Mars adjacent to the Lagoon Nebula
(Planet and Emission Nebula)
Hartesbeespoort Dam South Africa
28th October (2014)
Graphite Pencil, smartphone photo using the invert function on PS phone app.
In Southern Skies at the moment and made the most of the opportunity to sketch some really nice deep sky objects in and around the teapot including M7 and the Lagoon Nebula (with Mars adjacent to it)
Object Name: M 27 dumbbell nebula
Object Type: Nebulosa Planetaria
Location : Monte Nieddu, Padru, Sardegna
Date : 17/10/2014
Media :graphite pencil, White paper , processed with gimp
observed with dobson SW 10″ goto at 96X with UHC filter.
SQM: 21.2
Dear ASOD,
I recently made the drawing on this spectacular Sunspot group. I used the drawing program MyPaint.
Also known as: Sun – AR 2192
Date/time: 2014.10.27. 08:10 – 09:30 UT
Equipment: 120/1000 Newton (Primary and secundary mirror withouth aluminium coating)+gaswelding schield (5 DIN) + OIII filter, Azimuthal mounting,
+ GSO Plössl 20mm + Scopium SWA 15,10mm + 2x Barlow
Seeing: 6-8/10
Transparency: 2-3/5
Temperature: 10°C
Humidity: –
Wind: –
Location: Zákány, Hungary N46°14′ 59,2” E16°57′ 15,3”
Observer: Bognár Tamás
http://univerzumkepekben.hu/ar2192-bognar-tamas/
Best Regards,
Tamas
http://univerzumkepekben.hu/
Object Name: AR 2192
Object Type: Sunspot group
Location: Carinthia
Date: 2014-10-26
Media: Graphite pencil on white paper. Digital work done with Gimp 2
Seeing was very good at the beginning of my observation – i was able to magnify 200x. The visible details were breathtaking and I decided to sketch just the most striking part of the sunspot.
I was also able to observe and sketch a nice X2-Flare.
Clouds made it not easy to observe the enormous sunspot group AR 2192 in the Low Countries. I had only one good day to observe and sketch this marvel at ease. Thanks to good seeing conditions I could see – despite my small telescope – an impressive amount of detail. I hope the group will survive his voyage on the far side of the sun and give us another beautiful display.
Clear skies
Jef De Wit
Object: Sun
Location: Biggekerke, Netherlands (51°29’ N 3°31’ E)
Date and time: 27 October 2014, around 9.30 UT
Equipment: 8 cm refractor, Baader Herschel wedge, Solar Continuum filter
Eyepiece: 13mm Nagler T6 (79x)
Medium: white, gray and black pastel pencils, a Pierre Noire pencil and a light gray soft pastel on white printing paper, scanned, mirror reversed, contrast adjustments with Paint Shop Pro
Hello,
Enormous sunspot AR2192 was one of the events lighthouse of these last days, so enormous as it was the object of several drawings of which this one, made on October 27th, 2014.
Four hours were necessary to realize it (2 hours behind the ocular + 2 hours to polish up it installed at a table).
Lunette of 102/1000 – ocular ES 6,7 mm – Prism Herchel and filter Continuum.
Department Yvelines – FRANCE.
Bye.
Wilfried COLOMINA
Object: Messier 77 (Seyfert galaxy, Cetus)
Date: 28. 11. 2011.
UT.: 21h01m-21h29m
Equipment: 305/1525 Dobsonian telescope
Mag.: 218x
FOV: 12’
S = 8 / 10 T = 5 / 5
Observer: János Gábor Kernya
Location: Sükösd, Hungary
Total Lunar Eclipse of October 8, 2014, observed T250, Australia, north of Katherine. Nice atmosphere in the twilight moonrise partially eclipsed silhouetted against the red cliffs. This string is selected among the eight drawings, sketches showing the COLLECTED colors and visibility of lunar formations.
Full Moon déssinée the eve of the eclipse. It served as the background image for the realization of the rosary.
Sincerely
Serge
Lunar Crater Copernicus
Across the Carpathian Mountains resting on the eastern Ocean of Storms is the
landmark crater of the Sea of Islands, mighty Copernicus. Copernicus is a 95
kilometer diameter complex crater that begins to show itself in all its majesty
two days past first quarter. During the time of “Snow-Ball Earth” 800 million
years ago the event that created Copernicus suddenly occurred. What remains is a
3.8 kilometer deep hummock covered flat floored, centrally peaked, terrace walled
spectacular sentinel. Especially during high sun the bright ray system of this
crater can be seen extending from the base of the glassy glacis in all directions.
The descent from the rampart to the mare floor below is about one kilometer. Three
of five peaks were clearly visible in morning sunlight. In 1999 the Clementine
near infrared camera detected magnesium iron silicates in the peaks indicating
rebound of this deep rock through the surface crust following the impact event.
To view this impressive crater all you need is a good pair of binoculars and an
opportunity between two days past first quarter and one day past last quarter.
Weather permitting, you can see it tonight.
Sketching:
For this sketch I used: black Strathmore 400 Artagain paper, 9”x 12”, white and
black Conte’pastel pencils and a blending stump.
Telescope: 13.1 inch f/5.9 Dobsonian and 9mm eyepiece 218x
Date: 11-03-2014, 00:45 – 02:10 UT
Temperature: 0°C (32°F)
clear, calm
Seeing: Antoniadi III
Co longitude: 23.2°
Lunation: 8.9 days
Illumination: 69.3 %
Phase: 67.4°
Frank McCabe
The (Planet) Jupiter is one of the most difficult objects to observe. lt has most delicate subtle figures on surface atmosphere. Speak frankly my 13″ og showed me nothing but two main belts and 3-4 minor belts since first light the fall 2013 that not ones to surpass 12″, 8″, 6″, or 5″ED or 8″ dob at least in detail performance. Tonight’ early morning It showed me countless wrinkles on the King’s face though just at the 5-6 number of times one time was only shortest moments 2-3 seconds for 10 minutes with rated 9/10 seeing. The other interesting features were as you see [1], on the nights last autumn just near the first light night, the Europa’s color was turkish blue gray, but on this night it was pale yellow, the surface color of Europa really changed after one year ? The optical train was(is) same; flat-og-tv bino- tv nagler 7sThe [2]….. 13″ OG showed Ganymede’s contact moment with Jupiter’s limb, because the 13″ achromat’s chromatic dispersion effect of light produced weak contrast, could not identifyed the exact situation of the contact moment. For 10 minutes Ganymede moved 5280kmx0.7=3696km, the projected velocity of Ganymede is calculated as 3696km/ 600s= 6.16km/every second. # l usually write the observing date till fully to dawn as the same day .
—————-
13″ refractor, x530- x770
Location ; Backyard home in South. Korea
white paper [A4] Daler Rowney , graphite pencils
Date of observe; Oct. 28( 29). 2014.
