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Moon and Seasons

Earth Science

QuestionAnswer
Highlands mountain ranges that soar thousands of meters into the black sky. Appear as the light areas we see on the moon. Made of rocks called Anorthosites.
Rilles long valleys that crisscross most of its surface. May prove that there was previous volcanic activity, thought to be leftover lava channels/
Maria dark areas of solidified lava are flat plains. They are dark because they reflect less light/
Rays bright streaks that extend out from impact area/
Regolith crushed rock and dust (lunar surface is covered in it)/
Craters Bowl shaped depression made from leftover debris from solar system formation that struck the moon/
Crust near side is thinner than far side, far side more mountainous and has less Maria than near side/
Mantle made of silica, magnesium and iron/
Lunar Rocks igneous, mostly oxygen and silicon, do not contain any water/
Interior of moon The moon has a near side and a far side because one side of the moon always faces earth, Small iron core/
Apogee when the moon is at the farthest point in its orbit around the earth/
Perigee when the moon is at the closest point in its orbit around the earth/
Giant Impact Hypothesis Mars sized object hit earth, Blasted part of mantle into space, Debris revolved around Earth, Eventually material joined to form our moon
Lunar rotation The moon rotates on its axis and revolves around the Earth… because its rotation and revolution take the same amount of time we always see the same side of the moon
Tides the rise and fall of the oceans/
Spring tides When the moon is full or new, the gravitational pull of the moon and sun are combined. At these times, the high tides are very high and the low tides are very low. This is known as a spring high tide (spring straight)/
Neap tides During the moon's quarter phases the sun and moon work at right angles, causing the bulges to cancel each other. The result is a smaller diff between high and low tides (known as a neap tide). Neap tides are especially weak tides
Solar Eclipse Sun-Moon-Earth (moon blocks the sun)
Lunar eclipse Sun-Earth-Moon (earth shadows the moon)
Umbra inner part of the shadow, where you can see the full eclipse
Penumbra outer part of the shadow
Seasons determined by earth's tilt
Aphelion the point on its orbit when the Earth is farthest from the sun, earth moves slowly on its orbit/
Perihelion the point on its orbit when the Earth is closest to the sun, earth moves faster on its orbit/
Summer solstice June 21st. It is the day with the longest amount of sunlight during the year.
Autumnal Equinox Sept. 21/22. There is equal daylight and night time.
Winter solstice Dec. 21st. This is the day with the least amount of the sunlight during the year.
Vernal equinox March 21/22. There is equal daylight and night time.
Ptolemy Geocentric
Copernicus Heliocentric
Kepler planets revolve around sun, planets move in an elliptical shape this is known as Kepler’s First Law
Galileo first person to use telescope to observe the sky, found 4 moon’s orbiting Jupiter
Newton Planets motion around sun is the result of inertia and gravity
Created by: elarocco
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