Jeopardy Final Jeopardy ??Mystery?? Stellar Evolution HR Diagram Solar

Slides:



Advertisements
Similar presentations
Sun Mr. Skirbst Physical Science Topic 26. The Sun.
Advertisements

DO NOW QUESTION Yesterday we talked about the future of the universe. What do you think will happen to the universe?
Stars & Universe.
Stars, Galaxies, and the Universe- Course 3
The Layers of a Star The corona is the wide, outermost layer of a Sun’s atmosphere – (AL) The chromosphere is the orange-red layer of the Sun’s atmosphere,
Key Ideas How are stars formed?
Lesson 3.3: The Sun.
I. Stars A.The Brightness of Stars -Star: A hot glowing sphere of gas that produces energy by fusion. -Fusion: The joining of separate nuclei. Common.
The Sun 24.3 A typical star powered by nuclear reactions Mostly the (fusion of hydrogen to form helium) Which releases energy.
Definitions  Sun: Star at the center of our solar system. Also another name for any star.  Luminosity: measures how bright a star would be in relation.
The Sun Unit 5 PESS 2. Energy from the Sun Electromagnetic energy is a type of energy that can travel through space an example is visible light Light.
Astronomy – Stellar Evolution What is a Star? Stars are hot bodies of glowing gas that start their life in Nebulae.(1) 2.
The Sun Photo from
Astronomy 1 Review.
Stars The Brightness of Stars -Star: A luminous sphere of gas with enormous mass, that produces energy by fusion. -Fusion: The joining of separate nuclei.
Our Sun 93 million miles from Earth 150 million kilometers Earth 99.8% of the mass of our solar system.
Chapter 30 Section 2 Handout
Life Cycle of a Star Star Life Cycle: Stars are like humans. They are born, live and then die.
Star Life Cycle Review. Transports energy from the radiative zone to the surface of the sun. Sunspot Corona Photosphere Convective zone.
Galaxies The basic structural unit of matter in the universe is the galaxy A galaxy is a collection of billions of _____________, gas, and dust held together.
Unit 1 Lesson 3 The Life Cycle of Stars
Sun Lesson 3. Sun The sun is a star located at the center of our solar system. The nearest star from earth and our engine for life. It is a medium-sized.
DAY 16 September 17, Agenda 1 st RP ‘Stuff’ back Grade Sheets Complete Star Notes Star Concept Map.
Hosted by Mrs. Walia Choice1Choice 2Choice 3Choice
The Sun’s Energy. Sun Fact’s The sun is the closest star to the earth. It provides earth’s adequate heat for life to exist Temperature= 5,600 Kelvin (K).
The Sun Average in size… yes AVERAGE!!
Unit 1 Lesson 3 The Life Cycle of Stars
Unit 2- Stars.
Act 1: Small or Medium Stars
Stage 1: Nebula – Latin for “cloud”
Stars.
STARS.
12-2 Notes How Stars Shine Chapter 12, Lesson 2.
Stars Section 1: The Sun Section 2: Measuring the Stars
Earth, Moon, and Sun Astronomy Unit.
Welcome to ASTRONOMY Jeopardy!.
Handout 2-1a Stellar Evolution.
Stars.
Chapter 30 Section 2 Handout
Since fusing hydrogen into helium causes a star to be on the main sequence, why do smaller stars stay on the main sequence longer than massive stars that.
The Sun and Other Stars How do stars shine? How are stars layered?
Stars.
Chapter 24 Stars and Galaxies.
Notes using the foldable
The Sun’s Energy The core of the sun acts like a furnace.
Life Cycle of a Star Star Life Cycle: Stars are like humans. They are born, live and then die.
The Sun and Stars Lesson 2 pg. 808
Star Life Cycle Review.
A star's Life Cycle at a Glance
Bell Ringer Monday, March 26th
Planets Inner vs. outer Composition – inner planets are rocky/outer are gas Size – inner are smaller/outer are much larger Distance from sun – inner are.
Astronomy – Stellar Evolution
Jeopardy Final Jeopardy ??Mystery?? Stellar Evolution HR Diagram Solar
The Sun’s Layers and Solar Activity
Astronomy Star Notes.
8th Grade Second Trimester Standard D
Stars.
From protostars to supernovas
STELLAR EVOLUTION. STELLAR EVOLUTION What is a star? A star is a huge ball of hot gas, held together by its own gravity. Most of the gas is hydrogen.
I. Stars The Brightness of Stars
Lives of Stars.
Unit 2: Stellar Evolution and Classification …The stars are a lot more than belonging to constellations! Unit 2 Miss Cohn.
STARS.
Planets Inner vs. outer Composition – inner planets are rocky/outer are gas Size – inner are smaller/outer are much larger Distance from sun – inner are.
The Sun and Other Stars 14-2.
Stellar Evolution Chapter 30.2.
Sun Lesson 3.
Stars From Nebula to Black Holes.
Science Unit D Review Chapter 2.
Presentation transcript:

Jeopardy Final Jeopardy ??Mystery?? Stellar Evolution HR Diagram Solar Activity Nuclear Fusion $100 $100 $100 $100 $100 $200 $200 $200 $200 $200 $300 $300 $300 $300 $300 $400 $400 $400 $400 $400 $500 $500 $500 $500 $500 Final Jeopardy

1 - $100 This is the visible surface of the sun Photosphere

1 - $200 List stars from hottest to coolest Blue, White, Yellow, Orange, Red

1 - $300 Solar winds interact with Earth to create what? Auroras

1 - $400 What does a white dwarf become when fusion stops and it no longer shines? Black dwarf

1 - $500 Which stars live longer… low mass or high mass? WHY? Low mass because they use their fuel more slowly.

2 - $100 Before a star is formed it is just the gas and dust of a Nebula

2 - $200 A star is born when what begins Fusion

2 - $300 When the outward force of fusion is greater than the inward force of gravity what forms? Giant

2 - $400 An explosion that marks the end of a high mass star’s life Supernova

2 - $500 This is the force that causes a nebula to contract Gravity

3 - $100 Two characteristics that an HR diagram relates Temperature and Brightness

3 - $200 Where are the white dwarfs located Bottom left

3 - $300 This is the area on the HR diagram where stars spend most of their lives Main Sequence

3 - $400 Where are the giants located Top Right

3 - $500 Characterize Giants Extremely bright with low temperatures

4 - $100 This is a dark area of the photosphere that is cooler than the surrounding areas Sunspot

4 - $200 This is a loop or arch or gas that extends from the photosphere Prominence

4 - $300 This is an explosive release of energy from the sun Solar flare

4 - $400 How long is the sunspot cycle? 10-11 years

4 - $500 Where on Earth do we usually see auroras? Near the north and south poles

5 - $100 This is where fusion occurs in stars Core

5 - $200 This is the product of nuclear fusion in stars Helium

5 - $300 Fusion begins when these 2 particles collide 2 protons

5 - $400 The helium atom made during fusion has ________ protons 2

5 - $500 The amount of hydrogen in a star increases/decreases as fusion continues Decreases

Final Jeopardy Explain why the Earth has seasons. Because the Earth is tilted on its axis: In the summer, the Earth is tilted TOWARD the sun, making the sun rays more direct and the temperature warmer. In the winter, the Earth is tilted AWAY from the sun, causing the rays to be less direct and the temperature colder.