This was one of those nights things just fall together. Excellent seeing and light enough from the Moon that I could see the paper well. After finishing my sketch at the eyepiece I went inside to clean it up and was pleasantly surprised that I liked it pretty much the way it was.
110km wide Gassendi Crater showed some excellent roughened floor details with hummocks casting shadows as well as floor rilles illuminated as bright & dark lines. Rima Mersenius is brilliantly lit on the terminator and the bright scarp of Rupes Liebig can be seen at the base of the wall.
Gassendi Crater, Mersenius Rille, Rupes Liebig, Mare Humorum @11.7 days lunation
.12/2/14 2030-2140 HST
12.5″ Portaball, 227x
Canson Black paper and white and black Conte’ Crayon, white charcoal pencil
Photoscape to adjust contrast
Cindy (Thia) Krach
Haleakala Amateur Astronomers
Object Name: Gassendi
Object Type: Lunar Crater
Location: Dunboyne Ireland
Date: 4th October 2014
Media: Graphite pencil H2, H3 & B6 with standard white stock and technical drawing equipment.
This is actually sketched as observed through the eyepiece with a 15mm on a 9.25 SCT rather than from the phone screen. The seeing was fair but a weather front was fast approaching and just managed to observe long enough to capture this detail. At the same time I took some snapshots through the eyepiece with my smartphone for a smartphone astronomy site – so got to do both before the clouds rolled in. Adding the phone to the sketch allows me to add a technical drawing into the mix which I not (only) enjoy but also allows me to capture the evenings activities and optical equipment used during the session.
Here is a sketch of the Moon on the 5th of September from my backyard
in Adelaide, South Australia.
The moons phase was waxing at 83%, with only the very western edge
still in shadow. I observed with a C11 SCT. Seeing was quite
reasonable, so I took a 15mm eyepiece + 2x Barlow for a close look.
The shallow illumination on Mare Humorum made the creases on the mare
floor stand out. Crater Gassendi, toward the bottom, showed stark
shadows. Rimae Hippalus was visible, passing through the partially
submerged crater Hippalus at the top right. Because I used a diagonal
prism, the sketch is mirror imaged.
I used pastel chalks and black and white pastel pencils on black
Object Name Sinus Iridium
Object Type Lava plain on the Moon
Location Deventer, the Netherlands
Date April 13, 2011
Media White pastel on black paper
I have made a pastel sketch of one of the features on the Moon which beauty always strikes me whenever it’s visible: Sinus Iridium (Bay of Rainbows). It is a very large feature and always looks very nice in even the smallest telescopes. On that evening of April 13 the Sun’s angle was just right to give the surface that gradient view: dark near Montes Jura with a gradual brightening towards the west. A few rilles were also visible. It was a very pretty sight through my 300mm f/4 truss Dob using a 5mm HR Planetary eyepiece (240x). The sky was a bit hazy while I made the sketch, but the seeing was great.
On a beautiful spring evening with mostly clear, warm skies, I was able to sketch the famous fourth ring of the Nectaris basin, namely, the Altai scarp or Rupes Altai. Sunlight was bouncing off the outermost visible rim of this combination basin ring / fault enhancing its visibility north of impressive crater Piccolomini (88 km.) and beyond for 500 kilometers. Some of the sheer cliffs are 3.5 – 4 km.high and are nicely treated and described in Steve Bounce’s interesting study and profile in Selenology Today #10, June 2008.
What was also eye catching about this view was the fine illumination and shadow on the terraces of crater Piccolomini. The 2 km. tall central peaks of this crater above its smooth floor added to the grandeur of the eyepiece view.
Sketched on white paper using graphite pencils (HB, 4B, 6B), blending stumps, white Pearl erasers
10” f/ 5.7 Newtonian riding on an equatorial platform and a 6mm eyepiece for 241x
Date and Time: April 10, 2011, 01:50-02:40 UT
Weather: partly, calm, 65 degrees F (18 degrees C)
Seeing: Antoniadi II-III
Lunation: 6.4 days
Moon 34.8% illuminated
Mare Crisium is that interesting isolated sea on the northeastern side of the visible lunar surface. Only about half of it was visible during this sketching session.
