Timocharis

2010 06 21, 0300 UT
Timocharis
PCW Memorial Observatory, OH, USA
Erika Rix
Zhumell 16”, 8mm TV Plossl, 225 x

Phase: 64.8
Lunation: 8.66. d
Illumination: 71.3%
Lib. Lat: 7°30’
Lib. Long: 4°47’
Az: 215°14’, Alt: 27°21’

This complex crater has a crushed central relief and the area was
completely enveloped with shadow. I could make out some of the western
terraced walls within the crater. Heinrich (9.5 km), B (5 km) and C (4
km), were very clear as well as a small portion of the wrinkle ridge to
the southeast. Timocharis was formed ~ 3.2 to 1.1 billion years ago
during the Erathosthenian period. Height is estimated to be 3110 meters.
Faint small rays can be spotted with decent seeing conditions.

Sketched scopeside on black Strathmore Artagain paper, charcoal, black
wax pencil, white Conte’ crayon and pencils.

Erika Rix

Eudoxus and Aristoteles from Either Side of the Pond

Aristoteles and Eudoxus
Eudoxus and Aristoteles
By Dale Holt and Frank McCabe

During my morning and Dale’s afternoon we were communicating back and forth by e-mail about sketching during our respective evenings. We realized at some point that we could possibly sketch the same lunar target albeit at slightly different times. We selected two dominant craters near the terminator, namely Eudoxus and Aristoteles.
Dale began sketching first with the moon in his western sky and with very little time he did a remarkable job in only 40 minutes using a 6 inch Apo refractor.
When Dale had finished his sketch and completed another of planet Saturn that is when I got started.
I was using a 10 inch dob and much higher magnification. I rotated my sketch 180° so north would be up as in Dale’s sketch. I should also add I spent more than 3 times as long sketching so I naturally captured more of the two craters whereas Dale got the wide view including the environs of Mare Frigoris.
Aristoteles is 87 km in diameter and a large Eratostherian era crater with just some minor central peaks and steep walls. Note the shadow changes on the floor because of the time interval between these sketches. Eudoxus is slightly smaller (70 km.) and younger as a Copernican era impactor and has steeper walls with shadow changes on the floor that are a little less evident.
That was fun let’s do that again soon when we both have equal time.

The evenings of May 19th 2010
The moon just a little under (UK) and a little over (USA) 6 days into lunation

Warmest regards from both of us
Dale Holt and Frank McCabe

Locations: Chippingdale Observatory, NE Hertfordshire, UK and Oak Forest, Illinois USA

Classical Crater

Lunar Crater Copernicus
Observed at Bristol UK

22nd May 2010 ; 22:50 using Nexstar 8SE

I love this crater. It’s what a lunar crater should be – full of
mystery, depth, extravagant structures and always changing.

Sketched at the scope using 2B, 4B and 6B on a field sketch pad
(white, medium surface cartridge). I use a colour gradation scale
(1-10) which I update later. The sketch is then scanned into
Photoshope where I blend the sketch onto a gray background as well
as cloning away the gradation figures. I add additional emphemeris
information using “Virtual Moon”.

Chris Lee

Craters: Guericke, Parry, Bonpland and Fra Mauro

On this last evening of Spring, I selected for sketching this region of the moon close to the terminator between Mare Nubium and Mare Cognitum. Four large craters noticeably damaged by low flying Imbrium ejecta formed the subject matter of this sketch. From south to north I sketched crater Guericke (59 km) with its flat lava flooded floor that opens to Mare Nubium. Crater Parry, smaller at 49 km in diameter is older than the former and also flat floored. The other two craters which look ghostly at high sun are larger, even older and share common walls with Parry. These craters are Bonpland (61 km.) to the west and Fra Mauro (96 km.) to the north of Parry. The wall of Parry encroaches on Bonpland and both together on Fra Mauro to betray the cratering sequence. The Apollo 14 landing site would be just beyond the bottom edge of the sketch. Thirty nine and a half years ago the late Alan Shepard Jr. and Edgar D. Mitchell were walking around at Fra Mauro while the late Stuart Roosa orbited the moon in the command module.

Sketching:
For this sketch I used: Black Strathmore 400 Artagain paper 9”x 14”, white and black Conte’ Pastel pencils and crayons, blending stumps, Pink pearl plastic eraser.
Telescope: 10 inch f/ 5.7 Dobsonian, 9mm eyepiece 161x
Date: 6-21-2010, 1:15-2:45 UT
Temperature: 20°C (68°F)
Clear, calm
Seeing: Antoniadi III
Colongitude: 19.5°
Lunation: 8.6 days
Illumination 70.6%
Observing Location: +41°37′ +87° 47′

Rűkl: Chart 42 and 43

Frank McCabe

Mercator and Campanus

Mercator and Campanus
Craters Mercator and Campanus
By Chris Lee

Observed at Bristol UK

23rd May 2010

This is my second sketch of a lunar feature. Trying to balance sketch shape accuracy and colour contours is not as straightforward as globulars/clusters! However it gives me something to attempt while we have these lighter evenings…

Sketched at the scope using 2B, 4B and 6B on a field sketch pad (white, medium surface cartridge). I use a colour gradation scale (1-10) which I update later. The sketch is then scanned into Photoshope where I blend the sketch onto a gray mottled background as well as cloning away the gradation figures. I add additional information using “Virtual Moon”.

