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.

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

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

Pluto From Pluto

Pluto from Pluto

“Pluto from Pluto” after Mel Hunter
By Frank McCabe

  In the spring of 1963 I was a junior in high school and purchased for 75 cents a
Pyramid book titled “Nine Planets”. The author of the book, Dr. Alan E. Nourse
worked his way through medical school by writing magazine articles about science
fact and also science fiction. I found this author’s writing style riveting as a
young lad. Today most of the content of this book is quite outdated although in
1963 it was an exciting read. Planet Pluto, the “Mighty Midget” as the author
describes it is more unknown than known and will be explored. The author
speculates on the nature of this mysterious planet in the chapter titled, “Pluto
and the Outer Reaches”.
  So this chapter too will become part of the discarded speculation of the past
because in another 7 years new information about Pluto will be gathered by the New
Horizons spacecraft during the July 2015 close
encounter.(http://pluto.jhuapl.edu/) At that time the former planet Pluto will go
from unknown minor planet to known minor planet.
  The author had some wonderful assistance in writing and proof reading the book
from well known artist Mel Hunter. Eight of his beautiful paintings are shown in
black and white and can be found between pages 128 and 129. The last one “The
surface of Pluto, with the Sun in the distance” was the one I was looking at to
create this color crayon drawing that I made in the spring of 1963 some 45 years
ago.
  I requested and happily received permission from Mel Hunter’s widow sculptor Susan
Smith-Hunter to make this post.
  Information about these two talented artists can be found at Smith-Hunter Gallery
http://www.smithhuntergallery.com/biogrophies.html and
http://en.wikipedia.org/wiki/Mel_Hunter

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

Ringed World With “Children” in Tow

Saturn

Saturn, March 3rd 2008
By Carlos E. Hernandez 

I made an observation of Saturn on March 3, 2008 (03:45 U.T.) using my 9-inch F/13.5 Maksutov-Cassegrain (163x). I noted a good amount of detail over the globe and rings. Both the South Equatorial Belt (SEB) and North Equatorial Belt (NEB) were visible as brownish-reddish bands. The South Polar region (SPR) appeared brownish with a dark center. The North Polar Region (NPR) was also brownish. The inner portion of Ring B was dusky (4/10). Rhea (9.8m) and Dione (10.2m) were visible north and following the planet. Titan (8.4m) was visible preceding and south of the planet.

A digital rendering produced in Photoshop CS3.

Carlos

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