cyanic-selkie/wikianc huggingface dataset:
LG G4
Spésifikasi
G4 dikirimkeun bareng jeung Android 5.1 "Lollipop", sanajan pangalaman pamaké sacara keseluruhan ampir sarua jeung G2 ogé. Software kaméra diupgrade kalayan rojongan gambar atah, bareng jeung mode manual anyar nu nawarkeun kamampuh pikeun ngatur fokus, gancangna shutter, ISO katut kasaimbangan bodas. Pilihanana, poto bisa dicokot sacara otomatis ku cara dua kali ngeklik salah sahiji tombol volume sok sanajan layar keur paéh ogé.
Panarimaan
Rupa-rupa opini ngeunaan G4 ditarima ti masarakat, sok sanajan lolobanaana mangrupa kritik positif ogé. The Verge ngarasa yén G4 bisa leuwih ngirut nu maké lamun miceun panyimpen tambahan katut batré nu bisa dicopotna kawas Samsung Galaxy S6. Layarna dipuji ku akurasi kelir katut pamakéan dayana dibandingkeun jeung G3, nu kacatet "sahadé, lamun teu leuwh hadé", tinimbang S6. Kaméra tukang G4 dipuji ku alatan kualitas katut réproduksi kelirna, babarengan jeung modu manual nu "kompréhénsif" katut kamampuh "henteu ilaharna" pikeun nyimpen Raw image, tapi perlu dicatet yén fokus otomatisna kadang-kadang salah fokus atawa lila teuing pikeun meunangkeun fokus, tur yén modu manualna henteu bisa ngadalikeun saturasi katut kaseukeutna. Software LG dikritik alatan teu pati robah ti batan G3, sarta kurang boga feature creep katut éstétika nu "édun". G4 meunang peunteun 7.9 ti 10, nu nyimpulkeun yén "Lain telepon cerdas nu goréng — fungsina hadé — tapi anjeun moal nempo ieu HP bisa kacekel ku unggal jalma dina paméran nagara usum panas ieu."
Kinerja LG G4 henteu kawas parabot nu maké Qualcomm's Snapdragon 810 SoC (kawas LG G Flex 2), nu panas teuing antukna Ars Technica ngarasa perlu ngurangan tugas nu loba maké CPU pikeun ngurangan kaleuwihan panas nu ngaganggu kinerjana. Sanggeus ngabandingkeun sarta nguji hal-hal séjéna, kacatet yén sistim dina képéng Snapdragon 808 G4 mah leuwih hadé ti batan 810 (uji babandingan maké HTC One M9), nu ahirna méré catetan yén "sacara subjéktif, [G4] karasa gancang, tur kami leuwih resep kaluaran panasna 808. Lamun anjeun boga perhatian kana skor babandingan, G4 kawas Samsung Exynos SoC dina Galaxy S6." Bari nganggap yén kamérana mangrupa bagéan panghadéna dina ieu parabot, Ars Technica nyimpulkeun yén G4 mangrupa "telepon cerdas kompetén nu sampurna, tapi teu pati luar biasa."
Sindangbarang, Bogor Barat, Bogor
Sindangbarang nyaéta salah sahiji désa di kacamatan Bogor Barat, Kota Bogor, Propinsi Jawa Barat, Indonésia.
2007 GY5
Ari 2007 GY5 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.392, sedengkeun magnitudo mutlakna 24.0. Ari nu jadi référénsina mah nyaéta MPO�119728.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Konéktor BNC
Konéktor BNC nyaéta hiji wangun konéktor RF nu dipigunakeun keur nerminasi kabel koaksial. The connector was named after its bayonet mount locking mechanism and its two inventors, Paul Neill of Bell Labs (inventor of the N connector) and Amphenol engineer Carl Concelman (inventor of the C connector). It is a lot smaller than N and C connectors. Nicknames the BNC has picked up over the yéars include: "Baby Neill-Concelman", "Baby N connector", "British Naval Connector", "Bayonet Nut Connector".
The BNC connector is used for professional video connections, both for analog and Serial Digital Interface signals, amateur radio antenna connections, and on néarly every piece of electronic test equipment manufactured in the last 35 or so yéars. This connector is an alternative to the RCA connector when used for composite vidéo on commercial vidéo devices, however many consumer electronics with RCA jacks have been utilized on commercial vidéo equipment with BNC jacks via adaptor. BNC connectors were commonly used on 10base2 thin Ethernet networks, both on cable interconnections and network cards, though these have largely been replaced by newer Ethernet devices whose wiring does not use coaxial cable. Some ARCNET networks use BNC terminated coax.
The BNC connectors are commonly used in NIM electronics, but they are now often replaced by LEMO miniature connectors which allow for higher densities.
Tumbu Luar
מחבר RF コネクタ Коаксиальный радиочастотный разъём
Kertanegara, Kertanegara, Purbalingga
Kertanegara nyaéta salasahiji désa di Kacamatan Kertanegara, Purbalingga, Propinsi Jawa Tengah, Indonésia.
Gepuk
Gepuk (atawa sok disebut ogé empal) nyaéta jinis kadaharan anu bahan poko nyieunna tina daging (ilaharna mah daging sapi), nu saterusna disamaraan ogé dikulub mangjam-jam, geus kitu kakara wéh digoréng. Dina kahirupan sapopoé, gepuk téh kadaharan nu sok disuguhkeun minangka deungeun sangu. Gepuk atawa empal téa anu pangkakoncarana mah nyaéta gepuk asal Kota Bandung, nikakeun ku urang deungeun mah gepuk téh dianggep minangka kadaharan has tatar sunda. Margalantarannana mah nyaéta ku sabab rasana anu sedep tur dagingna hipu, gampang digayemna ogé henteu liat.
