document_title: Moon

question_text: what are the light areas on the moon called

question_tokens: what are the light areas on the moon called

text: Moon

text: Name and etymology

text: The usual English proper name for Earth's natural satellite is "the Moon".[12][13] The noun moon is derived from moone (around 1380), which developed from mone (1135), which is derived from Old English mōna (dating from before 725), which ultimately stems from Proto-Germanic *mǣnōn, like all Germanic language cognates.[14] Occasionally, the name "Luna" is used. In literature, especially science fiction, "Luna" is used to distinguish it from other moons, while in poetry, the name has been used to denote personification of our moon.[15]

text: The principal modern English adjective pertaining to the Moon is lunar, derived from the Latin Luna. A less common adjective is selenic, derived from the Ancient Greek Selene (Σελήνη), from which is derived the prefix "seleno-" (as in selenography).[16][17] Both the Greek Selene and the Roman goddess Diana were alternatively called Cynthia.[18] The names Luna, Cynthia, and Selene are reflected in terminology for lunar orbits in words such as apolune, pericynthion, and selenocentric. The name Diana is connected to dies meaning 'day'.

text: Formation

text: Several mechanisms have been proposed for the Moon's formation 4.51 billion years ago,[f] and some 60 million years after the origin of the Solar System.[19] These mechanisms included the fission of the Moon from Earth's crust through centrifugal force[20] (which would require too great an initial spin of Earth),[21] the gravitational capture of a pre-formed Moon[22] (which would require an unfeasibly extended atmosphere of Earth to dissipate the energy of the passing Moon),[21] and the co-formation of Earth and the Moon together in the primordial accretion disk (which does not explain the depletion of metals in the Moon).[21] These hypotheses also cannot account for the high angular momentum of the Earth–Moon system.[23]

text: The prevailing hypothesis is that the Earth–Moon system formed as a result of the impact of a Mars-sized body (named Theia) with the proto-Earth (giant impact), that blasted material into orbit about the Earth that then accreted to form the present Earth-Moon system.[24][25]

text: The far side of the Moon has a crust that is 30 mi (48 km) thicker than the near side of the Moon. This is thought to be due to the Moon having been amalgamated from two different bodies.

text: This hypothesis, although not perfect, perhaps best explains the evidence. Eighteen months prior to an October 1984 conference on lunar origins, Bill Hartmann, Roger Phillips, and Jeff Taylor challenged fellow lunar scientists: "You have eighteen months. Go back to your Apollo data, go back to your computer, do whatever you have to, but make up your mind. Don't come to our conference unless you have something to say about the Moon's birth." At the 1984 conference at Kona, Hawaii, the giant impact hypothesis emerged as the most popular.

text: Before the conference, there were partisans of the three "traditional" theories, plus a few people who were starting to take the giant impact seriously, and there was a huge apathetic middle who didn’t think the debate would ever be resolved. Afterward there were essentially only two groups: the giant impact camp and the agnostics.[26]

text: Giant impacts are thought to have been common in the early Solar System. Computer simulations of a giant impact have produced results that are consistent with the mass of the lunar core and the present angular momentum of the Earth–Moon system. These simulations also show that most of the Moon derived from the impactor, rather than the proto-Earth.[27] More recent simulations suggest a larger fraction of the Moon derived from the original Earth mass.[28][29][30][31] Studies of meteorites originating from inner Solar System bodies such as Mars and Vesta show that they have very different oxygen and tungsten isotopic compositions as compared to Earth, whereas Earth and the Moon have nearly identical isotopic compositions. The isotopic equalization of the Earth-Moon system might be explained by the post-impact mixing of the vaporized material that formed the two,[32] although this is debated.[33]

text: The great amount of energy released in the impact event and the subsequent re-accretion of that material into the Earth-Moon system would have melted the outer shell of Earth, forming a magma ocean.[34][35] Similarly, the newly formed Moon would also have been affected and had its own lunar magma ocean; estimates for its depth range from about 500 km (300 miles) to its entire depth (1,737 km (1,079 miles)).[34]

text: While the giant impact hypothesis might explain many lines of evidence, there are still some unresolved questions, most of which involve the Moon's composition.[36]

text: In 2001, a team at the Carnegie Institute of Washington reported the most precise measurement of the isotopic signatures of lunar rocks.[37] To their surprise, the team found that the rocks from the Apollo program carried an isotopic signature that was identical with rocks from Earth, and were different from almost all other bodies in the Solar System. Because most of the material that went into orbit to form the Moon was thought to come from Theia, this observation was unexpected. In 2007, researchers from the California Institute of Technology announced that there was less than a 1% chance that Theia and Earth had identical isotopic signatures.[38] Published in 2012, an analysis of titanium isotopes in Apollo lunar samples showed that the Moon has the same composition as Earth,[39] which conflicts with what is expected if the Moon formed far from Earth's orbit or from Theia. Variations on the giant impact hypothesis may explain this data.

text: Physical characteristics

text: Internal structure

text:
Chemical composition of the lunar surface regolith (derived from crustal rocks)[40]

Compound
Formula
Composition (wt %)

Maria
Highlands

silica
SiO2
45.4%
45.5%

alumina
Al2O3
14.9%
24.0%

lime
CaO
11.8%
15.9%

iron(II) oxide
FeO
14.1%
5.9%

magnesia
MgO
9.2%
7.5%

titanium dioxide
TiO2
3.9%
0.6%

sodium oxide
Na2O
0.6%
0.6%

Total
99.9%
100.0%

tag: table

text: The Moon is a differentiated body: it has a geochemically distinct crust, mantle, and core. The Moon has a solid iron-rich inner core with a radius of 240 km (150 mi) and a fluid outer core primarily made of liquid iron with a radius of roughly 300 km (190 mi). Around the core is a partially molten boundary layer with a radius of about 500 km (310 mi).[41][42] This structure is thought to have developed through the fractional crystallization of a global magma ocean shortly after the Moon's formation 4.5 billion years ago.[43] Crystallization of this magma ocean would have created a mafic mantle from the precipitation and sinking of the minerals olivine, clinopyroxene, and orthopyroxene; after about three-quarters of the magma ocean had crystallised, lower-density plagioclase minerals could form and float into a crust atop.[44] The final liquids to crystallise would have been initially sandwiched between the crust and mantle, with a high abundance of incompatible and heat-producing elements.[1] Consistent with this perspective, geochemical mapping made from orbit suggests the crust of mostly anorthosite.[9] The Moon rock samples of the flood lavas that erupted onto the surface from partial melting in the mantle confirm the mafic mantle composition, which is more iron rich than that of Earth.[1] The crust is on average about 50 km (31 mi) thick.[1]

text: The Moon is the second-densest satellite in the Solar System, after Io.[45] However, the inner core of the Moon is small, with a radius of about 350 km (220 mi) or less,[1] around 20% of the radius of the Moon. Its composition is not well defined, but is probably metallic iron alloyed with a small amount of sulfur and nickel; analyses of the Moon's time-variable rotation suggest that it is at least partly molten.[46]

text: Surface geology

text: The topography of the Moon has been measured with laser altimetry and stereo image analysis.[47] Its most visible topographic feature is the giant far-side South Pole–Aitken basin, some 2,240 km (1,390 mi) in diameter, the largest crater on the Moon and the second-largest confirmed impact crater in the Solar System.[48][49] At 13 km (8.1 mi) deep, its floor is the lowest point on the surface of the Moon.[48][50] The highest elevations of the Moon's surface are located directly to the northeast, and it has been suggested might have been thickened by the oblique formation impact of the South Pole–Aitken basin.[51] Other large impact basins, such as Imbrium, Serenitatis, Crisium, Smythii, and Orientale, also possess regionally low elevations and elevated rims.[48] The far side of the lunar surface is on average about 1.9 km (1.2 mi) higher than that of the near side.[1]

text: The discovery of fault scarp cliffs by the Lunar Reconnaissance Orbiter suggest that the Moon has shrunk within the past billion years, by about 90 metres (300 ft).[52] Similar shrinkage features exist on Mercury.

