Sunny Hawaii

 Sunny Hawaii

A unique sunspot grouping, AR963, emerged this week and has been dubbed by some “the
Hawaiian Islands”. The large ‘island’ is about the size of Neptune and all the little ones are each about the size of Earth. Atmospheric conditions prevented anything but brief glimpses at the Sun through heavy clouds and gusty winds.

This grouping is definitely one to keep an eye on!

The Sun with AR963
100mm acromat refractor at 48x (25mm Plossl + 2x Barlow).
Graphite pencil on white paper, blending stumps.

Andrew English

Gibbous Ruby World

Gibbous Mars 1

I had intended to catch up with Mars in June to begin my
observations and sketches of this exciting opposition.
Unfortunately a long run of poor weather in the UK prevented me
from doing this. Finally I caught up with the Red one early on the
morning of Sat 8th July. It was hard work but I sucked out some
detail in the end from the distant ruby planet.
  
Dale Holt

Here is the original SPA observation form with all the details about Dale’s sketch:

Gibbous Mars

Edge-on galaxy

NGC 4565 

I was observing Melotte 111 with a richfield scope when I ran into this galaxy.
While being limited to a maximum power of x63, I tried to make the best of the
observation. This galaxy looked rather faint. I needed to jiggle the scope to set
this galaxy in motion. This technique helped me to determine the real shape of this
beautiful but elusive edge-on galaxy. I would like to repeat this observation in the
future with higher powers of x80 and x120, to see if more details are visible in a
four inch scope. I hope you like the view

Date : May 5, 2007
Time : 22.30UT
Scope : SkyWatcher 102/500
Vixen LV Zoom at 8mm
Power : 62.8
FOV: 47′
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.

Lights Out for Eratosthenes

Eratosthenes

   At the southern end of the lunar Apennines on the border between the Bay of
Billows (mostly in darkness) and Sea of Rains lies 60 km. crater Eratosthenes. I
was off and on observing over most of the night. By morning twilight when the moon
was high in the east, Eratosthenes crater was experiencing sunset. The deep, dark
caldera-like aperture was undergoing sunset at the beginning of my sketch. This
3.2 billion year old land mark crater is the defining feature of the Eratosthenes
time period. While sketching I could clearly see much of the ejecta pitting of
Copernicus and its ray material which crossed the region 2 billion years after
Eratosthenes formed. I did not include much of the Copernicus crater impact
features because they are in my opinion more suitable for high resolution
photography or direct visual examination at high power. In this sketch I tried to
briefly capture the overall eyepiece view.
  
  
  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: 7-8-2007, 9:15-10:30 UT
  Temperature: 22° C (73° F)
  Clear to partly cloudy, light winds
  Seeing:  Antoniadi II
  Colongitude 190.2 °
  Lunation 23.25 days
  Illumination 42.2 %
  
  Frank McCabe

Splash in the water

Prom sequence 

This erupting prominence sequence reminded me of a rock plopping in the water. It
was brilliant to watch. This observing session nearly made me late for my brother’s
wedding, but I just couldn’t tear my eyes away from the view to to give myself ample
time to look presentable for the special occasion. As a last minute idea to add to
their wedding present, I framed the first sketch of this sequence with the date for
them….starting their new lives together with a bang, so to speak. Number 963 for
the sun, day one for my brother and his new wife. Sketches done with black
Strathmore paper and white Conte’ crayon.

Erika Rix
Zanesville, Ohio

This is a link to an animated sequence of the same session that Erika produced herself!

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.