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A clock position, or clock bearing, is the direction of an object observed from a vehicle, typically a vessel or an aircraft, relative to the orientation of the vehicle to the observer. The vehicle must be considered to have a front, a back, a left side and a right side. These quarters may have specialized names, such as bow and stern for a vessel, or nose and tail for an aircraft. The observer then measures or observes the angle made by the intersection of the line of sight to the longitudinal axis, the dimension of length, of the vessel, using the clock analogy.
In this analogy, the observer imagines the vessel located on a horizontal clock face with the front at 12:00. Neglecting the length of the vessel, and presuming that he is at the bow, he observes the time number lying on the line of sight. [1] For example, 12 o'clock means directly ahead, 3 o'clock means directly to the right, 6 o'clock means directly behind, and 9 o'clock means directly to the left.
The clock system is not confined to transportation. It has general application to circumstances in which the location of one object with respect to another must be systematized.
This is a system of denoting impromptu relative bearing widely used in practical navigation to give the position of an observed object readily and comprehensibly. "Relative" means that it does not state or imply any compass directions whatsoever. The vessel can be pointed in any direction. The clock numbers are relative to the direction in which the vessel points. The angular distance between adjacent clock numbers is 30 degrees, a round unit that simplifies mathematical juggling. A quick clock number can be shouted by a lookout, whereas after a calculation and comparison of compass points, which might be unknown anyway, it might be too late for the vessel to avoid danger.
As an example of a standard use, the clock position of every approaching vessel is monitored. If the clock number for the observed vessel does not change, it is on a collision course for the observer vessel, as vessels that pass by must change relative bearing. In warfare the clock system is especially useful in drawing attention to enemy locations.
The clock system is easily converted into a 360 degree system for more precise denotation. One bearing, or point, is termed an azimuth. [2] The convention is that of analytic geometry: the y-axis at zero degrees is the longitudinal axis of the vehicle. Angles grow larger in the clockwise direction. Thus, directly to port is at 270 degrees. Negative angles are not used. In navigational contexts, the bearing must be stated as 3 digits: 010 (not so in other contexts). [3] These circles are not to be confused with latitude and longitude, or with any sort of compass reading, which are not relative to the vehicle, but to the magnetic and spin axes of the Earth.
For maritime and aviation applications, the clock bearing is almost always a relative bearing; i.e., the angle stated or implied is angular distance from the longitudinal axis of the vessel or imaginary vessel to the bearing. However, if the 12:00 position is associated with a true bearing, then the observed position is also.
For example, clock position on a 12-hour analog watch can be used to find the approximate bearing of true north or south on a day clear enough for the sun to cast a shadow. The technique takes a line of sight (LOS) on the visible sun, or on the direction pointed to by a shadow stick, through the hour hand of the watch. It exploits the one true bearing of the sun in its course across the sky: the LOS from the observer to the zenith of its course. There the sun is seen mid-way between sunrise and sunset. A vertical plane including sun and observer is perpendicular to the plane of the sun's course. Its intersection with the surface of the earth is a meridian, a line passing through a geographical pole. If the sun is in the southern half of the sky, the zenith bearing points true south; if northern, north. The time at that moment is 12:00 P.M., solar time. The clock position to the observer is 12.
If the watch is set to uncorrected solar time, both hands point to the sun. In a 12-hour watch, the sun and the hour hand both advance, but not at the same rate; the sun covers 15 degrees per hour, and watch 30. To keep the hour hand on the sun, 12:00 must recede from the zenith at the same rate the hour hand advances. Thus when the observer takes an arbitrary LOS, the zenith LOS – true north or south – is to be found at half the angle between 12 and the LOS. On a 24-hour watch, the sun and the hour hand advance at the same rate. There is no need to half the angle.
The zenith LOS is only an approximation due to changes in the time kept by the watch. That time is based on mean solar time rather than observed solar time. Also, time changes with longitude, and the institution of daylight saving time. The time generally available for watch settings in the observer's region is called civil time. It can be corrected to solar time, but LOS on a watch is generally too imprecise to make the trouble worth the effort. [4]
In World War II aircraft pilots needed a quick method of communicating the relative position of threats, for which the clock system was ideal. The gunners of a bomber, or the other aircraft in the squadron, had to be kept informed for purposes of immediate response. However, in aviation, a clock position refers to a horizontal direction. The pilots needed a vertical dimension, so they supplemented the clock position with the word high or low to describe the vertical direction; e.g., 6 o'clock high means behind and above the horizon , while 12 o'clock low means ahead and below the horizon. [5]
The horizon line was only visible in clear weather in daylight, and was only useful as a reference line in straight and level flight, when it appeared on the nose of the aircraft. The vocabulary therefore was only of use during daylight patrols or missions. The reference line and reference clock positions did not exist during combat aerobatics, at night, or during cloudy weather, when other means had to be found for locating the combatants, such as radar.
