Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

Jump to content

Kirkwood (crater)

Kirkwood
Clementine mosaic
Coordinates68°48′N 156°06′W / 68.8°N 156.1°W / 68.8; -156.1[1]
Diameter68.12 km
Depth5.29 km (3.29 mi)[2]
Colongitude200° at sunrise
EponymDaniel Kirkwood

Kirkwood is a well-formed lunar impact crater that is located on the far side of the Moon,[3] on the northern hemisphere, approximately 68 kilometers in diameter. It lies just to the northeast of the crater Sommerfeld, and Hippocrates is located to the east-northeast. It was named after American astronomer Daniel Kirkwood.[1]

This formation dates to the Eratosthenian epoch of the lunar geologic timescale.[4] The perimeter of this crater is generally circular, with a few slight outward notches particularly to the southeast. It displays very little appearance of wear, and neither the interior nor the outer rampart are marked by any craters of note.

The inner wall has slumped somewhat, and has formed a few terrace-like structures. The interior ejecta spreads a good way across the inner floor, covering nearly half the diameter. At the midpoint appear several small hills producing a central peak formation.

Satellite craters

[edit]
Image taken by the Lunar Orbiter 5 (1967)

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Kirkwood.[5]

FeatureLatitudeLongitudeDiameterRef
Kirkwood T 69.4° N 165.2° W 18.61 km WGPSN
Kirkwood Y 72.2° N 157.5° W 17.21 km WGPSN

See also

[edit]

References

[edit]
  1. 1 2 "Kirkwood (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. Joshi, Maitri P. (February 2017). "Physical properties of lunar craters". Research in Astronomy and Astrophysics. 17 (3). id. 24. Bibcode:2017RAA....17...24J. doi:10.1088/1674-4527/17/3/24.
  3. Moore, Patrick (2000). The Data Book of Astronomy. CRC Press. p. 68. ISBN 978-1-4200-3344-1.
  4. Tompkins, Stefanie; Pieters, Carle M. (January 1999). "Mineralogy of the lunar crust: Results from Clementine". Meteoritics & Planetary Science. 34 (1): 25–41. Bibcode:1999M&PS...34...25T. doi:10.1111/j.1945-5100.1999.tb01729.x.
  5. Grego, P. (2015). "Satellite Crater". In Hargitai, H.; Kereszturi, Á. (eds.). Encyclopedia of Planetary Landforms. New York, NY: Springer. doi:10.1007/978-1-4614-3134-3_328.

Sources

[edit]