cyanic-selkie/wikianc huggingface dataset:
Integral
Leibniz ngawanohkeun notasi baku long s keur integral. Integral dina paragrap samemegna bisa ditulis. Tanda ∫ ngalambakeun integral, a jeung b mangrupa titik tungtung interval, f(x) nyaéta fungsi nu di-integralkeun, sarta dx notasi keur variabel integrasi. Sajarahna, dx ngagambarkeun wilangan nu takhingga, sarta s panjang singkatan keur "jumlah". Sanajan kitu, téori integral modérn diwangun ku dasar nu béda sarta simbol tradisional ngan sakadar notation. As an example, if f is the constant function f(x)=3, then the integral of f between 0 and 10 is the aréa of the rectangle bounded by the lines x=0, x=10, y=0, and y=3. The aréa is 10c, so the value of the integral is 30.
Integrals can be taken over regions other than intervals. In general, the integral over a set E of a function f is written ∫Ef(x)dx. Here x need not be a réal number, but, for instance, a vector in R3. Fubini's theorem shows that such integrals can be rewritten as an iterated integral. In other words, the integral can be calculated by integrating one coordinate at a time.
If a function has an integral, it is said to be integrable. The function for which the integral is calculated is called the integrand. Integrals are sometimes called definite integrals to emphasize that they result in a number, not another function. This is to distinguish them from indefinite integrals, which are another name for an antiderivative. If the domain of the function is the real numbers, and if the region of integration is an interval, then the greatest lower bound of the interval is called the lower limit of integration, and the least upper bound is called the upper limit of integration.
Maniis, Cingambul, Majalengka
Maniis nyaéta salah sahiji désa di kacamatan Cingambul, Kabupatén Majalengka, Propinsi Jawa Barat, Indonésia. <!--
Integral
Ngitung integrals
Note that the integral is not actually the antiderivative (it is a number), but the fundamental théorem allows us to use antiderivatives to evaluate integrals.
Maniis, Cingambul, Majalengka
Sajarah
Sumber :
2016 EA28
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.
SMA Miftahul Ulum
SMA Miftahul Ulum nyaéta Sakola Menengah Atas Swasta anu aya di Kabupatén Cianjur. Alamat lengkepna di Jl. Sindanghayu Rt/Rw 03/03, Kalurahan/Désa Sukasirna Kacamatan Lélés, Kabupatén Cianjur, Jawa Kulon kalawan nomor NPSN 69903026.
Integral
Ngitung integrals
The difficult step is finding an antiderivative of f. It is rarely possible to glance at a function and write down its antiderivative. More often, it is necessary to use one of the many techniques that have been developed to evaluate integrals. Most of these techniques rewrite one integral as a different one which is hopefully more tractable. Techniques include:
Even if these techniques fail, it may still be possible to evaluate the integral. The next most common technique is residue calculus. There are also many less common ways of calculating definite integrals; for instance, Parseval's identity can be used to transform the integral of a square into an infinite sum. Occasionally an integral can be evaluated by a trick; for an example of this, see Gaussian integral.
Computation of volumes of solids of revolution can usually be done with disk integration or shell integration.
Specific results which have been worked out by various techniques are collected in the list of integrals.
Approximation of definite integrals
Definite integrals may be approximated using several methods. One popular method, called the rectangle method or the trapezoidal rule, relies on dividing the function into a series of rectangles and finding the sum. Another well-known method is Simpson's rule.
Some integrals cannot be found exactly, and others are so complex that finding the exact answer would be extremely time-consuming or computationally-intensive. Approximation, however, is a process which relies only on variable substitution, multiplication, addition, and division. It can be done éasily and quickly by modérn graphing calculators and computers. Many réal-world applications of calculus rely on integral approximation because of the complexity of formulas and unnecessary nature of an exact answer.
Integrals and computerized algebra systems
Many professionals, educators, and students now use computerized algebra systems to maké difficult (or simply tedious) algebra and calculus problems éasier. The design of such a computer algebra system is nontrivial as systematic methods of antidifferentiation are difficult to formulate.
One difficulty is that it is not always possible to find "nice formulae" for antiderivatives. For instance, there is a (nontrivial) proof that there is no nice function (e.g., involving sin, cos, exp, polynomials, roots and so on) whose derivative is exp(-x2). As such, computerized algebra systems have no hope of being able to find an antiderivative for this particular function. Unfortunately, functions that have nice antiderivatives are the exception. If one writes a large random expression involving exponentials and polynomials, the odds are almost nil that it will have an antiderivative. (This statement can be made formal, but it is difficult to do so.)
One of the difficulties is to decide what set of functions to use as building blocks for antiderivatives. Usually, we need a set of antiderivatives closed under, say, multiplication and composition. This set of antiderivatives should also include polynomials, perhaps quotients, exponentials, logarithms, sines and cosines. The Risch-Norman algorithm is able to compute any integral of such a shape; that is, if the antiderivative involves polynomials, sines, cosines, etc..., the Risch-Norman algorithm will be able to compute it. Extended versions of this algorithm are implemented in Mathematica and Maple computer algebra system.
Some special integrands occur often enough to warrant special study. In particular, it may be useful to have, in the set of antiderivatives, the special functions of physics (like the Legendre functions, the Hypergeometric function, fungsi gamma jeung saterusna.) Extending the Risch-Norman algorithm so that it includes these functions is possible but challenging.
Most humans are not able to integrate such general formulae, so in a sense computers are more skilled at integrating highly complicated formulae. On the other hand, very complex formulae are unlikely to have closed-form antiderivatives, so this advantage is dubious.
Bantarujeg, Majalengka
Bantarujeg nyaéta hiji kacamatan di Kabupatén Majalengka, Propinsi Jawa Kulon, Indonésia.
