Key Hole

NGC 3372, Eta Carine nebula, Keyhole region
NGC 3372 - Eta Carine nebula - Keyhole region

Date: 2010 04 17
Place: Tivoli, Namibia
Scope: Dobson Obsession, 20”
Eyepieces: Panoptic 35mm and Nagler 16mm (nebula), nagler 9mm and 3.5mm (Eta Car)
Magnification: from 73x to 725x
Filter: Lumicon OIII (old, with H alpha included in passing band)
Duration of observation: 55 min (Eta Car) + 50 minutes (nebula)
Process: sketch with pencil on rough paper, with notes and curves of luminosity (isophotes) in a scale from 0 (black) to 10 (most luminous DSO spot in the sky)
Final process: drawing made with Paint Shop Pro

More details and drawings at www.deepsky-drawings.com.

Regards

Bertrand

Clouds Spoiled the Occultation

Moon and Xi Sagittarii
Moon and Xi Sagittarii

Hi.
Yesterday (October 31st) I went to see interesting occultation. The star Xi Sagittarii was to be obscured by the Moon. Unfortunately, five minutes before the occultation the clouds came. What a bad luck.
So I have only a sketch of the Moon and Xi Sgr in short distance from each other 🙁

Object: Moon & Xi Sagittarii
Date: October 31st, 2011
Time: About 18:25 (6:25 PM)
Place: Nowy Sącz, Poland
Equipment: Binoculars Bresser 10×50
Technique: White pastels on black art paper. Tooling, levels, color, light in GIMP2
Author: Aleksander Cieśla (Wimmer)

Supernova SN 2011fe in Messier 101

sn2011fe in Messier 101
SN 2011fe in Messier 101

Here is a sketch of the unusually bright supernova that appeared last August 24th in the Pinwheel Galaxy (M 101) in Ursa Major. SN 2011fe is now at its maximum around magnitude 10 and it is very easy to see in my 120mm refractor, but it was also easy with an 80mm refractor (I estimated magnitude 10.3 on Sept. 4th and 10.0 on 6th). In contrast, as I am observing with moderate light pollution and M 101 is low, the galaxy itself is barely visible and I only can see the central region with effort. SN 2011fe is a nearby type Ia supernova and the brightest one since 1987. 2011 is being a great year for supernova observers!

Sketch: 2HB graphite pencil on white paper, scanned and processed with Photoshop CS3
Object Name: Supernova SN 2011fe in M 101
Object Type: Galaxy and supernova
Location: Asturias, Spain
Date: September 4th, 2011
Instrument: 120mm f/8,3 refractor + Hyperion 13mm (77x)
NELM: around 5.2, moderate light pollution

Regards,
Diego González

Albireo – the Orange and Blue Star

Albireo
Albireo

Object Type: Triple star system
Location: Płaza, Poland
Date: 10.08.2011
Media: graphite pencil, white paper, inverted, Photoshop CS2

Albireo is a beautiful, triple star system that consisting of Beta Cygni A – the orange, cool supergiant (in fact this is double star, but they’re too close to see it resolved. The second component is the Beta Cygni B – the Be star.

Alpha and Epsilon Lyrae

Alpha and Epsilon Lyrae
Alpha and Epsilon Lyrae

This is my first attempt at sketching a star field.

Object Name: Alpha Lyra – Epsilon 1 & 2 Lyra
Object Type: Double Star
Location: Locust Grove, VA
Date: 17 July 0130 UTC
Media: Graphite #2 Pencil on white paper. Photoshop inversion, enhancement.
Instrument: Oberwerk 15 x 70mm Binoculars
Weather: Clear/Partly Cloudy, 80 degF, Seeing 4/5, Transparency 4/5
Notes: Alpha Lyra drew my attention right at the end of twilight, and it was a beautiful sight with the Epsilon 1&2 double nearby. I could not quite discriminate (split) Zeta 1&2 to the lower right of Alpha, but I could tell it was elongated showing a hint that it was double.

