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Marcus Manilius
Marcus Manilius (fl. 1st century AD) was a Roman poet, astrologer, and author of a poem in five books called '' Astronomica''. The ''Astronomica'' The author of ''Astronomica'' is neither quoted nor mentioned by any ancient writer. Even his name is uncertain, but it was probably Marcus Manilius; in the earlier books the author is anonymous, the later give Manilius, Manlius, Mallius. The poem itself implies that the writer lived under Augustus or Tiberius, and that he was a citizen of and resident in Rome, suggesting that Manilius wrote the work during the 20s CE. According to the early 18th century classicist Richard Bentley, he was an Asiatic Greek; according to the 19th-century classicist Fridericus Jacob, an African. His work is one of great learning; he had studied his subject in the best writers, and generally represents the most advanced views of the ancients on astronomy (or rather astrology). Manilius frequently imitates Lucretius. Although his diction presents some pe ...
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Wenceslas Hollar - Manilius
Wenceslaus, Wenceslas, Wenzeslaus and Wenzslaus (and other similar names) are Latinized forms of the Czech name Václav. The other language versions of the name are german: Wenzel, pl, Wacław, Więcesław, Wieńczysław, es, Wenceslao, russian: Vyacheslav, hr, Vjenceslav, lt, Venckus among others. It originated as a Latin spelling for Czech rulers. It is a Slavic dithematic name (of two lexemes), derived from the Slavic words ''veli/vyache/więce/više'' ("great(er), large(r)"), and ''slava'' ("glory, fame"), both very common in Slavic names. It roughly means "greater glory". People named Wenceslaus or spelling variations thereof include: * Wenceslaus I, Duke of Bohemia (907–935 or 929), saint and subject of the Christmas carol "Good King Wenceslas" * Wenceslaus II, Duke of Bohemia (died 1192) * Wenceslaus I of Bohemia (c. 1205–1253), King of Bohemia * Wenceslaus II of Bohemia (1271–1305), King of Bohemia and Poland * Wenceslaus III of Bohemia (1289–1306), King of Hu ...
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Harry Eyres
Harry Eyres (born 1958) is a British journalist, writer and poet Biography and Career Eyres was educated as a King's Scholar at Eton College, where he won the Newcastle Scholarship in 1975, and at Trinity College, Cambridge, where he studied English language and literature. He holds a Diploma de Estudios Hispanicos from Barcelona University and an MSc in Environmental Assessment and Evaluation from the London School of Economics (LSE). Eyres was a theatre critic and arts writer for ''The Times'' from 1987 to 1993, the wine editor of ''Harpers & Queen'' from 1989 to 1996, and the wine columnist for ''The Spectator'' magazine from 1984 to 1989. He was Poetry Editor of ''The Daily Express'' from 1996 to 2001. Prior to his writing career, in the early 1980s, he was a junior expert at Christie's wine department, working under wine critic Michael Broadbent. From 2004 to 2015, Eyres wrote a weekly column for ''The Financial Times The ''Financial Times'' (''FT'') is a Britis ...
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Silver Age Latin Writers
Silver is a chemical element with the symbol Ag (from the Latin ', derived from the Proto-Indo-European ''h₂erǵ'': "shiny" or "white") and atomic number 47. A soft, white, lustrous transition metal, it exhibits the highest electrical conductivity, thermal conductivity, and reflectivity of any metal. The metal is found in the Earth's crust in the pure, free elemental form ("native silver"), as an alloy with gold and other metals, and in minerals such as argentite and chlorargyrite. Most silver is produced as a byproduct of copper, gold, lead, and zinc refining. Silver has long been valued as a precious metal. Silver metal is used in many bullion coins, sometimes alongside gold: while it is more abundant than gold, it is much less abundant as a native metal. Its purity is typically measured on a per-mille basis; a 94%-pure alloy is described as "0.940 fine". As one of the seven metals of antiquity, silver has had an enduring role in most human cultures. Other than in cur ...
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Ancient Roman Astrologers
Ancient history is a time period from the beginning of writing and recorded human history to as far as late antiquity. The span of recorded history is roughly 5,000 years, beginning with the Sumerian cuneiform script. Ancient history covers all continents inhabited by humans in the period 3000 BCAD 500. The three-age system periodizes ancient history into the Stone Age, the Bronze Age, and the Iron Age, with recorded history generally considered to begin with the Bronze Age. The start and end of the three ages varies between world regions. In many regions the Bronze Age is generally considered to begin a few centuries prior to 3000 BC, while the end of the Iron Age varies from the early first millennium BC in some regions to the late first millennium AD in others. During the time period of ancient history, the world population was already exponentially increasing due to the Neolithic Revolution, which was in full progress. While in 10,000 BC, the world population stood at ...
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Year Of Death Unknown
A year or annus is the orbital period of a planetary body, for example, the Earth, moving in its orbit around the Sun. Due to the Earth's axial tilt, the course of a year sees the passing of the seasons, marked by change in weather, the hours of daylight, and, consequently, vegetation and soil fertility. In temperate and subpolar regions around the planet, four seasons are generally recognized: spring, summer, autumn and winter. In tropical and subtropical regions, several geographical sectors do not present defined seasons; but in the seasonal tropics, the annual wet and dry seasons are recognized and tracked. A calendar year is an approximation of the number of days of the Earth's orbital period, as counted in a given calendar. The Gregorian calendar, or modern calendar, presents its calendar year to be either a common year of 365 days or a leap year of 366 days, as do the Julian calendars. For the Gregorian calendar, the average length of the calendar year (the mea ...
