Sparkling Lagoon

M8 

14th June, 2007., around 21:00 UT
Petrova gora, Croatia

Last night I had another opportunity to observe. But this time, we went
to the Petrova gora, mountain maybe 1000 ft high, about 40 miles South
from the Zagreb and 20 miles South-East from the Karlovac (pop: 60 000).
Light pollution is still evident on northern horizon but to the South,
skies are beautiful. NELM near zenith was 6.10, not much difference from
the best night in my backyard (NELM 5.80) but big difference is that
there is no glare from street lamps and glow from nearby populated
places so sky is much darker. Watching MW composed from many clouds,
with few bright spots (M24, M8, M25), seeing M7 by naked eye is
wonderful feeling. Statement that there is no substitute for dark skies
hold very well. Of course, I used this opportunity to make more
sketches. I hope you will like results.

My process of creating sketches goes like this:
First, I observe and draw field sketch, full of notes, corrections and
other helpful stuff. After returning to house, I redraw all sketches to
include missing details, remove errors and to get better contrast under
white light. Next step is scanning of sketches. Afters scanning, I do
further adjustments of contrast in the Photoshop and add circle
representing that represents FOV. Last thing is description and saving
sketch in .tff and .jpg format.

I’m sketching on plain A4 paper with graphite pencils of different
hardness.

Vedran Vrhovac

Eight views of the Great Opposition of 2003

Mars composite 

This series of sketches covers my observations of Mars around the opposition
of 2003. Various telescopes were used including a 105mm Astro-Physics apo, a
200mm TEC Fluorite apo, a 13-inch Merz Refractor (circa. 1859, Herstmonceux,
Sussex, England) and a 28-inch Grubb Photo-visual Refractor (circa. 1893,
Royal Observatory, Greenwich, England). Simple graphite sketches with colour
notes were carried out at the eyepiece, generally over a 30 minute to one
hour period, these coloured pencil sketches then being drawn as soon as
possible afterwards. Interestingly the same sort of view is distilled out of
each observation regardless of the aperture being used!

Though the view didn’t appear to change very much from one evening to
another, the shrinking southern polar cap and changing phase of Mars is
distinctly seen over the three month observing period. My personal challenge
for the current Mars apparition is to catch the gibbous phase BEFORE
December 2007 opposition as well as afterwards.

The disc diameter of the sketches (image flipped to the correct orientation)
is approx. 5cm, and south is up.

Sally Russell

Fractured floor and a rim shot

Taruntius with Cameron on its Rim 

Crater Taruntius with Cameron on its Rim

Between southern Mare Tranquillitatius and northwestern Mare Fecundatatius lies the Copernican period crater Taruntius (57 km). This crater was some distance from the terminator but with surrounding smaller craters showing deep shadows, it is clear that Taruntius is a shallow crater. Note the deep shadow in Cameron (12 km) on the northwest rim of Taruntius. In addition to Cameron other rim features include breaches to the north and south along the rim and interesting rough ramparts to the lava floor beyond the crater especially southward. This floor fractured crater presents a small central peak surrounded by dark ash deposits from volcanic activity on the crater floor.

Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’
pastel pencils and a blending stump. Brightness was slightly decreased after scanning.
Telescope: 10 inch f/ 5.7 Dobsonian and 6 eyepiece 241x

Date: 6-20-2007 1:15-1:50 UT
Temperature: 21° C (70° F)
Clear, calm
Seeing:  Antoniadi III
Colongitude: 326.2 °
Lunation: 4.9 days
Illumination: 26.6 %

Frank McCabe

Our galactic dance partner

Andromeda Galaxy 

Andromeda galaxy
 
This sketch of the Andromeda galaxy (M31) was done on a very clear, transparant
night in November 2006 with my 8” f/5 dob. M32 was always visible as an out focus star. M110 was visible too, but very faint. I could get an image of the three in my GSO superview 30mm. the sketch was done using the 24 & 15mm panoptic eyepieces. I think I saw 1 and perhaps a second dustlane in the galaxy.
 
The sketch was done with pencils on standard printerpaper, scanned and inverted the
colors. Only the brightness is increased a bit trying to imitate the background glow
of the sky, making the sketch more realistic I feel.
 
Sketched on the 26th November 2006 from my home in Bornem, Belgium. I used my 8” f/5
dob at 33x (30mm gso superview), 42x (24mm panoptic) and 66x (15mm panoptic).

Kris Smet

Cat’s Eye in a dracon’s hand

NGC 4563

Cat’s Eye Nebula

One of the better known bright summer planetary nebulas in the constellation of Draco is NGC 6543. This blue-green planetary appears to be about one third of a minute of arc across, although its “outer corona” brings it out to about six arc minutes. The brightest part of this “outer corona” is IC 4677. None of this outer region can be seen from my urban site. The glow around the dying, hot, type O central star (or perhaps close binary pair) appears homogenous. None of the curlicue compressed gas loops were visible that can be seen in photographs. Some darkness was seen around the tenth magnitude central star. At a visual magnitude of 8.1 and at a distance of somewhere between 3300-3600 light years, this thousand year old planetary nebula looks great in telescopes much smaller than 18 inches.

Sketching:

Date and Time: 6-17-2007, 518-5:50 UT
Scope: 18” f/5 Dobson Ian. 12mm, 9mm eyepieces 191x, 254x
8”x12” white sketching paper, B, 2B graphite pencils, light brown colored pencil for nebula, scanned and inverted, contrast mean value adjustment using Imageenhance, star magnitude adjustments using Paint
Seeing: Pickering 7/10
Transparency: poor 2/5
Nelm: 3.9

Frank McCabe

With family in tow

Saturn and moons 

Saturn & family

When I pointed my scope at Saturn at the evening of the first May 2007 I was kindly
surprised to see 5 of the Saturnian moons all on one side of the planet!
From left to right and with their magnitude: Titan(M8.4), Iapetus (M10.6), Rhea
(M9.8), Dione (M10.5) & Thetys (M10.3).