text: Volcanic features

text: The dark and relatively featureless lunar plains, clearly seen with the naked eye, are called maria (Latin for "seas"; singular mare), as they were once believed to be filled with water;[53] they are now known to be vast solidified pools of ancient basaltic lava. Although similar to terrestrial basalts, lunar basalts have more iron and no minerals altered by water.[54][55] The majority of these lavas erupted or flowed into the depressions associated with impact basins. Several geologic provinces containing shield volcanoes and volcanic domes are found within the near side "maria".[56]

text: Almost all maria are on the near side of the Moon, and cover 31% of the surface of the near side,[57] compared with 2% of the far side.[58] This is thought to be due to a concentration of heat-producing elements under the crust on the near side, seen on geochemical maps obtained by Lunar Prospector's gamma-ray spectrometer, which would have caused the underlying mantle to heat up, partially melt, rise to the surface and erupt.[44][59][60] Most of the Moon's mare basalts erupted during the Imbrian period, 3.0–3.5 billion years ago, although some radiometrically dated samples are as old as 4.2 billion years.[61] Until recently, the youngest eruptions, dated by crater counting, appeared to have been only 1.2 billion years ago.[62] In 2006, a study of Ina, a tiny depression in Lacus Felicitatis, found jagged, relatively dust-free features that, due to the lack of erosion by infalling debris, appeared to be only 2 million years old.[63] Moonquakes and releases of gas also indicate some continued lunar activity.[63] In 2014 NASA announced "widespread evidence of young lunar volcanism" at 70 irregular mare patches identified by the Lunar Reconnaissance Orbiter, some less than 50 million years old. This raises the possibility of a much warmer lunar mantle than previously believed, at least on the near side where the deep crust is substantially warmer due to the greater concentration of radioactive elements.[64][65][66][67] Just prior to this, evidence has been presented for 2–10 million years younger basaltic volcanism inside Lowell crater,[68][69] Orientale basin, located in the transition zone between the near and far sides of the Moon. An initially hotter mantle and/or local enrichment of heat-producing elements in the mantle could be responsible for prolonged activities also on the far side in the Orientale basin.[70][71]

text: The lighter-coloured regions of the Moon are called terrae, or more commonly highlands, because they are higher than most maria. They have been radiometrically dated to having formed 4.4 billion years ago, and may represent plagioclase cumulates of the lunar magma ocean.[61][62] In contrast to Earth, no major lunar mountains are believed to have formed as a result of tectonic events.[72]

text: The concentration of maria on the Near Side likely reflects the substantially thicker crust of the highlands of the Far Side, which may have formed in a slow-velocity impact of a second moon of Earth a few tens of millions of years after their formation.[73][74]

text: Impact craters

text: The other major geologic process that has affected the Moon's surface is impact cratering,[75] with craters formed when asteroids and comets collide with the lunar surface. There are estimated to be roughly 300,000 craters wider than 1 km (0.6 mi) on the Moon's near side alone.[76] The lunar geologic timescale is based on the most prominent impact events, including Nectaris, Imbrium, and Orientale, structures characterized by multiple rings of uplifted material, between hundreds and thousands of kilometres in diameter and associated with a broad apron of ejecta deposits that form a regional stratigraphic horizon.[77] The lack of an atmosphere, weather and recent geological processes mean that many of these craters are well-preserved. Although only a few multi-ring basins have been definitively dated, they are useful for assigning relative ages. Because impact craters accumulate at a nearly constant rate, counting the number of craters per unit area can be used to estimate the age of the surface.[77] The radiometric ages of impact-melted rocks collected during the Apollo missions cluster between 3.8 and 4.1 billion years old: this has been used to propose a Late Heavy Bombardment of impacts.[78]

text: Blanketed on top of the Moon's crust is a highly comminuted (broken into ever smaller particles) and impact gardened surface layer called regolith, formed by impact processes. The finer regolith, the lunar soil of silicon dioxide glass, has a texture resembling snow and a scent resembling spent gunpowder.[79] The regolith of older surfaces is generally thicker than for younger surfaces: it varies in thickness from 10–20 km (6.2–12.4 mi) in the highlands and 3–5 km (1.9–3.1 mi) in the maria.[80] Beneath the finely comminuted regolith layer is the megaregolith, a layer of highly fractured bedrock many kilometres thick.[81]

text: Comparison of high-resolution images obtained by the Lunar Reconnaissance Orbiter has shown a contemporary crater-production rate significantly higher than previously estimated. A secondary cratering process caused by distal ejecta is thought to churn the top two centimetres of regolith a hundred times more quickly than previous models suggested–on a timescale of 81,000 years.[82][83]

text: Lunar swirls

text: Lunar swirls are enigmatic features found across the Moon's surface, which are characterized by a high albedo, appearing optically immature (i.e. the optical characteristics of a relatively young regolith), and often displaying a sinuous shape. Their curvilinear shape is often accentuated by low albedo regions that wind between the bright swirls.

text: Presence of water

text: Liquid water cannot persist on the lunar surface. When exposed to solar radiation, water quickly decomposes through a process known as photodissociation and is lost to space. However, since the 1960s, scientists have hypothesized that water ice may be deposited by impacting comets or possibly produced by the reaction of oxygen-rich lunar rocks, and hydrogen from solar wind, leaving traces of water which could possibly persist in cold, permanently shadowed craters at either pole on the Moon.[84][85] Computer simulations suggest that up to 14,000 km2 (5,400 sq mi) of the surface may be in permanent shadow.[86] The presence of usable quantities of water on the Moon is an important factor in rendering lunar habitation as a cost-effective plan; the alternative of transporting water from Earth would be prohibitively expensive.[87]

text: In years since, signatures of water have been found to exist on the lunar surface.[88] In 1994, the bistatic radar experiment located on the Clementine spacecraft, indicated the existence of small, frozen pockets of water close to the surface. However, later radar observations by Arecibo, suggest these findings may rather be rocks ejected from young impact craters.[89] In 1998, the neutron spectrometer on the Lunar Prospector spacecraft showed that high concentrations of hydrogen are present in the first meter of depth in the regolith near the polar regions.[90] Volcanic lava beads, brought back to Earth aboard Apollo 15, showed small amounts of water in their interior.[91]

text: The 2008 Chandrayaan-1 spacecraft has since confirmed the existence of surface water ice, using the on-board Moon Mineralogy Mapper. The spectrometer observed absorption lines common to hydroxyl, in reflected sunlight, providing evidence of large quantities of water ice, on the lunar surface. The spacecraft showed that concentrations may possibly be as high as 1,000 ppm.[92] In 2009, LCROSS sent a 2,300 kg (5,100 lb) impactor into a permanently shadowed polar crater, and detected at least 100 kg (220 lb) of water in a plume of ejected material.[93][94] Another examination of the LCROSS data showed the amount of detected water to be closer to 155 ± 12 kg (342 ± 26 lb).[95]

text: In May 2011, 615–1410 ppm water in melt inclusions in lunar sample 74220 was reported,[96] the famous high-titanium "orange glass soil" of volcanic origin collected during the Apollo 17 mission in 1972. The inclusions were formed during explosive eruptions on the Moon approximately 3.7 billion years ago. This concentration is comparable with that of magma in Earth's upper mantle. Although of considerable selenological interest, this announcement affords little comfort to would-be lunar colonists—the sample originated many kilometers below the surface, and the inclusions are so difficult to access that it took 39 years to find them with a state-of-the-art ion microprobe instrument.

text: Gravitational field

text: The gravitational field of the Moon has been measured through tracking the Doppler shift of radio signals emitted by orbiting spacecraft. The main lunar gravity features are mascons, large positive gravitational anomalies associated with some of the giant impact basins, partly caused by the dense mare basaltic lava flows that fill those basins.[97][98] The anomalies greatly influence the orbit of spacecraft about the Moon. There are some puzzles: lava flows by themselves cannot explain all of the gravitational signature, and some mascons exist that are not linked to mare volcanism.[99]

text: Magnetic field

text: The Moon has an external magnetic field of about 1–100 nanoteslas, less than one-hundredth that of Earth. It does not currently have a global dipolar magnetic field and only has crustal magnetization, probably acquired early in lunar history when a dynamo was still operating.[100][101] Alternatively, some of the remnant magnetization may be from transient magnetic fields generated during large impact events through the expansion of an impact-generated plasma cloud in the presence of an ambient magnetic field. This is supported by the apparent location of the largest crustal magnetizations near the antipodes of the giant impact basins.[102]

text: Atmosphere

text: The Moon has an atmosphere so tenuous as to be nearly vacuum, with a total mass of less than 10 metric tons (9.8 long tons; 11 short tons).[105] The surface pressure of this small mass is around 3 × 10−15 atm (0.3 nPa); it varies with the lunar day. Its sources include outgassing and sputtering, a product of the bombardment of lunar soil by solar wind ions.[9][106] Elements that have been detected include sodium and potassium, produced by sputtering (also found in the atmospheres of Mercury and Io); helium-4 and neon[107] from the solar wind; and argon-40, radon-222, and polonium-210, outgassed after their creation by radioactive decay within the crust and mantle.[108][109] The absence of such neutral species (atoms or molecules) as oxygen, nitrogen, carbon, hydrogen and magnesium, which are present in the regolith, is not understood.[108] Water vapour has been detected by Chandrayaan-1 and found to vary with latitude, with a maximum at ~60–70 degrees; it is possibly generated from the sublimation of water ice in the regolith.[110] These gases either return into the regolith due to the Moon's gravity or are lost to space, either through solar radiation pressure or, if they are ionized, by being swept away by the solar wind's magnetic field.[108]

text: Dust

text: A permanent asymmetric moon dust cloud exists around the Moon, created by small particles from comets. Estimates are 5 tons of comet particles strike the Moon's surface each 24 hours. The particles strike the Moon's surface ejecting moon dust above the Moon. The dust stays above the Moon approximately 10 minutes, taking 5 minutes to rise, and 5 minutes to fall. On average, 120 kilograms of dust are present above the Moon, rising to 100 kilometers above the surface. The dust measurements were made by LADEE's Lunar Dust EXperiment (LDEX), between 20 and 100 kilometers above the surface, during a six-month period. LDEX detected an average of one 0.3 micrometer moon dust particle each minute. Dust particle counts peaked during the Geminid, Quadrantid, Northern Taurid, and Omicron Centaurid meteor showers, when the Earth, and Moon, pass through comet debris. The cloud is asymmetric, more dense near the boundary between the Moon's dayside and nightside.[111][112]