For airplanes in rapid maneuvers, air traffic controllers will issue the eight cardinal compass points instead. [6]
In 1916, J.B. Plato devised a clock system to identify farms around reference points in rural areas. A clock face was imagined centered on a rural community with 12:00 pointing true north. The circle was divided into concentric numbered bands at each mile of radius. The bands were divided into 12 segments at each position of the clock numbered after the clock hour. Within a segment, every building was assigned a letter. For instance, Alton 3-0 L meant house L in segment 3 of the central circle of 1 mile radius at Alton, where 3 was at 3:00. [7]
Medical pathology uses the clock system to describe the location of breast tumors. A clock face is considered imposed over each breast, left and right, centered on the alveolar region, with the positions shown around it. Tumors are located at one or more subsites, or clock positions, identified by one or more clock numbers. In addition the numbers are arranged in quadrants: Upper Outer Quadrant (UOQ), Lower Inner Quadrant (LIQ), and so on. Codes are assigned to the quadrants, the alveolar region, and the whole breast. [8]
Golf players use the clock system to study the course of the ball in putting situations. For holes that are on a slope, the hole is imagined to be the center of a clock face with 12:00 at the high point and 6:00 at the low point. The ball will only run true when hit from the high or low points; otherwise, its course will break, or bend on the slope. Some golfers practice clock drill – hitting the ball from all the positions of the clock – to learn how it breaks. [9]
An article in the Journal of Applied Microscopy for 1898 recommends the use of a polar coordinate system in the form of a clockface for recording the positions of microscopic objects on a slide. The face is conceived centered on the circle visible under the lens. The pole is the center. Angle is given as a clock number, and distance as a decimal percentage of the radius through the object. For example, “3,9” means 3:00 o'clock at 9 tenths of the radius. [10]
Air traffic controls can only infer the aircraft heading from the ground track of an aircraft, which may not reflect the aircraft's actual heading due to drift angle caused by the wind. As a result, pilots should give due consideration and apply drift correction when an air traffic controller provides traffic advisories. Additionally, the error could also occur when the radar traffic information is issued while the aircraft is changing course. [11]
Although the raw clock position is invaluable or indispensable in many circumstances requiring rapid response, for ordinary careful navigation it is not sufficiently precise. It can be made precise by various methods requiring the use of instruments.
The clock face with its clock positions is a heritage of Roman civilization, as is suggested by the survival of Roman numerals on old clocks and their cultural predecessors, sundials. The mechanical clock supplanted the sundial as the major timekeeper, while the Hindu–Arabic numeral system replaced the Roman as the number system in Europe in the High Middle Ages. The Romans, however, had adapted their timekeeping system from the Ancient Greek. The historical trail leads from there to ancient Mesopotamia through the ancient Greek colonies placed on the coast of Anatolia in the 1st millennium BC. The first known historian, Herodotus of Halicarnassus, who was a native of that border region, made the identification:
The polos (“pole”) was a sundial of a concave face resembling the concavity of the universe (named a “pole” in this case). [13] The gnomon was the pointer.
The Babylonian time system is documented by thousands of Mesopotamian cuneiform tablets. The Babylonians inherited the better part of their system from the Sumerians, whose culture they absorbed. Tablets of different periods reveal the development of a sexagesimal numbering system from decimal and duodecimal systems, which reveals itself in the construction of unique symbols for numerals 1-59 from natural finger decimals (ten fingers, ten symbols). Why they developed this system is a matter for academic debate, but there are multiple advantages, including division by several factors, offering several possible subdivisions, one of which is by 12's. [14] Classical civilization adopted and adapted the Mesopotamian time system, and modern civilization adapted it still further. The modern system retains much of the sexagesimalism of the Sumerians, but typically not with the same detail. [15]
Time today and generally in ancient Mesopotamia is given mainly in three digits. Today's state the hours , minutes , and seconds . In a strict sexagesimal system these three would be expressed in a single, three-digit sexagesimal number: h,m,s with values on each of the three letters of 0-59; that is, hours up to 60, minutes up to 60, and seconds up to 60. Because integer numbers are expressed as sums, in this case
for the number of seconds, h, m, and s can be broken out and treated as separate numbers. Each number, however, implies the other two; e.g., a minute implies 60 seconds. m and s are straightforward, but h is different. There are no explicit 60 hours; the number instead is 24, and yet they are part of an implied sexagesimal system. 60 minutes is implied by one of the 24 hours, not one of the 60. The system is not strictly sexagesimal but is based on the sexagesimal.