For sketches of planets I mostly use Orthoscopic’s, for this one I used the 4mm wich
gave me 250x power.

The sketch was done on standard A4 printerpaper with a template of Saturn printed on
it. I then scanned it and added a grey background and the 5 moons in Microsoft
Paint.

Sketched on the 1st May 2007 from my home in Bornem, Belgium. I used my 8” f/5 dob
at 250x through a 4mm University Optics Ortho eyepiece.

Kris Smet

Namibia Globular

NGC 6388 

Globular clusters display distinct “personalities” to an attentive observer. Some
appear as pale, starless discs in large aperture telescopes while others, like Omega
Centauri, begin to resolve in small refractors. Less frequently, they will display
subtle color. My sketch of NGC 6388 in Scorpius is an example of this. Using the
Sossusvlei Mountain Lodge 12″ Schmidt-Cassegrain with a 31mm Nagler (~100x), the
globular’s star-like core appeared to be weakly yellow. The tint disappeared at
higher magnification (250X/12mm Nagler).

The original drawing was done at the eyepiece using a soft lead pencil. I prepared a
copy based on this drawing and my field notes. First, a “smudge” of graphite was
dotted with acrylic ink. A garden variety Bic pen with blue ink formed the core —
and when color inverted — captured my visual impression of the yellow color fairly
closely. The nucleus was then enhanced with Photoshop and the entire drawing blurred
to simulate the rather poor resolution caused by the seeing conditions.

Dave Riddle
Smyrna, Georgia USA

Terrific Trifid

M20 

Emission Nebula M20

14th June, 2007., around 21:30 UT
Petrova gora, Croatia

Last night I had another opportunity to observe. But this time, we went
to the Petrova gora, mountain maybe 1000 ft high, about 40 miles South
from the Zagreb and 20 miles South-East from the Karlovac (pop: 60 000).
Light pollution is still evident on northern horizon but to the South,
skies are beautiful. NELM near zenith was 6.10, not much difference from
the best night in my backyard (NELM 5.80) but big difference is that
there is no glare from street lamps and glow from nearby populated
places so sky is much darker. Watching MW composed from many clouds,
with few bright spots (M24, M8, M25), seeing M7 by naked eye is
wonderful feeling. Statement that there is no substitute for dark skies
hold very well. Of course, I used this opportunity to make more
sketches. I hope you will like results.

My process of creating sketches goes like this:
First, I observe and draw field sketch, full of notes, corrections and
other helpful stuff. After returning to house, I redraw all sketches to
include missing details, remove errors and to get better contrast under
white light. Next step is scanning of sketches. Afters scanning, I do
further adjustments of contrast in the Photoshop and add circle
representing that represents FOV. Last thing is description and saving
sketch in .tff and .jpg format.

I’m sketching on plain A4 paper with graphite pencils of different
hardness.

Vedran Vrhovac

Two great philosophers meet on the Moon

Aristoteles and Eudoxus 

Aristoteles and Eudoxus  

  
Warm moist air from the south and cool dryer air from the north have been battling it out over the Chicago area for the last week. This morning the cold air was winning as the thermometer in my yard was reading 47°F. Fortunately the cold high pressure air mass was accompanied by better than average seeing and transparency.

The 20 day old waning gibbous moon was about 30° above the southern horizon at an hour and a half before sunrise. For sketching targets I chose Aristoteles and Eudoxus along the northern terminator. The view in my 10” f/5.7 Newtonian held up well at both 241X and 362X. I sketched at the eyepiece using both magnifications. Twin peaks on the floor of Aristotles were visible with the southeastern most peak surrounded by shadow. This 90 km Eratosthenian crater was displaying nicely terraced wall on the steep eastern side. Off to the terminator side (east) and overlapped by Aristoteles is the shadowed floor crater Mitchell (31 km.) an older Imbrian formation. Further north along the terminator margin is rim illuminated crater Galle which stretches 22 km in diameter and is about the same age as Aristoteles. The other large and younger crater to the south is Eudoxus (70 km.) which also has steep terraced walls. A small part of the Caucasus mountain range can be seen west and southwest of Eudoxus. Due west of Aristoteles the ancient eroded  ghost-like crater Egede at 37 km in diameter can be seen in contrast to the younger craters named above.
   
Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’ pastel pencils and a blending stump.  Brightness was slightly decreased after scanning.
Telescope: 10 inch f/ 5.7 Dobsonian and 6 and 4 mm eyepiece 241 and      362X
Date: 6-6-2007 9:05-10:00 UT
Temperature: 8° C (47° F)
Clear, calm
Seeing:  Antoniadi II-III
Colongitude: 158.7 °
Lunation: 20.6 days
Illumination: 72.7 %
   
Frank McCabe

Kemble’s Cascade

Kemble’s Casade

Here is an observation with a low power scope at x14 (made on 2/15/07 around 21.45
UT). The fov is 3.8°. The small ETX is great for rich field views. The object is
easy to find with a pair of bino’s when going straight up from Algol to Mirphak and
continuing for about 9 degrees. The cluster at the end of the cascade did not reveal
much detail with this power, but I only wanted to give a general impression of the
scene. High clouds were interfering my site, and with my limiting magnitude.

The raw sketch was made at the EP with a HB mechanical pencil. The final sketch was
digitally rendered in Photopaint (thus eliminating the tedious scanning procedure).
North is up, matching a binocular orientation.

Rony De Laet

http://www.geocities.com/rodelaet, my personal website.