Media Combinations – Page 30 – Astronomy Sketch of the Day

Flocking to Scutum

M11
Sketch and Details by Kiminori Ikebe

M11(NGC 6705) Sct open cluster
Difficulty level 1

Date of observation: 1999/10/06 20:23
Observing site: Makinoto
Transparency/seeing/sky darkness: 3/5/3
Instruments: 32cm Dobsonian with XL14 at 110x
Width of field: 0.6 degree
This is a fine and bright cluster containing many stars. At 110x it is highly concentrated but almost completely resolved. There is a 7.8-magnitude star near the center. It is very conspicuous. There are two faint stars nearby. It is a fine sight with an equal double on the south side, which is as bright as the star near the center. The distribution of the resolved stars is quite uneven. The general shape of the cluster is that of a diamond and a beautiful chain of stars is seen in the southeast outlying area. Dark areas and dense patches of stars are intermingled. There are scattered outliers northeast of the cluster. They seem to be members of the cluster.

Raising Eyebrows on the Floor of Imbrium

Aristillus and Autolycus
Sketch and Details by Richard Handy

Sitting replendently on the the eastern margin of Mare Imbrium, 56 km Aristillus and 41 km Autolycus, brothers of Copernician age, are a startling sight in the late lunar afternoon sunshine. Hexagonal in appearance, Aristillus’s broad and radially splayed glacis dominates the mare surface in this region. It’s wide, brilliantly lit terraces apparently have evidenced some mass wasting since its creation a little over a billion years ago. Resting on the floor, some 3650 m deep, the glowing central peaks are roughly 900 meters high. Rays, some quite prominent, emanate from the crater’s center. To the northwest of Aristillus, swathes of darker mare may indicate areas not fully dusted by the ejecta from this massive impact, or perhaps ejecta excavated from deep within the extant mare is responsible for these low albedo areas. Approximately 60 km to the south, Autolycus’s glacial nimbus appears almost serene in comparison to the complex nature of Aristillus’s glacis. Half of the floor of Autolycus is composed of quite torturous terrane including a strange floor subsidence to the eastern section of the floor.

Here are the sketch details:

Subject: Aristillus and Autolycus Rukl: 12
Date: 10-13-06 Start: 9:15 UT End: 10:50 UT
Lunation: 20.90 days Phase: 277.5 deg Illumination: 56.5%
Colongitude: 164.8 deg Lib. in Lat.: -5 deg 40 min Lib. in Long.: +7 deg 39 min
Seeing: Antoniadi III-IV with 30 seconds of Ant. II every 20 minutes
Weather: Clear early, turning to occasional clouds mid to late during session, 10-15 knot winds late.
Telescope: 12″ Meade SCT F10
Binoviewer: W.O. Bino-P with 1.6X Nosepiece.
Eyepieces: W.O. WA 20mm Plossls
Magnification: 244X
Lunation: 18.48 days Phase: 311.1 deg Illumination: 82.9%
Colongitude: 133.7 deg Lib in Lat.: -3 deg 53 min Lib in Long.: +5 deg 12 min
Sketch medium: White and black Conte’ Crayons on black textured Strathmore paper.
Sketch size: 18″ x 24″

Morning at Crater Walther

Walther Crater
Sketch and Details by Frank McCabe

On this spring evening I drove over to our local community college to pick up and bring home the observatory telescope which was in need of cleaning and minor repairs. When I finished that work the sky was clear so I decided to use the scope to make a lunar sketch. The target I selected for drawing was the large (140 km.) Nectarian period walled plain crater Walther. On older lunar atlases this crater is either labeled Walter or Valtherus but in 1982 the name was changed to the current Walther by the IAU. I have always found the moon shows off some of its best large craters at this time in the lunation. Walther is one of those great old highland craters with much to offer a careful observer. Most seasoned lunar observers are well aware of the Walther sunset ray, but even at sunrise this crater has its rewards. A combination of craters with a common dark floor rests on the eastern rim three kilometers above the shadowed floor of Walther. To the west beyond the dark floor is the cratered, off-centered “central” mountain group casting a long triangular shadow across the resurfaced floor to crater Walter E (13 km.). Four small 4-6 km. craterlets can be seen in the drawing although at the eyepiece additional smaller ones were clearly visible in moments of steady seeing. To the northeast of Walther another large 3.9 billion year old crater Aliacensis (80 km.) was showing terraced walls and a central peak. The large younger Eratosthenian crater to the north of Walther is Werner (71 km.). Like the other two it has an off-centered central peak as well.

