Interstellar Maelstrom: M42

I get a warm feeling at the first view of the Orion constellation each year.  Just viewed with the naked eye, late at night against a clear black sky it is a wonderful sight that somehow seems strangely reassuring but for the astronomer and especially astrophotographers, there are many exciting targets that hold great promise, principal of which is M42 the Great Orion Nebula.  This winter my first view of Orion was last October, rising from the eastern horizon in the early morning, just as I was about to go to bed after a late-night imaging session. Unfortunately, it was more than two months before the weather relented and I was finally able to snatch an albeit brief image of the said Orion Nebula. 

M42 and other nearby diffuse & reflection nebula (M43 & NGC1975 AKA the Running Man Nebula) is one of the most famous star-forming regions, which being the brightest nebula in the northern hemisphere and just over 1,300 light years distance from Earth, can itself also been seen with the naked eye on a clear night.  To my surprise, I hadn’t imaged this beguiling object for 6-years, during which much had changed: a new mount, camera & filters + I had learned a few more processing tricks.

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” (see starless image below) .  Moreover, these powerful, young stars unleash vast streams of ultraviolet radiation that sculpt the nebula into a myriad of fantastic shapes, further highlighted by a red tint that arises due to the presence of hydrogen gas.  For astronomers, such activities reveal much about the processes of how stars and planetary systems are formed from collapsing clouds of gas and dust.

Known as the Trapezium, four stars tightly located at the centre of M42 are very difficult to image, because of the overpowering bright white light that obscures this area from sight.  However, for astrophotographers the elusive nature of the Triangulum is therefore considered to be the ultimate measure of a good Orion Nebula image.  To overcome this problem, the key is to image the nebula across a range of exposures, from very short to long, which can then be compiled into a single final photograph that equally captures details of bright and darker areas alike.

Although poor weather conditions limited the shoot to a relatively short integration time, I’m pleased to say that the subsequent application of various new processing techniques (*see footnote for details) has created an exciting final image, full of detail and colour, as well as the aforesaid Triangulum, that I believe does justice to this magnificent object that is surely the real star of the winter night sky. 

  • Blemish Blaster by Seti Astro – helps remove inevitable blemishes of the starless image created by StarXTerminator process, which I found much easier to use than PixInsight’s Clone Stamp mostly with better results too;
  • Star Stretch also by Seti Astro – Makes the often-tricky action of stretching star images from StarXTerminator a complete doddle;
  • Astro Image Detail by Hidden Light Photography – An excellent script that makes a great job of teasing out detail from the nebula, that results in a really exciting final image.     

 

  

 

2024 The Year In Pictures

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 11th 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.

 COVERASTRO IMAGING MONTAGE: This colourful splash is a random selection of images, mostly taken from Redhill over the past +10-years of my astrophotography.
JANUARYSEAGULL 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!
FEBRUARYTAURUS MOLECULAR CLOUD:  Located northeast of the Pleiades, below (south) the California Nebula (see November), spanning more than 30o 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.
MARCHHIND’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.
 
APRILLEO 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.
 
JUNESOMBRERO 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?
JULYPuWe-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.
AUGUSTNORTH 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.
SEPTEMBERFORSAKEN 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!
OCTOBERTHE 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.
  
NOVEMBERCALIFORNIA 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.
 
DECEMBERROSETTE 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 2025

Surf’s Up! The California Nebula – NGC 1499

Curving across the Autumn night sky somewhat alone in the Perseus constellation, is the large (100 light-years ~ 2.50o) California Nebula.  Being something of a prelude to the arrival of Orion and all its exciting objects, I have somewhat neglected this astronomical behemoth, only imaging it for short periods from time to time in the past.  Despite continuing poor conditions and with some difficulty, on this occasion I manged nearly 8-hours integration, which with careful processing has brought out the true majesty of this exciting feature.

The final image has been flipped 180 degrees, which for some reason seems to enhance the depth?

An emission nebula located some 1,000 light years from Earth, the billowing clouds of hydrogen and sulphur gases and dust, and the faint, wispy veil of oxygen are clearly evident in this powerful SHO image.  The intense ultraviolet radiation from the nearby massive star Menkib – with a surface temperature of about 37,000 K and radiation 330,000 times greater than our Sun – plays a key role in ionizing the gasses of the nebula, which ultimately brings this majestic monster to life.  

