Twinkle, Twinkle………

Astronomy is full of surprises, and learning of the mere existence and nature of globular clusters was a revelation to me.  Perhaps less spectacular and much younger but no less interesting and attractive are open clusters. The so-called Double Cluster is something of a highlight of autumn and winter skies that I had not, until now imaged; not by neglect but because until recently moving to Somerset my previous view of the north sky in Surrey was completely obscured by my house!  Their combined luminosity makes the Double Cluster visible to the naked eye from dark locations, appearing as a hazy patch to the east of the Cassiopeia constellation and are excellent imaging objects too.

 

NGC 869 and NGC 884, known as the Double Cluster or h and χ (chi) Persei, is one of the most striking celestial pairings visible in the northern sky.  Located in the Perseus spiral arm of the Milky Way, these two open star clusters are located about 7,500 light-years away but separated by only a few hundred light-years. Their proximity, similar age, and shared motion through space suggests that they formed from the same giant molecular cloud, making them a physically associated pair rather than a chance encounter.

Double Cluster Up Close

Each cluster contains thousands of stars*, many of which are hot, blue and massive, thereby indicating an early stage of stellar development; estimates indicate an age of approximately 12 to 14 million years. Their youth explains the abundance of B-type and even O-type stars—stellar heavyweights that shine intensely but live only briefly.

The resulting image shows the Double Cluster as a dazzling field of stars. NGC 869, slightly denser and more compact, contains a bright core of hot blue stars. In contrast, NGC 884 appears more loosely concentrated, with a distinctive scattering of bright stars across its central region. Both clusters show subtle hints of red and orange from K-type supergiant stars, evidence that even at their youthful age, some massive stars have already begun to leave the main sequence. 

*processing software identified 22,000 stars in the image!

COMPARISON: GLOBULAR v OPEN CLUSTERS
FeatureGlobular ClustersOpen Clusters
Typical StarsOld, metal-poorYoung, metal-rich
Number of Stars10⁵–10⁶+10²–10³
ShapeSpherical, denseIrregular, loose
LocationGalactic haloGalactic disk
Age10–13 billion years1 million–few billion years
LongevityVery long-livedShort-lived (astronomically)

Astronomical Smorgasboard

The Lobster Claw Nebula (SH2-157) and Bubble Nebula (NGC 7635) are two striking emission nebulae located close to the border of Cassiopeia and Cepheus constellations. The Lobster Claw Nebula derives its name from the curved, segmented shapes that resemble a lobster’s pincers. It is an Ha II region of glowing ionized hydrogen excited by the intense ultraviolet radiation of nearby hot, young stars. Notably, within it lies the young Wolf-Rayet star 157, whose powerful stellar winds sculpt the surrounding gas into complex arcs and filaments.

Relatively nearby, the Bubble Nebula features a spherical bubble of gas about seven light-years across. The bubble is ‘blown’ by the fierce stellar wind of a massive O-type star (SAO 20575) at its centre. The expanding shell of gas glows where it collides with denser regions of the interstellar medium, producing a visually stunning contrast of colours.

Notwithstanding the spectacular nature of both of these nebulae, the image captures a myriad of other objects, which are identified in the accompanying plate solved image, notable of which are the open star clusters of M52 AKA the Scorpio Cluster and NGC 7510. Overall, the constellation of Cassiopeia is full of interesting nebulae and bright star clusters, which my second image from Castle Farm Observatory has caught in abundance.

Somerset Magic

I try to ensure that since Watch This Space (Man) blasted off in August 2014, it does what it says on the tin (top of the page): A personal discovery of the Universe through astronomy and astrophotography. Naturally, alongside this journey life goes on, which this year has been a significant challenge for me in many ways.  Shortly after imaging the Flaming Star Nebula at Fairvale Observatory, Surrey, in early January, I underwent major surgery to replace my right knee and inevitably, all physical astronomy came to a halt; latterly I managed to remotely obtain and process data from sources in Texas, USA and Chile, which was good fun.

Just two months later, whilst still in early recovery (which can take over a year), serendipity made an unexpected appearance, and by at the end of June, after 40-years living in Redhill, Surrey, we moved to a new house just outside England’s smallest city of Wells (population 11,145), in the beautiful countryside of north Somerset.  This upheaval, combined with my recovery, has led to a protracted absence from astrophotography imaging but, at last, I’m now very pleased to present my first image from the new Castle Farm Observatory, in Somerset, of course.

