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.

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.

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.

A Dust Lane Runs Through It

NGC 4565

NGC 4565
Sketch By Serge Vieillard

Located 31 million light years away in the constellation Coma Berenices, lies the spectacular edge-on galaxy, NGC 4565. It’s length is bisected by a prominent dust lane, and is thought to resemble our own Milky Way if viewed from outside. Serge Vieillard sketched this galaxy with graphite pencil, and inverted it to resemble the view through the eyepiece.

The Fall Spectacle of 2007

Comet 17P/Holmes

Comet 17P/Holmes
Sketch and Commentary By Frank McCabe

Comet 17P/Holmes can be seen close to Mirfak (Alpha Persei) this night. The comet remains brighter than 4th magnitude. Under clear, cold skies I was able to sketch the comet without optical aide after spending an hour dark adapting. In order to see the extent of the comet I used averted vision on the comet and on some of the fainter stars. The constellation Cassiopeia is also included in the sketch to the left of Perseus. For sketching I used a piece of white sketching paper 7” x 10” and 2H and HB graphite pencils. After scanning and inverting, I adjusted the star magnitudes from written notes and cleaned up some of the star shapes to round using Microsoft Paint. The sketch took about 30 minutes to complete after starting at 4:00 UT 11/16/2007.

Frank McCabe

Globular with a Wealth of Variables

M3

M3
By Cyprien Pouzenc

Lying about 33,900 light years away in the constellation Canes Venatici, M3 is a globular cluster populated by about a half million stars. This cluster is notable for being rich in variable stars and also contains a relatively large number of Blue Stragglers. It provides a visual delight to the telescopic observer, as noted by Cyprien Pouzenc in this sketch from Southern France. Cyprien’s translated notes can be seen below:


Sketch done with graphite pencil on white paper.

Object : M 3
Nature : Globular Cluster
Constellation : CVn

RA : 13h 42′ 11,2″
Dec. : +28° 22′ 48″

– Date, hour, duration : 10-05-07, 22:35 TU, 9′
– Location, elevation : La Roque d’Anthéron (south of France), 175m

– No wind, T°16
– T1 (limit magnitude in UMi with naked eye : 6.17), P1 (light
pollution), S2/200x (Seeing) — all in 0 to 5 scale, 0 is the best.

– Reflector : Meade Lx90, 203/2000, F/10

Comments :
200x, H=73°; Circular cluster saw in direct vision, seemingly
fully resolved in beautiful dust of stars. A luminous central area
without important gradient is surrounded by a halo less luminous and by
a crown very grainy.

Web page of this object : http://cyprien.pouzenc.free.fr/M-3.htm
Web site : http://cyprien.pouzenc.free.fr

Clear Sky !


Cyp

An Irregularity in the Local Group

NGC 6822

NGC 6822 (Barnard’s Galaxy)
Sketch and Commentary by Eric Graff

NGC 6822 is a dwarf irregular galaxy and a member of the Local Group at a distance of 2.8 million light years. As such it is the best example of a dwarf irregular galaxy accessible to observers in the northern hemisphere. This galaxy was discovered visually by renowned astronomer Edward Emerson Barnard using the 5-inch Byrne refractor at Vanderbilt University in 1884. It is named Barnard’s Galaxy in his honor. In 1924 Edwin Hubble resolved NGC 6822 to its core in photographs with the 100-inch telescope at Mt. Wilson and discovered many Cepheid variable stars in the galaxy. Recent studies by the Hubble Space Telescope have suggested that the galaxy has maintained a relatively stable rate of star formation over the past 12-15 billion years.

Here are a few things to keep in mind, and look for, as you observe this object: NGC 6822 is one of those strange objects that apparently become more difficult to see with increasing aperture. Hubble noted that the object was easy in a 4-inch finderscope, but nearly impossible to detect visually in the Mt. Wilson 100-inch. Luginbuhl and Skiff in their Observing Handbook and Catalogue of Deep-Sky Objects, mention a similar effect as aperture is increased from 6 cm (2.4 inches) to 30 cm (12 inches). Robert Burnham Jr. “found the galaxy not particularly difficult” in 6-10 inch scopes at low power and estimated that it was easier to detect than the Veil Nebula in Cygnus (without a filter, I presume). Stephen James O’Meara suggests that it might be possible for amateurs to visually detect individual stars in NGC 6822 with “small telescopes”, suggesting Burnham’s estimate of 15th magnitude for the brightest stars is a little on the faint side. O’Meara also claims to have detected a pale green tinge in this galaxy.

I swept up NGC 6822 (panning due west from Beta Capricorni) in the 30mm Plössl (30x magnification), just northeast of the 5th magnitude star HD 186185 in Sagittarius. In fact, I swept right past this low-surface brightness spectre on my first try. This irregular galaxy has the initial appearance of a faint, mottled, stain on the velvety background of the night sky. Its shape is that of an elongated, slightly curved triangle, wider toward the north and concave toward the west. A few faint stars are superimposed on the faint glow, and many more are scattered across a rich field of view. Mottling is apparent, even at low magnifications, with slightly brighter patches north and south of center. Knowing that this Local Group member has a number of large HII regions, I tried to tease them out with Lumicon OIII and UHC filters. The results of this experiment were inconclusive at this magnification, but unlike most galaxies, which have a tendency toward vanishing with these filters in place, NGC 6822 remained steadily visible in both filters. The planetary nebula, NGC 6818 masquerades as a blue green 9th-magnitude star at the NNW edge of the field.

At 60x, NGC 6822 becomes a little more conspicuous due to the increased image scale and better contrast with the sky background. The mottling becomes more apparent as well in a highly irregular pattern. The brightest portions of the galaxy seem to be concentrated somewhat toward the southern half (near the apex of the triangle). Use of the OIII filter brings out a couple of potential HII regions near the northern edge of the galaxy. They appear nearly stellar in my scope, but an examination of nearly any photograph of this galaxy confirms their presence. (Here are a couple of Hubble photos of HII regions in NGC 6822: Hubble-X and Hubble-V.) At 120x, NGC 6822 morphs into a feeble, ghostly glow, difficult to distinguish from the black night sky. Nevertheless, some additional detail may be observed. Most of the galaxy’s light is concentrated in a bar running N-S with faint nebulous extensions to the west and east. The bar itself is broken into several feeble knots of light (possibly due in part to unresolved foreground stars, or stars in the galaxy itself).