New World

It’s early days at my new Castle Farm Observatory and I’m still feeling my way into the benefits of Somerset’s superior darkness, which is noticeably better than my previous home in Surrey.  But my new Bortle 4 location is not without some issues: there are a couple of nearby streetlights that can now find its way to my observatory since autumn leaves have fallen, occasional vehicle lights pass by and, inevitably, sections of the sky are obscured by our house and trees. 

Westerly view from Castle Farm Observatory

After more than 12-years of imaging almost exclusively looking south, I must now adjust imaging plans looking southwest or north, which are my main sightlines in Somerset. This might seem a minor issue but as the sky moves around an axis defined in the north by the Polaris star, it thus follows an inclined equatorial grid relative to Earth and the impact on potential imaging plans can be quite profound. Previously looking southwards, the transit of objects during the night (and day) was from the east to west horizons, which on a clear night enabled up to 6-hours imaging of a single object, compared with a westerly view which only catches the latter period of the aforesaid transit.  As a result, objects I used to image say from November onwards now only appear in the available (western) section of sky two or three months later. On a more positive note, I am now able to image circumpolar objects looking high and northwards for the first time, which has literally opened new world of possibilities.

Given the aforesaid issues, I recently chose to image an old favourite which is currently in a favourable position at this time of the year, the North America Nebula (NAN), located high in the early evening night sky looking due west. Spanning some 100 light-years, NAN is a great narrowband object, which by using the Hubble SHO palette always results in an exciting and colourful image.

Over two nights I manged to obtain nearly 9-hours of good data, which at my previous Bortle 6 Surrey observatory would probably be the equivalent of more than 12 hours.  The final processed SHO image brings all three channels into a delicate balance: vibrant without being garish, detailed without overwhelming noise. The iconic “Gulf of Mexico” region forms a deep void in the nebula, which becomes even more pronounced with the various gradients of blue converging around its dark centre.  But on this occasion, I was particularly keen to emphasize details of the fabulous Cygnus Wall (see cropped image below), situated in the lower right corner of the main image i.e. ‘West Texas and Mexico’!

The Cygnus Wall is a striking, heavily sculpted region within the North America Nebula, which itself is worthy of image, which would require a larger telescope. The dense ridge of gas and dust glows brightly as nearby young, massive stars bombard it with intense ultraviolet radiation, causing it to ionize and shine.  Its dramatic pillars, ridges, and cavities resemble a cosmic coastline, shaped by stellar winds and ongoing star formation. For some reason it’s been 8-years since I last imaged NAN, except with my Samyang widefield rig, but with the excellent night skies of Somerset I feel sure I’ll be back sooner next time, perhaps with a bigger telescope?

 

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! 

    

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!

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

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.