The Hyades and Pleiades Clusters imaged with the Sony α68 DSLR

I think that it’s fair to say that Sony have been concentrating on their mirrorless cameras over the last few years (see article about the Sony A 5000) and their APSC sensor DSLRs have not been upgraded for some time. They use a fixed, partially reflecting, mirror to allow light to fall on the array of autofocus sensors above.  This reduces the light falling on the sensor by ~1/3 stop − so one might say that they would not be suitable for astrophotography use.  Some have thought that the fixed mirror in the light path might affect the stellar images but I think that the imaging exercise described here shows that this is not the case.

[At the end of the article, is a description of the two current Sony APSC cameras including the A68, 24 megapixel, camera employed for this exercise. They do have some interesting features not found on the Cannon or Nikon DSLRs.]

On the morning of the 2nd October 2019 the sky was transparent and there was no Moon so, in the pre-dawn sky I decided to do a test with a second hand (but nearly new) Sony A68 DSLR that had arrived the previous day.  It was mounted on my StarSync tracker (see article ‘Three Tracking Mounts’) which was aligned on the NCP using a laser pointer.  The Sony sensors are ISO invariant (*), and using a low ISO can sometimes give better results than higher ones and so the ISO was set at 100.

(*) In the past I have tended to use ISO 800, but this was an experiment which, as the result showed, seemed to work well. I have written about this in the article ‘What ISO to use for Astrophotography’.

An f/1.8 50 mm prime lens was used, set to f/3.5 to give better stellar images than at full aperture, and a total of 24, 30 second, frames taken before clouds intervened.  The camera was controlled with an external interfervalometer.  Jpegs were captured which might limit the quality of the result, but when many Jpeg frames are stacked, one effect is to increase the effective bit-depth of the result and the use of Raw capture may not have made a significant difference.

These were stacked in Sequator and the 16 bit Tiff result loaded into Photoshop.  Now that LED street lighting is employed locally, the light pollution is less than it was.  The stacked image had a blue cast rather than a red one as dawn was not far off. 

As usual, the image was duplicated and the stars in the upper layer were removed using the ‘Dust and Scratches’ filter in Photoshop.  (I have described how this can also be achieved using GIMP – see article ‘Removing Light Pollution in Photoshop and Gimp’.)  The two layers were then flattened using the ‘Difference blending mode’ to give the result below.   As ISO 100 had been used, relatively few stars were visible, but as the noise level in the image was so low, it could easily be stretched to bring out the fainter stars.

The image was stretched using several applications of the ‘Levels’ command with the middle slider moved leftwards to 1.2.  This brightens the fainter stars more than the brighter ones.  A final levels application was used to bring up the ‘Black Point’ using the left hand slider to remove the noise from the image. 

Digital images tend not to make the brighter stars stand out so an image of the brighter stars only was made by moving the black point (left hand slider in levels) to the right.  These were made ‘larger’ by applying a little Gaussian Blur and their brightness brought back using the ‘Brightness/contrast’ tool. 

These ‘brighter stars’ were added into the stretched image above using the ‘Screen’ blending mode to give the final result at the head of the article.  The image quality of the camera/lens combination cannot be seen in the full, much reduced, image so, below are two 50% images.  Though I bought this camera for landscape and video use, I do really think that it is suitable for wide-field astrophotography. 

Hyades Cluster and open cluster NGC 1467 above.


The two current models, the α77 II and the, lower priced, α68 cameras do have some good features for general use.  The fact that the mirror does not have to move each time an image is taken allows for a very fast burst rate which can help in capturing the ‘decisive moment’.  This also allows focus tracking when taking video sequences, so it does have its merits.

In contrast to Nikon and Canon, they include in-body image stabilisation (IBIS) – which could allow somewhat longer exposures to be made so compensating for the slight light loss due to the fixed mirror.  They have two useful modes to increase the effective dynamic range of images.  In this case  one should expose the scene to preserve the highlights.  In the first mode, its allows five adjustment levels to increasingly lift up the darker regions of the image whilst in the second, a true HDR mode, the camera takes two rapid exposures and combines them to give the final image.  The camera can align the two images even if the camera is hand held.  The former method, assuming it uses the raw data captured by the sensor, should give a lower noise level in the dark areas than if, for example, the ‘shadows and highlights’ tool in Photoshop is used to lift up their brightness in post processing.

Both cameras employ Sony Exmore 24.2 Megapixel sensors and the same Bionz X processor so the image quality should be very similar.  Both use, as they must, electronic viewfinders with that of the α77 II having a higher resolution and this camera also has a larger, and higher resolution, rear screen which in both cases can be tilted away from the camera body – good for astrophotogaphy as it allows better cooling to the rear of the camera and may make it easier to frame objects at high elevation.

As Sony cameras with A-mounts are less popular now, I have been able to acquire prime lenses at quite low cost for my previous A450 camera.  As Sony took over the A-mount from Minolta, Minolta lenses can also be used.