hour angle oor Masedonies

hour angle

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en
(astronomy) the angular distance of a celestial point measured westward along the celestial equator from the zenith crossing; the right ascension for an observer at a particular location and time of day

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unit of angle
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Mean solar time is the hour angle of the mean Sun plus 12 hours.
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For example, at 10:30 AM local apparent time the hour angle is -22.5° (15° per hour times 1.5 hours before noon).
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Observing the sun from earth, the solar hour angle is an expression of time, expressed in angular measurement, usually degrees, from solar noon.
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Negative hour angles indicate the time until the next transit across the meridian; an hour angle of zero means the object is on the meridian.
Не ми е грижаWikiMatrix WikiMatrix
The hour angle is paired with the declination to fully specify the location of a point on the celestial sphere in the equatorial coordinate system.
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In astronomy and celestial navigation, the hour angle is one of the coordinates used in the equatorial coordinate system to give the direction of a point on the celestial sphere.
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At solar noon the hour angle is 0.000 degree, with the time before solar noon expressed as negative degrees, and the local time after solar noon expressed as positive degrees.
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In astronomy, hour angle is defined as the angular distance on the celestial sphere measured westward along the celestial equator from the meridian to the hour circle passing through a point.
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In astronomy, declination (abbreviated dec; symbol δ) is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle.
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The hour angle of a point is the angle between two planes: one containing Earth's axis and the zenith (the meridian plane), and the other containing Earth's axis and the given point (the hour circle passing through the point).
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During this time, it has passed overhead (culmination) once and underfoot once (at an hour angle of 00:00 and 12:00 respectively), so in many places the period of strongest tidal forcing is the above-mentioned, about 12 hours and 25 minutes.
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At solar noon, h = 0.000 so cos(h)=1, and before and after solar noon the cos(± h) term = the same value for morning (negative hour angle) or afternoon (positive hour angle), i.e. the sun is at the same altitude in the sky at 11:00AM and 1:00PM solar time, etc. The sidereal hour angle (SHA) of a body on the celestial sphere is its angular distance west of the vernal equinox generally measured in degrees.
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This bird has reached a speed of 217 miles per hour [349 km/hr] at a 45-degree angle of descent!
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These angles can be measured in time (24 hours to a circle) or in degrees (360 degrees to a circle)— one or the other, not both.
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Was it mere chance that caused the earth to move around the sun at just the right speed, to rotate on its axis every 24 hours, and to have just the correct angle of tilt?
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15 sinne gevind in 9 ms. Hulle kom uit baie bronne en word nie nagegaan nie.