The sun is actually a star of about medium size; it appears larger than the other stars because of its relative nearness to the earth. The earth's distance from the sun varies from 91,377,000 mi (147,053,000 km) at perihelion to 94,537,000 mi (152,138,000 km) at aphelion (see apsis). The mean distance is c.92,960,000 mi (149,591,000 km); this is taken as the astronomical unit (AU) of distance used for measuring distances within the solar system. The sun is approximately 865,400 mi (1,392,000 km) in diameter, and its volume is about 1,300,000 times that of the earth. Its mass is almost 700 times the total mass of all the bodies in the solar system and 332,000 times that of the earth. The sun's surface gravity is almost 28 times that of the earth; i.e., a body on the surface of the sun would weigh about 28 times its weight on earth. The density of the material composing the sun is about one fourth that of the earth; compared with water, the sun's average density is 1.41. At its center, the sun has a density of over 100 times that of water, a temperature of 10 to 20 million degrees Celsius, and a pressure of over 1 billion atmospheres.
Observations of sunspots and studies of the solar spectrum indicate that the sun rotates on its axis from east to west; because of its gaseous nature its rate of rotation varies somewhat with latitude, the speed being greatest (a period of almost 25 days) in the equatorial region and least at the poles (a period of about 35 days). The axis of the sun is inclined at an angle of about 7° to the plane of the ecliptic.
The bright surface of the sun is called the photosphere. Its temperature is about 6,000°C;. The photosphere appears darker near the edge (limb) of the sun's disk because of greater absorption of light by the sun's atmosphere in this area; this phenomenon is called limb darkening. During an eclipse of the sun the chromosphere and the corona (the outer layers of the sun's atmosphere) are observed. Also of interest is the high-speed, tenuous extension of the corona known as the solar wind.
The vast and continual production of solar energy cannot be attributed merely to combustion, to the gradual cooling of a hot body, to the fall of meteorites into the sun, or to gradual shrinkage with transformation of potential energy into heat (a theory proposed by Helmholtz). The theory of relativity with its implication of the equivalence of mass and energy led to the assumption that energy stored in the atoms constituting the sun's gases is constantly being released by conversion of some of the masses of the atom's nuclei during nuclear transmutations (see nuclear energy). H. A. Bethe proposed a cycle of nuclear reactions known as the carbon cycle, or CNO bi-cycle, to account for the nuclear changes. In this cycle carbon acts much as a catalyst, while hydrogen is transformed by a series of reactions into helium and large amounts of high-energy gamma radiation are released. It is now thought that the so-called proton-proton process is a more important energy source; this process begins with the collision of two protons and ends with the production of helium, while gamma radiation is released throughout.
See nucleosynthesis; stellar evolution.
By means of the spectroscope much has been learned about the composition of the sun. There are numerous dark lines of varying widths in the solar spectrum. These were first intensively studied by Joseph Fraunhofer and are commonly known by his name. From a study of the lines the chemical composition of the sun is determined on the basis of the discovery by Kirchhoff that the dark lines correspond in position to the bright lines characteristic of the spectra produced by elements in the laboratory. The darkness of the lines in the sun's spectrum is attributed to the presence of a slightly cooler layer of gases above the photosphere, known as the reversing layer, which absorbs selectively the light of the photosphere and thus causes dark lines instead of bright ones to be observed through the spectroscope. By comparison of the sun's spectrum with laboratory spectra of incandescent elements, most of the elements known on earth have been identified in the sun's atmosphere.
Beyond the red portion of the visible solar spectrum is the infrared spectrum; for the study of these heat rays S. P. Langley invented the bolometer, a highly sensitive electrical device for measuring temperature. Solar heat and energy are measured by an instrument called the pyrheliometer. Other instruments devised especially for the study of the sun are the coronagraph and the spectroheliograph. These instruments have revealed a number of interesting phenomena occurring during the periods of solar activity associated with sunspots, e.g., faculae, plages (flocculi), prominences, and flares.
Without the heat and light of the sun, life as we know it could not exist on the earth. Since solar energy is used by green plants in the process of photosynthesis, the sun is the ultimate source of the energy stored both in food and fossil fuels. Solar heating sets up convection currents, and thus is the source of the energy of moving air. Falling rain also owes its energy to the sun because of the relation of solar radiation to the water cycle.
See K. Hufbauer, Exploring the Sun: Solar Science since Galileo (1993); R. Krippenhahn, Discovering the Secrets of the Sun (1994); K. J. H. Phillips, Guide to the Sun (1995); P. O. Taylor, Beginners Guide to the Sun (1996); S. T. Suess and B. T. Tsurutani, ed., From the Sun: Auroras, Magnetic Storms, Solar Flares, Cosmic Rays (1998).
Sun fled China in 1895, after an abortive revolt, and then toured the world several times to enlist the aid of overseas Chinese in financing his activities. In that period he made an intensive study of Western political and social theory and was deeply impressed with the writings of Karl Marx and Henry George. Sun organized (1905) a revolutionary league, the T'ung Meng Hui, in Japan and gradually perfected his political conceptions, which were based on the Three People's Principles: nationalism, democracy, and the people's livelihood. Revolution erupted in China, and Sun was elected provisional president of the Chinese republic in Dec., 1911, but two months later he resigned in favor of Yüan Shih-kai. Later, when Sung Chiao-jen transformed the T'ung Meng Hui into a federated political party called the Kuomintang, Sun served as its director.
