White Conté on Black Paper – Page 2 – Astronomy Sketch of the Day

Posidonius and Northern Serpentine Ridge

With the first clear night in more than one week, I was able to catch the sunset across crater Posidonius (99 km) at the northeastern edge of Mare Serentatis. Posidonius A (11 km.) , the highest of the small central peaks and the tilted and uplifted concentric ridge were the last features catching the light at sunset inside the rim. Also visible and included in this sketch was the northern most portion of Serpentine Ridge. As temperatures were falling throughout the night, I found myself stopping to warm my hands indoors not once but several times. The lunar viewing was excellent this night.

Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’ pastel pencils and a blending stump.

Telescope: 10 inch f/ 5.7 Dobsonian and 9 mm eyepiece 161X
Date: 01-02-2013: 04:30 – 06:00 UT
Temperature: – 16° C (2° F)
Clear, calm
Seeing: Antoniadi III
Colongitude: 150°
Lunation: 19.83 days
Illumination: 79.6%

Frank McCabe

Craters Lansberg and Reinhold

Both of these craters look similar when their floors are in shadow as was the case when I viewed them. Lansberg (40 km) is a walled plain crater sitting where Mare Insularum meets south Imbrium. This old impact dates back to the Upper Imbrian and is near the center of my sketch. Reinhold (49 km) is a prominent lunar impact crater of the Eratosthenian period and is also on Mare Insularum. It is below Lansberg near the bottom center of the sketch which by direction is north as per the inverted Newtonian telescope view. At the top of the sketch (south) I was able to catch the Riphaeus Mountains receiving first light during this waxing gibbous phase.

Sketching:

For this sketch I used: black Canson paper 9″x 10″, white and black Conte’ pastel pencils and blending stumps. Sketch was scanned

Telescope: 10 inch f/ 5.7 Dobsonian and 6 mm eyepiece 242x
Date: 10-25-2012, 00:30 – 01:25 UT
Temperature: 16°C (60° F)
hazy, high clouds, calm
Seeing: average Antoniadi III
Transparency: poor
Colongitude: 29.0 °
Lunation: 9.52 days
Illumination: 79.0 %

Frank McCabe

The Modified Crater Heraclitus

The southern lunar highlands expose the ancient anorthositic crust between craters. Centered in this southern highland sketch is the buried pre-Imbrian crater Heraclitus (92 km.) with its unusual central mountain crest. This ridge or crest looks much like the one on the floor of the elongated crater Schiller formed during its shallow angle impact. The ends of Heraclitus are buried under Licetus (77 km.) to the north and Heraclitus D (52 km.) to the south. Its easy to imagine this possible Schiller twin here partly hidden. To the east is crater Cuvier (76 km.) with its smooth floor and western wall pressing in on Heraclitus.

Sketching:

For this sketch I used: black Canson paper 9″x 12″, white and black Conte’ pastel pencils and blending stumps. The scanned sketch is unmodified

Telescope: 10 inch f/ 5.7 Dobsonian and 4 mm eyepiece 362x
Date: 09-24-2012, 00:15 – 01:50 UT
Temperature: 10°C (50° F)
clear, calm
Seeing: average Antoniadi III
Colongitude 11.3 °
Lunation 7.9 days
Illumination: 63.5 %

Frank McCabe

Western rim of Mare Crisium

Mare Crisium (Move mouse over image to view labels)

2012 09 04, 0330 UT – 0615 UT Mare Crisium
Erika Rix, Texas – www.pcwobservatory.com

AT6RC f/9 1370mm, LXD75, Baader Planetarium Hyperion 8-24mm Mark III (FOV 68 degrees at 171x), no filter
84F, 56% H, winds gusting 5-10 mph, clear, Antoniadi IV increasing to II, T 3/6
Alt: 11deg 43´, Az: 83deg 22´ to Alt: 46deg 21´, Az: 105deg 21´
Phase: 318.4 degrees, Lunation: 17.48 d, Illumination: 87.4%
Lib. Lat: -03:07, Lib. Long: +03.74

Type: Sea (Sea of Crisis)
Geological period: Nectarian (From -3.92 billion years to -3.85 billion years)
Dimension: 740km
Floor: lava-filled and is ~ 1.8 km below lunar datum
Outer rim: ~3.34 km above lunar datum

Eyepiece sketch on black Strathmore Artagain paper, white Conte’ crayon and pencil, Derwent watercolor pencil, black charcoal, black oil pencil.

The evening started off with DSO hunting while waiting for the Moon to come up, even though the stars were and faint galaxies were starting to wash out from the moonlight rounding the eastern horizon. I started a sketch of M12 that will have to wait for another night to complete when the Moon isn’t so much of a factor.

