right) compare with the LRO one (far left) and Japanese one (far right)?

Well, for once the LO image isn’t too bad. There are differences in shading and orientation, but many of the craters visible in the Apollo and LRO images can be identified with little difficulty.

What happens if we zoom in a little more, sat on the largest of the craters?

At first glance it looks like we may finally have found a LO image (centre right) that matches an Apollo one for detail, but are first impressions deceptive? The LRO version is on the far left, and Kaguya on the far right.

This time the LO does show a good match. Just for once, Apollo and LO are in almost complete agreement, but it has to be said that the are quality issues with the LO view, as well as very obvious lighting differences.

There is no denying that in some areas the LO photograph exceeds the Apollo image in terms of quality. For once, we have to concede the point - in this one image it is possible that a Lunar Orbiter photograph could have been used as the basis for an Apollo orbital image, once the people faking the mission had completely redrawn every crater to allow for lighting differences. Where this falls down is in the overexposed areas of the LO image, particularly the relative young impact crater below centre.

If we zoom in a little closer on this overexposed crater, we can see that the Apollo image reveals details that are comparable to a close-up LRO version, but Lunar Orbiter falls short. Japan’s Kaguya image on the far right is a late addition, and while most of it is in shadow there is still a wealth of detail around the crater rim that corroborates the Apollo view and confirms that the LRO view is accurate. The LO shot has hardly any detail.

Several Apollo images exist of this crater, including similar, but less clear, oblique views from the Mapping Cameras of Apollo 15 and  Apollo 17. The best image for Posidinius is, however, from magazine 91 of the Hasselblads, and this is an excellent magazine to use because it contains not just images of the lunar surface, but also shows parts of the Apollo ship itself and several images of Earth at the beginning and end of the mission that can be dated very accurately using weather satellite images.

The image itself, AS15-91-12366 is shown below, together with the best of the LO images - the H1 frame from image 86 taken by LO4. As usual I have used the highest resolution version of the LO photograph for any actual analysis.

OK, so it’s quite a big crater, so let’s split it up into more manageable chunks. The first bit to look at is the little wriggle of rille that is at 9 o’clock on the Apollo image heading from from just inside the crater to the crater wall. In order to make the images more directly comparable, I have stretched the LRO oblique image (right) so that it matches what we can see in the LO4 (centre) and Apollo (left) views.

The LO4 image does show the broader features visible in LRO and Apollo photographs, but once you look beyond that it doesn’t take craters and other objects to get much smaller before they disappear from LO4’s radar. Also very noticeable are the mottling effects on the crater rim that aren’t there in LO4.

Now let’s look at the large crater within Posidonius, captured not quite in its entirety by Apollo and LRO. As before, the LRO view has been stretched to make comparison easier

While there aren’t many craters around this one, there is plenty of mottling within it that matches the crater, and subtle markings around the rim, that are very obviously there in the Apollo and LRO images but not the LO4 one.

For the next crop I’ve zoomed in a little further (hence the larger arrows - they’re actually the same size as the previous ones in terms of pixels used) on a small range of hills along the rille that divides the crater.

Lack of space prevents the inclusion of the zoomed Lunar Orbiter view, but trust me it does not show the level of detail that the others do. Once again Apollo provides details you can’t see in images that pre-date the missions. Feel free to check for yourself.

Another point to make is that the viewing angle of the crater here is not one that could be achieved from Earth - it’s looking obliquely from the north, whereas from Earth you would only be able to look at this from above.

We could go on, but there are other photographs to look at.

Could these details have been seen from Earth? Well, I haven’t seen any photographs showing them, and the Apollo view is taken from an angle that can’t e replicated from Earth and also sits amongst photographs that prove when and where it was taken: orbiting the Moon.