This was one of those observing nights when you wish time would stand still. I watched the long triangular shadow from Walther’s central peak shorten by 40% in just 2 hours.
I must say this was a beautiful night for moon viewing.

Sketching:

For this sketch I used: black Strathmore 400 Artagain paper, 9”x 12”, white and black Conte’pastel pencils and a blending stump. Brightness was slightly decreased (-2) and contrast increased (+2) after scanning using Microsoft Office Picture Manager.

Telescope: 13.1 inch f/ 6 Dobsonian and 6mm eyepiece 333x
Date: 5-13-2008 1:35 – 3:20 UT
Temperature: 7° C (45° F)
high clouds, calm
Seeing: Antoniadi III
Co-longitude: 4°
Lunation: 7.6 days
Illumination: 59.7 %
Phase: 78.8°
Observing Location: +41°37′ +87°47′

Frank McCabe

Planet Number Six

Saturn
Sketch and Details by Frank McCabe

This was my first attempt at sketching the planet Saturn while using white Conte’ crayons on black paper. Over a period of 3 hours I made 4 drawings of Saturn. The first 3 made during the first two hours looked terrible but the third one, although rough and grainy looking, came out recognizable as a ringed planet. I have nothing but the highest respect for those sketchers that regularly and beautifully draw this planet.
I could clearly see the dark planet shadow on the A and B rings. I could not hold the C ring constantly visible and so I did not include it in the drawing. The Cassini division was clearly visible but not the Encke division. Contrast between the brighter equatorial zone and the southern equatorial belt above it were easily seen. Four of Saturn’s moons were easily seen when the high thin clouds moved on. Clockwise starting above the planet in the drawing is Titan (mag.8.8), then Tethys (mag.10.7), next Rhea (mag.10.2) and finally Dione (mag.10.8). Mimas and Enceladus were in the field of view but hidden by the planets glare.
Saturn and its moon make wonderful targets for a clear night at the eyepiece of a telescope. Sketching the view just simply adds to the enjoyment.

Sketching:

For this sketch I used: black Strathmore 400 Artagain paper, 8”x 11”, white and black Conte’pastel crayons, an eraser shield, and a blending stump. Brightness was slightly decreased (-5) and contrast increased (+3) after scanning using Microsoft Office Picture Manager.

Telescope: 10 inch f/5.7 Dobsonian and 6mm eyepiece 241x
Date: 5-5-2008 4:00 – 5:00 UT
Temperature: 13°C (56°F)
high clouds, calm
Seeing: Pickering 6.5

A Splinter in Virgo

NGC 5170
Sketch and Details by Kiminori Ikebe

NGC 5170 Vir galaxy
2000.04.09 01:35
32cm at 150x

A good contrast with the face-one galaxy NGC 5247 located 1.7 degrees to the east. Not very bright but a fine sight with a very long and narrow shape. No bulging at the center. A long and narrow central condensation with a gradual fading towards the ends.

The Sun, Pencils or Camera?

H-Alpha Sun
Sketch and Details by Les Cowley
Comparison Photos by Pete Lawrence

The Sun is an ever-changing target. In H-alpha light, prominences light and
dim, shift and change literally by the minute. Fascinating to watch and
sketch but just how accurate are drawings grabbed in a few minutes during
variable seeing and under a black hood?

May 7th was an opportunity to find out when Cloudy Nights held an
“International Day of the Sun”. Expert UK photographers Peter Lawrence and
Nick Howes suggested imaging or sketching a prominence every 30 minutes on
the hour and half hour!