The Nectarian Period event that formed this feature occurred more than 3.8 billion years ago. The mare portion of the basin is about 500 kilometers across. In the grazing sunlight across the floor, wrinkled ridges were visible in the north to south direction. Also on the western floor craters Picard (24 km.), Peirce (19 km.) and Swift (11km.) stood out in the low light. I could clearly see the lighter colored bench lava that partly buried craters here such as Yerkes (37 km.). Tall flat top mountains (massifs) beyond the shore stand at 2-5 kilometers above the sea. Also beyond the sea to the West crater Proclus (28 km.) with its remarkable bright rays was reflecting some sunlight.
For this sketch I used: 400 series black Strathmore Artagain paper 9″x 12″, white and black Conte’
pastel pencils , and Conte’crayons, a blending stump, plastic eraser. Brightness was decreased -2 and contrast increased +1 using the scanner for this sketch
Telescope: 10 inch f/ 5.7 Dobsonian with 6mm (241x)
Date: 12-23-2010 10:00 – 11:30 UT
Temperature: -8°C (18°F)
Weather: clear, calm
Seeing: Antoniadi III
Co longitude: 120°
Lunation: 17.7 days
Staring down the telescope eyepiece last night, I saw the terminator crossing Mare Crisium in such a way that all the main basin rings were visible. That only left the challenge of illustrating them in a sketch; not an easy thing when you consider the breadth of lunar landscape they cover and the amount of detail they include. So: from inner to outer here they are – can you spot them all?
1. The inner wrinkle ridge just inside and parallel to the Mare border (Dorsum Oppel).
2. The mountainous terrain of the mare border itself.
3. The Cleomedes ring. Cleomedes is the large terraced crater to the north of the Mare and partially in shadow. You can identify the high ground surrounding it by virtue of the low ground either side. To the south of the Mare this low ground is also visible in amongst the more jagged mountains.
4. The Geminus ring. Geminus is the large crater at the top of the drawing totally in shadow. A ring of slightly higher ground arcs right round the north of the mare, with a gap to the west, then rejoins as the mountains to the Mare’s south.
The multiple rings of Crisium are quite obvious once you know they are there, so it’s amazing how it took the Lunar Orbiter images of Mare Orientale to really focus the hunt for similar features on the lunar near-side. I drew this in about 40 minutes, finishing it quickly mainly because I was cold and tired. But I also find that forcing myself to sketch fast helps me to focus on observing the main features first and getting them down on paper.
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.
Lunar craters Mairan, Sharp, Harpalus and the Jura Mountains Sketch and Details by Frank McCabe
The lunar feature known as the Jura Mountains includes the rim of the Sinus Iridium impact and is visible here in late day sunlight. The debris field can be seen extending westward to Mare Frigoris. All of Sinus Iridium is in shadow which gives this region an unfamiliar appearance. The impact that created the large mountainous debris field occurred during the Upper Imbrium period (3.8 billion years ago). Some of the mountains are a lofty 5 kilometers high. Superimposed on these mountains are two forty kilometer complex craters known as Mairan and Sharp; another similar sized crater can be seen on Mare Frigoris and is called Harpalus (39 km.). At high sun this crater shows a bright young crater ray system in addition to a fine glacis. There are 3 pillow-like features to the far left in the sketch at the edge of the Iridium ejecta. The two that are closest together are the famous large lunar domes known as Gruithuisen Gamma and Delta.
It is always worth while when not expecting a rigorous day ahead to get up a little earlier than usual to see what is going on in the sky before sunrise. This is especially true when the sky is clear and very transparent.