For Apollo 16’s choice we are fortunate in having a magazine containing precisely datable images of Earth (see here) as well as views of the lunar far side. The candidate for this mission is AS16-118-19002, which is available as a low resolution version and more recently a high resolution one at the Project Apollo Flickr archive. It shows a fairly bland selection of craterlets near Green crater, although the largest crater seen does have some distinctive markings that should help us. There are also several areas with distinctive craterlet patterns.  There is coverage of the area from an LO1 image, but we just miss out on a high resolution version.

The two images are shown below, with AS14-80-10468 (left) from the centre of the crater and AS14-80-10511 (right) to the west.

What we can do now is, as usual, see how the LRO view (using screenshots from the quickmap viewer) compares with the Lunar Orbiter view, the best of which is from Lunar Orbiter 4: 4084 H2. We’ll show them in the same sequence, 10468 on the left and 10511 on the right. Orbiter first:

Now LRO:

The Chinese data are not of a high enough resolution to match the LRO, but they can confirm that there are features in the Apollo images not visible in the LO4 views. Japan’s data certainly confirm what we are seeing as genuine.

As far as the LO4 image, as usual there is a superficial similarity, but once fine detail is examined, the LRO images are far superior, and show, as usual, that the Apollo image contains a high level of detail that could not have been known about in advance.

By way of demonstration, let’s zoom in a bit. The first image below is a comparison of the well defined small crater just to the right of centre in AS14-80-10468. Japan’s view of the same crater is shown on the right.

The amount of detail present in the Apollo image is indeed impressive, and none of the rocks or craterlets visible can be seen in the LO4 image. Japan’s relatively low resolution view of the same crater can still pick out features visible in the Apollo image. Just to prove a point, here’s a close-up of the crater on the centre line at the right of the image. Japan’s view is again shown on the right.

Again, an impressive level of detail from a camera being flown on a manned Apollo craft above the lunar surface that shows details not photographed again for decades, and certainly not known about in advance. The Japanese view is included for consistency, but is not as helpful here thanks to brightness of the sun’s reflection. The smaller craters on the periphery can still be made out, however.

We can even check some of the images in the Preliminary Science Report against Chandrayaan, as some of the ones in there overlap what is available from a totally non-NASA source. The images from the PSR aren’t of the highest quality, so it will be interesting to see whether they still out-perform the LO4 images.

The screenshot below shows the orbital path of Apollo 14 on Google Moon, and superimposed on that we have the PSR images available to us. The ones we’re going to focus on here are those that sit on Chandrayaan images, which I have also superimposed over the western and eastern rims of Theophilus.

While the resolution of Chandrayaan’s image is not as good as either the LRO or Apollo photographs, it is still possible to make out the craters that Apollo imaged in greater detail than the original Lunar Orbiter probe did. So you can’t just say “oh it’s all NASA it’s all NASA” like some demented moronic parrot, because India confirms that Apollo’s data are correct.

We can look at another non-landing mission for our next piece, Apollo 10. In this mission, I’ve picked out AS10-35-5195, for which we don’t even have a high resolution version.

It’s usefulness, however, is that it is of a quite nondescript, bland little crater, Benedict, part of the larger Mendelev crater, again on the lunar far side, and more importantly that the photograph is sandwiched between several Earthrise views, which again can be precisely dated (see here). The Apollo image covers an area roughly 30 km wide.

Despite much searching, I have only found a few distant views of Mendelev crater, and the best one (for now) is this one from LO1. This frame does have high resolution coverage, but not of Benedict crater.

Again, there is a wealth of fine detail in the Apollo view that is matched by the LRO and even by the lower resolution Japanese image.

Now let’s look at 10511, using the brighter crater in the bottom left:

And also Chinese views of the same areas:

I’ll start on the eastern rim, and I’ll ignore the two images that only get a partial overlap. Of the two that sit inside Chandrayaan’s image footprint, the first one taken is AS14-80-10441. This is shown below (centre) compared with the Chandrayaan view (left), Japan’s (centre right, this time the ‘evening’ view to show the craters on the slopes) and the LO4 version (far right) of the same spot.

