Post Activity/ Homework Questions: 1. Before a star forms A. Where do you think the gas and dust originally came from?

Similar documents
Life Cycle of a Star Worksheet

The Life Cycle of Stars. : Is the current theory of how our Solar System formed.

Life Cycle of a Star - Activities

Life of a Star. Pillars of Creation

They developed a graph, called the H-R diagram, that relates the temperature of a star to its absolute magnitude.

Stellar Evolution Notes

Ch. 29 The Stars Stellar Evolution

Reading and Announcements. Read Chapter 14.1, 14.2 Homework #6 due Tuesday, March 26 Exam #2, Thursday, March 28

21/11/ /11/2017 Space Physics AQA Physics topic 8

Low-mass Stellar Evolution

Stars. The composition of the star It s temperature It s lifespan

What is a star? A body of gases that gives off tremendous amounts of energy in the form of light & heat. What star is closest to the earth?

Protostars on the HR Diagram. Lifetimes of Stars. Lifetimes of Stars: Example. Pressure-Temperature Thermostat. Hydrostatic Equilibrium

GraspIT Questions AQA GCSE Physics Space physics

*Generally speaking, there are two main life cycles for stars. *The factor which determines the life cycle of the star is its mass.

Star Formation A cloud of gas and dust, called a nebula, begins spinning & heating up. Eventually, it gets hot enough for fusion to take place, and a

17.3 Life as a High-Mass Star

Abundance of Elements. Relative abundance of elements in the Solar System

Chapter 12 Review. 2) About 90% of the star's total life is spent on the main sequence. 2)

Birth & Death of Stars

Stars and their properties: (Chapters 11 and 12)

Daily Science 03/30/2017

Page 2. Q1. The diagram shows part of the life cycle of a star which is much bigger than the Sun.

Chapter 12: The Life Cycle of Stars (contʼd) How are stars born, and how do they die? 4/9/09 Habbal Astro Lecture 25 1

Review: HR Diagram. Label A, B, C respectively

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

The Formation of Stars

Stars and Galaxies. Evolution of Stars

Protostars on the HR Diagram. Lifetimes of Stars. Lifetimes of Stars: Example. Pressure-Temperature Thermostat. Hydrostatic Equilibrium

LIFE CYCLE OF A STAR

1. Star: A object made of gas found in outer space that radiates.

A Star Becomes a Star

Life and Death of a Star. Chapters 20 and 21

Stellar Evolution and the HertzsprungRussell Diagram 7/14/09. Astronomy 101

Stellar Astronomy Sample Questions for Exam 4

Chapter 17 Lecture. The Cosmic Perspective Seventh Edition. Star Stuff Pearson Education, Inc.

Outline - March 18, H-R Diagram Review. Protostar to Main Sequence Star. Midterm Exam #2 Tuesday, March 23

Astronomy 104: Stellar Astronomy

CONTENT EXPECTATIONS

Lifespan on the main sequence. Lecture 9: Post-main sequence evolution of stars. Evolution on the main sequence. Evolution after the main sequence

What You Should Know About Stars With Less Than 8 Solar Masses!

December 18, What do you know about the life of a star?

Age of M13: 14 billion years. Mass of stars leaving the main-sequence ~0.8 solar masses

Why Do Stars Leave the Main Sequence? Running out of fuel

What do the Roman numerals mean and how do stars die

Supernovae and cosmology

Ch. 25 In-Class Notes: Beyond Our Solar System

25.2 Stellar Evolution. By studying stars of different ages, astronomers have been able to piece together the evolution of a star.