Babasan
Sakapeung, istilah gepuk téh ku urang Sunda mah sok dijieun guyonan. Nyaéta minangka istilah jeung paribasa mun dahar euweuh nanaon, cohagna mah ngan ukur jeung kurupuk hungkul. Gepuk téh diguyonkeunna nyaéta minangka singgetan tina “gep kurupuk-gep kurupuk”. Hartina pas unggal dahar téh ngan jeung kurupuk deui waé. Ieu singgetan lain singgetan asli, mung jadi kirata lamun keur teu bararoga deungeun sangu.
Lawe Kinga Gabungan, Semadam, Aceh Tenggara
Lawe Kinga Gabungan nyaéta salah sahiji Gampong di kacamatan Semadam, Kabupatén Aceh Tenggara, Propinsi Acéh, Indonésia.
(138937) 2001 BK16
Ari (138937) 2001 BK16 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.678, sedengkeun magnitudo mutlakna 17.5. Ari nu jadi référénsina mah nyaéta MPO�372047.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Triharjo, Merbau Mataram, Lampung Kidul
Triharjo nyaéta salah sahiji Désa di kacamatan Merbau Mataram, Kabupatén Lampung Kidul, Propinsi Sumatra Kalér, Indonésia.
Samagaha panonpoé
Samagaha atawa Gerhana Panonpoé téh kajadian katutupna cahya Panonpoé ka Marcapada alatan kahalangan Bulan. <!--This configuration can only occur during a New Moon, when the Sun and Moon are in conjunction as seen from the Earth. In ancient times, and in some cultures today, solar eclipses are attributed to mythical properties. Total solar eclipses can be frightening events for people unaware of their astronomical nature, as the Sun suddenly disappears in the middle of the day and the sky darkens in a matter of minutes. However, the spiritual attribution of solar eclipses is now largely disregarded.
Total solar eclipses are very rare events for any given place on Earth because totality is only seen where the Moon's umbra touches the Earth's surface. A total solar eclipse is a spectacular natural phenomenon and many people consider travel to remote locations in order to observe one.
The 1999 total eclipse in Europe, said by some to be the most-watched eclipse in human history, helped to increase public awareness of the phenomenon. This was illustrated by the number of people willing to make the trip to witness the 2005 annular eclipse and the 2006 total eclipse. The next total solar eclipse will occur on August 1, 2008.
Types of solar eclipses
There are four types of solar eclipses:
The Earth's distance from the Sun is about 400 times the Earth's distance from the Moon. The Sun's diameter is about 400 times the diameter of the Moon. Because these ratios are approximately the same, the sizes of the Sun and the Moon as seen from Earth appear to be approximately the same: about 0.5 degree of arc in angular measure.
Because the Moon's orbit around the Earth is an ellipse, the Moon's distance from the Earth varies, so the apparent sizes of the Sun and Moon likewise vary. The magnitude of an eclipse is the ratio of the apparent size of the Moon to the apparent size of the Sun during an eclipse. An eclipse when the Moon is near its closest distance from the Earth (i.e., near its perigee) will be a total eclipse because the Moon will appear to be large enough to cover completely the Sun's bright disk, or photosphere; a total eclipse has a magnitude greater than 1. Conversely, an eclipse when the Moon is near its farthest distance from the Earth (i.e., near its apogee), will be an annular eclipse because the Moon will appear to be slightly smaller than the Sun; the magnitude of an annular eclipse is less than 1. Slightly more solar eclipses are annular than total because, on average, the Moon lies too far away from Earth to cover the Sun completely. A hybrid eclipse occurs when the magnitude of an eclipse is very close to 1: the eclipse will appear to be total at some locations on Earth and annular at other locations.
The Earth's orbit around the Sun is also elliptical, so the Earth's distance from the Sun varies throughout the year. This also affects the apparent sizes of the Sun and Moon, but not so much as the Earth's varying distance from the Moon. When the Earth approaches its farthest distance from the Sun (the aphelion) in July, this tends to favor a total eclipse. As the Earth approaches its closest distance from the Sun (the perihelion) in January, this tends to favor an annular eclipse.
Terminology
Central eclipse is often used as a generic term for a total, annular or hybrid eclipse. This is, however, not completely correct: the definition of a central eclipse is an eclipse during which the central line of the umbra touches the Earth's surface. It is possible, though extremely rare, that part of the umbra intersects with Earth (thus creating an annular or total eclipse), but not its central line. This is then called a non-central total or annular eclipse.
The term solar eclipse itself is technically a misnomer. The phenomenon of the Moon passing in front of the Sun is not an eclipse, but an occultation. Properly speaking, an eclipse occurs when one object passes into the shadow cast by another object. For example, when the Moon disappears at Full Moon by passing into Earth's shadow, the event is properly called a lunar eclipse. Therefore, the proper, but rarely used, term for what is commonly called a solar eclipse is eclipse of the Earth.
Geometry of an eclipse
The diagram to the right shows the alignment of the Sun, Moon and Earth during a solar eclipse. The dark gray region below the moon is the umbra, where the Sun is completely obscured by the Moon. The small area where the umbra touches the Earth's surface is where a total eclipse can be seen. The larger light gray area is the penumbra, in which only a partial eclipse can be seen.
As noted above, the Moon's orbit is also elliptical. The Moon's distance from the Earth can vary by about 6% from its average value. Therefore, the Moon's apparent size varies with its distance from the Earth, and it is this effect that leads to the difference between total and annular eclipses. The distance of the Earth from the Sun also varies during the year, but this is a smaller effect. On average, the Moon appears to be slightly smaller than the Sun, so the majority (about 60%) of central eclipses are annular. It is only when the Moon is closer to the Earth than average (near its perigee) that a total eclipse occurs.
