Theophilus (crater)

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Template:Short description Template:Infobox Lunar crater

File:Theophilus Si Barbero Zetta Ferruggia.jpg
Theophilus in a selenochromatic image; more infos here: https://www.gawh.it/main/selenocromatica
File:Theophilus crater AS16-113-18295HR.jpg
Oblique view of Theophilus from Apollo 16 as the lunar module Orion approached its landing point about 450 km to the west
File:Theophilus crater 3078 med.jpg
Oblique view of Theophilus from Lunar Orbiter 3
Oblique view of the central part of Theophilus from Apollo 16 Panoramic Camera

Theophilus is a prominent lunar impact crater that lies between Sinus Asperitatis in the north and Mare Nectaris to the southeast. It partially intrudes into the comparably sized crater Cyrillus to the southwest. To the east is the smaller crater Mädler and further to the south-southeast is Beaumont.<ref>Template:Cite web</ref> It was named after the 4th-century Coptic Pope Theophilus I of Alexandria.<ref name="a">Autostar Suite Astronomer Edition. CD-ROM. Meade, April 2006.</ref>

Theophilus, Cyrillus and Catharina form a prominent group of large craters visible on the terminator 5 days after the new moon.

Description

The rim of Theophilus has a wide, terraced inner surface that shows indications of landslips. It is 4200 metres deep with massive walls and has broken into a second formation, Cyrillus.<ref>Moore, Patrick (2001). On the Moon. Sterling Publishing Co.. Template:ISBN.</ref> It was created during the Eratosthenian period, from 3.2 to 1.1 billion years ago.<ref>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 12.2.</ref> It has an imposing central mountain, 1,400 metres high, with four summits.<ref name="a"/>

The floor of the crater is relatively flat, and it has a large, triple-peaked central mountain that climbs to a height of about 2 kilometres above the floor. The western peak is designated Psi (ψ), the eastern Phi (φ), and the northern peak is Alpha (α) Theophilus. The western slopes of this ridge are wider and more irregular, whereas the peaks descend more sharply to the floor on the northern and western faces.<ref>Template:Cite book</ref>

The Apollo 16 mission collected several pieces of basalt that are believed to be ejecta from the formation of Theophilus.<ref>Template:Cite web</ref>

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 Theophilus.<ref>Template:Cite book</ref>

Theophilus Latitude Longitude Diameter
B 10.5° S 25.2° E 8 km
E 6.8° S 24.0° E 21 km
F 8.0° S 26.0° E 13 km
G 7.2° S 25.7° E 19 km
K 12.5° S 26.3° E 6 km
W 7.8° S 28.6° E 4 km

References

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