Great Great Grandfathers Comets

Bond1

The three comet sketches shown here were made by American astronomer and former
director of Harvard College Observatory, George Phillips Bond, son of the first
director William Cranch Bond. George discovered eleven comets and worked closely
with his father at Harvard College Observatory. Together the Bonds are credited
with the discovery of Saturn’s moon Hyperion at the same time famous British
astronomer and co-discoverer, William Lassell, also spotted it in 1848. The Bonds
were also credited with the discovery of the dusty crepe ring as William Lassell
later named it.

Bond2 

Using the new Daguerre’s photographic process, George P. Bond took the first
photograph of a star (Vega) in 1850 and within 7 years he was photographing double
stars like Mizar and attempting to use photography to determine stellar
magnitudes.

Bond3 

One of the most spectacular comets of the 19th century was Donati’s comet named
after its Italian discoverer in Florence. This comet reached a magnitude of -1 in
September of 1858 and had a tail extending 60° across the sky. The first sketch of
Donati’s comet was made without optical aid. The second sketch was made at the
eyepiece of the Harvard College Observatory’s 15 inch refractor. The last sketch
was made at the eyepiece of the same telescope of another comet the following year
called ‘the Great Comet of 1859’. In that same year George took over the
directorship of the observatory from his father. Six years later George P. Bond
died of tuberculosis before reaching his 40th birthday.
  
  Frank McCabe
  
  Sketches are from Astronomy for Everybody by Simon Newcomb© 1902, McClure,
  Phillips & Company, pages 268, 270 and 272

The Elusive Great Comet

Comet Mc Naught 

Great comet C/2006 P1 Mc Naught at 08.00 UT on Jan 19th 2007.

The comet rose above the low eastern horizon along with the rosy glow of the
approaching Sun. It was easily visible to the naked eye complete with tail hanging
above a distant telegraph post. This sketch shows the view in 10X50mm binoculars
with a 1 degree long white dust tail pointing at a shallow angle to the NE with the
‘shadow of the nucleus’ feature splitting the dust tail in two. I only had it in
view for 5 min’s before clouds rolled in but what a view it was!

Mag: -1.7 Dia: 3′ D.C: 9 and only 13 degrees from the sun.

Pencil and paper sketch inverted in photoelements.

Thanks

Martin Mc Kenna

N. Ireland

Silent Hunter

NGC 457 

NGC 457 is a beautiful Open Cluster in the Constellation Cassiopeia with
a pretty interesting shape: the two brightest stars, which glow in a
warm golden-yellow, form the two eyes of an owl, the rest of the stars
comprise the beak, the wings, the body and the claws, hence the name
“The Owl Cluster”. It is not difficult to draw and easily accessible with all
kinds of telescopes and thus well worth a visit.

Date: December 23, 2006
Location: Erbendorf, Bavaria, Germany
Instrument: Vixen Newtonian 4.5″ f/8 on Vixen GP
Constellation: Cassiopeia
Seeing: II-III of VI
Transparency: III of VI
NELM: 5m0
Magnification: 100x
Technique: pencil on white paper, digitally enhanced in Photoshop

Regards,
Sebastian

Cleomedes in the Waning Light

Cleomedes

Just north of Mare Crisium and formed during the Nectarian period more than 3.7
billion years ago is the 128 km. walled plain crater Cleomedes. This crater has a
high but worn margin and was nicely catching the last rays of sunlight overnight.
The large flat floor may have been flooded by lava that reached the crater floor
through fractures from the molten lava of Mare Crisium. What remains of the
central peak is a low wall oriented north-south and somewhat off center. A hint of
60 km. long ‘y’ shaped Rima Cleomedes was just detectable north of the central
wall running off to the southeast. To the northwest of Cleomedes is 57 km. crater
Burckhardt straddled by its close partners E and F. To the east of Cleomedes is
crater Delmotte (32 km.) and off to the northwest is crater Tralles (43 km.)
hugging the rim. On the floor from north to south are A and larger E which
together damaged the wall of Cleomedes upon formation. Crater B can be seen
south of the central wall and  then J to the southeast on the floor. Resting on the
south rim is crater C. This region of the lunar surface was fascinating to observe
in this part of the lunation.
  
  Sketching:
  For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’
  pastel pencils and a blending stump. Contrast was slightly increased after scanning.
  Telescope: 10 inch f/ 5.7 Dobsonian and 6 mm eyepiece 241X
  Date: 7-2-2007, 4:10-5:30 UT
  Temperature: 18° C (65° F)
  Clear, light winds
  Seeing:  Antoniadi II
  Colongitude  116.6 °
  Lunation  17.25 days
  Illumination 96.4 %
  
  Frank McCabe

Open and close

Melotte 111 

Melotte 111

Hello sketchers,

What is called the second closest star cluster to our sun? Looking at it with a
scope is of little use, because the grouping covers about 5° of sky. Some of its
stars look so bright in a scope, as if one can almost touch them. So here it is, my
impression of this beautiful naked eye cluster. I used the lowest power available,
but even the fov of 3° is not large enough to cover the cluster. So the sketch is a
composite image of overlapping observations. Because of the low power, the sky-glow
washes out al stars fainter than mag 10.9. I hope you like my impression.

Date : May 5, 2007
Time : 22.00UT
Scope : SkyWatcher 102/500
TV SP 32mm eyepiece
Power : 15
FOV: 5°
Filter : none
Seeing : 2.5/5
Nelm : 5.1
Sketch Orientation : N up, W right.
Digital sketch made with a digital tablet and PhotoPaint, based on a raw pencil sketch.

Rony De Laet

http://www.geocities.com/rodelaet, my personal website.

