Geodetic Astronomy

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53 Terms

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Celestial Sphere

An imaginary surface whose center is the earth, where all celestial bodies are contained

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360˚ 59.14' per 24 hours

The speed of rotation of the celestial sphere

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celestial pole/s

the apparent axis of rotation of the earth; the points of intersection of the axis of rotation of the earth and the sphere

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celestial equator

A great circle perpendicular to the celestial poles

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Ephemeris

an

astronomic almanac containing tables giving the computed positions of the sun, the planets, and various stars for everyday of a given period

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Equator

Observer's Reference Plane fr observing latitude

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Primary Meridian

Observer's Reference Plane fr observing longitude

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ALTITUDE (H or a)

the angular distance of the body from the horizon as measured along the vertical circle; complement of zenith distance

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AZIMUTH (Z or A)

the angle, measured clockwise along the celestial horizon, from the north or south point to the vertical circle of the star

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ZENITH DISTANCE (z)

the angular distance between the zenith and the celestial body measured along the vertical circle through the body.

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HOUR ANGLE (t or h)

the angle, measured clockwise along the equatorial plane, from the zenith side of the celestial meridian (t = 0°) to the hour circle of the star

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DECLINATION (δ or D)

the angular distance, north or south of the equator, measured along the hour circle from the equator to the body; complement of polar distance

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POLAR DISTANCE (P)

the angular distance between the pole and the celestial body measured along the hour circle through the body

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RIGHT ASCENSION (α)

the angle between the equinoctial colure and the hour circle of the star, measured from the vernal equinox τ, in the plane of the celestial equator

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ECLIPTIC LATITUDE (β)

the angular distance, measured along the ecliptic meridian of the star, between the ecliptic and the direction of the star

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ECLIPTIC LONGITUDE (λ)

the angle measured counterclockwise along the ecliptic, measured from the vernal equinox τ, to the ecliptic meridian of the star

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ECLIPTIC POLAR DISTANCE

the complement of the ecliptic latitude

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Celestial Horizon

the intersection of the observer's horizon/horizontal plane and the celestial sphere

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Celestial Meridian / Observer's Celestial Meridian

the great circle passing through the zenith, nadir and the poles

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Vertical Circles

great circles of the celestial sphere that passes through the zenith and the nadir

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Prime Vertical Circle

vertical circle that is perpendicular to the observer's celestial meridian

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Almucantars

parallels of altitude, intersection of any plane parallel to the celestial horizon and the celestial sphere

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Zenith

the point of intersection (at the top) of the observer's vertical line and the celestial sphere

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Nadir

the point of intersection (at the bottom) of the

observer's vertical line and the celestial sphere

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North Point

the point of intersection of the celestial horizon and observer's celestial meridian nearest to the North Celestial Pole (NCP).

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South Point

the point of intersection of the celestial horizon and observer's celestial meridian nearest to the South Celestial Pole (SCP)

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East and West Point

points of intersection of the prime vertical circle and the celestial horizon

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Hour Circle

any great circle in the celestial sphere that passes through the north and south celestial poles

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6th Hour Circle

hour circle perpendicular to the meridian

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Celestial Parallel

the intersection of any plane parallel to the celestial equator and the celestial sphere

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Ecliptic

the intersection of the plane of the earth's orbit

around the sun and the celestial sphere

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Vernal Equinox

the point of intersection of the celestial equator and the ecliptic (when the sun's declination is 0°) following the winter season

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Autumnal Equinox

the point of intersection of the celestial equator and the ecliptic (when the sun's declination is 0°) following the summer season.

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Winter/Summer Solstice

point on the ecliptic defined when the sun's declination is greatest

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Equinoctial Colure

a great circle in the celestial sphere passing through the celestial poles and the equinoxes

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Solstitial Colure

a great circle in the celestial sphere passing

through the celestial poles and the solstices

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Plane of the Ecliptic

the plane containing the center of the sun, the barycenter of the earth-moon system, and the inertial heliocentric velocity vector of the earth-moon vector of the earth-moon system; plane of orbit of the earth around the sun

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Ecliptic Poles

points of intersection of the line perpendicular

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Ecliptic Parallel

intersection of any plane parallel to the ecliptic and the celestial sphere

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Ecliptic Meridian

great circle in the celestial sphere that passes through the ecliptic poles

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Obliquity of the Ecliptic (ε)

the acute angle between the plane of the ecliptic and the plane of the equator (23.5°)

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PARALLACTIC ANGLE (p or γ)

the angle between the vertical circle and hour circle of the star

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Rising/Setting

Instant when the star intersects the celestial horizon of the place (for equatorial stars only)

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Prime Vertical Crossing

Instant when the star intersects the prime vertical circle

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Culmination/Transit

Instant when the star intersects the celestial meridian

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Elongation

Occurs when the hour circle and vertical circle of star are perpendicular to each other (for Type 1 stars only)

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First-order (Precision) Instruments

Portable instruments which can provide standard deviations of less than 0.3"

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Observatory (High-precision) Instruments

Permanently installed in laboratories; Used for repeated measurements of time and latitude

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Second-order (Geodetic) instruments

Provides standard deviations of less than 1.0"

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Lower order (Surveying) instruments

Used for property and engineering surveys

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parallax

an error observed in vertical angle due to the fact that it is observed on the surface and not on the center of the earth

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Index error

occurs when the instrument's initial vertical angle is not at the zero level, even if the telescope is set to be horizontally leveled

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Refraction of the Ray

The angle of deviation of the ray from its direction at the surface of the earth