A full Babylonian time determination also had three digits. [16] Zeros were blank spaces, causing some difficulty of discerning them from character separators. For reasons that are not clear, the Mesopotamians adopted a standard of 12 hours per day for their first-order digit. Their day, however, was designed for measurement on their most ancient and widely used timepiece, the sundial, which showed only daylight hours. Daylight was the time between sunrise and sunset, each of those being defined as the appearance or disappearance of the top rim of the sun on the horizon. Daylight hours problematically were seasonal; that is, due to the variation of the length of the day with time of year, hour length was variable also. The Mesopotamians had discovered, however, that if the darkness was divided into 12 hours also, and each run of 12 was matched number for number: 1st to 1st, 2nd to 2nd, etc., the sum of each match was constant. [17]
The 12-hour, seasonal day was one of many metrological arrangements that had developed during the 3rd millennium BC. It was in use in the Ur III period, at the end of the 3rd millennium. [18] The vocabulary of time was not yet set. For example, the 60-hour day existed as the time-shekel, 1/60 of a working day, presumably so named from the labor cost of one hexagesimal hour. This was a time of strong kings and continuing administrations that took responsibility for weights and standards. Englund distinguishes two main types of system: the cultic, in which the events of the seasonal calendar assume religious significance, and are perpetuated for religious reasons, and a second, new type, the state, defined by an administration that needed to standardize its time units.
The state system came to predominate in the subsequent Old Babylonian period. The state administrators had perceived that the sun advances at a uniform rate no matter what the season. One sun cycle is always the same. Moreover, it matches the cycle of rotation of the stars around the pole star, the real reason being that the Earth rotates at a constant angular velocity. If hours were to represent divisions of the uniform rotation, they must also be uniform, and not be variable. There were two days of the year when all 24 hours were of the same length: the two equinoxes. The standard double hour (beru), of equinoctial length, representing two modern hours, of which there were 12 in the standard day (umu), was not conceived as being one of day and one of night, but as being just two consecutive equal-length hours. One standard day thus went on to become two consecutive equal 12-hour clockfaces in modern clock time. 30 standard days were a standard month, and 12 of those a standard year of 360 days. Some juggling of month lengths to make the 12 months fit the year was still required.
Within a day, single hours were unreliable. They came in all sizes. The double hour, however, originally the sum of a daylight hour and the corresponding night hour, was always the same. The statists therefore chose to use double units in definition. The 12-hour daytime had been divided into three seasonal watches. These were matched to three seasonal night watches, 1st to 1st, 2nd to 2nd, etc. One double watch (8 hours) was four double hours. One single watch (four hours) was two double hours.
To produce a second-order digit of a Babylonian time, the statists changed from solar to stellar time. The stars moved in visible circles at a fixed rate, which could be measured by the constant escape of water from a water clock. The single standard watch of 4 hours (two double hours) was divided into 60 time-degrees (ush). One double hour had 30, and one complete stellar day, 360 (12 times 30). [19] This assignment was the creation of the 360-degree circle, as the degree went from being a time division to an angular distance of rotation. Time-degrees were all the same (one is about 4 minutes of modern time). The second-order digit counted the degrees that had gone by in the hour, notwithstanding the fact that its number of degrees were seasonal.
The third and last order digit divided the time-degree into 60 parts (the gar), which appears to be sexagesimal. In modern time it is 4 seconds. There are not 60 time-degrees in an hour, nor 60 hours in a day. The Babylonian time was thus three different numbers, only one of which was sexagesimal. Only its general features are modern: the 12-hour day followed by a 12-hour night, the 60-division 3rd-order digit, and the 360-degree circle.
The 1949 movie Twelve O'Clock High takes its title from the system. In this case, the position would be ahead and above the horizon, an advantageous position for the attacker.
The phrase "on your six" refers to the six o'clock or the adjacent positions; that is, the expression cautions that someone is behind you or on your tail.
A minute of arc, arcminute (arcmin), arc minute, or minute arc, denoted by the symbol ′, is a unit of angular measurement equal to 1/60 of one degree. Since one degree is 1/360 of a turn, or complete rotation, one arcminute is 1/21600 of a turn. The nautical mile (nmi) was originally defined as the arc length of a minute of latitude on a spherical Earth, so the actual Earth's circumference is very near 21600 nmi. A minute of arc is π/10800 of a radian.
