2025 The Year In Pictures

January 1, 2026 by grahamrob in Broadband, Deep Sky Objects, DSLR, Earth, Equipment, Galaxy, General Astronomy, Imaging, Narrowband, Night Scapes, Solar system, Widefield Imaging and tagged astronomy, Astrophotography, Cygnus, DSO Imaging, Galaxies, Milky Way, Nebulae, Orion, Photography, Science, space | Leave a comment

The year 2025 was like no other. Starting with a knee replacement operation in January, shortly after we finally found a new house in March and moved to the lovely dark skies of Somerset at the end of June. Unfortunately, the ensuing turmoil left only a limited time for astronomy. Notwithstanding, I was able to supplement images from Redhill and our new home in Wookey, with some excellent data from Texas, USA and Chile to produce, what I hope you will agree, is an exciting 2026 calendar.

For other pictures and information, go to my website https://watchthisspaceman.com/ or a video of the calendar can be found here on YouTube https://www.youtube.com/watch?v=gn3ls_s71lQ and is best accessed on a PC or smart TV screen. Background music this year is Massive Attack’s track Atlas Air.

COVER	*NIGHT SKY MONTAGE AT CASTLE FARM OBSERVATORY:* All these images (at the top of the page) were taken at various times from the same location at our house in Wookey, Somerset. Clockwise from bottom left: (1) Nightscape of a small coppice looking south (2) Double Cluster – a pair of open star clusters in the Perseus constellation (3) Star trails (4) Sunset looking west.
JANUARY	THE GREAT ORION NEBULA, M42 ⁽¹⁾ The Orion Nebula is a gigantic cosmic cloud of interstellar dust and gas, which is the basis for the birth of numerous new stars or a “star nursery”. Being the brightest nebula in the northern hemisphere and just over 1,300 light-years distance from Earth, it can be seen with the naked eye on a clear night.
FEBRUARY	FLAMING STAR NEBULA, IC405 ⁽¹⁾ This nebula is illuminated by a powerfully bright blue variable star, AE Aurigae. The object’s epithet comes from the brightly lit ripples of gas and dust at the top of the image, illuminated by AE Aurigae and glowing hydrogen gas. This “runaway star” was ejected by a collision two million years ago from the Triangulum region of The Great Orion Nebula.
MARCH	CRAB NEBULA, M1 ⁽³⁾ This small but beautiful supernova Remnant (SNR) was the result of the explosion of the star CM Tau just over 970 years ago. Located at the centre of the nebula, the remaining Crab Pulsar neutron star spins at the rate of 30 times per second.
APRIL	PINWHEEL GALAXY, M101 ⁽³⁾ At nearly twice the size of the Milky Way and containing at least an estimated trillion stars, M101 is the second largest galaxy of the Messier catalogue and certainly one of the highlights of the spring galaxy season.
MAY	SCULPTOR GALAXY, NGC 253 ⁽³⁾ One of the advantages of obtaining data from Texas, USA, is that it enables views of objects in the Southern Hemisphere that are impossible from the UK. Also known as the Silver Dollar, it is one of the brightest galaxies in the night sky, which results from very high rates of star formation that are fed by the abundance of thick dust lanes.
JUNE	NEEDLE GALAXY, NGC 4546 ⁽³⁾ Seen edge-on from Earth, the Needle Galaxy is thought to be a barred spiral galaxy, some 33% larger than the Milky Way. It has at least two satellite galaxies and 240 globular clusters. Seen through a telescope the Needle Galaxy appears like a thin streak drawn across the dark night sky but look closer and its detailed magnificence is revealed.
JULY	WIZARD NEBULA, NGC 7380 ⁽²⁾ Formed only a few million years ago, the gases of this young emission nebula glow due to intense radiation from hot, massive stars within. Interwoven within this glowing gas are dark, dense regions of dust that sculpt the nebula’s dramatic and somewhat mystical appearance, in this case a wizard – which marks my first image from Somerset.
AUGUST	LOBSTER CLAW & BUBBLE NEBULAE, SH2-157 & NGC 7635 ⁽²⁾ Located in the Perseus Arm of the Milky Way, the Lobster consists of ionized hydrogen gas energized by ultraviolet radiation from nearby hot, young stars. The nebula’s distinctive claw-like shape arises from intricate filaments of glowing gas and dark dust. Nearby the Bubble Nebula owes its distinctive looks to a single, massive star, which emits fierce stellar winds that sweep up the surrounding gas into a nearly perfect, glowing shell.
SEPTEMBER	MILKY WAY ⁽²⁾ The night sky in Somerset is three times darker than Redhill, providing significantly better astronomy views. In this case a spectacular image of the Milky Way’s galactic centre.
OCTOBER		THE CYGNUS WALL ⁽²⁾ The Wall is a prominent ridge located within the much larger North America Nebula in the Cygnus constellation. It is an active star-forming region, about 20 light-years long, composed of gas and dust that glows from the energy of young stars.
NOVEMBER		GREAT BARRED GALAXY, NGC 1365 ⁽⁴⁾ A double-barred spiral galaxy located 56-million light-years away, spans over 200,000 light-years across, twice the Milky Way. The most distinctive feature is its massive central bar, which plays a crucial role in channelling gas and dust into the galactic core. As a Seyfert galaxy the nucleus is extremely bright due to energetic processes around its black hole.
DECEMBER		CORONA AUSTRALIS, NGC 6729 ⁽⁴⁾ This spectacular image is a combined reflection and emission nebula, set within the Australis Molecular Cloud. This wonderful, hazy looking nebula unusually exhibits both variable brightness and morphology over time.
*Image Data Source:* ⁽¹⁾Redhill, Surrey ⁽²⁾Castle Farm, Somerset ⁽³⁾USA ⁽⁴⁾Chile
HAPPY NEW YEAR + CLEAR SKIES FOR 2026

