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.

The Highlands Between Grimaldi and Mersenius

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

Orange Embers and Blue Ice in Messier 18

M18

M18
Sketch and Commentary by Wade Corbei

Here is an older sketch that has been hiding in the middle of my current sketch book. As the date indicates, this sketch was made back in October of ’07 when Sagittarius was still fairly prominant towards the south.

My notes also make note that I was a little more than 1 hour at the EP while plotting all the faint stars that surround this great open cluster, and that there was no Moon in the sky, which allowed for some great dark-sky observing.

I also noted that this cluster had a few stars of varying colors as well, a few that were slightly orange as well as a few almost ice-blue. The rich starfield of this region just adds to the overall experience of observing this large OC. This is indeed a fairly large OC as well. Although I tried several EP’s (15mm Expanse, 10mm, 6.3mm) I got my best over-all view of this OC with my 20mm.

The Hub of the Antennae

NGC 4038 and 4039

NGC 4038 and 4039 – The Antennae Galaxies
Sketch by Eiji Kato

This colliding pair of galaxies lies about 65 million light years away in the constellation Corvus. They are named after the long tidal tails that were strewn out some 200 to 300 million years ago when the galaxies first began interacting. As the collision proceeds, billions of new stars will eventually be formed. This fascinating merger gives us a preview of what may happen when the Milky Way and Andromeda Galaxies collide in the distant future.

Sources: HubbleSite News Center, NOAO

The Makings of a Coronal Mass Ejection

Sun

Sun-White Light

Sun – Featuring NOAA 10987, 10988, 10989
Sketches and Commentary by Erika Rix

2008 March 26, 1335ST – 1452ST (1735UT – 1852UT)
Solar H-alpha and White Light
PCW Memorial Observatory, Zanesville, Ohio, USA, Lat: 40.01 / Long: -81.56
Erika Rix

Temp: 57.0 °F / 13.9 °C
Winds: West 18 mph gusting to 25 mph
Humidity: 33%
Seeing: 5/6
Transparency: 2/6
Alt: 50.4 Az: 157.5

Equipment:
Internally double stacked Maxscope 60mm, LXD75, 40mm ProOptic Plossl, 21-7mm Zhumell
ETX70 AT, tilt plate, 8mm Televue Plossl

Sketch Media:
H-alpha – Black Strathmore Artagain paper, white Conte’ and Prang pencils, white vinyl eraser.
Added –5 brightness, +30 contrast after scanning in color at 300 dpi. Tilting Sun program used for digital Sun insert.

White Light – white copy paper, #2 pencil, .5mm mechanical pencil, photographed sketch instead of scanning for better contrast.

It was said that today NOAA 10989 produced an M2-class eruption causing a CME. I have to say that each of the three active regions had very bright plage seeming to curve around the dark specks of sunspots within each region. It’s not often I get such a great view of the sunspots themselves in h-alpha, but today 10988 had the largest umbral area and they all had one or two smaller dark spots. I could hardly wait to pull out the ETX70 with a white light filter to see the sunspots themselves in much greater detail.

Prom activity was very modest. After 3-4 strolls around the limb tweaking the Etalon, 6 areas of very small prominences came to view. The filaments on the disk were showy, especially the large blotchy one to the south of 10988.

With the white light filter, facula was clearly viewable around 10989, reaching out in several directions. Penumbrae were seen in most of the sunspots. I had hoped to increase magnification for a closer view, but with transparency becoming worse, as well as viewing in white light in the front yard rather then in the protection of the observatory, the white light view was already too soft. Increasing magnification would have made it impossible.

That’s No Moon…

Mars - Cimmerium and Elysium regions

Mars – Cimmerium and Elysium Regions
Sketch and Commentary By Carlos E. Hernandez

I made a pair of observations on December 28, 2007 using my 9-inch (23-cm) F/13.5 Maksutov-Cassegrain. I noted a significant amount of detail over the Mare Cimmerium and Elysium regions of Mars. I welcome any comments on my observations.