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Year Of Birth Unknown
A year or annus is the orbital period of a planetary body, for example, the Earth, moving in its orbit around the Sun. Due to the Earth's axial tilt, the course of a year sees the passing of the seasons, marked by change in weather, the hours of daylight, and, consequently, vegetation and soil fertility. In temperate and subpolar regions around the planet, four seasons are generally recognized: spring, summer, autumn and winter. In tropical and subtropical regions, several geographical sectors do not present defined seasons; but in the seasonal tropics, the annual wet and dry seasons are recognized and tracked. A calendar year is an approximation of the number of days of the Earth's orbital period, as counted in a given calendar. The Gregorian calendar, or modern calendar, presents its calendar year to be either a common year of 365 days or a leap year of 366 days, as do the Julian calendars. For the Gregorian calendar, the average length of the calendar year ( ...
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Alfred Edward Housman
Alfred Edward Housman (; 26 March 1859 – 30 April 1936) was an English classical scholar and poet. After an initially poor performance while at university, he took employment as a clerk in London and established his academic reputation by publishing as a private scholar at first. Later Housman was appointed Professor of Latin at University College London and then at the University of Cambridge. He is now acknowledged as one of the foremost classicists of his age and has been ranked as one of the greatest scholars at any time. His editions of Juvenal, Manilius, and Lucan are still considered authoritative. In 1896 he emerged as a poet with '' A Shropshire Lad'', a cycle in which he poses as an unsophisticated and melancholy youth. After a slow start, this captured the imagination of young readers, its preoccupation with early death appealing to them especially during times of war. In 1922 his ''Last Poems'' added to his reputation, which was further enhanced by the large numb ...
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The Latin Library
The Latin Library is a website that collects public domain Latin texts. It is run by William L. Carey, adjunct professor of Latin and Roman Law at George Mason University. The texts have been drawn from different sources, are not intended for research purposes nor as substitutes for critical editions, and may contain errors. There are no translations at the site. See also *Latin literature *Corpus Corporum *Library of Latin Texts The Library of Latin Texts (LLT) is a subscription-based database of Latin texts, from antiquity up to the present day. Started in 1991 as the ''Cetedoc Library of Christian Latin Texts'' (CLCLT), it continues to be developed by the ''Centre ‘T ... References External links * {{DEFAULTSORT:Latin Library Latin-language literature Computing in classical studies American digital libraries ...
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Mare Vaporum
Mare Vaporum (Latin ''vapōrum'', the "sea of vapors") is a lunar mare located between the southwest rim of Mare Serenitatis and the southeast rim of Mare Imbrium. It was named by Giovanni Battista Riccioli in 1651.''Autostar Suite Astronomer Edition''. CD-ROM. Meade, April 2006. The mare lies in an old basin or crater that is within the Procellarum basin. It is in diameter and in area, and is bordered to the northeast by the mountain range Montes Apenninus. In the south of the mare is Rima Hyginus, a rille intersected by the crater Hyginus. The lunar material surrounding the mare is from the Lower Imbrian epoch, and the mare material is from the Eratosthenian The Eratosthenian period in the lunar geologic timescale runs from 3,200 million years ago to 1,100 million years ago. It is named after the crater Eratosthenes, which displays characteristics typical of craters of this age, including a surface ... epoch. References External links Mare Vaporum at The Moon Wiki ...
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Manilius (crater)
Manilius is a lunar impact crater on the northeast edge of Mare Vaporum. Its diameter is 38 km. Description Manilius has a well-defined rim with a sloping inner surface that runs directly down to the ring-shaped mound of scree along the base, and a small outer rampart. The small crater interior has a higher albedo than the surroundings, and it appears bright when the sun is overhead. Within the crater is a central peak formation near the midpoint. The crater also possesses a ray system that extends for a distance of over 300 kilometers. Despite the presence of these rays, which generally indicate the age of the crater as Copernican, the crater is currently mapped as Eratosthenian age. Names Manilius is named after the Roman astronomer Marcus Manilius. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized. Earlier lunar cartographers had given the feature different names. Michael ...
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Moon
The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of Australia). The Moon is a planetary-mass object with a differentiated rocky body, making it a satellite planet under the geophysical definitions of the term and larger than all known dwarf planets of the Solar System. It lacks any significant atmosphere, hydrosphere, or magnetic field. Its surface gravity is about one-sixth of Earth's at , with Jupiter's moon Io being the only satellite in the Solar System known to have a higher surface gravity and density. The Moon orbits Earth at an average distance of , or about 30 times Earth's diameter. Its gravitational influence is the main driver of Earth's tides and very slowly lengthens Earth's day. The Moon's orbit around Earth has a sidereal period of 27.3 days. During each synodic period ...
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Impact Crater
An impact crater is a circular depression in the surface of a solid astronomical object formed by the hypervelocity impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically have raised rims and floors that are lower in elevation than the surrounding terrain. Lunar impact craters range from microscopic craters on lunar rocks returned by the Apollo Program and small, simple, bowl-shaped depressions in the lunar regolith to large, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth. Impact craters are the dominant geographic features on many solid Solar System objects including the Moon, Mercury, Callisto, Ganymede and most small moons and asteroids. On other planets and moons that experience more active surface geological processes, such as Earth, Venus, Europa, Io and Titan, visible impact craters are less common because they become eroded ...
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