> Some astrophotography myths busted
Reading a new product that claims to be 100x time more powerful then conventional telescope, I realise that this is just an astrograph with a digital camera that is doing stacked images and show them trought eyepiece or App. So what we can expect from this instrument is something that I already do, but it is put together in one compact place and added connectivity functionality that can contribute to scientific projects.
It has diameter of 114mm and f3.9 and small Sony Xmor sensor IMX224 with high QA. https://unistellaroptics.com
This instrument reminds me that some myths are already busted due to improving architecture of the sensors:
1. The larger the pixel size is the more QA and more light sensitive the sensor is:
This is no more so true as latest sensors are back illuminated and also have microlenses to collect all the photons that hit the sensor.
Old CCD architecture was commonly build interline and this rule was true for them. For example APS-C 10Mpix CCD of Pentax KM has less QA then same size CMOS of Pentax K5 with 16Mpix.
This improvement is especially visible in the recent mobile camera market development.
2. The larger the sensor is the better:
This is true when we want to have a wide filed images but in most cases it is better to have a smaller sensor with higher pixel density and to use it on a faster telescope. The faster telescopes from other site has more compact and lightweighting design. In such way we can also collect faster the data we need or to collect much more of it. This is so called crop factor and it is a good way to get higher equivalent magnification and details without loosing relative aperture. A f5 telescope is a still f5 instrument no matter what size sensor you will put on it. Of course the atmospheric turbulence and the optics quality are becoming critical with the crop factor increase. But if we need to put additional optics to boost the magnification we will also introduce more aberations and light lost. That is way the DSLR lenses with less elements are better then those with more. For example SMC Pentax DA 18-55 was improved in the past to have 11 optic elements instead of 12.
3. Long exposure is better then short and stacked images:
The staked images eliminates noise issues, guiding imperfections, vibration, even atmospheric turbulence and it increases dynamic range.
4. Limited magnitude for a scope is fixed value that is estimated only by the aperture:
Unistellaroptics claims that their 114mm instrument could see up to 16 magnitude. For visual observation this value is around 14.
With better sensor it could collect more light and detect even fainter objects. So the limit is actually the sky background glow and the integration time we use. Of course the larger aperture we got, the easier is to collect light.
You no more need large sensors and heavy equipment to do good general photos. The recent development of image sensors put silicon chip capabilities to it's limit by
Knowing what you are looking for is more then half way to achieving it. Breakthrough Listen is a SETI kind of project that listen for artificial signals from 1700 nearby stars up to 160 light years.
Some shots from Sofia. A very bright sky place. Zenith sky brightness info (2015): SQM 19.13 mag./arc sec2 Brightness 2.41 mcd/m2, Artif. bright. 2230 μcd/m2, Bortle class 6.
It is very important how you manage your data. So much shots, so much frames. They are full of hidden data that could be revealed later. The far we look the more we see. Each feint dot could be a galaxy far far way.
Nowadays we are so into the globalization and technologies, that I can submit observation plan to a remote, professional observatory at the other part of the word!