Tycho (crater)
Encyclopedia : T : TY : TYC : Tycho (crater)
| Crater characteristics | |
|---|---|
| Selenographic coordinates>Coordinates | |
| Diameter | 85 km |
| Crater depth>Depth | 4.8 km |
| Selenographic colongitude>Colongitude | 12° at sunrise |
| Eponym | Tycho Brahe |
Tycho is a relatively young crater, with an estimated age of 108 million years, as estimated from samples of the crater rays recovered during the Apollo 17 mission. The crater is sharply defined and free of the wear that affects older craters. The interior has a high albedo that is prominent when the sun is overhead, and the crater is surrounded by a distinctive ray system forming long spokes that reach as long as 1,500 kilometers. Sections of these rays can be observed even when Tycho is only illuminated by earthlight.
The ramparts beyond the rim have a lower albedo than the interior for a distance of over a hundred kilometers, and are free of the ray markings that lie beyond. This darker rim may have been formed from minerals excavated during the impact.
Its inner wall is slumped and d, sloping down to a rough but nearly flat floor exhibiting small, knobby domes. The floor displays signs of past volcanism, most likely from rock melt caused by the impact. Detailed photographs of the floor show that it is covered in a cross-crossing array of cracks and small hills. The central peaks rise 1.6 kilometers above the floor, and a lesser peak stands just to the northeast of the primary massif.
Infrared observations of the lunar surface during an eclipse have demonstrated that Tycho cools at a slower rate than other parts of the surface, making the crater a "hot spot". This effect is caused by the difference in materials that cover the crater.
The rim of this crater was chosen as the target of the Surveyor 7 mission. The robotic spacecraft safely touched down north of the crater in January, 1968. The craft performed chemical measurements of the surface, finding a composition different from the maria. From this one of the main components of the highlands was theorized to be anorthosite, an aluminium-rich mineral. The crater was also imaged in great detail by the Orbiter V.
From the 1950s through the 1990s, NASA aerodynamicist Dean Chapman and others advanced the "lunar origin" theory of tektites. Chapman used complex orbital computer models and extensive wind tunnel tests to support the theory that the so-called Australasian tektites originated from the Rosse ejecta ray of Tycho. Until the Rosse ray is sampled, a lunar origin for these tektites cannot be ruled out.
This crater was drawn on lunar maps as early as 1645, when Antonius Maria Schyrleus de Rheita depicted the bright ray system.
The Tycho crater figures prominiently in the film and book , in which it is the location of a mysterious alien monolith which "appears to have been deliberately buried."
It also serves as the location of "Tycho City" in ; a lunar metropolis by the 24th century.
Satellite craters
By convention these features are identified on Lunar maps by placing the letter on the side of the crater mid-point that is closest to Tycho crater.
| Tycho | Latitude | Longitude | Diameter |
|---|---|---|---|
| A | 39.9° S | 12.0° W | 31 km |
| B | 43.9° S | 13.9° W | 13 km |
| C | 44.3° S | 13.7° W | 7 km |
| D | 45.6° S | 14.0° W | 27 km |
| E | 42.2° S | 13.5° W | 14 km |
| F | 40.9° S | 13.1° W | 16 km |
| H | 45.2° S | 15.8° W | 8 km |
| J | 42.5° S | 15.3° W | 11 km |
| K | 45.1° S | 14.3° W | 6 km |
| P | 45.3° S | 13.0° W | 8 km |
| Q | 42.5° S | 15.9° W | 21 km |
| R | 41.8° S | 13.6° W | 5 km |
| S | 43.4° S | 16.1° W | 3 km |
| T | 41.2° S | 12.5° W | 14 km |
| U | 41.0° S | 13.8° W | 19 km |
| V | 41.7° S | 15.3° W | 4 km |
| W | 43.2° S | 15.3° W | 19 km |
| X | 43.8° S | 15.2° W | 13 km |
| Y | 44.1° S | 15.8° W | 19 km |
| Z | 43.1° S | 16.2° W | 24 km |
References
- See the reference table for the general listing of literature and web sites that were used in the compilation of this page.
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