Celestial Sphere Essay

Celestial SphereWhat we see, it contains the stars, orbiters, Sun, and Moon Celestial Equator- the imaginary line that divides the planet into Northern and confederationernern hemispheres. The airy equator is a similar imaginary roach around the supernal sphere, also known as the visible universe. The supernal equator divides the visible universe in twain, creating the Northern and Southern aerial hemispheres. This helps us locate aerial bodies. Ecliptics -an imaginary line on the sky that attach the annual path of the sun. It is the projection of orbs orbit onto the supernal sphere.Besides define the path of the sun, the ecliptic marks the line along which eclipses occur, the moon around and planets and asteroids wander, the Zodiac constellations live. The ecliptic is even the starting delegate for the celestial coordinate system use by astronomers to pin top the location of every star, nebula, and galaxy. Meridian-a great circle of the world pas infernog through the poles and any given point on the humankinds surface. The half of such a circle included surrounded by the poles. Astronomy. the great circle of the celestial sphere that passes through its poles and the commentators zenith. A point or period of highest development,greatest prosperity,or the like. an of the path way sin the body along vital energy flows. Zenith-The point on the celestial sphere that is directly to a higher place the observer.The upper region of the sky.The highest point above the observers horizon attained by a celestial body. Nadir-the point of the celestial spherethat is directly opposite the zenithand vertically downward from the observer Celestial terminals-Either of two diametrically opposite points at which the extensions of the earths bloc intersect the celestial sphere. Either of the two points at which a nitrogen westsideward or conspiracyerlyward projection of the Earths axis intersects the celestial sphere. The magnetic northwest and south cel estial poles are analogous to Earths geographic poles and are used in determining make up ascension in the equatorial coordinate system. Depending on which hemisphere an observer is in, the stars and other celestial objects appear to revolve once around the north or south celestial pole every 24 hours, an military force produced by the rotation of the Earth on its axis.Because of the precession of Earths axis, the celestial poles gradually shift patch in the sky oer a nearly 26,000-year cycle. Solstices-As the Earth travels around the Sun in its orbit, the north-south position (declination) of the Sun changes over the course of the year due to the changing taste of the Earths tilted rotation axes with respect to the Sun. It is this change in the position of the sun that is responsible for seasons.Solstices occur when Sun reaches maximum offsets from the equator intercommunicate on the sky . This offset corresponds to thetilt angle of Earths rotational axis with respect to its orbital plane, called the Earths obliquity.either of the two measure a year when the sun is at its greatest distance from the celestial equator about June 21, when the sun reaches its northernmost point on the celestial sphere, or about Dec. 22, when it reaches its southernmost point. Either of the two points in the ecliptic farthest from the equator.Equinoxes-Either of the two points on the celestial sphere where the ecliptic(the apparent path of the Sun) crosses the celestial equator. The point at which the Suns path crosses the celestial equator moving from south to north is called the vernal equinox. The vernal equinox marks the zero point in both the equatorial and ecliptic coordinate systems horizontal angulate distances are measured eastward from this point.The vernal equinox is also known as the first point of Aries because when first devised some 2,000 years ago this point occurred at the beginning of Aries in the zodiac. The point at which the Suns path crosses the cele stial equator moving from north to south is called the autumnal equinox. Longitude-Lines of longitude, called meridians, run perpendicular to lines of latitude, and all pass through both poles. Each longitude line is part of a great circle. thither is no obvious 0-degree point for longitude, as there is for latitude. Throughout history numerous different starting points have been used to measure longitude. By international agreement, the meridian line through Greenwich, England, is currently given the appraise of 0 degrees of longitude this meridian is referred to as the Prime Meridian.Longitude values are indicate the angular distance between the Prime Meridian and points east or west of it on the surface of the Earth. Latitude-A line connecting all the points with the same latitude value is called a line of latitude. This term is usually used to refer to the lines that even up values in whole degrees. All lines of latitude are collimate to the Equator, and they are sometimes also referred to as parallels. Parallels are equally spaced. There are 90 degrees of latitude going north from the Equator, and the North Pole is at 90 degrees N. There are 90 degrees to the south of the Equator, and the South Pole is at 90 degrees S. When the directional designators are omitted, northern latitudes are given positive values and southern latitudes are given shun values.Right Ascension-The azimuthal angle at which the hour circleof a celestial object is located. The rotation axis taken as the direction of the celestial pole. Right ascension is usually measured in units of time (hours, minutes, and seconds), with mavin hour of time approximately equal to 15 of arc (360/24 hours=15/hour). Declination-On the celestial sphere, the position of a celestial object north or south of the celestial equator. Declination is measured in degrees along a great circle drawn through the object macrocosm measured and the north and south celestial poles, with positive values north o f the celestial equator and negative values south of it, so that the equator itself is 0 and the north and south celestial poles are +90 and -90 declination respectively the angular distance of a celestial body north or to the south of the celestial equator expressed in degrees used with right ascension to determine positions on the celestial sphere