Meanwhile, opposition developed to Yüan's dictatorial methods; in 1913 Sun led an unsuccessful revolt against Yüan, and he was forced to seek asylum in Japan, where he reorganized the Kuomintang. He returned to China in 1917, and in 1921 he was elected president of a self-proclaimed national government at Guangzhou in S China. To develop the military power needed for the Northern Expedition against the militarists at Beijing, he established the Whampoa Military Academy (now Huangpu Military Academy), with Chiang Kai-shek as its commandant and with such party leaders as Wang Ching-wei and Hu Han-min as political instructors. In 1924, to hasten the conquest of China, he began a policy of active cooperation with the Chinese Communists and he accepted the help of the USSR in reorganizing the Kuomintang.
After Sun's death, when the Communists and the Kuomintang split (1927), each group claimed to be his true heirs. The official veneration of Sun's memory (especially in the Kuomintang) was a virtual cult, which centered around his tomb in Nanjing. His widow, the former Soong Ch'ing-ling (see Soong, family), whom he married in 1914, rose to a high position in the government of Communist China. He wrote San Min Chu I (tr. 1928), Memoirs of a Chinese Revolutionary (1927, repr. 1970), and Fundamentals of National Reconstruction (tr. 1953).
See biographies by L. Sharman (1934) and B. D. Martin (1952); L. S. Hsu, Sun Yat-sen, His Political and Social Ideals: A Sourcebook (1933); S. C. Leng and N. D. Palmer, Sun Yat-sen and Communism (1960); H. Z. Schiffrin, Sun Yat-sen and the Origins of the Chinese Revolution (1970); M. Wilbur, Sun Yat-sen (1977).
See The Art of War (tr. by S. B. Griffith, 1971).
See B. L. Weinstein and R. E. Firestine, Regional Growth and Decline in the United States: The Rise of the Sunbelt and the Decline of the Northeast (1978); C. Abbott, The New Urban America (1987); R. M. Miller and G. E. Pozzetta, ed., Shades of the Sunbelt: Essays on Ethnicity, Race, and the Urban South (1988); R. A. Mohl, ed., Searching for the Sunbelt (1990).
Veneration of the sun or its representation as a deity. It appears in several early cultures, notably in ancient Egypt, Indo-Europe, and Mesoamerica, where urban civilizations were combined with a strong ideology of sacred kingship, in which kings ruled by the power of the sun and claimed descent from it. The imagery of the sun as the ruler of both the upper and the lower world, which he visits daily, was prominent. Sun heroes and deities also figure in many mythologies, including Indo-Iranian, Greco-Roman, and Scandinavian. In late Roman history, sun worship was of such importance that it was later called “solar monotheism.” Seealso Amaterasu, Re, Shamash, Sol, Surya, Tonatiuh.
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Most important religious ritual of the Plains Indians of North America. Ordinarily held by each tribe once a year in early summer, it is simultaneously an opportunity to reaffirm basic beliefs about the universe and the supernatural through rituals and a highly sacred event through which personal sacrifice is undertaken for the general well-being of the community and the individual. The ritual originated long ago and has been widely adopted by indigenous Plains peoples from Saskatchewan, Can., to Texas, U.S. The central rite involves male supplicants who, in order to fulfill a vow, to seek spiritual energy and insight, and for the health of the community, pledge to dance for several days without stopping for food, drink, or sleep, their ordeal ending in exhaustion. Among some tribes, piercing and sun gazing are practiced.
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Smallest member (Helarctos malayanus) of the bear family (Ursidae), found in South Asian forests. Nocturnal and tree-climbing, the sun bear weighs 60–140 lbs (27–64 kg) and is 3–4 ft (1–1.2 m) long, with a 2-in. (5-cm) tail, large forepaws, and short black fur with an orange-yellow crescent on the chest. It uses its long, curved claws to tear or dig for insect nests, particularly those of bees and termites. It also eats fruit, honey, and small vertebrates. The sun bear is shy and intelligent; legends say that its chest crescent represents the sun.
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Sun Yat-sen
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Star around which the components of the solar system revolve. It is about five billion years old and is the dominant body of the system, with more than 99percnt of its mass. It converts five million tons of matter into energy every second by nuclear fusion reactions in its core, producing neutrinos (see solar neutrino problem) and solar radiation. The small amount of this energy that penetrates Earth’s atmosphere provides the light and heat that support life. A sphere of luminous gas 864,950 mi (1,392,000 km) in diameter, the Sun has about 330,000 times the mass of Earth. Its core temperature is close to 27 million °F (15 million °C) and its surface temperature about 10,000 °F (6,000 °C). The Sun, a spectral type G (yellow) star, has fairly average properties for a main-sequence star (see Hertzsprung-Russell diagram). It rotates at different rates at different latitudes; one rotation takes 36 days at the poles but only 25 days at the equator. The visible surface, or photosphere, is in constant motion, with the number and position of sunspots changing in a regular solar cycle. External phenomena include magnetic activity extending into the chromosphere and corona, solar flares, solar prominences, and the solar wind. Effects on Earth include auroras and disruption of radio communications and power-transmission lines. Despite its activity, the Sun appears to have remained relatively unchanged for billions of years. Seealso eclipse; heliopause.
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(born Jan. 6, 1920, Kwangju Sangsa Ri, P'yŏngan-puk province, Korea) South Korean religious leader. Convinced that he was designated by God as a successor to Jesus, Moon began to preach a new religion, loosely based on Christianity, in North Korea in 1946. After being imprisoned by North Korean authorities, he escaped or was released and went to South Korea, where he founded the Unification Church in 1954 and built a multimillion-dollar business empire. In 1973 he moved his headquarters to Tarrytown, N.Y., U.S., where he became the focus of controversies over fund-raising techniques, tax evasion, and the indoctrination of followers (popularly called Moonies). In 1982 Moon was convicted of tax evasion, sentenced to 18 months in prison, and fined $25,000. He has also suffered from a damaging exposé by his daughter-in-law. In the 1990s the church began operations in Brazil, where its purchase of large tracts of rainforest has been widely criticized.
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