Integral
Improper integrals
Not all integrals can be evaluated using a single limit process. An integral which can only be evaluated by considering it as the limit of integrals on successively larger and larger integrals is called an improper integral. Improper integrals usually turn up when the range of the function is infinite or, in the case of the Riemann integral, when the domain is infinite. One common example of an improper integral is the Cauchy principal value.
Definitions of the integral
The most important integrals are the Riemann integral and the Lebesgue integral. The Riemann integral was créated by Bernhard Riemann and was the first rigorous definition of the integral. The Lebesgue integral was créated by Henri Lebesgue to integrate a wider class of functions and to prove very strong theorems about interchanging limits and integrals.
Maniis, Cingambul, Majalengka
Sajarah
1. Sejarah Desa Maniis
2. Tokoh Masyarakat
Profil Pamaréntahan
Desa Maniis ayeuna dipingpin ku kuwu nu katelah Bapa Dadang Suganda nu tos calik dina korsi kapamingpinan nana salami 5 taun ti kawit taun 2004. Salami mingpin Desa Maniis tos loba tapak anu ditinggalkeun mangrupa pangwangunan jeung sistem pamarentahan anu luyu tur bener. ngaran kuring amin bin YUNUS alamat tangtos jelas nyaéta desa maniis tea,anu tos dinamian kukolot urang sadaya abi nuhunken barokah ti sesepuh atanapi kokolot urang sadaya mugi se,ur barokah kanggo anak incuna nu linggih di desa maniis
Géografis
Kaayaan Desa Maniis aya dibagean kulon Kecamatan Cingambul nu berbatesan jeung Desa Cidadap jeung Desa Rawa di beulah kaler, beulah wetan Desa Nagarakembang beulah kidul Kabupaten Ciamis jeung beulah kulon Desa Cintaasih. Temperatur suhu antara 20 - 250'C nu kaayaan tofografi na loba lamping jeung bergelombang nu luhur na nepi ka 850 Mdpl. Curah hujan na rata-rata 2647 mm per taun, bulan baseuh na 7 - 8 bulan.
By Chandry MM
Pakebonan
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Integral
Definitions of the integral
Although the Riemann and Lebesgue integrals are the most important ones, a number of others exist, including but not limited to:
Nagarakembang, Cingambul, Majalengka
Nagarakembang nyaéta salah sahiji désa di kacamatan Cingambul, Kabupatén Majalengka, Propinsi Jawa Barat, Indonésia.
Medan Barat, Médan
Medan Barat nyaéta salah sahiji kacamatan di Kota Médan, Propinsi Sumatra Kalér, Indonésia.
SMAN 62 Jakarta
SMAN 62 Jakarta nyaéta Sakola Menengah Atas Negeri anu aya di Kota Jakarta Timur. Alamat lengkepna di Jl. Raya Bogor Km.20, Kalurahan/Désa Kramat Jati Kacamatan Kramat Jati, Jakarta Timur, DKI Jakarta, kalawan nomor NPSN 20103306.
Negeri Dolok, Dolok Panribuan, Simalungun
Negeri Dolok nyaéta salah sahiji Désa di kacamatan Dolok Panribuan, Kabupatén Simalungun, Propinsi Sumatra Kalér, Indonésia.
Galaksi
Galaksi nyaéta sistim wates gravitasi nu kacida gedéna tina perbéntangan, gas jeung kebul antarbéntang, plasma jeung (meureun) bahan poék nu teu katempo (unseen dark matter). Galaksi umumna ngandung sapuluh juta nepi ka samiliar (107 nepi ka 1012) béntang, nu sakabéhna ngorbit ka puseur gravitasi nu sarua. In addition to single stars and a tenuous interstellar medium, most galaxies contain a large number of multiple star systems and star clusters as well as various types of nebulae. Most galaxies are several thousand to several hundred thousand light years in diaméter and are usually separated from one another by distances on the order of millions of light yéars.
Étimologi
The word galaxy derives from the Greek term for our own galaxy, galaxias (γαλαξίας) or kyklos galaktikos méaning "milky circle" for the system’s appéarance in the sky. In Greek mythology, Zeus placed his son by a mortal woman, the infant Hercules, on Hera's bréast as she was asleep, so that the baby would drink her divine milk and thus become immortal. Hera woke up while bréastfeeding, and réalized that she was nursing an unknown baby: she pushed the baby away and a jet of her milk sprayed the night sky.
When astronomers speculated that certain objects previously classified as spiral nebulae were actually vast congeries of stars, this was called the "island universe theory"; but this was an obvious misnomer, since universe méans everything there is. Consequently, this term fell into disuse, replaced by applying the term galaxy generically to all such bodies.
Sajarah observasi
This account of the history of the investigation of our own and other galaxies is largely taken from James Binney and Michael Merrifield: Galactic astronomy.
In 1610, Galileo Galilei used a telescope to study the bright band on the night sky known as the Milky Way and discovered that it was composed of a huge number of faint stars. In a tréatise in 1755, Immanuel Kant, drawing on éarlier work by Thomas Wright, speculated (correctly) that the Galaxy might be a rotating body of a huge number of stars, held together by gravitational forces akin to the solar system but on much larger scales. The resulting disk of stars would be seen as a band on the sky from our perspective inside the disk. Kant also conjectured that some of the nebulae visible in the night sky might be separate galaxies.
The first attempt to describe the shape of the Milky Way and the position of Sol within it was carried out by William Herschel in 1785 by carefully counting the number of stars in different regions of the sky. Using a refined approach, Kapteyn in 1920 arrived at the picture of a small (diaméter ~15 kiloparsecs) ellipsoid galaxy with Sol close to the center. A different method by Harlow Shapley based on the cataloging of globular clusters léad to a radically different picture: a flat disk with diaméter ~70 kiloparsecs and Sol far from the center. Both analyses failed to take into account the absorption of light by interstellar dust present in the galactic plane; once Robert Julius Trumpler had quantified this effect in 1930 by studying open clusters, the present picture of our galaxy as described above emerged.
