Messier 41

M41

M41
Sketch by Michael Vlasov

M41 is an open cluster containing about 100 stars, including several red giants with a chemical composition similar to our sun. The stars are distributed over a volume about 25 to 26 light years across, and the cluster is receding from us at 34 km/sec. at a distance of 2300 light years.

M41 was possibly recorded by Aristotle in 325 BCE. Hodierna was the first to catalog it before 1654, then it was rediscovered by John Flamsteed in 1702. It was found again by LeGentil in 1749, and finally by Charles Messier in 1765. Phew.

H-Alpha Sun

Solar - April 6, 2008

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

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 Sombrero Galaxy

M104

Sombrero Galaxy (M-104), NGC 4594
Sketch and Commentary by Frank McCabe

Occasionally from my home observing site the humidity drops low enough to dramatically reduce the light scatter making it possible to observe bright galaxies. This night was one of those times.
Many of the bright galaxies of northern hemisphere springtime were visible this night and I selected the bright Sombrero galaxy in Virgo for sketching. This bright (9.0 visual magnitude), Sa spiral is just north of the Corvus border. Pierre Mechain discovered it in May of 1781 and 5 days later Charles Messier added it to his copy of the Messier catalog.
Vesto Slipher in the second decade of the 20th century measured the rotation rate and red shift of this magnificent spiral. This galaxy is receding at 1024 km/sec and is somewhere between 27.7 and 30.9 million light years distant. The nearly edge-on galaxy has a large glowing central bulge and a dark dust lane that can be detected with dark adapted vision in a 10 inch telescope. A spiral galaxy with large central bulge usually implies many globular clusters in association with that central bulge. This galaxy may have as many as 1200-2000 globulars in motions around the center. A research group led by John Kormendy in the mid 1990s discovered a super massive black hole at the core of this galaxy that measured one billion solar masses. This is a galaxy worth taking a look at on a clear night. You will find it at R.A. 12h 40 min. Dec. -11º 37min.

Sketching:
9”x12” white sketching paper; 4B graphite pencil and a blending stump made from a dowel rod; 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: 26 mm widefield eyepiece 56x and 8 mm eyepiece 181x
Date and Time: 4-3-2008, 4:00-4:50 UT
Seeing: Pickering 7/10
Transparency: Excellent 4/5
NELM: 4.8

Frank McCabe
Oak Forest, Il. USA

Ripples Around Castor

Castor

Castor (Alpha Geminorum / Struve 1110)
Sketch and Commentary by Jeremy Perez

The fussy seeing provided a beautiful view of this brilliant double. The diffraction patterns shimmered and danced, adding a bit of challenge to viewing the pair, but also providing a mesmerizing, speckled light show. The primary of Castor appeared bright white while its companion hinted at a subtle blue.

Measuring this duo using the Dobsonian scope was very challenging. I was attempting the PA measurement without my external dial, and although it was very tough to get the primary to drift through the exact center of the eyepiece, the measurement worked out fairly well–differing from Workman’s calculated 2008.2 value by only .8 degrees. The separation estimate was worse though, since I couldn’t track and allow the stars to hover over the scale. (My estimate of 6.9 arc seconds was a bit over compared to the calculated value of 4.5 arc seconds).

Subject Alpha Geminorum (Castor / STF 1110)
Classification Multiple Star
Position (J2000) Gemini [RA: 07:34:35.7 / Dec: +31:53:16]*
Position Angle* 59° [2008.2 my measurement]
58.2° [2008.2 Brian Workman’s DS Calculator]
Separation* 6.9″ [2008.2 my measurement]
4.5″ [2008.2 Brian Workman’s DS Calculator]
Magnitudes* 2.0 / 2.9
Spectral Types* A1V / A2Vm
Date/Time MAR 19, 2008 – 10:45 PM MST (MAR 20, 2008 – 05:45 UT)
Observing Loc. Phoenix, AZ
Instrument Orion XT8 (203 mm dia./1200 mm F/L)
Eyepieces/Mag. 10 mm Sirius Plössl + 2X Barlow (240X)
12 mm Meade Astrometric EP + 2X Barlow (200X)
Conditions Mostly Clear, Gibbous Moon
Seeing 3-4/10 Pickering
Transparency NELM Mag ~4.0
*References The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996); Starry Night Pro Plus 5.8

Lead Cars in a Comet Train

Comet 73P-C

73P-C/Schwassmann-Wachmann 3

Comet 73P-B

73P-B/Schwassmann-Wachmann 3
Sketches by Kiminori Ikebe

Two years ago, comet 73P/Schwassmann-Wachmann put on a memorable show for observers. The two brightest components of the fragmented comet had reached 6th magnitude and were separated by about 9 degrees when Kiminori Ikebe sketched them on the night of April 30, 2006.

Markarian’s Chain

Markarian’s Chain

Markarian’s Chain
Sketch by Eric Graff

This beautiful chain of island universes lies some 70 million light years away, at the heart of the Virgo Cluster of Galaxies. The cluster contains more than 2000 galaxies, about 1 percent of which are visible in Eric Graff’s sketch above. Eric created this mosaic while observing with his 6″ Newtonian reflector.

