The Great Andromeda Galaxy and Her Attendants

Object Name M31/32/110
Object Type Galaxy, dwarf galaxy
Location la Ferme des étoiles, Gers, France
Date 16/07/2010
Media black paper, pastel
A nice night in an astronomy center. I didn’t have the time to make with precision the details, the periphery of the galaxy is less brighter than on the sketch and black region less dark too. The sky was nice, with a little bit light pollution. fujinon 25×150. Think’s to François Couturier who let me practice with this big binoculars !

clear sky,
Boris

Down the Whirlpool

NGC 5194/5195 (M-51)
The “Whirlpool Galaxy”
Interacting galaxies
24/05/06
Ilford NSW Australia
41cm f4.5 dobsonian telescope
Field: 23′
Magnification: x210
Canes Venatici

Black Canford paper
White pen
White pencil
White pastel chalk
Blending stump
Paint brush

What can I say about the Whirlpool Galaxy?

At my location Messier 51 is at a little over +47 deg, so it is about as far north as I can go without getting ridiculous, especially when there is a big chunk of glass sitting at the bottom of the telescope.
At this extreme declination I only require a modest chair to sit on as the object is so low in the northern sky.

I done this sketch in 2006 in my old 41cm dob, which was before I purchased a sky quality meter so information on the “seeing” conditions is a bit scant.

However the northern sky from my site always seems to look a bit hazy down low despite the fact that there is no major city in that direction except from the
rural township of Mudgee some 40km away.

I best leave any thoughts on my interpretation of NGC 5194/5195 for those who observe it far higher in the sky than me.

Scott Mellish

Dancing in the Virgo Supercluster

NGC 5566/5569/5560
Galaxies
Virgo
14/05/10
Ilford NSW Australia
56cm f5.0 dobsonian telescope
Field: 17′
Magnification: 354x
Sky quality meter reading: 21:38

Black Canford paper
White pen
White pencil
White pastel chalk
Fine tip paint brush

From the Realm Of The Nebulae comes this interesting trio of relatively bright galaxies.

From the top of the sketch we have NGC 5569 followed by NGC 5566 (Arp 286) and at the bottom is
NGC 5560.

Deep images show that these galaxies are interacting, with the dominant member being NGC 5566.

One of the best images of this little combination featured on APOD recently http://apod.nasa.gov/apod/ap100813.html
and shows them in all their glory.

Though I would have to say that sketching materials are a lot less expensive than fitting oneself of with CCD gear.

Scott Mellish

Light in the Heart of Darkness

Hi gentlemen,
I propose to day not a showpiece, but a part of it: the dark lane of NGC 5128, Centaurus A, aka The radio galaxy.
Most of the time, when they sketch this galaxy, amateur astronomers resume the dark lane by a black and narrow patch, with one or two details.
But if you can observe it through a big scope, under good skies, and at high power, you will discover a world in itself.
A river with a long and narrow island in the middle, several regions where the depth is strong, and consequently the color of the water in these parts totally dark, but other places with shallow water and the bottom visible in more or less grey color.
There are also some isolated settlements with small lights, and even a village with a hazy spot of non resolved lights on the north shore. A strange thing with this river is its two rivermouths, one at each end!
Of course, this is a rather poetic description, where stars are the lights of settlements, the opacity the consequence of the depth of the water, and so and.
But, really, it’s worth it: you might believe it if you stay a long time at the eyepiece, as I did with a 20” Obsession, at Tivoli Lodge, Namibia.
Have a good dream…
Bertrand Laville, from Marseille / France
www.deepsky-drawings.com

A Vision of Andromeda Galaxy

Hello friends,

A vision of M31 through a 40mm eyepiece. The view was fascinating.

Object Name: M31 Andromeda Galaxy
Location: Benacebada, Granada (Spain)
Date: 2010.07.09
Media: graphite pencil, white paper. Inverted with PS

Telescope: 16″ Dob. The observing conditions: with new moon, the seeing and transparency excellent.

I hope you like it!
Leonor


Visita nuestra web de Leonor y Fernando:
www.astronomadas.com

Swing Your Partner

Object Name: The Whirlpool Galaxy (M51, NGC 5194 – 95, Arp 85)
Object Type: Interacting galaxies
Telescope: 28 inch f/4 alt-az Newtonian
Location: Star Party, RTMC
Date: June 2009 to July 2010 (total of seven hours observing/sketching spread out over six nights)
Media: HB graphite pencil on white acid free Canson paper (8 inch x 5 inch sketch book). Inverted sketch created in Adobe Photoshop Elements.

Back in March 2009 I had perhaps my best view ever of the Whirlpool Galaxy, M51, but was too lazy to start sketching. It was a great sight – blazingly bright spiral arms full of star clouds, and the companion galaxy was wreathed in a veil of faint, “E” shaped nebulosity. Frankly, the amount of detail was a bit overwhelming to start a sketch.

