New Horizons

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!

Obstech El Sauce Observatory, Chile

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!

    

The Needle Galaxy

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.

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.

 

Cosmic Crustacean

This small but beautiful supernova Remnant (SNR) was the result of the explosion of the star CM Tau, which followed a core-collapse just over 970 years ago.  Located at the centre of the Carb Nebula is the remaining Crab Pulsar neutron star, some 30km in diameter spinning at the rate of 30 times per second.  

 

Footnote & credit: Following a recent knee replacement operation I’m currently unable to set-up and use my astronomy equipment, fortunately I’m still able to continue processing using this excellent public amateur data from the MOANA project located near Fort Davis, Texas, USA  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.  

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.