Southern Orion in a Wide Field View
An image of Orion from January 2023 taken with a QHY268C cooled astronomy camera mated with a Samyang 135mm lens to give a very wide field view.
Full sized image here (opens in a new tab).
The image is composed of 56 x 120s exposures at F2.8. I used my wide field rig with autofocus to get the stars and nebulosity sharp and tight. I captured flats, darks and dark-flats. Mounted on NEQ6 with a guider scope and image data captured with NINA. All pre and post development is done in PixInsight.
Captured over two nights 20th and 23rd January 2023 when Orion was high to the south. From my back yard in Saxondale, Nottinghamshire - suburban, Bortle 4-5.
I have also captured the Constellation of Orion here.
Collinder 399 "The Coathanger" Samyang 135mm
Collinder 399 or Brocchi's Cluster is offered nicknamed "The Coathanger" for its striking resemblance to that wardrobe item! If you look at the stars in the middle of the image and it looks very much like a coathanger on its side. It is located within the constellation of Vulpecula - The Fox - within a larger asterism called The Summer Triangle. The Coathanger is a chance, line-of-sight effect and the stars that form the appearance of the coathanger are not physically associated with each other at all and range from 350 to 2300 light years in distance.
The stars are backdropped against the vast clouds of glowing hydrogen that dominate the spiral arms of the Milky Way galaxy.
Image Technical Data
Uncompressed version of the image is here (opens in new tab).
Image captured in my backyard in Nottingham, UK on Sunday 20th September 2020. I used a Samyang (Rokinon) 135mm DSLR lens with a Moravian Instruments G2-8300 cooled CCD camera. This was mounted on my NEQ6 mount and guided with a Skywatcher Evoguider and ASI120MM guidecam. All exposures are binned 1x1.
Red > 12 x 300s; Green 10 x 300s; Blue 11 x 300s
All processing is done in PixInsight and image capture was with SGP.
North American Nebula in a wide field with Samyang 135mm and QHY268C camera
This is my first ever image capture with the excellent NINA software. I used my wide-field rig which consists of the Samyang 135mm lens and QHY268C OSC camera using an IDAS 2" LP filter. The wide angle view brings out the North American nebula (NGC 7000) and The Pelican nebula to its right very nicely. There is also a lot of other background luminosity in the image.
The image set is a modest 18 x 180s exposures captured in August 2021, all the data being binned 1x1. Pre-processed and processed in PixInsight with a few tweaks in Photoshop.
Simeis 147 (Samyang 135 mm)
Simeis 147 (Sharpless Sh2-240) sometimes called The Spaghetti Nebula is a supernova remnant of a star that exploded forty thousand years ago. It sits across the border of Taurus and Auriga and is a huge object, about six moon widths across. It is located about 3000 light years away. Because of its extremely low surface brightness it was only discovered as recently as 1952. It is an exceptionally difficult object to observe visually and to have any hope of seeing it with your own eyes at the eyepiece requires extremely dark skies (Bortle 1), specialist filters, immaculate seeing and transparency and extreme dark adaption of your eyes. This rules out almost anywhere near civilisation. Personally speaking, I have never known any astronomer who has seen it visually. Even with photography it requires very long exposure times to bring out any detail.
Image Technical Data
This image was created with my wide-field rig in my backyard in Nottingham UK (Bortle 5 on the dark sky scale) on the 20 and 21 December 2019. It is such a wide-field object that I used my Samyang 135mm lens and Moravian Instruments G2-8300 cooled CCD camera with Astrodon RGB and Ha(3nm) filters. This delivers a FoV of 8x6 degrees.
All exposures binned 1x1:
Ha (3nm) > 22 x 300s ; Red > 8 x 300s ; Green > 9 x 300s ; Blue > 10 x 300s
The total integration time is four hours so far and this is a rather short time for this object. More data would bring out finer structures in the nebula. As a result, I may revisit this at some point and add to the data set already acquired. However, the current result is not so bad for the limited amount of data so far captured. Simeis 147 is so faint that it can consume as much data as you can throw at it and I have seen images of it with 30,40 and even 50 hours of data!
The Image data is captured with Sequence Generator Pro and processed with PixInsight and Photoshop CC.
Other versions of this object often include an Oxygen channel (OIII) because supernova remnants are rich in Hydrogen and Oxygen. I may capture this channel too at some point.
