Yesterday morning (3rd Dec 2021) Comet C/2021 A1 (Leonard) had a close encounter with the lovely globular cluster called M3. When I say ‘close’ I mean in an apparent way because the comet is in our Solar System and the globular cluster is about 34,000 light years away above the galactic plane!
I took this image with my remote telescope in Spain. It’s quite tricky creating a pretty image of the comet and the starry background at the same time because the comet moved slightly during the 20 minutes it took to capture all the images. This comet was aligned and stacked separately from the stars and then the two images were merged together.
This is the first image I have posted using data from my new remote telescope setup in Spain and it is, perhaps, the ‘deepest’ image I have ever processed. I have only recently taken over this system after I purchased it from First Light Optics who also kindly bequeathed me all their images taken over the last year or so that the system has been in operation. The images used to make up this image were taken over April and May 2021 when M81 and M82, both in Ursa Major, were higher in the sky. The larger galaxy on the left is M81 – Bode’s Galaxy and the smaller one is M82 – The Cigar Galaxy.
M81 and M82 were both discovered in 1774 by the German astronomer Johann Bode who reported his observation to Charles Messier who then added them to his famous catalogue. Both galaxies are about 12 million light years away (which is 114 million million km or 770,000 times further away than the Sun).
Here is the colour image; click on it to see a bigger version. More details follow the image below:
What else can we see in this image? Directly above M81 is a blue patch – you can see it better in the full sized image. This is a satellite galaxy to M81 called Holmberg IX. This is a dwarf, irregular galaxy and based on the observed age distribution of stars it contains it is thought to have formed within the last 200 million years, making it the youngest nearby galaxy known. This would explain the blue colour as the stars within it will be young and hot.
The faint wisps all around the galaxies are all part of the Integrated Flux Nebula (IFN), so-called because it shines by the total (integrated) light of all the stars in our Milky Way Galaxy. The IFN lies beyond the main body of our galaxy, and is illuminated by the whole thing. It is incredibly faint and only recently discovered in 1984 by the IRAS satellite. To show it better, I have stretched the histogram of the luminance channel of the above image even more. This monochrome image is shown below:
For those interested in the technical details of the image acquisition and processing, the image contains a total of 78.5 hours of exposures made up as follows:
112 x 5 minute exposures
112 x 5 minute exposures
98 x 5 minute exposures
287 x 5 minute exposures
83 x 20 minute exposures
The above table shows the actual number of exposures that were used in the integration to make the final image. Many more were rejected because of satellite or plane trails, or thin cloud etc (for example 73 of 360 L images were rejected). All images were calibrated with bias, dark and flat frames and all processing was performed in the amazing PixInsight software.
Here is my latest image from here in Ham, near Selsey. This is the beautiful Iris Nebula (NGC 7023) in the constellation of Cepheus. I took the images last night in a lovely clear, moonless sky from astronomical dusk to dawn. In all, 120 x 5 minute exposures were captured and I only had to throw away three of them because of very bright plane or satellite trails. This time, because there was no Moon, I was able to use the full bandwidth of a luminance filter on the QHY268C one-shot cooled colour camera.
The Iris nebula is an example of a Reflection Nebula. This is what Wiki has to say about these kind of objects:
In astronomy, reflection nebulae are clouds of interstellar dust which might reflect the light of a nearby star or stars. The energy from the nearby stars is insufficient to ionize the gas of the nebula to create an emission nebula, but is enough to give sufficient scattering to make the dust visible. Thus, the frequency spectrum shown by reflection nebulae is similar to that of the illuminating stars. Among the microscopic particles responsible for the scattering are carbon compounds (e. g. diamond dust) and compounds of other elements such as iron and nickel. The latter two are often aligned with the galactic magnetic field and cause the scattered light to be slightly polarized.
So, we can see that there could be diamonds in that dark dust!
Here’s the image. As always, click on it to see a much larger version in a new window.
This image of IC1805 – The Heart Nebula, in the constellation of Cassiopeia, shows what can be done when the Moon is very bright. Generally speaking, it is not easy to image faint deep-sky objects when the Moon is around, but it is possible to be productive by using narrowband filters. It’s not a great idea if the full Moon is also very close to the target, but as long as the Moon is 40 or more degrees away I find I can get reasonable results.