The Moon orbits the Earth in approximately 27.3 days, relative to a fixed frame of reference. This is known as the sidereal month. However, during one sidereal month, the Earth has revolved around the Sun, making the average time between one New Moon and the next longer than the sidereal month: it is approximately 29.6 days. This is known as the synodic month, and corresponds to what is commonly called the lunar month. The Moon crosses from south to north of the ecliptic at its ascending node. However, the nodes of the Moon's orbit are gradually moving in a retrograde motion, due to the action of the Sun's gravity on the Moon's motion, and they make a complete circuit every 18.5 years. This means that the time between each passage of the Moon through the ascending node is slightly shorter than the sidereal month. This period is called the draconitic month.
The Moon's orbit intersects with the ecliptic at the two nodes that are 180 degrees apart. Therefore, the New Moon occurs close to the nodes at two periods of the year approximately six months apart, and there will always be at least one solar eclipse during these periods. Sometimes the New Moon occurs close enough to a node during two consecutive months. This means that in any given year, there will always be at least two solar eclipses, and there can be as many as five. However, some are visible only as partial eclipses, because the umbra passes above Earth's north or south pole, and others are central only in remote regions of the Arctic or Antarctic.
Path of an eclipse
During a central eclipse, the Moon's umbra (or antumbra, in the case of an annular eclipse) moves rapidly from west to east across the Earth. The Earth is also rotating from west to east, but the umbra always moves faster than any given point on the Earth's surface, so it almost always appears to move in a roughly west-east direction across a map of the Earth (there are some rare exceptions to this which can occur during an eclipse of the midnight sun in Arctic or Antarctic regions).
The width of the track of a central eclipse varies according to the relative apparent diameters of the Sun and Moon. In the most favourable circumstances, when a total eclipse occurs very close to perigee, the track can be over 250 km wide and the duration of totality may be over 7 minutes. Outside of the central track, a partial eclipse can usually be seen over a much larger area of the Earth.
Occurrence and eclipse cycles
Total solar eclipses are rare events. Although they occur somewhere on Earth approximately every 18 months, it has been estimated that they recur at any given place only once every 370 years, on average. Then, after waiting so long, the total eclipse only lasts for a few minutes, as the Moon's umbra moves eastward at over 1700 km/h. Totality can never last more than 7 min 40 s, and is usually much shorter: during each millennium there are typically fewer than 10 total solar eclipses exceeding 7 minutes. The last time this happened was June 30 1973. Observers aboard a Concorde aircraft were able to stretch totality to about 74 minutes by flying along the path of the Moon's umbra. The next eclipse of comparable duration will not occur until June 25, 2150. The longest total solar eclipse during the 8,000-year period from 3000 BC to 5000 AD will occur on July 16 2186, when totality will last 7 min 29 s.
If the date and time of any solar eclipse are known, it is possible to predict other eclipses using eclipse cycles. Two such cycles are the Saros and the Inex. The Saros cycle is probably the best known, and one of the most accurate, eclipse cycles. The Inex cycle is itself a poor cycle, but it is very convenient in the classification of eclipse cycles. After a Saros cycle finishes, a new Saros cycle begins one Inex later, hence its name: in-ex. A Saros cycle lasts 6,585.3 days (a little over 18 years), which means that after this period a practically identical eclipse will occur. The most notable difference will be a shift of 120° in longitude (due to the 0.3 days) and a little in latitude. A Saros series always starts with a partial eclipse at a pole, then shifts over the globe through a series of annular or total eclipses, and ends on the other pole a couple of millennia later.
Final totality
Due to tidal acceleration, the orbit of the Moon around the Earth is unstable, and becomes approximately 3.8 cm more distant each year. It is estimated that in 600 million years, the distance from the Earth to the Moon will have increased by 23500 km, meaning that it will no longer be able to completely cover the Sun's disk. This will be true even when the Moon is at perigee, and the Earth at aphelion.
A complicating factor is that the Sun will increase in size over this timescale. This makes it even more unlikely that the Moon will be able to cause a total eclipse. We can therefore say that the last total solar eclipse on Earth will occur in slightly less than 600 million years.
Historical solar eclipses
A solar eclipse of 15 June 763 BC mentioned in an Assyrian text is important for the Chronology of the Ancient Orient. This is the earliest solar eclipse mentioned in historical sources that has been identified beyond reasonable doubt. There have been other claims to date earlier eclipses, notably that of Mursili II (likely 1312 BC), in Babylonia, and also in China, but these are highly disputed and rely on much supposition.
It has also been attempted to establish the exact date of Good Friday by means of solar eclipses, but this research has not yielded conclusive results.
Observing a solar eclipse
Looking directly at the photosphere of the Sun (the bright disk of the Sun itself), even for just a few seconds, can cause permanent damage to the retina of the eye, because of the intense visible and invisible radiation that the photosphere emits. This damage can result in permanent impairment of vision, up to and including blindness. The retina has no sensitivity to pain, and the effects of retinal damage may not appear for hours, so there is no warning that injury is occurring.
Under normal conditions, the Sun is so bright that it is difficult to stare at it directly, so there is no tendency to look at it in a way that might damage the eye. However, during an eclipse, with so much of the Sun covered, it is easier and more tempting to stare at it. Unfortunately, looking at the Sun during an eclipse is just as dangerous as looking at it outside an eclipse, except during the brief period of totality, when the Sun's disk is completely covered (totality occurs only during a total eclipse and only very briefly; it does not occur during a partial or annular eclipse). Viewing the Sun's disk through any kind of optical aid (binoculars, a telescope, or even an optical camera viewfinder) is even more hazardous.
