Ganymede Transit
Sketch by Lambert Spix
– 29.7.2008, 1:15 MEST
– 102/1000mm Refractor, 150x
– Pencil on white paper, scanned
M8 – The Lagoon Nebula
Sketch and Details by Kiminori Ikebe
M8 (NGC 6523) Sgr diffuse nebula
Difficulty level 1
The Lagoon Nebula
Date of observation: 1998/05/27 03:20
Transparency/seeing/sky darkness: 3/3/4
Instruments: 32cm Dobsonian with XL21 at 70x and OIII Filter
Width of field: 0.9 degree
Complex structures are visible. There is the open cluster NGC 6530 near the center, which can be seen clearly even with the OIII filter. The brighter part of the nebula is divided into three regions. A triangular-shaped nebulosity in the southwest is the brightest with 9 Sgr (mag 6.1) shining at the center. There is a small, somewhat fainter region south of 9 Sgr. The second brightest region extend from the center to the south, which contains the open cluster NGC 6530. Between the brightest and next brightest regions lies a clear winding dark lane like a large river. The “banks of the river” is bright and a magnificent sight. At the southern end a sharp protrusion like a horn is visible. Although it is faint, the outline is sharp. North of the brightest region lies the third brightest region. It extends from the east to the west and the eastern half is bright providing a fine sight. With a close examination you can detect a faint nebulosity east of NGC 6530. It is large and looks like a very faint mist. In 10×42 binoculars, there are two bright spots side by side in the east-west direction within a narrow triangle. There is a double involving 7 Sgr at the western end of the triangle. There is a star near the center of the western part of the bright region. This star is 9 Sgr and the bright nebulosity surrounding it is clearly seen. The eastern part is rather elongated with the same orientation with NGC 6520. The globular cluster NGC 6544 is clearly seen in the southeast.
Trumpler 32
Sketch and Details by Eric Graff
Object Name: Trumpler 32
Also Known As: C1814-133, Harvard 19
Object Type: Open Cluster
Constellation: Serpens (Cauda)
Right Ascension (2000.0): 18h 17.2m
Declination (2000.0): –13° 21′
Magnitude: 12.2
Size: 4′
Date/Time: 4 July 2008 • 06:45 to 07:10 UT
Location: Oakzanita Springs (4,010 ft. elevation), San Diego Co., California, USA
Telescope: Parks Astrolight EQ6 • 6″ f/6 Newtonian Reflector
Eyepiece/Magnification: Parks 20mm Gold Series Plössl + 2x Barlow • 90x • 35′ FoV
Filters: None
Conditions: Clear, calm, 62°F
Seeing: Pickering 4-5
Transparency: NELM 6.3; TLM 14.0
Approximately ½° northwest of M16 you might notice a small delicate patch of mist strewn with faint stars. This is the open cluster known as Trumpler 32. The cluster is elongated north to south and I count about two dozen stars superimposed on a haze of fainter, unresolved members. A curious dark lane separates the southern third of the cluster from the rest of the group.
M11 – The Wild Duck Cluster
Sketch and Details by Carlos Hernandez
I was able to observe one of my favorite open clusters M11 (NGC 6705) in Scutum on August 9, 2008 (5:00 U.T.). This magnificent open cluster appears as an explosion of jewels in space. This spectacular collection of stars has an estimated 2,900 members of which 500 are brighter than 14th magnitude. It lies at an estimated distance of between 220 to 250 million light years. I made the observation using my 9-inch (23-cm) F/13.5 Maksutov-Cassegrain at 78x.
A digital image made using Photoshop CS3.
Links:
http://www.hawastsoc.org/deepsky/sct/index.html
http://apod.nasa.gov/apod/ap030122.html
http://www.maa.clell.de/Messier/E/m011.html
Carlos
Partial Lunar Eclipse
Sketch and Details by Isabel Roblas
“Object type”: Moon
“Title of your sketch”: Partial eclipse of moon
“Your name”: Isabel Roblas
Partial eclipse of moon of August 16, 2008. Seville. Spain.