I explained a bit more about the dual-band narrowband filter I have been using with my one-shot colour CMOS camera in this post.
This image is composed of 48, 10 minute exposures over two nights last week. About two-thirds of them were during the night of the full Moon, the rest under an 85% Moon and drifting thin clouds.
As usual, click on the image to see the full-sized version.
The Heart Nebula is an emission nebula about 7,500 light years away. The great astronomer William Herschel discovered this nebula in 1787. Glowing in the light of ionised Hydrogen gas, the signal is strong in the H-Alpha part of the spectrum. The OIII signal is much weaker and since the H-Alpha is mapped to the red channel, the colour is predominately red.
There is a cluster of stars at the centre known as Mellotte 15 and this is shown as a crop from the main image below.
I’m very excited about this! I have finally taken the plunge and now have (or will have in early November) a remote imaging rig in Southern Spain. It is located at the PixelSkies remote hosting facility near Castilléjar in the province of Granada, Andalucia.
The imaging rig itself was originally built in 2020 and owned by First Light Optics, and it was used to capture images for a monthly image processing competition. I learned from Ian King that it was for sale and I couldn’t resist the opportunity to buy this, already proven, setup. Normally, one has to buy the kit and ship it out to the hosting location, all of which takes time, planning and money.
Here’s a picture of the whole system located in one of the roll-off roof sheds. More details and pictures are below.
The telescope itself is a StellaMira 104mm ED2 Triplet f/6.25 APO Refractor (with field flattener) and this rides on an amazing 10Micron GM 1000 HPS mount which has absolute encoders. The detector is a Starlight XPress TRIUS PRO 694 mono CCD camera which has 2750×2200 pixels in a medium format Sony chip. The resulting field of view is 66 x 53 arcminutes at a resolution of 1.44 arcseconds per pixel. To give an idea of what this means, the Moon would fit twice across the resulting images. The picture below shows the CCD camera connected to the telescope.
Also visible in the picture above is the 7-position filter wheel containing Optolong 1.25″ filters. The filters are the usual set of LRGB filters and the three 7nm narrowband filters for HA, OIII and SII. Notice also the Off-Axis Guider (OAG) with the Starlight Xpress LoadStar V2 guide camera siticking out to the right of the filter wheel. The pick-off prism for the OAG is in front of the filters so that unfiltered light always hits the CCD sensor of the LoadStar.
The picture below shows the 10Micron mount more clearly and also the Lakeside Astro motorised focuser. It is, of course, vital to be able to accurately focus remotely and the focus point will vary with temperature during the night, and is also different for each filter.
Also shown above is the mounting plate on top of the telescope cradles which has the red Hitec Astro Mount Hub Pro V4 control box. This has a full USB hub along with software controllable power ports and dew heater controller. This hub allows the cabling to be kept shorter and neater. Without a control hub like this, all the cabling would have to travel down to the PC on the floor and would create potential cable snagging issues as the telescope slews around. Here is a close up of the hub:
Another fantastic feature of this setup is the built-on flat panel. This Alnitak Flip-Flat will allow me to take my own flat-field images without asking anyone to arrange for a flat panel to be balanced on the telescope. This device can be seen at the front end of the telescope and it also acts as a lid for the telescope to prevent dust getting on to the objective lens. The opening and closing of the panel is software controlled as is the brightness of the flat panel. During cloudy nights I can also take bias and dark frames when the panel is in the closed position, but turned off. See the picture below which also shows the wide angle video camera (the red device below the flip-flat). This sensitive camera provides a wide view of the sky, useful for spotting clouds or generally admiring the constellations and the Milky Way.
Mounted on the mount pillar is a small Astromi.ch MBox device. This is a small, self-contained weather sensing device that delivers barometric pressure, temperature, humidity and dew point information with high accuracy. There are other bits and pieces (including the main Windows 10 control PC), but I have described the main components.
In due course I’ll share more information about how I get on with this fantastic system, and hopefully, lots of great images from this dark-sky site.