Four Old Battered Ones

Four old battered ones

On a frosty early morning in the fall of 2006, just a couple of days past third
quarter moon, I selected for sketching a famous old battered region between Mare
Nubium and Mare Cognitum. This region includes four large craters that were
damaged by low flying Imbrium ejecta that caused them to look old and battered
before their time. Nearest the terminator to the north is crater Guericke (59km)
with its flat lava flooded floor that opens to Mare Nubium. Crater Parry, smaller
at 49 km in diameter is older and also flat floored. The other two craters which
look ghostly in the sketch are larger and older and share common walls with Parry.
These craters are Bonpland (61 km.) to the west and Fra Mauro (96 km.) to the
north of Parry. The wall of Parry encroaches on Bonpland and both together on to
Fra Mauro to betray the cratering sequence of these three.
  
  Sketching:
  For this sketch I used: copy paper 8.5”x11”, #2HB graphite pencil,
  Pink pearl eraser.
  Telescope: 6 inch f/ 7.9 Dobsonian at 208x ( first light for this scope)
  Date: 10-15-2006 10:30-11:15 UT
  Temperature: 0° C (32° F)
  Clear, calm
  Seeing:  Antoniadi III
  Co longitude: 190 °
  Lunation: 23 days
  Illumination: 36 %
  
  Frank McCabe

Joys of Jupiter

Jupiter cropped

This was the first sketch for me in a long while. It is a medium that I had moved
away from as I moved more into astrophotography. This site compeled me to give it
another go. You can see how the Jovian bands have become more mixed in the recent
months. This was also shown on a recent release of photos from Hubble. My sketch was
done with pencil on a sketch pad and reflect what I saw through a 12″ DOB using a
Televue Nagler type 6 7mm ep. It was really fun to experience this medium again. I
will certainly not wait so long for the next sketch. I hope that you enjoy it as
much as I enjoyed doing it.
 
  Hulett Keaton
  Eagle Mountain Station
  Carpe noctem

Clarity brought to complexity

Stofler 
This is my impression of the Lunar Formation Stofler. It was sketched with a #2HB
0.5mm mechanical pencil on Strathmore Wind Power Sketching Paper. Other pertinent
details are on the sketch itself. I found this lunar feature to be one of the most
interesting that I have seen. It appeared to me, that this piece of lunar real
estate was painted with a giant bulls eye.

Jason Aldridge

Repsold on the rim

Repsold crater 

A favourable lunar libration put the crater Repsold at a better
perspective than what one usually finds.  And finding it on the
terminator made it an object for a quick sketch despite the obstacles. 
It was only a few days before a June full moon so the moon was quite low
(from 50 degrees north lat.) even when near the meridian.  Turbulence 
and generally poor seeing kept things from looking sharp for more than
brief  instants.  And the mosquitoes were bad enough that at times they
cast long shadows across my sketching paper.   Sketch done using
graphite pencils,  ink and some not entirely successfull applications of
whiteout.   I usually like to take longer with a sketch but the
mosquitoes kept the viewing short.  North is more or less up and east is
to the left.   Viewed through 150mm f/6 Maksutov Newtonian with
binoviewer, 2x barlow and 23mm eyepieces.

Repsold is a rather large crater at approximately 110 kms diameter that
is known for a prominant rille of the same name that runs through it. 
Some of the unusual highpoints in the sunlight of my sketch might be
part of that formation as they are oriented in an agreeable direction.  
But  being unfamiliar with that extreme limb crater,  I cannot say for
certain.  Sketching limb craters present its own unique challenges and I
find myself thinking more of the three-dimensionality of the crater as
you are no just ‘looking down’ onto the third dimension.

Gerry Smerchanski

Heart of the vortex

M51 A
M51

May 29, 2006

Raw pencil sketch (HB lead), negative view lightly processed with
Photoshop Elements

Raw sketch was drawn at the eyepiece

28 inch f4 Newtonian at 710x

Seeing 8/10

Transparency 8/10

Limiting magnitude 6.4

Once upon a time, or last May 29th to be exact, I was lucky enough to
experience one of those amazing nights that we all hope for every time
the sky clears. The sky was dark, transparent and steady and the
temperature was surprisingly comfortable. In short, just about perfect.
But the best part was seeing something new and surprising in an object
I’ve looked at many, many times through all sizes of telescopes.

M51 was near the zenith and looked great at first glance, which wasn’t
unexpected since I was looking at it through a 28″ Newtonian after all –
it should look great! But it looked even better than normal because of
the excellent sky conditions which to me means piling on the
magnification. One of the features I enjoy trying to see within M51 is
the beginning of one of the main spiral arms coming out of the core.
They look like two faint prongs projecting out from the northern side of
the core and quickly blend into that spiral arm. These prongs are
visible in almost every M51 photo which inspired me to try to see them
visually in the first place. I’ve seen them well in a 16 inch scope and
suspect a 12 inch would be able to pull them in too.

 M51 B

At 710x I started seeing small glimmerings of light shimmer in and out
of view within the prongs, like they were studded with tiny, barely seen
stars. But at 31 million light years distant M51 I must have been seeing
something else. Looking at the latest HST image of M51 these objects are
probably HII star forming regions and huge star clusters and probably a
Milky Way foreground star or two.

A brief aside on my sketch – I concentrated on the core area and the
star-like points that glimmered in and out of view and that the farther
from the core I got the less detail I put in the sketch. Also, the fine
textures around the core and prongs are probably an artifact originally
caused by the texture of my notebook paper. The original pencil sketch
was scanned and enlarged about 300%, and then lightly processed in
Photoshop.

Howard Banich

Portland, Oregon