A Monotone Scoop of Neopolitan Ice Cream

Schickard and Lehmann

Lunar craters Schickard and Lehmann
Sketch and Details by Jeremy Perez

It’s hard to get used to the fact that the moon plays misery on DSO observations two weeks out of every month. I can see that my biggest interest leans toward those dim patchy things, but given a little time exploring the moon, it still turns out to be very rewarding. So I took some time this bright moonlit evening to explore some likely craters listed in the Astronomical League’s Lunar 100.

Schickard is a large crater on the western limb of the almost full moon. There is an intersecting crater on the north end that looks about 20% as big.The southwest floor has a series of ridges or cracks that run northwest to southeast. There is also a half-circle of craters on the western floor. On the east side floor, a distinct white patch is visible.

After getting past the dazzling array of contrasting crater-wall shadows, I noticed to my surprise that the floor of the crater gave the appearance of a monotone scoop of Neopolitan ice cream. The north half and southeast tenth of the crater floor were darker than the rest of the floor. These three distinct shaded areas didn’t owe their differences to some lucky angle of light, as their boundaries ran roughly parallel to the angle of the sun. Also very noticeable was a rough jumble of terrain outside the crater along the west-southwest rim. It was tough to sketch that and make it look like it belonged to the local terrain without spending an eternity linking it to continuing terrain further west. So it is what it is.

Factoids:

According to the The Moon Observer’s Guide, Schickard is one of the Moon’s largest craters at 227 km in diameter. Its walls rise 2500 meters above the floor. Its southwestern floor has been noticeably disrupted by debris thrown from the Orientale impact over 1000 km to the west. This debris carved valleys and chains of craters along this part of the crater. Periods of lava flooding have given the crater floor a multi-toned appearance with darker sections in the northern and southeastern sections–the most striking example of this on the Moon’s face.

The crater intersecting the north side of Schickard is Lehmann Crater. Lehmann is 47 km wide (20.8% the width of Shickard–hahah!) with 800 m walls.

Subject Schickard and Lehmann Craters
Classification Lunar Craters
Position Southwest edge
Phase/Age 12 days old
Size* Schickard Crater: (dia. 227 km);
Lehmann Crater (dia. 47 km)
Date/Time January 22, 2005 – 9:15 PM (January 23, 2005 – 04:15 UT)
Observing Loc. Flagstaff, AZ – Home
Instrument Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)
Eyepieces/Mag. 10 mm + 2X Barlow (240X)
Conditions Clear, cool (34�F)
Seeing 4-5/10
Sources The Moon Observer’s Guide By Peter Grego
* Based on published data.

Jeremy Perez

International Year of Astronomy Mural

International Year of Astronomy Mural on U Tube and UNAWE

This mural kicked off on April 23rd and finished on Tuesday June 23rd.
I was invited to give a presentation to the children from 5th class,
followed up with some lunar and solar observing then an interview.

Sarah – Jayne Reid a friend and Arts Facilitator kindly got me involved
and it took off from there. Sarah – Jayne helped the children to express
their ideas on the wall. I did a presentation and some lunar and solar
observing with them.

Hopefully it speaks for itself
There is a short description on the U Tube site

Full version on here vimeo.com/5319106
the full version has an interview with Sarah – Jayne Reid at the end.


Deirdre Kelleghan

Outreach Coordinator IFAS
http://www.irishastronomy.org/
http://www.deirdrekelleghan.com/

The Lunar/Antares Occultation

Lunar/Antares occultation

The Lunar Occultation of Antares
Sketch and Details by Michael Rosolina

Hello,

I was fortunate to be able to view the occultation of the red supergiant Antares by the nearly full Moon as it rose on the evening of June 6th. The Moon was still sixteen hours from full which caused the lunar limb to have an odd, irregular appearance in places. Antares, “the Heart of the Scorpion” disappeared in an eyeblink behind the invisible dark edge of Luna before it ever reached the sunlit mountains and mares.

Antares means “the rival of Mars” in Greek, but it was easily overwhelmed by Selene that night.

This field sketch was done with white and gray Conte’ crayon, black charcoal pencil, and orange color pencil on black paper.

