The biggest obstacle to taking clear images of the Moon and planets is Earth's turbulent atmosphere, which causes a heat -haze like effect. Astronomers use a technique called lucky imaging to overcome this. A video is taken of the target and stacking software used to identify and combine the sharpest frames. This makes it possible to recover detail impossible to see in the source video or at the eyepiece.

The image above was taken with a 12" dobsonian telescope with a 2x barlow lens, giving an effective focal length of 3,000mm. For comparison, a very large telephoto lens might have a focal length of 600mm, one fifth the magnification.

AutoStakkert 3.1.4 was used to analyse and stack the source video. As well as the atmospheric turbulence it was able to cope with some uneven motion from the telescope as it tracked the target crater imperfectly. 

So why doesn't technique this work with CCTV footage? If the subject stays quite still it is possible to recover a bit more detail by combining frames, but this won't work if they are moving. Also, the quality of any image is constrained by the size and quality of the optics, and the image sensor.  A small lens and cheap sensor produces images with limited resolution even under the best conditions.

Copernicus crater, on the near side of the Moon, is 93km across and 3.8km deep - not quite big enough to fit the county of Cornwall inside it. It's a relatively young crater, thought to have excavated by an impact some 800 million years ago. It's surrounded by a visible system of rays pointing outwards, lighter materiel that was ejected and that still lies on the Moon's surface.

The best place to photograph it is from Lunar orbit rather than the surface of the Earth, 360,000km away, but that's not an option for most astronomers. These two spectacular images were taken during the Apollo 12 mission.

The montage shows the progression of the September 2015 lunar eclipse over a period of about two hours, as Earth's curved shadow passes across it. Unusually, this eclipse coincided with a so-called supermoon, where the full moon is at the closest point in its orbit and appears slightly larger to the eye - such an event will not occur again until 2033. At totality the Moon is still visible as some sunlight still reaches it by passing through the Earth's atmosphere. However, it appears much dimmer and redder than normal - at a second the final exposure in the sequence is 1,000 times longer than the first. The deep red colour is caused by the same phenomena that makes our sky blue - our atmosphere scatters blue light more readily so that more red light reaches the Moon's surface, and is reflected back to Earth.

Taken by Ken Bennett, with the aid of a 5" refracting telescope, DSLR camera and some choice Cornish cursing-words.