For this sketch I used: black Canson paper 9″x 12″, white and black Conte’
pastel pencils , and Conte’crayons, a blending stump, plastic and gum erasers. Brightness was decreased -2 using the scanner for this sketch
Telescope: 10 inch f/ 5.7 Dobsonian with 9mm (161x) eyepiece
Date: 11-12-2009 11:00-12:00 UT
Temperature: -3°C (27°F)
Clear to partly cloudy, calm
Seeing: Antoniadi III
Co longitude 212.7°
Lunation days 25.27
Seeing: Very turbulent with intermittent stillness.
The Montes Rook and Cordillera with labelled features Sketch and Details by Peter Mayhew
The moon was 14 days old and this part of the south west limb was the only region under contrast. Craters were only visible when close to the terminator, or if rayed or darkened with basalt flows. The mountain peaks stood out perfectly in moments of stillness. The three concentric mountain rings around the (not-visible) Mare Orientale were clearly defined. I include a labelled version.
Mare Humorum, the “Sea of Moisture” Sketch and Details by Frank McCabe
One month ago (August 15) I began a sketch I was unable to complete due to interfering clouds and lucky for me early on the morning of September 13 with the moon at approximately the same phase, I completed the graphite sketch of most of the mare Humorum basin (380 km.). This impact basin is a different shape and somewhat smaller in size than Marie Crisium (600 km.). Research mapping data puts the age of this sea at about 3.9 billion years, a Nectarian period formation. The floor is flooded over by a thick layer of basaltic lava especially over the central region. Additionally a number of large interesting craters ring the margins of this basin. At the southern edge (12 o’clock position in the sketch) you can see craters: Vitello, Lee and Doppelmayer. At the north edge (6 o’clock position) you can see crater Gassendi and on its rim Gassendi A. The lighting on both occasions was excellent for viewing the lava ridges on the eastern side of the maria. Both days were excellent for viewing a steady lunar image with a notable amount of fog on the second viewing morning.
Sketch was made over two observing sessions
For this sketch I used: white sketching paper 10”x 8”, HB, 4B, 6B graphite pencils, a blending stump and a plastic eraser and eraser shield. After scanning, Brightness was decreased (-2) and contrast increased (+2) using Microsoft Office Picture Manager.
Telescope: 10 inch f/ 5.7 Dobsonian and 6 mm eyepiece 241x
Dates: 8-15-2009, 9:30-10:25 UT; 9-13-2009, 10:00-11:10 UT
Temperature: 15° C (59° F), 16° C (61° F)
clear, calm, then cloudy the first day, Very humid both days, dense fog on the second day
Seeing: Antoniadi II-III
Colongitude 205.5°, 200.2°
Lunation 24.27 days, 24 days
Illumination 32.7 %, 35.3 %
Lunar crater Gassendi on the shores of Mare Humorum Sketch and Details by Richard Handy
One hundred and fourteen kilometers in diameter, filled with rilles and a rich variety of terrain, Nectarian era Gassendi sits on the northwestern shores of Mare Humorum in the South West Quadrant of the Moon. Gassendi is a great example of a FFC (Floor Fractured Crater). Why is it fractured? Well, the real lowdown on the rilles is that they are created by magma that finds its way to the surface through weaknesses and fissures in the breccia beneath Gassendi. As the magma fills these volumes, it pushes up on the material on the crater floor causing these characteristic fractures in the surface and in the process providing a vent for lavas. The really amazing thing was the number of rilles on the floor that were bifurcated, some seemly splitting at obtuse angles while others paralleled the rim. I could sense that there was a level of detail hidden by the seeing, a larger population of smaller rilles awaiting that moment of perfect clarity to reveal themselves. However with Antoniadi III as my average, it wasn’t going to be tonight. On the northwestern wall of Gassendi resting on its northwestern margin, much as Gassendi is to Humorum, is 33 km Copernican era, Gassendi A. Above and to the northwest is the 26 km flat floored Gassendi B. I wonder how much is floor fill is from his bigger and (younger?) brother to the south, the result of slow and steady mass wasting or a carpeting of material from a larger event. The whole area to the north and west of Gassendi seemed to be filled with these arcuate grooves. Towards the southern sunken rim of Gassendi, the northwest part of a Basin rim seemed elevated above the Mare as it rose to meet a collapsed section of Gassendi’s rim in the middle of the western outer wall. I could tell the area to the west of this arc had a different texture to the terrain, as if they were only partially submerged in the mare lavas. There were arcuate rilles here as well, paralleling the Basin. I hoped you all enjoyed this, I know I had a rille wonderful time sketching this one and sharing it with you.