New Horizons

September 14, 2025 by grahamrob in Deep Sky Objects, Galaxy, General Astronomy, Imaging and tagged Astrophotography, Galaxies | Leave a comment

Although some time back I lived and worked in Southern Africa for five years and subsequently spent much time visiting and working in many other countries south of the equator, since taking up astrophotography 12-years ago I’ve had no opportunity to work with data from the southern hemisphere, until now. The benefit of obtaining data remotely, which has become very popular in recent years, is that it provides access to different objects and better sky conditions. I did work with a telescope based in New Mexico, USA a few years ago, which was a fun experience but being in the Northern Hemisphere most targets were much the same as here in the UK, except they did have more than 250 clear skies each year. However, this time I’ve moved to what is widely considered to be the holy grail for astronomy, Chile, where night skies are rated as the best in the world!

The dataset was obtained from the famous El Sauce Observatory located in the Rio Hurtado Valley, south of the Atacama Desert, using a Planewave CDK20 astrograph telescope; currently retailing at First Light Optics for just over £42,000! Unsurprisingly, the combination of location and this telescope resulted in the best of the best datasets, which has been nothing less than a privilege to process.

My first target from the Southern Hemisphere therefore had to be something special and NGC 1365, also known as the Great Barred Spiral Galaxy, is just that. A double-barred spiral galaxy, it is located some 56 million light-years away in the Fornax constellation and spans over 200,000 light-years across, making it nearly twice the size of the Milky Way. The Great Barred Spiral Galaxy is also a dominant member of the Fornax Galaxy Cluster group of 58 galaxies.

*Several members of the Fornax Galaxy Cluster are imaged by the VLT Survey Telescope, including the barred spiral NGC 1365 on the lower right Credit: ESO/A. Grado/L. Limatola/VLT*

The most distinctive feature of NGC 1365 is its massive central bar, which plays a crucial role in channelling gas and dust into the galactic core. This inflow of material fuels both star formation and the activity of the galaxy’s central supermassive black hole, which is estimated to be some 2-million solar masses. Various observations in X-rays, infrared, and visible light wavelengths, reveals numerous star-forming regions along the spiral arms, particularly where they connect to the bar, giving the galaxy a luminous appearance.

NGC 1365 is also classified as a Seyfert galaxy, whereby the nucleus is extremely bright due to energetic processes around its black hole. Studies also indicate that the outer edges of the galactic disc are moving at about 84% of the speed of light!