Glancing at the Sun with all or most of its disk visible is unlikely to result in permanent harm, as the pupil will close down and reduce the brightness of the whole scene. If the eclipse is near total, the low average amount of light causes the pupil to open. Unfortunately the remaining parts of the Sun are still just as bright, so they are now brighter on the retina than when looking at a full Sun. As the eye has a small fovea, for detailed viewing, the tendency will be to track the image on to this best part of the retina, causing damage.
Viewing partial and annular eclipses
Viewing the Sun during partial and annular eclipses (and during total eclipses outside the brief period of totality) requires special eye protection, or indirect viewing methods. The Sun's disk can be viewed using appropriate filtration to block the harmful part of the Sun's radiation. Sunglasses are not safe, since they do not block the harmful and invisible infrared radiation which causes retinal damage. Only properly designed and certified solar filters should ever be used for direct viewing of the Sun's disk.
The safest way to view the Sun's disk is by indirect projection. This can be done by projecting an image of the disk onto a white piece of paper or card using a pair of binoculars (with one of the lenses covered), a telescope, or another piece of cardboard with a small hole in it (about 1 mm diameter), often called a pinhole camera. The projected image of the Sun can then be safely viewed; this technique can be used to observe sunspots, as well as eclipses. However, care must be taken to ensure that no one looks through the projector (telescope, pinhole, etc.) directly. Viewing the Sun's disk on a video display screen (provided by a video camera or digital camera) is safe, although the camera itself may be damaged by direct exposure to the Sun. The optical viewfinders provided with some video and digital cameras are not safe.
Viewing totality during total eclipses
Contrary to popular belief, it is safe to observe the total phase of a solar eclipse directly with the unaided eye, binoculars or a telescope, when the Sun's photosphere is completely covered by the Moon; indeed, this is a very spectacular and beautiful sight, and it is too dim to be seen through filters. The Sun's faint corona will be visible, and even the chromosphere, solar prominences, and possibly even a solar flare may be seen. However, it is important to stop directly viewing the Sun promptly at the end of totality. The exact time and duration of totality for the location from which the eclipse is being observed should be determined from a reliable source.
Also very beautiful are the effects just before (and just after) totality. When the shrinking visible part of the photosphere becomes very small, Baily beads will occur (see picture). These are caused by the sunlight still being able to reach Earth through lunar valleys, but no longer where mountains are present. Totality then begins with the diamond ring effect, the last bright flash of sunlight. Note that it is not entirely safe to view Baily beads or the diamond ring without proper eye protection (because in both cases the photosphere is still visible).
Paul Bettany
Paul Bettany (gumelar di London, Inggris, 27 Méi 1971) nyaéta saurang aktor asal Inggris. Paul mangrupa salaki ti aktris Jennifer Connelly anu papanggih nalika babarengan ngabéntangan pilem The Beautiful Mind (2001), nu harita ogé dipanggihkeun jeung aktor Russell Crowe. Paul sorangan ti umur salapan belas taun geus ngagugulung mengeluti dunya akting, liwat pangung téater. Disusul ku tawaran pikeun merankeun dina pilem layar lébar. Akting-akting kasohorna di antarana nalika merankeun Géoffrey Chaucer dina pilem A Knight's Tale (2001), tuluy salaku Charles Herman dina THE BéaUTIFUL MIND (2001), salaku Dr. Stephen Maturin dina pilem Master And Commander: The Far Side Of The World, salaku Peter Colt dina dokuménter Wimbledon (2004) jeung peranna salaku Silas dina pilem kontrovérsial The Da Vinci Code (2006). Dina kahirupanna Bettany kakojot ku masalah jeung narkoba, malah mah pernah kabeulit masalah jeung patugas hotél, alatan pangaruh kokain. Tapi karirna mah teu pati kapangaruhan nepi ka kiwari popularitasna masih kénéh nanjeur.
Samagaha panonpoé
Other observations
For astronomers, a total solar eclipse forms a rare opportunity to observe the corona (the outer layer of the Sun's atmosphere). Normally this is not visible because the photosphere is much brighter than the corona. According to the point reached in the solar cycle, the corona can appear rather small and symmetric, or large and fuzzy. It is very hard to predict this prior to totality.
Special observation campaigns
In 1919, the observation of a total solar eclipse helped to confirm Einstein's theory of general relativity. By comparing the apparent distance between two stars, with and without the Sun between them, the theoretical predictions about gravitational lenses were confirmed (though the data were ambiguous at the time). Of course the observation with the Sun between was only possible during totality, since the stars are visible then.
Over the years, some less important special observations took place:
Solar eclipse before sunrise or after sunset
The phenomenon of atmospheric diffraction makes it possible to observe the Sun (and hence a solar eclipse) even when it is slightly below the horizon. It is however possible for a solar eclipse to attain totality (or in the event of a partial eclipse, near totality) before (visual and actual) sunrise or after sunset from a particular location. When this occurs shortly before the former or after the latter, the sky will appear much darker than it would otherwise be immediately before sunrise or after sunset. On these occasions, an object (especially a planet, often Mercury) may be visible near the sunrise or sunset point of the horizon when it could not have been seen without the eclipse.
Simultaneous occurrence of eclipses and transits
In principle, the simultaneous occurrence of a Solar eclipse and a transit of a planet is possible. But these events are extremely rare because of their short durations. The next anticipated simultaneous occurrence of a Solar eclipse and a transit of Mercury will be on July 5, 6757, and a Solar eclipse and a transit of Venus is expected on April 5, 15232.
Melakasari, Babakan, Cirebon
Melakasari nyaéta salah sahiji désa di kacamatan Babakan, Kabupatén Cirebon, Propinsi Jawa Barat, Indonésia.
