Comparing Messier’s globs
Sketching globular clusters is fun (really!). It’s impossible to draw every single star in the correct position, but still a lot of details can be collected like shape, size, condensation, distribution of the stars, star chains, brightness, color (GC’s appear blue to me in most cases), darker spots or area’s within the cluster etc. In the end it’s always the goal to show the identity of each and every object and with globs that can be hard because at first glance they appear so much alike. In this section I’ll try to show the individual characteristics of all the Messier globular cluster as realistically as possible, often by comparing them directly to each other.
During my trip to La Palma in June 2018 I finally had a chance to observe the three Messier globular clusters close to eachother at the bottom of the “teapot” for a bit of a longer period. On photographs they are quite alike in size and structure, but through the eyepiece it was easy to see their differences. I thought it would be fun to do a comparison sketch so that the differences can be seen at a glance. The observations were done with the 10″ newton at 240x from the top of the Roque de los Muchachos.
M69 – has a bright and triangular core, a bit more stretched to the N-E. It appears grainy, but can’t be resolved. The outer region is short and a bit more grainy, but still can’t be resolved. On the S-E boundary I see a bit of a dark lane.
M70 – has a very small core in the shape of a reversed heart and can’t be resolved. the large halo can be resolved a bit better than that of M69 with averted vision, but I don’t see any individual stars, just a grainy glow.
M54 – is the largest of the three (just) and looks like an elliptical galaxy on first impression. The 1/3 brighter core gradually flows into the halo and only with effort I can see some graininess in here. The halo too flows very gradually into the sky background.
A month later and back at home in The Netherlands I decided to do another comparison of 3 globs near eachother. This time it was the turn for Ophiuchus where no less than 6 Messier globs reside. The three of them with the highest declination are still nicely visible from my northern latitude. They are all very different and striking in their own way. The observations were done with the 16″ Alkaid at 181x from Breezanddijk and the Knardijk.
M12 – The smallest one, but with a large and rich halo. Easiest to resolve. Has a diamond shaped core with a somewhat darker region N-E of it. Star chains are numerous and most prominent on the W-side. The cluster is underlined by three bright stars and surrounded by a bit weaker stars in the shape of a “V”, which make it my personal favorite of the three.
M10 – Beautiful. Perhaps a bit harder to resolve. Also here many starchains can be seen flowing away from the core. There is a notable line of brighter stars crossing the cluster in N-S direction and a few dark dustlanes crawling like worms in front of the core. The shape reminds me of an arrow being shot upwards.
M14 – The most condensed one and it’s even a bit hard to see the graininess. Almost perfectly round, just slightly more confined and “pointy” on the E-side. The brightness fades away softly from the not too bright core to the outer region. The halo is short. Only a few stars can be seen blinking up in the core now and then, of which one exactly in the centre. One starchain meanders towards the S-W. Must be a showpiece from a more southern and darker location, but here it remains a bit too dim for my taste.
In 2017 I was in the French Pyrenees and had the chance to do some observing during my two week family holiday, although the weather didn’t really prove favorable. On one night however I was able to take my 16″ Alkaid up the “Port de Balès”, a mountain passage at a height of 1800 mtrs and a very beautiful and very dark location. I haven’t sketched a lot during my four short sessions, but couldn’t resist the urge to put these two globular clusters on paper which I viewed one after another. How different can two GC’s really get?!
M55 is a (Shapley) class XI cluster and with that it’s very loose and almost resembles a dense open cluster. It was dim, perhaps because of the (still) low declination and the brightness of the stars was quite uniform. About 7 or 8 stars were a bit brighter than the rest and the shape of the cluster reminded me of a pentagram. It was large too(!) and could almost compete with the nearby M22 in size. I was surprised to find it so striking this time, compared to other occasions when I’d seen it.
M75 on the other hand is VERY dense. Being a class I object I had a lot of difficulty to even see that it was a globular cluster as no stars could be resolved… The small core shines like a bright pearl, surrounded by a weak halo where only the suggestion of graininess could be suspected.