Here are the sketch details:
Subject: Gassendi and environs Atlas: Rukl 52
Date: 9-3-06 Start time 4:20 UT Ending time: 5:56UT
Seeing: Antoniadi III with moments of II every 3-5 min, Weather: clear to partly cloudy
Lunation: 11.38 days Colongitude 46 deg Phase: 49.9 deg
Illumination: 82.2 % Lib. in Lat. : +6 deg 28 min Lib. in Long.: – 6 deg 53 min
Telescope: 12″ Meade SCT F10
Binoviewer: W.O. Bino-P with 1.6X Nosepiece
Eyepieces: W.O. 20mm WA Plossls
Sketch medium: White and black Conte’ on Black textured Conte’ paper
Sketch size: 18″ x 24″
Mare Crisium Sketch and Details by Aleksander Cieśla, text by Rich Handy
This superbly drawn sketch of Mare Crisium by Aleksander Cieśla shows that the 638 Km
Nectarian aged Sea, even during Full Moon, still displays details such as its platform
massifs, isolated mesa like formations, and its circular scarps that identify it
as a Multi Ring Basin.
Object: Moon – Mare Crisium
Scope: Schmidt-Cassegrain 5” + Speers-Waler 7,4mm
Place: Poland, Wroclaw – near city center
Weather: Good. Seeing 7/10. Light Pollution.
Date: 12 January 2009
Technique: White pastel crayons on black paper
Tooling: Contrast and gamma levels only
Lunar Basin Bailly Sketch and Details by Frank McCabe
The terminator was approaching the southwestern limb of the moon as the basin Bailly, nicely visible due to favorable libration, came under full illumination. Bailly is large for a crater but small for a ringed basin at 300 kilometers in diameter. In the grazing sunlight the irregular basin floor with numerous craters was evident but no sign of the inner crater ring was visible as can be seen in overhead spacecraft images. The far side inner wall was beautifully illuminated in direct sunlight while features beyond were in total darkness. The depth of this basin is about 6 kilometer below the rim. The two large bright rimmed craters at the south end of Bailly’s floor are first older Bailly B at 65 km. and then younger Bailly A at 38 km. Also notable in this view is a portion of a bright ray of ejecta traceable back to Tycho (not in the drawing) and crossing crater Kircher (75 km.) before reaching the south end of Bailly. The 3 large craters below the Tycho ray are in descending size: Bettinus (73km.), Segner (70km.), and Zucchius (66 km.) which is the youngest of this group of craters.
This was the first evening the moon has been visible from my location since this lunation began. Although a little bit on the chilly side for sketching, it was a pleasure to get out and draw the moon again.
For this sketch I used: black Strathmore 400 Artagain paper 9”x 7”, white and black Conte’ pastel pencils and a blending stump. After scanning, Brightness was decreased (-2) using the scanner.
Telescope: 10 inch f/ 5.7 Dobsonian and 9 mm eyepiece 161x
Date: 12-11-2008, 5:15 – 7:00 UT
Temperature: – 3°C (26° F)
Seeing: Antoniadi III
Colongitude 73.1 °
Lunation 13.58 days
Illumination: 97 %
Libration: in Lat. -6° 3’, in Long. -3° 45’