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Tycho (lunar crater)

Coordinates: 43°19′S 11°22′W / 43.31°S 11.36°W / -43.31; -11.36
From Wikipedia, the free encyclopedia
Tycho seen by Lunar Reconnaissance Orbiter (rotate display if you see a crater illusion due to the atypical position of the light source). NASA
Coordinates43°19′S 11°22′W / 43.31°S 11.36°W / -43.31; -11.36
Diameter85 km (53.4 miles)
Depth4.7 km (2.9 mi)[1]
Colongitude12° at sunrise
EponymTycho Brahe
Location of Tycho as seen from the Northern Hemisphere
3D model of Tycho crater

Tycho (/ˈtk/) is a prominent lunar impact crater located in the southern lunar highlands, named after the Danish astronomer Tycho Brahe (1546–1601).[2] It is estimated to be 108 million years old.[3]

To the south of Tycho is the crater Street, to the east is Pictet, and to the north-northeast is Sasserides. The surface around Tycho is replete with craters of various sizes, many overlapping still older craters. Some of the smaller craters are secondary craters formed from larger chunks of ejecta from Tycho. It is one of the Moon's brightest craters,[3] with a diameter of 85 km (53 mi)[4] and a depth of 4,700 m (15,400 ft).[1]

Age and description


Tycho is a relatively young crater, with an estimated age of 108 million years (Ma), based on analysis of samples of the crater ray recovered during the Apollo 17 mission.[3] This age initially suggested that the impactor may have been a member of the Baptistina family of asteroids, but as the composition of the impactor is unknown this remained conjecture.[5] However, this possibility was ruled out by the Wide-field Infrared Survey Explorer in 2011, as it was discovered that the Baptistina family was produced much later than expected, having formed approximately 80 million years ago.[6]

The crater is sharply defined, unlike older craters that have been degraded by subsequent impacts. 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 illuminated only by earthlight. Due to its prominent rays, Tycho is mapped as part of the Copernican System.[7]

The large ray system centered on Tycho

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 terraced, 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 criss-crossing array of cracks and small hills. The central peaks rise 1,600 meters (5,200 ft) 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.

Panoramic view of the lunar surface taken by Surveyor 7, which landed about 29 km (18 mi) from the rim of Tycho

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 Lunar Orbiter 5.

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 A.M.S. de Rheita depicted the bright ray system.



Tycho is named after the Danish astronomer Tycho Brahe.[2] Like many of the craters on the Moon's near side, it was given its name by the Jesuit astronomer G.B. Riccioli, whose 1651 nomenclature system has become standardized.[8][9] Earlier lunar cartographers had given the feature different names. Pierre Gassendi named it Umbilicus Lunaris ('the navel of the Moon').[10] van Langren's 1645 map calls it "Vladislai IV" after Władysław IV Vasa, King of Poland.[11][12] And Johannes Hevelius named it 'Mons Sinai' after Mount Sinai.[13]

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 Tycho.

Tycho Coordinates Diameter, km
A 39°56′S 12°04′W / 39.94°S 12.07°W / -39.94; -12.07 (Tycho A) 29
B 43°59′S 13°55′W / 43.99°S 13.92°W / -43.99; -13.92 (Tycho B) 14
C 44°07′S 13°28′W / 44.12°S 13.46°W / -44.12; -13.46 (Tycho C) 7
D 45°35′S 14°04′W / 45.58°S 14.07°W / -45.58; -14.07 (Tycho D) 26
E 42°20′S 13°40′W / 42.34°S 13.66°W / -42.34; -13.66 (Tycho E) 13
F 40°55′S 13°13′W / 40.91°S 13.21°W / -40.91; -13.21 (Tycho F) 17
H 45°17′S 15°55′W / 45.29°S 15.92°W / -45.29; -15.92 (Tycho H) 8
J 42°35′S 15°25′W / 42.58°S 15.42°W / -42.58; -15.42 (Tycho J) 11
K 45°11′S 14°23′W / 45.18°S 14.38°W / -45.18; -14.38 (Tycho K) 6
P 45°26′S 13°04′W / 45.44°S 13.06°W / -45.44; -13.06 (Tycho P) 7
Q 42°30′S 15°59′W / 42.50°S 15.99°W / -42.50; -15.99 (Tycho Q) 20
R 41°55′S 13°41′W / 41.91°S 13.68°W / -41.91; -13.68 (Tycho R) 4
S 43°28′S 16°18′W / 43.47°S 16.30°W / -43.47; -16.30 (Tycho S) 3
T 41°09′S 12°37′W / 41.15°S 12.62°W / -41.15; -12.62 (Tycho T) 14
U 41°05′S 13°55′W / 41.08°S 13.91°W / -41.08; -13.91 (Tycho U) 20
V 41°43′S 15°26′W / 41.72°S 15.43°W / -41.72; -15.43 (Tycho V) 4
W 43°18′S 15°23′W / 43.30°S 15.38°W / -43.30; -15.38 (Tycho W) 21
X 43°50′S 15°15′W / 43.84°S 15.25°W / -43.84; -15.25 (Tycho X) 12
Y 44°07′S 15°56′W / 44.12°S 15.93°W / -44.12; -15.93 (Tycho Y) 22
Z 43°14′S 16°21′W / 43.23°S 16.35°W / -43.23; -16.35 (Tycho Z) 23

