|
Sothic Cycle
The Sothic cycle or Canicular period is a period of 1,461 Egyptian civil years of 365 days each or 1,460 Julian years averaging 365¼ days each. During a Sothic cycle, the 365-day year loses enough time that the start of its year once again coincides with the heliacal rising of the star Sirius ( egy, spdt or , 'Triangle'; grc-gre, Σῶθις, ) on 19 July in the Julian calendar.. It is an important aspect of Egyptology, particularly with regard to reconstructions of the Egyptian calendar and its history. Astronomical records of this displacement may have been responsible for the later establishment of the more accurate Julian and Alexandrian calendars. Mechanics The ancient Egyptian civil year, its holidays, and religious records reflect its apparent establishment at a point when the return of the bright star Sirius to the night sky was considered to herald the annual flooding of the Nile. However, because the civil calendar was exactly 365 da ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Hubble Heic0206j
The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most versatile, renowned both as a vital research tool and as a public relations boon for astronomy. The Hubble telescope is named after astronomer Edwin Hubble and is one of NASA's Great Observatories. The Space Telescope Science Institute (STScI) selects Hubble's targets and processes the resulting data, while the Goddard Space Flight Center (GSFC) controls the spacecraft. Hubble features a mirror, and its five main instruments observe in the ultraviolet, visible, and near-infrared regions of the electromagnetic spectrum. Hubble's orbit outside the distortion of Earth's atmosphere allows it to capture extremely high-resolution images with substantially lower background light than ground-based telescopes. It has recorded some of the most detailed ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Year
A tropical year or solar year (or tropical period) is the time that the Sun takes to return to the same position in the sky of a celestial body of the Solar System such as the Earth, completing a full cycle of seasons; for example, the time from vernal equinox to vernal equinox, or from summer solstice to summer solstice. It is the type of year used by tropical solar calendars. The solar year is one type of astronomical year and particular orbital period. Another type is the sidereal year (or sidereal orbital period), which is the time it takes Earth to complete one full orbit around the Sun as measured with respect to the fixed stars, resulting in a duration of 20 minutes longer than the tropical year, because of the precession of the equinoxes. Since antiquity, astronomers have progressively refined the definition of the tropical year. The entry for "year, tropical" in the '' Astronomical Almanac Online Glossary'' states: An equivalent, more descriptive, definition is " ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Thebes, Egypt
, image = Decorated pillars of the temple at Karnac, Thebes, Egypt. Co Wellcome V0049316.jpg , alt = , caption = Pillars of the Great Hypostyle Hall, in ''The Holy Land, Syria, Idumea, Arabia, Egypt, and Nubia'' , map_type = Egypt , map_alt = , map_size = , relief = yes , coordinates = , location = Luxor, Luxor Governorate, Egypt , region = Upper Egypt , type = Settlement , part_of = , length = , width = , area = , height = , builder = , material = , built = , abandoned = , epochs = , cultures = , dependency_of = , occupants = , event = , excavations = , archaeologists = , condition = , ownership = , management = , public_access = , website = , notes = , designation1 = WHS , designation1_offname = Ancient Th ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Cairo
Cairo ( ; ar, القاهرة, al-Qāhirah, ) is the capital of Egypt and its largest city, home to 10 million people. It is also part of the largest urban agglomeration in Africa, the Arab world and the Middle East: The Greater Cairo metropolitan area, with a population of 21.9 million, is the 12th-largest in the world by population. Cairo is associated with ancient Egypt, as the Giza pyramid complex and the ancient cities of Memphis and Heliopolis are located in its geographical area. Located near the Nile Delta, the city first developed as Fustat, a settlement founded after the Muslim conquest of Egypt in 640 next to an existing ancient Roman fortress, Babylon. Under the Fatimid dynasty a new city, ''al-Qāhirah'', was founded nearby in 969. It later superseded Fustat as the main urban centre during the Ayyubid and Mamluk periods (12th–16th centuries). Cairo has long been a centre of the region's political and cultural life, and is titled "the city of a thousand m ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Memphis, Egypt
, alternate_name = , image = , alt = , caption = Ruins of the pillared hall of Ramesses IIat Mit Rahina , map_type = Egypt#Africa , map_alt = , map_size = , relief = , coordinates = , location = Mit Rahina, Giza Governorate, Egypt , region = Lower Egypt , type = Settlement , part_of = , length = , width = , area = , height = , builder = Unknown, was already in existence during Iry-Hor's reignP. Tallet, D. Laisnay: ''Iry-Hor et Narmer au Sud-Sinaï (Ouadi 'Ameyra), un complément à la chronologie des expéditios minière égyptiene'', in: BIFAO 112 (2012), 381–395available online/ref> , material = , built = Earlier than 31st century BC , abandoned = 7th century AD , epochs = Early Dynastic Period to Early Middle Ages , cultures = , dependency_of = , occupants = , event ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Heliopolis (Ancient Egypt)
Heliopolis (I͗wnw, Iunu or 𓉺𓏌𓊖; egy, I͗wnw, 'the Pillars'; cop, ⲱⲛ; gr, Ἡλιούπολις, Hēlioúpοlis, City of the Sun) was a major city of ancient Egypt. It was the capital of the 13th or Heliopolite Nome of Lower Egypt and a major religious centre. It is now located in Ayn Shams, a northeastern suburb of Cairo. Heliopolis was one of the oldest cities of ancient Egypt, occupied since the Predynastic Period.. It greatly expanded under the Old and Middle Kingdoms but is today mostly destroyed, its temples and other buildings having been scavenged for the construction of medieval Cairo. Most information about the ancient city comes from surviving records. The major surviving remnant of Heliopolis is the obelisk of the Temple of Ra-Atum erected by Senusret I of Dynasty XII. It still stands in its original position, now within Al-Masalla in Al-Matariyyah, Cairo. The high red granite obelisk weighs 120 tons (240,000 lbs) and is believed to be the ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Thoth (month)