IMAGING DETAILS
Object	NGC 1365, AKA Great Barred Spiral Galaxy or Fornax Propellor Galaxy
Constellation	Fornax
Distance	56 million light-years
Size	11.2 x 6.2 arc minutes (201,700 to 306,800 light years)
Apparent Magnitude	+10.3

Scope	Planewave CDK20
Mount	Planewave L500
Focuser	Optec Gemini
Camera	QHY600PH-M
Filters	Chroma LRGB + Ha 3nm
Processing	Deep Sky Stacker & PixInsight v1.9-3
Image Location & Orientation	Centre: RA 03:34:34.323 DEC -36:08:30.36 Up = North
Exposures	Ha x 62 10 mins, L x 78, R x 78, G x 71, B x 70 @ 5mins Total Integration Time: 35hr 5min
Location & Darkness	Obstech El Sauce Observatory, Chile
Date	August 2024

The Needle Galaxy

June 1, 2025 by grahamrob in Broadband, Deep Sky Objects, Galaxy, Imaging and tagged Coma Berenices, DSO Imaging, Galaxies, Universe | Leave a comment

Perspective is everything – in life and so it is, with astronomy. Hipparchus first pointed the way in 127 BC when he described the procession of the equinoxes and, as they say one thing led to another as, Nicolas Copernicus (1473-1543), Tycho Brahe (1546-1601), Galileo Galilei (1564-1642), Johannes Kepler (1571–1630), Johannes Hevelius (1611–1687), Giovanni Cassini (1625-1712), John Flamsteed (1646-1719) and others opened our eyes to the night sky and what lay beyond Earth. Notwithstanding, it was Edwin Hubble’s discovery of galaxies in 1924 that ultimately led to mankind’s recognition that there was much, much more, that we now take for granted to be the Universe. However, even to the experienced modern astronomer the scale, complexity and beauty of the Universe can be somewhat overwhelming, like when we consider that the observable Universe may consist of 2 trillion galaxies!

Since Hubble’s work we have become familiar with many types of galaxies, which the average person might describe as a colourful spinning firework-like disc, consisting of vast gravitationally bound systems of stars, stellar remnants, interstellar gas, dust and dark matter. This stereotypic impression arises because most galaxy images are viewed face-on or at an inclined angle, so that we can see the structures and processes that have created it. However, given the number of galaxies and therefore the many possible views, it is not surprising that some can only be seen edge-on from our perspective on Earth, the Needle Galaxy AKA NGC 4546 is one of these.

Thought to be a barred spiral galaxy, NGC 4546 is some 33% larger than the Milky Way. It has at least two satellite galaxies, about 240 globular clusters (Milky Way ~ 150) and is the brightest of the Coma 1 Group of galaxies. Seen through a telescope or when imaged the Needle Galaxy it appears like a thin streak drawn across the dark night sky but look closer and its magnificence is revealed, as in the image above.

Here ribbons of dust can be seen criss-crossing along the edge of the thin galactic disc, thereby blocking much of the from light behind. However, it is the bright central bulge that inevitably catches the eye but remains something of an enigma, as little can be seen from within. This excellent data set obtained using the MOANA 10” Newtonian telescope located in Texas’ dark skies, reveals such exquisite details that are provided by the less common edgewise perspective of this intriguing galaxy.

Footnote & credit: Following a knee replacement I’m currently unable to set-up and use my astronomy equipment, fortunately I havve been able to continue processing using this excellent public amateur data from the MOANA project located near Fort Davis, Texas https://erellaz.com/moana/. Many thanks to its creator Elleraz.

IMAGING DETAILS
Object	Needle Galaxy AKA NGC 4565
Constellation	Coma Berenices
Distance	40 million light-years
Size	15.9 x 1.85 arc minutes
Apparent Magnitude	+10.4

Scope	MOANA 10” f/4.5 Newtonian
Mount	Astro-Physics 1100GOTO
Guiding	Off axis guider + QHY 5L2M
Camera	ZWO1600MM Pro
	FOV 45’ x 35’ Resolution 0.5915”/pix Image size 4,656 x 3,520 pix
Filters	Baader 36mm RGB
Capture & Processing	NINA, Deep Sky Stacker & PixInsight v1.9-3
Image Location & Orientation	Centre RA 12:36:08.12 DEC +25:55:59.31 Left = North
Exposures	R x 45, G x 47, B x 45 @ 300 sec Total Integration Time: 11hr 25 min
	@ 90 Gain
Calibration	300 sec Dark & RGB Flats
Location & Darkness	Near Fort Davis, Texas, USA
Date	May 2023

Sculptor Galaxy

May 6, 2025 by grahamrob in AstroBin, Broadband, Deep Sky Objects, Galaxy, Imaging and tagged astronomy, Astrophotography, Galaxies, MOANA, Sculptor, space, travel | Leave a comment

One of the advantages of obtaining data from Texas, USA, is that it enables views of objects in the Southern Hemisphere that are impossible from my location in Surrey, UK. Located close to the University of Texas’ renowned McDonald Observatory at latitude 30.6795^o, the MOANA project is more than 20^ofurther south and, furthermore, boasts some of the best dark skies in North America, what better place to image the exciting spiral Sculptor Galaxy? Also known as NGC 253 or the Silver Dollar, it is one of the brightest galaxies in the night sky, which results from very high rates of star formation that are fed by the abundance of thick dust lanes.