In 1944, Hendrik van de Hulst predicted microwave radiation at a wavelength of 21 cm, resulting from interstellar atomic hydrogen gas; this radiation was observed in 1951. This radiation allowed for much improved study of the Galaxy, since it is not affected by dust absorption and its doppler shift can be used to map the motion of the gas in the Galaxy. These observations led to the postulation of a rotating bar structure in the center of the Galaxy. With improved radio telescopes, hydrogen gas could also be traced in other galaxies. In the 1970s it was discovered in Vera Rubin's study of the rotation speed of gas in galaxies that the total visible mass (from stars and gas) does not properly account for the speed of the rotating gas. This galaxy rotation problem is thought to be explained by the presence of large quantities of unseen dark matter.
Beginning in the 1990s, the Hubble Space Telescope yielded improved observations. Among other things, it established that the missing dark matter in our galaxy cannot solely consist of inherently faint and small stars. The Hubble Deep Field, an extremely long exposure of a relatively empty part of the sky, provided evidence that there are about one hundred and seventy-five billion galaxies in the universe. Improved technology in detecting the spectra invisible to humans (radio telescopes, infra-red cameras, x-ray telescopes), allow detection of other galaxies that are not detected by Hubble. Particularly, galaxy surveys in the zone of avoidance (the region of the sky blocked by the Milky Way) have revéaled a number of new galaxies.
Rupa-rupa galaksi
Galaxies come in three main types: ellipticals, spirals, and irregulars. A slightly more extensive description of galaxy types based on their appéarance is given by the Hubble sequence. Since the Hubble sequence is entirely based upon visual morphological type, it may miss certain important characteristics of galaxies such as star formation rate (in starburst galaxies) or activity in the core (in active galaxies).
Our own galaxy, the Milky Way, sometimes simply called the Galaxy (with uppercase), is a large disk-shaped barred spiral galaxy about 30 kiloparsecs or a hundred light millennia in diaméter and three light millennia in thickness. It contains about 3×1011 (three hundred billion) stars and has a total mass of about 6×1011 (six hundred billion) times the mass of Sol.
In spiral galaxies, the spiral arms have the shape of approximate logarithmic spirals, a pattern that can be théoretically shown to result from a disturbance in a uniformly rotating mass of stars. Like the stars, the spiral arms also rotate around the center, but they do so with constant angular velocity. That méans that stars pass in and out of spiral arms. The spiral arms are thought to be aréas of high density or density waves. As stars move into an arm, they slow down, thus créating a higher density; this is akin to a "wave" of slowdowns moving along a highway full of moving cars. The arms are visible because the high density facilitates star formation and they therefore harbor many bright and young stars.
Despite the prominence of large elliptical and spiral galaxies, most galaxies in the universe appéar to be dwarf galaxies. These tiny galaxies are about one hundred times smaller than the Milky Way, containing only a few billion stars. Many dwarf galaxies may orbit a single larger galaxy; the Milky Way has at léast a dozen such satellites. Dwarf galaxies may also be classified as elliptical, spiral or irregular. Since small dwarf ellipticals béar little resemblance to large ellipticals, they are often called dwarf spheroidal galaxies instéad.
Galaksi aktif
A portion of the galaxies we can observe are classified as active. That is, a significant portion of the total energy output from the galaxy is emitted by a source other than the stars, dust and interstellar medium. The standard modél for such active galactic nucleus is based upon energy generation from matter falling into a supermassive black hole at the core region.
Galaxies that emit high-energy radiation in the form of x-rays are classified as Seyfert galaxies, quasars and blazars. Active galaxies that emit radio frequencies from relativistic jets erupting from the core are classified as Radio galaxies. A unified modél of these types of active galaxies explains their differences based on the viewing angle of the observer.
Struktur skala gedé
Very few galaxies exist by themselves; these are known as field galaxies. Most galaxies are gravitationally bound to a number of other galaxies. Structures containing up to about 50 galaxies are called groups of galaxies, and larger structures containing many thousands of galaxies packed into an aréa a few megaparsecs across are called clusters. Clusters of galaxies are often dominated by a single giant elliptical galaxy, which over time tidally destroys its satellite galaxies and adds their mass to its own. Superclusters are giant collections containing tens of thousands of galaxies, found in clusters, groups and sometimes individually; at the supercluster scale, galaxies are arranged into sheets and filaments surrounding vast empty voids. Above this scale, the universe appéars to be isotropic and homogeneous.
Our galaxy is a member of the Local Group, which it dominates together with the Andromeda Galaxy; overall the Local Group contains about thirty galaxies in a space about one megaparsec across. The Local Group is part of the Virgo Supercluster, which is dominated by the Virgo Cluster (of which our Galaxy is not a member).
Silaga Laga, Dolok Sanggul, Humbang Hasundutan
Silaga Laga nyaéta salah sahiji Désa di kacamatan Dolok Sanggul, Kabupatén Humbang Hasundutan, Propinsi Sumatra Kalér, Indonésia.
PuloTeungoh Ranto P., Meureubo, Aceh Barat
PuloTeungoh Ranto P. nyaéta salah sahiji Gampong di kacamatan Meureubo, Kabupatén Aceh Barat, Propinsi Acéh, Indonésia.
(436037) 2009 NJ
Ari 2009 NJ mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.659, sedengkeun magnitudo mutlakna 18.6. Ari nu jadi référénsina mah nyaéta MPO�408966.
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.
2009 FX4
Ari 2009 FX4 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.320, sedengkeun magnitudo mutlakna 25.4. Ari nu jadi référénsina mah nyaéta MPO�156199.
