Arrowhead, Butterfly or Starfish?

M93

M93, an open cluster in the constellation Puppis
Sketch and Details by Jeremy Perez

This is a triangular arrow shaped cluster with its tip pointing southwest. This southwest tip hosts one orange and one yellow star. In the center lies a trapezium-like arrangement of stars. The main body appears to be 16′ in diameter. The brightest neighboring star lies 30′ to the southeast.

Factoids:
M93 lies 3600 light years away and its 80 or so member stars span 20-25 light years across. Its brightest stars are B9 Blue Giants, and its age is estimated at 100 million years. While its stars form a triangular shape, Kenneth Glyn Jones found it to look like a butterfly, while Admiral Smyth found it more like a starfish. It was one of the last deep sky objects discovered by Charles Messier personally and was cataloged in 1781.

Subject M93 (NGC 2447)
Classification Open Cluster
Position* Puppis [RA: 07:44.6 / Dec: -23:52
Size* 22′
Brightness* 6.0
Date/Time February 4, 2005 – 9:15 PM
(February 5, 2005 – 04:15 UT)
Observing Loc. Flagstaff, AZ – Home
Instrument Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)
Eyepieces/Mag. 32 mm (37X)
Conditions Clear, 29�F
Seeing 2/10
Transparency Mag 5.0
Sources SEDS
*Based on published data.

A Flower in a Field of Space

M63

M63, the Sunflower Galaxy
Sketch and Details by Frank McCabe

There are a handful of bright springtime galaxies that can be reached by modest telescopes in the light polluted south suburbs of Chicago. At approximately 9th magnitude M-63 is one of those galaxies. A spiral galaxy with a bright central bulge of about 4”of arc, this galaxy quickly drops off in brightness where you might hope to see many short spiral arms and knotty dust bands. However they were not visible at the eyepiece of a 10 inch telescope under my sky conditions. Three days after I drew this sketch my daughter and I had an opportunity to observe M-63 under exceptionally transparent conditions at Kitt Peak National Observatory using a 20” RC telescope. The galaxy appeared much brighter and more than twice the diameter but the spiral arms were not detected at all. Never the less this is a beautiful galaxy to see at the eyepiece by direct vision. It is the astrophotography that gives this galaxy the name sunflower.

This galaxy is easily located between Cor Caroli in Canes Venatici and Alkaid in Ursa Major. It was discovered 229 years ago this month by Pierre Méchain.

Sketching:

9”x12” white sketching paper; 4B graphite pencil and a blending stump; after sketching a 6” circle was cut from the sketching paper;

Scanned and inverted; brightness of stars adjusted with MS Paint.

Scope: 10” f/5.7 Dobsonian: 24 mm widefield eyepiece 60x and 12 mm eyepiece 121x

Date and Time: 6-2-2008, 3:00-4:30 UT

Seeing: Pickering 7/10

Transparency: Good 3/5

NELM: 4.6

Frank McCabe

A Rima Runs Through It

Rima Ariadaeus

Rimae Agrippa
Sketch by Bognár Tamás

This beautiful sketch of Rima Ariadaeus was sent in by Bognár Tamás of Zakany Hungary. This rille, one of the most dramatic on the Moon, runs for a length of over 200 kilometers, cutting through hills and crater walls before vanishing into Mare Tranquillitatis.

Rimae Agrippa
Telescope: 3″ F/11 Newton and 7,5 mm Super Plossl eyepiece
Date: 02-13-2008 16:10 – 17:30 UT
Co-longitude: 354,5°
Observing Location: Zakany – Hungary, 46° 15′ N 16° 57’E elev.: 129m

A Triplet of Craters in the Southern Highlands

Crater Cuvier

Craters Cuvier, Heraclitus, and Licetus
Sketch and Details by Frank McCabe

It has been a long time since I have attempted to use charcoal pencils on white sketching paper but I found an unused pair among my drawing supplies. They turned out to be less messy than ones I have used in the past. I liked the way they worked on the medium weight drawing paper I had on hand.

Two years ago in March of 2006 the European Space Agency (ESA) spacecraft Smart-1 imaged the crater Cuvier to test the high resolution camera (AMIE) with great success. I noted this crater was well placed along the terminator last evening for sketching. No sooner than having seen it, I decided it would be my target for sketching. Cuvier a 77km walled-plain crater is eastern most in the sketch. The crater has a nearly flat, lava flooded floor and at 3.5 billion years old is still younger than its neighbor to the southwest Heraclitus. Elongated crater Heraclitus is from the Pre-Imbrian period and dates back more than 4 billion years. A central mountain ridge runs down the center of this crater from northeast to southwest. This ridge line was illuminated in the morning sunlight. Within the shadow of this crater 25% of the dark southwest floor is occupied by Heraclitus D. Finally the large 74 km. crater to the northwest is Pre-nectarian crater Licetus. It like Cuvier infringes upon Heraclitus.