The Moon and Antares
Occultation
0226 UT 7 June 2009

Michael Rosolina
Friars Hill, WV USA

Craters Babbage, Harpalus, and South

Babbage, Harpalus, and South

Lunar craters Babbage, Harpalus, and Short
Sketch and Details by Frank McCabe

On this fine evening the large (144 km.), ancient (Pre-Nectarian), walled plain crater Babbage with its sizable central crater Babbage A (32 km.) formed a focal point for the eye along the terminator. The morning sunlight was bouncing off what remains of the old battered rim of Babbage and the smooth walls of crater A. Sharing an eastern rubbly wall with Babbage is another 4 billion year old wall plain crater or what remains of it called South (108 km.). This one is on the beach of Mare Frigoris. Judging from the shape of the wall between Babbage and South, the latter is the younger impact feature. Resting within the Sea of Cold is Copernican period crater Harpalus (41 km.), its pristine appearance betraying its youth. Harpalus crater was made famous in the Classic Science fiction film from August of 1950 titled Destination Moon. This crater was the rocket landing site for the astronauts in this George Pal motion picture which won awards for special effects.

Sketching:

For this sketch I used: a small 7”x 7” piece of black Strathmore 400 Artagain paper, white and black Conte’
pastel pencils. Brightness and contrast slightly increased after scanning
Telescope: 10 inch f/ 5.7 Dobsonian with 6mm eyepiece (241x)
Date: 6-5-2009 2:15-2:45 UT
Temperature: 14°C (57°F)
Clear, calm
Seeing: Antoniadi III
Colongitude 54.6 degrees
Lunation 11.6 days
Illumination 93%

Oak Forest, Illinois

Frank McCabe

Sunrise on the Moon: Gates of Mare Imbrium and Ptolemaeus

Gates of Imbrium and Ptolemaeus

Gates of Mare Imbrium and Ptolemaeus
Sketch and Details by Leonor Ana Hernández

Object name: oriental region of Mare Imbrium and Ptolemaeus crater
Object Type: Lunar Crater and Maria

The last sunday 31th we could point the telescope to the moon in a beautiful place called “Las Inviernas” Guadalajara, Spain. The moon was just on the seventh day and stood high on the beautiful background of blue sky. I looked through the telescope and I was fascinated by the beauty of the image it shows: “it was dawning at the gates of the east of Mare Imbrium”…

Leonor Ana

Ancient But Well Preserved

Petavius

The Lunar crater Petavius

Sketch and Details by Frank McCabe

Crater Petavius

I have waited more than 2 years for conditions to be just right for re-sketching this magnificent crater. I got set up to observe under what looked to be hopeless circumstances. Although we have been under heavy cloud cover all week, the weather service forecasted clearing and as an added bonus my nearest “Clear Sky Chart” predicted the best possible seeing conditions until midnight. Both of these came true! Alas, heaven on earth.

Petavius crater (180 km.) is one of the best known and remarkable impact features on the lunar surface. It is a walled plain and floor fractured crater with impressive multiple central peaks (1.7 km), beautiful wall terraces, mare patches, volcanic ash regions, a raised floor and remarkable looking ramparts. In addition there is a special feature of this crater called Rimae Petavius. All three parts of this rille system could be seen clearly under the excellent seeing conditions that persisted during the entire observation. Connected to Petavius to the west is crater Wrottesley (57 km). South of Wrottesley the double rim of crater Petavius can be seen. There was so much detail visible in this area I could not hope to capture but a fraction of it.
Although Petavius is 3.8 billion years old it looks younger, stately and better preserved.

Sketching:

For this sketch I used: black Strathmore 400 Artagain paper, white and black Conte’
pastel pencils and a hard blending stump.
Telescope: 10 inch f/ 5.7 Dobsonian with 6mm (241x) and 4 mm (362x) eyepieces
Date: 5-29-2009 1:20-3:15 UT
Temperature: 13°C (55°F)
Clear, calm
Seeing: Antoniadi mostly I, [ the collapsed lava tube down the center of Vallis Alps would have been easy under the seeing conditions of this night ]
Colongitude 329.5 degrees
Lunation 4.5 days
Illumination 28%
Moon was at Perigee just 3 days ago

Frank McCabe

Immersed in Darkness

Copernicus

Lunar crater Copernicus
Sketch and Details by Krzysztof Jastrzebski (Jarzbi)

Hi.
I’m sending the charcoal sketch of the crater Copernicus immersed in darkness.

Object Name:
* Object Type (Moon: Copernicus crater)
* Location (Skawina City in Poland)
* Date (03 May 2009, 20:00 UTC)
* Equipment: Synta 8” Dob, Eyepice SP10 mm.

Greetings,
Krzysztof Jastrzebski (Jarzbi)