Giant Veil Nebula

Subject: Giant Veil Nebula

Hello Artists,all o.k.?I’m in holyday in this moment,the break from work,so, for me….very good days!!!
I sent my first sketch of great nebula in Cygnus made with my dobson 10″ and great old eyepiece,the Meade “Reserch Grade”12,4mm + UHC-S.
At first time i want made this sketch in one page of my album,but….the impressive dimension oblige me for two pages!
I sent you three photos of sketch,the particulars and totally of this.It’s impossible to insert in my scanner….
Excuse me for my english,clear sky.
At next and compliments at all sketchers for your works.
Ciao a tutti,Giorgio.

Site:Pergola,Serraspinosa Hill 400 meters of altitude,
Marche Region,Center Italy.
Date:2 of August 2010
Instrument:Dobson GSO 10”
Eyepiece:Meade 12,4mm “Reserch Grade”
Filter:Baader UHC-S
Seeing :Good
Air: Fresh,no wind.
Technics:White pencill and penn on black paper “Fabriano 3”

Giorgio Bonacorsi

Explosion in the Keel

Observation of eta Carinae

Object information

Object name:

eta Carinae

Object type:

Star

Magnitude:

-0.80

RA:

10h 45m 30s

Dec:

59° 44′ 39″ S

Constellation:

CAR

Observation details

Date of observation:

12 avr. 2010 19:05 UT

Length of observation:

58 min

Object position:

Alt: 52.0°, Az: 166.8°

Weather conditions:

Day: ++/- (33% cumulus) Wind V2-3, temp 30°, humidity 31%, Transparency 1 (on a scale from 1, best, to 5, very bad

Observation conditions:

Nught: SQM 21.57 in Crv (60° high), limited nake eye mag in Crv 7.2, seeing quite good S2/156 3/280 4/520 4-5/725

Observing site:

Namibie Tivoli

Instrument:

TN 508 Dobson Tivoli

Main eyepiece:

Televue Nagler 9mm Type 6

Barlow:

(None)

Magnification:

282x

Notes:

x282 Nagler 9mm, then

x529 Nagler 4.8mm, then

x725 Nagler 3.5mm

I have to increase gradually the power in order to have a deep and detail view of the object, then decrease it to improve the contast, and the color.

with 282x, The two small lateral “mustaches” are obvious, and precisely analysable, with the luminosity of their end decreasing regulary. The two dark spots of the SE lobe are well separated, and also analysable, including their shape, and orientation. The NW lobe is as large as the opposite one, but much less luminous, L3 instead of L6, in a scale from 1, limit, to 10, extremely bright.

The color is fantastic: deep, vivid, and strong orange. The star, itself, is even more saturated ! Probably the most beauteful orange anywhere in the sky

This drawing is the third I did.: Eta Carina is an extraordinary object, very much detailed, and each time, you discover new features.

Pencil and ink of China on Canson paper 21 x 29.7 cm, 200gr/cm2, then scanned, and some improvements with Paintshop Pro.

Much more details on my website: www.deepsky-drawings.com

Bertrand Laville

Stippling Cauchy and Rumker

PCW Memorial Observatory, OH, USA
Erika Rix

2010 06 30, 0533-0839 UT
Cauchy, rilles, & domes
Zhumell 16”, 12mm Burgess, 2x Barlow, 300x mag
Temp: 11.2°-9.7°C, > 90% humidity
S: Antoniadi III increasing to II-I
Phase: 118°
Lunation: 17.77 d
Illumination: 87.2%
Lib. Lat: -3°28’
Lib. Long: +00°33’
Az: 135°22’, Alt: 25°44’

2010 06 25, 0229 UT
Mons Rumker
Zhumell 16”, 12mm Burgess, 2x Barlow, 300x mag
Phase: 16.2°
Lunation: 12.64 d
Illumination: 98%
Lib. Lat: 3°37’
Lib. Long: 5°33’
Az: 153°57’, Alt: 19°25’

One of the joys of the types of observing sessions we do is trying new
techniques and media to sketch the objects we view (except for my solar
sketches….I’ve sort of settled for the comfortable ol’ shoe feeling of
my black paper and Conte’). I’ve played around with quills and India ink
for years, actually since I was in my early teens. The thought of having
an open bottle of India ink next to me in the dark while observing was a
not appealing. In fact, as messy as I am with ink, nothing within a 10’
radius would have been safe from being splattered black, including my
optics.