An hour is a unit of time historically reckoned as 1⁄24 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.
The second is a unit of time, historically defined as 1⁄86400 of a day – this factor derived from the division of the day first into 24 hours, then to 60 minutes and finally to 60 seconds each.
In astronomy and celestial navigation, the hour angle is the dihedral angle between the meridian plane and the hour circle.
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.
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 over the course of a year. The change of position is a result of the shifting of the angle in the sky of the path that the Sun takes in respect to the stars. The diagram resembles a figure eight. Globes of the Earth often display an analemma as a two-dimensional figure of equation of time vs. declination of the Sun.
Sexagesimal, also known as base 60, is a numeral system with sixty as its base. It originated with the ancient Sumerians in the 3rd millennium BC, was passed down to the ancient Babylonians, and is still used—in a modified form—for measuring time, angles, and geographic coordinates.
Solar time is a calculation of the passage of time based on the position of the Sun in the sky. The fundamental unit of solar time is the day, based on the synodic rotation period. Traditionally, there are three types of time reckoning based on astronomical observations: apparent solar time and mean solar time, and sidereal time, which is based on the apparent motions of stars other than the Sun.
Celestial navigation, also known as astronavigation, is the practice of position fixing using stars and other celestial bodies that enables a navigator to accurately determine their actual current physical position in space or on the surface of the Earth without relying solely on estimated positional calculations, commonly known as dead reckoning. Celestial navigation is performed without using satellite navigation or other similar modern electronic or digital positioning means.
Babylonian cuneiform numerals, also used in Assyria and Chaldea, were written in cuneiform, using a wedge-tipped reed stylus to print a mark on a soft clay tablet which would be exposed in the sun to harden to create a permanent record.
Noon is 12 o'clock in the day. 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.
In navigation, bearing or azimuth is the horizontal angle between the direction of an object and north or another object. The angle value can be specified in various angular units, such as degrees, mils, or grad. More specifically:
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 has been developed since the second millennium BC and reached its modern form in the 16th century.
Midnight sun, also known as polar day, is a natural phenomenon that occurs in the summer months in places north of the Arctic Circle or south of the Antarctic Circle, when the Sun remains visible at the local midnight. When midnight sun is seen in the Arctic, the Sun appears to move from left to right. In Antarctica, the equivalent apparent motion is from right to left. This occurs at latitudes ranging from approximately 65°44' to exactly 90° north or south, and does not stop exactly at the Arctic Circle or the Antarctic Circle, due to refraction.
The equation of time describes the discrepancy between two kinds of solar time. The word equation is used in the medieval sense of "reconciliation of a difference". The two times that differ are the apparent solar time, which directly tracks the diurnal motion of the Sun, and mean solar time, which tracks a theoretical mean Sun with uniform motion along the celestial equator. Apparent solar time can be obtained by measurement of the current position of the Sun, as indicated by a sundial. Mean solar time, for the same place, would be the time indicated by a steady clock set so that over the year its differences from apparent solar time would have a mean of zero.
An analog watch (American) or analogue watch is a watch whose display is not digital but rather analog with a traditional clock face. The name is an example of a retronym; it was coined to distinguish analog watches, which had simply been called "watches", from newer digital watches. It strictly refers to the design of the display, regardless of the timekeeping technology used within the watch movement or module, although its counterpart, "digital watch", usually connotes digital electronics in both. A digital watch is one in which the time is displayed as a series of digits, e.g. "04:32". An analog watch is one in which the display is not digital, but is indicated (typically) by the continuous motion of one, two, or three rotating pointers or hands pointing to numbers arrayed on a circular dial.
A degree, usually denoted by °, is a measurement of a plane angle in which one full rotation is 360 degrees.
Babylonian mathematics is the mathematics developed or practiced by the people of Mesopotamia, as attested by sources mainly surviving from the Old Babylonian period to the Seleucid from the last three or four centuries BC. With respect to content, there is scarcely any difference between the two groups of texts. Babylonian mathematics remained constant, in character and content, for over a millennium.
The Whitehurst & Son sundial was produced in Derby in 1812 by the nephew of John Whitehurst. It is a fine example of a precision sundial telling local apparent time with a scale to convert this to local mean time, and is accurate to the nearest minute. The sundial is now housed in the Derby Museum and Art Gallery.
Direction determination refers to the ways in which a cardinal direction or compass point can be determined in navigation and wayfinding. The most direct method is using a compass, but indirect methods exist, based on the Sun path, the stars, and satellite navigation.