The day dawned clear and after breakfast the selected prominence was viewed.
It was the ugliest assortment of filaments, clouds and loops that you could
imagine with parts changing and dancing about even as you watched. The
‘scope was a Coronado Solarmax60 mounted on a manual altazimuth. Seeing
started fairly good so I used an 8mm Radian, I need eyeglasses to sketch and
the Radian gives enough eye relief. The drawings were on A4 black Canford
paper filling half the sheet per sketch with Derwent Watercolour pencils
used sharp and dry.

Serious observing started about 8 minutes before each time mark with the
main proportions starting to be put in 5 minutes before the mark. Then finer
and finer details were quickly added, not in any order just wherever good
seeing happened to show them. This quickly brought the time to the mark and
then the whole view was assessed for accuracy. It was changing so fast!
Finally 3-5 minutes after the mark were spent getting the relative
intensities right and generally tidying up.

By 09:45 there were frequent periods of superlative seeing and I changed to
a 5mm Radian and clutched the dark hood around close to shield the daylight.
For long periods (but never, ever during the allocated 10 minute slots!) the
visible structures were exquisitely resolved into delicate stacked filaments
with even those sometimes doubling and breaking into knots – you would need
an hour or hours to capture all that! After 10:30 the seeing deteriorated
and that combined with not a little fatigue ended the sketching run.

Pete Lawrence was imaging some 150 miles to the south with about the same
seeing conditions. He used a Solarscope SF-70, a Rolls-Royce of H-alpha
filters. His images for the same times are on a reduced scale at the base
but you need to see the originals (http://www.digitalsky.org.uk/ and Cloudy
Nights) to really appreciate their superlative quality.

So can sketching such ephemeral objects ever be accurate? I’m still
deciding. There is maybe a tremendous amount to be leaned from a careful
comparison of sketch fragments with simultaneous photographs about how the
eye-brain interprets fine details and tends to join others into spurious
larger structures. If some of that can be understood then hopefully it might
improve the sketching accuracy.

Les Cowley, England

Hickson 44

Hickson 44
Sketch and Commentary by Kiminori Ikebe

NGC 3185 Leo galaxy
NGC 3187 Leo galaxy
NGC 3190 Leo galaxy
NGC 3193 Leo galaxy
HCG44

1997.01.12 01:27
32cm at 110x

A fine group of four different-type galaxies.
NGC 3185: The largest of the group, but faint and diffuse. Elongated. A fainter halo appears to envelop the galaxy, but not confirmed.
NGC 3187: Barely detectable. A long, narrow shape is barely discerned.
NGC 3190: A sharp, long, spindle-shape. The brightest of the group. A stellar nucleus and a small central condensation.
NGC 3193: Small and round. A dull glow of a stellar nucleus and very weak central condensation.

H-Alpha Sun

Solar H-Alpha
Sketch and Commentary by Erika Rix

2008 04 06, 1240ST – 1330ST (1640UT – 1730UT)
Solar H-alpha
PCW Memorial Observatory, Zanesville, Ohio, USA, Lat: 40.01 / Long: -81.56
Erika Rix

Temp: 62.1 °F / 16.7 °C
Winds: 3.5 mph from the East
Humidity: 52%
Seeing: 5/6 with moments of 2/6
Transparency: 4/6
Alt: 51.3 Az: 143.3

Equipment:
Internally double stacked Maxscope 60mm, LXD75, 40mm ProOptic Plossl, 21-7mm Zhumell

Sketch Media:
H-alpha – Black Strathmore Artagain paper, white Conte’ and Prang pencils, white vinyl eraser.
Added –25 brightness, +15 contrast after scanning in color at 300 dpi. Tilting Sun program used for digital Sun insert.