Fictional references

  • In R.A. Heinlein's 1940 short story "Blowups Happen", a character speculates that Tycho may have been the location of a sentient race's main atomic power plant, in a past time when the Moon was still habitable—and that the plant exploded, causing the craters, the rays spreading from Tycho, and the death of all life on the Moon.
  • C.D. Simak set his 1961 novelette The Trouble with Tycho, at the lunar crater. He also postulated that the crater's rays were composed of volcanic glass (tektites) akin to a theory postulated by NASA researchers Dean Chapman and John O'Keefe in the 1970s.
  • In the 1987 film Can't Buy Me Love, Cindy notices Tycho while looking through a telescope on her final "contractual" date with Ronny in the Airplane Graveyard.
  • It also serves as the location of "Tycho City" in the 1996 film Star Trek: First Contact; a lunar metropolis by the 24th century.
  • In Jack Williamson's 2001 novel Terraforming Earth, the crater is utilized for "Tycho Base", a self-sustaining, robot-controlled installation aimed at restoring life to the (dead) planet Earth after an asteroid sterilizes the biosphere.
  • In the 2019 film Ad Astra, the Moon base is situated in the Tycho crater. This is Roy's first stop on his journey to Mars.
  • In R.M. Allen's Hunted Earth novels, the 'naked purples' own a former penal colony in or around Tycho crater known as "Tycho Purple Penal" (see The Ring of Charon).
  • Tycho is referenced in the band Cojum Dip's song, Waltz in E Major, Op. 15 "Moon Waltz".

See also



  1. ^ a b Margot, Jean-Luc; Campbell, Donald B.; Jurgens, Raymond F.; Slade, Martin A. (25 May 1999). "The topography of Tycho Crater". Journal of Geophysical Research: Planets. 104 (E5): 11875–11882. Bibcode:1999JGR...10411875M. doi:10.1029/1998JE900047.
  2. ^ a b "Tycho (lunar crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program., accessed 19 February 2019
  3. ^ a b c "The floor of Tycho crater". Lunar Reconnaissance Orbiter. NASA. 3 August 2017. Archived from the original on 30 March 2017. Retrieved 1 July 2018.
  4. ^ Wood, Charles A. (1 August 2006). "Tycho: The metropolitan crater of the Moon". Sky & Telescope. Retrieved 19 June 2018.
  5. ^ "Breakup event in the main asteroid belt likely caused dinosaur extinction 65 million years ago". Physorg. 5 September 2007. Retrieved 6 September 2007.
  6. ^ Plotner, Tammy (24 December 2015). "Did asteroid Baptistina kill the dinosaurs? Think other-WISE". Universe Today.
  7. ^ McCauley, John F.; Trask, Newell J. (1987). Wilhelms, D.E. (ed.). The Geologic History of the Moon (Report). Professional Paper. Vol. 1348. United States Geological Survey. Plate 11: Copernican system.
  8. ^ Whitaker 2003, pp. 61.
  9. ^ Riccioli map of the Moon (1651)
  10. ^ Whitaker 2003, pp. 33.
  11. ^ Whitaker 2003, pp. 198.
  12. ^ Langren's map of the Moon (1645)
  13. ^ Hevelius map of the Moon (1647)