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QUESTION 1 Match the following coordinates or properties up to their corresponding definitions: A, This is the point found directly overhead for an observer. The stars that pass through this point will change depending on the observer's location. H. v Horizon A. v Zenith C. v Altitude B. This is one of the coordinates used in the celestial equatorial system and it measures the angle that a target makes North or South of the celestial equator on the celestial sphere. C. This is one of the coordinates used in the local horizon system and it measures how high something appears to be in the sky for an observer at a given time. B. v Azimuth F. v Declination E. v Right Ascension D. This line is similar to the Prime Meridian on Earth in that it is a relatively arbitrarily chosen zero point for one of the equatorial coordinates. E. This is one of the coordinates used in the celestial equatorial system and it measures how far along the celestial sphere something appears relative to the Sun's position at the time of the vernal equinox. It is measured in units of hours, minutes, and seconds and increases to the East. D. v Vernal Equinox Point G. v Celestial Equator F. This is a projection of the line that encompasses the Earth from which we measure latitude. As a result, we measure a celestial coordinate that is similar to latitude relative to this line. G. This is one of the coordinates used in the local horizon system and it measures the angle from due North that a target is found for a given location and time as the angle increases towards the East. H. This is the line where an observer's ground meets the sky. From this line, we are able to measure how high something appears in the sky or how far along this line something is from due North for an observer at a given time.

QUESTION 1 Match the following coordinates or properties up to their corresponding definitions: A, This is the point found directly overhead for an observer. The stars that pass through this point will change depending on the observer's location. H. v Horizon A. v Zenith C. v Altitude B. This is one of the coordinates used in the celestial equatorial system and it measures the angle that a target makes North or South of the celestial equator on the celestial sphere. C. This is one of the coordinates used in the local horizon system and it measures how high something appears to be in the sky for an observer at a given time. B. v Azimuth F. v Declination E. v Right Ascension D. This line is similar to the Prime Meridian on Earth in that it is a relatively arbitrarily chosen zero point for one of the equatorial coordinates. E. This is one of the coordinates used in the celestial equatorial system and it measures how far along the celestial sphere something appears relative to the Sun's position at the time of the vernal equinox. It is measured in units of hours, minutes, and seconds and increases to the East. D. v Vernal Equinox Point G. v Celestial Equator F. This is a projection of the line that encompasses the Earth from which we measure latitude. As a result, we measure a celestial coordinate that is similar to latitude relative to this line. G. This is one of the coordinates used in the local horizon system and it measures the angle from due North that a target is found for a given location and time as the angle increases towards the East. H. This is the line where an observer's ground meets the sky. From this line, we are able to measure how high something appears in the sky or how far along this line something is from due North for an observer at a given time.

Applications and Investigations in Earth Science (9th Edition)
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
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QUESTION 1 Match the following coordinates or properties up to their corresponding definitions: A. This is the point found directly overhead for an observer. The stars that pass through this point will change depending on the observer's location. H. v Horizon A. v Zenith B. This is one of the coordinates used in the celestial equatorial system and it measures the angle that a target makes North or South of the celestial equator on the celestial sphere. v Altitude C. This is one of the coordinates used in the local horizon system and it measures how high something appears to be in the sky for an observer at a given time. B. v Azimuth F. v Declination D. This line is similar to the Prime Meridian on Earth in that it is a relatively arbitrarily chosen zero point for one of the equatorial coordinates. E. v Right Ascension D. v Vernal Equinox Point E. This is one of the coordinates used in the celestial equatorial system and it measures how far along the celestial sphere something appears relative to the Sun's position at the time of the vernal equinox. It is measured in units of hours, minutes, and seconds and increases to the East. G. v Celestial Equator E. This is a projection of the line that encompasses the Earth from which we measure latitude. As a result, we measure a celestial coordinate that is similar to latitude relative to this line. G. This is one of the coordinates used in the local horizon system and it measures the angle from due North that a target is found for a given location and time as the angle increases towards the East. H. This is the line where an observer's ground meets the sky. From this line, we are able to measure how high something appears given time. sky or how far along this line something is from due North for an observer at a QUESTION 2 In the local horizon coordinate system, the line that arcs from due North to due South through the zenith is called the local meridian It is of particular interest to astronomers because the altitude of stars as they cross this line represents the North or South that it will be for a given location. This is because an object's altitude should be increasing (choose increasing or decreasing) to the East of this line or decreasing (choose increasing or decreasing) to the West of this line.
Transcribed Image Text:QUESTION 1 Match the following coordinates or properties up to their corresponding definitions: A. This is the point found directly overhead for an observer. The stars that pass through this point will change depending on the observer's location. H. v Horizon A. v Zenith B. This is one of the coordinates used in the celestial equatorial system and it measures the angle that a target makes North or South of the celestial equator on the celestial sphere. v Altitude C. This is one of the coordinates used in the local horizon system and it measures how high something appears to be in the sky for an observer at a given time. B. v Azimuth F. v Declination D. This line is similar to the Prime Meridian on Earth in that it is a relatively arbitrarily chosen zero point for one of the equatorial coordinates. E. v Right Ascension D. v Vernal Equinox Point E. This is one of the coordinates used in the celestial equatorial system and it measures how far along the celestial sphere something appears relative to the Sun's position at the time of the vernal equinox. It is measured in units of hours, minutes, and seconds and increases to the East. G. v Celestial Equator E. This is a projection of the line that encompasses the Earth from which we measure latitude. As a result, we measure a celestial coordinate that is similar to latitude relative to this line. G. This is one of the coordinates used in the local horizon system and it measures the angle from due North that a target is found for a given location and time as the angle increases towards the East. H. This is the line where an observer's ground meets the sky. From this line, we are able to measure how high something appears given time. sky or how far along this line something is from due North for an observer at a QUESTION 2 In the local horizon coordinate system, the line that arcs from due North to due South through the zenith is called the local meridian It is of particular interest to astronomers because the altitude of stars as they cross this line represents the North or South that it will be for a given location. This is because an object's altitude should be increasing (choose increasing or decreasing) to the East of this line or decreasing (choose increasing or decreasing) to the West of this line.
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