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Our Solar System and Beyond
Earth Goes Around The Sun
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http://studyjams. scholastic
Day and Night
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Day and Night
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Rotation – spin on axis; takes Earth 24 hours
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Revolution – one complete cycle around the Sun; takes Earth 365 ¼ days
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Rotation and Revolution sung to the tune of “Row Your Boat”
Ro – Ro- Rotation For 24 hours we say! The Earth Spins on its axis This will make a day! Rev- Rev- Revolution The Earth goes round the Sun Three hundred sixty-five days Until a year is done!
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U. S. Standard Time Zones Eastern Central Mountain Pacific
Standard Time Zone – a vertical belt about 15 degrees wide in longitude in which all locations have the same time U. S. Standard Time Zones Eastern Central Mountain Pacific
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International Date Line
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http://studyjams. scholastic
Seasons
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Reasons for Seasons The Earth’s orbit around the Sun.
The tilt of the Earth’s axis at an angle of 23.5 degrees.
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Solstice The Sun reaches its greatest distance north or south of the equator twice each year. Each of these days, when the Sun is farthest north or south of the equator, is known as a solstice.
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Solstice The day when it is farthest north of the equator is the Summer Solstice. This occurs on June 21 of each year. It is the longest day of the year.
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Solstice When the Sun is farthest south of the equator, this is the Winter Solstice. This occurs around December 22.
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Equinoxes Halfway between the solstices, neither hemisphere is tilted toward or away from the Sun. The noon Sun is directly above the equator. The Spring Equinox occurs around March 21.
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Equinoxes The autumnal equinox occurs around September 22. It marks the beginning of fall.
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Eclipses Solar Eclipse – the blocking of sunlight to Earth that occurs when the Moon is directly between the Sun and the Earth Lunar Eclipse – the blocking of sunlight to the Moon that occurs when Earth is directly between the Sun and the Moon
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Solar Eclipse
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Solar Eclipses Total Solar Eclipse Partial Solar Eclipse
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Lunar Eclipse
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Lunar Eclipses Total Lunar Eclipse Partial Lunar Eclipse
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The Life Cycle of a Star
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A giant ball of gases held together by gravity.
What is a Star? A giant ball of gases held together by gravity.
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A Star is Born! Born in a nebulae – vast clouds of dust and gas in space At 10 million degrees, nuclear fusion occurs A protostar is born
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Main Sequence After a star forms, it is in its main life period called the main sequence period. This can last for MILIONS of years!
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The Death of a Star A star swells up into a glowing red giant that may be a hundred times larger than the original star. What happens next depends on the star’s mass.
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The Death of a Star Medium Sized Star Cools off Core collapses
Star shrinks White dwarf Black dwarf Giant or Supergiant Star Huge explosion called a supernova Neutron star Black hole
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Colors of Stars Blue Yellow Red White
Color of A Star Colors of Stars Blue Yellow Red White
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Red Stars 3,000 degrees Coolest Also called M-type stars
Example: Betelgeuse
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Yellow Stars 5,000 degrees Also called G-type stars Example: Sun
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Blue Stars Hottest 20,000 degrees Also known as O-type stars
Example: Spica
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White Stars 10,000 degrees Example: Sirius
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Elliptical galaxy Spiral galaxy Barred spiral galaxy Irregular galaxy
Way Ballad Types of Galaxies Elliptical galaxy Spiral galaxy Barred spiral galaxy Irregular galaxy
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Spiral Galaxy
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Elliptical Galaxy
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Barred Spiral Galaxy Scientists now classify our galaxy, the Milky Way, as a barred spiral galaxy.
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https://www. youtube. com/watch
Irregular Galaxy
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