Holmes’ Mega Coma

Comet 17P/Holmes

Comet 17P/Holmes
Sketch and details by Martin Mc Kenna

Nov 3/4 18.20 – 20.00 local time.

Tonight 17P/ Holmes was a spectacular object to those lucky enough to have dark skies. This was a night of revelation for me. In the 8.5″ F/7 reflector I measured the brighter inner coma at 15′ in dia. It was a bright lemon colour with beautiful segmented ring around the perimeter like a horse shoe with bright enhancements and dark obscurations. The N side described a beautiful curve with the S section soft and broken in profile. At centre was a very faint and soft false nucleus which looks more like a well defined smudge rather than stellar in the 32mm eyepiece. The dust fan was still bright and elongated to the south where it merged into a vague void of complexity where all the finer action was taking place. Surrounding the FN was 3 dark wedge-shaped holes or pits in the region between the FN and inner coma. By sweeping the telescope back and forth I could see the green transparent outer coma for 30′ either side of the inner coma. Since this central region was 15′ across I got a total diameter for the outer coma at 75′ or 2.5 times the apparent size of the Moon. The other coma has a very sharp edge with obvious cut off point where the coma ended and the background sky began. It was a disk-like shape very much like a CD. This effect was enhanced by the stunning dark ‘lip’ which surrounded the inner coma like a jet black scarf much like what is now being picked up on CCD images. This dark collar was very well defined and by letting the comet drift across the field I could see its passage with ease as it first entered then drifted in transit across the 1 degree FOV. The shape of this feature reminded me of an ‘Arcus’ or ‘Shelf Cloud’ which marks the gust front of a thunderstorm. I observed two long Ion tails, the first to the S and the second to the SE with the first being 1 degree in length. A nice fan of multiple fine streamers spread across the void between these two long linear features where the inner and outer coma meet.

My 10x50mm binoculars have a FOV of 5 degrees. Using these I was astounded to see the coma taking up much of the field which I estimated at 3 degrees in dia or 6 full Moon diameters!!. I couldn’t believe what I was seeing and was reserving severe doubts about the whole thing until I saw it easily again with well defined edge which flirted with the eastern most stars within the large open cluster between Alpha and Delta Persei. The entire sharp dark green outer coma looked like a smaller version of the Gegenschein during the times when it can be seen as an oval glow. Further more the ‘disk’ was not a perfect circle. The southern end looked ‘missing’ as if a wedge shaped section had been cut from the coma with scissors. I recently recall one observer describing this outer coma as shaped like a Jelly Fish and this was more or less what I could see also. Extending from the void in the southern section was a long linear ray of light approx 2 degree long. I do not know if this was a long ion tail or just an enhancement along the inner edge of the coma. Confused by the whole thing I decided to delay this observation until I could confirm it myself.

Tonight (Nov 4/5) the sky was stunning and very dark. In the 10x50s I could see the same size of coma and shape as observed on the night before. However even more astonishing was the view with the naked eye on this grand night. Using my finger tips held at arm’s length I could see the entire coma extending for approx 5 degrees in dia (10 Moon diameters) with the naked eye!!!.

I now believe that any future visual mag estimates and D.C estimates will be almost impossible with any degree of accuracy but for what it is worth I will stick to my last estimate of +2.5 at D.C:7

Jupiter – August 9, 2008

Jupiter

Jupiter – August 9, 2008
Sketch and Details by Carlos Hernandez

I made an observation of Jupiter on August 9, 2008 using my 9-inch F/13.5 Maksutov-Cassegrain. Much detail was noted over the planet, especially the North Equatorial Belt (NEB) and South Equatorial Belt (SEB). The seeing conditions were above average (5/10) for a short time before the clouds came in and ended my observing session. I welcome any comments that you may have on my observation.

Date (U.T.): August 9, 2008
Time (U.T.): 03:50
L1 201.1, L2 319.1, L3 316.6
Diameter (Equatorial): 46.4″
Instrument: 9-inch (23-cm) F/13.5 Maksutov-Cassegrain
Magnification: 163x
Seeing (1-10): 5, Antoniadi (I-V): III
Transparency (1-6): 4

Notes:
South Polar Region (SPR): Appears dark to dusky (3-4) and mottled.
South Temperate Zone (STZ): Appears thin and shaded (6/10).
South Temperate Belt (STB): Appears dark to dusky (3-4/10), thin and divided (northern component darker than southern). No ovals visible within it.
South Tropical Zone STrZ): Appears bright (7/10) with a thin, dusky (4/10) band over it’s central portion.
South Equatorial Belt (SEB): Appeared dark to dusky (3-4) and containing dark (3/10) dark condensations along it’s northern border and bright (7/10) undulating sections (strips) within it (preceding section wider in latitude than following).
Equatorial Zone (EZ): Appeared shaded to bright (6-7/10) with a thin, dusky (4/10) band across the center of it.
North Equatorial Belt (NEB): Appeared dark to dusky (3-4/10) and thin with dark rods (barges) along it’s northern border. Blue festoons (3/10) noted along it’s southern border.
North Tropical Zone (NTrZ): Appeared bright (7/10), but no other detail visible within it.
North Temperate Belt (NTB): Appeared thin, dark to dusky (3-4/10) and divided by a thin, bright (7/10) zone.
North Polar Region (NPR): Appeared dark to dusky (3-4/10) and mottled.