It really does not take a genius to work out that the view presented by a poorly photocopied low resolution scan is still much better than what was visible in the LO4 photograph, much of which shows this area in shadow. Not only that, but the Indian satellite’s photograph if the same area shows a wealth of detail that can also be found in the Apollo 14 photograph. The only feature than can be identified with any certainty in the LO4 view, other the broad outline of the ridges, is the shallow crater on the main ridge line just off centre.

The next image, AS14-80-10448 has two different versions open to us. The first is the same size as others in the PSR, but the second is a cropped version of it, and it is cropped to focus on a specific feature. The feature in question is a boulder trail, and it is specifically referred to and discussed in a document that was published, let’s not forget, many decades before any other probes went and photographed the same area in detail.

To save time, I’ll just focus on the cropped version of the photograph as it is more detailed than the larger one, and again it’s shown with the LO4 version (from 4077) to the far right and the Chandrayaan view to the left. Japan’s view isn’t of high enough resolution to show the boulder trail, but is included to show that it still reveals other details not visible in the LO4 view.

The arrows labelled ‘1’ and ‘2’ on the Apollo photographs mark the path of the boulder and the boulder itself respectively.

As before, it should be clear that even a low quality scan shows an exact match for Chandrayaan’s view of the scene, and the LO4 has nothing to offer other than a broad hint of lunar surface morphology. Is it worth a closer look at the Apollo and Chandrayaan photos just for fun? Of course it is:

Could it be more conclusive? You can pick out the rocks and the boulder trail, and a probe from India confirms what sane people knew all along: Apollo went to the moon. We can make it even more obvious by using an image from the real PSR, not an online one, as I now have my own copy. I’ll even include a photo of the page to prove it:

The LO4 view is slightly better lit this time, and a few of the larger craters can be made out. In contrast, there are many smaller rocks and craters visible in the Apollo reproduction that can be made out easily on the Chandrayaan and Kaguya shots. Again, let’s zoom in on an area to show this more clearly.

Isn’t pareidolia wonderful?

So, the next time some hoaxer idiot tries to claim that there is some conspiracy to hide images, tell them they’re wrong, and that even if the only copies out there are poor ones, they still have enough information in them to prove that Apollo happened, and that it can be verified by satellites that aren’t American.


So, after picking photographs from all the missions, taken from the lunar surface and in orbit, what can we reasonably conclude from this exercise?

The main thing is that wherever there is an identifiable surface feature photographed or filmed by Apollo that falls within the optical capabilities of the LRO, it can be found in an LRO image.

We have to concede that there are some areas where the Lunar Orbiter data are an equivalent to the LRO images, but for the most part the fine details in Apollo images don’t appear in Orbiter photographs. The fine details that do appear are arguably more a product of modern techniques of reproducing the LO images.

NASA themselves did a comparison of Orbiter and Apollo photographs after Apollo 8, as reported in the Analysis of Photography and Visual Observations. Those carrying out the comparisons felt that Apollo photographs had much better quality and dynamic range, allowing smaller features to be identified - particularly in areas where sunlight added glare. The lack of a mosaic effect from the ‘banding’ produced by the scanning process made for clearer images, and stereo imaging allowed much better mapping and photogrammetry.

They also concluded that, good as Lunar Orbiter photographs were, Apollo photographs were better. Only with the introduction of the LRO’s superior cameras did the features photographed by Apollo come to be photographed again. In fact, the images were so good they replaced Lunar Orbiter images altogether for some training exercises in Apollo 10 (Apollo 10 Photography Report). Likewise the Apollo 10 photographs were also much more useful in seeing smaller feature and deriving measurements of slope angle and other mapping processes.

For the hoax proponents to be correct, every single inch of the LRO’s surface coverage that was photographed by Apollo would have to have been gone over and manipulated to make sure it matched with an Apollo view, because you never know when some other country might put a probe up there that will prove it all fake! This would also apply to the many areas that only recently have been identified from Apollo photographs. There are a number of Apollo photographs whose locations were not known and were simply left as unidentified by the original cataloguers. It was up to enthusiastic amateurs (like myself) to identify the locations of those images. How could they fake them if they didn’t know where they were taken?