Binocular Beehive – M44

M44

M44
Sketch and Commentary by Rony De Laet

M44 in Cancer is a typical binocular object. With a total magnitude of 3.1 the Beehive Cluster or Praesepe was known since antiquity. And indeed, at a distance of 520 lightyears, the cluster is faintly visible as a large nebulous patch to the naked eye. With a simple pair of binoculars the patch resolves into a beautiful V-shaped open cluster measuring more than 1° across. Several multiple stars are visible at low power. The binocular view is perfect for such a large object. Most telescopes don’t offer a wide enough view to show the cluster in it’s ‘natural environment’. While studying the object, I got the impression of a deeper darkness behind the cluster, compared to the overal background brightness. Could this be an optical effect created by the contrast between the cluster stars and the background? I don’t know if it shows in the sketch. The bright star in the lower left part of the sketch is Delta Cancri. The one in the upper left corner is Gamma Cancri.

Observing data:
Date : March 31, 2008
Time : around 20.30UT
Binoculars : Bresser 8×56
FOV: 5,9°
Filter : none
Mount : Trico Machine Sky Window
Seeing : 2,5/5
Transp. : 2,5/5
Nelm : 5,0
Sketch Orientation : N up, W right.
Digital sketch made with PhotoPaint, based on a raw pencil sketch.

Comet 46P/Wirtanen

Comet 46P/Wirtanen

Comet 46P/Wirtanen
Sketch and Commentary by Martin Mc Kenna

The great thing about short period comets is there periodicity, if you miss a comet during one apparition then you can catch it again during the next one. However patience is required, because even with the short period comets one has to wait years between acts. When 46P/Wirtanen was last visible 6.71 years ago I was a young and eager comet observer. The only comets which I had seen during that time were Hale-Bopp, 2P/Encke, C/1999 S4 LINEAR and C/1999 T1 Mc Naught – Hartley. I would have done anything to see another and add it to my very short but growing list. I knew that 46P was visible back then, and where, but I did not see it. Something happened in my private life at that time which caused me a period of great depression. I could not even motivate myself to take the telescope outside and look so I locked myself away into my own world within my room until I managed to recover and return to a more resourceful state of mind. By this time the comet had now retreated further away from the Sun and had faded from the light grasp of my 8″ LX10 F/10 S.Cass telescope. I made a decision then and there that I would never let anything or anyone get in the way of my interests ever again. I also made a vow that when this comet returned again I would do my very best to track it down. This was a personal score to settle!

On February 24th 2008 the sky was delightful. After a long period of bad weather and hazy skies a passing cold front during the previous night had beat the atmosphere clean with Atlantic showers. This evening I had the 8.5″ F/7 dobsonian reflector with 32mm 1.25″ eyepiece set up in my front yard during evening twilight. The sky was 100% clear and dark. The waning gibbous Moon was far below the NE horizon and would not rise for several hours. My goal was 46P/ Wirtanen which was now well placed half way up the evening sky in the SW. Before dark I had plotted its RA and DEC onto my sky atlas 2000 showing the comet’s positions for the 24th and 25th. It was located within Aries in a very blank region of sky where Aries, Cetus, and the Pleiades meet. I put the comet’s position to memory then headed out during twilight to get dark adapted. I made sure my telrad finder was aligned accurately and checked focus on the naked eye star Almach in Andromeda.

I guided the scope upwards to Wirtanen’s location and began sweeping without success, twilight was still evident so I decided to wait until the sky darkened further. Meanwhile I began searching for new comets low in the western twilight through Pegasus but I was getting very angry and frustrated quickly. The head lights of passing cars and the security lights belonging to the neighbours had destroyed my prime search area. The telescopic FOV was a bright white glow and even in the areas away from the lights I was getting a bright ghost image in every field. I was furious with anger and after 15 min’s of hunting I had to stop. I was not in a good mood at all. I then calmed down and concentrated my efforts on 46P. I spent a long long time slowly sweeping for the comet using vertical and horizontal movements and still it was nowhere to be seen. By now a sharp frost was forming and despite wearing gloves my hands were freezing from touching the scope for such long periods of time. My fingers were red in colour and painful. I was going to give up then I gave myself a mental slap. I told myself that I was not going to leave the telescope until I found this comet. 20 min’s later at 20.00 UT the ghostly glow of the comet entered the field of my moving telescope. I actually said out loud, ”I got Ya!!!”.

Wirtanen was no easy catch. The coma had a nice green hue and was of a fairly large elliptical shape with very diffuse edges. Difficult to tell where the coma ended and the sky began. The coma got slightly brighter toward centre and had a faint white-coloured soft stellar condensation. The comet was best seen with averted vision and no tail was detected. I suspect the coma may be larger than this when seen from a darker site. I made the above sketch at the time. I watched the comet contently for 30 min’s then it lowered into the murk and was gone. I was delighted by the catch, in fact, it made my night!. There are now no tense feelings between Wirtanen and I. The comet can relax and sail through the solar system at peace and I can tick it off my list and concentrate on hunting down other cometary prey!.

Mag: +9.0 Dia: 6′ D.C: 3 Elongation from Sun: 69.9 degrees. This is my 43rd comet catch.