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   » » Wiki: Heliacal Rising
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The heliacal rising ( ) of a or a occurs annually when it becomes visible above the eastern at just before (thus becoming "the morning star"). A heliacal rising marks the time when a star or planet becomes visible for the first time again in the after having set with the Sun at the western horizon in a previous (its heliacal setting), having since been in the only during , obscured by sunlight.

Historically, the most important such rising is that of , which was an important feature of the Egyptian calendar and astronomical development. The rising of the heralded the start of the sailing season, using celestial navigation, as well as the farming season (attested by in his Works and Days). Heliacal rising is one of several types of risings and settings, mostly they are grouped into morning and evening risings and settings of objects in the sky. in the evening and then morning is set apart by half a year, while on the other hand risings and settings in the evenings and the mornings are only at the equator set apart by half a year.


Cause and significance
Relative to the stars, the Sun appears to drift eastward about one degree per day along a path called the because there are 360 degrees in any complete revolution (circle), which takes about 365 days in the case of one revolution of the Earth around the Sun. Any given "distant" star in the belt of the ecliptic will be visible at night for only half of the year, when it will always remain below the horizon. During the other half of the year it will appear to be above the horizon but not visible because the sunlight is too bright during the day. The star's heliacal rising will occur when the Earth has moved to a point in its orbit where the star appears on the eastern horizon at dawn. Each day after the heliacal rising, the star will rise slightly earlier and remain visible for longer before the light from the rising sun overwhelms it. Over the following days the star will move further and further westward (about one degree per day) relative to the Sun, until eventually it is no longer visible in the sky at sunrise because it has already set below the western horizon. This is called the acronycal setting.

The same star will reappear in the eastern sky at dawn approximately one year after its previous heliacal rising. For stars near the , the small difference between the and due to will cause their heliacal rising to recur about one (about 365.2564 days) later, though this depends on its . For stars far from the ecliptic, the period is somewhat different and varies slowly, but in any case the heliacal rising will move all the way through the in about 26,000 years due to precession of the equinoxes.

Because the heliacal rising depends on the observation of the object, its exact timing can be dependent on weather conditions.

Heliacal phenomena and their use throughout history have made them useful points of reference in .


Non-application to circumpolar stars
Some stars, when viewed from not at the , do not rise or set. These are , which are either always in the sky or never. For example, the (Polaris) is not visible in Australia and the is not seen in Europe, because they always stay below the respective horizons.

The term circumpolar is somewhat localised as between the Tropic of Cancer and the Equator, the Southern polar constellations have a brief spell of annual visibility (thus "heliacal" rising and "cosmic" setting) and the same applies as to the other polar constellations in respect of the reverse tropic.


History
Constellations containing stars that rise and set were incorporated into early or . The , , Egyptians, and all used the heliacal risings of various stars for the timing of agricultural activities.

Because of its position about 40° off the ecliptic, the heliacal risings of the bright star in occurred not over a period of exactly one but over a period called the "" (from "Sothis", the name for the star Sirius). The Sothic year was about a minute longer than a Julian year of 365.25 days.. Since the development of , this has occurred at approximately on July 19 on the .. Its returns also roughly corresponded to the onset of the annual flooding of the , although the flooding is based on the tropical year and so would occur about three quarters of a day earlier per century in the Julian or Sothic year. (July 19, 1000 BC in the Julian Calendar is July 10 in the proleptic Gregorian Calendar. At that time, the sun would be somewhere near in Leo, where it is around August 21 in the 2020s.) The ancient Egyptians appear to have constructed their 365-day civil calendar at a time when Wep Renpet, its , corresponded with Sirius's return to the night sky. Although this calendar's lack of caused the event to shift one day every four years or so, astronomical records of this displacement led to the discovery of the and, later, the establishment of the more accurate and Alexandrian calendars.

The Egyptians also devised a method of telling the time at night based on the heliacal risings of 36 , one for each 10° segment of the 360° circle of the zodiac and corresponding to the ten-day "weeks" of their civil calendar.

To the Māori of , the are called , and their heliacal rising signifies the beginning of the new year (around June). The of called the Pleiades Ngauponi which in the vicinity of the (Mapuche new year) will disappear by the west, lafkenmapu or ngulumapu, appearing at dawn to the East, a few days before the birth of new life in nature. Heliacal rising of Ngauponi, i.e. appearance of the Pleiades by the horizon over an hour before the sun approximately 12 days before the winter solstice, announced we tripantu.

When a planet has a heliacal rising, there is a conjunction with the sun beforehand. Depending on the type of conjunction, there may be a syzygy, , transit, or of the sun.


Acronycal and cosmic(al)
The rising of a planet above the eastern horizon at is called its rising, which for a signifies an opposition, another type of syzygy. When the Moon has an acronycal rising, it will occur near and thus, two or three times a year, a noticeable .

can refer to rising with sunrise or setting at sunset, or the first setting at morning twilight.

Risings and settings are furthermore differentiated between apparent (the above discussed) and actual or true risings or settings.


Overview
The use of the terms cosmical and acronycal is not consistent. The following table gives an overview of the different application of the terms to the rising and setting instances.

Morning (matutinal)True (in daylight)CosmicalAcronycal/Cosmical
Apparent (in twilight)Heliacal
(first appearance)
Heliacal/Cosmical
(last morning appearance)
Evening (vesper)True (in daylight)AcronycalCosmical/Acronycal
Apparent (in twilight)Heliacal/Acronycal
(first evening appearance)
Heliacal
(last night sky appearance)


See also


Notes
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