Heavenly Art

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.

                         

Celestial Fleur-De-Lys

Whilst the highlight is the alluring bright blue reflection nebula NGC 7023 AKA Iris Nebula, careful processing reveals that this celestial flower is enveloped within a vast region of interstellar dust, altogether making for a spectacular image.   Strictly speaking NGC 7023 refers to an open cluster within the reflection nebula, which is itself illuminated by a magnitude +7.4 star designated HD 200775 – the cropped starless image shows the beautiful detail that makes up the Iris ‘flower’. 

Starry Messenger

The first galaxies were identified in the 17th Century by the French astronomer Charles Messier, although at the time he did not know what they were.  It was only when in 1924 American astronomer Edwin Hubble measured the distance to the Andromeda galaxy using cepheid variables, that the existence of other galaxies was finally established.  One hundred years on it’s now estimated that there are between 200 billion and 2 trillion galaxies in the Universe; as Douglas Adams said in the Hitchhikers Guide to the Galaxy, “Space…….is really big”! 

For astronomers this time of the year is generally referred to the ‘Galaxy Season’, as our view of the Milky Way from Earth changes from the winter sky of the Orion Spur and Perseus Arm to the summer view with Cygnus overhead down to Sagittarius in the south, in between we’re looking into deep space.  With very few exceptions, galaxies are located very far from Earth, which from our perspective makes them small and therefore a challenge for my imaging equipment.  However, this Spring I’ve been imaging the spectacular Leo Galaxy Cluster, a mere 330 million light-years from Earth (see cropped version of cluster at the top of the page).

Containing at least 70 major galaxies, the Leo Cluster unusually consists mostly of spiral galaxies, which are best seen here cropped from the original widefield image.  The bright elliptical galaxy near the centre of the image, NGC 3842, has one of the largest known black holes in the universe, which is about 10 billion times more massive than our sun! 

We have come a long way since Galileo Galilei published his astronomical treatise Sidereus Nuncius AKA Starry Messenger in 1610, the first scientific publication based on observations made through a telescope. Galileo’s work completely changed the way humanity understood the night sky and, by extension, our place in space, later leading to the acceptance of the heliocentric model of the planets.  Profound as that was, our understanding of the Universe since 1924 has even greater implications.  Moreover, the ability for an amateur to image something like the Leo Cluster from my back garden is exciting and very rewarding (see widefield version above + image location + orientation where the red dot = top left of image).        

Nocturnal Bloom

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.

                          

Avian Astronomy: Seagull Nebula

Located 3,650 light-years from Earth, in the area between the Monoceros and Canis Major constellations, is the emission and reflection nebulae complex of the so-called Seagull Nebula.  It’s been 8-years since I last briefly dabbled with imaging this exciting object and for good reason.  From my position, this bird flies at a maximum 28o above the southern horizon (-11 DEC) and, furthermore, spends much of its time behind houses, trees, and tall hedges, thus providing just two short windows for imaging; combined with this winter’s terrible weather it made for a tough but ultimately rewarding target. 

   

The Seagull’s approximate flight path seen from Fairvale Observatory makes imaging difficult

Whilst popularly known as the Seagull Nebula, the bird consists of a number of fabulous objects spanning some 200 light-years in their entirety: the Seagull’s head (SH2-292) and wings (IC 2177), the large open star cluster along the leading edge of the left wing (NGC 2335) and a smaller cluster on the edge of the right wing (NGC 2327), the nebula at the tip of the right wing (Sh2-297), as well as many other named features (Sharpless and LBN) that are highlighted in the following plate solved image (below).

Despite the difficulties posed by the low transit of the bird in the night sky, each of the Ha, OIII and SII wavelengths are strong, making for good data acquisition and a very pleasing final SHO image.      

Dark Art: Taurus Molecular Cloud

Located northeast (left) of Pleiades, south of California Nebula and north (above) of Aldebaran, spanning more than 30o of the night sky is the Taurus Molecular Cloud (TMC), a rich area of dark nebulae punctuated by bright areas of new star formation.  Moreover, the TMC is thought to be the nearest star forming region to Earth.

Herschel Space Observatory far-infrared’s view of the TMC & approximate image location

All-in-all, the very large TMC provides many promising imaging opportunities.  This image captures numerous, complex dark nebulae across the field-of-view, including Barnard 10 & 214, LDN 1495 & VdB 27, together with bright reflection nebulae LBN 782 & 785 and the odd galaxy – if you look carefully.