It was a beautiful night to observe and sketch the moon.

Sketching:

For this sketch I used: White CPP sketching paper, 9”x 12”, Number 4B charcoal pencils, a blending stump, gum eraser and an eraser shield. After scanning, Brightness was slightly decreased (-2) and contrast increased (+2) using Microsoft Office Picture Manager.

Telescope: 10 inch f/ 5.7 Dobsonian and 6mm eyepiece 241x
Date: 6-11-2008 1:05 – 2:05 UT
Temperature: 24° C (76° F)
clear, calm
Seeing: Antoniadi III
Co-longitude: 358.9°
Lunation: 7.29 days
Illumination: 55.1 %
Phase: 84.1°
Observing Location: +41°37′ +87° 47′

Frank McCabe

A Double and a Trifid

M20

M20 (The Trifid Nebula)
Sketch by Eiji Kato

M20, The Trifid Nebula, is a famous and beautiful target for astro-photographers. 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).

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. William Herschel assigned catalog numbers to 4 different parts of the nebula (H IV.41, H V.10, H V.11, and H V.12).

Unusual Earthshine

Earthshine

Moon with Earthshine
Sketch and Details by Carlos E. Hernandez

I was struck by the Waxing Crescent Moon (2.4 days old) over the western horizon (~11 degrees) tonight (January 11, 2008 at 00:00 U.T.) as it appeared that the Earthshine over the unilluminated portion was asymmetric. I turned my 11 x 56 Oberwerk binoculars upon it and noted a brightening over the Moon’s northern (upper) limb. My wife also noted the brightening without my suggestion. There also appeared to be a “glow” surrounding the crescent Moon. I have never observed this over the Moon at this or any other phase. This most likey represnts an atmospheric phenomena (e.g. haze or diffuse cloud).

A digital rendering in Corel Painter X.

Carlos

To Sketch a Sketch for the Sake of Science

Mars

Modified Test Drawing of Mars: 1890
Drawing by Professor Schiaparelli, modified by test administrators

The above sketch was used as part of an experiment in determining the origin of the observation of Martian canals. Excerpts from the article are shown below. The entirety of this interesting and enlightening article can be read at Google Books (see link at the end of this post).


Experiments as to the Actuality of the, “Canals” observed on Mars.
By J. E. Evans and E. Walter Maunder.The experiments described in the following paper were undertaken in order to ascertain whether the impression of a network of fine lines, such as forms what is now known as the “canal system” of Mars, could be produced upon entirely unbiassed observers without those lines having a real objective existence; and, should this prove to be the case, to find out the conditions most favourable for the creation of such an impression. The experiments were made in the following manner. A circular disc, varying according to circumstances from 3.1 to 6.3 inches in diameter, was given to a class of boys to sketch. The boys in the class were usually twenty in number, and were seated at various measured distances from the disc. These distances varied in the extreme from 15 feet up to 62 feet, but more generally from about 17 feet to 38 feet. The boys were all supplied with a piece of drawing-paper upon which a circle 3 inches in diameter had been described, and were instructed to fill in that circle with all the details which they could perceive upon the disc. No hint was given them that they ought to see lines or dots or any other form of marking ; they were simply urged to draw all that they could see and be sure of, each for himself, without noting what his neighbours were drawing….

….The boys employed in the experiments were from the Royal Hospital School, Greenwich. Their ages ranged from twelve to fourteen for the most part; a few were either a little older or a little younger than these ages. All of them were wholly and entirely ignorant of the appearance of Mars in the telescope, and of the discussions which have taken place as to the markings on his surface. They were simply shown, what was to them, an odd-looking figure, and were told to reproduce it as well as they could. The first series of experiments was made on 1902 July 1, the last on 1903 May 22, the great majority having been made in the spring of the present year….

….Experiments 8 and 9.—Drawing 6.25 inches based upon one by Professor Schiaparelli made 1890 May 16 (La Plancte Mars, p. 474). In this experiment none of the canals shown by Professor Schiaparelli were inserted, but a number of small irregular markings were inserted at haphazard. River-like marks were drawn flowing into Dawes’ Forked Bay and the smaller marking of the same character which Schiaparelli has represented some 30° from it at the mouth of the Phison. The region of Meroe Island was put in in half-tone….