Rd Ariffien
Radén Ariffien (gumelar di Cimahi, Jawa Kulon, 23 Juni 1902 – tilar dunya 28 Désémber 1976 dina umur 74 taun) nyaéta wartawan, sutradara, jeung pamaén filem Indonésia. Mimitina anclub kana sandiwara dina rék kajadian Perang Dunya II. Sareng Andjar Asmara, Bahtiar Effendi, jeung Suska ngadirikeun sandiwara "Bolero" nu tos ngurilingan Sumatra jeung Singapura. Salian ti sandiwara, anjeunna ogé sok nulis artikel nu disebarkeun ka kota-kota gedé di Indonésia dina waktu panjajahan Jepang. Seueur pangalaman anu dijalankeun ku anjeunna, di antarana pernah jadi pingpinan rédaksi majalah hiburan Varia saanggeus pupusna Andjar Asamara. Seueur pisan filem anu disutradai anjeunna.
2016 HN3
Ari 2016 HN3 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.554, sedengkeun magnitudo mutlakna 21.6. Ari nu jadi référénsina mah nyaéta MPO�392479.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Samagaha panonpoé
Simultaneous occurrence of eclipses and transits
More common, but still quite rare, is a conjunction of any planet (not confined exclusively to Mercury or Venus) at the time of a total solar eclipse, in which event the planet will be visible very near the eclipsed Sun, when without the eclipse it would have been lost in the Sun's glare. At one time, some scientists hypothesized that there may be a planet (often given the name Vulcan) even closer to the Sun than Mercury; the only way to confirm its existence would have been to observe it during a total solar eclipse. However, it is now known that no such planet exists, although there remains some possibility for small Vulcanoid asteroids to exist, although none have ever been found.
Solar eclipses by and from artificial satellites
Artificial satellites can also get in the line between the Earth and the Sun, but none is large enough to cause an eclipse. At the altitude of the International Space Station, for example, an object would need to be about 3.35 km across to blot the Sun out entirely. This means the best you can get is a satellite transit, but these events are difficult to watch, because the zone of visibility is very small. The satellite passes over the face of the Sun in about a second, typically. As with a transit of a planet, it will not get dark.
Artificial satellites do play an important role in documenting solar eclipses. Images of the umbra on the Earth's surface taken from Mir and the International Space Station are among the most spectacular eclipse images in history. Observations of eclipses from satellites orbiting above the Earth's atmosphere are of course not subject to weather conditions.
The direct observation of a total solar eclipse from space is rather rare. The only documented case is Gemini 12 in 1966. The partial phase of the 2006 total eclipse was visible from the International Space Station. At first, it looked as though an orbit correction in the middle of March would bring the ISS in the path of totality, but this correction was postponed.
References
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Kuala Raja, Kuala, Bireuen
Kuala Raja nyaéta salah sahiji Gampong di kacamatan Kuala, Kabupatén Bireuen, Propinsi Acéh, Indonésia.
Mondrali, Idanogawo, Nias
Mondrali nyaéta salah sahiji Désa di kacamatan Idanogawo, Kabupatén Nias, Propinsi Sumatra Kalér, Indonésia.
Banjar TV
Banjar TV nyaéta setasion TV lokal di Indonésia.
Lubuk Mandarsah, Tengah Ilir, Tebo
Lubuk Mandarsah nyaéta salah sahiji désa di kacamatan Tengah Ilir, Kabupatén Tebo, Propinsi Jambi, Indonésia.
1094
Taun ka-1094 Maséhi dina Kalénder Grégorian.
2015 BT4
Ari 2015 BT4 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.637, sedengkeun magnitudo mutlakna 21.4. Ari nu jadi référénsina mah nyaéta MPO�386892.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Noel Gallagher
Noel Gallagher anu boga ngaran lengkep Noel Thomas David Gallagher (gumelar 29 Méi 1967-ayeuna) nyaéta penyanyi jeung penulis lagu, lian ti éta, Noel kasohor salaku gitaris grup musik Oasis .Noel nyaéta lanceukna Liam Gallagher, vokalis Oasis. Lalaki anu gumelar di Longsight, Mancherster, Inggris ieu mulai maén gitar ti umur 13 taun sacara otodidak. Noel pernah ngalaman kacelakaan anu ngabalukarkeun suku katuhuna cidera terus teu meunang gawé beurat, tapi ieu hal dipaké pikeun latihan gitar jeung nulis lagu ku Noel. Noel nikah jeung Meg Mathews taun 1997, nalika manéhna keur nyiapkeun album Be Here Now, tapi ahirna mah cerai bulan Januari 2001 sabab aya awéwé séjén dina kahirupan Noel. Lalaki anu resep kana sepak bola ieu ngajalin hubungan jeung awéwé asal Skotlandia, Sara MacDonald, tina ieu hubungan, Noel boga anak nu kadua.
Taun 1998, Noel ngiluan audisi pikeun jadi personil grup musik Inspiral Carpets tapi gagal, terus manéhna asup jadi personil Oasis jeung lanceukna, Liam Gallagher (vokal), Paul McGuigan (bass), Tony McCarroll (drum), jeung Paul Arthurs (gitar). Noel geus méré kontribusi anu gédé dina penulisan katut garapan lagu-lagu Oasis, di antarana: Definitely Maybe, (What's the Story) Morning Glory?, Be Here Now Standing on the Shoulder of Giants, Heathen Chemistry, Don't Believe the Truth, Oasis Studio Album VII dan juga album kompilasi The Masterplan jeung Stop the Clocks.
Sabada Oasis bubar, ahirna Noel balik deui ka panggung salaku penyanyi solo. Konser perdana jeung grup musik nu mirigna High Flying Birds ieu dilaksanakeun di Dublin tanggal 23 Oktober 2011. Noel mawakeun 20 lagu anu hampir sakabéhna materi anyar kaasup 9 lagu Oasis.