text: Seasons

text: The Moon's axial tilt with respect to the ecliptic is only 1.5424°,[113] much less than the 23.44° of Earth. Because of this, the Moon's solar illumination varies much less with season, and topographical details play a crucial role in seasonal effects.[114] From images taken by Clementine in 1994, it appears that four mountainous regions on the rim of Peary Crater at the Moon's north pole may remain illuminated for the entire lunar day, creating peaks of eternal light. No such regions exist at the south pole. Similarly, there are places that remain in permanent shadow at the bottoms of many polar craters,[86] and these dark craters are extremely cold: Lunar Reconnaissance Orbiter measured the lowest summer temperatures in craters at the southern pole at 35 K (−238 °C; −397 °F)[115] and just 26 K (−247 °C; −413 °F) close to the winter solstice in north polar Hermite Crater. This is the coldest temperature in the Solar System ever measured by a spacecraft, colder even than the surface of Pluto.[114] Average temperatures of the Moon's surface are reported, but temperatures of different areas will vary greatly depending upon whether they are in sunlight or shadow.[116]

text: Relationship to Earth

text: Orbit

text: The Moon makes a complete orbit around Earth with respect to the fixed stars about once every 27.3 days[g] (its sidereal period). However, because Earth is moving in its orbit around the Sun at the same time, it takes slightly longer for the Moon to show the same phase to Earth, which is about 29.5 days[h] (its synodic period).[57] Unlike most satellites of other planets, the Moon orbits closer to the ecliptic plane than to the planet's equatorial plane. The Moon's orbit is subtly perturbed by the Sun and Earth in many small, complex and interacting ways. For example, the plane of the Moon's orbit gradually rotates once every 18.61[117] years, which affects other aspects of lunar motion. These follow-on effects are mathematically described by Cassini's laws.[118]

text: Relative size

text: The Moon is exceptionally large relative to Earth: a quarter its diameter and 1/81 its mass.[57] It is the largest moon in the Solar System relative to the size of its planet,[i] though Charon is larger relative to the dwarf planet Pluto, at 1/9 Pluto's mass.[j][119] Earth and the Moon are nevertheless still considered a planet–satellite system, rather than a double planet, because their barycentre, the common centre of mass, is located 1,700 km (1,100 mi) (about a quarter of Earth's radius) beneath Earth's surface.[120]

text: Appearance from Earth

text: The Moon is in synchronous rotation: it rotates about its axis in about the same time it takes to orbit Earth. This results in it always keeping nearly the same face turned towards Earth. However, due to the effect of libration, about 59% of the Moon's surface can actually be seen from Earth.

text: The Moon used to rotate at a faster rate, but early in its history, its rotation slowed and became tidally locked in this orientation as a result of frictional effects associated with tidal deformations caused by Earth.[121] With time, the energy of rotation of the Moon on its axis was dissipated as heat, until there was no rotation of the Moon relative to the Earth. The side of the Moon that faces Earth is called the near side, and the opposite the far side. The far side is often inaccurately called the "dark side", but it is in fact illuminated as often as the near side: once per lunar day, during the new moon phase we observe on Earth when the near side is dark.[122] In 2016, planetary scientists, using data collected on the much earlier Nasa Lunar Prospector mission, found two hydrogen-rich areas on opposite sides of the Moon, probably in the form of water ice. It is speculated that these patches were the poles of the Moon billions of years ago, before it was tidally locked to Earth.[123]

text: The Moon has an exceptionally low albedo, giving it a reflectance that is slightly brighter than that of worn asphalt. Despite this, it is the brightest object in the sky after the Sun.[57][k] This is partly due to the brightness enhancement of the opposition effect; at quarter phase, the Moon is only one-tenth as bright, rather than half as bright, as at full moon.[124]

text: Additionally, colour constancy in the visual system recalibrates the relations between the colours of an object and its surroundings, and because the surrounding sky is comparatively dark, the sunlit Moon is perceived as a bright object. The edges of the full moon seem as bright as the centre, with no limb darkening, due to the reflective properties of lunar soil, which reflects more light back towards the Sun than in other directions. The Moon does appear larger when close to the horizon, but this is a purely psychological effect, known as the Moon illusion, first described in the 7th century BC.[125] The full moon subtends an arc of about 0.52° (on average) in the sky, roughly the same apparent size as the Sun (see § Eclipses).

text: The highest altitude of the Moon in the sky varies with the lunar phase and the season of the year. The full moon is highest during winter. The 18.61-year nodes cycle also has an influence: when the ascending node of the lunar orbit is in the vernal equinox, the lunar declination can go as far as 28° each month. This means the Moon can go overhead at latitudes up to 28° from the equator, instead of only 18°. The orientation of the Moon's crescent also depends on the latitude of the observation site: close to the equator, an observer can see a smile-shaped crescent moon.[126]

text: The Moon is visible for two weeks every 27.3 days at the North and South Pole. The Moon's light is used by zooplankton in the Arctic when the sun is below the horizon for months on end.[127]

text:
The distance between the Moon and Earth varies from around 356,400 km (221,500 mi) to 406,700 km (252,700 mi) at perigees (closest) and apogees (farthest), respectively. On 14 November 2016, it was closer to Earth when at full phase than it has been since 1948, 14% closer than its farthest position in apogee.[130] Reported as a "super moon", this closest point coincides within an hour of a full moon, and it was 30% more luminous than when at its greatest distance due to its angular diameter being 14% greater, because

1.14

2

≈
1.30

{\displaystyle \scriptstyle 1.14^{2}\approx 1.30}

.[131][132][133] At lower levels, the human perception of reduced brightness as a percentage is provided by the following formula:[134][135]

text:
perceived reduction

%
=
100
×

actual reduction

%

100

{\displaystyle {\text{perceived reduction}}\%=100\times {\sqrt {{\text{actual reduction}}\% \over 100}}}

text: When the actual reduction is 1.00 / 1.30, or about 0.770, the perceived reduction is about 0.877, or 1.00 / 1.14. This gives a maximum perceived increase of 14% between apogee and perigee moons of the same phase.[136]

text: There has been historical controversy over whether features on the Moon's surface change over time. Today, many of these claims are thought to be illusory, resulting from observation under different lighting conditions, poor astronomical seeing, or inadequate drawings. However, outgassing does occasionally occur, and could be responsible for a minor percentage of the reported lunar transient phenomena. Recently, it has been suggested that a roughly 3 km (1.9 mi) diameter region of the lunar surface was modified by a gas release event about a million years ago.[137][138] The Moon's appearance, like that of the Sun, can be affected by Earth's atmosphere: common effects are a 22° halo ring formed when the Moon's light is refracted through the ice crystals of high cirrostratus cloud, and smaller coronal rings when the Moon is seen through thin clouds.[139]

text:
The illuminated area of the visible sphere (degree of illumination) is given by

(
1
−
cos

e
)

/

2
=

sin

2

(
e

/

2
)

{\displaystyle (1-\cos e)/2=\sin ^{2}(e/2)}

, where

e

{\displaystyle e}

 is the elongation (i.e., the angle between Moon, the observer (on Earth) and the Sun).

text: Tidal effects

text: The gravitational attraction that masses have for one another decreases inversely with the square of the distance of those masses from each other. As a result, the slightly greater attraction that the Moon has for the side of Earth closest to the Moon, as compared to the part of the Earth opposite the Moon, results in tidal forces. Tidal forces affect both the Earth's crust and oceans.

text: The most obvious effect of tidal forces is to cause two bulges in the Earth's oceans, one on the side facing the Moon and the other on the side opposite. This results in elevated sea levels called ocean tides.[140] As the Earth spins on its axis, one of the ocean bulges (high tide) is held in place "under" the Moon, while another such tide is opposite. As a result, there are two high tides, and two low tides in about 24 hours.[140] Since the Moon is orbiting the Earth in the same direction of the Earth's rotation, the high tides occur about every 12 hours and 25 minutes; the 25 minutes is due to the Moon's time to orbit the Earth. The Sun has the same tidal effect on the Earth, but its forces of attraction are only 40% that of the Moon's; the Sun's and Moon's interplay is responsible for spring and neap tides.[140] If the Earth were a water world (one with no continents) it would produce a tide of only one meter, and that tide would be very predictable, but the ocean tides are greatly modified by other effects: the frictional coupling of water to Earth's rotation through the ocean floors, the inertia of water's movement, ocean basins that grow shallower near land, the sloshing of water between different ocean basins.[141] As a result, the timing of the tides at most points on the Earth is a product of observations that are explained, incidentally, by theory.

