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Eagle Exercise A meteorologist used radar to analyze the wind during a storm in the central plains of United States. The winds were at 145 miles per hour.

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Presentation on theme: "Eagle Exercise A meteorologist used radar to analyze the wind during a storm in the central plains of United States. The winds were at 145 miles per hour."— Presentation transcript:

1 Eagle Exercise A meteorologist used radar to analyze the wind during a storm in the central plains of United States. The winds were at 145 miles per hour and were moving in a circular pattern. According the data, which event was the meteorologist most likely observing? Lightening storm Tornado Rainbow Cloud formation

2 Facts About Tornadoes. A tornado is as a rotating, funnel-shaped cloud that extends from a thunderstorm to the ground with whirling winds that can reach 300 mph. Damage paths of tornadoes can be in excess of one mile wide and 50 miles long.

3 Purpose for Learning GLE Analyze information about the major components of the universe.

4 Explain the life cycle of a star.
Learning Expectation I can... Explain the life cycle of a star.

5 What stage of life does a star go through?
GUIDING QUESTION What stage of life does a star go through? S

6 Apparent Magnitude A star’s apparent magnitude is its brightness as seen from Earth Just like a flashlight looks brighter the closer it is to you, a star looks brighter the closer it is to Earth

7 Absolute Magnitude A star’s absolute magnitude is the brightness the star would have if it were at a standard distance from Earth Stars in a globular cluster are all at about the same distance from Earth, so scientists can study clusters to determine absolute magnitude

8 What determines the life cycle of a star?
Its size

9 Gallery Walk You will take a gallery walk to determine the birth of a star. Put the stars in order from

10 What am I What am I What am I What am I What am I What am I What am I

11 Life Cycle of a Star A STAR IS BORN All stars start as a nebula. A nebula is a large cloud of gas and dust. Gravity can pull some of the gas and dust in a nebula together. The contracting cloud is then called a protostar. A protostar is the earliest stage of a star’s life. A star is born when the gas and dust from a nebula become so hot that nuclear fusion starts. Once a star has “turned on” it is known as a main sequence star. When a main sequence star begins to run out of hydrogen fuel, the star becomes a red giant or a red super giant. THE DEATH OF A LOW OR MEDIUM MASS STAR After a low or medium mass or star has become a red giant the outer parts grow bigger and drift into space, forming a cloud of gas called a planetary nebula. The blue-white hot core of the star that is left behind cools and becomes a white dwarf. The white dwarf eventually runs out of fuel and dies as a black dwarf. THE DEATH OF A HIGH MASS STAR A dying red super giant star can suddenly explode. The explosion is called a supernova. After the star explodes, some of the materials from the star are left behind. This material may form a neutron star. Neutron stars are the remains of high-mass stars. The most massive stars become black holes when they die. After a large mass star explodes, a large amount of mass may remain. The gravity of the mass is so strong that gas is pulled inward, pulling more gas into a smaller and smaller space. Eventually, the gravity becomes so strong that nothing can escape, not even light.

12 Brainpop: Life of a Star
heuniverse/lifecycleofstars/

13 Eagle Exit


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