Thout ( cop, Ⲑⲱⲟⲩⲧ, ), also known as Thoth ( grc-gre, Θωθ, ''Thōth'') and Tut. ( ar, توت), is the first month of the ancient Egyptian and Coptic calendars. It lies between 11 September and 10 October of the Gregorian calendar. The month of Thout is also the first month of the Season of ''Akhet'' (Inundation) in Ancient Egypt, when the Nile floods historically covered the land of Egypt; it has not done so since the construction of the High Dam at Aswan. Name The name of the month comes from Thoth, the Ancient Egyptian God of Wisdom and Science, inventor of writing, patron of scribes, and "he who designates the seasons, months, and years." Thoth presided over the "House of Life," which were composed and copied all texts necessary for the maintenance and replenishment of life. Coptic Synaxarium of the month of Thout See also * Egyptian, Coptic, and Islamic calendar The Hijri calendar ( ar, ٱلتَّقْوِيم ٱلْهِجْرِيّ, translit=al-ta ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Censorinus
Censorinus was a Roman grammarian and miscellaneous writer from the 3rd century AD. Biography He was the author of a lost work ''De Accentibus'' and of an extant treatise ''De Die Natali'', written in 238, and dedicated to his patron Quintus Caerellius as a birthday gift. The contents are of a varied character: the natural history of man, the influence of the stars and '' genii,'' music, religious rites, astronomy, the doctrines of the Greek philosophers, and antiquarian subjects. The second part deals with chronological and mathematical questions, and has been of great service in determining the principal epochs of ancient history. The whole is full of curious and interesting information. The style is clear and concise, although somewhat rhetorical, and the —for the period—good. The chief authorities used were Varro and Suetonius. Some scholars, indeed, hold that the entire work is practically an adaptation of the lost ''Pratum'' of Suetonius. The fragments of a work '' ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Egyptian Chronology
The majority of Egyptologists agree on the outline and many details of the chronology of Ancient Egypt. This scholarly consensus is the so-called Conventional Egyptian chronology, which places the beginning of the Old Kingdom in the 27th century BC, the beginning of the Middle Kingdom in the 21st century BC and the beginning of the New Kingdom in the mid-16th century BC. Despite this consensus, disagreements remain within the scholarly community, resulting in variant chronologies diverging by about 300 years for the Early Dynastic Period, up to 30 years in the New Kingdom, and a few years in the Late Period. In addition, there are a number of "alternative chronologies" outside scholarly consensus, such as the " New Chronology" proposed in the 1990s, which lowers New Kingdom dates by as much as 350 years, or the " Glasgow Chronology" (proposed 1978–1982), which lowers New Kingdom dates by as much as 500 years. Overview Scholarly consensus on the general outline of the c ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Eduard Meyer
Eduard Meyer (25 January 1855 – 31 August 1930) was a German historian. He was the brother of Celticist Kuno Meyer (1858–1919). Biography Meyer was born in Hamburg and educated at the Gelehrtenschule des Johanneums and later at the universities of Bonn and Leipzig. After completing his studies, he spent one year in Istanbul. In 1879, he went to the University of Leipzig as privatdocent. He was appointed professor of ancient history at Breslau in 1885, at Halle in 1889, and at Berlin in 1902. He lectured at Harvard in 1909 and the University of Illinois, Urbana-Champaign in 1910. Honorary degrees were given him by Oxford, St. Andrews, Freiburg, and Chicago universities. He died in Berlin. Egyptology In 1904 Meyer was the first to note the Sothic cycle of the Heliacal rising of Sirius, which forms the basis for the traditional chronology of Egypt. Works His principal work is his "''Geschichte des Altertums''" (1884-1902; third edition, 1913). He also published: * ''Forsch ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Celestial Equator
The celestial equator is the great circle of the imaginary celestial sphere on the same plane as the equator of Earth. This plane of reference bases the equatorial coordinate system. In other words, the celestial equator is an abstract projection of the terrestrial equator into outer space. Due to Earth's axial tilt, the celestial equator is currently inclined by about 23.44° with respect to the ecliptic (the plane of Earth's orbit), but has varied from about 22.0° to 24.5° over the past 5 million years due to perturbation from other planets. An observer standing on Earth's equator visualizes the celestial equator as a semicircle passing through the zenith, the point directly overhead. As the observer moves north (or south), the celestial equator tilts towards the opposite horizon. The celestial equator is defined to be infinitely distant (since it is on the celestial sphere); thus, the ends of the semicircle always intersect the horizon due east and due west, regardless ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Proper Motion
Proper motion is the astrometric measure of the observed changes in the apparent places of stars or other celestial objects in the sky, as seen from the center of mass of the Solar System, compared to the abstract background of the more distant stars. The components for proper motion in the equatorial coordinate system (of a given epoch, often J2000.0) are given in the direction of right ascension (''μ''α) and of declination (''μ''δ). Their combined value is computed as the ''total proper motion'' (''μ''). It has dimensions of angle per time, typically arcseconds per year or milliarcseconds per year. Knowledge of the proper motion, distance, and radial velocity allows calculations of an object's motion from our star system's frame of reference and its motion from the galactic frame of reference – that is motion in respect to the Sun, and by coordinate transformation, that in respect to the Milky Way. Introduction Over the course of centuries, stars appear t ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
_(Vallée_des_Rois%2C_Thèbes_ouest)_-4.jpg "Click for more on -> Egyptian Chronology")