text: While gravitation causes acceleration and movement of the Earth's fluid oceans, gravitational coupling between the Moon and Earth's solid body is mostly elastic and plastic. The result is a further tidal effect of the Moon on the Earth that causes a bulge of the solid portion of the Earth nearest the Moon that acts as a torque in opposition to the Earth's rotation. This "drains" angular momentum and rotational kinetic energy from Earth's spin, slowing the Earth's rotation.[140][142] That angular momentum, lost from the Earth, is transferred to the Moon in a process (confusingly known as tidal acceleration), which lifts the Moon into a higher orbit and results in its lower orbital speed about the Earth. Thus the distance between Earth and Moon is increasing, and the Earth's spin is slowing in reaction.[142] Measurements from laser reflectors left during the Apollo missions (lunar ranging experiments) have found that the Moon's distance increases by 38 mm (1.5 in) per year[143] (roughly the rate at which human fingernails grow).[144] Atomic clocks also show that Earth's day lengthens by about 15 microseconds every year,[145] slowly increasing the rate at which UTC is adjusted by leap seconds. Left to run its course, this tidal drag would continue until the spin of Earth and the orbital period of the Moon matched, creating mutual tidal locking between the two. As a result, the Moon would be suspended in the sky over one meridian, as is already currently the case with Pluto and its moon Charon. However, the Sun will become a red giant engulfing the Earth-Moon system long before this occurrence.[146][147]

text: In a like manner, the lunar surface experiences tides of around 10 cm (4 in) amplitude over 27 days, with two components: a fixed one due to Earth, because they are in synchronous rotation, and a varying component from the Sun.[142] The Earth-induced component arises from libration, a result of the Moon's orbital eccentricity (if the Moon's orbit were perfectly circular, there would only be solar tides).[142] Libration also changes the angle from which the Moon is seen, allowing a total of about 59% of its surface to be seen from Earth over time.[57] The cumulative effects of stress built up by these tidal forces produces moonquakes. Moonquakes are much less common and weaker than are earthquakes, although moon quakes can last for up to an hour—a significantly longer time than terrestrial quakes—because of the absence of water to damp out the seismic vibrations. The existence of moonquakes was an unexpected discovery from seismometers placed on the Moon by Apollo astronauts from 1969 through 1972.[148]

text: Eclipses

text: Eclipses can only occur when the Sun, Earth, and Moon are all in a straight line (termed "syzygy"). Solar eclipses occur at new moon, when the Moon is between the Sun and Earth. In contrast, lunar eclipses occur at full moon, when Earth is between the Sun and Moon. The apparent size of the Moon is roughly the same as that of the Sun, with both being viewed at close to one-half a degree wide. The Sun is much larger than the Moon but it is the precise vastly greater distance that gives it the same apparent size as the much closer and much smaller Moon from the perspective of Earth. The variations in apparent size, due to the non-circular orbits, are nearly the same as well, though occurring in different cycles. This makes possible both total (with the Moon appearing larger than the Sun) and annular (with the Moon appearing smaller than the Sun) solar eclipses.[150] In a total eclipse, the Moon completely covers the disc of the Sun and the solar corona becomes visible to the naked eye. Because the distance between the Moon and Earth is very slowly increasing over time,[140] the angular diameter of the Moon is decreasing. Also, as it evolves toward becoming a red giant, the size of the Sun, and its apparent diameter in the sky, are slowly increasing.[l] The combination of these two changes means that hundreds of millions of years ago, the Moon would always completely cover the Sun on solar eclipses, and no annular eclipses were possible. Likewise, hundreds of millions of years in the future, the Moon will no longer cover the Sun completely, and total solar eclipses will not occur.[151]

text: Because the Moon's orbit around Earth is inclined by about 5.145° (5° 9') to the orbit of Earth around the Sun, eclipses do not occur at every full and new moon. For an eclipse to occur, the Moon must be near the intersection of the two orbital planes.[152] The periodicity and recurrence of eclipses of the Sun by the Moon, and of the Moon by Earth, is described by the saros, which has a period of approximately 18 years.[153]

text: Because the Moon is continuously blocking our view of a half-degree-wide circular area of the sky,[m][154] the related phenomenon of occultation occurs when a bright star or planet passes behind the Moon and is occulted: hidden from view. In this way, a solar eclipse is an occultation of the Sun. Because the Moon is comparatively close to Earth, occultations of individual stars are not visible everywhere on the planet, nor at the same time. Because of the precession of the lunar orbit, each year different stars are occulted.[155]

text: Observation and exploration

text: Ancient and medieval studies

text: Understanding of the Moon's cycles was an early development of astronomy: by the 5th century BC, Babylonian astronomers had recorded the 18-year Saros cycle of lunar eclipses,[156] and Indian astronomers had described the Moon's monthly elongation.[157] The Chinese astronomer Shi Shen (fl. 4th century BC) gave instructions for predicting solar and lunar eclipses.[158] Later, the physical form of the Moon and the cause of moonlight became understood. The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former.[159][160] Although the Chinese of the Han Dynasty believed the Moon to be energy equated to qi, their 'radiating influence' theory also recognized that the light of the Moon was merely a reflection of the Sun, and Jing Fang (78–37 BC) noted the sphericity of the Moon.[161] In the 2nd century AD Lucian wrote a novel where the heroes travel to the Moon, which is inhabited. In 499 AD, the Indian astronomer Aryabhata mentioned in his Aryabhatiya that reflected sunlight is the cause of the shining of the Moon.[162] The astronomer and physicist Alhazen (965–1039) found that sunlight was not reflected from the Moon like a mirror, but that light was emitted from every part of the Moon's sunlit surface in all directions.[163] Shen Kuo (1031–1095) of the Song dynasty created an allegory equating the waxing and waning of the Moon to a round ball of reflective silver that, when doused with white powder and viewed from the side, would appear to be a crescent.[164]

text: In Aristotle's (384–322 BC) description of the universe, the Moon marked the boundary between the spheres of the mutable elements (earth, water, air and fire), and the imperishable stars of aether, an influential philosophy that would dominate for centuries.[165] However, in the 2nd century BC, Seleucus of Seleucia correctly theorized that tides were due to the attraction of the Moon, and that their height depends on the Moon's position relative to the Sun.[166] In the same century, Aristarchus computed the size and distance of the Moon from Earth, obtaining a value of about twenty times the radius of Earth for the distance. These figures were greatly improved by Ptolemy (90–168 AD): his values of a mean distance of 59 times Earth's radius and a diameter of 0.292 Earth diameters were close to the correct values of about 60 and 0.273 respectively.[167] Archimedes (287–212 BC) designed a planetarium that could calculate the motions of the Moon and other objects in the Solar System.[168]

text: During the Middle Ages, before the invention of the telescope, the Moon was increasingly recognised as a sphere, though many believed that it was "perfectly smooth".[169]

text: In 1609, Galileo Galilei drew one of the first telescopic drawings of the Moon in his book Sidereus Nuncius and noted that it was not smooth but had mountains and craters. Telescopic mapping of the Moon followed: later in the 17th century, the efforts of Giovanni Battista Riccioli and Francesco Maria Grimaldi led to the system of naming of lunar features in use today. The more exact 1834–36 Mappa Selenographica of Wilhelm Beer and Johann Heinrich Mädler, and their associated 1837 book Der Mond, the first trigonometrically accurate study of lunar features, included the heights of more than a thousand mountains, and introduced the study of the Moon at accuracies possible in earthly geography.[170] Lunar craters, first noted by Galileo, were thought to be volcanic until the 1870s proposal of Richard Proctor that they were formed by collisions.[57] This view gained support in 1892 from the experimentation of geologist Grove Karl Gilbert, and from comparative studies from 1920 to the 1940s,[171] leading to the development of lunar stratigraphy, which by the 1950s was becoming a new and growing branch of astrogeology.[57]

text: By spacecraft

text: 20th century

text: Soviet missions

text: The Cold War-inspired Space Race between the Soviet Union and the U.S. led to an acceleration of interest in exploration of the Moon. Once launchers had the necessary capabilities, these nations sent uncrewed probes on both flyby and impact/lander missions. Spacecraft from the Soviet Union's Luna program were the first to accomplish a number of goals: following three unnamed, failed missions in 1958,[172] the first human-made object to escape Earth's gravity and pass near the Moon was Luna 1; the first human-made object to impact the lunar surface was Luna 2, and the first photographs of the normally occluded far side of the Moon were made by Luna 3, all in 1959.

text: The first spacecraft to perform a successful lunar soft landing was Luna 9 and the first uncrewed vehicle to orbit the Moon was Luna 10, both in 1966.[57] Rock and soil samples were brought back to Earth by three Luna sample return missions (Luna 16 in 1970, Luna 20 in 1972, and Luna 24 in 1976), which returned 0.3 kg total.[173] Two pioneering robotic rovers landed on the Moon in 1970 and 1973 as a part of Soviet Lunokhod programme.

text: United States missions

text: During the late 1950s at the height of the Cold War, the United States Army conducted a classified feasibility study that proposed the construction of a manned military outpost on the Moon called Project Horizon with the potential to conduct a wide range of missions from scientific research to nuclear Earth bombardment. The study included the possibility of conducting a lunar-based nuclear test.[174][175] The Air Force, which at the time was in competition with the Army for a leading role in the space program, developed its own similar plan called Lunex.[176][177][174] However, both these proposals were ultimately passed over as the space program was largely transferred from the military to the civilian agency NASA.[177]

text: Following President John F. Kennedy's 1961 commitment to a crewed moon landing before the end of the decade, the United States, under NASA leadership, launched a series of uncrewed probes to develop an understanding of the lunar surface in preparation for crewed missions: the Jet Propulsion Laboratory's Ranger program produced the first close-up pictures; the Lunar Orbiter program produced maps of the entire Moon; the Surveyor program landed its first spacecraft four months after Luna 9. The crewed Apollo program was developed in parallel; after a series of uncrewed and crewed tests of the Apollo spacecraft in Earth orbit, and spurred on by a potential Soviet lunar flight, in 1968 Apollo 8 made the first crewed mission to lunar orbit. The subsequent landing of the first humans on the Moon in 1969 is seen by many as the culmination of the Space Race.[178]

text:
"That's one small step ..."