Footnote & credit: Following a recent knee replacement I’m currently unable to set-up and use my astronomy equipment, fortunately I’m still able to continue processing using the excellent public amateur data from the MOANA project located near Fort Davis, Texas https://erellaz.com/moana/. Many thanks to its creator Elleraz.

IMAGING DETAILS
Object	Sculptor Galaxy AKA Silver Dollar or NGC 253
Constellation	Scuptor
Distance	11.4 million light-years
Size	27.5 x 6.8 arc minutes
Apparent Magnitude	+8.0

Scope	MOANA 10” f/4.5 Newtonian
Mount	Astro-Physics 1100GOTO
Guiding	Off axis guider + QHY 5L2M
Camera	ZWO1600MM Pro
	FOV 45’ x 35’ Resolution 0.5915”/pix Image size 4,656 x 3,520 pix
Filters	Baader 36mm RGB
Capture & Processing	NINA, Deep Sky Stacker & PixInsight v1.9-3
Image Location & Orientation	Centre RA 00:47:37.993 DEC -25:17:36.49 Right = North
Exposures	RE x 102, G x 99, B x 98 @ 120 sec Total Integration Time: 9hr 58 min
	@ 90 Gain
Calibration	120 sec Dark & RGB Flats
Location & Darkness	Near Fort Davis, Texas, USA
Date	November & December 2023

Pinwheel Galaxy

April 21, 2025 by grahamrob in Broadband, Deep Sky Objects, Equipment, Galaxy, Imaging and tagged astronomy, DSO Imaging, Galaxies, Milky Way, Ursa Major | Leave a comment

This time of the year is perfect to observe the spectacular face-on spiral M101 or Pinwheel galaxy. At nearly twice the size of the Milky Way and containing at least an estimated trillion stars, M101 is the second largest galaxy of the Messier catalogue and certainly one of the highlights of the spring galaxy season.

A loosely bound cluster of galaxies known as the M101 Group, primarily located in the Ursa Major constellation, is also dominated by the Pinwheel Galaxy, which moreover, is considered to form part of a larger structure within the Virgo Supercluster. Many of the other galaxies in this group are companions to M101, orbiting and interacting with it gravitationally.

Despite its size, M101 is challenging for my William Optics GT81, though I did manage a reasonable image in March 2019. On this occasion using nearly 17 hours of data from the much larger MOANA 10” Newtonian based at the Dark Sky Observatory in Texas, USA, the resulting image shows the galaxy’s beauty to good effect.

Footnote & credit: Following a recent knee replacement I’m currently unable to set-up and use my astronomy equipment, fortunately I’m still able to continue processing using the excellent public amateur data from the MOANA project located near Fort Davis, Texas https://erellaz.com/moana/. Many thanks to its creator Elleraz.

IMAGING DETAILS	IMAGING DETAILS
Object	M101 (NGC 5457) Pinwheel galaxy
Constellation	Ursa Major
Distance	20..9 light-years
Size	29 x 27 arc minutes or 170,000 light-years
Apparent Magnitude	+7.9

Scope	MOANA 10” f/4.5 Newtonian
Mount	Astro-Physics 1100GOTO
Guiding	Off axis guider + QHY 5L2M
Camera	ZWO1600MM Pro
	FOV 45’ x 35’ Resolution 0.5915”/pix Image size 4,656 x 3,520 pix
Filters	Baader 36mm RGB & SHO 6.5nm
Capture & Processing	NINA, Deep Sky Stacker & PixInsight v1.9-2
Image Location & Orientation	Centre RA 14:03:12.0 DEC +54:20:34 Top = North
Exposures	R x 61, G x 73, B x 69 @ 300 sec Total Integration Time: 16hr 55 min
	@ 90 Gain
Calibration	300 sec Dark & LRGB & SHO Flats
Location & Darkness	Near Fort Davis, Texas, USA
Date	May 2023