Astronomically speaking, only one thing counts when imaging and that is the quality of viewing conditions (and clear skies), which I can already attest to be excellent here in Somerset.  At my previous location just south of London in Surrey, conditions were poor, with an SQM value of 19.82 that was further complicated by low flying aircraft from three nearby airports.  In comparison, the SQM at Castle Farm Observatory is 21.11, which being a log scale equates to a difference of x3.28 better sky darkness than before and, moreover, overflying aircraft are no longer a problem.  Given this setting, combined with clear skies and a new moon in early September, I had high expectations for my first imaging session since moving to Somerset and was not disappointed by the results obtained of the object chosen for this auspicious occasion, the Wizard Nebula.    

The Wizard Nebula, designated by the central star cluster of NGC 7380, is an emission nebula, in which its gases glow due to intense radiation from hot, massive stars from within the aforesaid embedded cluster.  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.   NGC 7380 was only formed a few million years ago and within it, young and massive O- and B-type stars generate strong stellar winds that shape and erode the surrounding material.

Thus, after an unprecedented break of some 257 days, I’m more than pleased to return to my own backyard astrophotography again, now based in the magic county of Somerset.  The quality of the subs obtained on this first occasion confirmed the outstanding sky conditions, which were literally saturated by stars (see starless image above).  Altogether, it was significantly better than experienced in Surrey and bodes well for what I hope will be an exciting time here at Castle Farm Observatory – Watch This (new) Space! 

    

Tangled In Space

As Douglas Adams succinctly puts it in the Hitchhiker’s Guide to the Galaxies: Space…..is big. Really Big.  If he had lived longer, even he would be surprised to learn how true these words were.  Recent analyses using data from the James Webb Space & Hubble Telescopes, suggests there could be some 2 trillion galaxies.  Notwithstanding, as this applies only to the observable universe, which is about 93 billion light-years across, the entire universe could be significantly larger, with many more galaxies beyond what we can already observe!

Perhaps then it is not so surprising that from time-to-time galaxies run into each other – our own Milky Way Galaxy is expected to collide with the Andromeda Galaxy in about 4.5 billion years.  But there are already many exciting examples of such phenomena that we can image today, of which the Antennae Galaxies are one of the most famous and visually striking examples of two colliding galaxies.  Located in the constellation Corvus, they provide a striking insight into what happens when massive galaxies merge – a process that reshapes their structure, triggering intense star formation, thereby setting the stage for the eventual creation of a single, larger galaxy, all played out over 100’s or even billions of years.

The Antennae Galaxies earned their name from the long, curved tidal tails of gas, dust, and stars that extend outward from the colliding pair of galaxies (NGC 4038 & 4039), thus resembling the antennae of an insect. These tails were created by the immense gravitational forces at play during the collision. As the two galaxies then pass through each other, their mutual gravity distorts their original spiral shapes, pulling out vast streams of stars and interstellar material. These tidal tails stretch for tens of thousands of light-years, making them some of the most spectacular features of any known galactic merger.

At the core of the Antennae Galaxies lies a chaotic and extremely active region. The violent gravitational interactions have compressed enormous clouds of gas and dust, sparking a burst of intense star formation, at a rate hundreds of times faster than that of our own Milky Way. Many of these newly formed stars are massive but short-lived, destined to explode as supernovae, thus enriching the surrounding space with heavy elements. Within another 400 million years, the Antennae’s nuclei will collide and therafter become a single galactic core with stars, gas, and dust swirling around it. 

Imaging such a feature from Earth requires significant telescopic power, the darkest of night skies and the acquisition of lots of data.  Located at the El Sauce Observatory in Chile, 50 hours of data acquired using the Planewave CDK20 astrograph is such a set-up worthy of the task.  However, despite the excellent data quality, I found processing this complex event difficult so as to both show the complexity of the merging galaxies, whilst at the same time preserving the delicate nature of the tails of galactic debris.  The final image is as profound as it is beautiful, demonstrating the immense forces across the cosmos and the inevitable consequences for the many galaxies that occupy the vastness of the Universe.

 

             

Sculptor Galaxy

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 30.6795o, the MOANA project is more than 20o further 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.

Pinwheel Galaxy

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.

 

Star On The Run: IC405

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 65o 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!

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.