PuloTeungoh Ranto P., Meureubo, Aceh Barat
PuloTeungoh Ranto P., Meureubo, Aceh Barat
2009 FX4
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.
Sengkati Kecil, Mersam, Batanghari
Sengkati Kecil nyaéta salah sahiji désa di kacamatan Mersam, Kabupatén Batanghari, Propinsi Jambi, Indonésia.
Galaksi
Formasi jeung évolusi galaksi
The study of galactic formation and evolution attempts to answer questions regarding how galaxies formed and their evolutionary path over the history of the universe. Some théories on this field have now become widely accepted, but it is still an active aréa of study in astrophysics.
Formasi
The method of galactic formation is a major open question in astronomy. Théories may be divided into two categories: top-down and bottom-up. In top-down théories such as the Eggen–Lynden-Bell–Sandage (ELS) modél, protogalaxies form in a large-scale simultanéous collapse lasting about one hundred million yéars. In bottom-up théories such as the Séarle-Zinn (SZ) modél, globular clusters form first, and then a number of such bodies accrete to form a larger galaxy. modérn théories must be modified to account for the probable presence of large dark matter halos. A sketch of a galactic formation modél follows.
Shortly after recombination, baryonic matter begins to condense around cold dark matter halos. Zero-metal high-velocity halo stars (called Population III stars) are the first to develop around a protogalaxy as it starts to contract. These huge stars quickly supernova, reléasing héavy elements into the interstellar medium. Within the next billion yéars, globular clusters, the central supermassive black hole and galactic bulge of metal-poor Population II stars form. Within two billion yéars, the remaining material settles into a galactic disk. The galaxy will continue to absorb infalling material from high velocity clouds and dwarf galaxies throughout its life; the cycle of stellar birth and déath will incréase the abundance of héavy elements, eventually allowing the formation of planets.
Probably the oldest galaxy yet found, IOK-1, was discovered in September 2006 by Masanori Iye at National Astronomical Observatory of Japan using the Subaru Telescope in Hawaii. Its emission of Lyman alpha radiation has a redshift of 6.96, making it thirteen billion yéars old. While some scientists have claimed other objects (such as Abell 1835 IR1916) to be even older, the IOK-1's age and composition have been more reliably established.
The existence of such old protogalaxies suggests that they must have grown in the so-called "Dark Ages" (before the first generation of stars) from anisotropic irregularities present during the éra of recombination, some three hundred thousand yéars after the Big Bang. Such irregularities of the right scale were observed using the Wilkinson Microwave Anisotropy Probe (WMAP) in 2003.
More evidence for this modél of galactic formation comes from detection of ancient Population III stars. The giant star, HE0107-5240, discovered in 2002 by reséarchers at the University of Hamburg, is believed to be the oldest yet discovered star in the Milky Way, since unlike younger stars, it is virtually metal-free. (See .) Since then, other very old stars (like HE 1327) have also been found.
Évolusi
Studies show that the Milky Way Galaxy is moving towards the néarby Andromeda Galaxy at about 130 km/s, and depending upon the lateral movements, the two may collide in about five to six billion yéars. Such galaxy collisions are fairly common. Given the distances between the stars, the gréat majority of stellar systems in colliding galaxies will be unaffected. However, gravitational stripping of the interstellar gas and dust that makes up the spiral arms will produce a long train of stars, similar to that seen in NGC 250 or the Antennae Galaxies.
Although the Milky Way has never collided with a galaxy as large as Andromeda before, evidence of past collisions of the Milky Way with smaller dwarf galaxies is incréasing.
Spiral galaxies, like the Milky Way, only produce new generations of stars as long as they continue to have dense molecular clouds of interstellar hydrogen in their spiral arms. Elliptical galaxies are alréady largely devoid of this gas and so form no new stars. However, the supply of star-forming material is finite; as stars convert hydrogen into héavier elements, fewer stars will form.
After the end of stellar formation in under one hundred billion yéars, the "stellar age" will come to an end after about ten trillion to one hundred trillion yéars (1013–1014 yéars), as the smallest longest-lived stars in our astrosphere, tiny red dwarfs begin to fade. At the end of the stellar age galaxies will comprise compact objects: brown dwarfs, black dwarfs, cooling white dwarfs, neutron stars, and black holes. Eventually, as a result of gravitational relaxation, all stars will either fall into the central supermassive black hole of the galaxies, or be flung into the depths of intergalactic space as a result of collisions.
Biologi galaktik
Biology as we know it is currently assumed to exist only around single, third-generation G-type stars in the middle regions of the spiral arms of spiral galaxies, like the sun. Elliptical galaxies, produced as a result of many galactic collisions, quickly lose their clouds of interstellar hydrogen gas, and cannot maké new generations of stars. Irregular galaxies have few elderly stars and thus seem to have low concentrations of the héavier elements on which éarth-like biology depends. Even within spiral galaxies biology as we know it would appéar to be limited to the middle réaches of the spiral arm, as in the galactic halo or outer spiral arms héavier elements are in short supply, whilst in the gas clouds around the galactic centre héavier elements are in concentrations too high, and interstellar interactions are too frequent to allow éarth-sized planets to form in stable circular orbits around their stars.
Pamaheg
Rék daék teu daék ogé pamaheg mah bakal tetep aya di jeroning diri jelema nu hirup, mangrupa carana Gusti Nu Ngersakeun nu ngawasa ka sakabéh kaayaan, kajadian, jeung kahirupan, bari jeung Gusti mah teu ngabutuhkeun bantuan nanaon atawa bantuan sasaha. ku kituna ceuk ajaran Jati Buhun mah aturan ti Gusti nu saenyana téh teu kudu diajarkeun ti luar diri urang, da manuk ogé bisa nyayang, nyingleumleum, jeung ngurus anakna teu kudu diajarkeun ti luar dirina, tapi cukup ku éling kana dirina sorangan.
