A photogenic pair

Theophilus and Cyrillus at Sunrise 

Theophilus and Cyrillus at Sunrise

Sketched over a 1.5 hour period at the eyepiece on Sunday April 22,
2007.  (2:30 to 4:00  UT 23/04/2007)   More time spent afterwards
colouring in shadow regions etc.  Done with graphite pencils (4H to
4B),  black ink and whiteout on white paper.   Scope was Celestron
9.25,  binoviewer,  2x barlow,  and 24mm eyepieces.  Picture was
reversed left to right once scanned to give a upright and correct
left/right view.

At the public star party last month (March) with the moon at the same
phase, I used a similar scope setup trained on these same craters to
illicit some “oohs”  and “wows” from the crowd.   After spending most of
the time looking at these craters I realized that the pair was quite
‘photogenic’ and would make for a nice sketch.    This month,  they were
even more strategically placed to reveal the terrain.  The smaller
crater Madler was also quite interesting and included.    One thing that
made this sketch a bit out of the ordinary was the unusual interior to
Cyrillus which has some unusual landscapes near the border with
Theophilus.  The light and shadows between Theophilus and the terminator
was also unusual and complicated.  My first sketch in over a year; it
seems I’m slowing up.  Taking this much time to capture all the details
is not the best for accuracy on transient lighting on lunar features.

Gerry Smerchanski

Darkness over Swansea

Darkness over Swansea 

The lunar eclipse of March 2007 fell over midnight of the 3rd and 4th,
the Moon being in Leo, and in the mouth of the Lion was the planet Saturn. The
sketch is based around 00.30 hours UT, sketched at the top of 600 foot high Kilvey
Hill. The path leading to the summit has a cluster of communication masts on one
side and a Bronze Age burial chamber, now only just visible above the surface, on
the other side. Standing there between the two, looking at the eclipse with the
City of Swansea spread out below, all was very quiet and for once it was a very
clear sky. It felt like a scene out of the fifties TV sci-fi series ‘Quatermass’.
 
J.E. Thomas

Category: Moon – Total Eclipse
Title:  ‘Darkness Over Swansea’
Media: Conte Pastel Pencil on Black Camford Paper
Size: 142 kb

Fire in the sky

The Flame Nebula 

I used a Watec 120N deep sky video camera running through a Synta 6″ F5 refractor to display a real time image of ‘The Flame Nebula’ NGC 2024 on a TV monitor. This image was Superior to that at the eyepiece of my 14″ F5 Newtonian on which the refractor rode even when employing a UHC filter!

Using light weight black card, white watercolour pencils and blending stumps I attempted to record the spectacle as best I could, resulting in this scanned and totally unprocessed image.

Dale Holt

Shadow on the cloudtops

Jupiter/Io Shadow Transit 

Jupiter/Io Shadow Transit

With its large apparent diameter, turbulent belts and zones, and Great Red Spot,
Jupiter is a fascinating object to observe.  This fascination goes up another notch
when one of the four Galilean moons makes a transit across the Jovian disk.

A transit occurs when the orbit of one of Jupiter’s moons takes it across the face
of the planet as seen from our vantage point here on Earth.  The moon itself can be
hard to detect, but the inky black shadow that it casts on the planet’s cloud tops
is easily seen with most telescopes.

In the hour of time recorded in the sketch, Jupiter is rotating from left
(following) to right (preceding).  Because the Great Red Spot happened to be visible
during the transit, the observer can get a sense of the incredible rotational speed
of this giant planet–one complete rotation about every ten hours!

The sketch was done at the eyepiece with 2B, HB, and 9B pencils on Strathmore 400
series 80 lb. paper.

Michael Rosolina

Observational Data:

Time: 23 May 2006  0300-0400 UT
Telescope: 8″ (20cm) SCT f/10
Magnification: 254x & 200x
Filters: Wratten #11, #56, #80A, & IL
Seeing: 4-5/10 (Pickering)
Transparency: 4/6
System II: 102° & 138°
Altitude: 35°
Diameter: 44.2″
Magnitude: -2.5

Kiss of the spider

The tarantula Nebula 

NGC 2070 (30 Doradus) The Tarantula Nebula

Located in the Large Magellanic Cloud in Southern Skies, the Tarantula
Nebula has an apparent magnitude of 8 and is about 160,000 light years
distant.