Star On The Run: IC405

February 14, 2025 by grahamrob in Deep Sky Objects, Imaging, Narrowband, Nebula and tagged astronomy, Astrophotography, Auriga, DSO Imaging, nasa, Nebulae, space, stars | Leave a comment

At this time of the year various objects within the Orion Constellation are perhaps the most popular astrophotography targets. Notwithstanding, a few days after imaging The Great Orion Nebula myself early in the New Year, I slewed my camera some 65^o further north to the Auriga constellation, location of many other fascinating objects, some of which two years ago I captured in a two panel widefield mosaic. This time it was time to concentrate on just one of those objects, the exciting IC405 AKA the Flaming Star Nebula.

This emission and reflection nebula is a glowing cloud of gas and dust that is illuminated by a powerfully bright blue variable star, AE Aurigae. The object’s epithet arises from the brightly lit ripples of gas and dust at the top of the image, illuminated by the aforesaid AE Aurigae and glowing hydrogen emission. By reducing the dominant reddish hydrogen glow in the image, the full impact bright blue light from AE Aurega can be better appreciated (see image below).

Though some considerable distance from Orion, studies now indicate that the star AE Auriga was probably itself ejected after a collision two million years ago from the Triangulum region of The Great Orion Nebula and, as a runaway star has now made its way to Auriga – what a small world!

IMAGING DETAILS
Object	IC405 Flaming Star Nebula – Emission / Reflective Nebula
Constellation	Auriga
Distance	1,500 light-years
Size	37 x 10 arc min
Apparent Magnitude	+6.0

Scope	William Optics GT81 + Focal Reducer FL 382mm f4.72
Mount	ZWO AM5 + ASIair plus
Guiding	William Optics 50mm guide scope
	ZWO120MM mini
Camera	ZWO ASI294MM CMOS sensor
	FOV 2.87^o x 1.96^o Resolution 2.50”/pix Max. image size 4,144 x 2,822 pix
EFW	ZWOx8 EFW & 31mm Chroma 3nm Ha, OIII, SII & LRGB filters
Capture & Processing	ASIair plus, Deep Sky Stacker & PixInsight v1.9.2
Image Location & Orientation	Centre = RA 05:15:28.63 DEC +34:09:07.0 Top = North
Exposures	Ha x20 + OIII x20 + SII x20 @ 300 sec L x10 + R + G x10 + B x20s @ 60 sec Total Integration Time: 5hr 40 min
	@ Gain 120 @ -15^oC
Calibration	5 x 300 sec Darks + 10 x NB Flats & Dark Flats LRGB x20 each Flats & Dark Flats @ ADU 32,000
Location & Darkness	Fairvale Observatory – Redhill – Surrey – UK Typically Bortle 5 to 6
Date & Time	7 & 8 ^th January 2025 +18.45h
Weather	Approx. <=0^oC RH >=65% 🌙 50% Waxing

2024 The Year In Pictures

January 1, 2025 by grahamrob in Broadband, Dark Nebula, Deep Sky Objects, Galaxy, General Astronomy, Globular Cluster, Imaging, Narrowband, Nebula, Planetary Nebula, Processing, Solar system and tagged astronomy, Astrophotography, DSO Imaging, Galaxies, nasa, Nebulae, Photography, space, stars | Leave a comment

Long periods of bad weather made 2024 one of the most difficult years for my astrophotography but, I am pleased to say that this, the 11^th calendar is another belter! Purchased in 2014, I continue to use a William Optics GT81 telescope for most images taken from home, but this means that I’m running out of suitable targets for this equipment. Part of the answer has been to upgrade related equipment and improve my processing, which I hope you will see reflected in this year’s images. Moreover, I have used new skills and techniques to process the better-quality data in new ways – I hope you like the results?

Below is a brief summary of the calendar images used this year but for other pictures and more detailed information, please refer elsewhere to this website, my Flickr page or Astrobin page. In addtion, a video of the calendar can be viewed HERE on YouTube, which is best accessed on a PC or smart TV screen. The background music this year is from Jean-Michel Jarre’s Oxygène album.