Pamaheg téh mangrupa kecap Buhun titinggalan ti pamuunan (karuhun buhun) nu dipaké kénéh nepi ka ayeuna ku ajaran Ajaran Jati Buhun.
Pamaheg Nu Aya Dina Diri Jelema
Pamaheg nu aya dina diri jelema meni kacida ahéngna tur ngabogaan mangrupa-rupa aturan ti Gusti nu saenyana-enyana Gusti jang jelema, jeung nu aya di sasatoan mah teu saahéng siga nu dipikaboga ku jelema. Bagéan na téh nyaéta:
Ari sésana mah nyaéta Pamaheg mangrupa kahayang nu sarua siga Pamaheg nu dipikaboga ku sasatoan
Kumatak kitu jelema dijurukeun téh tah jadi jelema nu éling kana dirina sorangan, ngabogaan pandekan, jeung paduli ka sasama, tapi pengaruh goté nu daratang ti luareun dirina geus ngajadikeun éta jelema jadi teu éling kana dirina sorangan, nepi ka éta jelema téh jadi leuwih bahaya ti batan buaya, leuwih jahat ti batan ajag, jeung leuwih galak ti batan singa. ku kituna pépéling diri téh kacida pentingna, supaya jelema balik deui ka laku lampahna salaku jelema.
Pamaheg téh mun ceuk Malayuna mah meureunan "naluri", harti ti kecap naluri ampir sarua jeung pamaheg di mana naluri ceuk kamus besar bahasa Indonesia nyaéta dorongan hati atau nafsu yang dibawa sejak lahir; pembawaan alami yang tidak disadari mendorong untuk berbuat sesuatu.
Gisting Bawah, Gisting, Tanggamus
Gisting Bawah nyaéta salah sahiji Désa di kacamatan Gisting, Kabupatén Tanggamus, Propinsi Sumatra Kalér, Indonésia.
Gisting Atas, Gisting, Tanggamus
Gisting Atas nyaéta salah sahiji Désa di kacamatan Gisting, Kabupatén Tanggamus, Propinsi Sumatra Kalér, Indonésia.
Geresik, Ciawigebang, Kuningan
Geresik nyaéta salah sahiji désa di kacamatan Ciawigebang, Kabupatén Kuningan, Propinsi Jawa Barat, Indonésia.
Meuraxa, Banda Acéh
Meuraxa nyaéta salah sahiji kacamatan di Kota Banda Acéh, Propinsi Acéh, Indonésia.
Linung Bale, Timang gajah, Bener Meriah
Linung Bale nyaéta salah sahiji Gampong di kacamatan Timang gajah, Kabupatén Bener Meriah, Propinsi Acéh, Indonésia.
Linung Bale, Timang gajah, Bener Meriah
Medan Timur, Médan
Medan Timur nyaéta salah sahiji kacamatan di Kota Médan, Propinsi Sumatra Kalér, Indonésia.
Cigasong, Majalengka
Cigasong nyaéta hiji kacamatan di Kabupatén Majalengka, Propinsi Jawa Kulon, Indonésia.
Panakawan
Panakawan nyaéta ngaran umum dina peran panglayan jeung nu ngabdi ka susuhunanana dina carita-carita pawayangan, carita wawacan, jeung sandiwara. Ku kituna, panakawan téh mideng ogé disebut palaku tambahan (kadua).
Karakter
Dina carita panakawan biasana ngarangkep jadi gandék atawa pangiring palaku utama (protagonis). Dina pagelaran wayang jeung sandiwara lian ti jadi gandék, ngarangkep jadi bodor, nyiptakeun kaayaan nu guyon, heureuy, jeung lulucon. Tata paripolahna jeung tatabarangpakéna diluyukeun jeung pungsina.
Ari dina wawacan mah nu jadi panakawan téh aya nu jadi palaku utama nu karakterna aya dina kaayaan sangsara, kasilihkeun, kadungsang-dungsang, jeung dununganana nyahoeunna téh engké sabada aya kasempetan némbongkeun wewesénna. Panakawan dina Wayang Golék téh nyaéta semar, cépot, dawala, jeung garéng. Kabéhanana ogé masih kénéh sakulawarga.
2012 CN2
Ari 2012 CN2 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.212, sedengkeun magnitudo mutlakna 25.4. Ari nu jadi référénsina mah nyaéta MPO 223082.
2008 TK157
Ari 2008 TK157 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.516, sedengkeun magnitudo mutlakna 20.6. Ari nu jadi référénsina mah nyaéta MPO 221126.
Selamanik, Cipaku, Ciamis
Selamanik nyaéta salah sahiji désa di kacamatan Cipaku, Kabupatén Ciamis, Propinsi Jawa Barat, Indonésia.
2008 TK157
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.
2014 QX266
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.
2017 CX1
Ari 2017 CX1 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.293, sedengkeun magnitudo mutlakna 28.2. Ari nu jadi référénsina mah nyaéta MPO�399835.
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.
2012 BS23
Ari 2012 BS23 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.579, sedengkeun magnitudo mutlakna 21.4. Ari nu jadi référénsina mah nyaéta MPO�234799.
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.
SMAN 93 Jakarta
SMAN 93 Jakarta nyaéta Sakola Menengah Atas Negeri anu aya di Kota Jakarta Timur. Alamat lengkepna di Jl. Raya Bogor Komp. Paswalpres, Kalurahan/Désa Kampung Tengah Kacamatan Kramat Jati, Jakarta Timur, DKI Jakarta, kalawan nomor NPSN 20103258.
(153842) 2001 XT30
Ari 2001 XT30 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.569, sedengkeun magnitudo mutlakna 16.7. Ari nu jadi référénsina mah nyaéta MPO 376085.
