Rhaeticus (crater)

Rhaeticus is a lunar impact crater that lies astride the equator of the Moon, on the southeast edge of the Sinus Medii. To the north-northwest is the crater Triesnecker, and due south can be found the worn remnant of the walled plain Hipparchus. The crater was named after Austrian astronomer Georg Joachim Rheticus.[1][2]

Rhaeticus
Coordinates0.0°N 4.9°E / 0.0; 4.9
Diameter43 × 49 km
Depth1.6 km
Colongitude254° at sunrise
EponymGeorg Joachim Rheticus
Oblique view of Rhaeticus facing north, and showing Rhaeticus A crater in upper right. From Apollo 12
Oblique view of Rhaeticus facing west at low sun angle. From Apollo 10

Description

The outer wall of Rhaeticus is heavily disintegrated, with rifts and notches in the northeast. The wall is most intact along the eastern face, while in the northwest it is little more than a low rise in the surface. There is also a low cut in the south-southeast wall. The overall shape of the rim is that of a rough hexagon that is slightly elongated in the north-south direction. The interior has been resurfaced by lava, and only a few low rises remain in the surface. Beginning at the crest of the eastern wall is a chain of craterlets that continue to the east-northeast for about a crater diameter.[3]

Running southwest from Rhaeticus to the crater Réaumur is a long rille, which is difficult to make out near Rhaeticus because of the group of mountains at that crater's southwest. The crater itself is 43 kilometers wide at one diameter and 49 kilometers long at another. It is from the Pre-Imbrian period, which lasted from 4.55 to 3.85 billion years ago.[2]

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 Rhaeticus.[4]

Rhaeticus and its satellite craters map
Rhaeticus Latitude Longitude Diameter
A 1.8° N 5.2° E 11 km
B 1.7° N 6.8° E 6 km
D 0.9° N 6.2° E 7 km
E 0.1° S 6.0° E 5 km
F 0.1° S 6.5° E 18 km
G 1.0° N 6.4° E 6 km
H 1.0° S 5.4° E 6 km
J 0.7° S 3.2° E 4 km
L 0.2° N 3.6° E 14 km
M 1.0° N 3.8° E 7 km
N 1.2° N 4.2° E 12 km
gollark: Is it going to just send a description of what to draw? In that case, lots of overhead and problems porting to different environments since for example each GUI framework will end up needing its own module communication layer.
gollark: For one thing, is a module just going to be allowed somehow to draw on the region of the screen it's meant to be set up for?
gollark: Yes it is.
gollark: These "modules", they could communicate over some sort of unified IPC framework with some standard format or whatever, but probably each language/framework would end up having to implement its own method of rendering what gets sent over.
gollark: They can just send JSON-serialized messages or whatever, it's just slower than using one binary.

References

  1. "Rhaeticus (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. Autostar Suite Astronomer Edition. CD-ROM. Meade, April 2006.
  3. Wlasuk, Peter T. (2000). Observing the Moon. Springer. ISBN 1-85233-193-3.
  4. Bussey, B.; Spudis, P. (2004). The Clementine Atlas of the Moon. New York: Cambridge University Press. ISBN 0-521-81528-2.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.