Problems playing this file? See media help.

text: Neil Armstrong became the first person to walk on the Moon as the commander of the American mission Apollo 11 by first setting foot on the Moon at 02:56 UTC on 21 July 1969.[179] An estimated 500 million people worldwide watched the transmission by the Apollo TV camera, the largest television audience for a live broadcast at that time.[180][181] The Apollo missions 11 to 17 (except Apollo 13, which aborted its planned lunar landing) returned 380.05 kilograms (837.87 lb) of lunar rock and soil in 2,196 separate samples.[182] The American Moon landing and return was enabled by considerable technological advances in the early 1960s, in domains such as ablation chemistry, software engineering and atmospheric re-entry technology, and by highly competent management of the enormous technical undertaking.[183][184]

text: Scientific instrument packages were installed on the lunar surface during all the Apollo landings. Long-lived instrument stations, including heat flow probes, seismometers, and magnetometers, were installed at the Apollo 12, 14, 15, 16, and 17 landing sites. Direct transmission of data to Earth concluded in late 1977 due to budgetary considerations,[185][186] but as the stations' lunar laser ranging corner-cube retroreflector arrays are passive instruments, they are still being used. Ranging to the stations is routinely performed from Earth-based stations with an accuracy of a few centimetres, and data from this experiment are being used to place constraints on the size of the lunar core.[187]

text: After the first Moon race there were years of near quietude but starting in the 1990s, many more countries have become involved in direct exploration of the Moon. In 1990, Japan became the third country to place a spacecraft into lunar orbit with its Hiten spacecraft. The spacecraft released a smaller probe, Hagoromo, in lunar orbit, but the transmitter failed, preventing further scientific use of the mission.[188] In 1994, the U.S. sent the joint Defense Department/NASA spacecraft Clementine to lunar orbit. This mission obtained the first near-global topographic map of the Moon, and the first global multispectral images of the lunar surface.[189] This was followed in 1998 by the Lunar Prospector mission, whose instruments indicated the presence of excess hydrogen at the lunar poles, which is likely to have been caused by the presence of water ice in the upper few meters of the regolith within permanently shadowed craters.[190]

text: India, Japan, China, the United States, and the European Space Agency each sent lunar orbiters, and especially ISRO's Chandrayaan-1 has contributed to confirming the discovery of lunar water ice in permanently shadowed craters at the poles and bound into the lunar regolith. The post-Apollo era has also seen two rover missions: the final Soviet Lunokhod mission in 1973, and China's ongoing Chang'e 3 mission, which deployed its Yutu rover on 14 December 2013. The Moon remains, under the Outer Space Treaty, free to all nations to explore for peaceful purposes.

text: 21st century

text: The European spacecraft SMART-1, the second ion-propelled spacecraft, was in lunar orbit from 15 November 2004 until its lunar impact on 3 September 2006, and made the first detailed survey of chemical elements on the lunar surface.[191]

text: The ambitious Chinese Lunar Exploration Program began with Chang'e 1, which successfully orbited the Moon from 5 November 2007 until its controlled lunar impact on 1 March 2009.[192] It obtained a full image map of the Moon. Chang'e 2, beginning in October 2010, reached the Moon more quickly, mapped the Moon at a higher resolution over an eight-month period, then left lunar orbit for an extended stay at the Earth–Sun L2 Lagrangian point, before finally performing a flyby of asteroid 4179 Toutatis on 13 December 2012, and then heading off into deep space. On 14 December 2013, Chang'e 3 landed a lunar lander onto the Moon's surface, which in turn deployed a lunar rover, named Yutu (Chinese: 玉兔; literally "Jade Rabbit"). This was the first lunar soft landing since Luna 24 in 1976, and the first lunar rover mission since Lunokhod 2 in 1973. China intends to launch another rover mission (Chang'e 4) before 2020, followed by a sample return mission (Chang'e 5) soon after.[193]

text: Between 4 October 2007 and 10 June 2009, the Japan Aerospace Exploration Agency's Kaguya (Selene) mission, a lunar orbiter fitted with a high-definition video camera, and two small radio-transmitter satellites, obtained lunar geophysics data and took the first high-definition movies from beyond Earth orbit.[194][195] India's first lunar mission, Chandrayaan I, orbited from 8 November 2008 until loss of contact on 27 August 2009, creating a high resolution chemical, mineralogical and photo-geological map of the lunar surface, and confirming the presence of water molecules in lunar soil.[196] The Indian Space Research Organisation planned to launch Chandrayaan II in 2013, which would have included a Russian robotic lunar rover.[197][198] However, the failure of Russia's Fobos-Grunt mission has delayed this project.

text: The U.S. co-launched the Lunar Reconnaissance Orbiter (LRO) and the LCROSS impactor and follow-up observation orbiter on 18 June 2009; LCROSS completed its mission by making a planned and widely observed impact in the crater Cabeus on 9 October 2009,[199] whereas LRO is currently in operation, obtaining precise lunar altimetry and high-resolution imagery. In November 2011, the LRO passed over the large and bright Aristarchus crater. NASA released photos of the crater on 25 December 2011.[200]

text: Two NASA GRAIL spacecraft began orbiting the Moon around 1 January 2012,[201] on a mission to learn more about the Moon's internal structure. NASA's LADEE probe, designed to study the lunar exosphere, achieved orbit on 6 October 2013.

text: Upcoming lunar missions include Russia's Luna-Glob: an uncrewed lander with a set of seismometers, and an orbiter based on its failed Martian Fobos-Grunt mission.[202][203] Privately funded lunar exploration has been promoted by the Google Lunar X Prize, announced 13 September 2007, which offers US$20 million to anyone who can land a robotic rover on the Moon and meet other specified criteria.[204] Shackleton Energy Company is building a program to establish operations on the south pole of the Moon to harvest water and supply their Propellant Depots.[205]

text: NASA began to plan to resume crewed missions following the call by U.S. President George W. Bush on 14 January 2004 for a crewed mission to the Moon by 2019 and the construction of a lunar base by 2024.[206] The Constellation program was funded and construction and testing begun on a crewed spacecraft and launch vehicle,[207] and design studies for a lunar base.[208] However, that program has been cancelled in favor of a crewed asteroid landing by 2025 and a crewed Mars orbit by 2035.[209] India has also expressed its hope to send a crewed mission to the Moon by 2020.[210]

text: Planned commercial missions

text: In 2007, the X Prize Foundation together with Google launched the Google Lunar X Prize to encourage commercial endeavors to the Moon. A prize of $20 million will be awarded to the first private venture to get to the moon with a robotic lander by the end of 2017.[211] As of August 2016, 16 teams are participating in the competition.[212]

text: In August 2016, the US government granted permission to US-based start-up Moon Express to land on the Moon.[213] This marked the first time that a private enterprise was given the right to do so. The decision is regarded as a precedent helping to define regulatory standards for deep-space commercial activity in the future, as thus far companies' operation had been restricted to being on or around Earth.[213]

text: Astronomy from the Moon

text: For many years, the Moon has been recognized as an excellent site for telescopes.[215] It is relatively nearby; astronomical seeing is not a concern; certain craters near the poles are permanently dark and cold, and thus especially useful for infrared telescopes; and radio telescopes on the far side would be shielded from the radio chatter of Earth.[216] The lunar soil, although it poses a problem for any moving parts of telescopes, can be mixed with carbon nanotubes and epoxies and employed in the construction of mirrors up to 50 meters in diameter.[217] A lunar zenith telescope can be made cheaply with ionic liquid.[218]

text: In April 1972, the Apollo 16 mission recorded various astronomical photos and spectra in ultraviolet with the Far Ultraviolet Camera/Spectrograph.[219]

text: Legal status

text: Although Luna landers scattered pennants of the Soviet Union on the Moon, and U.S. flags were symbolically planted at their landing sites by the Apollo astronauts, no nation claims ownership of any part of the Moon's surface.[220] Russia and the U.S. are party to the 1967 Outer Space Treaty,[221] which defines the Moon and all outer space as the "province of all mankind".[220] This treaty also restricts the use of the Moon to peaceful purposes, explicitly banning military installations and weapons of mass destruction.[222] The 1979 Moon Agreement was created to restrict the exploitation of the Moon's resources by any single nation, but as of 2014, it has been signed and ratified by only 16 nations, none of which engages in self-launched human space exploration or has plans to do so.[223] Although several individuals have made claims to the Moon in whole or in part, none of these are considered credible.[224][225][226]

text: In culture

text: Mythology

text: A 5,000-year-old rock carving at Knowth, Ireland, may represent the Moon, which would be the earliest depiction discovered.[227] The contrast between the brighter highlands and the darker maria creates the patterns seen by different cultures as the Man in the Moon, the rabbit and the buffalo, among others. In many prehistoric and ancient cultures, the Moon was personified as a deity or other supernatural phenomenon, and astrological views of the Moon continue to be propagated today.