Chapter 12: The Lives of Stars. How do we know it s there? Three Kinds of Nebulae 11/7/11. 1) Emission Nebulae 2) Reflection Nebulae 3) Dark Nebulae

8.8A describe components of the universe, including stars, nebulae, galaxies and use models such as HR diagrams for classification

Astro 21 first lecture. stars are born but also helps us study how. Density increases in the center of the star. The core does change from hydrogen to

Life and Death of a Star 2015

BANG! Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf. Lives of High Mass Stars

10/26/ Star Birth. Chapter 13: Star Stuff. How do stars form? Star-Forming Clouds. Mass of a Star-Forming Cloud. Gravity Versus Pressure

Today. Stars. Evolution of High Mass Stars. Nucleosynthesis. Supernovae - the explosive deaths of massive stars

Chapters 12 and 13 Review: The Life Cycle and Death of Stars. How are stars born, and how do they die? 4/1/2009 Habbal Astro Lecture 27 1

STARS AND GALAXIES STARS

Universe Celestial Object Galaxy Solar System

Low mass stars. Sequence Star Giant. Red. Planetary Nebula. White Dwarf. Interstellar Cloud. White Dwarf. Interstellar Cloud. Planetary Nebula.

Instructions. Students will underline the portions of the PowerPoint that are underlined.

chapter 31 Stars and Galaxies

To infinity, and beyond!

Describe the lifecycle of a star in chronological order and explain the main stages, relating the stellar evolution to initial mass

AST 101 Introduction to Astronomy: Stars & Galaxies

NSCI 314 LIFE IN THE COSMOS

Birth and Death of Stars. Birth of Stars. Gas and Dust Clouds. Astronomy 110 Class 11

Brock University. Test 1, February, 2017 Number of pages: 9 Course: ASTR 1P02 Number of Students: 480 Date of Examination: February 6, 2017

LIFE CYCLE OF A STAR

Guiding Questions. The Deaths of Stars. Pathways of Stellar Evolution GOOD TO KNOW. Low-mass stars go through two distinct red-giant stages

The Deaths of Stars 1

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS.

Guiding Questions. The Deaths of Stars. Pathways of Stellar Evolution GOOD TO KNOW. Low-mass stars go through two distinct red-giant stages

Stellar Evolution: The Deaths of Stars. Guiding Questions. Pathways of Stellar Evolution. Chapter Twenty-Two

2. Very generally, describe how the Milky Way Galaxy formed. (Words or labeled picture)

Brock University. Test 1, January, 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 500 Date of Examination: January 29, 2015

M42 (The Orion Nebula) and M43

The Evolution of Low Mass Stars

Planetary Nebulae White dwarfs

Astronomy Notes Chapter 13.notebook. April 11, 2014

Unit 1: Space. Section 2- Stars

(nuclear) reactor 1. (average) time taken for number of nuclei to halve or (average) time taken for count-rate / activity to halve

17.1 Lives in the Balance. Our goals for learning: How does a star's mass affect nuclear fusion?

Stars, Galaxies, and the Universe

Edwin Hubble Discovered galaxies other than the milky way. Galaxy:

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars

1. What is the primary difference between the evolution of a low-mass star and that of a high-mass star?

Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Earth Space Systems. Semester 1 Exam. Astronomy Vocabulary

2.) 3.) Igneous Sedimentary Metamorphic Characteristic:

CHAPTER 9: STARS AND GALAXIES

Stellar Evolution. The lives of low-mass stars. And the lives of massive stars

1. Four different processes are described in List A. The names of these processes are given in List B.

Stars IV Stellar Evolution

The origin of the Solar System

Logistics. Test 3 will be 4/24 MRS 2 due Thursday 4/17

Chapter 21: Stars Notes

How Do Stars Appear from Earth?

Stars and Galaxies. Evolution of Stars

Lecture 21 Formation of Stars November 15, 2017

AST 101 Introduction to Astronomy: Stars & Galaxies

Transcription:

Critical Thinking Questions: (work on these with a partner) 1. During the formation of a Red Giant Star, the core of a star pushes the outer shell back only enough to make the star larger. However, during the formation of a planetary nebula, the outer shell of a star gets pushed way out into the solar system. Explain how and why you think this difference is caused. In other words, explain how and why the outer shell is pushed out a little bit vs. pushed out far away. Post Activity/ Homework Questions: 1. Before a star forms A. Where do you think the gas and dust originally came from? 2. Protostars & Main Sequence Stars A. Why is a protostar not classified as an actual star? & what needs to occur for a star to transform from a Protostar to an actual star? B. Why is our sun classified as a Main Sequence Star? C. Describe what needs to happen to our sun for it to transform into a Red Giant. & Will this happen to our Sun? When? 2. Average sized stars like our Sun do not explode as supernova, but super-massive stars do. Both types of stars undergo nuclear fusion and have an outer shell influenced by gravity. Explain why a star like our Sun will not go supernova, but a super-massive star will. Explain your answer describing the processes of nuclear fusion and gravitational force. D. Complete the following Venn Diagram Protostars? How are both Similar? Actual Stars 3. Stars do not have enough energy to fuse elements heavier than iron. If this is true, how and why are elements that are heavier than iron created? 3. Red Giant vs. White Dwarf Star Complete the Venn Diagram: What is Unique How are both What is Unique during the formation formations Similar? of Red Giants during the formation of a White Dwarf 4. Once you figured out question #3, identify how the following elements were created: Element How was it created Oxygen Gold Carbon Lead 4. Planetary Nebula & New Stars A. Use the Internet to research the reason why Planetary Nebula's a are named so, even though they have nothing to do with planets B. Describe the process that would need to take place for a planetary nebula to form a whole new star.

\/ SCROLL DOWN FOR KEY \/

SCROLL DOWN FOR KEY \/

Critical Thinking Questions: (work on these with a partner) 1. During the formation of a Red Giant Star, the core of a star pushes the outer shell back only enough to make the star larger. However, during the formation of a planetary nebula, the outer shell of a star gets pushed way out into the solar system. Explain how and why you think this difference is caused. In other words, explain how and why the outer shell is pushed out a little bit vs. pushed out far away. During Red Giant formation, the core fuses a new element (Helium) and the star restabilizes. Once Helium runs out, fusion can't continue in the core and gravity is the only force left. The core can't balance the shell anymore and kicks it away one last time. 2. Average sized stars like our Sun do not explode as supernova, but super-massive stars do. Both types of stars undergo nuclear fusion and have an outer shell influenced by gravity. Explain why a star like our Sun will not go supernova, but a super-massive star will. Explain your answer describing the processes of nuclear fusion and gravitational force. Post Activity/ Homework Questions: 1. Before a star forms A. Where do you think the gas and dust originally came from? The Big Bang 2. Protostars & Main Sequence Stars A. Why is a protostar not classified as an actual star? & what needs to occur for a star to transform from a Protostar to an actual star? A protostar is not an actual star because fusion doesn't occur. To become an actual star, nuclear fusion needs to occur. B. Why is our sun classified as a Main Sequence Star? The force of fusion in the core is balanced with the shells gravity C. Describe what needs to happen to our sun for it to transform into a Red Giant. & Will this happen to our Sun? When? Our sun needs to run out of hydrogen and begin fusing helium This will happen to our sun in 5 billion years D. Complete the following Venn Diagram Protostars? How are both Similar? Nuclear Fusion does not occur It does not create & give off light They both contain gas and dust They both have a core and an outer shell Actual Stars Nuclear fusion occurs It creates & gives off light Because a super-massive star has more mass, it has a larger fusion force and gravitational force. When fusion stops in the core of a super-massive star, the gravitational force is so strong on the core, that the star explodes. 3. Stars do not have enough energy to fuse elements heavier than iron. If this is true, how and why are elements that are heavier than iron created? The explosion of a supernova gives off a lot more energy to fuse heavier elements 4. Once you figured out question #3, identify how the following elements were created: Element How was it created Oxygen Gold Carbon Lead 3. Red Giant vs. White Dwarf Star Complete the Venn Diagram: What is Unique How are both What is Unique during the formation formations Similar? of Red Giants during the formation of a White Dwarf The star begins by fusing hydrogen & ends by fusing helium The outer shell remains held to the star Both formations begin by fusing something. Both involve the core pushing the outer shell of the star The star begins by fusing helium & ends by not fusing anything at all. The outer shell doesn't remain held to the star 4. Planetary Nebula & New Stars A. Use the Internet to research the reason why Planetary Nebula's a are named so, even though they have nothing to do with planets B. Describe the process that would need to take place for a planetary nebula to form a whole new star.