Exeligmos, the Glossary
An exeligmos (lit) is a period of 54 years, 33 days that can be used to predict successive eclipses with similar properties and location.[1]
Table of Contents
27 relations: Antikythera mechanism, Coordinated Universal Time, December 1963 lunar eclipse, Eclipse, Eclipse cycle, Eclipse season, Gamma (eclipse), January 2018 lunar eclipse, List of solar eclipses in the 22nd century, Longitude, Lunar eclipse, Lunar month, Lunar node, Magnitude of eclipse, Orbit of the Moon, Oxford University Press, Saros (astronomy), Solar eclipse, Solar eclipse of August 12, 2045, Solar eclipse of July 11, 1991, Solar eclipse of June 21, 2020, Solar eclipse of June 8, 1937, Solar eclipse of May 20, 1966, Solar eclipse of May 6, 1883, Solar eclipse of September 14, 2099, Solar Saros 136, Supermoon.
- Ancient Greek astronomy
- Eclipses
Antikythera mechanism
The Antikythera mechanism is an Ancient Greek hand-powered orrery (model of the Solar System), described as the oldest known example of an analogue computer used to predict astronomical positions and eclipses decades in advance. Exeligmos and Antikythera mechanism are Ancient Greek astronomy.
See Exeligmos and Antikythera mechanism
Coordinated Universal Time
Coordinated Universal Time (UTC) is the primary time standard globally used to regulate clocks and time.
See Exeligmos and Coordinated Universal Time
December 1963 lunar eclipse
A total lunar eclipse took place on Monday, December 30, 1963.
See Exeligmos and December 1963 lunar eclipse
Eclipse
An eclipse is an astronomical event which occurs when an astronomical object or spacecraft is temporarily obscured, by passing into the shadow of another body or by having another body pass between it and the viewer. Exeligmos and eclipse are eclipses.
Eclipse cycle
Eclipses may occur repeatedly, separated by certain intervals of time: these intervals are called eclipse cycles. Exeligmos and eclipse cycle are eclipses and time in astronomy.
See Exeligmos and Eclipse cycle
Eclipse season
An eclipse season is a period, roughly every six months, when eclipses occur. Exeligmos and eclipse season are eclipses and time in astronomy.
See Exeligmos and Eclipse season
Gamma (eclipse)
Gamma (denoted as γ) of an eclipse describes how centrally the shadow of the Moon or Earth strikes the other body.
See Exeligmos and Gamma (eclipse)
January 2018 lunar eclipse
A total lunar eclipse occurred on 31 January 2018.
See Exeligmos and January 2018 lunar eclipse
List of solar eclipses in the 22nd century
This is a list of solar eclipses that will occur in the 22nd century.
See Exeligmos and List of solar eclipses in the 22nd century
Longitude
Longitude is a geographic coordinate that specifies the east–west position of a point on the surface of the Earth, or another celestial body.
Lunar eclipse
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. Exeligmos and lunar eclipse are eclipses.
See Exeligmos and Lunar eclipse
Lunar month
In lunar calendars, a lunar month is the time between two successive syzygies of the same type: new moons or full moons.
Lunar node
A lunar node is either of the two orbital nodes of the Moon, that is, the two points at which the orbit of the Moon intersects the ecliptic.
Magnitude of eclipse
The magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed. Exeligmos and magnitude of eclipse are eclipses.
See Exeligmos and Magnitude of eclipse
Orbit of the Moon
The Moon orbits Earth in the prograde direction and completes one revolution relative to the Vernal Equinox and the stars in about 27.32 days (a tropical month and sidereal month) and one revolution relative to the Sun in about 29.53 days (a synodic month).
See Exeligmos and Orbit of the Moon
Oxford University Press
Oxford University Press (OUP) is the publishing house of the University of Oxford.
See Exeligmos and Oxford University Press
Saros (astronomy)
The saros is a period of exactly 223 synodic months, approximately 6585.321 days (18.04 years), or 18 years plus 10, 11, or 12 days (depending on the number of leap years), and 8 hours, that can be used to predict eclipses of the Sun and Moon. Exeligmos and saros (astronomy) are eclipses and time in astronomy.
See Exeligmos and Saros (astronomy)
Solar eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Exeligmos and solar eclipse are eclipses.
See Exeligmos and Solar eclipse
Solar eclipse of August 12, 2045
A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, August 12, 2045, with a magnitude of 1.0774.
See Exeligmos and Solar eclipse of August 12, 2045
Solar eclipse of July 11, 1991
A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, July 11, 1991, with a magnitude of 1.08.
See Exeligmos and Solar eclipse of July 11, 1991
Solar eclipse of June 21, 2020
An annular solar eclipse occurred at the Moon’s ascending node of orbit on Sunday, June 21, 2020, with a magnitude of 0.994.
See Exeligmos and Solar eclipse of June 21, 2020
Solar eclipse of June 8, 1937
A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, June 8, 1937, with a magnitude of 1.0751.
See Exeligmos and Solar eclipse of June 8, 1937
Solar eclipse of May 20, 1966
An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, May 20, 1966, with a magnitude of 0.9991.
See Exeligmos and Solar eclipse of May 20, 1966
Solar eclipse of May 6, 1883
A total solar eclipse occurred on May 6, 1883.
See Exeligmos and Solar eclipse of May 6, 1883
Solar eclipse of September 14, 2099
A total solar eclipse will occur at the Moon's descending node of orbit on Monday, September 14, 2099, with a magnitude of 1.0684.
See Exeligmos and Solar eclipse of September 14, 2099
Solar Saros 136
Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which are umbral (6 annular, 6 hybrid, 44 total).
See Exeligmos and Solar Saros 136
Supermoon
A supermoon is a full moon or a new moon that nearly coincides with perigee—the closest that the Moon comes to the Earth in its elliptic orbit—resulting in a slightly larger-than-usual apparent size of the lunar disk as viewed from Earth.
See also
Ancient Greek astronomy
- Ancient Greek astronomy
- Antikythera mechanism
- Armillary sphere
- Astrolabe
- Astronomical clock
- Astronomical rings
- Callippic cycle
- Celestial Matters
- Celestial Sphere Woodrow Wilson Memorial
- Celestial spheres
- Concentric spheres
- Counter-Earth
- Deferent and epicycle
- Dioptra
- Dynamics of the celestial spheres
- Equant
- Equatorial ring
- Exeligmos
- Geocentric model
- Globe of Matelica
- Gnomon
- Heliocentrism
- Hellenistic astrology
- Hipparchic cycle
- Metonic cycle
- Minoan Moulds of Palaikastro
- Mural instrument
- Octaeteris
- Pythagorean astronomical system
- Scaphe
- Spherical Earth
- Sublunary sphere
- The Sand Reckoner
- Triquetrum (astronomy)
- Urania
Eclipses
- Baily's beads
- Besselian elements
- Eclipse
- Eclipse cycle
- Eclipse photography
- Eclipse season
- Eclipses in mythology and culture
- Exeligmos
- High Altitude Observatory
- Inex
- Ketu (mythology)
- List of films featuring eclipses
- Lunar eclipse
- Lunar eclipses
- Lunar occultation of Venus
- Magnitude of eclipse
- Rahu
- Saros (astronomy)
- Solar eclipse
- Solar eclipses
- Svarbhānu
- Syzygy (astronomy)
- Tiangou
- Tritos
- Tzolkinex