Some formations of interest: Wargentin is the largest crater (84 km) filled to the rim (by lava?). Schiller is strangely elongated crater (179x71 km), it must have been created by and extremely oblique impact.
Wargentin is an unusual lunar impact crater which has been filled to its rim by a basaltic lava flow, forming a raised plateau. When the lava flow occurred, it erupted from within the crater walls and proceeded to accumulate until overrunning the lowest portion of the rim. Some blockage then prevented the lava flow from returning to equilibrium.
We can also be used as a 20 Dec 2020 Inghirami Crater: Wargentin, Nasmyth, Phocylides 2005.0422 16:41 UT Age 13.3 days. 10-inf/6+4X+ToLK:am, 35% resized. Image T061:. Other examples that deserve observation are the "ghost-crater" Lamont, and the the completely flooded crater Wargentin. moon_clavius.jpg (24580 bytes) Bookcover of Wargentin (Crater). Omni badge Wargentin (Crater) Physics, astronomy · Betascript Publishing (2011-03-30) - ISBN-13: 978-613-3-48376-7.
Use features like bookmarks, note taking and highlighting while reading The Complete (For Now) Wargentin Crater Chronicles. Wargentin crater 4172 h1 h2.jpg 1,800 × 1,800; 496 KB Wargentin satellite craters map 1.jpg 600 × 296; 13 KB Wargentin satellite craters map.jpg 1,633 × 714; 71 KB Localització de Wargentin (cantó superior esquerre de la imatge) El cràter es troba farcit de lava fosca fins a dalt, formant-se així un altiplà circular de 300 m d'altitud, sent un dels pocs cràters de la Lluna el sòl de la qual s'ha inundat per sobre de la planícia circumdant. Wargentin je lávou zaplavený kráter nacházející se v jihozápadní části přivrácené strany Měsíce a díky tomu je pozorovatelný ze Země se značným zkreslením. Má průměr 84 km a je největší z řídce se vyskytujících kráterů zaplněných až po okraj ztuhlou lávou. [1] A beautiful capture of this southwest crater group. On the floor of Schickard you nicely captured the two large dark lava flow out regions. On the floor of crater Wargentin you captured the shadow cast by the frozen lava ridge across the crater floor that is invisible at high sun.
Nasmyth. Schickard. Nöggerath.
The vast majority of craters have floors that are lower than the surounding plains! This image was captured as the Sun was rising, bringing out the wrinkle ridges that cross this "mini mare". A number of craterlets in the 1-2 km range can be seen on Wargentin's "floor". The crisp crater in the top left hand corner is Wargentin A (21 km).
ghost crater buried by 43 Wargentin. A crater filled to the rim with lava or ejecta. 49.6S. 60.2W.
Full Moon Atlas: Sector G-1 Schickard-Wargentin Frontier/ Southwestern Limb. The Moon's rugged southwestern frontier, dominated by wide Crater Schickard (227 km diameter; right of center in the photograph), with meandering Lacus Excellentiae visible towards the upper right corner. A trio of large craters — Wargentin, Nasmyth and Phocylides — are clustered south of Schickard.
Wargentin is a crater that has filled up with lava. The floor of this crater is 1400 feet above the surrounding area. Moon's age: 12 days 4 hours 59 minutes.
When the lava flow occurred, it erupted from within the crater walls and proceeded to accumulate until overrunning the lowest portion of the rim. There are times that I pursued a picture of Wargentin , and although this has not been to my liking due to bad seeing was the one I got today.WargentinCraters of the genuine type Wargentin are few and far between on the lunar surface .She has the look of money and should have been filled with lav
Detta är en lista över månens kratrar.Den stora majoriteten av dessa är nedslagskratrar.Kratrarnas nomenklatur styrs av Internationella astronomiska unionen (IAU) och denna lista inkluderar endast objekt som är officiellt erkända av dem.
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Má průměr 84 km a je největší z řídce se vyskytujících kráterů zaplněných až po okraj ztuhlou lávou. [1] A beautiful capture of this southwest crater group. On the floor of Schickard you nicely captured the two large dark lava flow out regions. On the floor of crater Wargentin you captured the shadow cast by the frozen lava ridge across the crater floor that is invisible at high sun. Very impressive sketching.
Nomenclature has been added to aid identification of the craters under discussion in this report. The ‘elevated plateau’ appearance of Wargentin is quite marked on this image. Annotated image of the Schickard group of craters to show nomenclature.
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• Wargentin: On Monday night, check out the crater Wargentin (Field Map of the Moon grid SW/P4). This is one of the more unusual craters on the Moon. When you catch Wargentin in the right light, it has a fascinating story to tell. There is an almost inviolable rule that crater floors must be lower than their surrounding terrain. Not so with
The vast majority of craters have floors that are lower than the surounding plains! The Complete (For Now) Wargentin Crater Chronicles - Kindle edition by Shimbo, Fara.
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Some formations of interest: Wargentin is the largest crater (84 km) filled to the rim (by lava?). Schiller is strangely elongated crater (179x71 km), it must have been created by and extremely oblique impact.
Han var också initiativtagare till svensk befolknings statistik och tabellverkets upphovsman. Pehr Wilhelm Wargentin 1717-1783) 151 _ _ ‡a Wargentin 4xx's: Alternate Name Forms (9) 451 _ _ ‡a Basedow ‡9 g:Landkreis Mecklenburgische Seenplatte ‡x Wüstung Wargentin Perhaps the oldest theory of the volcanic origin of the lunar craters was that The peculiar plateau of Wargentin and Phoclydes b, * “General Astronomy”: 1889 . Attached to the northern rim is the lesser crater Lehmann, and to the northeast is the even smaller Drebbel. Southwest of Schickard is Wargentin, a lava-flooded why lunar craters were circular, an obvious difficulty for the impact hypothe- sis as it was Wargentin is another example of this rare type of crater. The most eBook Kindle. The Complete (For Now) Wargentin Crater Chronicles (English Edition) eBook Kindle. R$20,83.