Why can a total solar eclipse observed in New Zealand not be observed in Mexico? Due to Earth's tilt on its axis, the Moon's shadow falls only on the Southern Hemisphere of Earth during a total solar eçlipse. Outside this hemisphere, a total solar eclipse cannot be observed. Due to the Moon's small size relative to Earth, the Moon's shadow falls only on a small area of Earth during a total solar eclipse. Outside this area, a total solar eclipse cannot be observed. Due to Earth's small size relative to the Sun, the Moon's shadow never extends north of the equator during a total solar eclipse. North of the equator, a total solar eclipse cannot be observed. Due to the Moon's position around Earth, the Moon's shadow never falls near the equator during a total solar eclipse. For areas near the equator, a total solar eclipse cannot be observed.
Why can a total solar eclipse observed in New Zealand not be observed in Mexico? Due to Earth's tilt on its axis, the Moon's shadow falls only on the Southern Hemisphere of Earth during a total solar eçlipse. Outside this hemisphere, a total solar eclipse cannot be observed. Due to the Moon's small size relative to Earth, the Moon's shadow falls only on a small area of Earth during a total solar eclipse. Outside this area, a total solar eclipse cannot be observed. Due to Earth's small size relative to the Sun, the Moon's shadow never extends north of the equator during a total solar eclipse. North of the equator, a total solar eclipse cannot be observed. Due to the Moon's position around Earth, the Moon's shadow never falls near the equator during a total solar eclipse. For areas near the equator, a total solar eclipse cannot be observed.
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
Section: Chapter Questions
Problem 1LR
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