  

2023 The Year In Pictures

This Christmas marks the 10th edition of my astrophotography calendar, consisting of my better images from the previous 12-months, which I produce for myself and members of the family.  Wow doesn’t time fly? Based on these images, I also compile a video of the images set to music, which we all watch together before seeing the actual calendar.  It’s become something of an occasion and is a great way to present the images, which look wonderful on today’s smart TV’s and is fun to watch and share with the family.

THE CALENDAR

Much longer imaging times (total of more than 145 hours), re-imaging old favourites in new ways and unusual, overlooked, or difficult objects, resulted in a very good 2023 astrophotography year and perhaps the best calendar yet?  The calendar for 2024 on YouTube can be viewed by clicking HERE and below is a brief overview of each image.  More detailed background information and imaging details for those interested can be found in relevant blogs I posted on this website.  The background music is the track Appleshine from Underworld’s album Drift.

 COVERSH2-284: Close-up of April’s image – along the inside of the ring structure are many dark dust pillars and globules, which on the right seem to resemble a hand with a bony finger pointing inwards!  
JANUARYNGC 1333: Nestled within the western area of the Perseus Molecular Cloud, some 1,100 light-years from Earth is the colourful NGC 1333 reflection nebula, one of the closest and most active star-forming regions of the night-sky.  
FEBRUARY  Spaghetti Nebula: Straddling the boundary of Taurus and Auriga constellations, is the giant supernova remnant (SNR) Simeis-147.  The stellar explosion occurred 40,000 years ago, leaving a rapidly spinning neutron star or pulsar at the core of the now complex and the expanding SNR.  
MARCHAurora Borealis: Situated just below the Arctic Circle, Iceland is well known both for its geology and views of the Aurora Borealis, which we saw in March on the south coast near Kirkjubaejarkklaustur.  
APRILSH2-284: A star-forming region of dust and gases, sculpted by radiation and interstellar winds emanating from a young (3 to 4 million years) star cluster located near the centre.       
MAYM3 Globular Cluster*: Consisting of 500,000 stars and over 11 billion years old, M3 is one of150 globular clusters that orbit around the Milky Way Galaxy.  
JUNEM27 Apple Core Nebula*: A planetary nebula, consisting of a glowing shell of ionized gas ejected from a red giant star in its late stage of life to become a white dwarf. Complex hydrogen (red) and oxygen (blue) fans form around the outer regions, with a pulsar-like beam transecting the nebula.  
JULYMonkey Head Nebula: Located 6,400 light years from Earth in the Orion constellation, the ‘Monkey’ is a so-called emission nebula, where new stars are being created within at a rapid rate.  
AUGUSTSH2-115: This widefield image contains a richness of various emission nebulae, centred around the distinctive large blue SH2-115 region.  Just to the left of SH2-115 is the small but enigmatic SH2-116 a faint, blue disc thought to be a planetary nebula.    
SEPTEMBERLDN-768 Black Cat Nebula: Close to M27 in the constellation of Vulpecula (“Little Fox”), is a dense region of stars broken-up by dark nebulae to create intriguing shapes. Here strung out from left-to-right, several of the dark nebulae seem to coalesce (visually) to create the form of a black cat.
OCTOBERSH2-126 Great Lacerta Nebula: On the western edge of the Milky Way in the southern part of Lacerta, is the very large but faint emission nebula SH2-126.  The red filament structures stretch over 3 degrees, to the right is the Gecko Nebula, a molecular cloud associated with bright young stars.
NOVEMBERFlaming Star & Tadpoles Nebula: Two emission nebulae: dust & gas of the Flaming Star (below) combined with red ionized hydrogen gas produces a flame affect. Above, the stellar winds and radiation pressure from hot massive stars creates the Tadpoles ‘wriggling’ away from the centre.
DECEMBERM51 Whirlpool Galaxy*: As the smaller galaxy passes behind M51, joint gravitational forces are interacting, resulting in the misalignment of stars and unusually bright blue and pink areas across the Whirlpool galaxy. Their fates are inextricably linked and might eventually merge.
                 Footnote: All images taken from Redhill, Surrey or telescope at a dark sky site in
          New Mexico, USA shown by an asterisk*
HAPPY NEW YEAR + CLEAR SKIES FOR 2024