Mars on the Evening of June 10, 2010

Mars - June 10, 2010
Mars – June 10, 2010
By Carlos E. Hernandez

I made an observation of Mars on June 10, 2010. Although the angular diameter was less than six arc-seconds (5.7” to be exact) I was able to detect albedo features when the seeing steadied for moments at a time.

Date (U.T.): June 10, 2010
Time (U.T.): 01:00-01:15
CM: 276.2*W-279.9*W
Ls 102.4*, De 23.1*, Ds 24.2*
p 90%, 5.7” (Diameter)
Instrument: 9-inch (23-cm) F/13.5 Maksutov-Cassegrain
Magnification: 295x and 388x
Filters (Wratten): 30 (Magenta) and 38A (Blue)
Seeing (1-10): 5-6, Antoniadi (I-V): III
Transparency (1-6): 4

Notes:
01:00 U.T. (CM 276.2*W, Wratten 30 (Magenta): The North Polar Cap (NPC) appears small and brilliant (10/10) with a dark (3/10) collar surrounding it. Lemuria and Cecropia appeared dark to dusky (3-4/10) and mottled. Utopia and Casius appeared dark to dusky (3-4/10; Casius appearing as a dark (3/10) “spike-like” albedo feature). Elyisum appeared bright to very bright (7-8/10) with a very bright (8/10) cloud over it. The Hyblaeus Extension appeared dark to dusky (3-4/10) following Elysium. Mare Cimmerium appeared dusky to dull (4-5/10) over the south-preceding limb. Electris and Eridania appeared shaded (6/10). Mare Tyrrhenum and Syrtis Minor appeared dark to dusky (3-4/10) on the central meridian (CM). Syrtis Major appeared as dark to dusky (3-4/10), mottled, wedge-shaped albedo feature following the CM. Hellas appeared very bright (8/10) with a cloud over it. Zephyria, Aeolis, Aethiopis, Aetheria, Isidis Regio, Neith Regio, Meroe Insula, and Aeria appeared bright (7/10). Extremely bright (9/10) evening limb haze (ELH), south polar limb haze (SPLH), and morning limb haze (MLH) were noted as well.

A digital image produced in Pixelmator.

Carlos E. Hernandez
Pembroke Pines, Broward County, Florida

McNaught’s Best View Yet


Comet C/2009 R1 (McNaught) – June 15, 2010
By Juanchin

Object : Comet C/2009 R1 McNaught
Date : June 15, 2010
Time : 03:00 LST / 10:00 UT
Location : Wickenburg Arizona USA
Instrument : Orion 25 x 100 FOV 2.5 Deg.
Magnitude : ~ 6.5
Weather : Dark and clear sky, slightly gusty winds, cool upper 70’s with a chance of Sagittarids! : )

Comments :
A major prediction for this comet was that perhaps being a first timer to swing around our Sun, it might have a dramatic outburst display like that of Comet Holmes.
Last week of June the 9th, I sketched McNaught while it passed by M34, but the Moon was the factor that was robbing me of some extra details. Details that tonight
were more noticeable. The ionic tail is longer, I’d say at least over 1.5 Degrees. A fine thin tail stretching subtlely into a North-Northwest direction. Also, what I believed was
the dust tail, a spur emanating from the coma and shooting towards the West was visible. It kind of pointed towards the bright yellow star of Delta Persei.
The coma itself showed its greenish tint along with a very bright white core. I’m not very precise on determining the size of the coma but I’d say it was in the vicinity of 10 arcminutes.(Someone can help me here, will appreciate) ; ) I noticed the comet had shifted during the course of about 1 hour. A star North of the comet and grazing the tail was now on the the Southwest side and embedded close to the dust tail. By a wild guess again, this comet had traveled almost its own coma diameter in that 1 hour time lapse.

This will be my last chase for comet McNaught, twilight starts creeping very fast soon after 11:00 UT. It hinders any chance to see the comet rise higher and the dawn light starts washing everything away. As the days progress the comet will be lower and lower into the horizon and finally out of sight. I enjoyed every bit of observation and I hope there are more of you out there who did the same and sketched it.

Wishing all clear and dark skies,

Juanchin

P.S. I only saw about 3 Sagittarids that night, very bright with short trains !!!

Comet 8P/Tuttle

Comet 8P/Tuttle
Comet 8P/Tuttle
By Per-Jonny Bremseth

Hey!

I send you comet 8P/ Tuttle “mother of the Ursids”. The comet was not so bright, but has a famous history (info on my sketch). I could see a brighter, soft glow in the central part , but the outer part was diffuse and did not see a limit of the outer coma. This sketch was made with crayons on black paper only.

The observation location : near Trondheim city, Norway.
Thank you very much for posting my sketches!!