Most hoax proponents will just arm wave away this research - I’ve made it up, it’s all lies, NASA hides everything etc etc blah blah. I’ll no doubt be accused of manipulating photographs, so I’ll put that to bed now - I have altered nothing apart from brightness levels and added the occasional bit of sharpening, and I have done this in all photographs, including the LO ones. I’ve always used the best example from the LO collection. I’ve not fiddled it to make sure that I picked areas without good LO coverage - I always picked the Apollo image first, then found the photos to match. Besides, if it was all fiddled, wouldn’t NASA have fiddled with data they had, rather than risk getting caught out?

The simple fact is that we went to the moon, and the reasons that the Apollo photographs match the LRO views is because astronauts were on the moon. That’s it. They could not have produced anything on a lunar set on Earth, because they did not have the detail available to do that. They did not manipulate the photographs once better images came along, because they had already been published and were freely available for sale (don’t believe me? Check out the back of those photography reports).

The morons who refuse to accept the evidence of their own eyes will just have to deal with it, their hoax theory just took another battering.

If you want to check things out yourself, then you should go look at:

India’s images (needs registration).

Japan’s images.

China’s images

For one final look at orbital images we stop looking at Hasselblad views and look instead at two of the images taken by the Hycon Lunar Topographic Camera. This was carried on Apollo 13 and 14 and was intended to be used at relatively low orbital altitudes (10-12 nautical miles) to image at very high levels of detail. Apollo 13’s were not done for obvious reasons, and Apollo 14’s intended high detail survey of the eventual Apollo 16 landing site of the Descartes highlands was curtailed by the camera’s malfunction.

In the end, only two magazines were exposed early on in the mission, and only one of those contained images that were of any use (magazine W). Of the 200+ images that were taken over Theophilus crater, only a handful have been reproduced in with any degree of quality in the Preliminary Science Report, and also in this report. Most of magazine W can be found in low resolution in the Photographic Catalog. Only two high resolution images are currently readily available online, ironically on UFO websites as they supposedly contain some sort of flying saucer or other. Two others emerged after this page was written and they are discussed later.

To give an idea of how small an area these images cover, here they are in context on Google Moon, each one covering an area roughly 5.5 km by 4.5 km.

To complete the picture, let’s now head over to the other side or the crater. Here there’s only one image from the PSR that is covered by Chandrayaan, AS10-80-10490. As before I’ll show it in comparison with the LO4 coverage (this time from 4084) of the same area on the centre right, Chandrayaan on the left, Japan on the far right.

And we can do the same as before with one photographed from my own copy of the PSR:

The LRO view taken from the Quickmap link has quality problems of its own, and is a composite of several passes, but the inner markings are clear enough to see, as are several smaller craters around the rim. The Apollo image (on which I have changed brightness levels, and stretched to compensate for the oblique angle) even as a low resolution copy shows features that can be identified as appearing on the LRO view. It would be interesting to see how a high quality print of the photograph compares.

By contrast, the LO image shows hardly any detail, and even if it did, the western half would show nothing at all as it is in shadow. It would be interesting to see if a high resolution pass exists, but as of the time of writing I have not found it.

As it happens, sometime after this page was originally written, higher quality scans of the Apollo image did appear at the Project Apollo Flickr Archive, and Benedict crater is big enough to show good levels of detail in Japanese (below centre) and Chinese (below right) images. The higher resolution Apollo image is shown below left, and is again stretched to match the overhead views of the probes.

Moving on to the next mission.

Apollo 12’s photographic record is not the best. The bulk of the orbital images are in a couple of continuous transects, and relatively few are far side vertical shots.