Finally, watch this video to see the system being assembled a year or so ago.
Following on from my last post with the Andromeda Galaxy, here is another beautiful galaxy which is also part of a group of galaxies known as the Local Group. The Andromeda Galaxy and our own Milky Way are the two largest in the group and this one known as the Triangulum Galaxy is third.
Why the Triangulum Galaxy? This is simply because it can be found in the small constellation of Triangulum – the Triangle! Just about any group of three stars might do, but this particular triangle is found above Aries and below Andromeda.
Again, as with my M31 image, the Optolong L-Extreme filter was used to collect the H-Alpha data which was then blended into the red channel. This enhances the pinky-red regions on nebulosity in the spiral arms of the galaxy.
As usual, click on the image below to see the full-size version.
For the technically-minded, this article shows the equipment used to take this image.
I acquired the images using N.I.N.A. software. I took 72 x 300s exposures with the QHY268C camera for the RGB and 17 x 600s exposures using the L-Extreme dual-narrowband filter to get the Ha data which I combined with the red channel from the RGB. All processing with PixInsight.
Messier 31, the great galaxy in the constellation of Andromeda is one of the most photographed night-sky objects of all, probably second only to the Orion Nebula. Every few years I get an itch to image it again. Most astro-photographers like to revisit old targets once in a while, and this often happens when new telescopes and cameras have been purchased, and this is the reason why I’m having another go at this beautiful object. I showed off my new kit in my previous post.
It is often said of M31 that it is the furthest away object that can be seen with the naked eye. This is an amazing thing when you think about it! This galaxy is about 2.5 million light years away and it is the nearest large galaxy to our own Milky Way galaxy which is not too different in structure from M31 itself. In a dark, moonless sky, M31 looks like a fuzzy blob to the naked eye. Some people say they can also detect another nearby galaxy called M33 – The Triangulum Galaxy with the naked eye. I personally can’t see M33, but it is further away from us than M31 at around 2.75 million light years, so M33 really does represent the furthest thing anyone can see without optical aid of any kind. I’ve asked a lot of people if they can see M33 in a good, dark sky in the UK, but I’ve never found anyone who can, so I’m happy that those photons that left the Andromeda Galaxy when Homo habilis first walked the Earth, enter my eye and are detected by my retina represent the most ancient particles of light that can ever stimulate the human consciousness.
Here is my latest image of M31. Click on the image below to view a much larger version (4000 pixels across). Next, I will describe some more details of how this image was acquired and processed.
Firstly, what are we looking at here? The first thing to realise is that we are viewing this spiral galaxy from an angle of about 45 degrees. If we could fly over the galaxy and look directly down on it, we would see a vast spiral shape. Another thing to understand is that all of the distinct, bright stars in the image are all relatively close-by stars in our own Milky Way – in other words we are looking through a ‘curtain’ of nearby stars to see outside our own galaxy. We should understand that galaxies are vast islands of stars, separated by huge distances of near-empty space. The Andromeda Galaxy contains about a trillion stars (that’s a million, million stars) which is about twice the number in our own Milky Way galaxy. So, you are looking at all of these trillion stars in this image which are too far away to see them individually, so they glow like a huge mass.
What else can we see here? Well, you will see the dark regions in the galaxy. These are huge lanes of cosmic dust which are obscuring the light from stars behind them. Also, if you zoom in to the big image you will see the disk of red regions that glow around the galaxy. Here’s a zoomed in region that shows the red regions nicely. Each of these red areas shines be the light of Hydrogen-Alpha. All of them would be seen as nebulae to any inhabitants of planets orbiting the stars in M31 and any of them could be the equivalent of, say, the Orion Nebula that we see locally here in our region of the Milky Way.
Lastly, there is a bright elliptical blob showing below M31 in the main image. This is a dwarf elliptical galaxy called M110 which is a satellite to M31 itself. We have similar objects associated with the Milky way and they are known as the large and small Magellanic Clouds.