From Per-Jonny Bremseth.

Comet C/2009 R1 (McNaught) – June 11, 2010

C/2009 R1 (McNaught)
C/2009 R1 (McNaught)
By Michael Rosolina

Hi,

This comet, a new visitor from the far outer reaches of our solar system, is currently visible to the northeast in the early morning skies. It has been brightening rapidly as it approaches the Sun, but this proximity to the Sun means that an observer has only a short time to see the comet before it disappears in the skyglow of morning twilight.

Another result of solar proximity is the comet’s tail. R1 McNaught has a long gas tail (at least 1° in length) and a short, stubby dust tail which have been visible in images. In this sketched observation, I was able to visually detect part of the gas tail, which is pushed straight away from the Sun by the pressure of the solar wind.

The sketch was done in the field just at the onset of twilight with a 2B pencil and stump on white sketch paper and inverted digitally. Good luck with your own comet chasing!

Michael Rosolina

C/2009 R1 (McNaught)
Comet
Friars Hill, WV USA
0820-0830 UT 11 June 2010

C/2009 R1 (McNaught) Blazes Near M34

McNaught
C/2009 R1 (McNaught) and Messier 34
By Juanchin

Object: C/2009 R1 McNaught
Date: June 09 2010
Time: 02:15 – 03:00 Local / 0715 – 1000 UT
Location: Wickenburg Arizona USA, at the foothills of Vulture Peak trailheads.
Equipment: Binoculars 12 x 60 Oberwerk and 25 x 100 Orion Giant view
Magnitude: ~7.5
Weather: Clear sky, calm winds, noctilucent clouds to the East but not in the way. high 70’s in this part of town!

Comments:
Greetings everyone! I sound like a stranger to this site but I haven’t had a chance to devote some time to one of my favorite doings. We’ll here you have it, I had read weeks prior that C/2009 R1 McNaught was going to become a visible comet to the unaided eye. Since that’s all it takes to get me excited, I decided to give it a try and start chasing this bad boy. I didn’t want to loose the opportunity like I did with the McNaught of 2007. (remember that one?)

Starting and staring visually, I couldn’t detect the comet when it drifted into view above the mountainous horizon.At about 15 to 20 degrees from the horizon, using the 12 x 60’s I readily spotted and would say that it sported a magnitude of 7.5 or so. Sort of hard to see at that brightness and altitude without optical aid. I was able to frame the comet with the star cluster M34 in the 5 degree FOV given by the binoculars. A fuzzy ball with no trace of a tail but that would change. I mounted the 25 x 100’s and like my kids would say nowadays- O.M.G !!! (Oh My God!)

I still had that wide vista that included both the comet and the star cluster, though a little tight in the view. Something that I have a hard time to detect is the aqua bluish glow given off by comets but here it was, pale but noticeable. With a little averted vision and the trick of swaying the parallelogram mount slightly, the ionic tail was unequivocally present. I was able to perceive it as being maybe about 1 degree long and stretching outward to a Northeasterly direction.

I decided to include a set of aligned stars outside the FOV to show how far I was able to detect the tail, it probably stretched longer. The Moon!, Oh that slice of cheese can sure ruin a good dark nite. I had to wrap everything up after the waning crescent ruined the view. The following days should prove to get better for observing but this was my only chance for me. Hopefully I will see future sketches posted here on ASOD to see what you all have to show us from this comet.

Juanchin

A Moon with a View

Saturn
Saturn – Large Sketch from Observation Through the Telescope With Artists Conception Below
By Mark Seibold

From Sandy Oregon, 30 miles east of Portland, at the home driveway – Saturn Observed February 28 ~ March 2 Through 10.1″ Newtonian- Large Pastel Sketch produced:

I observed Saturn through my 10.1″ Newtonian at medium to high power magnification (120X ~ 240X) on several evenings last week, in effort to see some detail in the rings and surface cloud banding. Seeing was medium to marginal at times through the evenings. Using Sol Robbins template and other images from the web to accurately proportion the rings, I rendered this 19” X 25” pastel impression showing about what is seen in a good medium telescope if one stands back say 25 feet from the full image on a standard computer screen. Saturn’s disc was sketched at 7 ¾” at the equator. The Cassini division was easily visible and the crepe ring only hinted at high magnification at 240x through a 5mm Super Plossl eyepiece through my 10.1″ f/4.5 Newtonian-Dobsonian telescope with average seeing conditions at times with glimpses through steady atmosphere.

The foreground was quickly added from imagination for depth and drama as a final touch, which seems to captivate a view from one of Saturn’s moons, possibly Titan with a suggestion to an ocean-scape.