text: In the Ancient Near East, the moon god (Sin/Nanna) was masculine. In Greco-Roman mythology, Sun and Moon are represented as male and female, respectively (Helios/Sol and Selene/Luna). The crescent shape from an early time was used as a symbol representing the Moon. The Moon goddess Selene was represented as wearing a crescent on her headgear in an arrangement reminiscent of horns. The star and crescent arrangement also goes back to the Bronze Age, representing either the Sun and Moon, or the Moon and planet Venus, in combination. It came to represent the goddess Artemis or Hecate, and via the patronage of Hecate came to be used as a symbol of Byzantium.

text: An iconographic tradition of representing Sun and Moon with faces developed in the late medieval period.

text: The splitting of the moon (Arabic: انشقاق القمر) is a miracle attributed to Muhammad.[228]

text: Calendar

text: The Moon's regular phases make it a very convenient timepiece, and the periods of its waxing and waning form the basis of many of the oldest calendars. Tally sticks, notched bones dating as far back as 20–30,000 years ago, are believed by some to mark the phases of the Moon.[229][230][231] The ~30-day month is an approximation of the lunar cycle. The English noun month and its cognates in other Germanic languages stem from Proto-Germanic *mǣnṓth-, which is connected to the above-mentioned Proto-Germanic *mǣnōn, indicating the usage of a lunar calendar among the Germanic peoples (Germanic calendar) prior to the adoption of a solar calendar.[232] The PIE root of moon, *méh1nōt, derives from the PIE verbal root *meh1-, "to measure", "indicat[ing] a functional conception of the moon, i.e. marker of the month" (cf. the English words measure and menstrual),[233][234][235] and echoing the Moon's importance to many ancient cultures in measuring time (see Latin mensis and Ancient Greek μείς (meis) or μήν (mēn), meaning "month").[236][237][238][239] Most historical calendars are lunisolar. The 7th-century Islamic calendar is an exceptional example of a purely lunar calendar. Months are traditionally determined by the visual sighting of the hilal, or earliest crescent moon, over the horizon.[240]

text: Modern art and literature

text: The Moon has been the subject of many works of art and literature and the inspiration for countless others. It is a motif in the visual arts, the performing arts, poetry, prose and music.

text: Lunacy

text: The Moon has long been associated with insanity and irrationality; the words lunacy and lunatic (popular shortening loony) are derived from the Latin name for the Moon, Luna. Philosophers Aristotle and Pliny the Elder argued that the full moon induced insanity in susceptible individuals, believing that the brain, which is mostly water, must be affected by the Moon and its power over the tides, but the Moon's gravity is too slight to affect any single person.[241] Even today, people who believe in a lunar effect claim that admissions to psychiatric hospitals, traffic accidents, homicides or suicides increase during a full moon, but dozens of studies invalidate these claims.[241][242][243][244][245]


document_title: Republic of Ireland at the FIFA World Cup

question_text: when did republic of ireland last qualify for world cup

root

text: FIFA World Cup record[edit]

text:
FIFA World Cup record

FIFA World Cup Qualification record

Year

Round

Position

Pld

W

D*

L

GF

GA

Pld

W

D

L

GF

GA

Position

 1930

Did not enter

–

–

–

–

–

–

–

 1934

Did not qualify

2

0

1

1

6

9

3/3

 1938

2

0

1

1

5

6

2/2

 1950

4

1

1

2

6

7

2/3

 1954

4

2

0

2

8

6

2/3

 1958

4

2

1

1

6

7

2/3

 1962

4

0

0

4

3

17

3/3

 1966

3

1

0

2

2

5

Lost Playoff

 1970

6

0

1

5

3

14

4/4

 1974

4

1

1

2

4

5

2/3

 1978

4

1

1

2

2

4

3/3

 1982

8

4

2

2

17

11

3/5

 1986

8

2

2

4

5

10

4/5

 1990

Quarter-finals

8th

5

0

4

1

2

3

8

5

2

1

10

2

2/5

 1994

Round of 16

15th

4

1

1

2

2

4

12

7

4

1

19

6

2/7

 1998

Did not qualify

12

5

4

3

25

11

2/6 Lost Playoff

  2002

Round of 16

12th

4

1

3

0

6

3

12

8

3

1

25

6

2/6 Won Playoff

 2006

Did not qualify

10

4

5

1

12

5

4/6

 2010

12

4

7

1

13

10

2/6 Lost Playoff

 2014

10

4

2

4

16

17

4/6

 2018

12

5

5

2

13

11

2/6 Lost Playoff

 2022

To be determined

To be determined

   2026

Total

Quarter-finals

3/21

13

2

8

3

10

10

141

56

43

42

199

169

text:
showFIFA World Cup History

Year
Round
Score
Result
Republic of Ireland scorers

1990

Round 1
 Republic of Ireland 1 – 1  England
Draw
Kevin Sheedy  73'

Round 1
 Republic of Ireland 1 – 1  Netherlands
Draw
Niall Quinn  71'

Round 1
 Republic of Ireland 0 – 0  Egypt
Draw

Round 2
 Republic of Ireland 0(5) – 0(4)  Romania
Draw

Quarter-finals
 Republic of Ireland 0 – 1  Italy
Loss

1994

Round 1
 Republic of Ireland 1 – 0  Italy
Win
Ray Houghton  11'

Round 1
 Republic of Ireland 1 – 2  Mexico
Loss
John Aldridge  84'

Round 1
 Republic of Ireland 0 – 0  Norway
Draw

Round 2
 Republic of Ireland 0 – 2  Netherlands
Loss

2002

Round 1
 Republic of Ireland 1 – 1  Cameroon
Draw
Matt Holland  52'

Round 1
 Republic of Ireland 1 – 1  Germany
Draw
Robbie Keane  90+2'

Round 1
 Republic of Ireland 3 – 0  Saudi Arabia
Win
Robbie Keane  7'  Gary Breen  61'  Damien Duff  87'

Round 2
 Republic of Ireland 1(2) – 1(3)  Spain
Draw
Robbie Keane  90' (pen.)

text: Republic of Ireland at Italy 1990[edit]

text:
showvteRepublic of Ireland squad  –  1990 FIFA World Cup
1 Bonner
2 Morris
3 Staunton
4 McCarthy (c)
5 Moran
6 Whelan
7 McGrath
8 Houghton
9 Aldridge
10 Cascarino
11 Sheedy
12 O'Leary
13 Townsend
14 Hughton
15 Slaven
16 Sheridan
17 Quinn
18 Stapleton
19 Kelly
20 Byrne
21 McLoughlin
22 Peyton
Coach: Charlton

text: Group F[edit]

text:
Team

Pld

W

D

L

GF

GA

GD

Pts

 England

3
1
2
0
2
1
+1
4

 Republic of Ireland

3
0
3
0
2
2
0
3

 Netherlands

3
0
3
0
2
2
0
3

 Egypt

3
0
2
1
1
2
-1
2

text: Note: Republic of Ireland awarded second place by drawing of lots

tag: p

text:
England

1 – 1

 Republic of Ireland

Lineker  8'

(Report)

Sheedy  73'

text:
Republic of Ireland

0 – 0

 Egypt

(Report)

text:
Netherlands

1 – 1

 Republic of Ireland

Gullit  10'

(Report)

Quinn  71'

text: Knockout phase[edit]

text:
Republic of Ireland

0 – 0 (a.e.t.)

 Romania

(Report)

Penalties

Sheedy Houghton Townsend Cascarino O'Leary

5 – 4

 Hagi Lupu Rotariu Lupescu Timofte

text:
Italy

1 – 0

 Republic of Ireland

Schillaci  38'

(Report)

text: Republic of Ireland at USA 1994[edit]

text:
showvteRepublic of Ireland squad  –  1994 FIFA World Cup
1 Bonner
2 Irwin
3 Phelan
4 Moran
5 McGrath
6 Keane
7 Townsend (c)
8 Houghton
9 Aldridge
10 Sheridan
11 Staunton
12 G. Kelly
13 Kernaghan
14 Babb
15 Coyne
16 Cascarino
17 McGoldrick
18 Whelan
19 McLoughlin
20 D. Kelly
21 McAteer
22 A. Kelly
Coach: Charlton

text: Group E[edit]

text:
Team

Pld

W

D

L

GF

GA

GD

Pts

 Mexico

3
1
1
1
3
3
0
4

 Republic of Ireland

3
1
1
1
2
2
0
4

 Italy

3
1
1
1
2
2
0
4

 Norway

3
1
1
1
1
1
0
4

text:
Italy

0 – 1

 Republic of Ireland

(Report)

Houghton  11'

text:
Mexico

2 – 1

 Republic of Ireland

García  42'  65'

(Report)

Aldridge  84'

text:
Republic of Ireland

0 – 0

 Norway

(Report)

text: Knockout phase[edit]

text:
Netherlands

2 – 0

 Republic of Ireland

Bergkamp  11'Jonk  41'

(Report)

text: Republic of Ireland at Korea/Japan 2002[edit]

text:
showvteRepublic of Ireland squad  –  2002 FIFA World Cup
1 Given
2 Finnan
3 Harte
4 Cunningham
5 Staunton (c)
6 Roy Keane
7 McAteer
8 Holland
9 Duff
10 Robbie Keane
11 Kilbane
12 Kinsella
13 Connolly
14 Breen
15 Dunne
16 Kiely
17 Quinn
18 G. Kelly
19 Morrison
20 O'Brien
21 Reid
22 Carsley
23 A. Kelly
Coach: McCarthy

text: Group E[edit]

text:
Team

Pld

W

D

L

GF

GA

GD

Pts

 Germany

3
2
1
0
11
1
+10
7

 Republic of Ireland

3
1
2
0
5
2
+3
5

 Cameroon

3
1
1
1
2
3
-1
4

 Saudi Arabia

3
0
0
3
0
12
-12
0

text:
Republic of Ireland

1 – 1

 Cameroon

Holland  52'

(Report)

Mboma  39'

text:
Germany

1 – 1

 Republic of Ireland

Klose  19'

(Report)

Robbie Keane  90+2'

text:
Saudi Arabia

0 – 3

 Republic of Ireland

(Report)

Robbie Keane  7'Breen  61'Duff  87'

text: Knockout phase[edit]

text:
Spain

1 – 1 (a.e.t.)