So, how did I create this image? I used the telescope and camera system I showed in my previous post. Over four clear nights in October 2021, I took lots of long exposure photographs of M31. The telescope was guided very accurately by the separate guide scope that was checking the guiding accuracy every 2 seconds throughout the whole time, and instructed the mount to make tiny corrections to keep the galaxy perfectly still on the chip of the sensitive camera. Eventually I had about 22 hours of exposures stored on my imaging computer. By the time I weeded out the poorer frames, I had 10 hours of data from my broadband luminance filter, and about 7 hours of data from my narrowband filter.
The narrowband filter I used was the 2″ Optolong L-Extreme filter. This passes light from both H-Alpha and Oxygen-III sources, both with a passband of 7nm wide. In this image I only wanted the H-Alpha data, so I extracted the red channel from the narrowband images and threw away the green and blue which shared the OIII signal. Then I merged the H-Alpha signal with the red channel from the broadband RGB images. This enhanced the red emission nebulae in M31 beautifully.
I’ll write a more detailed blog about my process next…
Since the early Summer of 2021 I have been building up a new deep-sky imaging setup based around the beautiful and venerable Takahashi FSQ-85EDX Refracting telescope. I’ve always wanted a ‘Tak’ and decided to go for this model known ad the ‘Baby-Q’. The optics are glorious and the focuser is incredibly rugged and can carry heavy cameras and filter wheels.
The idea, eventually, is to turn this setup into a fully robotic system which will be mounted low to the ground and housed in a simple box-like structure with a sliding roof. For now, I’m testing out the system to see how it performs.
Here is a small gallery of photos of the current system. I will add more details about the components below.
Here’s a list of the main components that you can see in the above photos:
Telescope: Takahashi FSQ-85EDX F/5.3 Apochromatic Refractor with 1.01x field flattener.
Mount: Skywatcher AZ-EQ6 Pro
Camera: QHY268C cooled CMOS camera (one-shot colour, full 16-bit)
Filter Wheel: Starlight Xpress 5 x 2″ filter wheel
Guide Scope: ZWO 60mm. Focal length is 280mm, F/4.67
Guide Camera: ZWO ASI290MM Mini mono
Auto Focuser: Pegasus Astro FocusCube2
Power, Dew Heater and USB Hub: Pegasus Ultimate Powerbox V2
Dew Heater bands on both scopes
Windows Computer: Beelink Mini PC (in the plastic box on the ground running N.I.N.A.)
If you look at the photos with all the cabling, you will see a plastic box on the ground below the mount. This contains a ‘headless’ mini PC running Windows 10. Think of an Intel NUC and you will get the idea, but this is a Beelink with an Intel i5 CPU which comes cheaper than a NUC. This computer has all of the software installed to control the rig. I’m using the free N.I.N.A. software here and the little PC is connected to the wireless router I have in my dome just a few feet away. This allows me to use remote desktop from the comfort of my dome, office or house.
The thing that really was a ‘game-changer’ for me is the Pegasus Powerbox which is mounted just below the lens of the main scope. This provides all of the 12-volt power ports I need to run the various bits of kit and also has a USB hub with 6 ports. Additionally it can power and control the heat of three heater bands and can detect the dew-point so that it can intelligently adjust the power to the bands to keep the lenses free from dew. Because nearly everything connects to this hub, there are only two cables that need to be connected to the big plastic box on the ground. One is the 12V power to the hub and the other is the USB3 port to the Beelink mini PC.
I run the amazing free N.I.N.A (Nightime Imaging ‘N’ Astronomy) software on the mini PC and the recently added Advanced Scheduler is amazing allowing me to power up the system before dark and set up various targets to image during the night. The system will do everything such as cooling the camera, auto-focusing, slewing and centring targets, flipping across the meridian and shutting down at dawn. It can also deal with re-focusing during the night if the focus drifts and re-centring after a cloudy spell.
Assuming I get some clear nights over the Autumn months, I will hopefully be posting some new images soon.
The beautiful Veil Nebula in the constellation of Cygnus (the Swan) covers a large apparent area of the sky. When I say ‘large’ I mean it in a relative way. It covers a large enough area to make it hard for the average telescope to cover in one frame. To put this into perspective, the full Moon (or the Sun) is about half a degree across, but we need a field of view (FOV) of about 3 by 3 degrees to encompass the whole of the Veil Nebula. Thus, we can say that the full Moon would fit about 6 times across the apparent span of the Veil Nebula.
