An equinoctial hour is one of the 24 parts of the full day consisting of light day and the night.
Its length, unlike the temporal hour, does not vary with the season, but is constant. The measurement of the full day with equinoctial hours of equal length was first used about 2,400 years ago in Babylonia to make astronomical observations comparable regardless of the season. Our present hour is an equinoctial hour, freed only from its seasonal variation and from the small error due to some uniform Earth rotation, and realized by modern technical means ( atomic clock, satellite and VLBI- Astrometry).
With the temporal hour, the light day and night, whose lengths vary greatly throughout the year, were divided into 12 hours each. This corresponded to the earlier sentiment and custom of not grouping the night with the light day.
The name equinoctial hours refers to the fact that the temporal hours of the light day and those of the dark night are of equal length at the equinoxes ( equinoxes).  They are also called Equal hours for a simpler expression.
Equinoctial hours ( Ancient Greek: ὥραι ἰσήμεραι, romanized: horai isemerai) are found, in distinction to the ὥραι καιρικαί, the 'unequal' hours, at least in Ancient Greece.
Geminos of Rhodes reported the observation of Pytheas of Massalia that the duration of the night depended on the geographical latitude of the place in question. However, it is not clear from his explanations whether he meant equal or equinoctial hours.  Otto Neugebauer cites this account as the oldest testimony to the concept of hour (¹ra) as a defined measure of time. 
The Babylonian Calendar knew no division of the day into 24 time units, so Old Egyptian Influence for this system can be considered probable. The period of its origin can be dated to the 4th century century BC, since Pytheas of Massalia refers to the terminus G¨j perÐodoj introduced by Eudoxos of Knidos. 
The use of equinoctial hours is later in Hipparchus of Nicaea an already familiar arithmetic. In the appendix to his commentary on Aratos of Soloi and Eudoxos of Knidos, he uses the well-known 24-hour circles and names stars whose rises are separated from each other by about one equinoctial hour in certain seasons.[ citation needed]
With the invention of the Stroke clock, it was possible for the first time to read equinoctial hours mechanically without having to perform astronomical astronomical calculations. A mechanical clock displaying the previously used temporal hours would be very costly, but occasionally its construction was nevertheless attempted. Equinoctial hours are first attested in conjunction with striking clocks in Padua in 1344, in Genoa in 1353, and in Bologna in 1356. Subsequently, striking clocks came into use throughout Europe. 
In Ancient Egypt, the earliest use of equal hours is attested by an Inscription from the time of Amenophis I around 1525 BC. The use of Water clocks allowed individual units of hours; for example, for the division of Decan star intervals, where fractions of hours were also taken into account.[ citation needed]
Ten equivalent hours were used for the time between two sunrises.[ citation needed]
The temporal hour was unknown to the Babylonians until the third century BC.  However, attempts have been made to establish a second ideal calendar with seasonal hours alongside the astronomical system of equivalent hours. Bartel Leendert van der Waerden analyzed the Babylonian system of the ideal calendar in 1974.:
The conversion of the BERU double hours does not correspond to the later Greek exact method, but represents only a very inaccurate division of the day.— Bartel Leendert van der Waerden 
Otto Neugebauer reiterated this finding in 1975 as an important distinguishing feature from the later Greek temporal hours.  The duration of the light day and night was measured by the Babylonian astronomers with a gnomon and a water clock further in BERU as well as UŠ. The time periods were divided into equivalent time units with respect to celestial observation. The use of a gnomon in connection with a water clock is documented in the MUL.APIN- cuneiform tablets already around 700 BC. 
From their contents it is clear that the values for the duration of the light day and night were recorded during four colures aligned with the longest and shortest day of the year.  The records have gnomon tables, but they are preserved only for the 15th of Nisan and the 15th of Tammuz. The tables for the 15th Tishrei and the 15th Tevet were at the beginning of the broken away second column. The gnomon tables are written in the form that the length of the gnomon corresponds to a Mesopotamian cubit,  which measured between 40 and 50 cm. 
A 24-hour day contained twelve Dannas,  which in turn, taking into account the Babylonian model of the mean sun, comprised twelve equinoctial units, each lasting 120 minutes  The equivalent hours had the sumerian System of the distance covered on foot in broad daylight as a basis. The unit of measurement, which has a distance of about 10 km as a computational value, is also erroneously called "double hour" in modern literature.