I’ve been studying some of Harold Hill’s beautiful sketches and fancied
trying my hand at stippling for lunar observations instead of my typical
charcoal or pastels. I believe the norm is to do a schematic sketch in
pencil and label it with a legend. The idea of this is to bring the
sketch back inside and stipple over it with the quill and ink in the
comfort of your home with light. If you took care with your notes and
the labeling, you could even do this days later. It takes me long enough
to write my reports and record all the data from my sessions and I don’t
relish the idea of spending extra time working on a sketch once my
session at the eyepiece is over. Above all, I certainly don’t trust my
ability to redraw (or draw over a schematic sketch) using a shading
legend, which is one reason my sketches are completed at the telescope.
I want to ensure that there is no chance of me messing up (adding
details, misplacing markings, wrong shadings…) the details that I
actually see during my session.

Taking all that into consideration, a good alternative to India ink is
using a marker. Grabbing what I could find on hand, I used white card
stock paper and a permanent marker with a finer point for my sketch of
Mons Rumker. Since this was my first attempt, I went ahead and tried the
schematic sketch with labels first of Mons Rumker. I ended up with lines
and numbers all through the sketch so that soon I was unable to make
neither rhyme nor reason of the sketch itself.

Next, I tried drawing the dome with a pencil as if I were making a quick
regular sketch of it. Then I redrew it inside the house using the marker
for stippling. Although it was kind of fun, if I’m going to do a sketch
with a pencil anyway, what’s the point of doing it all over again with
stippling? Plus, I accidentally inverted my craterlets in the re-sketch.
The final straw was when I showed the stippled sketch to Paul, my
husband who is also an amateur astronomer, and after studying it for a
moment, he asked me what it was.

My next attempt turned out much better. I can’t help but to think part
of that is because I sketched while viewing instead of having to try
decipher my notes or markings of a schematic sketch after my observing
session was over. I was sketching all the subtle blendings instead of
having lined borders where the contrasts changed. Of course, the change
in markers plus a little more experience helped too. I sketched the area
around Cauchy with the rilles and domes nearby. I used an ultra-fine
black permanent marker with Rite in the Rain paper and created the
entire sketch at the eyepiece. I didn’t find a need to use erasers nor
pencils for the Cauchy sketch.

Harold Hill is a master and I’ve got a lot of work ahead of me. But the
first step is actually do it. The second is doing it again and again.
Throw in a few tweaks to the media or techniques, and my stippled
sketches are bound to show a result of my efforts.

NGC 6384

NGC 6384
NGC 6384
By Erika Rix

2010 June 8, 0457 UT

NGC 6384, Galaxy type SAB(r)bc I, Ophiuchus, ~80 million light years away
Hazy oval with a brighter oblong middle, 6.4’ x 4.3’, magnitude 10.4v

PCW Memorial Observatory, Zanesville, Ohio USA – Erika Rix
16” Zhumell, 13mm Ethos and 8mm TeleVue Plossl, magnification ~138x – 225x
Temp: 8C, Humidity 92%
Seeing: P 7, Transparency: 3/6

Sketch created scopeside with Rite in the Rain paper, black ballpoint ink pen, #2 pencil then the stars cleaned up in Photoshop and inverted with adjustment to brightness and contrast.

At first glance, this spiral galaxy looked small and oblong nesting with a triangle of stars. Putting a dark cloth over my head and studying it further, I was able to make out a larger fainter portion of it extending to nearly two of the stars in the triangle. I couldn’t make out any structure on the outer portion other than it was almost oval. The inner, brighter portion was more oblong and the density was uneven.

During this observation, two satellites crossed the lower portion of my FOV, traveling west to east. The second one came through about half hour after the first. It seemed to be moving a little slower and was not as bright as the first. The second was at 0440UT. The courses were marked on my sketch by the dashed lines.

NGC 4755 – The Jewel Box

NGC 4755
NGC 4755
By Scott Mellish

NGC 4755 “The Jewel Box”
Open Cluster
Crux
18/03/10
Ilford NSW Australia
56cm f5 Dobsonian
Field: 27′
Magnification: 149x
Sky Quality Meter reading: 21:46

There was a bit of haze around while I was out observing, along with intermittent thin cloud so I decided to stick with something bright.

I have sketched NGC 4755 a number of times, but I have to say that a sketch can never do justice to this very beautiful object.

With this sketch I put in an extra effort to try and get as accurate a representation as I could.

The “Jewel Box” was discovered by Nicolas Louis de Lacaille when he was in the southern hemisphere during the years 1751-53

John Hershel was suitably impressed when he observed the cluster and wrote the following description-

“this cluster, though neither a large nor a rich one, is yet and extremely brilliant and beautiful object when viewed through an instrument of sufficient aperture to show distinctly the very different colour of its constituent stars, which give it the effect of a superb piece of fancy jewellery”

NGC 4755 contains some of the most luminous supergiant stars within the Milky Way ranging from around 83 000 to 75 000 times the brightness of the Sun. The central orange coloured star in the sketch is a massive red supergiant about equal to Betelguese.

One really has to look at this object through a telescope to really enjoy the visual treat of this exquisite open cluster.

Scott Mellish.