I have a lot of different telescopes and cameras! Some telescopes, such as the popular Schmidt Cassegrain design, are good for viewing the planets and small galaxies, but these typically have very small FOVs because they have long focal lengths to provide the high magnification which we need to see the belts on Jupiter, the craters on the Moon, or the rings of Saturn. Think of these telescopes as the telephoto lenses of the astronomer’s toolkit. Then there are the shorter focal length, smaller telescopes. These are the type (typically small refractors) that can give a wider view of the starry sky and they are ideal for delivering a larger FOV on to the camera’s sensor. However, only the smallest of these could cover the 3 by 3 degrees we require, and so I have resorted to the technique of imaging one half of the Veil Nebula on one night, followed by the other half on another night! I used an using an 85mm F/5.3 refractor. The two sets of images are ultimately processed and seamlessly joined together in a mosaic to show the Veil Nebula in one final image. Although this sounds complicated, there are advantages to this approach as the final image provides a much higher resolution of the target than could been obtained with a telescope that could fit the whole thing in in one go. The final image ends up with more pixels too.
The Veil Nebula is a Supernova remnant. The star that blew itself to pieces was 20 times more massive than the Sun and was just over 2,000 light years away. This cataclysmic event happened about 10,000 years ago. The remaining remnant structure is about 110 light years across and contains the beautiful glowing filaments that you can see in the image. The red colour is caused by ionised Hydrogen atoms, and the green from doubly ionised Oxygen atoms. The filter that I used to capture this image allows light of these two colours (wavelengths) to pass through, but cuts off everything else, including general light pollution and moonlight etc. Astronomers call this narrowband imaging.
Click on the image below to see a full-sized version.
Here, on the south coast of England, the nights get very short indeed for a couple of months around the Summer Solstice. In fact, there are several weeks where theoretical ‘astronomical twilight’ never ends and the Sun never drops below 18 degrees below the horizon. I normally abandon deep-sky imaging but, this year, I was testing out a new system and decided to have a go at a few easy and classic Summer deep-sky targets.
The main thing that helped my productivity during these short nights was a new dual-band narrowband filter from Optolong called the L-Extreme. These multi-band filters are becoming very popular with deep-sky imagers these days. The pass-band spectrum graph is shown below, and you can see that there are two peaks – one centred on H-Alpha and the other on OIII and both are 7nm wide.
I’ve been imaging with Ha, OIII and SII narrowband filters for many years, but so often in the past I have been unable to capture a full set of sub images due to poor weather or lack of time, and this filter brings the possibility of acquiring more finished images as these three testify. By the way, the SII band is not included with this filter but, so often, the SII signal is so weak it rarely adds much to an image. However, since I have this filter in my filter wheel (so that I can use a Luminance filter for RGB imaging) I still have the option of adding my SII filter into the mix if I so desire.
I should mention that these narrowband filters are generally used with one-shot colour cameras. The Ha signal ends up in the red channel and the OIII signal is often mixed between green and blue. My new system includes the amazing QHY268C one-shot colour cooled CMOS camera which is very sensitive and has 16-bit resolution.
I will add a separate article showing the new setup, but it includes the superb Takahashi FSQ-85EDX APO refractor working at f/5.4 riding on a Skywatcher AZ-EQ6 Pro mount. The field of view is 179′ x 120′ which is 3 x 2 degrees (1.72 arc-seconds per pixel).
All three images consist of just over 2 hours of exposures – that’s all the darkness I had on each night! I took 600 second exposures throughout and calibrated with dark, flat and flat-dark frames.
Please click on each image below to see the full size of the images (which are only 50% of the originals).
The first image is the North America Nebula in Cygnus (NGC7000)
The second is IC1396 in Cepheus which contains the Elephant Trunk Nebula near the middle.
Lastly, NGC6888, The Crescent Nebula in Cygnus which is sometime referred to a van Gogh’s Ear!
Hopefully, my next article will not be too long coming. Thanks for reading.