Date (U.T.): December 28, 2007
Time (U.T.): 01:20 (left image, IL) and 01:50 (right image, Wratten 38A)
CM: 227.5*W (left image) and 234.9*W (right image)
Ls: 009.0* (Early Northern Spring/Southern Autumn)
De: 0.7* North, p 1.00, Dia. 15.7″
Instrument: 9-inch (23-cm) F/13.5 Maksutov-Cassegrain
Magnification: 163x, 273x, and 359x
Seeing (1-10): 6-7, Antoniadi (I-V): II
Transparency (1-6): 5

Notes:
01:20 U.T. (Left image, CM 227.5*W, IL): The South Polar Region (SPR) appears obscured by a very bright to extremely bright (8-9/10). Mare Australe appears dusky to shaded (4-6/10) north of the haze. Electris, Eridania, and Ausonia appear to be obscured by a bright to very bright (7-8/10) haze. Mare Cimmerium appears dark to dusky (3-4/10) and mottled. The northern border of Mare Cimmerium contains projections (Laestrygonum Sinus, Cyclopum Sinus, and Cerberi Sinus, preceding to following). “Valhalla” was visible north of Mare Cimmerium as a dusky (4/10) band. Hesperia appears as a bright (7/10) diagonal strip between Mare Cimmerium and Mare Tyrrhenum. Mare Tyrrhenum appears dark to shaded (partially obscured by a very bright (8/10) morning limb haze (MLH). Zephyria, Aeolis, Aethiopis, and Aetheria appears bright (7/10). Amazonis and Arcadia appear dusky to shaded (4-6/10) and mottled. A very bright (8/10) orographic cloud is visible over Olympus Mons over the north-preceding (evening) limb. Trivium Charontis, Phlegra, and Azania appear dark to dull (3-5/10). The Propontis Complex (Propontis I and II, Castorius Lacus, and Euxinus Lacus) appears dark to dusky (3-4/10). Elysium appears bright with a very bright (8/10) cloud over it’s north-preceding sector. Panchaia appears bright (7/10) and Lemuria (dusky (4/10). The Hyblaeus Extension appears dark to dull (3-5/10) following Elysium. Syrtis Major appears to be obscured the very bright (8/10) MLH. The North Polar Cap (NPC) appears brilliant (10/10) along the northern limb.

01:50 U.T. (Right image, CM 234.9*W, Wratten 38A (Blue) filter): Mare Cimmerium appears dusky (4/10). The southern limb, preceding (evening) limb, northern limb, and following (morning) limb appear very bright (8/10). A very bright (8/10) orographic cloud appear over Olympus Mons over the preceding limb. A very bright (8/10) cloud appears over Elysium.

The best of luck in your own observations of Mars.

Regards,
Carlos E. Hernandez

Sparkling Winter Blossom

NGC 2174

NGC 2174
Sketch and Commentary by Bill Ferris

NGC 2174 is a truly spectacular nebula; one belonging on every amateur’s “must see” list. My sketch captures a 109X view in the 18-inch Obsession. The emission nebula ranges throughout the 45′ diameter field of view. The bright star near the center is 7.6 magnitude HD 42088. A clump of seven 8th through 10th magnitude stars blazes immediately to the north and east. Another 60+ stars are scattered across the field. A UHC filter enhances the breadth of the nebula. An OIII filter seems to give the dark rifts more oomph. The brightest portion of NGC 2174 surrounds HD 42088. From here, prominent branches extend to the north and southwest. More subtle patches of fluorescing gas are strewn about the field. What a magnificent object! You’ll find NGC 2174 in the northern-most reaches of Orion. 4.6 magnitude Chi2 (62) Orionis shines just 1.5 degree to the west.

A Cluster Between the Two Dogs

M47

M47
Sketch by Michael Vlasov

According to the fine folks at SEDS, M47 lies about 1600 light years away, contains around 50 stars, and spans 12 light years. Overall, the population of stars is similar to that of the Pleiades. It contains two orange K-type giants with masses about 200 times that of the sun. It is estimated to be 98 million years old and is receding from us at 9 km/sec. Charles Messier cataloged it in 1771, but due to an error in marking its position, it was not recognized as a Messier object and so re-discovered by William Herschel in 1785. In 1984, a book by Hodierna came to light in which he described the cluster as “a Nebulosa between the two dogs” in 1654, making him the original discoverer on record.