Galactic Queue

Markarian’s Chain

Markarian’s Chain
Sketch and Details by Ernest Shekolyan

Hi!

Let me contribute to ASOD one of my pictures

That is Markarian`s chain as it was seen 9/10 apr. 2007 in eyepiece of my scope at village Shumba, 50 km from St.Petersburg, Russia. That was visual limit 6.2m.

10″ Starfinder, 24 mm UWA, 46x, FOV: 105 ang. minutes, graphite pencil, white paper, then photocopy + level correction, crop and inverting in ACDSee

Sincerely yours, Ernest Shekolyan

Exquisite Eratosthenes

Eratosthenes and environs

Eratosthenes and environs
Sketch and Details by Richard Handy

Description: Eratosthenes is the exquisite jewel sitting next to the Hope Diamond of Lady Luna, Copernicus. Consequently, Eratosthenes is often overshadowed by the spectacle of this lunar Juggernaut, however this sparkling gem of a crater and its immediate environment convey some of the major events that dominated the northwestern quadrant of the Moon. From 4.5 billion to 4.2 Billion years ago, a few hundred million years before the period of Heavy Bombardment, the large impactor Gargantuan, first proposed by the British geologist Peter Cadogan, struck the Moon with a force and fury far beyond our comprehension. The possibility that this impact could have, in one single event, reshaped the mean crustal thickness on both sides of the Moon is a staggering thought. Fed by fissures and cracks in the broken crust created by the force of the impact, magmas found easy passage to the basin floor. Over the intervening eons, the great basin formed by that event would eventually fill in with mare lavas to form Oceanus Procellarum. About 3.85 billion years ago, during the period of Late Heavy bombardment (3.8-4.0 by ago) the Moon received another enormous blow to this same northwest quadrant. The impactor, though half the size, formed another great basin, again flooding with mare lavas like Procellarum, to become the beautiful Mare Imbrium. To the east of Eratosthenes, the arcuate sweep of the Montes Apenninus, part of the remnant rim of giant Imbrium, seem to diminish to a few low outcrops as they approach the crater, probably appearing much like a mesa would if you were strolling on the surface. There are a few of these buried massifs on Eratosthenes’ northwestern flanks, although the great circular mountain range disappears in this region only to reappear as the Montes Carpatus to the northwest of Copernicus. There is a wonderful flame-like mountainous formation to the southwest of Eratosthenes, it appears to have been shaped by the fluidized flow fronts from the Imbrium event. Both Copernicus and Eratosthenes are benchmark features, meaning their formations correspond to the beginning of a geological period. Fifty-eight kilometer Eratosthenes was excavated by a 3 km wide impactor some 3.2 billion years ago. It’s rugged walls and terraces show significant scalloping and craterlet battering. The mare around Eratosthenes seemed coated in rays from 93 km Copernicus, which formed 1.1 billion years ago by an impactor 4.5 km in diameter, inaugurating the Copernican period. During this last 1000 million years most complex plant and animal life on Earth evolved.

Sketch details:
Subject: Eratosthenes and environs
Date: 12-28-2006 Start 5:27 UT End 6:50 UT
Lunation: 8.64 days Phase: 68.6 deg Colongitude: 19.8 deg
Illumination: 68.2 % Lib in Lat: -03 deg 24 min Lib in Long.: +01 deg 36 min
Seeing: Terrible most of the session, Antoniadi IV-V, only very occasionally III
Weather: clear
Telescope: 12” Meade SCT f/10
Barlow: 2X Televue
Binoviewer: Williams Optics Bino-P with 1.6X nosepiece
Eyepieces: 20 mm W.O. Plossls
Magnification: 396X
Sketch Medium: White and black Conte’ Crayon on textured black Strathmore paper
Sketch size: 18”x 24”

Omega Blossom

M17

M17
Sketch by Serge Vieillard

Serge Vieillard worked on this detailed drawing of M17 over two nights while visiting Spain in 2007. He used a 46 cm Obsession telescope, a variety of magnifications and an OIII filter to prepare the drawing. He was not satisfied with the proportions of the first night’s sketch and so made use of an accurate, pre-plotted star field to concentrate on observing and redrawing the nebula on the second night.

Luminous Goldschmidt

Goldschmidt Crater

Craters Goldschmidt, Anaxagoras and Epigenes
Sketch and Details by Frank McCabe

Crater Goldschmidt is an ancient pre-Nectarian period walled-plain crater that is situated only 480 km. from the lunar North Pole. The floor of this crater appears light in color and little crater Goldschmidt A (7km.) was seen on the southern floor.
Along the western rim of Goldschmidt are craters Anaxagoras (53 km.) and Anaxagoras A (18 km.). Anaxagoras is a young Copernican period crater with an expected ray system that includes some I saw during the observation and included here to the east and southeast. The crater to the southwest of Goldschmidt is Epigenes (55 km.), an ancient Nectarian period crater with a more typical dark floor for this region. With the moon crossing the meridian so low it never resolved well in the eyepiece and scintillated and shimmered in the warm air rising from the ground. All in all it was a wonderful opportunity to view and sketch the moon.

Sketching

For this sketch I used: black Strathmore 400 Artagain paper 10”x10”, white and black Conte’ pastel pencils and a blending stump. After scanning, Brightness was decreased (-5) and contrast increased (+5) using Microsoft Office Picture Manager.