So, let’s be brave. Let’s pick one from the near side. The smallest area covered is that on AS12-52-7448. It shows a small but bright crater south of Kepler crater. The image is 25 km across, and the crater itself is about 10 km across. This time we have a high resolution image from LO4 to use, which is nice, but we also have a high resolution image from Apollo 12, so once again we’ll focus in on the details to see how we get on.

Again, at the risk of repeating myself, the Apollo photograph (especially the high resolution one) reveals remarkable detail of this crater, details that are clearly seen in the LRO and Japanese views and which are not seen at all in the LO4 picture. A high resolution LO4 image taken from a lower altitude may well have revealed more detail, but there isn’t one, so how did Apollo get that photograph?

By being there.

We can do some more work for Apollo 15 thanks to this website, which produced a beautiful oblique image of the crater Posidonius. This image is shown below, and has been inverted to show the correct view. The full size and uninverted image is here.

What happens, as usual, is that the superficially detailed image from LO1 becomes much less useful in identifying surface features. The Apollo photograph, on the other hand, contains a wealth of detail that is replicated exactly in the LRO image (which is from Quickmap and now uses a more detailed layer). While the Kaguya view is partially in shadow, there is still enough there to corroborate the Apollo and LRO view, Once again even low resolution orbital images taken by Apollo show features that it would take another 40 years to reveal to new cameras.

Granted a skilled interpreter could have deduced the size of the crater floor from the arrangement of the shadows, but in the absence of any other detail they could not have predicted the distribution of material in the crater, and the pattens of light and shade this produces. I would argue here that, good as the LO view is, a higher resolution Apollo image would have wiped the crater floor with it in terms of the level of detail revealed.

For the final mission of the Apollo lunar landings, we have a photograph taken of the centre of Marconi crater, AS17-149-22833, covering an area again about 25 km wide. While we only originally only had a low resolution Apollo photograph the Flickr Archive supplied a better one. We do at least have a high resolution LO1 image, albeit from relatively high up. The Apollo magazine also contains datable views of Earth (see here) as well as images of the LM returning from the lunar surface.

As with so many others, there is more detail in the Apollo view than it seems. Even a poor quality reproduction of an Apollo scan contains more information than was available during Apollo, and this is proven by a satellite that has nothing to do with NASA. The use of better quality images improves the level of detail, and the level of proof, even more.

In a later development on the HYCON images of Theophilus, a small amount of detective work did unveil a source for new images of the crater. Specifically, they are the 4 photographs currently missing from the Photography Catalog hosted by ASU and linked to above.

Prior to their appearance, the only source of the missing photographs was from low resolution poor quality reproductions of what appear to be microfiche images. These images are definitely from the same copy of the catalog at ASU, despite attempts by the person who posted them to hide the fact.

The claim appeared to be that because these images were missing there was a grand conspiracy, the point of which was never entirely made clear.

The 4 new images are shown below top right, along with top left the Chandrayaan views of the same area, bottom left by the poor quality microfiche copies, and bottom right Japan’s Kaguya photographs.





I think we can agree a couple things here.

Firstly, the quality of the photographs sent to me are far superior in quality to those hosted by the website that first claimed to discover them, and are also of better quality than the images in the Photography Catalog. They are not just missing pages from the catalog, as evidenced by blemishes in AS14-80-10443 on the strip across the image that are not shown in the poor quality scan.  The strip of tape may be a fault in resulting from the camera’s documented problems, or from the development process, but I believe it is more likely to be a strip of tape holding two halves together, which would suggest that the image in the catalog is the same one scanned for this page.

Secondly, the images are undoubtedly on the moon, and undoubtedly show details not visible in other pre-Apollo views. Indeed, given that the main conspiracy claim for these 4 images is that they have never been publicly available, you have to wonder just how they go the details so exact.

Just for the sake of completeness, let’s look at the LRO view in a small area on the centre left of AS10-80-10442. I’ve rotated the Apollo photo to match the true orientation, and altered the brightness slightly to bring out detail. The sequence below is Apollo (left) LRO (centre left), Chandrayaan (centre right) and Kaguya (right).