COVER	ASTRO IMAGING MONTAGE: This colourful splash is a random selection of images, mostly taken from Redhill over the past +10-years of my astrophotography.
JANUARY	SEAGULL NEBULA, IC 2177: Located 3,650 light-years from Earth is the emission and reflection nebula complex of the so-called Seagull Nebula, some 200 light-years in size. It’s been 8-years since imaging this object and for good reason. From my location, the bird flies very low on the southern horizon and thus spends much of its time behind houses, trees, and tall hedges!
FEBRUARY	TAURUS MOLECULAR CLOUD: Located northeast of the Pleiades, below (south) the California Nebula (see November), spanning more than 30^o of the night sky is the Taurus Molecular Cloud (TMC), a rich area of dark nebulae punctuated by bright areas of new star formation. The TMC is thought to be the nearest star forming region to Earth which, if you look carefully, includes numerous complex dark and reflection nebulae and the odd galaxy.
MARCH	*HIND’S VARIABLE NEBULA & HYADES, NGC 1555:** Discovered by the English astronomer John Russell Hind in 1852 this nebula is situated 400 light-years away in the constellation of Taurus, between the stars of Aldebaran and the Pleiades. The nebula is a Herbig-Haro object – a bright patch of nebulosity in which new stars are forming – which often change in apparent size and brightness.
APRIL	LEO GALAXY CLUSTER: With few exceptions, galaxies are located very far from Earth, making them very small from our perspective and a challenge for my equipment. However, here I imaged the spectacular Leo Galaxy Cluster, a mere 330 million light-years from Earth. Containing at least 70 major galaxies, the Leo Cluster unusually consists mostly of spiral galaxies. The bright elliptical galaxy near the centre of the image, has one of the largest known black holes in the universe, which is about 10 billion times more massive than our sun!
MAY	IRIS NEBULA, NGC 7023*: While the focus of the image is the alluring bright blue reflection nebula, careful processing reveals that this celestial flower is enveloped within a vast region of interstellar dust.
JUNE	SOMBRERO GALAXY, MESSIER 104: Seen from Redhill, the Sombrero galaxy is even lower in the summer sky than the aforesaid Seagull, transiting between the trees and along the top of our +15-foot hedge! An unbarred galaxy, its bright bulbous centre is encircled by dark dust lanes, which viewed side-on from Earth creates the appearance of a sombrero hat or perhaps a flying saucer?
JULY	PuWe-1*: Is a very faint planetary nebula in the Lynx constellation, discovered in 1980 by Purgathofer & Weinberger. It is one of the largest planetary nebulae visible, with a diameter like the full moon and at 1,200 light-years, is one of the closest to Earth. A planetary nebula is a region of cosmic gas and dust formed from the cast-off outer layers of a dying star; despite the name, planetary nebulae have nothing to do with planets.
AUGUST	NORTH AMERICA & PELICAN NEBULAE: It’s at this time of the year (August) I usually turn my attention to the Cygnus constellation and the plethora of imaging opportunities it provides, which inevitably tend to be narrowband targets. Interstellar dust illuminated by large bright areas of star formation are responsible for the formation of both these popular objects.
SEPTEMBER	FORSAKEN NEBULA, IC 5068: This complex area is known for the graphically shaped streaks of cold, dark dust clouds that criss-cross the dense, brightly coloured gas regions of nebulosity. Situated within the adjacent Cygnus molecular cloud just below the Pelican Nebula and close to other more famous objects, this low emission nebula is unfortunately known as the Forsaken Nebula!
OCTOBER		*THE CHINESE CHARACTER, LDN 673:** It might seem paradoxical but often it is the absence of light that makes an image interesting. About 600 million light-years from Earth, within the Aquila constellation, is Lynd’s Dark Nebula (LDN) 673. Some 7-light years in size, this fragmented dark molecular cloud complex contrasts against the colourful molecular clouds and stars of the Milky Way, which is reminiscent of a Chinese character.
NOVEMBER		CALIFORNIA NEBULA, NGC 1499: Located in the Perseus constellation, in the Orion arm of the Milky Way 1,000 light-years from Earth, NGC 1499 is a large emission nebula about 100 light-years long. First imaged in 2016, new improved data and processing now discloses the full grandeur of this object.
DECEMBER		ROSETTE NEBULA, NGC 2244: Approximately 5,000 light-years away, the vast cloud of gas and dust had been sculpted into the distinctive rose-like shape, while meanwhile a central star cluster has blown-away a large hollow within the molecular cloud. Revisiting this old favourite for the fourth time since 2015, here I have experimented with an unusual colour palette combination that has produced an exciting alternative image of the night sky’s rose.
*Footnote:* All images taken from Redhill, Surrey or at a dark sky site in New Mexico, USA shown by an asterisk*
*HAPPY NEW YEAR + CLEAR SKIES FOR 202*5

