Here is my sketch of Messier 77 (Seyfert Galaxy). It was done on January 19, 2007, with a 12″ Lightbridge. The seeing and transparency were both average. The medium I used was Graphite pencil.
Messier 77 is a beautiful face on spiral that lies is the midst of a small group of galaxies in the southern constellation of Cetus. It has the distinction of being one of the most distant of Messier’s famous non comet inventory at about 60 million light years away. This sprawling city of stars is fully 100,000 light years wide and appears to harbor a supermassive blackhole that is currently energizing an accretion disc of infalling dust and gas. Studies with the Chandra Observatory show a beam of X-Ray radiation that is aligned along an axis passing through the galaxy’s core. The presumed engine is the dynamo action of the accretion disc; hot plasmas race around the hole at close to the speed of light, creating magnetic fields that confine and eject matter along the rotation axes of the monsterous gravitational maw.
The Orion Nebula (M42, NGC 1976) is one of the most well known and observed nebulae in the heavens. This magnificent collection of gas and dust visible as the “middle star” of the sword of Orion measures 30 light years across and lies approximately 1,500 light-years away. The Orion Nebula represents a stellar nursery in which stars are formed from the accretion of hydrogen gas and dust into protoplanetary disks (or proplyds) as imaged by the Hubble Space Telescope (HST).
I made wide-field observation of the Orion Nebula on February 14, 2007 using an 8-inch (20 cm) F/9 Klevtsov-Cassegrain reflector (a catadioptric design employing a sub-aperture meniscus correcting lens combined with a Mangin mirror-lens secondary). The observation was made under very transparent (6/6) and steady (5-7/10) conditions. The core of the nebula appeared brilliant in the field containing the famous Trapezium. Fainter extensions were noted to project from the core, including elongated ones to the north and south. The rendering was initially made using graphite (6H to HB) on Bristol Board paper (smooth), scanned into Photoshop and reversed.
Carlos E. Hernandez
Here is a sketch of NGC 2261, the Hubble’s variable nebula.
Some informations :
– Telescope : Dobson Lukehurst 495/2032, Pentax XW 7 mm (x290), no filter.
– Date : 30/10/06, 04:00 UT.
– Place : Nailly, Yonne, France.
– Sky : not transparent (lim. magnitude about 5,0) but with very good seeing.
A draft was made during the observation, then I made two sketches : one with the stars, the other with the nebula (on a white paper and with a lead pencil). Then, I scanned the two sketches and saved negative pictures. The picture with the nebula was colored in a light green. And finally, I added the two images. The sketch is not perfect : the east side of the nebula was more luminous than the west side – it is not obvious in the sketch. But the color of the nebula seems (to me) well shown.
Here’s a link to a archived post on Astronomy Picture of the Day that discusses some of the fascinating aspects of Hubble’s variable nebula.
Markarian’s Chain of galaxies
Sketch was made on copy machine paper, A4 in size, with regular graphite pencil and blending stump. Conditions were good, transparency was excellent , limiting magnitude was 5.70 but seeing wasn’t that great. I used 8″ F6 dobson and 10.5mm Baader Hyperion Eyepiece. Magnification was 114x.
70 million light years away, the sprawling Virgo Cluster is home to perhaps thousands of galaxies. In fact the Virgo cluster, despite it’s great distance, subtends an angle of about five full degrees in our sky, making it ten times larger than the angle the Moon subtends. Markarian’s Chain, beautifully rendered by Vedran, includes M84, M86 and M88 along with a host of smaller elliptical, spiral and irregular galaxies. Studies indicate that seven of the galaxies in the Chain actually move together at the same relative velocity.
M16 Eagle nebula
This nebula was drawn with graphite pencils on
white paper and then inversed after scanning.
The main field stars (until about magnitude 11)
was printed with a charting software and the
fainter stars and nebula were added during the
observation. It took about an hour to lay all the
details on paper.
17.5-inch dobsonian, F/4.5, 74 &125x, OIII filter
used for the fainter parts; 15/august/2004,
22h00UT, good transparency (visual limit of 6.31
in UMi); from La Clapière in the french alps at
an elevation of 1650m.