The drawing is of the image of the moon in a hollow that the clouds, sight left with the prismatic ones 10×50
(sorry my english)
Isabel
Seville, Spain
NGC 457: The Owl Cluster
Sketch and Details by Frank McCabe
At a distance of 9,300 light years (2850 parsecs) this youthful open cluster is about the same age as the Perseus Double Cluster – eight million years old. NGC 457 in Cassiopeiae is composed of nearly 100 stars brighter than magnitude 13 and many fainter members. The cluster has several names including the Owl cluster, the E.T. cluster, the Phi Cas. cluster and others. The two brightest stars here, Phi Cas. and HD7902 may not actually be members of this open cluster but rather foreground stars. These two stars form the bright eyes of the owl. Phi Cas. is a magnitude 5 yellow star and HD 7902 is a magnitude 7 bluish star. If the brighter member is a cluster star at 9,000 light years it would have a luminosity of 275,000 suns. The integrated visual magnitude of this cluster is about 6.4 and it is 16’ across. This object was discovered by William Herschel in 1787. It can easily be found 2° south-southwest of delta Cas. (R. A. 1h. 22’, Dec. +58° 2’).
Sketching
Date and Time: 8-11-2008, 5:20-6:40 UT
Scope: 10” f/5.7 Dobsonian. 13mm eyepiece 111x
8”x11” white recycled sketching paper, 4B soft charcoal pencil, HB hard charcoal pencil, blending stump, scanned and inverted, some star magnitude adjustment made at the time of scanning.
Seeing: Pickering 5/10
Transparency: Average 3/5
Nelm: 4.2
Frank McCabe
Hickson 68
Sketch and Details by Bill Ferris
Move mouse over sketch to see labels.
Hickson 68: Galaxy Cluster (Canes Venatici)
RA: 13h 53.5m / DEC: +40º 17′.0
Instrument: 18-inch Obsession
Here’s a fine galaxy cluster that adorns the spring sky. Hickson 68 resides in eastern Canes Venatici and is closer to the bright stars of Boötes than to Cor Caroli. My sketch presents a 199X view in the big Obsession and is dominated by NGC 5350. This 11.3 magnitude barred spiral is northernmost in the group and has the designation, Hickson 68C. Its stellar core is embedded within a 3′.3 by 2′.4 oval nebulosity that becomes gradually brighter toward the middle. The bright stellar pair immediately west of NGC 5350 are 6.5 magnitude HD 121197 and 10.5 magnitude PPM 53793. A skosh more than 4′ south of Hickson 68C, resides a pair of galaxies sharing the same patch of sky. NGC 5353 is Hickson 68A. It is the larger and, at 10.9 magnitude, brighter of the pair. Its 2′.7 by 1′.5 oval form is aligned northwest to southeast and features a stellar core. Hickson 68B (NGC 5354) lies an arcminute to the north. Just the bright inner core of this 11.3 magnitude gotham is seen. The 1′ circular patch of haze is anchored to the sky by a faintly stellar core. Two galaxies are stationed to the east of center in my drawing. NGC 5355 (Hickson 68D) stands about 5′ west of NGC 5350. This 1′.2 by 0′.7 galaxy shines at 13.1 magnitude and is aligned north-northeast to south-southwest. NGC 5358 is the most challenging member of Hickson 68. Hickson 68E is a 14.6 (B) magnitude galaxy. It appears 1′.5 by 0.5 in size and is arranged northwest to southeast. A close pair of 13th magnitude GSC stars simmer an arcminute to the southwest.
NGC 246
Sketch by Eiji Kato
Further information about this fascinating planetary nebula can be found here: The Internet Encyclopedia of Science: NGC 246 – The Skull Nebula.
The Great Red Spot
Sketch and Details by Carlos Hernandez
I made an observation of the Great Red Spot (GRS) and surrounding region (South Equatorial Belt (SEB)) on August 10, 2008 (04:30 U.T.). The amount of detail visible within and surrounding the Great Red Spot (GRS) was impressive. The core of the GRS was a dark salmon color (3-4/10) surrounded by a reddish pink to white color (5-7/10) over the rest of the GRS. The South Equatorial Belt (SEB) was a light brown to a greenish-brown color (3-4/10) with bright (7/10), undulating rifts over it’s northern half. The South Tropical Zone (STrZ) appeared bright with a dusky to dull (4-5/10) band appearing to connect to the southern border of the GRS. A dark (3/10) elongated condensation appeared within it following the GRS. An elongated, and bright (7/10) oval BA was noted within the dark (3/10) South Temperate Belt (STB). The center of the GRS was timed at 130.3 (L2, 128.4 L3).
A digital image produced in Photoshop CS3.
Carlos