Heavenly Art

October 20, 2024 by grahamrob in AstroBin, Dark Nebula, Deep Sky Objects, Imaging, Narrowband, Nebula, Processing and tagged astronomy, Astrophotography, Cygnus, DSO Imaging, nasa, Nebula, Nebulae, space | Leave a comment

It’s at this time of the year I turn my attention to Cygnus and the plethora of imaging opportunities it provides, which inevitably tend to be narrowband targets. This year it is IC 5068, a low emission nebula often overlooked because of its location near the more popular North American and Pelican nebulae, as well as many other fabulous targets within the adjacent Cygnus molecular cloud, and as a result is unfortunately known as the Forsaken Nebula!

Located just below the Pelican Nebula and close to the blue supergiant Deneb star (see above), this complex area is known for the graphically shaped streaks of cold, dark dust clouds that criss-cross the dense, brightly coloured gas regions of nebulosity.

As a narrowband target my initial choice of image processing was the traditional Hubble Palette SHO configuration, which as envisaged, resulted in an exciting and colourful rendition of the busy IC 5068 (see image below). Notwithstanding, having recently discovered some other, fairly new Pixinsight processing techniques (NB Color Mapper & NB Image Blend), I decided to give them a try to produce an alternative blended HOO–S image. Though still very much recognisable as IC 5068, the resulting (warm) colours and details reveal a very different and perhaps more dynamic image (see image at the top of the page).

Narrowband images leave much to the imagination when processing and often take on a stirring look when completed. In the case of IC 5068, each of the images produced seem to have the feel of abstract art, whilst at the same time posing many questions regarding the origin of many unusual features. I believe this exciting region deserves much greater attention and should belong in the pantheon of popular Cygnus objects such as the North American, Pelican & Veil nebulae. Moreover, the so-called Foresaken Nebula warrants a name more befitting of its exciting beauty.

IMAGING DETAILS
Object	IC5068
Constellation	Cygnus
Distance	1,600 light-years
Apparent Magnitude	Various

Scope	William Optics GT81 + Focal Reducer FL 382mm f4.72
Mount	ZWO AM5 + ASIair plus
Guiding	William Optics 50mm guide scope
	ZWO120MM mini
Camera	ZWO ASI294MM CMOS sensor
	FOV 2.87^o x 1.96^o Resolution 2.50”/pix Max. image size 4,144 x 2,822 pix
EFW	ZWOx8 EFW & 31mm Chroma Ha, OIII, SII filters
Capture & Processing	ASIair plus, Deep Sky Stacker & PixInsight v1.8.9-3
Image Location & Orientation	Centre = RA 20:51:16.50 DEC +42::30 : 05.30 Top = North
Exposures	Ha x56 + OIII x46 + SII x44 x 300 sec Total Integration Time: 12hr 10 min
	@ Gain 120 @ -20^oC
Calibration	5 x 300 sec Darks 10 x NB Flats & Dark Flats @ ADU 32,000
Location & Darkness	Fairvale Observatory – Redhill – Surrey – UK Typically Bortle 5-6
Date & Time	14^th 18^th 19^th September + 3^rd & 10^th October 2024 +20.15h
Weather	Approx. <10^oC RH >=60% 🌙 50% Waxing

Dark Eagle

July 8, 2024 by grahamrob in Broadband, Dark Nebula, Equipment, Imaging and tagged Aquila, astronomy, Astrophotography, DSO Imaging, Milky Way, Nebula, Nebulae | Leave a comment

It might seem paradoxical but sometimes it is the absence of light that makes an astrophotography image interesting. Such a feature is the so-called Aquila Rift, a vast, dark interstellar cloud that spans the constellations of Aquila (Eagle), Serpens Cauda and eastern Ophiuchus. Towards the central section of the rift, about 600 million light-years from Earth, within the Aquila constellation and not far from the Summer Triangle’s Altair star, is Lynd’s Dark Nebula (LDN) 673.

Some 7-light years in size, this fragmented dark molecular cloud complex contrasts well against the colourful molecular clouds and stars of the Milky Way; the very dense dust of the dark nebulae scatters the blue light of the surrounding stars, producing a yellow-red bias. In places the density within the nebula that energetic outflows can be seen in the form of the red nebulosity of RNO 109 and Herbig-Haro object HH-32.

