The scientific study of the universe beyond the earth especially the observation, calculation, and theoretical interpretation of the positions, dimensions, Distribution, motion, composition, and evolution of celestial bodies and phenomena
Prior to 1609, when the telescope was invented, the naked eye was used for measurements
Astronomical geodesy
A technique that uses the sun, moon, stars, and other natural objects as beacons; takes the celestial horizon coordinates of such objects as observations; and finally determines the geographical position of the station and the azimuth of one direction
Celestial Sphere
An imaginary sphere on which are projected objects in space
Used to locate the positions of real and imaginary celestial objects
Components of the Celestial Sphere
Zenith (Z)
Nadir (Z')
North Celestial Pole (P)
South Celestial Pole (P')
Polar Axis
Observer's Vertical
Observer's Meridian Circle
Observer's Horizon
Vertical Circle
Celestial Equator
Hour Circle
Polaris
The star in the center of the star field that shows essentially no movement because Earth's axis points almost directly to it
The east to west daily motions of stars, planets, the Moon, and the Sun are caused by the rotation of the Earth on its axis
Constellations with respect to the North Pole
Polaris is the last star in the tail of the constellation Ursa Minor and is located by finding the constellation of Ursa Major first
The two outermost stars in the cup of the "dipper" (Merak and Dubhe) are called the "pointers" because they describe a straight line that points to the North Star
The constellation of Cassiopeia, which looks like a big "W", is always opposite Ursa Major
Polaris rotates in a counter clockwise direction and makes a complete revolution in approximately every 24 hours
Horizon System
Uses the observer's local horizon as the fundamental plane to define two angles: altitude and azimuth
Primary Reference: THEHORIZON
Secondary Reference: VERTICALCIRCLES
ALTITUDE – angle from the horizon to star
AZIMUTH – the angular distance measured along the horizon
from the observer’s meridian to the vertical circle through the
body.
EquatorialSystem
Uses two measurements: right ascension and declination Right ascension (abbreviated RA) is similar to longitude and is measured in hours, minutes and seconds eastward along the celestial equator.
References: Equator, Hourcircles
parameter: Declination - angle from the equator to the star; RightAscension - The angle taken counter clockwise along the celestial equator from the first point of Aries to the hour circle of the star.
Equinox
Vernal Equinox: Two moments in the year when the Sun is exactly above the Equator and day and night are of equal length
Autumnal Equinox: Two moments in the year when the Sun is exactly above the Equator and day and night are of equal length
Solstice
Summer Solstice: Two moments during the year when the path of the Sun in the sky is farthest north in the Northern Hemisphere (June 20 or 21) or farthest south in the Southern Hemisphere (December 21 or 22)
Winter Solstice: Twomoments during the year when the path of the Sun in the sky is farthest south in the Northern Hemisphere (December 21 or 22) and farthest north in the Southern Hemisphere (June20 or 21)
the imaginary point that is directly above an observe
Zenith
the point on the celestial sphere directly below an observer
Nadir
the point in the sky about which all the stars seen from the
Northern Hemisphere rotate
North Celestial Pole
he point in the sky about which all the stars seen from the
Southern Hemisphere rotate
South Celestial Pole
an imaginary line that extends through the north and
south geographic poles
Polar axis
A vertical line at the position of the observer coincides with the
plumb line and is normal to the observer's horizon plane
Observer’sVertical
a great circle on the celestial sphere that passes through the north and south points of the horizon as well as through the zenith of the observer.
Observer’s Meridian Circle
any great circle (similar to longitude) on the celestial sphere that passes through the celestial poles that is perpendicular to the plane of celestial equator
Hour Circle
great circle of celestial sphere where plane, perpendicular to the plumb line(observer's vertical) at the place of observation and passing through the center of the earth
observer'shorizon
a circle perpendicular to the polar axis, which is the extension of the earth's equator
celestialequator
circle which is perpendicular to the observer's horizon and passes through the observer's zenith and any celestial body.
verticalcircle
orbit sequence of the Polaris
upperculmination, easternelongation, lowerculmination, westernelongation. The middle is the celestialnorthpole
the position of the celestial body is based on the location of the observer
Hour Angle System
Hour Angle system
LOCAL HOUR ANGLE (LHA)-The angle measured clockwise from the upper branch of the meridian of observation to the meridian of the celestial body.
SIDEREAL HOUR ANGLE (SHA)-The angle measured clockwise from the meridian of the First Point of Aries to the meridian of the body.
GREENWICH HOUR ANGLE (GHA)-The angle measured clockwise from the Greenwich meridian to meridian of the celestial body