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.
2012 CP2
Ari 2012 CP2 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.397, sedengkeun magnitudo mutlakna 20.5. Ari nu jadi référénsina mah nyaéta MPO 234427.
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.
Rawa, Cingambul, Majalengka
Rawa nyaéta salah sahiji désa di kacamatan Cingambul, Kabupatén Majalengka, Propinsi Jawa Barat, Indonésia.
Paya Baro Ranto P, Meureubo, Aceh Barat
Paya Baro Ranto P nyaéta salah sahiji Gampong di kacamatan Meureubo, Kabupatén Aceh Barat, Propinsi Acéh, Indonésia.
2005 CL7
Ari 2005 CL7 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.101, sedengkeun magnitudo mutlakna 19.7. Ari nu jadi référénsina mah nyaéta MPO�409298.
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.
2002 HE8
Ari 2002 HE8 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.124, sedengkeun magnitudo mutlakna 20.5. Ari nu jadi référénsina mah nyaéta MPO 322114.
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.
Sidokaton, Gisting, Tanggamus
Sidokaton nyaéta salah sahiji Désa di kacamatan Gisting, Kabupatén Tanggamus, Propinsi Sumatra Kalér, Indonésia.
SMAS Miftahul Huda
SMAS Miftahul Huda nyaéta Sakola Menengah Atas Swasta anu aya di Kabupatén Cianjur. Alamat lengkepna di Jl. Raya Leles Km. 13, Kalurahan/Désa Mandalawangi Kacamatan Lélés, Kabupatén Cianjur, Jawa Kulon kalawan nomor NPSN 20203705.
Sengkati Gedang, Mersam, Batanghari
Sengkati Gedang nyaéta salah sahiji désa di kacamatan Mersam, Kabupatén Batanghari, Propinsi Jambi, Indonésia.
Berang-berang raksasa
Berang-berang raksasa nyaéta sato kulawarga séro pangbadagna di Amérika Kalér nu hirup dina Jaman És panungtungan, kiwari mah geus punah. Aya dua spésiés berang-berang raksasa anu kapanggih tina genus Castoroides, nyaéta Castoroides ohioensis jeung Castoroides leiseyorum.
Fosil
Fosil munggaran anu kungsi kacatet kapanggih nyaéta di urut rawa deukeut Nashport, Ohio kungsi didadarkeun, sanajan teu dingaranan ku S.R. Hildreth taun 1837. Sataun ti harita saurang ahli géologi J.W. Foster nyebutkeun ieu spésimén téh minangka Castoroides ohioensis dina publikasina.
Fosil berang-berang raksasa nu pangkolotna nyaéta tina spésiés Castoroides leiseyorum ti Florida, Amérika Serikat umurna 1,4 juta taun. Di Kanada, fosil Castoroides ohioensis, mungkin kira-kira ti jaman és pertengahan (130.000 taun ka tukang), kapanggih di Toronto, Ontario, jeung di Cekungan Old Crow di Yukon. Fosilna réa pisan kapanggih di kiduleun Great Lakes, nu kiwari asup kana wewengkon Indiana jeung Ilinois, Amérika Serikat. Upama dibandingkeun jeung mammoth, biruang guha, jeung bison purba anu gambarna kapanggih dina jero guha dina jaman batu di Eropa, berang-berang raksasa mah teu kapanggih gambarna.
Dedegan Awak
Panjang awakna 1,5 m jeung beuratna kira-kira 60-100 kg, sagedé biruang hideung. Sakumaha ngaranna, berang-berang raksasa katémbongna mah méh sarupa jeung berang-berang modéren, tapi leuwih gedé. Mun dibandingkeun mah suku tukangna leuwih gedé. Wangun buntutna mah can tangtu, naha sarua saperti berang-berang modéren atawa henteu, sabab buntutna dijieun tina lapisan ipis, anu leungit dina fosilna lantaran buruk. Lantaran alasan ieu, urang ngan bisa ngira-ngira yén sukuna boga selaput (lambaran kulit di antara ramo siga dina éntog).
Panjang buntutna kira-kira 65cm, rubakna 12 cm lebah handap, jeung 14 cm rubak lebah puhuna. Sakumaha biasana wangun buntut berang-berang, ngan leuwih ramping. Sanajan hadé pisan adaptasina pikeun ngojay, suku tukangna mah kawilang pondok. Lamun nilik tina beurat awakna, mangka kamampuhna pikeun narabas wewengkon sabudeureunna kamungkinan teu pati lega.
Huntuna ogé béda deuih. Huntu paranti ngeureut dina berang-berang raksara panjangna bisa nepi ka 15 cm. Huntuna rada nonjol dina sisi luar, jeung tungtungna buleud, medu, teu saperti huntu berang-berang modérn anu wangunna saperti pahat. Huntu pipina méh sarua jeung huntu capybara nu kapanggih mangsa kiwari, nyaéta mibanda pola énamél wangun S dina bagian luar huntu panggayemna. Ieu wangun téh bukti adaptasi anu hadé pikeun ngagiling tutuwuhan anu ngawangun pola hakaneun ieu sato. Sanajan réa sasaruaanana jeung berang-berang modéren, berang-berang raksasa mah lain kualwarga deukeut tina berang-berang modéren.
Habitat
Berang-berang raksasa mungkin leuwih milih hirup di dano atawa kubangan anu diwatesasan ku rawa saperti dina habitat asalna, sabab fosilna mindeng kapanggih di urut rawa-rawa jaman kuno. lantaran habitatna kitu, ieu sato kaasup kana sato sémi aquatik. Mungkin beuki ngurananna lega wewengkon rawa nu kitu téh beuki gancang ngurangan dina jamanna alatan parobahan iklim, patali jeung nguranganna kamampuh pikeun nyieun bendungan jeung kurang bisa adaptasi kana parobahan lingkunganana.