A digital image made using Photoshop CS3.

The best of luck in your own observations of Jupiter.

Regards,
Carlos

Details of the Great Red Spot

Great Red Spot

The Great Red Spot
Sketch and Details by Carlos Hernandez

I made an observation of the Great Red Spot (GRS) and surrounding region (South Equatorial Belt (SEB)) on August 10, 2008 (04:30 U.T.). The amount of detail visible within and surrounding the Great Red Spot (GRS) was impressive. The core of the GRS was a dark salmon color (3-4/10) surrounded by a reddish pink to white color (5-7/10) over the rest of the GRS. The South Equatorial Belt (SEB) was a light brown to a greenish-brown color (3-4/10) with bright (7/10), undulating rifts over it’s northern half. The South Tropical Zone (STrZ) appeared bright with a dusky to dull (4-5/10) band appearing to connect to the southern border of the GRS. A dark (3/10) elongated condensation appeared within it following the GRS. An elongated, and bright (7/10) oval BA was noted within the dark (3/10) South Temperate Belt (STB). The center of the GRS was timed at 130.3 (L2, 128.4 L3).

A digital image produced in Photoshop CS3.

Carlos

Planet Eight

Neptune

Neptune
Sketch and Details by Frank McCabe

Currently Neptune is the farthest planet from the sun with the demotion of Pluto to minor planet status. Neptune is slightly more massive than planet Uranus but is less voluminous than the seventh planet. Along with Uranus, Neptune is an ice giant. Neptune’s atmosphere contains much hydrogen and helium as well as ices of ammonia, methane and water. Much of Neptune’s blue color is due to measurable amounts of methane.
The discovery of Neptune was done by calculation. Neptune was co-discovered by John Crouch Adams beginning in 1843 and independently by Urbain LeVerrier in 1846. It was the perturbance of the orbit of Uranus in its revolution about the sun that led these astronomers to predicting the location of plant eight in the sky.
Currently the planet Neptune is in the constellation of Capricornus and is 29.1 astronomical units from earth. Its angular size is small at 2.3 arcseconds and at magnitude 7.8 it is not visible to the naked eye as Uranus (mag. 5.8) is from a dark sky site. It is positioned in northeastern Capricornus near several bright stars and therefore is easily located. Neptune reaches opposition in just a few weeks and makes a great target for any size telescope. If your scope can reach magnitude 13.5 try for Neptune’s moon Triton which can be found using the on-line Sky and Telescope’s Triton Tracker and a good high power ocular.

Sketching:
9”x11” white sketching paper; 4B, HB graphite pencils, light brown drawing pencil for Neptune and a blending stump; Scanned and inverted after cutting the sketch from the drawing paper and placing it against a brown paper background.

Scope: 10” f/5.7 Dobsonian: 24 mm widefield eyepiece 60x and 12 mm eyepiece 121x
Date and Time: 7-24-2008, 5:50-6:30 UT
Seeing: Pickering 7/10
Transparency: partly cloudy, Average 3/5
NELM: 4.3

Frank McCabe

Boattini’s Morning Reprise

C/2007 W1 (Boattini)

C/2007 W1 (Boattini)
Sketch and Details by Michael Rosolina

At present, there are two comets in the night sky that bear the name Boattini. One, C/2008 J1 (Boattini), is currently moving out of Cepheus and is visible all night long. The other, C/2007 W1 (Boattini), dipped below the horizon for northern hemisphere observers back at the end of May and did not reappear until the beginning of July. To see C/2007 W1, an observer had only a short time span as the comet rose with the constellation Cetus and was soon lost in the dawn glare.

My sketch shows how W1 Boattini appeared to me through my 15×70 binoculars on the morning of July 15th. I then was able to take advantage of clear weather and plot the comet’s position over the next two mornings as it traveled to the NNW through Cetus past the 4th magnitude star lambda Ceti.

The original sketch and position updates were done in the field on Strathmore sketch paper with a 2B pencil and blending stump. I then inverted the sketch after scanning, applied 5% blur, and added the text.

Like most comets, W1 Boattini was easiest to see from dark, moonless skies with good transparency. It was difficult to impossible to observe visually while the Moon was bright, but now that Luna is on the wane, it will once again be possible to observe it. It is now in Aries, higher in the sky and visible earlier and for a longer time before morning twilight. If you get the weather and opportunity, try and observe it over several mornings to detect its motion against the background stars.

Michael Rosolina
Friars Hill, West Virginia, USA