 Republic of Ireland

Morientes  8'

(Report)

Robbie Keane  90' (pen.)

Penalties

Hierro Baraja Juanfran Valerón Mendieta

3 – 2

 Robbie Keane Holland Connolly Kilbane Finnan

text: Record players[edit]

text: Defender Steve Staunton has represented the Irish team in all of their 13 World Cup matches, captaining the team in 2002.

text:
No.

Name

Matches

World Cups

1

Steve Staunton
13
1990, 1994 and 2002

2

Pat Bonner
9
1990 and 1994

Ray Houghton
9
1990 and 1994

Paul McGrath
9
1990 and 1994

Andy Townsend
9
1990 and 1994

6

John Aldridge
8
1990 and 1994

7

Niall Quinn
7
1990 and 2002

8

Tony Cascarino
6
1990 and 1994

Gary Kelly
6
1994 and 2002

Jason McAteer
6
1994 and 2002

text: Top goalscorers[edit]

text:
No.

Name

Goals

World Cups

1

Robbie Keane
3
2002

2

Niall Quinn
1
1990

Kevin Sheedy
1
1990

John Aldridge
1
1994

Ray Houghton
1
1994

Gary Breen
1
2002

Damien Duff
1
2002

Matt Holland
1
2002


document_title: American Horror Story: Apocalypse

question_text: what is the first episode of american horror story apocalypse

text: American Horror Story: Apocalypse

text: Plot

text: Apocalypse takes place in the West Coast of the United States in the near future. Following a nuclear blast that wipes out the world, Outpost 3, an underground bunker, is constructed in order to shelter specific survivors with strong genetic makeup. Wilhemina Venable (Sarah Paulson) and Miriam Mead (Kathy Bates) both command the bunker, dispensing torture towards those who reside there. People inside consist of hairdresser Mr. Gallant (Evan Peters), his grandmother Evie (Joan Collins), talk show host Dinah Stevens (Adina Porter), her son Andre (Jeffrey Bowyer-Chapman), the billionaire Coco St. Pierre Vanderbilt (Leslie Grossman), her assistant Mallory (Billie Lourd), and couple Timothy Campbell (Kyle Allen) and Emily (Ash Santos), all of which face the wrath of the two women. However, Michael Langdon (Cody Fern) arrives and begins to throw the order into chaos as he intends to bring those worthy to a "sanctuary".

text: Furthermore in the season, the arrival of Cordelia Goode, Madison Montgomery (Emma Roberts), Myrtle Snow (Frances Conroy) as well as the return of Zoe Benson (Taissa Farmiga), Queenie (Gabourey Sidibe) and Misty Day (Lily Rabe), provides background of the world before the fateful apocalypse as well as the inclusion of characters from Murder House.

text: Cast and characters

text: Main

text:
Sarah Paulson as Wilhemina Venable, Cordelia Goode, and Billie Dean Howard[3][4][5]
Evan Peters as Mr. Gallant, James Patrick March, and Tate Langdon[6][7][8]
Adina Porter as Dinah Stevens[9][4]
Billie Lourd as Mallory[10][4]
Leslie Grossman as Coco St. Pierre Vanderbilt[9][4]
Cody Fern as Michael Langdon[11]
Emma Roberts as Madison Montgomery[12]
Cheyenne Jackson as John Henry Moore[9]
Kathy Bates as Miriam Mead[6][4][5]

tag: ul

text: Recurring and guest

text:
Jeffrey Bowyer-Chapman as Andre Stevens[13][14]
Kyle Allen as Timothy Campbell[13][8]
Ash Santos as Emily[15][8]
Erika Ervin as the Fist[16]
Billy Eichner as Brock[9]
Chad James Buchanan as Stu
Sean Blakemore as a cooperative agent
Lesley Fera as a cooperative agent[17]
Joan Collins as Evie Gallant and Bubbles McGee[18][8]
Frances Conroy as Myrtle Snow and Moira O'Hara[19][20]
Taissa Farmiga as Zoe Benson and Violet Harmon[19][20][7]
Gabourey Sidibe as Queenie[19][21]
Jon Jon Briones as Ariel Augustus[22]
Billy Porter as Behold Chablis[23]
BD Wong as Baldwin Pennypacker[24][25]
Lily Rabe as Misty Day[19][20]
Stevie Nicks as herself[19][20]
Wayne Pére as Mr. Kingery
Dylan McDermott as Dr. Ben Harmon[26][27]
Connie Britton as Vivien Harmon[26][27]
Jessica Lange as Constance Langdon[3]
Carlo Rota as Anton LaVey
Naomi Grossman as Samantha Crowe[28]
Mena Suvari as Elizabeth Short
Sam Kinsey as Beau Langdon
Celia Finkelstein as Gladys
Lance Reddick as Papa Legba
Jamie Brewer as Nan