Sonia Natalia
Sonia Natalia atanapi anu biasa dikenal ku Sonia atanapi Wawa (ogé katelah Sonia JKT48) (salami janten anggota JKT48) nyaéta salah sahiji penyanyi asal Indonesia sareng urut anggota grup idola JKT48. Anjeunna adi ngora panyanyi sareng aktris, nyaéta Stella Cornelia. Ayeuna, Sonia parantos aya dina Tim T ti saprak 1 Juli 2018, sareng ogé Sonia salaku anggota tarian sub unit JKT48 Dance Project.
Aek Bolon Julu, Balige, Toba Samosir
Aek Bolon Julu nyaéta salah sahiji Désa di kacamatan Balige, Kabupatén Toba Samosir, Propinsi Sumatra Kalér, Indonésia.
Stasion Réndéh
Stasion Réndéh (RH) (Aksara Sunda Baku: ) nyaéta stasion karéta api anu perenahna di Réndé, Cikalong Wétan, Bandung Kulon. Stasion ieu boga dua jalur kalawan jalur 2 minangka jalur lurus. Stasion ieu dilayanan ku Karéta api lokal Purwakarta-Cicaléngka jeung Karéta api lokal Cibatu.
Tumbu kaluar
Situs resmi PT Kereta Api Indonesia
2010 NN
Ari 2010 NN mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.447, sedengkeun magnitudo mutlakna 28.4. Ari nu jadi référénsina mah nyaéta MPO�179639.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
2010 RB130
Ari 2010 RB130 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.525, sedengkeun magnitudo mutlakna 24.3. Ari nu jadi référénsina mah nyaéta MPO 190732.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Park Min-woo
Park Min-Woo nyaéta saurang aktor Koréa Kidul. Park ngamimitian peranna minangka peran babantu dina sérial drama komédi romantis Flower Boy Ramen Shop taun 2011. Tuluy manéhna bijil dina drama tipi, saperti I Need a Fairy taun 2012 jeung Play Guide taun 2013. Park Min-woo ogé salah sahiji aktor matuh variety show Roommate anu mimiti midang dina taun 2014.
SMKS Bina Putra Mandiri
SMKS Bina Putra Mandiri nyaéta Sakola Menengah Kajuruan Swasta anu aya di Kabupatén Bogor. Alamat lengkepna di Bina Putra Mandiri No 1, Kalurahan/Désa Parungpanjang Kacamatan Parung Panjang, Kabupatén Bogor, Jawa Kulon kalawan nomor NPSN 20255780.
Blok Bengkel, Kota Sigli, Pidie
Blok Bengkel nyaéta salah sahiji Gampong di kacamatan Kota Sigli, Kabupatén Pidie, Propinsi Acéh, Indonésia.
Blok Bengkel, Kota Sigli, Pidie
Indraloka I, Way Kenanga, Tulang Bawang Kulon
Indraloka I, Way Kenanga, Tulang Bawang Barat
2016 TZ10
Ari 2016 TZ10 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.205, sedengkeun magnitudo mutlakna 23.9. Ari nu jadi référénsina mah nyaéta MPO 389510.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
SMK Darul Hikam Binong
SMK Darul Hikam Binong nyaéta Sakola Menengah Kajuruan Swasta anu aya di Kabupatén Subang. Alamat lengkepna di Jl. Pasar Wates No. 23, Kalurahan/Désa Binong Kacamatan Binong, Kabupatén Subang, Jawa Kulon kalawan nomor NPSN 20271052.
Ramy Sabry
Ramy Sabry (رامي صبري; ) nyaéta saurang aktor sareng panyanyi Mesir.
Situgedé, Bogor Barat, Bogor
Situgedé nyaéta salah sahiji désa di kacamatan Bogor Barat, Kota Bogor, Propinsi Jawa Barat, Indonésia.
(425250) 2009 WG54
Ari 2009 WG54 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.288, sedengkeun magnitudo mutlakna 21.2. Ari nu jadi référénsina mah nyaéta MPO 380240.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Mergasana, Kertanegara, Purbalingga
Mergasana nyaéta salasahiji désa di Kacamatan Kertanegara, Purbalingga, Propinsi Jawa Tengah, Indonésia.
2005 XW77
Ari 2005 XW77 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.356, sedengkeun magnitudo mutlakna 20.7. Ari nu jadi référénsina mah nyaéta MPO 221063.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Lawe Kinga Tebing Tinggi, Semadam, Aceh Tenggara
Lawe Kinga Tebing Tinggi nyaéta salah sahiji Gampong di kacamatan Semadam, Kabupatén Aceh Tenggara, Propinsi Acéh, Indonésia.
SMAN 1 Kasokandel
SMAN 1 Kasokandel nyaéta Sakola Menengah Atas Negeri anu aya di Kabupatén Majalengka. Alamat lengkepna di Jl. Desa Kasokandel Timur No.65, Kalurahan/Désa Kasokandel Kacamatan Kasokandel, Kabupatén Majalengka, Jawa Kulon kalawan nomor NPSN 20213883.
Panca Tunggal, Merbau Mataram, Lampung Kidul
Panca Tunggal nyaéta salah sahiji Désa di kacamatan Merbau Mataram, Kabupatén Lampung Kidul, Propinsi Sumatra Kalér, Indonésia.
Balam Jaya, Way Kenanga, Tulang Bawang Kulon
Balam Jaya nyaéta salah sahiji Désa di kacamatan Way Kenanga, Kabupatén Tulang Bawang Kulon, Propinsi Sumatra Kalér, Indonésia.
Balam Jaya, Way Kenanga, Tulang Bawang Barat
2013 BB70
Ari 2013 BB70 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.302, sedengkeun magnitudo mutlakna 23.9. Ari nu jadi référénsina mah nyaéta MPO�254842.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Lueng Daneun, Peusangan Siblah Krueng, Bireuen
Lueng Daneun nyaéta salah sahiji Gampong di kacamatan Peusangan Siblah Krueng, Kabupatén Bireuen, Propinsi Acéh, Indonésia.