The sketch was photographed with a Sigma 35mm DSLR under white balanced studio lights.

Jupiter – May 26, 2010

Jupiter
Jupiter – May 26, 2010
By Michael Rosolina

Hello,

I was happy to see Per-Johnny’s historical sketch of Jupiter and sorry that the King is too low for him to make a current observation. Veteran Jupiter observers report that the South Equatorial Belt (SEB) follows a cycle of disappearance and reappearance over the years.

I was fortunate to get an opportunity to see Jupiter during the present cycle of disappearance. The SEB isn’t completely gone–the northern component was faintly visible. Some say that the SEB doesn’t really go away, but rather is covered by the bright zonal clouds bordering it, but no one knows for sure.

What is certain is that Jupiter looks very different without the symmetry of the northern and southern belts. Hopefully, all who wish to will get a chance to see this visual phenomenon.

The sketch was done in the field with HB and 2B pencils on white copy paper. Other notes are with the sketch.

Best to all,

Michael Rosolina

Jupiter
Planet
Friars Hill, WV USA
26 May 2010 0945-1000 UT

Venus – May 23, 2010

Venus
Venus – May 23, 2010
By Aleksander Cieśla (Wimmer)

Hello.
I want to present my latest sketch of the planet Venus.

Object: Venus
Scope: Schmidt-Cassegrain 5″ with SW SWA58 9mm (also with barlow x1,6)
Filter: #80A Blue
Date & time: May 23th, 2010. 9:10 PM
Place: Wrocław, Poland
Weather: Good. Seeing 3/5. Transparency 3/5
Technique: Graphite pencil.
Tooling: GIMP 2
Observer: Aleksander Cieśla (Wimmer)

Jupiter Has Lost a Stripe

Daylight Jupiter
Jupiter – May 23, 2010
By Jef De Wit

Everybody knows that even in a small telescope you can see on Jupiter two brown belts. However when you turn your telescope on the planet now, you will see only one stripe!

The South Equatorial Belt (SEB), twice as wide as Earth and more than twenty times as long, is not actually gone, but may be just hiding underneath some higher white clouds. The last time this happened was in 1993.

When Jupiter is visible from my garden, the Sun is already high up in the sky. It took me 15 minutes to find the planet. Searching an object (except the Sun, the Moon and Venus) with a Dobson in broad daylight isn’t an easy job! Once in the eyepiece I could even see Jupiter easily in the finderscope (9×50).

Jupiter in daylight seems like a ghost. You have the impression to look through the planet. The North Equatorial Belt (NEB) was easy to see. But I was never so happy I couldn’t find something (this doesn’t happen fast in astronomy!). The SEB was nowhere. I guess the thin line is the northern border of the SEB.

Some details are not like actual photos of Jupiter. I saw the South Polar Region (SPR) brighter than the region just north of it. The north side of Jupiter looked as white as the Equatorial Zone (EZ), but in reality it is much darker.

Information: Science@NASA

Clear skies
Jef De Wit

Object Name: Jupiter
Object Type: planet
Location: Hove, Belgium (51°09’ north lat. 4°28’ east long.)
Date and time: 23 May 2010 7.00-7.30 UT
Equipment: Orion Optics UK 12” Dobson
Eyepiece: 7mm Nagler T6 (magnification 171x)
NELM: daylight
Planet information: diam. 36.7″, mag -2.2, alt. 37°
Medium: pastel pencils, cotton swap, blending stump, blue printing paper, scanned (with some adjustments), labels were added with Paint

Receding Mars – May 22, 2010

Mars - May 22, 2010
Mars – May 22, 2010
By Charles Galdies

Mars
Planet
Malta 35:52N; 14:26E; http://znith-observatory.blogspot.com
22 May 2010, 19:32 UT
Media (coloured pencils, white paper, scanning software, image processing)
200mm SCT f/10, 422x, seeing 4/10, trans 3/5

The style of this sketch portrays the feeling of ‘distancing’ from the planet Mars, shown as a small globe against a larger, black background.

Mars’ apparent diameter is now reduced to around 6″, which is far from a maximum of 14″ I have viewed and sketched last January. Still, 5 minutes of observation time in not so ideal atmospheric conditions (lots of air turbulence) and bright moonlight were enough to detect the main albedo features on the surface of Mars, currently residing in the constellation of Leo.

I didn’t think it worthwhile to use colour filters due to the limited seeing conditions. However a light blue filter could have slightly enhanced the visibility of the features.

The much reduced north polar cap was seen as tiny bright patch adjacent to Niliacus Lacus. Underneath, the prominent Mare erythraeum was also visible.

No other subtle features were detected along the edge of M. erythraeum next to Chryse. Tharsis appeared bright.

Charles Galdies