Related Category: Astronomy: General
in astronomy, a coordinate in the equatorial coordinate system.
The angle between an observer's and the on which some celestial body lies.
Hour Angle The angle, measured westwards around the celestial equator, between the observer's meridian and the hour circle of an object.
The angle to an object measured westward from the prime meridian (the great circle for a particular observer which goes through the celestial poles and the zenith).
the telescope based coordinate specifying the angle, in the equatorial plane, from the meridian to a plane containing the celestial object and the north and south celestial poles.
H-R Diagram ...
Angular distance on the celestial sphere measured westward along the celestial equator from the meridian to the hour circle that passes through a celestial object.
Hour Circle ...
The sidereal time that has elapsed since the object was on the meridian (hour angle west, positive) or until it will again be on the meridian (hour angle east, negative).
Of a celestial object as seen from a particular location, the difference between the local sidereal time and the right ascension (H.A. = L.S.T. - R.A.).
H-R diagram - (n.) ...
An hour angle referred to the ephemeris meridian. [S92]
Longitude (see Longitude, Terrestrial) measured eastward from the ephemeris meridian. [S92]
Ephemeris Meridian ...
the system is fixed to the Earth like the geographic coordinate system ...
HA; hour angle ((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) ...
right ascension (RA, ),
local (LHA) ...
hour angle Angular distance west of a celestial meridian or hour circle; the arc of the celestial equator, or the angle at the celestial pole, ...
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The next concept we want to define is that of an hour angle. For this, we first define the hour circle as a great circle on the celestial sphere that passes through the north and south celestial poles (which are directly above the north and south ...
This method works even with the oldest-style setting circles that only read from the celestial meridian instead of right ascension.
2.04 The point directly overhead an observer is the...
These deposits will then appear slightly darker than they would if sunlight was directly reflected at the observer. If that same deposit were nearer to the noon then more sunlight would reflect back and it would appear brighter.
Information was acquired during the cislunar, the photo ellipse, and the extended mission (from end of the photographic mission to July 11, 1967) phases. Doppler, ranging, hour angle points, ...
See also: Earth, Astro, Sun, Solar, Orbit