Triangulum’s Spectacular Spiral

M33 and HII Regions

M33 and HII Regions

By Kiminori Ikebe


From the English translation at Mr. Ikebe’s website:

M33 (NGC 598) Triangulum Galaxy – Difficulty Level: 2/5
NGC 588 Tri Star Cloud – Level: 5/5
NGC 592 Tri Diffuse nebula – Level: 4/5
NGC 595 Tri Diffuse nebula – Level: 4/5
NGC 604 Tri Diffuse nebula – Level: 3/5
Date of observation: 1998/11/14 21:55
Observing site: Makinoto
Transparency: 3/5
Seeing: 4/5
Sky darkness: 4/5
Instruments: 32cm Dobsonian and Pentax XL14
Magnification: 110x
Width of field: 0.6 degreeThis is a galaxy with a dynamic spiral arm.
The haze around the core is very faint and requires dark adaptation to see its extent. Once your eye is fully adapted, you will be surprised how extensive the haze is. NGC 604 is bright and located in the northeast of this galaxy. If you spend enough time, you will be able to detect this galaxy’s magnificent spiral structures as well as star clusters and nebulae such as NGC 588, NGC 592, and NGC 595 within the galaxy. The core is compact and elongated. At its center lies a small shining nucleus. There are two arms visible, one in the south and the other in the north; both are spiraled counter-clock-wise. The southern arm is divided into three regions. The northern arm is thin and broken off at places while embedded in haze. Other regions of the galaxy appear as faint haze.

NGC 604: Almost circular and small, but as bright as the center of M33.
NGC 595: A small faint object located near where the northern arm starts. The center of this object appears stellar surrounded by fuzzy nebulosity.
NGC 592: This object looks like a faint small spot.
NGC 588: It is located far from the center of M33 and easily missed. It is a much smaller spot than NGC 592.


Mr. Ikebe uses white pencil and “poster color” on black drawing paper. An extensive collection of his sketches can be found on the English section of his website. A larger collection can be found at the Japanese language site.

Tuning in to a Cloven Galaxy

NGC 5128

Fifteen million light years away in the constellation Centaurus lies the nearest radio galaxy, NGC 5128. Also known as Centaurus-A, it is categorized as an intermediate galaxy type, with qualities of both an elliptical (which describes its main body) and spiral galaxy (due to the prominent dust band encircling it). Loads of information about this fascinating galaxy can be found at the solstation website. This galaxy’s beautiful and unusual structure has been made famous through astro photographs, but it is also accessible to astronomical sketchers.

This sketch of NGC 5128 by Eiji Kato, was made at the Twinstar Guesthouse Observatory in Queensland, Australia. He notes: “As for my sketch of NGC 5128, it was made at Ballandean using my new 18″ f/4.5 (Galaxy Optics) mirror at 290x (Naglar 7mm eyepiece). It was drawn on white paper with black graphite, and then inverted after scanning. I am still working on this object for further refinement, but have to wait until next season as it is too low now.”

More of Eiji’s deep sky and comet sketches can be found in his gallery. (Note that a few of the links are broken, but don’t let that discourage you from viewing his excellent work.)

A Promenade Through a Royale Garden

IC 1396 

IC1396, a promenade through the Royale Garden.

One of the known highlights of Cepheus is Mu Cephei, a deep orange star. This night Mu Cephei served as the guiding light to IC1396. This region is a beautiful field of stars. There was something peaceful about this place. I felt like strolling through an exotic garden covered with haze. The place seemed majesticaly silent with Mu Cephei as a guard of honour at the border of the eyepiece. I don’t know if I saw IC1396 at all. I just noted all the light I could absorb in this field. A strange fact is that Mu Cephei kept his orange color through the UHC filter.

Date : October 13, 2007
Time : 21.00UT
Scope : Skywatcher 102/500
Meade SP 26mm
Power : x20
FOV: 150′
Filter : Lumicon UHC
Seeing : 3.5/5
Transp. : 3/5
Nelm : 5.3
Sketch Orientation : N up, W right.
Digital sketch made with PhotoPaint, based on a raw pencil sketch.

Rony De Laet
Belgium

Hiding In the Open

M33 

I found M33 a hard to find object in the past. I used to observe with long focal scopes. M33 never showed up in the eyepiece. Last year, I could finally detect the central part of this galaxy with my ETX105. This night, I was studying the milkyway in the Cygnus region with the Skywatcher for an hour or so. I wanted to end the observing session with a different type of object. I made a quick peek at M15 and M2 and then I turned my head to Andromeda and Triangulum. I aimed the scope to that spot where I could never find M33, just for fun. And there it was, in the middle of the low power eyepiece! I discovered the soft oval glow of M33. That was not so hard with this scope. I could not resist the urge to make a sketch of the scene. The Baader Contrast Booster filter joined in as well.

Date : October 13, 2007
Time : 22.00UT
Scope : Skywatcher 102/500
Meade SP 26mm
Power : x20
FOV: 150′
Filter : Baader Contrast Booster
Seeing : 3.5/5
Transp. : 3/5
Nelm : 5.4
Sketch Orientation : N up, W right.
Digital sketch made with PhotoPaint, based on a raw pencil sketch.

Rony De Laet
Belgium

An Extragalactic Pass in the Night

M51 

M51

I have been going through my sketchbook and finding those objects that I have yet to convert over to digital images. M51 (The Whirlpool Galaxy) is one of many that were in need of such treatment.

