Roman timekeeping

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Sundial at the Temple of Apollo (Pompeii) Temple of Apollo (7238818732) detail.jpg
Sundial at the Temple of Apollo (Pompeii)

In Roman timekeeping, a day was divided into periods according to the available technology. Initially, the day was divided into two parts: the ante meridiem (before noon) and the post meridiem (after noon). With the advent of the sundial circa 263 BC, the period of the natural day from sunrise to sunset was divided into twelve hours. [1]

Contents

Variation

An hour was defined as one twelfth of the daytime, or the time elapsed between sunset and sunrise. Since the duration varied with the seasons, this also meant that the length of the hour changed. Winter days being shorter, the hours were correspondingly shorter and longer in summer. [1] At Mediterranean latitude, one hour was about 45 minutes at the winter solstice, and 75 minutes at summer solstice. [2]

The Romans understood that as well as varying by season, the length of daytime depended on latitude.

Subdivision of the day and night

Duration and distribution of horae and vigiliae on equinoxes and solstices of the year AD 8 for Forum Romanum. Ancient Roman time keeping hora vigilia equinox solstice.svg
Duration and distribution of horae and vigiliae on equinoxes and solstices of the year AD 8 for Forum Romanum.

Civil day

The civil day (dies civilis) ran from midnight (media nox) to midnight. [3] The date of birth of children was given as this period. [4]

It was divided into the following parts:

  1. Media nox (midnight)
  2. Mediae noctis inclinatio (the middle of the night)
  3. Gallicinium (cock crowing)
  4. Conticinium (cock stops crowing)
  5. Diluculum (dawn)
  6. Mane (morning)
  7. Antemeridianum tempus (forenoon)
  8. Meridies (mid-day)
  9. Tempus pomeridianum (afternoon)
  10. Solis occasus (sunset)
  11. Vespera (evening)
  12. Crepusculum (twilight)
  13. Prima fax (lighting of candles)
  14. Concubia nox (bed-time)
  15. Intempesta nox (far into the night)
  16. Inclinatio ad mediam noctem (approaching midnight) [3]

Natural day

The natural day (dies naturalis) ran from sunrise to sunset. [4]

The hours were numbered from one to twelve as hora prima, hora secunda, hora tertia, etc. To indicate that it is a day or night hour, Romans used expressions such as for example prima diei hora (first hour of the day), and prima noctis hora (first hour of the night). [5]

Timekeeping devices

A Roman era sundial on display at a museum in Side, Turkey Museum side roman sun dial.JPG
A Roman era sundial on display at a museum in Side, Turkey

The Romans used various ancient timekeeping devices. Sundials were set up in public places, [2] beginning after one was imported from Sicily in 263 BC. [6] Sundials were used to calibrate water clocks. [7] The disadvantage of sundials, or shadow clocks, was that they worked only in sunshine and had to be recalibrated depending on the latitude and season. [8]

Legacy

See also

Related Research Articles

A day is the time period of a full rotation of the Earth with respect to the Sun. On average, this is 24 hours. As a day passes at a given location it experiences morning, noon, afternoon, evening, and night. This daily cycle drives circadian rhythms in many organisms, which are vital to many life processes.

<span class="mw-page-title-main">Hour</span> Unit of time equal to 60 minutes

An hour is a unit of time historically reckoned as 124 of a day and defined contemporarily as exactly 3,600 seconds (SI). There are 60 minutes in an hour, and 24 hours in a day.

<span class="mw-page-title-main">Minute</span> Unit of time equal to 60 seconds

The minute is a unit of time defined as equal to 60 seconds. One hour contains 60 minutes. Although not a unit in the International System of Units (SI), the minute is accepted for use in the SI. The SI symbol for minutes is min. The prime symbol is also sometimes used informally to denote minutes. In the UTC time standard, a minute on rare occasions has 61 seconds, a consequence of leap seconds; there is also a provision to insert a negative leap second, which would result in a 59-second minute, but this has never happened in more than 40 years under this system.

<span class="mw-page-title-main">Sundial</span> Device that tells the time of day by the apparent position of the Sun in the sky

A sundial is a horological device that tells the time of day when direct sunlight shines by the apparent position of the Sun in the sky. In the narrowest sense of the word, it consists of a flat plate and a gnomon, which casts a shadow onto the dial. As the Sun appears to move through the sky, the shadow aligns with different hour-lines, which are marked on the dial to indicate the time of day. The style is the time-telling edge of the gnomon, though a single point or nodus may be used. The gnomon casts a broad shadow; the shadow of the style shows the time. The gnomon may be a rod, wire, or elaborately decorated metal casting. The style must be parallel to the axis of the Earth's rotation for the sundial to be accurate throughout the year. The style's angle from horizontal is equal to the sundial's geographical latitude.

<span class="mw-page-title-main">Analemma</span> Diagrammatic representation of Suns position over a period of time

In astronomy, an analemma is a diagram showing the position of the Sun in the sky as seen from a fixed location on Earth at the same mean solar time, as that position varies over the course of a year. The diagram will resemble a figure eight. Earth often display an analemma as a two-dimensional figure of equation of time vs. declination of the Sun.

<span class="mw-page-title-main">Sunset</span> Daily falling of the Sun below the horizon

Sunset is the disappearance of the Sun below the horizon of the Earth due to its rotation. As viewed from everywhere on Earth, it is a phenomenon that happens approximately once every 24 hours, except in areas close to the poles. The equinox Sun sets due west at the moment of both the spring and autumn equinoxes. As viewed from the Northern Hemisphere, the Sun sets to the northwest in the spring and summer, and to the southwest in the autumn and winter; these seasons are reversed for the Southern Hemisphere.