Gedung Indonesia Menggugat
Gedung Indonésia Mengugat téh ayana di jalan Perintis Kemerdékaan nomer 5, Kota Bandung, Jawa Barat. Asalna mah imah urang Walanda nu diadegkeun taun 1907, tapi dina taun 1917 robah jadi Landraad (baléwatangan) pamarentah kolonial Walanda.
Taun 1930, Landraad jadi tempat sidang keur para pajoang, di antarana Soekarno, Maskoen, Gatot Mangkoepradja, Soepriadinata, Sastromoeljono, jeung Sartono. Soekarno disidang alatan dituding barontak ka pamaréntah kolonial, tapi Soekarno malah malik ngadakwa ka pamaréntah Walanda nu kajadianana kawentar ku sebutan “Indonésia Menggugat”. Tah, tina kajadian éta nu jadi lantaran kiwari dingaranan Gedung Indonésia Manggugat, nu emprona mah diistrénan taun 2005 ku Gupernur Jawa Barat, HC Mashudi, sanggeus diréhab.
Sabada kamerdikaan GIM sababaraha kali genti paké ku sababaraha lembaga, jadi kantor Palang Merah Indonésia (PMI) nepi taun 1950-an. Ti taun 1950-an nepika taun 1973 jadi Gedung Keuangan, sanggeus éta jadi Kantor Dinas Perdagangan dan Perindustrian Jawa Barat.
Pante Teungoh, Kota Sigli, Pidie
Pante Teungoh, Kota Sigli, Pidie
Gilles de Rais
Gilles de Rais mangrupikeun bangsawan Prancis dina abad ka-15, tentara jeung mangrupa réncang Joan of Arc salila Perang Saratus Taun ngalawan Inggris. karir militér Rais mawa Rais meunang loba pujian, tapi reputasi dibédakeun jeung gaya hirup méwah nyumputkeun sisi poék pikasieuneun nu mangrupa tuduhan Satanisme, pemerkosaan jeung pembunuhan. Ti taun 1430-an, Rais dilaporkeun nyiksa jeung maéhan barudak sacara brutal, loba ti maranéhna budak lalaki patani nu datang ka istanana keur garawé jadi tukang ngabersihan buruan. saenggeus penganiayaan seksual, Rais bakal maéhan maranéhna ku cara motongkeun genggerong atawa motongkeun beuheungna. nu séjén dipotong beuheung jeung dimutilasi, jeung rais nepika dikenal keur ngambeu sirah buntung sababaraha korbana.
Gilles de Rais bisa disebut psikopat. jalma nu saolah mibanda 2 karakter beda. keur saha ogé anu maca biografi atawa artikel ngeunaan Gilles de Rais, tangtubakal sarua pendapatna. Boh umpatan naon nu pantes dibikeun keur manéhna gara-gara kalakuan super telengesna éta. Korban nu metot haténa bakal dipenggal sirahna jeung diteundeun sarta dikoleksi jadi tanda manéhna ngahurmat sosok korban.
1093
Taun ka-1093 Maséhi dina Kalénder Grégorian.
Sibolahotang SAS, Balige, Toba Samosir
Sibolahotang SAS nyaéta salah sahiji Désa di kacamatan Balige, Kabupatén Toba Samosir, Propinsi Sumatra Kalér, Indonésia.
Gariswanci sajarah Islam abad ka-8
Tempo ogé
Gariswanci sajarah Islam
Pakusambén, Babakan, Cirebon
Pakusambén nyaéta salah sahiji désa di kacamatan Babakan, Kabupatén Cirebon, Propinsi Jawa Barat, Indonésia.
2001 AV43
Ari 2001 AV43 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.241, sedengkeun magnitudo mutlakna 24.6. Ari nu jadi référénsina mah nyaéta MPO�277116.
Bojongkerta, Bogor Selatan, Bogor
Bojongkerta nyaéta salah sahiji désa di kacamatan Bogor Selatan, Kota Bogor, Propinsi Jawa Barat, Indonésia.
Tetehosi, Idanogawo, Nias
Tetehosi nyaéta salah sahiji Désa di kacamatan Idanogawo, Kabupatén Nias, Propinsi Sumatra Kalér, Indonésia.
Indraloka II, Way Kenanga, Tulang Bawang Kulon
Indraloka II nyaéta salah sahiji Désa di kacamatan Way Kenanga, Kabupatén Tulang Bawang Kulon, Propinsi Sumatra Kalér, Indonésia.
Indraloka II, Way Kenanga, Tulang Bawang Barat
2015 HN10
Ari 2015 HN10 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.223, sedengkeun magnitudo mutlakna 25.9. Ari nu jadi référénsina mah nyaéta MPO 337076.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Karanglewas, Kutasari, Purbalingga
Karanglewas nyaéta salasahiji désa di Kacamatan Kutasari, Purbalingga, Propinsi Jawa Tengah, Indonésia.
SMKS Mulia Buana
SMKS Mulia Buana nyaéta Sakola Menengah Kajuruan Swasta anu aya di Kabupatén Bogor. Alamat lengkepna di Jl.Pesantren No.23, Kalurahan/Désa Kabasiran Kacamatan Parung Panjang, Kabupatén Bogor, Jawa Kulon kalawan nomor NPSN 20258522.
Indosiar
Indosiar nyaéta setasion TV nasional di Indonésia.