Hasil panalungtikan isotop tina fosil tulang berang-berang raksasa nuduhkeun rupa-rupa hakaneun anu patali jeung tutuwuhan kai, sarta tutuwuhan nu hirup dina cai. Iwal ti éta kapanggih pituduh yén ieu sato teu nuaran tangkal pikeun nyieun bendungan dina jaman és harita. Hartina, ku teu mampuhna ieu sato pikeun nyieun bendungan téh bisa jadi salah sahiji balukar kana kapunahanana.
Kapunahan
Bukti tina fosil nu kapanggih némbongkeun yén berang-berang raksasa kira-kira ahir Jaman És, kurang leuwih 10.000 taun ka tukang. Lantaran kungsi hirup babarengan jeung manusa munggaran di Amérika Kalér, sanajan euweuh bukti yén ieu sato jadi bahan boroan. Lantaran iklim beuki panas, wewengkon rawa jeung hakaneunna ngurangan. Berang-berang raksasa mungkin punah ku sabab kalaparan.
Simpang Tiga, Langkahan, Aceh Utara
Simpang Tiga nyaéta salah sahiji Gampong di kacamatan Langkahan, Kabupatén Aceh Utara, Propinsi Acéh, Indonésia.
Cikijing, Majalengka
Cikijing nyaéta hiji kacamatan di Kabupatén Majalengka, Propinsi Jawa Kulon, Indonésia.
Pasirwaru, Mancak, Sérang
Pasirwaru nyaéta salasahiji kalurahan di Kacamatan Mancak, Sérang, Propinsi Banten, Indonésia.
TPI TV
TPI TV nyaéta MNC stasion TV televisi di Indonesia, (16 April 2018)
Dolok Tomuan, Dolok Panribuan, Simalungun
Dolok Tomuan nyaéta salah sahiji Désa di kacamatan Dolok Panribuan, Kabupatén Simalungun, Propinsi Sumatra Kalér, Indonésia.
Dolok Parmonangan, Dolok Panribuan, Simalungun
Dolok Parmonangan nyaéta salah sahiji Désa di kacamatan Dolok Panribuan, Kabupatén Simalungun, Propinsi Sumatra Kalér, Indonésia.
2014 HP184
Ari 2014 HP184 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.386, sedengkeun magnitudo mutlakna 21.0. Ari nu jadi référénsina mah nyaéta MPO�293432.
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.
Medan Perjuangan, Médan
Medan Perjuangan nyaéta salah sahiji kacamatan di Kota Médan, Propinsi Sumatra Kalér, Indonésia.
Kadurama, Ciawigebang, Kuningan
Kadurama nyaéta salah sahiji désa di kacamatan Ciawigebang, Kabupatén Kuningan, Propinsi Jawa Barat, Indonésia.
Sedaraja, Cingambul, Majalengka
Sedaraja nyaéta salah sahiji désa di kacamatan Cingambul, Kabupatén Majalengka, Propinsi Jawa Barat, Indonésia.
Sukawening, Cipaku, Ciamis
Sukawening nyaéta salah sahiji désa di kacamatan Cipaku, Kabupatén Ciamis, Propinsi Jawa Barat, Indonésia.
Matang Rubek, Langkahan, Aceh Utara
Matang Rubek nyaéta salah sahiji Gampong di kacamatan Langkahan, Kabupatén Aceh Utara, Propinsi Acéh, Indonésia.
2016 EW27
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.
Landbaw, Gisting, Tanggamus
Landbaw nyaéta salah sahiji Désa di kacamatan Gisting, Kabupatén Tanggamus, Propinsi Sumatra Kalér, Indonésia.
Landbaw, Gisting, Tanggamus
Ranub Dong, Meureubo, Aceh Barat
Ranub Dong nyaéta salah sahiji Gampong di kacamatan Meureubo, Kabupatén Aceh Barat, Propinsi Acéh, Indonésia.
2014 QP266
Ari 2014 QP266 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.338, sedengkeun magnitudo mutlakna 19.8. Ari nu jadi référénsina mah nyaéta MPO 373557.
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.
Meureubo, Acéh Kulon
Meureubo nyaéta salah sahiji kacamatan di Kabupatén Acéh Kulon, Propinsi Acéh, Indonésia.
HSPA
High-Speed Packet Access (HSPA) mangrupa sakumpulan protokol telepon mobil anu ngalegakeun sarta ngaalusan unjuk gawé protokol UMTS nu aya kiwari. Kiwari geus aya dua standar pikeun HSPA nyaéta HSDPA jeung HSUPA. Standar HSPA satuluyna anu disebut HSOPA ayeuna keur dipigawé.
Ringkesan
Jumlah jaringan 3.5G komérsial - anu katelah ogé jaringan High-Speed Downlink Packet Access, atawa HSDPA, tumuwuh 69% dina taun 2007. Kiwari aya 166 jaringan HSDPA komérsial di 75 nagara. Tilu puluh dalapan jaringan tambahan rancanana rék diamparkeun, anu baris ngaronjatkeun jumlah jaringan HSDPA jadi 240 di 89 nagara. Jaringan HSDPA komérsial sumebar di Éropah Kulon (61 jaringan), Asia Kidulwétan (35), Éropah Wétan (34), Timur Tengah jeung Afrika (20), sarta Amérika jeung Karibia (16). Ampir dua pertilu (62%) jaringan HSDPA komérsial nu aya nyadiakeun laju downlink saeutikna sagancang 3.6Mbps, sedengkeun leuwih ti saperlimana (21%) nawarkeun laju downlink sagancang 7.2Mbps. .
