To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

Pitatus (crater)

From Wikipedia, the free encyclopedia

Pitatus
Coordinates29°53′S 13°32′W / 29.88°S 13.53°W / -29.88; -13.53
Diameter100.63 km[1]
Depth0.9 km
Colongitude13° at sunrise
EponymPietro Pitati

Pitatus is an ancient lunar impact crater located at the southern edge of Mare Nubium. It was named after Italian astronomer Pietro Pitati by the IAU in 1935.[1] Joined to the northwest rim is the crater Hesiodus, and the two are joined by a narrow cleft. To the south lie the attached Wurzelbauer and Gauricus.

YouTube Encyclopedic

  • 1/1
    Views:
    378
  • Moon through telescope QHY5L-II

Transcription

Description

The complex wall of Pitatus is heavily worn, and has been encroached by lava flows. The rim is lowest to the north, where the lava almost joins the Mare Nubium. Near the middle is a low central peak that is offset to the northwest of center. This peak only rises to a height of 0.5 km.

Pitatus is a floor-fractured crater, meaning it was flooded from the interior by magma intrusion through cracks and openings. (See also Gassendi and Posidonius for similar features.) The flooded crater floor contains low hills in the east and a system of slender clefts named the Rimae Pitatus. The larger and more spectacular of these rilles follow the edges of the inner walls, especially in the northern and eastern halves. The floor also contains the faint traces of deposited ray markings.

Just to the north of Pitatus in the neighboring mare is the half-buried rim of Pitatus S, covered in the past when Mare Nubium was formed.

Pitatus is a crater of Nectarian age.[2]

Satellite craters

Pitatus and its satellite craters

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Pitatus.

Pitatus crater in the Lunar Atlas (1898) by Ladislaus Weinek. North on the photo is downward
Pitatus Latitude Longitude Diameter
A 31.4° S 13.2° W 7 km
B 32.3° S 10.4° W 16 km
C 28.4° S 12.4° W 12 km
D 30.9° S 12.0° W 10 km
E 28.9° S 10.1° W 6 km
G 29.8° S 11.4° W 18 km
H 30.5° S 15.7° W 15 km
J 26.5° S 13.5° W 5 km
K 30.4° S 8.9° W 6 km
L 29.1° S 8.6° W 5 km
M 32.1° S 11.0° W 14 km
N 31.2° S 10.9° W 21 km
P 31.0° S 10.9° W 16 km
Q 30.5° S 10.8° W 12 km
R 31.1° S 14.6° W 7 km
S 27.3° S 14.0° W 12 km
T 29.4° S 11.2° W 5 km
V 28.9° S 11.7° W 5 km
W 27.9° S 11.2° W 13 km
X 28.4° S 11.6° W 19 km
Z 28.3° S 10.3° W 25 km

References

  1. ^ a b "Pitatus (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^ The geologic history of the Moon. USGS Professional Paper 1348. By Don E. Wilhelms, John F. McCauley, and Newell J. Trask. U.S. Government Printing Office, Washington: 1987. Table 9-4.
This page was last edited on 26 April 2023, at 19:59
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.