2013 NP8
Ari 2013 NP8 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.438, sedengkeun magnitudo mutlakna 21.7. Ari nu jadi référénsina mah nyaéta MPO 278278.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
2007 GX5
Ari 2007 GX5 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.556, sedengkeun magnitudo mutlakna 24.3. Ari nu jadi référénsina mah nyaéta MPO�121363.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
Canting
Canting nyaéta pakakas anu dipaké pikeun nyokot malam panas mangsa ngabatik. Canting dijieun tina tambaga kiwari aya ogé anu dijieun tina teflon, gagangna tina  awi aya ogé tina kai. anu aya di Museum Nasional Indonesia, Jakarta. Ditengah palebah luhur : canting, pakakas pikeun ngucurkeun lilin/malam; ti kénca ka katuhu: sikat tina tapas kalapa, kaliper beusi jang ngukur, kaliper, capit, palu, jeung kihkir.
Bagéan tina canting
Gedé jeung leutikna nyamplung gumantung kana gambar jeung pola anu bakal dijieun, nyamplung dikerelepkeun kana malam panas sangkan kaeusian.
Rupa-rupa canting dumasar kana cucukna
Cucuk canting aya sababaraha rupa gumantung kabutuhan:
(138893) 2000 YH66
Ari (138893) 2000 YH66 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.744, sedengkeun magnitudo mutlakna 18.1. Ari nu jadi référénsina mah nyaéta MPO�396155.
Bebentukan
Kawas sakumna astéroid, ieu astéroid kabentuk tina nébula panonpoé primordial minangka beubeulahan planétisimal, objék di nébula marcapada ngora nu teu cukup badag pikeun robah jadi planét.
SMK Imam Ghozali
SMK Imam Ghozali nyaéta Sakola Menengah Kajuruan Swasta anu aya di Kabupatén Subang. Alamat lengkepna di Dusun Tanjungwangi Rt.12 Rw.03, Kalurahan/Désa Karangwangi Kacamatan Binong, Kabupatén Subang, Jawa Kulon kalawan nomor NPSN 69952436.
Pelayangan, Babakan, Cirebon
Pelayangan nyaéta salah sahiji désa di kacamatan Babakan, Kabupatén Cirebon, Propinsi Jawa Barat, Indonésia.
Kebun Sere, Semadam, Aceh Tenggara
Kebun Sere nyaéta salah sahiji Gampong di kacamatan Semadam, Kabupatén Aceh Tenggara, Propinsi Acéh, Indonésia.
1092
Taun ka-1092 Maséhi dina Kalénder Grégorian.
Munjul, Kutasari, Purbalingga
Munjul nyaéta salasahiji désa di Kacamatan Kutasari, Purbalingga, Propinsi Jawa Tengah, Indonésia.
Mekar Jaya, Merbau Mataram, Lampung Kidul
Mekar Jaya nyaéta salah sahiji Désa di kacamatan Merbau Mataram, Kabupatén Lampung Kidul, Propinsi Sumatra Kalér, Indonésia.
Mekar Jaya, Merbau Mataram, Lampung Selatan
Machu Picchu
Machu Picchu (Quechua Machu Pikchu, Gunung Buhun, kadang disebut "Dayeuh Ingka nu Leungit", Lost City of the Incas) téh ruruntuk Inca pra-Columbus nu perenahna aya di puhu gunung anu luhurna kira 2,350 m, luhureun lembah Urubamba, Péru, kira 70 km kalér-kuloneun Cusco. Situs ieu mimiti kawentar ka sakuliah dunya nalika ahli arkéologi ti Yale, Hiram Bingham, ngagali deui ieu situs taun 1911, sarta nulis buku ngeunaan papanggihanana ieu. Kiwari, Péru keur narékahan tina jihat hukum sangkan titinggal/artéfak nu dibawa ku Bingham bisa dibalikkeun deui. Ti taun 1983, ieu situs diaku salaku Situs Warisan Dunya UNESCO.
Sajarah
Sigana mah situs ieu téh titinggal Karajaan Ingka nu pangweuteuhna. Numutkeun panalungtikan, kota ieu mimiti diwangun ku Sapa Inca Pachacuti, kira taun 1440, nepi ka talukna Péru ka Spanyol taun 1532. Bukti arkéologis (katut laporan/naskah kolonial) nunjukkeun yén Machu Picchu téh lain kota biasa, tapi mangrupa pangreureuhan/paniisan para ménak Ingka (sarupa jeung Paniisan Romawi). Di ieu situs aya karaton jeung candi sesembahan Ingka sabudeureun palataran, sarta wangunan lianna salaku wangunan pangrojong. Kota ieu bisa dieusi ku paling loba 750 jalma sakaligus, tapi mun keur teu dianjangan ku para ménak mah pangeusina téh ukur saeutik. <!-- It is thought that the site was chosen for its unique location and geological features. It is said that the silhouette of the mountain range behind Machu Picchu represents the face of the Inca looking upward towards the sky, with the largest peak, Huayna Picchu (meaning Young Mountain) representing his nose. The peak is also known as the "hitching post of the sun."
In 1913, the site received significant publicity after the National Geographic Society devoted their entire April 1913 issue to Machu Picchu.
SMK Tri Daya Budi Majalengka
SMK Tri Daya Budi Majalengka nyaéta Sakola Menengah Kajuruan Swasta anu aya di Kabupatén Majalengka. Alamat lengkepna di Jl. Raya Kasokandel No.62, Kalurahan/Désa Kasokandel Kacamatan Kasokandel, Kabupatén Majalengka, Jawa Kulon kalawan nomor NPSN 20247193.
Machu Picchu
Sajarah
One of the Chilean poet Pablo Neruda's best-known works is "The Heights of Machu Picchu", inspired by the city:
Location
Machu Picchu is located 70 kilometers to the northwest of Cusco, in the crest of the mountain Machu Picchu, located about 2,350 meters above sea level. It is one of the most important archaeological centers in South America and as a consequence the most visited tourist attraction in Peru.