….It appears to us in reviewing the entire series of the experiments that it is impossible to escape the conclusion that markings having all the characteristics of the canals of Mars can be seen by perfectly unbiassed and keen-sighted observers upon objects where no marking of such a character actually exists. They are in a sense truly “seen,” not imagined, because they are the natural rendering by the eye of real markings of a different character….

….Generally speaking, the best draughtsmen, that is to say, those who most truthfully represented the salient features of the drawing, also showed the greatest numbers of canals. It is also worth note that on the whole the agreement as to the canals was greater than the agreement as to the broad features of the original drawing….

….Our conclusion from the entire experiment is that the canals of Mars may in some cases be, as Mr. Green suggested, the boundaries of tones or shadings, but that in the majority of cases they are simply the integration by the eye of minute details too small to be separately and distinctly defined. It would not therefore be in the least correct to say that the numerous observers who have drawn canals on Mars during the last twenty-five years have drawn what they did not see. On the contrary they have drawn, and drawn truthfully, that which they saw; yet, for all that, the canals which they have drawn have no more objective existence than those which our Greenwich boys imagined they saw on the drawings submitted to them.

It seems a thousand pities that all those magnificent theories of human habitation, canal construction, planetary crystallisation, and the like are based upon lines which our experiments compel us to declare non-existent; but with the planet Mars still left, and the imagination unimpaired, there remains hope that a new theory no less attractive may yet be developed, and on a basis more solid than “mere seeming.”


Published in the Monthly Notices of the Royal Astronomical Society, Vol. LXIII, 1903, Pages 488-499 available at Google Books.

Galactic Smirk

NGC 5529

NGC 5529
Sketch and Details by Bill Ferris

NGC 5529: Edge-on Galaxy (Bootes) RA: 14h 15.6m / DEC: +36º 13′.6
Instrument: 18-inch Obsession

Here’s an interesting edge-on galaxy. NGC 5529 resides in west-central Boötes about 4 degrees southwest of 3rd magnitude Gamma (27) Bootis. My sketch presents a 199X view in the 18-inch Obsession. NGC 5529 is the thin sliver of light at the center. This 11.9 magnitude spiral covers a 6′ by 0′.7 patch of sky with that part west of the core appearing brighter than its counterpart to the east. The core region is slightly irregular in shape, looking like two small humps on either side of the core. An interesting three-star asterism stands a few arcminutes to the east. A faint 14th magnitude sparkler simmers close by, just off the galaxy’s eastern tip. And 1′.7 south of this star is where PGC 50952 emerges from the night. This 15.3 magnitude spiral presents as a 30″ diameter glow. It’s very subtle and best seen with averted vision. Even more challenging, is the delicate smudge some 5′ to the northwest. That tiny patch of fog is MCG +06-31-85a, a 16th magnitude galaxy with just the brighter 0′.3 diameter core being visible in the 18-inch. This galaxy is seen intermittently with averted vision, but always in the same location. This view is framed by twenty-five stars scattered throughout the field in my sketch.

Upon the Sea of Clouds

Bullialdus

Bullialdus Crater
Sketch and Details by Frank McCabe

Western Mare Nubium has been the home of complex, Eratosthenian period crater Bullialdus (61 km.) for the past three and a half billion years. The beautifully terraced inner walls to the east and kilometer high central peaks were clearly seen in the morning light. The outer downward sloping walls were showing alternating radial ridges and valleys down to the lava flooded floor of Nubium. The crater rim stands 2.4 kilometers above the crater floor and the floor is 1.2 kilometers below the surrounding Mare Nubium lava.
The ancient flow of lava across the Sea of Clouds breached the walls and flooded the floors of craters Kies (44 km.) to the southeast and Lubiniezky (44 km.) to the northwest of Bullialdus. Immediately to the south of Bullialdus are Bullialdus A and B, both twenty something kilometers in diameter with the closer A being the larger of the two. The famous 11 kilometer dome Kies л was clearly seen just to the west of crater Kies and to the northwest, crater König (23 km.) looked impressive with its dark shaded floor.

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 (-3) and contrast increased (+2) after scanning using Microsoft Office Picture Manager.

Telescope: 10 inch f/ 5.7 Dobsonian and 6mm eyepiece 241x
Date: 5-15-2008 2:10 – 3:45 UT
Temperature: 8° C (46° F)
passing clouds, calm
Seeing: Antoniadi III
Co-longitude: 28.8°
Lunation: 9.6 days
Illumination: 78.5 %
Phase: 55.3°
Observing Location: +41°37′ +87° 47′

Frank McCabe