The scanned Apollo image is starting to lose the ability to resolve any more detail at this resolution, but it is still very obviously a match for what is visible in the LRO and Chandrayaan views.

In a late addition to this page, two more high resolution copies of Magazine 80 images were discovered in the US National Archives site, namely AS14-80-10456 (below left) and AS14-80-10500 (below right). A red square on each identifies an area examined in more detail subsequently.

As you can see, the only pre-Apollo view of Saenger Q is poor, and shows none of the details of the crater floor or the striping of the crater walls. Even though the Chinese and Indian probe images are relatively low resolution (they are not the full quality images from their websites), we can still see a good amount of detail.

Now that we know what foreign governments have done in terms of imaging this quiet little backwater, let’s look at what Apollo has seen from orbit. The first shot is from Apollo 10, AS10-29-4224. The magazine this came from also contains an image of Earth that can be dated precisely, so we know for certain when it was taken. Here’s a close up of Saenger Q from that image.

The key feature here is the dark stripe running vertically from the crater floor to rim. We are looking north-west across the crater, and thus the corresponding line in the Indian and Chinese view is at a different angle, but it is most definitely there. It can definitely not be seen in the LO2 image.

A couple of months later, Apollo 11 flew over the same area, and while there are a few images of crater Q the best come from the sequence showing the LM ascent module returning to meet Michael Collins in orbit. This sequence ends with photographs of the Earth rising above the horizon, and again these can be dated exactly. The image we use here is AS11-44-6627, shown below.

It should be obvious that the crater is both the same one featured in the Apollo 10 view, and is the same one pictured by Chinese and Indian satellites.

Different orbital parameters for subsequent missions meant that Saenger would not be revisited until 1972 and Apollo 16. We have an excellent image from that mission that again can be dated exactly: AS16-120-19187.

The oblique angle of the image means that only areas shown by China’s probe are visible, and I’ve added some markers to help with identification.

Apollo 16 also saw the use of high resolution mapping and panoramic cameras, and we have a couple of examples covering Saenger Q that allow comparison with the better quality Chandrayaan shot. The images used are AS16-M-0906 and AS16-P-5056.

The only differences that can be be made out here are those resulting from the angle at which the images were taken. It is completely undeniable that the Indian probe’s view (left) is showing the same crater details as those from the Panoramic (centre) and Metric (right) cameras. These details are totally absent from the LO2 image.

Apollo’s final visit to Saenger features it in a couple of magazines, but the most useful one is Magazine 151, as again it has images of Earth that allow exact dating of the photographs. The image used here is AS17-15-23224.

As before, the stripes and mottling on the crater walls, and the markings on the crater floor, are clearly identifiable and are an exact match for those of the Chinese and Indian photographs.

Again, we have an exact match with our Asiatic satellite sources.

As with Apollo 16, we also have Panoramic and Metric images showing Saenger Q, and two examples have been chosen to represent them, AS17-P-2540 (centre) and AS17-M-0886 (centre-right). Chandrayaan’s view is shown on the left, and just for luck Japan’s view is far right.

And again, unsurprisingly, we have photographs taken by an American camera in lunar orbit that exactly matches a photograph taken by an Indian probe in lunar orbit. Conspiracy theorists well desperately cling to the notion that this is because China, and Japan, and India, and whoever, are all in on it together, but the real reason is much simpler and more obvious: they were all taken in lunar orbit. None of the details in this crater were known about prior to Apollo.

Oh, and just for fun and to keep the UFO nuts happy, here’s what you get if you zoom in really close to the LRO view of the crater (right), compared with the Panoramic image (left): a giant alien stone man sitting on a throne talking to some minions:

I don’t think we need arrows to show that the Apollo image shows exactly the same features as the Chinese and Japanese photographs, and that those in turn are a match for the LRO view.