<span class="mw-page-title-main">Noon</span> 12 oclock in the daytime

Noon is 12 o'clock in the daytime. It is written as 12 noon, 12:00 m., 12 p.m., 12 pm, or 12:00 or 1200 . Solar noon is the time when the Sun appears to contact the local celestial meridian. This is when the Sun reaches its apparent highest point in the sky, at 12 noon apparent solar time and can be observed using a sundial. The local or clock time of solar noon depends on the date, longitude, and time zone, with Daylight Saving Time tending to place solar noon closer to 1:00pm.

The 12-hour clock is a time convention in which the 24 hours of the day are divided into two periods: a.m. and p.m.. Each period consists of 12 hours numbered: 12, 1, 2, 3, 4, 5, 6, 7, 8, 9, 10 and 11. The 12-hour clock was developed from the second millennium BC and reached its modern form in the 16th century.

<span class="mw-page-title-main">Midnight</span> Transition time from one day to the next

Midnight is the transition time from one day to the next – the moment when the date changes, on the local official clock time for any particular jurisdiction. By clock time, midnight is the opposite of noon, differing from it by 12 hours.

In modern usage, civil time refers to statutory time as designated by civilian authorities. Modern civil time is generally national standard time in a time zone at a fixed offset from Coordinated Universal Time (UTC), possibly adjusted by daylight saving time during part of the year. UTC is calculated by reference to atomic clocks and was adopted in 1972. Older systems use telescope observations.

<span class="mw-page-title-main">Time discipline</span> Social rules and conventions governing time

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<span class="mw-page-title-main">Terce</span> Former part of the canonical hours

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<span class="mw-page-title-main">Japanese clock</span> Mechanical clock that has been made to tell traditional Japanese time

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<span class="mw-page-title-main">24-hour analog dial</span> Clock or watch face showing the full 24 hours

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<span class="mw-page-title-main">Daytime</span> Period of a day in which a location experiences natural illumination

Daytime as observed on Earth is the period of the day during which a given location experiences natural illumination from direct sunlight. Daytime occurs when the Sun appears above the local horizon, that is, anywhere on the globe's hemisphere facing the Sun. In direct sunlight the movement of the sun can be recorded and observed using a sundial that casts a shadow that slowly moves during the day. Other planets and natural satellites that rotate relative to a luminous primary body, such as a local star, also experience daytime, but this article primarily discusses daytime on Earth.

<span class="mw-page-title-main">History of timekeeping devices in Egypt</span>

The ancient Egyptians were one of the first cultures to widely divide days into generally agreed-upon equal parts, using early timekeeping devices such as sundials, shadow clocks, and merkhets . Obelisks were also used by reading the shadow that they make. The clock was split into daytime and nighttime, and then into smaller hours.

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<span class="mw-page-title-main">Tide dial</span>

A tide dial, also known as a Mass or scratch dial, is a sundial marked with the canonical hours rather than or in addition to the standard hours of daylight. Such sundials were particularly common between the 7th and 14th centuries in Europe, at which point they began to be replaced by mechanical clocks. There are more than 3,000 surviving tide dials in England and at least 1,500 in France.

<span class="mw-page-title-main">Unequal hours</span> A system where hour lengths are unequal or not all 60 minutes

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Relative hour, sometimes called halachic hour, seasonal hour and variable hour, is a term used in rabbinic Jewish law that assigns 12 hours to each day and 12 hours to each night, all throughout the year. A relative hour has no fixed length in absolute time, but changes with the length of daylight each day - depending on summer, and in winter. Even so, in all seasons a day is always divided into 12 hours, and a night is always divided into 12 hours, which invariably makes for a longer hour or a shorter hour. At Mediterranean latitude, one hour can be about 45 minutes at the winter solstice, and 75 minutes at summer solstice. All of the hours mentioned by the Sages in either the Mishnah or Talmud, or in other rabbinic writings, refer strictly to relative hours.

References

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  2. 1 2 Laurence, Ray (2006). Roman Pompeii: Space and Society. Routledge. pp. 104–112. ISBN   978-1-134-76899-8 . Retrieved 24 December 2019.
  3. 1 2 Adam, Alexander (1791). Roman antiquities: or an account of the manners and customs of the Romans, respecting their government, magistracy, laws ... designed chiefly to illustrate the Latin classics. Edinburgh: William Creech. pp. 307–308. Retrieved 24 December 2019.
  4. 1 2 CENSORINUS (238). "DE DIE NATALI". elfinspell.com. Retrieved 25 December 2019.
  5. Traupman, John C. (2007). Conversational Latin for Oral Proficiency: Phrase Book and Dictionary, Classical and Neo-Latin (in Latin). Bolchazy-Carducci Publishers. p. 80. ISBN   978-0-86516-622-6 . Retrieved 24 December 2019.
  6. "Timekeeping in the Ancient Mediterranean and Near East". The MD Harris Institute. 29 September 2013. Retrieved 24 December 2019.
  7. Grattan, Kenneth. "A brief history of telling time". The Conversation. Retrieved 24 December 2019.
  8. "Ancient Everyday – Telling Time in the Roman World". Eagles and Dragons Publishing. 1 July 2017. Retrieved 24 December 2019.
  9. "Definition of SEXT". www.merriam-webster.com. Retrieved 25 December 2019.
  10. "What Time Is 'Noon'?". www.merriam-webster.com. Retrieved 25 December 2019.
  11. "noon". www.etymonline.com. Retrieved 25 December 2019.