IMAGING DETAILS
Object	LDN 673
Constellation	Aquila
Distance	600 light-years
Size	1^oor approx. 7 light-years
Apparent Magnitude	Varies

Scope	Takahashi FSQ 106 FL 530mm f/5 + Moonlight Nightcrawler focuser
Mount	Paramount MyT
Guiding	Yes
Camera	QSI 683-WSG8 KAF-8300 full frame CCD sensor 5.4nm pixels
	FOV 1.94^o x 1.46^o Resolution 2.1”/pix. Image array 3326 x 2,507 pix
Processing	Deep Sky Stacker, PixInsight v1.8.9-2
Image Location & Orientation	Centre – RA 19:20:50.72 DEC +11:15:16.20
Exposures	L x35, R x23, G x18, B x22 x 600 secs @ -20C Total Integration Time: 16hr 20min
Calibration	Darks, Bias & Flats
Location & Darkness	Deep Sky West – amateur hosting facility near Rowe, New Mexico – USA SQM Typically >= 21.7
Date & Time	Q4 2018

Nocturnal Bloom

April 1, 2024 by grahamrob in Deep Sky Objects, Imaging, Narrowband, Nebula and tagged art, astronomy, Milky Way, Monoceros, Nebulae, stars | Leave a comment

Like many astrophotographers, the Rosette Nebula holds a special attraction for me; it’s size, details and colours produce a perfect narrowband target. I revisited the old favourite again this year for the fourth time since 2015 (+2017 & 2018), in an attempt to capture even better its unique and dynamic beauty using newer equipment, skills, and techniques.

Located approximately 5,000 light-years away, this vast cloud of gas and dust has been sculpted into a distinctive rose-like shape. The central star cluster (NGC 2237) has blown-away a large hole within the surrounding molecular cloud (NGC 2244), which all together is some 1.7 degrees or 150 light-years in diameter. Numerous star-producing dark Bok globules are visible along the upper-left, central quadrant of the nebula, collectively referred to as the “Carnival of Animals”.

The skies this winter have been poor and, as a result, imaging possibilities have been very limited. However, over five nights from January to March I was eventually able to obtain 9-hours of Ha, OIII and SII integration time which, moreover, produced a good data set of 10-minute exposures.

I’m very pleased with the final SHO image (top of the page), which successfully displays the intricate details and colours that arise from the aforesaid make-up and processes that makes the nebula so popular. Furthermore, experimenting with an HSS palette produced an alternative and exciting image of this rose of night sky (see above), that might be even more in-keeping with its given moniker. All-in-all, despite this year’s difficulties I’m satisfied that I gave the Rosette my best shot, which is definitely a cut above my previous attempts – though I fully expect to return again in a few years seeking further improvements.

	IMAGING DETAILS
Object	Rosette Nebula NGC 2244 + 2237, 2238, 2239 & 2246
Constellation	Monoceros
Distance	5,000 light-years
Size	Approx. 100 light-years ~ 1.3^o
Apparent Magnitude	+9.0

Scope	William Optics GT81 + Focal Reducer FL 382mm f4.72
Mount	SW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
Guiding	William Optics 50mm guide scope
	+ Starlight Xpress Lodestar X2 camera & PHD2 guiding
Camera	ZWO ASI294MM CMOS sensor
	FOV 2.87^o x 1.96^o Resolution 2.50”/pix Max. image size 4,144 x 2,822 pix
EFW	ZWOx8 EFW & 31mm Chroma Ha, OIII, SII filters
Capture & Processing	Astro Photography Tool (APT), Deep Sky Stacker & PixInsight v1.8.9-2
Image Location & Orientation	Centre = RA 06:31:55.304 DEC +05:00:56.913 Left = North
Exposures	Ha x18 + OIII x18 + SII x18 x 600 sec R x20 + G x20 + B x20 x 60sec Total Integration Time: 10hr
	@ Gain 120 & 30 Offset 21 @ -15^oC
Calibration	5 x 600 sec Darks 10 x NB Flats & Dark Flats @ ADU 32,000
Location & Darkness	Fairvale Observatory – Redhill – Surrey – UK Typically Bortle 5-6
Date & Time	19^th January, 12^th February, 6^th 7^th March 2024 @ +20.00h
Weather	Approx. <6.0^oC RH >=70% 🌙 <+6% Waning