459

Last updated

Millennium: 1st millennium
Centuries:
Decades:
Years:
459 in various calendars
Gregorian calendar 459
CDLIX
Ab urbe condita 1212
Assyrian calendar 5209
Balinese saka calendar 380–381
Bengali calendar −134
Berber calendar 1409
Buddhist calendar 1003
Burmese calendar −179
Byzantine calendar 5967–5968
Chinese calendar 戊戌年 (Earth  Dog)
3156 or 2949
     to 
己亥年 (Earth  Pig)
3157 or 2950
Coptic calendar 175–176
Discordian calendar 1625
Ethiopian calendar 451–452
Hebrew calendar 4219–4220
Hindu calendars
 - Vikram Samvat 515–516
 - Shaka Samvat 380–381
 - Kali Yuga 3559–3560
Holocene calendar 10459
Iranian calendar 163 BP – 162 BP
Islamic calendar 168 BH – 167 BH
Javanese calendar 344–345
Julian calendar 459
CDLIX
Korean calendar 2792
Minguo calendar 1453 before ROC
民前1453年
Nanakshahi calendar −1009
Seleucid era 770/771 AG
Thai solar calendar 1001–1002
Tibetan calendar 阳土狗年
(male Earth-Dog)
585 or 204 or −568
     to 
阴土猪年
(female Earth-Pig)
586 or 205 or −567
The Avukana Buddha Statue (Sri Lanka) Buda de Avukana - 03.jpg
The Avukana Buddha Statue (Sri Lanka)

Year 459 ( CDLIX ) was a common year starting on Thursday (link will display the full calendar) of the Julian calendar. At the time, it was known as the Year of the Consulship of Ricimer and Patricius (or, less frequently, year 1212 Ab urbe condita ). The denomination 459 for this year has been used since the early medieval period, when the Anno Domini calendar era became the prevalent method in Europe for naming years.

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Events

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Roman Empire

Britannia

Europe

Asia

Other events

• Total lunar eclipse on May 3, in which totality was for 106 minutes and 32 seconds. A totality of this length will not occur until August 19, 4763. [1]

Births

Deaths

Related Research Articles

The 450s decade ran from January 1, 450, to December 31, 459.

<span class="mw-page-title-main">Baily's beads</span> Feature of total and annular solar eclipses

The Baily's beads, diamond ring or more rarely double diamond ring effects, are features of total and annular solar eclipses. Although caused by the same phenomenon, they are distinct events during these types of solar eclipses. As the Moon covers the Sun during a solar eclipse, the rugged topography of the lunar limb allows beads of sunlight to shine through in some places while not in others. They are named for Francis Baily, who explained the effects in 1836. The diamond ring effects are seen when only one or two beads are left, appearing as shining "diamonds" set in a bright ring around the lunar silhouette.

<span class="mw-page-title-main">Solar eclipse</span> Natural phenomenon wherein the Sun is obscured by the Moon

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. Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to the plane of Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of the Sun is obscured. Unlike a lunar eclipse, which may be viewed from anywhere on the night side of Earth, a solar eclipse can only be viewed from a relatively small area of the world. As such, although total solar eclipses occur somewhere on Earth every 18 months on average, they recur at any given place only once every 360 to 410 years.

<span class="mw-page-title-main">Solar eclipse of July 11, 2010</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Sunday, July 11 and Monday, July 12, 2010, with a magnitude of 1.058. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.6 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 1, 2008</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, August 1, 2008, with a magnitude of 1.0394. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.4 days after perigee, the Moon's apparent diameter was larger.

A total lunar eclipse will take place on Friday, 14 March 2025, the first of two total lunar eclipses in 2025. The Moon will take place near apogee during this eclipse, making it appear smaller than usual. The second eclipse will take place on 7-8 September 2025, happening near apogee. Occurring only 3.4 days before apogee, the Moon’s apparent diameter will be 5.4% smaller than average.

<span class="mw-page-title-main">Solar eclipse of November 13, 2012</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, November 13 and Wednesday, November 14, 2012, with a magnitude of 1.05. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 12 hours before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 2, 2019</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, July 2, 2019, with a magnitude of 1.0459. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.4 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of May 22, 2096</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit between Monday, May 21 and Tuesday, May 22, 2096, with a magnitude of 1.0737. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 13 hours after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of March 7, 1970</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, March 7, 1970, with a magnitude of 1.0414. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days after perigee, this eclipse occurred when the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of November 22, 1984</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Thursday, November 22 and Friday, November 23, 1984, with a magnitude of 1.0237. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.1 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 22, 2028</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, 22 July 2028, with a magnitude of 1.056. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.8 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of December 26, 2038</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit between Saturday, December 25 and Sunday, December 26, 2038, with a magnitude of 1.0268. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.7 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of May 9, 1929</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, May 9, 1929, with a magnitude of 1.0562. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.7 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of April 28, 1911</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Friday, April 28 and Saturday, April 29, 1911, with a magnitude of 1.0562. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.4 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 19, 1887</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Friday, August 19, 1887, with a magnitude of 1.0518. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.8 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of September 21, 1903</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, September 21, 1903, with a magnitude of 1.0316. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.1 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of April 28, 1930</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, April 28, 1930, with a magnitude of 1.0003. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The Moon's apparent diameter was near the average diameter because it occurred 7.2 days after apogee and 6 days before perigee.

<span class="mw-page-title-main">Solar eclipse of May 19, 1928</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, May 19, 1928, with a magnitude of 1.014. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 7 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of October 12, 1939</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, October 12, 1939, with a magnitude of 1.0266. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.8 days after perigee, the Moon's apparent diameter was larger.

References

  1. "EclipseWise - Six Millennium Catalog of Lunar Eclipses". eclipsewise.com. Retrieved May 21, 2024.
  2. Skidmore, Joel (2010). The Rulers of Palenque (PDF) (Fifth ed.). Mesoweb Publications. p. 18. Retrieved February 19, 2024.
  3. Hill, Jonathan (2010). Dictionary of Theologians: To 1308. Cambridge: James Clarke & Co. p. 514. ISBN   978-0-22717-906-2.