Once the Moon rose between two short junipers behind me, I switched to black paper and scanned the terminator. Mare Crisium looked like it was taking a bite out of the Moon. I’ve always been a bit intimidated at sketching rough terrain, but took a stab at it nevertheless. Sketching in the highlights makes it incredibly easier in fast moving areas such as along the terminator. The trick is to have very sharp pencils at hand, and I made sure of that during set up before it got dark outside – although I did have to resharpen once or twice during the session (as well as stand up and stretch.) It was a rush against time to render the basin’s western edge before the shadows swallowed the view.

I began with the inner ridge line along the terminator, marking each highlighted crest individually with a very sharp Conte’ pastel pencil. Then as quickly and accurately as I could, started working my way west, alternating between the Conte’, charcoal, Derwent and oil pencils, focusing first on the highlights, then the shadows, followed by albedo.

Of particular interest, Crisium sports the crash landing site(although not visible from last night’s lunar phase) of the Soviet’s Luna 15 in 1969 and the landing site of Luna 24, 1976, when soil samples where successfully brought back to earth.

This was my first time observing the Moon with the AT6RC and once seeing sharpened up, the views were crisp and clear with good contrast. It’s especially good that we’ve never had to collimate this scope and I’m looking forward to trying it out on Jupiter soon.

Lunar Terminator: Mare Spumans and Mare Undarum

On this evening, two days past full moon and with favorable libration on the eastern portion of the Moon, I chose two irregular maria targets for sketching. Mare Spumans was completely visible while Mare Undarum was only partly exposed beyond the terminator.

Although I have examined these little ancient “lakes” in the past this has been my first attempt to capture them on paper. Both are surrounded by bright, densely cratered upland and are close enough to Mare Crisium to be within its eject blanket and basin rings.

This is a very attractive region of the Moon for sketchers with craters Langrenus and Messier and Messier A nearby and Mare Crisium just to the north. I purposely kept these features out of my view to focus on lesser observed targets. In addition to the maria subjects, craters : Webb (22 km.), Apollonius (53 km.), and Firmicus (56 km.) provided eye catching targets across the view.

Sketching:

For this sketch I used: black Strathmore 400 Artagain paper 9″x 12″, white and black Conte’ pastel pencils and a blending stump. After scanning, Brightness was decreased just slightly using my scanner.

Telescope: 10 inch f/ 5.7 Dobsonian and 6 mm eyepiece 241x
Date: 08-04-2012, 04:00 – 05:50 UT
Temperature: 29°C (85° F)
hazy, calm
Seeing: Antoniadi III
Colongitude 110.6 °
Lunation 16 days
Illumination: 94.9 %
Libration: in Lat. -5° 45’, in Long. +05° 38’

Frank McCabe

Prominence Ejection Sequence – May 17, 2012

2012 05 17, 1245 UT – 1845 UT
NOAAs 11476, 11477, 11478, 11479, 11482, 11484, NE Prominence

PCW Memorial Observatory, Texas – Erika Rix
www.pcwobservatory.com
Temp: 20-30C, calm – S 5mph, clear.
Seeing: Wilson 4.8-1.2, Transparency: 5/6-4/6, 50x.
Maxscope DS 60mm H-alpha, LXD75, Baader Planetarium Hyperion 8-24mm Mark III.

Sketches created at the eyepiece with black Strathmore Artagain paper, white Conte’ crayon and pencil, white Prang color pencil, Derwent charcoal pencil, black oil pencil.

Link to gallery of individual sketches within the sequence.

During the time I observed, a very large prominence off the northeast limb was enlarging and in the process of ejecting as it broke free from the magnetic fields supporting it. I’ve never visually witnessed that large of a prominence breaking away from the Sun before. What really stunned me was how bright it remained over several hours that far off the limb. I grabbed an 8-sketch sequence spanning over 6 hours of the event, not including the full disk rendering I recorded earlier in the day. The last 35 minutes of my session, the prominence became very faint and diffuse. I stopped seeing any connection from the limb after 1717 UT. Of course, that doesn’t necessarily mean there wasn’t, but was perhaps too faint for my tired eyes to see.

Lunar Crater J Herschel

It is morning across the 165 km wide irregular floor of this walled plain
crater. J Herschel is a pre-Nectarian crater and in the observing light is well lit across its rubbly, slightly convex floor. This crater is a survivor of the Imbrium basin formation. The southern well defined outer rim to the south (to the left in the sketch) has its rampart buried under the lavas of Mare Frigoris. Along the south wall at the west end is crater Horrebow (26 km) which can be seen superimposed upon Horrebow A (25 km.). To the right and closer to the terminator and limb are craters Anaximander (70 km.) and Carpenter (61 km.) both of their rims are illuminated and only part of the floor of the former can be seen.

Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’ pastel pencils and a blending stump.
Telescope: 10 inch f/ 5.7 Dobsonian and 9 mm eyepiece 161X

Date: 05-3-2012 02:10 – 03:30 UT
Temperature: 21° C (70° F)
Partly cloudy, calm
Seeing: Antoniadi III
Colongitude: 53 °
Lunation: 11.8 days
Illumination: 86.6 %
Altitude of Moon about 41°

Very favorable libration for this crater

Frank McCabe

Solar h-alpha, Prominences – May 3, 2012

2012 05 03, 1845 UT – 2130 UT.
Solar h-alpha, Prominences and NOAAs 1469, 1471, 1472, 1473, 1474.

PCW Memorial Observatory, Texas – Erika Rix,
Temp: 33°C, winds SE 7 mph, occasional light cirrus,
Seeing: Wilson 2-3, Transparency: 4/6, 50x,
DS 60mm Maxscope, LXD75, Baader Planetarium Hyperion 8-24mm Mark III .

Sketch created scope-side with black Strathmore Artagain paper, white Conte’ crayon and pencil, Derwent charcoal pencil, black oil pencil.

With five active regions, the Sun made quite an appearance today in spite of the limb. There were a few decent prominences, especially to the eastern hemisphere. My favorite view, though, were magnetic fields surrounding 1471 made apparent by the very thin active region filaments (ARFs). They reached down like fingers from the sunspots in that region. Plage was very intricate and meshed into what I believe was AR 1472.

The quiet region filaments (QRFs) were in abundance in the southern northern hemisphere with a few speckled to the south. AR 1474 seemed a bit washed out with plage and faint darkened areas. There was only slight plage definition and no sunspots observed in h-alpha. I didn’t set up a white light filter today for comparison.

1473 and 1469 were blended together by the plage and many lines of ARFs, including filaments reaching out over the edge for short, bright prominences. Plage was very bright, forming the shape of a tuning fork in 1469. These were impressive sets of active regions when paired up.

This was my first solar observing session since moving to Texas about two and a half weeks ago. With all that took place in preparing the old house for sale and the move to Texas, I’ve been deprived of any observing other than naked eye. It was a relief to be behind an eyepiece once again.

Crater Furnerius

Beautiful evening with the 4 day old Moon above Venus and the planet Jupiter above the crescent Moon. After a careful look at the crescent Moon through the telescope at low power, I needed to decide if I should attempt a sketch of the beautiful view of western Mare Crisium or the crater Furnerius which was the easier target. Considering the air temperature which was cold, I took the easy way out and sketched Furnerius.

With the terminator well past this region, I knew I would have time to go indoors and warm up if I got too cold. I centered the eyepiece on my target and turned on the equatorial drive platform. Furnerius is a large 125 km. crater that has the appearance of the old pre-Nectarian period crater it is. Its walls and floor are battered with many small craters and Rima Furnerius was detectable on the northern side of the floor. Crater Fraunhofer (57 km.) another old crater was sketched to the south and much younger Stevinus (77 km.) was showing off its central peak to the west.

Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’ pastel pencils and a blending stump.

Telescope: 13.1 inch f/ 6 Dobsonian and 9 mm eyepiece 222x
Date: 02-26-2012 00:30 – 01:40 UT
Temperature: -6° C (21° F)
Clear, calm
Seeing: Antoniadi III
Colongitude: 315 °
Lunation: 4 days
Illumination: 15 %
Altitude of Moon about 33°

Frank McCabe

Heveluis

2012 01 07, 0200UT – 0340UT Hevelius, Lohrmann, Cavalerius
PCW Memorial Observatory, OH, USA, Erika Rix
www.pcwobservatory.com
16” Zhumell f/4.5 on a non-tracking Dobsonian mount, 24-8mm Baader Planetarium Mark III Hyperion, 225x, Moon filter
Temp6.5 C, 58% humidity, S: Antoniadi I-II, T: 4/6
Eyepiece sketch black Strathmore Artagain paper, Conte crayon and pastel pencil, charcoal pencil
Phase: 25.8 deg, Lunation: 13.35 d, Illumination: 95.0%
Lib. Lat: +01:33, Lib. Long: -04:22
Az: +206:07, Alt: +30:18

The trio of Hevelius, Lohrmann, and Cavalerius were the first to catch my eye along the terminator tonight. After a quick tour near the terminator, I settled on the trio and their surrounding area for a closer study. Grimaldi’s western rim was etched south of Lohrmann and had begun to fill with sunlight creeping over the waxing edge. The small central mountain of Hevelius and crater Hevelius A were spotted easily and the only hint of Hevelius rimae was a softened dark line reaching north to south just east of the central mountain. I didn’t realize it was even there until I came inside after my session and compared my sketch with an atlas of the area. The tormented outer slopes of the crater chain were very clear and sharp, making them very enjoyable to study and even more so to draw (in my feeble attempt to capture all the detail as accurately as I could). Cavalerius was completely filled in with shadow.

The fantastic find of the night was the Hevelius D 1 (dome) along the wrinkle ridge between Reiner and Hevelius. Reiner and Reiner Gamma were added as the sketch progressed, as they were too tempting to leave out.