Telescope: 10 inch f/ 5.7 Dobsonian and 6 mm eyepiece 241 x
Date: 7-14-2008, 2:20-3:40 UT
Temperature: 20° C (68° F)
Partly Cloudy, calm
Seeing: Antoniadi III-IV
Colongitude 41.9°
Libration in Latitude: +7° 19’
Lunation 11 days
Illumination 84.3 %

Frank McCabe

Dark Nebula Nexus

M20

M20 – The Trifid Nebula
Sketch by Kiminori Ikebe

Mr. Ikebe observed and sketched this view of M20 using a 50 cm Dobsonian at 220X.

M20, The Trifid Nebula, is a famous and beautiful target for astrophotographers and visual observers alike. The red emission nebula contains a young star cluster at its center, and is surrounded by a blue reflection nebula that is most noticeable at the northern end. It’s distance is not well agreed upon, and is listed anywhere from 2,200 light years (Mallas/Kreimer) to 9000 light years (Jeff Hester). Its magnitude estimate is also wide, and is listed from 9.0 (Kenneth Glyn Jones) to 6.8 (Machholz). Part of the magnitude difficulty comes from the very bright triple-star system at the heart of the nebula.

The dark nebula that crosses the Trifid was cataloged by Barnard and listed as B 85. The object was originally cataloged by Charles Messier in 1764, when he described it as a cluster of stars.

Moon River

Naked Eye Moon
Waxing Gibbous Moon
Sketch and Details by Carlos E. Hernandez

We are experiencing hurricane season (June 1 to December 1) in South Florida and therefore lots of rain. On July 16, 2008 (01:45 U.T.) I was fortunate to experience a break in the clouds which exposed a Waxing Gibbous Moon (12.7 days old) which had a copper glow to it floating within a river of dark blue sky. The clumps of clouds on either side of the Moon had a lavender tint to them. The cloud border west of the Moon had a reddish-orange half arc visible over it. It was a very beautiful sight to behold while fighting off bad weather.

A digital rendering made using Corel Painter X.

I hope to post telescopic observations as soon as possible. My hectic work schedule and weather have prevented me from making them. I look to everyone’s observation in the future.

Carlos

Binoculars Along the Spine of the Scorpion

Antares, M4, & Rho Oph
Antares, M4, and Rho Ophiuchi
Sketch and details by Michael Rosolina

Scorpius is well placed right now for northern hemisphere observers and holds many beautiful and interesting objects. Scanning the constellation with widefield binoculars can be particularly rewarding. I found that I could see this trio all at the same time with my 15×70 binoculars. They make an interesting combination: Antares, a red giant, Rho Ophiuchus, a bright binocular triple, and Messier 4, a globular cluster containing countless stars.

The sketch was done in the field with 2B and HB pencils and a stump loaded with 4B graphite for M4. I then scanned and inverted the sketch digitally, colorised Antares, and added a little blur (5%).

There are many images of this region–time exposures showing the stars embedded in glowing clouds of gas and dust. None of that can be seen visually, but the binocular view has its own beauty.

Michael Rosolina
Friars Hill, WV USA

Marbled Milky Way Magesty

NGC 6604
NGC 6604
Sketch and details by Eric Graff

Object Name: NGC 6604
Also Known As: H.VIII.15, Cr 373, C1815-122
Object Type: Open Cluster + Emission Nebula (Sh2-54)
Constellation: Serpens (Cauda)
Right Ascension (2000.0): 18h 18.0m
Declination (2000.0): –12° 14′
Magnitude: 6.5
Size: 6′ (some sources say 60′)
NGC Description: Cl, lRi, lC
Discovery: William Herschel, 15 July 1784

Date/Time: 4 July 2008 • 09:05 to 10:30 UT
Location: Oakzanita Springs (4,010 ft. elevation), San Diego Co., California, USA
Telescope: Parks Astrolight EQ6 • 6″ f/6 Newtonian Reflector
Eyepiece/Magnification: Parks 15mm Gold Series Plössl • 60x • 52′ FoV
Filters: Lumicon UHC, Lumicon OIII
Conditions: Clear, calm, 62°F
Seeing: Pickering 4-5
Transparency: NELM 6.3; TLM 14.0

If you sweep 1.6° north and slightly west of M16 you’ll chance upon a tight knot of five stars in a glittering field awash with hundreds of stars and marbled with complex swirls of bright and dark nebulosity. This small group (and undoubtedly many of the fainter stars that surround it) comprises the open cluster NGC 6604. The nebulosity (which I found remarkably easy to detect, even without filters) is the southernmost section of a large, but faint, HII region catalogued as Sh2-54. The 7th magnitude lucida of NGC 6604 is an O8 type star that is also an eclipsing binary (of the Beta Lyrae type) designated MY Serpentis. In spite of its spectral type, MY appears yellowish in the eyepiece; this is because the cluster (and nebulosity) is buried deeply in the Great Rift of the Milky Way, severely dimming and reddening its light.


In order to concentrate on the nebula itself, Eric notes: “I sketched the object(s) and a couple dozen of the brightest field stars and background nebulosity. Then, due to the extreme richness of the field I got out printed DSS negatives and started circling the stars I could see (which still took a fair amount of time). These were transferred to the sketches over the weekend. “