McNaught-Hartley in Motion

C/1999 T1 McNaught-Hartley

C/1999 T1 McNaught-Hartley B

C/1999 T1 McNaught-Hartley
Sketch and Commentary by Martin Mc Kenna

The top sketch shows C/1999 T1 Mc Naught – Hartley on Jan 14th 2001 at 06.30 LT low in the eastern pre dawn sky between Libra and Serpens in the 8″ F/10 S.Cass at 77X. Despite frozen mist, a harsh ground frost and a moon 4 days after full I could see this 8th magnitude comet quite easily and even picked out two tails, one of gas and one of dust.

The 2nd sketch shows the comet on Feb 25th 2001 at 05.47 LT in Hercules at magnitude 8.8. The sketch shows the comets NE movement over a 2 hour period.

This comet is very special to me as during Dec it was moving from the southern hemisphere into the northern hemisphere and I was desperate to see it. I tried to located it on every clear night even when the moon was full hoping to catch the comet as cleared horizon obstructions however despite trying so hard I could not get low enough in the eastern sky. The pre dawn hours of Christmas morning were cold, sharp with heavy snow on the ground and the corrector plate was threatening to freeze over at any moment. I guided the 8″ into the low eastern sky and began a hunt for new comets. 5 Minutes later as I swept through the southern section of Libra that was just rising over my neighbours rooftop and I found the comet! I was delighted beyond words and it felt like this comet was my Christmas present from the sky. I followed this icy wander on every clear night for months afterward as it moved from the morning sky into the evening sky. Mc Naught – Hartley taught me alot about observing comets, the long hours spent watching this comet have benefited me greatly with the future comets I have encountered.

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.

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 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

One Neat Comet

Comet C/2001 Q4 NEAT

C/2001 Q4 NEAT on May 14th 2004
By Martin McKenna

C/2001 Q4 NEAT on May 14th 2004 at 23.43LT through the 16″ F/4.5 reflector. The comet was a naked eye magnitude 3.7 object with a coma diameter of 20′ and a tail over 50′ long pointing to the NE through broken cloud. It was located in Cancer below the ‘Beehive Cluster’ (M44) low in the SW evening twilight at 71 degrees elongation from the sun. Overall the comet was a slight green colour with a broad fan shaped dust tail.

The rapidly rotating Earth placed the comet behind a tall tree in my back garden so I had to observe it through the gaps in the branches causing the comet to fade then brighten as it passed natures foreground obstructions in the telescopic field of view. Conor was also with me during this observing session who tracked the comet using my 8″ S.Cass – this was his first bright comet. Later Q4 NEAT dropped from view and joined T7 LINEAR – a situation that provided southern hemisphere observers with two naked eye comets!

Martin McKenna

Ephemeral Visitor to the Great Bear

Comet C/1999 S4 Linear

Comet C/1999 S4 LINEAR
By Martin McKenna

Comet C/1999 S4 LINEAR on July 23rd 2000 in the 8″ F/10 S.Cass at 00.43 BST. The comet was a faint naked eye object low in the bright summer twilight within Ursa Major. I watched with awe as the beautiful tail passed over several background stars dimming their light in the process. I had only started my comet hunting programme two months earlier so this comet was a very nice treat. Much to the surprise of astronomers the comet broke up soon after and disintegrated completely. I recall many mild summer nights watching this comet while being ate my midgets and pleasantly interrupted by bats and a large owl which gave me a visit from time to time.

Martin McKenna

McNaught’s Synchronic Bands

McNaught’s Synchronic Bands

McNaught sketch 2

McNaught’s Synchronic Bands (Charcoal above and Conte’ below)
By Jeremy Perez

Well, just when I thought this amazing comet would finish the rest of it’s presence in the southern hemisphere as a spectacle I would only be able to enjoy through photos, it pulled another surprise. Remnants of its huge tail began to be observed by observers in the northern hemisphere. A very rare feature, sometimes called synchronic bands, began to appear and to drift away from the sun. For those in the southern hemisphere, this makes for an unbelievably gorgeous sight in the evening sky. For those of us in the mid-northern latitudes, it presents an opportunity revisit this beauty for a bit longer.

After analyzing various recent photos of the comet from the southern hemisphere, I printed out a star chart, and marked the area in Piscis Austrinus where the most northern segments of the tail fragments were last imaged. I printed out a couple more sheets to take with me for sketches, and headed north of town to escape more stubborn clouds. After a 30 mile drive to Wupatki National Monument, I entered the park and drove in search of a parking spot with a good view of the western horizon. About 4 miles down the empty park road, I was surprised–but then again maybe not too surprised–to find Brent Archinal parked along the side of the road with his tripod and camera set up. Whaddaya know! So I set up next to him and waited for twilight to darken while enjoying a beautiful view of Venus and the crescent Moon setting together.

By about 6:50 PM with the sun about 14 degrees below the horizon, and the head of the comet 19 degrees below, a bright spoke began to show itself midway between Fomalhaut and Venus. It was amazingly long–about 20 – 25 degrees from the horizon up to Phi Aquarii. As the sky darkened more, and the Zodiacal Light became very prominent, more bands began to appear in a fan running from Piscis Austrinus through much of Aquarius. I finished shooting several photos at 7:05 PM when my batteries ran out. (I’m all about great planning.) I then spent the next half hour sketching every bit I could detect, which turned out to be a very good investment. My photos didn’t turn out well at all, and the sketches showed much more detail than the best shot (which can be seen below).

