Spook (crater)

Spook

Apollo 16 image, with Flag left of center and Spook right of center. Buster is the small crater north of Spook.
Coordinates 8°59′S 15°29′E / 8.98°S 15.48°E / -8.98; 15.48Coordinates: 8°59′S 15°29′E / 8.98°S 15.48°E / -8.98; 15.48
Diameter 340 m[1]
Eponym Astronaut-named feature

Spook crater is a small crater in the Descartes Highlands of the moon visited by the astronauts of Apollo 16. The name of the crater was formally adopted by the IAU in 1973.[1] Geology Station 2 is adjacent to Spook, between it and the smaller, younger crater called Buster to the north of it.

On April 21, 1972, the Apollo 16 lunar module (LM) Orion landed about 500 m east of Spook, which is between the prominent North Ray and South Ray craters. The astronauts John Young and Charles Duke explored the area over the course of three EVAs using a Lunar Roving Vehicle, or rover. They stopped at Spook during EVA 1, on the way back to the LM from Flag crater.

Spook crater is approximately 340 m in diameter and over 20 m deep.[2] Spook is about 550 m west of the landing site itself.

The Lunar Portable Magnetometer (LPM) was used to obtain a reading of approximately 180 γ (gamma) at Spook.[3] This was one of four locations at the landing site where the LPM was used.

The Lunar Portable Magnetometer (LPM) was used to take a magnetic field measurement at the north rim of Spook

Spook cuts into the Cayley Formation of Imbrian age.[4]

Samples

TV camera still of Charlie Duke's "juggling act" trying to catch sample 62275 at the rim of Buster crater. The sample is to the right of his helmet and above his outstretched hands.

The following samples were collected from the vicinity of Buster crater (Station 2), as listed in Table 6-II of the Apollo 16 Preliminary Science Report,[3] which does not include samples smaller than 25 g weight (of which there were many). Sample type, lithology, and descriptions are from the Lunar Sample Atlas of the Lunar and Planetary Institute.[5]

Sample Sample Type Lithology Photo Description
62235 rake breccia apparently homogeneous, coherent, hollocrystaline impact melt rock with classic poikilitic texture highly enriched in trace elements and siderophile elements and has been dated at 3.88 b.y., with an exposure history of 153 m.y.
62236 rake rock found to be a slowly-cooled plutonic rock (Takeda et al. 1979) with an age of ~4.3 b.y. (Borg et al. 1999).
62237 rock anorthite chalky white rock
62255 rock breccia has been crushed and granulated by shock and is penetrated with patches and veins of mafic melt
62275 rock anorthite very friable, chalky white rock that broke up into powder during handling in curatorial labs and has not been adequately studied.
62295 rake impact melt breccia blocky coherent impact melt rock with numerous micrometeorite pits on one side and none on the other

References

  1. 1 2 Spook, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
  2. ↑ Apollo 16 Landing Area, 78D2S1(50), NASA Lunar Topophotomap. Published by The Defense Mapping Agency, November 1974. Available from Lunar and Planetary Institute.
  3. 1 2 Apollo 16 Preliminary Science Report (NASA SP-315), 1972
  4. ↑ Geologic Map of the Apollo 16 (Descartes) Landing Area by Apollo Field Geology Investigation Team (D. P. Elston, E. L. Boudette, J. P. Schafer), United States Geological Survey, April 1972
  5. ↑ Lunar Sample Atlas, Lunar and Planetary Institute
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