The Fourcade-Figueroa Object

ESO 270-17
ESO 270-17
By Scott Mellish

ESO 270-17
18/03/10
“Fourcade-Figueroa Object”
Galaxy
Centaurus
Ilford NSW Australia
56cm f5 Dobsonian telescope
Field: 15′
Magnification: 314
Centaurus
Sky Quality Meter reading: 21:31

This is a sketch I done recently of the elusive galaxy ESO 270-17, sometimes described as the “Fourcade-Figueroa object”. Studies have shown that this galaxy could quite possibly have collided with NGC 5128 “Centaurus A” in the distant past and thus is considered as a “shred”.

The alignment of the dust band of NGC 5128 with ESO 270-17 and also its lack of rotation has lead researchers to conclude that this quite faint galaxy
had collision based origins.

A dark sky site and some decent aperture are essential for observing this unusual object.

Scott Mellish

NGC 5286

NGC 5286
NGC 5286
Sketch and Details by Scott Mellish

NGC 5286
Globular Cluster
Centaurus
18/03/10
Ilford NSW Australia
56cm f5 Dobsonian telescope
Field: 27′
Magnification: 218x
Sky Quality Meter reading: 21:39

This rather quaint little globular cluster was mostly resolved in the
56cm dob at 218x mag.

The bright orange/yellow tinged star in the field is the spectroscopic
binary M Centauri, a G-type star which lies around 257 ly from Earth,

Both the star and the globular cluster together make for a most pleasing
view.

Scott Mellish.

NGC 5291 – The Seashell

NGC 5291

NGC 5291

Sketch and Details by Scott Mellish

 

NGC 5291/”Seashell Galaxy” MCG -5-33-5
Interacting galaxies
Centaurus
Ilford NSW Australia
21/02/10
56cm f5.0 Dobsonian telescope
Field: 15′
Magnification: 314x
Sky Quality Meter reading: 21:60

Black Canford paper
White pen
White pastel chalk
Soft white pencil
White oil pencil

This strange little pair of galaxies first came to my attention many years ago when I purchased the lovely coffee table book “Exploring The Southern Sky” by Laustsen-Madsen-West. On page 106 there is a lovely negative image showing why the companion to NGC 5291 is called the “Seashell”.

In my 56cm dob it is a struggle to discern any hint of the unusual shape of this object even with averted vision. However this is a very interesting tight pairing and they both viewed quite easily in the 56cm dob.

Both objects I believe are classed as disturbed S0 type.
MCG-5-33-5 is the object to the left of the brighter NGC 5291 as seen in the sketch.

Also of note is the very faint galaxy PGC 4887, this galaxy can be barely seen about 7′  further to the left  of  NGC 5291/Seashell almost to the edge of the field.

The whole region surrounding this pair is strewn with numerous galaxies of varying brightness and size, all of which are part of the IC 4329 cluster.

I recommend those interested visit the CDS or NED databases  if you wish to view the “Seashell” in greater detail.

Scott Mellish

Ramshackle in Reticulum

NGC 1313
NGC 1313
Sketch and Details by Scott Mellish

NGC 1313
Star Burst Galaxy
Reticulum
12/12/09
Ilford NSW Australia
56cm f5 Dobsonian
Field: 17′
Magnification: 354x
Sky Quality Meter reading 21:67

Black Canford paper
White pen
White pastel
Soft white pencil
White oil pencil
Blending stump

I was not all that impressed with the quality of the observing conditions while I was sketching this impressive galaxy.
Waves of unsteady air were crossing the eyepiece field at intervals.

Still when there is a clear sky to be had then beggars cannot be choosers.

NGC 1313 is big and bright enough to hold its own in such conditions.
A noted Star Burst galaxy as is quite evident from its ramshackle appearance.

In a large dob this galaxy is a very rewarding sight.

Scott Mellish

AGCS 1014 Galaxy Cluster

AGCS 1014
AGCS 1014
Sketch and Details by Scott Mellish

AGCS 1014
Galaxy cluster
Octans
13/12/09
Ilford NSW Australia
56cm f5.0 Dobsonian telescope
Field: 15′
Magnification: 314x
Sky Quality Meter reading 21:72

White pen
White oil pencil
Soft white pencil

The far southern circumpolar constellation of Octans is not often considered rich in deep sky objects, at least not bright and pretty ones.

For the more adventurous observer there is a wealth of faint and fascinating galaxies scattered throughout the area to keep one engrossed for hours.

One such object is the remote Abell galaxy cluster AGCS 1014.
R.A: 22 23 47.9 DEC: -80 11 52.
This object is the most interesting of several extremely faint galaxy clusters that inhabit the region, and certainly the brightest one that is nearest the south celestial pole.

What is most rewarding with such little known objects is the fact that the observer may very well be one of only a handful of people on the planet to have seen it in a telescope.

Scott Mellish.