You’ll notice not one, but two sketches above. Both make use of a pre-printed star chart from Starry Night Pro so that I could concentrate on the comet tails during the limited time before it set. The first is a charcoal sketch using a chamois to blend in the zodiacal light and skyglow above the horizon. I then used a blending stump to add the synchronic bands. The second sketch is made with Conté pencil on black Strathmore Artagain paper. I traced the stars onto the paper from the same starchart, and then used a blending stump to add both the Zodiacal Light and synchronic bands (since the Chamois didn’t seem to work so well there). I’m definitely partial to the results of the first charcoal sketch. The Conté sketch does look better in person though.

McNaught Photo

Subject C/2006 P1 (McNaught) – Synchronic Bands
Classification Comet Tail Fragments
Position* Through Piscis Austrinus and Aquarius
Size Longest Segment: ~25°
Brightness –
Date/Time January 20, 2007, 07:00 – 07:40 PM MST
(January 21, 2007, 02:00 – 02:40 UT)
Observing Loc. Wupatki National Monument, AZ
Instrument Naked Eye
Eyepieces/Mag. –
Conditions Clear, breezy
Seeing –
Transparency ~ Mag 6.8+ NELM
*Sources Starry Night Pro Plus v. 5.8

Comet, Moon, and Mars

Comet, Moon and Mars

Comet 17/P Holmes, the Moon and Mars
By Carlos Hernandez

I was treated to a rare (at least these days in South Florida with our cloudy weather and tropical storms nearby) clearing of the heavens over the northern sky on October 30, 2007 (07:20 U.T.). I was able to view Comet Holmes (17P) in Perseus (~3.8 degrees from Alpha Persei (Mirfak, 1.78 m)) and I was impressed with the brightness of this interloper (Comet Holmes is currently estimated at magnitude 2.0). Capella (0.06 m) in Auriga was shining brightly nearby. The Waning Gibbous Moon (19.5 days old) was visible towards the east within Gemini close to a brilliant reddish-orange Mars (-0.58 m). The view was facing south and looking upwards (North at top and east to the left).

A digital image produced in Corel Painter X.

The best of luck in your own observations of this interesting comet.

Carlos

Celestial Scarab

Comet 17/P Holmes

After a couple days off from observing the comet, I was treated to more stunning views. The Moon was out of the sky, and Holmes was really showing its stuff. To the naked eye, it is a soft puff in Perseus. Through 15 x 70 binoculars, it is simply awesome, floating brightly amid a rich star field. Color is now hard to describe, but I think it looks like the most subtle aqua color. Through the telescope, it is wonderfully bright, and loaded with soft detail. The subtle outer halo makes the comet appear even brighter than it is, as though the radiance of the coma is lighting up its surroundings. The outer halo appears brighter to me along the southwest side. The coma sports a well-defined northeast side with a diffuse southwest edge. Its edges have a hairy appearance that looks like it is being blown gently to the southwest. Within the coma, the central condensation now looks detached from the pseudonucleus. Some very subtle radial features began to coalesce after 45 minutes of observing at 120X and 240X. I don’t know if these are real structures, or just the cometary version of Martian canals. A brighter jet seemed to connect the now faint pseudonucleus with the detached condensation.

My measurements with the astrometric eyepiece are as follows:

Central Condensation: 92 arc seconds / 1.5 arc minutes
Coma: 653 arc seconds / 10.9 arc minutes
Outer Halo: 1550 arc seconds / 25.8 arc minutes

Subject 17P / Holmes
Classification Comet
Position* 6:15 UT – Perseus: [RA: 03:45:52.4 / Dec: +50:32:29]
Size Central condensation: 92 arc seconds / 1.5 arc minutes
Coma: 653 arc seconds / 10.9 arc minutes
Outer halo: 1550 arc seconds / 25.8 arc minutes
Brightness* ~ 2.6 vMag
Date/Time October 31, 2007, 10:00 – 11:30 PM
(November, 2007, 05:00 – 06:30 UT)
Observing Loc. Flagstaff, AZ – Home
Instrument Orion XT8 (203 mm dia./1200 mm F/L)
Eyepieces/Mag. 25 mm Sirius Plössl (48X)
10 mm Sirius Plössl +/- 2X Barlow (120X/240X)
12 mm Meade Astrometric +/- 2X Barlow (~100X/200X)
Conditions Clear, calm
Seeing 3/10 Pickering
Transparency ~ Mag 5.8 NELM
*Sources Aerith.net; Starry Night Pro Plus 5 
*Based on published data.

A Speedy Reputation

Comet 8P/Tuttle

Comet 8P/Tuttle
By Michael Rosolina 

Comet 8P/Tuttle is a periodic comet that comes by our little corner of the solar
system every 13.6 years.  It was first discovered by Pierre Mechain 1790 but then
lost, not to be found again until Horace Tuttle spotted it in 1858.

This apparition is a particularly favorable one with Tuttle passing close to the
Earth–closest approach was 23.5 million miles/37.8 million km on January 1st.  By
the end of December, Tuttle had brightened to about magnitude 6, putting it at the
threshold of vision for sharp-eyed observers with dark skies. 

Because of its nearness to Earth, Tuttle lives up to the speedy reputation that the
word comet invokes.  At the time of this sketch, it was covering about 4 degrees of
arc every day as it moved rapidly south through the constellation Pisces into Cetus.
I have included Tuttle’s position at the start of my observation to give some
sense of the distance it traveled in less than an hour.

The sketch was done at the eyepiece on Strathmore 400 series medium weight recycled
sketch paper.  I used an HB pencil and a loaded stump and blended with my fingers.
After scanning I inverted the sketch digitally.