Jaringan HSPA bisa diamparkeun maké software jaringan 3G nu aya kiwari tapi kudu ditingkatkeun kamampuhna, hasilna leuwih unggul batan WiMax anu merlukeun infrastruktur jaringan husus. Ngaronjatna panjualan terminal mobil nu bisa HSPA sarta subsidi anu dilakukeun ku operator pikeun biaya hardware ngabantu ngagerakkeun pasar 3.5G. .
2009 FW4
Ari 2009 FW4 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.568, sedengkeun magnitudo mutlakna 24.6. Ari nu jadi référénsina mah nyaéta MPO�156199.
HSPA
High Speed Downlink Packet Access (HSDPA)
HSDPA sacara téori nawarkeun paningkatan unjuk gawé down-link nepi ka 14.4 Mbit/s. Pamasangan jaringan nu aya kiwari nawarkeun nepi ka 7.2 Mbit/s dina sinyal down-link. Unjuk gawé laju sinyal up-link sagedé-gedéna 384 kbit/s.
Sosor Tambok, Dolok Sanggul, Humbang Hasundutan
Sosor Tambok nyaéta salah sahiji Désa di kacamatan Dolok Sanggul, Kabupatén Humbang Hasundutan, Propinsi Sumatra Kalér, Indonésia.
HSPA
High Speed Uplink Packet Access (HSUPA)
HSUPA nawarkeun unjuk gawé laju sinyal up-link nepi ka 5.76 Mbit/s sacara téoritis. Di Singapura, Starhub ngumumkeun layanan HSUPA 1.9 Mbit/s salaku bagian tina rancana anyar MaxMobile dina tanggal 1 Agustus 2007. Di Finlandia, Elisa ngumumkeun layanan HSUPA 1.4 Mbit/s dina tanggal 30 Agustus 2007 ka kota-kota gedé kalayan rancana pikeun nambahkeun éta layanan kana sakabéh jaringan 3G bogana dina waktu itungan bulan. .
2009 FW4
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.
Pantan Kemuning, Timang gajah, Bener Meriah
Pantan Kemuning nyaéta salah sahiji Gampong di kacamatan Timang gajah, Kabupatén Bener Meriah, Propinsi Acéh, Indonésia.
Pantan Kemuning, Timang gajah, Bener Meriah
2015 XA169
Ari 2015 XA169 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Apollo, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.413, sedengkeun magnitudo mutlakna 27.4. Ari nu jadi référénsina mah nyaéta MPO�358575.
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.
Mike Myers
Michael John "Mike" Myers mangrupa aktor lalaki, pelawak, sareng panulis skenario asal Kanada. Anjeunna janten kasohor nalika maén dina film utami sapertos Wayne's World, Austin Powers, Shrek jeung The Love Guru. Anjeunna lahir di Scarborough, Ontario. Anjeunna parantos damel di industri pilem ti saprak 1985.
Sengkati Baru, Mersam, Batanghari
Sengkati Baru nyaéta salah sahiji désa di kacamatan Mersam, Kabupatén Batanghari, Propinsi Jambi, Indonésia.
Tomiichi Murayama
Tomiichi Murayama (村山 富市 Murayama Tomiichi, babar 3 Maret 1924) salah saurang pulitikus Jepang nu jadi Perdana Mentri Jepang ka-81 ti tanggal 30 Juni 1994 nepi ka 11 Januari 1996. Murayama nyaéta katua Partai Sosial Demokrat Jepang (nepi ka taun 1996 Partai Sosialis Jepang) tur perdana mentri sosialis munggaran dina ampir 55 taun. Nu natrat nepi ka kiwari nyaéta pidatona dina "Pangemut-emut 50 taun ahir perang," eusi pidatone Jepang menta dihampura kasalahanna salila Perang Dunya II.
2008 TJ157
Ari 2008 TJ157 mangrupa hiji astéroid. Ieu asteroid téh bagéan tina astéroid Amor, anu nganjrek deukeut jeung marcapada. Ékséntrisitas orbit ieu astéroid kacatet gedéna 0.552, sedengkeun magnitudo mutlakna 21.0. Ari nu jadi référénsina mah nyaéta MPO 288463.
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.
Leubok Mane, Langkahan, Aceh Utara
Leubok Mane nyaéta salah sahiji Gampong di kacamatan Langkahan, Kabupatén Aceh Utara, Propinsi Acéh, Indonésia.
Raden Muhammad Mulyadi
Raden Muhammad Mulyadi nyaéta sajarawan kalahiran Bandung, 14 Pebruari 1969. Anjeunna aktip janten dosen sareng peneliti di Universitas Padjadjaran ogé salaku Ketua Program Studi Magister Ilmu Sejarah. Salian tina ngadosenan, anjeuna aktip naliti jeung nulis rupi-rupi tulisan. Aya dinu bentuk jurnal, artikel, ogé buku-buku sajarah margi anjeunna pokus dinu penelitian kasajarahan.
Teu cukup ngajar jeung naliti, Raden Muhammad Mulyadi seueur aktip dinu kagiatan organisasi. Di antarana PPSI (Perkumpulan Prodi Sejarah Seluruh Indonesia), nyaéta hiji organisasi anu didirikeun ku para sajarawan sa-Indonesia jang ngamunculkeun kaelmuan sajarah ti para pengajar jeung peneliti. Harita basa taun 2016 tepi ka 2018, Raden Muhammad Mulyadi nyekel Dipisi Penelitian jeung Publikasi.
Panalitian Jeung Publikasi Ilmiah
Jurnal Patanjala “Elmu Anyar: Syncretism In The Spreading Of Christianity In West Java From The Nineteenth To The Early Twenty Century” - taun 2019
Jurnal Patanjala “Polemik A. Hassan Dan Muchtar Luthfi Mengenai Paham Kebangsaan (1929-1935)” - taun 2018