Triesnecker and Rimae on the Shores of the Central Bay

Triesnecker and Rimae on the shores of the Central Bay
By Richard Handy

Sinus Medii or Central Bay, is aptly named for its relation to the geographic midpoint of the Moon (the point on the surface where the Earth would appear at the zenith at all times). On the northeastern shore of Sinus Medii lies the Copernican Period crater Triesnecker, the 26 km archetypical complex crater. Only hints of its distinguishing characteristics are apparent is my sketch because most of the crater’s inner walls are cloaked in shadow in this view, awaiting lunar sunrise to reveal their contours. The intense highlights off the scalloped western wall is the only evidence of considerable mass wasting that the crater has experienced. Hidden in this view is a floor whose entire western half is buried in wall debris. The deviation from circular (polygonal) form that Triesnecker displays is apparent all around the periphery of the crater. Terrace collapse has resulted in a reduction in floor depth and a annular ring of hills that are hidden from our view here. A mid morning Triesnecker sports a central peak and a small mare like area of what appears to be impact melt. The larger the crater the higher the peak, a product of the rebound energy of a surface that is impacted. Triesnecker sized craters lie at the lowest energy level necessary to produce central peaks, consequently the peak heights hover around 300 to 500 meters, large craters between 80 and 100 km have central peaks that average 2 km high. Immediately to the east, the complex rille network of Rimae Triesnecker dominates the right side of my sketch. Several things intrigue me in this area. Despite Triesnecker’s obvious superposition on top of these features, it seems amazing to me that these rilles survived being buried by its ejecta blanket. However this sketch is probably telling for what it does not reveal, filled in rilles which might be responsible the isolated rimae segments I’ve rendered here. The biggest mystery to me is why these rilles are located in this area of the Moon in the first place. Wilhelm suggested extensional forces. Perhaps Procellarum/Imbrium and Serenitatis/Tranquillitatis mascons are responsible for their appearance here, meaning these rilles are interpreted as grabens. A quick look to the northeast and we are amidst the obviously volcanic domain of the Hyginus crater and Rima. The surface elevation in this region has subsided and that may be due to extensional forces and subsequent outflows of mare lavas and terminal eruptive episodes

Here are the sketch details:

Subject: Triesnecker and Rimae Rukl: 33, 34
Date: 1-26-07 Started- 4:38 UT End- 5:55 UT
Seeing: Antoniadi III to IV Weather: Clear
Telescope: 12″ Meade SCT f/10
Binoviewer: W.O. Bino-P with 1.6X Nosepiece.
Eyepieces: W.O. WA 20mm Plossls
Barlow: 2X Televue Powermate
Magnification: 396X
Lunation: 7.03 days Phase: 86.8 deg Illumination: 52.8%
Colongitude: 359.7 deg Lib in Lat.: -4 deg 33 min Lib in Long.: +03 deg 35 min
Sketch medium: White and black Conte’ Crayons on black textured Strathmore paper.
Sketch size: 18″ x 24″.

The Highlands Between Grimaldi and Mersenius

Highlands Between Grimaldi and Mersenius
Sketch and Commentary by Frank McCabe

With the moon at nearly full phase, the sunrise illumination was approaching the western limb on this evening of observing and sketching. The region I focused in on includes the highlands just beyond the southwestern portion of Oceanus Procellarum between the Grimaldi basin and crater Mersenius. Both of these features are outside the boundaries of this sketch. Normally in this light I can hold the linear Rille Sirsalis in view continuously, but on this night it was visible only intermittently. Twin craters Sirsalis (43 km.) and Sirsalis A (49 km.) were clearly visible with their bright rims and dark shadowed floors. It is clear from some light reaching the floor of Sirsalis A that Siralis is the deeper of the two.
Lava flooded Billy, an Imbrium crater at 46 kilometers is separated from slightly younger crater Hansteen (45 km.) by Mons Hansteen. Beyond these features the remains of Siralis E a ghostly 72 kilometer crater remnant was visible in the morning sunlight.

Sketching:

For this sketch I used: black Strathmore 400 Artagain paper, 8”x 11”, white and black Conte’pastel pencils and a blending stump. Brightness was slightly decreased (-5) and contrast increased (+6) after scanning using Microsoft Office Picture Manager.

Telescope: 10 inch f/5.7 Dobsonian and 9mm eyepiece 161x
Date: 3-20-2008 4:50 – 6:00 UT
Temperature: -2°C (28°F)
clear, calm
Seeing: Antoniadi III
Co longitude: 66.9°
Lunation: 12.5 days
Illumination: 97.5 %
Phase: 18.4°
Observing Location: +41°37′ +87° 47′

Frank McCabe