Above is the RGB only data. As you can see, there is very little to show for the data collected. It is when you blend this RGB with the Ha channel data below - especially with the red channel - that the detail in the main picture in this post at the top is revealed.
The California Nebula
The California Nebula - NGC 1499 - is a vast hydrogen gas emission nebula about 1000 light years away in the constellation of Perseus. It is named as such because of its vague resemblance to the US state of California.
It is a very large, faint and diffuse object, about four times the diameter of the moon. It is almost completely invisible visually without specialist filters and was not discovered until the advent of astrophotography in 1884. The nebula shines by reflecting the light of the bright star Markib. It shines red because Hydrogen atoms, when excited by nearby bright sources like stars, emit or re-radiate light at the 656nm wavelength which is in the red part of the spectrum to our eyes.
Image Technical Data
The California Nebula is so large that most telescopes cannot get the nebula in the field of view, nowhere near in fact. It is of course possible to create multi-panel mosaic images but these take a great deal of imaging sky time, something in very short supply in the UK rain and cloud infested skies! DSLR lenses are perfect for this type of wide field imaging, however. This image is almost eight degrees across by six degrees and was made with my wide field DSLR lens portable set up in my backyard, December 7th 2019. Samyang 135mm DSLR lens connected to Moravian Instruments G2-8300 cooled CCD camera and Astrodon E-series RGBHa (3nm) filters, all mounted on my Skywatcher NEQ6 mount.
All exposures binned 1x1:
Red > 14 x 300s ; Green > 8 x 300s ; Blue > 8 x 300s ; Ha(3nm) > 18 x 300s
To give a total integration time of four hours.
Captured with Sequence Generator Pro and processed with PixInsight.
Kemble's Cascade with Samyang 135mm
Kemble's Cascade (Kemble 1) is a chance straight-line alignment of 17 or so stars between the 5th and 10th magnitudes in the far northern constellation of Camelopardalis. The stars are of different colours and look lovely in a widefield telescope or binoculars. At the end of line of stars is the open star cluster NGC 1502. This asterism is named after the Franciscan monk and amateur astronomer Lucian Kemble. The cascade itself is about three angular degrees in length.
Image Technical Data
Imaged from my backyard in Nottingham, UK on 14 September 2020. Part of an automated capture sequence and the exposures were taken between 02:00 > 04:00 in the morning. Needless to say I was in bed asleep at the time :) I processed the images afterwards. I used Samyang 135mm DSLR lens connected to my Moravian Instruments G2-8300 CCD camera with Astrodon RGB Gen 2 E series filters on my NEQ6 mount. All exposures binned 1x1. No separate luminance (i.e. just RGB)
Red > 12 x 300s ; Green > 12 x 300s ; Blue > 10 x 300s
Total integration time is just short of three hours. Processed in PixInsight and Photoshop and captured with Sequence Generator Pro.
I just cut out the cascade stars from the image above. Personally, I prefer it in the wider setting in the topmost image
The inverted colour version above may make it easier to see the "cascade" of stars and make it easier for you to find them in the main image.
I hope you like it!
The Veil Nebula - Samyang 135mm Lens
The Veil Nebula in Cygnus is the remnant of a supernova of a star about 20 times the mass of the sun that exploded about 20000 years ago. The nebula is a huge, very faint and diffuse object, about six moon widths in diameter and is located about 2500 light years away. Very few telescopes can capture the entire Veil Nebula complex due to the huge angular size that it presents on the sky and creating a multi-frame mosaic is a very time consuming process, especially in the UK where clear nights are such a rare and premium time. This makes DSLR lenses ideal and few are better or as cost effective as the Samyang 135mm that was used to capture this image.
Image Technical Details
The image was captured from my backyard in Nottingham in the UK on the nights of the 13th and 14th September 2020. I left the systems capturing data overnight on an automated basis capturing the Veil nebula and several other targets whilst I was asleep in bed :). I used a Samyang 135mm lens (Samyang = Rokinon in the US/Canada) connected to my Moravian Instruments G2-8300 CCD camera with Astrodon RGBHa (3nm) filters on my NQ6 mount. All exposures binned 1x1:
Red > 14 x 300s ; Green > 14 x 300s ; Blue > 14 x 300s ; Ha > 31 x 300s
Total Integration time of just over six hours. The total width of the image is about 8 degrees by 6 degrees with a resolution of 8.5 arcsec/pixel.