M55 and M75 are placed in the sky in such a way that you can see them right after each other, so have a look for yourself and see if you are as astounded the way I was to see that two GC’s can look so much different from one another. M55 was sketched @129x and M75 was sketched @259x.
The following set is yet another example of two globular clusters which are very different. Both reside in the beautiful constellation of Scorpius.
M4 is large and loose and the not-too-bright core is showing a background glow in the shape of a mushroom (at least, this is how it appeared to me…) There is a remarkable star chain accross the surface from N-S which really stands out and another (weaker) chain on the left marks the outer halo of the cluster. With ease, hundreds of stars were visible in the field of view, a tremendous sight indeed.
M80 on the other hand is tiny with a 1/3 very bright core and 2/3 halo. The core and halo are well seperated from eachother and there’s a small arc of dim stars just set loose from the globular (like a mustache). The halo can be resolved somewhat, but the core is just a blazing dense glow.
Both globs were sketched at La Palma with the 10″ Alkaid and a 10mm eyepiece, giving a 120x magnification.
Some of the Messier globular clusters can’t be compared to anything else because they are a true masterpiece of their own. They deserve a full resolution sketch and I will show these below.
First one is M5, my personal favorite of the northern hemisphere (there, I said it). I was stunned with its beauty the first time I observed it under a dark sky with my 16″ Alkaid. I chose a magnification of (only) 181x to fully take in the surrounding field and started with sketching the stars around the GC and marked their brightness, like I normally do when drawing open clusters. Then I wrote down how M5 fitted within this star field and drew the obvious star chains; these are moving primarily to the south, east and (a bit less) to the north. On the western side (left in the sketch), M5 looks more flattened and there’s more of an absence of dim stars. This whole picture gives the impression that the cluster is resting in a “swing” of star chains. The core is bright, almost perfectly round and stars could be resolved almost into the very heart of it. On the NE side a “bite” seems to have been taken from it and placed back a bit remote.
Next one up is M92 and this one was sketched under less favorable conditions with the 16″ Alkaid at 259x. The grey nights had started here in the north already and the moon was still up, but this globular cluster is powerful enough to overcome these disadvantages and still provide a neat image.
Most noticeable are the stars immediately around the cluster that are arranged in a somewhat diamond shape. They appear to “box” the cluster. On the right side of the core there’s a curved darker zone visible in a “boomerang” shape and more dark blotches can be seen dimming the graininess a bit in other areas. After an hour of observing and drawing, two dark parallel lines are suspected crossing the core. As if two fingernails have made a scratch on it. Intriguing! Here’s the close-up version of the #2 globular cluster of the northern hemisphere (in my humble opinion…):
The density of M53 is average (Shapley class V) and it took high magnification well to break down the core, which showed an atypical triangular shape and seemed to have a few dark lines running through it. The direct halo around the core was not perfectly round, but had a bit of a “dent” on the upper side in the sketch, resembling a cheek-tooth. The right side was edged a bit sharper and curled around a brighter star under the centre in a comma-shape. Around the cluster some 25 brighter stars were noted, most of them close to the outer halo of the dimmest suns. Sketched with the 16″ Alkaid @362x.
On to a cluster that appears a bit strange: M30. It’s the toughest object during the Messier Marathon and in autumn the globular cluster rises to only about 15 degrees in my sky; not very favorable, but at least some details can be seen. The moderately sized cluster has quite a dense core which seems to be elliptical. Around it some graininess can be seen, especially with averted vision. The object seems to be sustained by two “canes” of stars, which gives it a funny look. Due to the low position in the sky I used a magnification of 181x with the 16″ Alkaid.
M71 is even more odd. This globular cluster was very interesting because of its particular shape and its strong resemblence to a dense open cluster (like M11 for example). The cluster was quite easy to resolve and although a glow of the faintest stars in the background still remains, I could see no stronger luminance in the core. I was able to distinguish about 15 stars that were a bit brighter, of which a double star stood near the centre, and another 10 stars a little less bright. The weakest visible stars provide for the grainy look and give the cluster a shape that is definitely triangular and because of two indentations and a “tail” it strongly reminded me of a moonfish. The cluster resides in a very rich part of the summer sky. Sketched with the 16″ Alkaid @259x.