Chris Lee

Timocharis

Timocharis
Timocharis Crater
Erika Rix

2010 06 21, 0300 UT
Timocharis
PCW Memorial Observatory, OH, USA
Erika Rix
Zhumell 16”, 8mm TV Plossl, 225 x

Phase: 64.8
Lunation: 8.66. d
Illumination: 71.3%
Lib. Lat: 7°30’
Lib. Long: 4°47’
Az: 215°14’, Alt: 27°21’

This complex crater has a crushed central relief and the area was completely enveloped with shadow. I could make out some of the western terraced walls within the crater. Heinrich (9.5 km), B (5 km) and C (4 km), were very clear as well as a small portion of the wrinkle ridge to the southeast. Timocharis was formed ~ 3.2 to 1.1 billion years ago during the Erathosthenian period. Height is estimated to be 3110 meters. Faint small rays can be spotted with decent seeing conditions.

Sketched scopeside on black Strathmore Artagain paper, charcoal, black wax pencil, white Conte’ crayon and pencils.

Pastel Moon

Moon
Full Moon
By Krzysztof Pieszczoch

Hi

I was waiting on this full Moon. It was my first experience with pastel crayon. I like sketching through the binocular 🙂

Object name: Moon
Object type: Moon
Location: Tarnów , Poland
Date: 27 May 2010 r.
Time: 21:30 UT
Artist: Krzysztof Pieszczoch (Astrokrzychu)
Equipment used: Binocular 16X50 (2″) FOV 4,25 deg. and 7X50 FOV 7,5 deg.
– white pastel and black paper

Weather conditions:
– warm evening
– beautiful clear sky

Yours sincerely,
Krzysztof Pieszczoch

Whole Moon in Pastel

Moon
Moon
By Roel Weijenberg

* Object Name: Moon
* Object Type: Moon
* Location: Deventer, The Netherlands
* Date: May 25, 2010
* Media: White pastel pencil on black paper

Yesterday the Moon was very low in the sky (maximum altitude 20 degrees) so I couldn’t see him from my backyard. So I took a very old 60mm f/6,9 refractor inside the house, placed it on a EQ-1 on top of my desk. At 32x the Moon was a nice bowl, almost full. I sketched it with a white pastel pencil on black paper. The disk on the paper was approx, 5″ in diameter. It took me about 30 minutes to complete this sketch. Next time I’ll probably use a larger disk to draw finer details, but this was my first try using white pastel on black paper so I’m pretty satisfied for now.

Kind regards,

Roel Weijenberg

Lunar Crater Prinz and Montes Harbinger

Crater Prinz
Lunar Crater Prinz and Montes Harbinger
By Ferenc Lovró

I was just cruising around the terminator of the Moon, testing the new cooling equipment on my OTA, when I found a very interesting mountain chain with some ruined crater at one end, near the crater Aristarchus which was right on the terminator. The view was so spectacular, that I decided to make a sketch. I found out that the large crater was Prinz, and the mountains attached are Montes Harbinger. I’ve sketched some additional minor craters nearby that have been cropped out from this image. A really unusual view, worth taking a peek when it’s near the terminator!

Also known as: Prinz, Krieger C, Vera, Angström, Montes Harbinger, Rimae Prinz
Date/time: 2010.03.26 20:00 UT
Equipment: 12″ f/5 Newtonian
Magnification and filter(s): 300x + 15% neutral filter(s)
Seeing: 2/10 Transparency: 4/5
Location: Nádasdladány, Hungary
Observer: Ferenc Lovró

Gibbous Moon With Sinus Iridum Detail

Gibbous Moon
Moon – Gibbous With Sinus Iridum Detail
By Mark Seibold

Technical Information regarding sketch:

A 19″ X 25″ pastel sketch [with the moons disc drawn at 12 ¾”] on black Strathmore Artagain pastel paper with use of various soft to hard pastel chalks on December 26th 2009 at 5UT ~ 9UT, partly produced from direct eyepiece observation over 2 to 3 hours, then finished indoors with photos taken from the eyepiece to produce a detailed close-up of the Sinus Iridum feature at the terminator. An artists conception was added at bottom as a final touch for a total work time of 4 ~ 5 hours. Observation was through my 10.1 inch f/4.5 Newtonian telescope with use of 32mm, 12mm, 9.7mm Super Plossls and 6mm Orthoscopic eyepieces. Ambient outdoor temperature in the 750 ft elevation foothills, west of the Cascades and Mount Hood, 30 miles east of Portland Oregon was approximately 34 degrees F. Wind gusting to 20 ~ 30 mph and subsiding to still at times.

*A slightly higher quality image may be viewed at
http://i10.photobucket.com/albums/a109/markseibold/Moon_PastelGibbous6_SinusIr.jpg.