Showing posts with label The Celestial Sphere. Show all posts
Showing posts with label The Celestial Sphere. Show all posts

Thursday, May 31, 2012

"The Celestial Sphere - Astronomy's Model of the Apparently Changing Night Sky"

"The Celestial Sphere - Astronomy's Model of the Apparently Changing Night Sky"," To add to this confusion, printed star charts frequently show the sky as a circle, and in addition make reference to the cardinal points. The idea of a celestial sphere is not new. In our enlightened age we scoff at this idea, yet it remains a very useful model of the night sky. In order to grasp the concept of the celestial sphere, try to visualise an imaginary straight line that passes through Earth's north and south poles and extends to infinity at either end. Then the celestial north pole is located where this imaginary line extends from Earth's north pole and passes through the celestial sphere; the celestial south pole is on the opposite side. THIS IS HOW YOU DO IT","night sky","99%" "The Night Sky Zone"," It's as if we're inside of some great celestial (sky) sphere upon which the stars appear to be attached. In science we like to use models to illustrate abstract concepts. The International Astronomical Union officially designated a total of 88 constellations in the entire celestial sphere in 1930. A circular cardboard cutout looking like a star map freely rotating on a central pivot and connected to a square cardboard piece can be set to a time and day of the month while facing a certain direction. Recognizing stars and constellations is a good start, but locating much smaller, specific areas of the sky requires a detailed set of star charts. Lines representing streets and roads going north-south and east-west on our earth map can be turned into lines representing celestial coordinates on our sky map. These celestial lines of latitude north and south of the equator are now called lines of declination. Each degree can be further subdivided into 60 equal minutes (not time) of arc (part of the circle formed by the complete line) and each minute divided into 60 equal seconds (again, not time) of arc. One minute of arc at the Earth's celestial equator is approximately equal to one nautical mile on the earth. They measure hour angles increasing westward from 1 to 24 (0 and 24 are the same line) and are subdivided further into minutes and seconds of actual time. Equatorial mountings for telescopes can incorporate setting circles to manually align the instrument or use computers and motors to locate and track celestial objects. . WHAT'S UP

     

Monday, April 2, 2012

The Celestial Sphere - Astronomy's Model of the Apparently Changing Night Sky

"The Celestial Sphere - Astronomy's Model of the Apparently Changing Night Sky"," To add to this confusion, printed star charts frequently show the sky as a circle, and in addition make reference to the cardinal points. The idea of a celestial sphere is not new. In our enlightened age we scoff at this idea, yet it remains a very useful model of the night sky. In order to grasp the concept of the celestial sphere, try to visualise an imaginary straight line that passes through Earth's north and south poles and extends to infinity at either end. Then the celestial north pole is located where this imaginary line extends from Earth's north pole and passes through the celestial sphere; the celestial south pole is on the opposite side. However, you know - but your ancestors didn't know - that the earth rotates about its polar axis from west to east once in 24 hours. The way in which these apparent movements occur depend on where you are situated on the earth's surface. On the other hand, for a person standing at one of the poles, the horizon coincides with the celestial equator, and it would appear that half the sky, i. , the part above the horizon, is turning about the pole - clockwise at the north pole, and anti-clockwise at the south pole. The height of the pole in degrees corresponds to the observers latitude. Then the celestial south pole would be located 30 degrees above your southern horizon. Of course, the same would apply if you found yourself in the northern hemisphere. A person who is familiar with the night sky would know that any given star appears to rise about four minutes earlier every night as seen from a particular place on Earth. It is this motion that changes our vantage point with respect to the background stars. . WHAT'S UP