Seeing as we’ve started with a crater per mission we may as well continue. The bulk of Apollo 11’s photographs are concentrated on the near side, and relatively few are on the far side. Picking an image at random gives us this one, AS11-42-6347. It shows a small double crater north-west of Vening Meinesz, east of the Mendelev crater used earlier, and the image covers an area about 25 km wide.

This time we do have a high resolution image to play with, so let’s zoom in and use a much smaller component of that photograph, outlined in red.

Japan has a contribution:

While the Apollo image is starting to degrade in terms of what it can show us relative to the LRO view, it still shows considerably more detail than the LO4 photograph - particularly in terms of the bright patches on the hills alongside the rille.

A later addition to the data archive is the availability of Japanese images, and the Kaguya versions of the three areas are shown below. Draw your own arrows -if you do you’ll come to the conclusion that the Japanese data are an exact match for both the LRO and Apollo photographs!

Enough said.

For one final look at orbital images we turn to one individual crater that has been imaged many times: Saenger.

Saenger is a far side crater whose shape and secondary cratering makes it easy to pick out. It also benefits from having been imaged by both Chandrayaan and Chang’e-2. In the images below you can see the Indian (left), Chinese (centre) and the best LO shot available of the crater from LO2 (LO-2-0196). We are focusing specifically on the sub-crater, Saenger Q, at the northern end.

Let’s cut to the chase and look at the areas inside the red square, firstly the one on the left above, which is compared with the LRO (centre) and Japan’s Kaguya probe (right).

You have to admit the Hycon camera is pretty impressive, with nearly every detail shown in the LRO image captured by it. Japan’s probe does less well, but confirms the broader detail. This crater shows what reports linked to earlier describe as a prominent bright peak. Let’s get even closer in:

As before we have a truly impressive level of detail from the Hycon, with features as small as 2 metres across easily visible.

How well does the Lunar Orbiter show these features?

The area covered here is 165m across.

Case closed.

Now for the other one:

Another Apollo 15 image comes courtesy of postings by another conspiracy nut, although this one at least thinks gthey went to the moon (just that the moon is an artificial object). The poster in question linked to AS15-97-13288 claiming it showed a dome, which it just bloody doesn’t - it’s Sosigenes crater, with its associated rimae. As luck would have it there are some excellent articles showing the rimae and craters here and here that show some very clear images taken by the LRO. Let’s have a look at the Apollo image, below left, and also zoom in on the feature in the centre (below right):

What we can do now is compare the detail in the Apollo image with that in Japanese (top left), Chinese (top right), LRO (bottom left) and Lunar Orbiter images (bottom right):

Superficially the Lunar Orbiter image does a decent job, so let’s go in further to be sure. Here we have Apollo (far left, stretched to compensate for the viewing angle), Japan (centre left), China (centre right) and the LRO (far right -taken from a low resolution version of the image)

In yet another development, a large print copy of AS14-80-10503 was contributed by Apollo image collector Apollo 16 UVC S201 in the form of AS16-123. The high resolution copy can be found here. A copy of this image is shown below together with its low resolution version from the Apollo catalog and Chinese and Japanese versions of the same area.

Now let’s have a look at the copy recently unearthed

And here’s how the best view from Lunar Orbiter looks.

Even Apollo 11’s TV images are better than Lunar Orbiter. No sooner had they settled into lunar orbit than they began a broadcast. It started over the far eastern edge of Mare Smythii, showing craters like Haldane and Schubert in colour and from an angle not possible from Earth. One of the craters they filmed was the one sown below, close to Hume crater. It’s shown here with a Chinese (left) and LRO (right) comparison:

This is the best view of the crater seen by Lunar Orbiter.

It’s close, I can give it that, but the fine detail of the ray pattern in and around the crater is missing - detail that is particularly visible under the sane lighting conditions in the Chinese photograph. Also noticeably absent are the numerous small bright craters.

There are some, but not all of them can be seen.