text: Episodes

text:
No.overallNo. inseasonTitleDirected byWritten byOriginal air dateProd.codeUS viewers(millions)851"The End"Bradley BueckerRyan Murphy & Brad FalchukSeptember 12, 2018 (2018-09-12)8ATS013.08[29]
In the near future, nuclear missiles destroy the world and start a nuclear winter. Thanks to her family's private plane, Coco St. Pierre Vanderbilt manages to escape the destruction of Los Angeles with her assistant Mallory, her hairdresser Mr. Gallant, and his grandmother, Evie. Meanwhile, an organization known as "The Cooperative", selects young adults to save from the apocalypse, based on their genetic makeup. Two of the selected, Timothy and Emily, are sent to Outpost 3, an underground base led by Ms. Venable. There, they are reunited with other survivors, including Coco, Mallory, Mr. Gallant, and Evie. Life at the Outpost includes strict rules and severe punishments. Eighteen months pass and the situation and food supplies are at critical condition at the Outpost. A man from the Cooperative, Michael Langdon, arrives and announces that he will judge who deserves to be truly saved.
862"The Morning After"Jennifer LynchJames WongSeptember 19, 2018 (2018-09-19)8ATS022.21[30]
Langdon introduces himself to the guests of Outpost 3 and explains his duty. He inquires Mr. Gallant about his sexual orientation and his hatred towards his grandmother. Later, the Rubber Man approaches Gallant in his bedroom and Evie catches the two having sex. She reports their insubordination to Ms. Mead. Timothy and Emily discover recent Cooperative e-mails detailing Venable's transgressions against proper Outpost protocol. Gallant refuses to reveal the identity of the Rubber Man to Venable. Gallant assures Langdon that he did not reveal his identity and Langdon asserts that he is not the Rubber Man and that he would never have sex with him. Timothy and Emily cast aspersions on the rules of Outpost 3 and they have sex for the first time. The Rubber Man attempts to seduce Gallant once again and Gallant stabs him with scissors. Langdon appears and Gallant finds himself looking upon his grandmother's bloody corpse. Timothy and Emily are caught in bed and are sentenced to death. Timothy shoots Mead in the stomach and her wound reveals internal wiring and white liquid.
873"Forbidden Fruit"Loni PeristereManny CotoSeptember 26, 2018 (2018-09-26)8ATS031.95[31]
Langdon unveils his true demonic form to Mallory and she makes flames shoot from a fireplace. Venable confides to Mead that she has not been selected to move on to the Sanctuary and Mead suggests they kill everyone. Brock navigates a nuclear wasteland and guns down a cannibalistic tribe. He then beholds a horse-drawn carriage pass by. The carriage delivers apples to Outpost 3 and Venable resolves to inject them with venom. Brock infiltrates Outpost 3 and attends Venable's Halloween masquerade ball. Coco, presuming Brock to be Langdon in costume, seduces him back to her bedroom. Brock then reveals himself to Coco and stabs her in the forehead. The Outpost 3 guests bob for poisonous apples. Venable instructs everyone to wait to eat simultaneously. The guests comply and concurrently succumb to the poison. Venable and Mead confront Langdon and Venable proclaims that they will be making the selections. Mead shoots Venable under order from Langdon. Langdon tells Mead she was modeled after a caregiver from his childhood, which consoles her. Later, Cordelia Goode, Madison Montgomery, and Myrtle Snow descend upon Outpost 3 and Cordelia resurrects Mallory, Dinah, and Coco.
884"Could It Be... Satan?"Sheree FolksonTim MinearOctober 3, 2018 (2018-10-03)8ATS042.02[32]
Three years before the nuclear bomb, the Hawthorne School for Exceptional Young Men seeks out Michael Langdon, who has been arrested for killing a man who insulted the woman Mead is modeled after. He is put to the test and displays tremendous abilities. Miss Robichaux's Academy is summoned for a meeting and Cordelia scoffs at the Grand Chancellor's suspicion that Michael may be the first male Supreme, known as the Alpha. To prove his power, Michael saves Queenie from eternal damnation at the Hotel Cortez and fetches Madison from her personal hell.
895"Boy Wonder"Gwyneth Horder-PaytonJohn J. GrayOctober 10, 2018 (2018-10-10)8ATS052.12[33]
Cordelia has a frightening vision of a destroyed Miss Robichaux's Academy and being attacked by disease-ridden people. Later, she announces that Langdon will take the Seven Wonders, something that she is berated for by Myrtle. Mallory's abilities soon intensify and Cordelia reveals that she is dying and slowly starting to lose her Supremacy. John Henry Moore discovers Langdon's true self but Mead interferes before he can warn anyone and kills him. During the test, Cordelia asks Langdon to bring Misty Day back to life, so he breaks her out of her personal hell. It is revealed that Cordelia has been planning an army against Langdon and used him to resurrect her students. Later, Cordelia asks Madison and a suspicious Behold to investigate Langdon's origins at the Murder House.
906"Return to Murder House"Sarah PaulsonCrystal LiuOctober 17, 2018 (2018-10-17)8ATS062.01[34]
Madison and Behold buy the Murder House on behalf of the Coven, under the pretense that they are a married couple. They cast a spell to force the spirits of the house to appear to them. They encounter the ghost of Constance Langdon, who agrees to provide information on her grandson Michael if they banish her old nemesis, Moira O'Hara, from the house. Madison and Behold exhume Moira's bones, and bury them with her mother's; Moira is then set free from the house. Constance tells them that she sensed an evil in Michael from very early on. In his youth, he began killing animals, and then his babysitter. After Michael ages ten years overnight, Constance enlists the help of a Catholic priest, whom Michael kills. Constance, out of hopelessness, commits suicide in the Murder House, where she is reunited with Tate, Beauregard, and her fourth child, a little girl with no eyes. Madison and Behold then interview Ben and Vivien Harmon, who further reveal the evil in Michael's soul. Vivien tells them that Michael's father is neither Ben nor Tate, but the evil of the Murder House. Before leaving with Behold, Madison reunites Tate and Violet.
917"Traitor"Jennifer LynchAdam PennOctober 24, 2018 (2018-10-24)8ATS071.85[35]
With the help of voodoo queen Dinah Stevens, Cordelia arranges a meeting with Papa Legba in an attempt to prevent Langdon's plans. Legba reveals that he owns Nan's soul, and agrees to help entrap Langdon under the condition that Cordelia give him the souls of the remaining girls. Cordelia refuses, and Legba disappears. In order to learn more about the warlocks and their plans, Madison enlists the help of Myrtle's long time friend, witch-actress Bubbles McGee, who specialises in reading the thoughts and souls of others. At a dinner party held by Myrtle, Bubbles discovers that Ariel and Baldwin know about the death of John Henry, and that they are planning to kill the women of the coven. Zoe suspects Mallory to be the true next Supreme after she saves Coco from choking and confides in Cordelia. Later, Mallory passes the Seven Wonders after successfully resurrecting John Henry. The coven then capture Ariel, Baldwin, and Mead, and burn them at the stake for treason.
928"Sojourn"[36]TBATBAOctober 31, 2018 (2018-10-31)TBATBD
939"Fire and Reign"[36]TBATBANovember 7, 2018 (2018-11-07)TBATBD
9410"Apocalypse Then"[36]TBATBANovember 14, 2018 (2018-11-14)TBATBD

text: Evan Peters will direct an episode of the season.[37]

text: Production

text: Development

text: On January 12, 2017, the series was renewed for an eighth season, which premiered on September 12, 2018.[1][2] In October 2016, series co-creator Ryan Murphy announced a "crossover" season between previous cycles Murder House and Coven.[38] In January 2018, he stated that the ninth season would most likely feature the crossover;[39] however, in June 2018, he announced that the eighth season was chosen instead.[40] Murphy has also stated that the eighth season would be set 18 months in the future and would feature an Asylum and Coven tone.[39][18] In July 2018, it was announced at the San Diego Comic-Con that the title of the season would be Apocalypse.[41]

text: In April 2018, it was revealed that series veterans Sarah Paulson and Evan Peters would each make their directorial debuts in an episode of the season.[37] It was later revealed that Paulson would direct the sixth episode.[3]

text: As with previous seasons, several teasers were released.[42] On September 4, 2018, a short trailer was released, followed by a longer trailer the next day.[43][44]

text: Casting

text: In October 2017, it was announced that series mainstay Sarah Paulson would return for the season. In March 2018, it was announced that Kathy Bates and Evan Peters would also return, leading the season with Paulson.[6] In April 2018, Joan Collins joined the cast as the grandmother of Peters' character.[18] In April and May 2018, Cult alumni Adina Porter, Cheyenne Jackson, Billy Eichner, Leslie Grossman, and Billie Lourd were also confirmed to return.[9][10]

text: In June 2018, Emma Roberts revealed that she would return for Apocalypse, reprising her role as Madison Montgomery from Coven.[12] That same month, Murphy revealed that other witches from Coven had all been invited to return,[12] and also stated that he had asked Anjelica Huston to join the cast,[45] while Paulson confirmed that she would reprise her Coven role, Cordelia Goode.[3] In July 2018, it was reported that Jeffrey Bowyer-Chapman and Kyle Allen would guest star in the season.[13] Later that month, Murphy revealed via Twitter that American Crime Story alum Cody Fern joined the cast as a grown-up Michael Langdon, the Antichrist born during the events of Murder House.[11]

text: In August 2018, Pose alum Billy Porter announced via Instagram that he would appear in the season.[23] Later, during the Television Critics Association press tour, it was announced that Jessica Lange would appear in the season's sixth episode as her Murder House character, Constance Langdon.[3] After FX released the season's first teaser, actress Lesley Fera revealed via Twitter that she would appear in the season premiere.[17] Later, Ryan Murphy confirmed via Twitter that Taissa Farmiga, Gabourey Sidibe, Lily Rabe, Frances Conroy, and Stevie Nicks would all appear during the season,[19] and that they would all reprise their Coven roles.[21][20] In the same month, Angela Bassett, who appeared in four previous seasons, confirmed that she would not appear in the season.[21] Later, Finn Wittrock, who appeared in three past seasons, confirmed that he would not appear in Apocalypse.[46] The same day, it was announced that original cast members Connie Britton and Dylan McDermott would be returning for the season,[26] and Ryan Murphy later confirmed that they would reprise their Murder House roles, Vivien and Ben Harmon, respectively.[27] Later, Murphy revealed that Evan Peters and Taissa Farmiga would be reprising their Murder House roles, Tate Langdon and Violet Harmon, respectively.[7]

text: In September 2018, it was revealed that Erika Ervin would be returning for Apocalypse after having a recurring role in Freak Show.[16] It was also reported that actress Ash Santos would appear in the season.[15]

text: Filming

text: In April 2018, Murphy revealed that filming for the season would begin in June 2018.[18]

text: Reception

text: Critical response

text: American Horror Story: Apocalypse received positive reviews from critics. The review aggregator Rotten Tomatoes gave the season a 92% approval rating, with an average rating of 7.86/10, based on 117 reviews.[47] On Metacritic, the season was given a score of 63 out of 100 based on 6 reviews, indicating "generally favorable reviews".[48]

text:
American Horror Story (season 8): Critical reception by episode

Season 8 (2018): Percentage of positive reviews tracked by the website Rotten Tomatoes[49]

text: Ratings

text:
No.

Title

Air date
Rating(18–49)
Viewers(millions)
DVR(18–49)
DVR viewers(millions)
Total(18–49)
Total viewers(millions)

1

"The End"

September 12, 2018
1.5
3.08[29]
1.5
3.17
3.0
6.26[50]

2

"The Morning After"

September 19, 2018
1.1
2.21[30]
1.2
2.41
2.3
4.63[51][a]

3

"Forbidden Fruit"

September 26, 2018
0.9
1.95[31]
N/A
N/A
N/A
N/A

4

"Could It Be... Satan?"

October 3, 2018
1.0
2.02[32]
1.6
3.05
2.6
5.08[52]

5

"Boy Wonder"

October 10, 2018
1.0
2.12[33]
1.4
2.82
2.4
4.95[53]

6

"Return to Murder House"

October 17, 2018
0.9
2.01[34]
TBD
TBD
TBD
TBD

7

"Traitor"

October 24, 2018
0.9
1.85[35]
TBD
TBD
TBD
TBD

text: Jump up ^ Live +7 ratings were not available, so Live +3 ratings have been used instead.

tag: ol