Jerry Hubbell
Lake of the Woods Observatory (MPC I24)
Locust Grove, VA

A 25 Million Year Old Announcement

Last week the supernova SN 2011dh in M 51 galaxy was near its maximum brightness around magnitude 12.3 and I was able to observe it with my 120mm refractor. The two famous interacting galaxies are very well placed in the sky these days. At the eyepiece, the main galaxy has a bright central region and a big, oval halo; the satellite galaxy has a nearly as bright core but a small and round halo. I needed 77x to spot the supernova in the southeast rim of the main galaxy, although the best view of it was at 149x. At this magnification the supernova was easily visible next to a fainter star. The sketch is a composite of both magnifications. It was remarkable that the supernova was visible even in late twilight conditions. SN 2011dh is a type IIb supernova that resulted from the explosion of a supergiant star with 18-22 solar masses, at a distance of 25 million light years. What a sight!

Sketch: 2HB graphite pencil on white paper, scanned and processed with Photoshop CS3
Object Name: The Whirlpool Galaxy (M51) and SN 2011dh
Object Type: Galaxy and supernova
Location: Asturias, Spain
Date: June 19th, 2011
Instrument: 120mm f/8,3 refractor + Hyperion 13mm (45x) & UWA 6.7mm (149x)
NELM: around 5.2, moderate light pollution

Regards,
Diego González

Stellar Explosion in The Whirlpool

Object : Supernova SN2011dh in Spiral Galaxy M51
Date : June 08, 2011
Time : 12:30-02:00 LST/ 07:30-09:00 UT
Location : Aguila, Arizona USA
Gear : Binoculars 25 x 100 and CPC1100 XLT with 25mm Plossl
Detector : Visual Sketch
Magnitude : 8.5 for M51 and 14.9 for SN2011dh(webtreatz.com)
Weather : Clear sky, no winds, low 70’s and quiet as a mouse!
Comments :
It’s interesting to ponder in awe, how a star that has turned into a supernova some 30 million light years distant is just NOW reaching our immediate universe, our light buckets our dilated pupils! This recently discovered supernova cataloged SN2011dh and found on May 31, 2011, might not last long. It’s believed to be diminishing in magnitude with a possible viewing window of some weeks or perhaps a couple of months. If you would like to get a glimpse of it, my suggestion is- don’t wait any longer!
With mounted binoculars it is quite easy to pick up M51 as it appears elongated and fuzzy. Some fidgetting of the eyeball around the circumference of the oculars and it’s companion NGC5195 emerges just as well. Both gravitationally interacting galaxies seem like puffs of smoke with their nucleus showing a hint of brightness.There are no noticeable spiral arms, no connecting bridge or other discernable features- not even the main attraction SN2011dh.
All this will change when I prepare the 11 inch SCT and aim it at the said subject with a 25mm Plossl. Yes, I had tried a 10mm and a 32mm but the 25mm gave me the best results. Peering down the eyepiece, Hazy blotches but distinct spiral structures are emanating from the soft glowing core of M51. Of the two major spiraling limbs, the one stretching all the way to NGC5195 or the one with the southeast orientation, will be the one sporting the newly discovered supernova. Four tiny specks of starlight ranging in magnitude from 13 -15 located on the southwest side of the Whirlpool and lined-up from East to West are clearly visible when using the cone receptors within the corners of your eyeballs. Averted vision here my friends, or you will miss the whole point. No pun intended! From recent photo submissions to various popular social websites, I made a mental note to see the whereabouts or location of SN2011dh. It’ll be nested on the spiral arm which embraces NGC5195 or the one facing the southeast coordinates.Much better seeing than explaining but after plotting their correct places among the broken segments of spiral arcs- one of the specks surely did fell where the photos had indicated it should be! I concluded my quest and my sketching for the night was done. Enjoy!

Dark and clear skies to all,

Juanchin 😀

The Whirlpool Welcomes a New Visitor

Object Name : M51, SN2011DH
Object Type : Face-on Galaxy, Supernova
Location : South Korea
Date : June 5th, 2011
Telescope : 15inch Discovery Dobsonian
Media : Black paper, White conte, White pastel

Nightwid (Cho Kang Uk)

Hi all, Supernova SN2011DH was easy to observing.
And I saw beautiful arms and bridge.. Because seeing is very good!