The exciting thing about ‘The Tarantula’ is that it is a nebula in ‘another
Galaxy’. If it was as close to us as the Orion Nebula is, it would fill 60
degrees of the sky and far outshine Venus!

It is named ‘The Tarantula’ due to it’s appearance being like a giant
spider.

Drawn with number 3 pencil on white art board, scanned and inverted in
Photoshop CS.  Red Hue added in Photoshop CS.
Date Drawn: 2006 while observing Tarantula through a 12″ reflector with a
32mm 2″ Erfle Eyepiece.

Ken James
Snake Valley, Australia

Over a scarlet limb

Over a scarlet limb 

Easter Parade

A Photoshop rendering of the solar limb as seen with a 70mm refractor (a “Pronto”)
using a 40mm Coronado H-alpha filter and a 12mm Nagler (~40x).

The dynamic chromosphere of our Sun seldom fails to surprise me. A quick setup to
look at the Sun last Sunday (April 8th at local noon) turned into an hour-long
observing session when my telescope revealed a small eruptive prominence.
Unfortunately, the seeing wasn’t as good as it sometimes can be so I patiently
waited for steady moments. Over a hour’s time the “spire” prominence slowly changed
shape with structure — knots — brightening and disappearing.  A small hedgerow
prominence (not seen in my drawing) remained virtually unchanged.

This is my first attempt at running one of my rough pencil sketches through
Photoshop. I hope, with time and practice — and better seeing — I can improve
my drawings.

Dave Riddle

The turbulent flower

The turbulent flower

Information about sketch:
 
Sketch is of M20 – the Trifid Nebula
 
Done on the 23rd of September last year
 
Drawn completely at the eyepiece of a 12.5″ f6 dob using a 13mm T6 Nagler
for around 143x.  It was done on white sketch pad paper using a graphite
pencil.  The sketch was then scanned and converted to the negative in
Irfanview.
 
Cheers
 
Andrew Durick
Brisbane, Australia

Thinking outside the circle

Virgo Cluster

Virgo Cluster panorama

This sketch was made from McDonald Observatory’s parking lot near Fort
Davis, Texas, during a trip down south. I used a 14.5″ Dobsonian and 26mm
Plossl eyepiece, and graphite on paper (reversed in Photoshop for effect). I
had prepared circles for sketching, but we ran into a streak of 6 clear
nights and I ran out, and had left my circle template back in Winnipeg. I
decided to just start sketching without the boundary of an eyepiece filed
and see what happened.  I really like the wide-field effect of not using an
eyepiece FOV circle – especially for clusters that need to be seen in
context.

Scott Young

When an iron heart stops beating

M1 Crab nebula

Messier 1
Meade Lx90 10″
167x
Seeing/Transparancy- Average
NELM- 5.8
Medium- Graphite

Sal Grasso

In the year 5,246 B.C., a star with a mass about three times that of our Sun was losing its life-long struggle with gravity. It had burned the hydrogen and helium in its core long ago and had begun burning ever more heavy elements until it reached iron, an energy absorbing reaction. Without the radiative core emitting enough energy to sustain a balance between gas pressure and gravitation, there was to be only one result. The crushing weight of the star’s atmosphere would collapse upon its iron core. The rebound energy would then produce a titanic explosion that would blow the star’s atmosphere into space and produce an intensely ferocious burst of neutrinos, gamma, x-ray and optical radiation. As it happened the stellar core would collapse even further (via implosion) and the electrons would be forced into very close proximity to protons, causing them to become neutrons. Only neutron degeneracy, an aspect of the Pauli  Exclusion Principle and the star’s initial mass prevented the runaway collapse to a black hole.  In this compact state, a city sized 10 km sphere contains the entire mass of the Sun and rotates at a dizzying 30 times per second. Retaining a strongly intensified magnetic field, it sends pulses of radiation from its magnetic poles at very regular intervals as it rotates.   

Six thousand three hundred years later, in 1054 A.D., Chinese astronomers took note of the position of a visitor star in the constellation of Taurus, the Bull. 953 years later, this visitor star is now seen as an expanding cloud of gas fully 12 light years wide. The rate of expansion is actually faster than the calculated rate for a free explosion, a result that indicates the intense magnetic environment accelerates electrons to relativistic velocities thus providing the energy for this “accelerated” expansion. Current measurements indicate that the complex filaments that thread the nebula are expanding at approximately 1000 meters per second.