Above are the Ha images made with the Astrodon 3nm Ha filter in the 31mm version. You can see the exquisite detail this filter picks out.
The RGB image is made from 42 x 300s exposures. It carries the colour of the image but is boosted by the blending of the Ha data which adds the punch and vibrancy of the master image at the top of the page.
The Heart and Soul Nebulae Samyang 135mm
The Heart and Soul Nebulae are a well known and famous pairing of Nebulae in the late summer/autumn sky of the Northern Hemisphere. These nebulae are located far away - 7500 light years - in the Perseus arm of the galaxy, further out from the core of the galaxy than the Sun and are vast star forming regions rich in Hydrogen Alpha that gives the images the intense red glow.
All image data collected with a Samyang 135mm lens at F2.8 with a Moravian G2-8300 CCD camera. Below is the RGB image gathered with Astrodon RGB filters. All binned 1x1: Red 14 x 300s; Green 13 x 300s; Blue 14 x 300s. This gives an RGB integration time of 210 minutes or three and a half hours.
The picture looks nice but it does lack punch and vibrancy as it stands. It needs the addition of the Hydrogen Alpha data that will enhance the details.
Below is the Hydrogen Alpha channel that consists of 36 x 300s exposure with an Astrodon 3nm Ha filter with Samyang 135mm and G2-8300 CCD camera, collected with an Astrodon 31mm 3nm Ha filter. The amount of detail in this image is very evident. Below this is a starless version of the Ha image used to blend into the RGB image.
I finally created the blended HaRGB images by using layers of the Ha channel blended at different opacities as overlay and lighting layers in Photoshop. This gives the best of both worlds; the colour present in the RGB and the detail in the Ha image. The total integration time of the image is about six and a half hours.
Finally an annotated version of the image showing many Sharpless Catalog (Sh2) objects present.
The Heart and Soul Nebulae Samyang 135mm
The Heart and Soul Nebulae are a well known and famous pairing of Nebulae in the late summer/autumn sky of the Northern Hemisphere. These nebulae are located far away - 7500 light years - in the Perseus arm of the galaxy, further out from the core of the galaxy than the Sun and are vast star forming regions rich in Hydrogen Alpha that gives the images the intense red glow.
All image data collected with a Samyang 135mm lens at F2.8 with a Moravian G2-8300 CCD camera. Below is the RGB image gathered with Astrodon RGB filters. All binned 1x1: Red 14 x 300s; Green 13 x 300s; Blue 14 x 300s. This gives an RGB integration time of 210 minutes or three and a half hours.
The picture looks nice but it does lack punch and vibrancy as it stands. It needs the addition of the Hydrogen Alpha data that will enhance the details.
Below is the Hydrogen Alpha channel that consists of 36 x 300s exposure with an Astrodon 3nm Ha filter with Samyang 135mm and G2-8300 CCD camera, collected with an Astrodon 31mm 3nm Ha filter. The amount of detail in this image is very evident. Below this is a starless version of the Ha image used to blend into the RGB image.
I finally created the blended HaRGB images by using layers of the Ha channel blended at different opacities as overlay and lighting layers in Photoshop. This gives the best of both worlds; the colour present in the RGB and the detail in the Ha image. The total integration time of the image is about six and a half hours.
Finally an annotated version of the image showing many Sharpless Catalog (Sh2) objects present.
IC1396 with Samyang 135mm
IC1396 - "the Elephant's Trunk Nebula" is a huge emission nebula in the constellation of Cepheus, about 2500 light years away. It has a huge angular diameter of about 2 x 3 degrees so it requires a wide field telescope/lens to capture it in its entirety.
It is a very popular imaging target both in a wide field setting like this picture and also as close up views of the "trunk" that you can see in the image at the 6 o'clock position.
Image Technical Data
Image data acquired September 13th 2019 from my backyard in Nottingham, UK. This image was taken with my Samyang 135mm lens with G2-8300 CCD camera and Astrodon RGBHa filters on NEQ6 mount. Everything is 300s in this image and binned 1x1:
Ha (3nm) x 13; Red x 12; Green x 8; Blue x 14