That lost opportunity got me going however and I began my “big M51” sketch in June 2009 at the Golden State Star Party. I’ve continued adding detail at every opportunity since then.

My intent with this sketch was to see and accurately record as much detail as possible with my 28 inch f/4 alt-az Newtonian, and that I would take as long as needed to give it my best effort. After a total of seven hours observing over six nights, which were spread out over a year, I’ve come up with the attached sketch. There’s more to see so I anticipate adding a few more details over time.

I started off with a blank page in my 8 inch by 5 inch notebook. My notebook is more of a sketch book that I also take notes in so I like to start with a blank page – no eyepiece circles. This gives me the freedom to expand or contract my sketch and take notes as needed for a particular object. Because of M51’s size and amount of detail I used an entire 8” x 5” page for my sketch.

After observing the Whirlpool for about five to ten minutes at low to medium powers (105x to 253x) I began lightly sketching by starting at the brightest and most distinctive areas. I then extended the light pencil marks out until the basic form was captured. This took some back and forth to get the proportions correct, and involved one do-over. A good eraser was as valuable as the right pencil.

Once the full form was adequately sketched in I started paying attention to small scale details, again working from the brightest area outward. At this point I was using higher powers as the seeing allowed. Specifically, I used magnifications from 408x to 816x, but most of the time I was in the 408x to 438x range. To see the most stellar-like points I used 710x to 816x.

I built up the basic outline and filled in most of the major details within the first two hours of my sketch in June 2009. The next five hours of observing and sketching were spread out over four different nights in May and July 2010, and at times I used photos of M51 to help track down subtle and faint details that would have otherwise been missed. The most subtle detail I detected with without specific photographic aid were the dark lanes running on the inside of the main spiral arms. Also, two faint background galaxies (IC 4277 and IC 4278) are shown in the upper right area of the sketch. 4278 was fairly easy to see but 4277, the one on the far right, required a big effort with averted vision to detect. In deep photos this is a small edge on galaxy. SQM readings for my observing sessions ranged from 21.4 to 21.7.

My sketch was made almost entirely at the eyepiece, with only some blending of discrete pencil lines and cleaning up the star points done later.

Best of all this effort has inspired me to start a series of “big” sketches of my favorite objects. Currently in the works is an M33 sketch and I look forward to starting on the Trifid Nebula next spring.

Howard Banich

Distant Andromeda

The Andromeda Galaxy & Companion Messier 32

August 11th, 2010

Location: Connecticut, USA (in an orange/red zone)

Drawn with black, grey, and white graphite colored pencil on white paper, with a black uni-ball pen for stars. Photographed with a Panasonic DMC-TZ3 and imported to Photoshop for inverting and touchups.

At time of drawing transparency was below average and so I really had to work hard to eke out any semblance of detail in M31. Aperture helped – I used a 203mm Newtonian for this drawing, even so, the one dust lane was only visible with averted vision. You may notice a strange lack of stars in the field, there are two reasons behind this: one is that too many stars become a distraction and two is that I generally only use them as reference points for my sketch.

Paul Schneider

Interactions

Object name: NGC 4038/4039 (Arp 244), in Corvus
Object type: Interacting Galaxies
Location: Texas Star Party, Fort Davis, Texas, USA
Date: 12th May 2010
Media: Graphite pencil on white paper, scanned then inverted in
Photoshop Elements 6.0
Equipment: 36″ (91.5cm) f5 Dob, 13mm Televue Ethos (352x),
Conditions: NELM 6.9, Good seeing (Ant II), transparency II-III (where I
=excellent, IV = poor)

I was at the 2010 Texas Star Party and got the opportunity to use a
variety of large scopes, from an 18″ up to a 48″. This sketch of the
Antennae was made while observing with Larry Mitchell’s 36″ f5 Obsession.
Notes: Huge in the eyepiece, bright and full of detail. HII regions are
bright and the tidal tails are seen with relative ease. 4038 is the
larger of the two and its tidal tail is more obvious than that of 4039
which is barely seen.

Faith Jordan

Beautiful Collision

NGC 4038/4039
“The Antennae”
Interacting galaxies
Corvus
13/05/10
Ilford NSW Australia
56cm f5 dobsonian telescope
Field: 17′
Magnification: 354x
Sky Quality Meter reading: 21:35

Black Canford paper
White oil pencil
White pastel pencil
White pastel chalk
White pen
Blending stump

The interacting galaxies NGC 4038/4039 are always good value in any size
telescope.

In the 56cm dob there was subtle detail visible without using averted
vision, I just wished the sky conditions were a bit better on the night.

The the protruding “Antennae” that are so spectacular in images were not
visible (which is not surprising).

When you look at the magnificent HST image of this object with all its
associated colours, and then look at the object in a large aperture dob
at fairly high magnification, its shape and form is not too dissimilar.

Scott Mellish