A fairly faint object due in part to the LP in this part of the sky from my location, it is nonetheless an impressive object when viewed through the EP. With averted vision, I was able to clearly see the overall shape and structure, but not a whole lot of finer detail(s).

Wade V. Corbei
Lodi, California

The Lord and the Leviathan

Lord Rosse M33 
This is a page from the observation/sketch notes of Lord Rosse, the 19th century Irish engineer and astronomer who built and operated the “Leviathan” at the time the largest telescope in the world, a 72″ metallic speculum mirror (actually there were two, one polished and ready for use and the other being polished and made ready to exchange when the first mirror started to show signs of tarnishing in the moisture prone weather of Birr Castle). This is just one page of many that Deirdre Kelleghan, the President of the Irish Astronomical Society, sent in to ASOD, Thanks Dee! We would also like to thank the the Webb Society for making these images available. Do you recognize this galaxy at the bottom of the page?

Rich Handy
ASOD Webmaster

Swing Your Partner

M51 

Arguably one of the finest galaxies for visual observation, M51 shows some structure
with averted vision under moderately light polluted skies. The core of the captured
dwarf galaxy hanging on to the edge of a spiral arm is quite apparent and makes M51
a favorite of many observers.
This sketch was rendered on Strathmore Windpower Sketch paper with a .5mm mechanical
pencil. MGI Photosuite III was used for post processing.

Jason Aldridge
North Port, FL

Ship of Stars on an Infinite Sea

NGC 6503 

2007 August 11, 0450 UT
Erika Rix
PCW Memorial Observatory
Zanesville, Ohio USA

NCG 6503

An Orion ED80 was used on an LXD75 mount, all of which were on antivibration pads in
the observatory.  The eyepiece was a Zhumell 21-7mm zoom and a WO dielectric
diagonal.

This sketch was done with Rite in the Rain paper, a number 2 and 0.3mm as well as
0.5mm mechanical pencils

Between the King and the Swan

NGC 6946 
Object Name: NGC 6946 (H.IV.76)

Object Type: Spiral Galaxy

Constellation: Cepheus

Right Ascension (2000.0): 20h 34.8m

Declination (2000.0): +60° 09′

Magnitude: 8.9

Dimensions: 11.5′ x 9.8′

Hubble Class: Sc

Telescope: Parks Astrolight EQ6 • 6″ f/6 Newtonian Reflector

Eyepiece: 7.5mm Parks Gold Series Plössl • 120x, 26′ FoV

Date & Time: 8 September 2007 • 04:15 UT

Seeing Conditions: NELM 6.3 • Pickering 8

Observing Location: Cuyamaca Mts., San Diego Co., California

NGC 6946 is a large face-on spiral galaxy on the Cepheus-Cygnus border.  The
constellation boundary runs north-south right through the center of the galaxy.
Most references and guidebooks place NGC 6946 in the constellation Cepheus, but
occasionally it will be listed in Cygnus (as is the case with Luginbuhl & Skiff’s
Observing Handbook and Catalogue of Deep-Sky Objects).  This galaxy is notable for
its proximity to open cluster NGC 6939 and the frequency with which it produces
supernovae (eight in the last century).  Like several other bright, nearby galaxies,
astronomers once considered NGC 6946 a possible member of the Local Group.  It is
now known to be a member of the Coma-Sculptor Cloud and is one of the nearest spiral
galaxies beyond the Local Group at a distance of 15 million light-years.

To locate this low-surface brightness spiral (its light is dimmed by about 1.6
magnitudes by it’s proximity to the plane of the Milky Way), center your scope on
3rd magnitude Eta (η) Cephei and look for the twin glows of NGC 6939 and NGC 6946
about 2° to the southwest.  The galaxy is the fainter of the two and lies 38′
southeast of the cluster.  At 30x magnification NGC 6946 appears as a subtle glow of
soft gray nebulosity in a rich star field, brighter toward the center with a poorly
defined perimeter.

Increasing the magnification reveals a very faint stellar nucleus embedded in a
moderately bright core, elongated north-south with a little counter-clockwise twist
at each end.  Surrounding the core is a slightly elliptical ring of nebulosity,
elongated northeast-southwest, but brighter on the northwest and southeast sides.
Beyond this ring, things start getting a little difficult.  Delicate strands of
nebulosity (spiral arm fragments) reveal themselves intermittently with averted
vision.

NGC 6946 was discovered on September 9, 1798 by William Herschel using his 18.7-inch
reflector; he classified it as a planetary nebula.

Eric Graff

Brightest Galaxy in Pegasus

NGC 7331 

  With the high pressure dry air mass moving out of Canada into the Midwestern
United States, we had a cool clear night for observing the night sky. I chose for
sketching the brightest galaxy in the constellation of Pegasus NGC 7331. This Sb
galaxy called a nebula by William Herschel in the late 18th century is 10’ x 2’ in
size as seen in the sky.  This spiral galaxy is somewhere between 43-49 million
light years away and glows at magnitude 9.7. NGC 7331 has been compared to our
milky way in size, spiral structure and general appearance. There are a number of
other galaxies fainter than 13th magnitude in the same field of view but
undetectable under my urban sky conditions with a 10” scope.
  
  
  Sketching:
  
  Date and Time: 9-12-2007, 3:20-3:50 UT
  Scope: 10” f/5.7 Dobsonian. 21mm and 12mm eyepieces 70x and 121x
  8”x12” white sketching paper, B, 2B graphite pencils, scanned and inverted, star
  magnitude adjustments using Paint
  Seeing: Pickering 8/10
  Transparency: above average 4/5
  Nelm: 4.9
  
  Frank McCabe