Astronomy 100 Are All Stars the Same?. Answer Now: Why does the Sun shine? Are all stars the same as our Sun? (How or how not?) Goal: – Be able to tell.

Slides:



Advertisements
Similar presentations
Stars The life and death of stars in our universe.
Advertisements

Nebula to Protostar Giant molecular clouds within a nebula contract under the gravitational pressure, increasing its thermal energy. CO, NO, OH- Giant.
The Life Cycle of a Star.
Review for Quiz 2. Outline of Part 2 Properties of Stars  Distances, luminosities, spectral types, temperatures, sizes  Binary stars, methods of estimating.
The Life Cycle of Stars. If you were preparing a timeline of your life, what would you include?
Classifying Stars Brightness. Some stars are so bright that you can see them even in a lighted city, while others are so dim that you can only see them.
The Evolution of Stars - stars evolve in stages over billions of years 1.Nebula -interstellar clouds of gas and dust undergo gravitational collapse and.
StarsStars. What is a STAR? The objects that heat and light the planets in a system A star is a ball of plasma held together by its own gravity –Nuclear.
The Universe Chapter 20.
The Life Cycle of a Star I can describe the life cycle of a star u Bell ringer – What type of magnitude is each definition referring to? 1. The true.
THE LIFE CYCLES OF STARS. In a group, create a theory that explains: (a)The origin of stars Where do they come from? (b)The death of stars Why do stars.
The Universe Pictures by the Hubble Space Telescope.
The Universe Science 8.
StarsStars. Essential Questions What is a celestial body? What is a star? Wat process powers a star? What is a light year? What is the lifecycle of a.
Astronomy (cont.) Cosmic Measurements Astronomical Unit (AU) - distance from earth to the sun ~150 million kilometers (93 million miles) - used to express.
Star Life Cycles. Stellar Nebula  Stars begin life as cloud of gas + dust  Cloud condenses and becomes more massive  Nuclear fusion begins (the power.
 A star is a ball of hydrogen, helium and enough mass that can bear nuclear fusion at its core  Stars are most often seen at night in a clear sky 
Star Formation Star = large balls of gas that produce energy and shine…. unless old. Nuclear Fusion = combines light elements to create heavy ones….
Lunar Phases. Size Largest stars = supergiants or giants The next step down in size are called medium stars. White dwarf stars are about the size of.
HR Diagram. Characteristics of Stars  Temperature/Color  Mass  Luminosity Absolute Magnitude Apparent Magnitude.
STARS Mrs. Anton.
Twinkle, Twinkle Little Star…. How I wonder what you are… Stars have Different colors Which indicate different temperatures The hotter a star is,
Chapter 15 – Stars, Galaxies and the Universe. Chapter 15 – History of the Universe Section 2 – Characteristics of Stars Section 2 – Characteristics of.
StarsStars. A Star…. Heats and lights the planets in a solar system Is a ball of plasma (4 th state of matter consisting of ionized particles) held together.
Stars.
Stars and Galaxies.
A Note Taking Experience.
Life Cycle of Stars Birth Place of Stars:
Aim: What is the life cycle of a star? I. Star – a massive, gaseous body held together by gravity and generally emitting light B. Life cycle of low massive.
Life Cycle of a Star Star Life Cycle: Stars are like humans. They are born, live and then die.
Life Cycle of Stars 4-3 The Life cycle of a star depends upon the size (Mass) of the star. Our Sun is an Average size Star.
Astronomy (cont.) Cosmic Measurements Astronomical Unit (AU) - distance from earth to the sun ~150 million kilometers - used to express distances to other.
‘The life-cycle of stars’
Recap: Death of Stars: Low and Medium Mass Red Giant Main Sequence Star Planetary Nebula White Dwarf Black Dwarf ?? Red Dwarf Low Mass Medium Mass.
STARS.
Star Properties and Stellar Evolution. What are stars composed of? Super-hot gases of Hydrogen and Helium. The sun is 70% Hydrogen and 30% Helium.
Stars Goal: Compare star color to star temperature.
“Twinkle, Twinkle Little Star” The Life Cycle of a Star: Nursery to Neverland Courtney Mutschler Geospace 355
The Life Cycle Of Stars.
Stars Chapter 11, Lesson 4. Where do stars come from? Stars form in a nebula, which is a large cloud of gas and dust in space. Gravity pulls some of the.
Stellar Evolution. Structure Mass governs a star’s temperature, luminosity, and diameter Hydrostatic Equilibrium – the balance between gravity squeezing.
Stars Not Dancing With….
Stars.
Stars.
The Life Cycle of a Star.
STARS A matter of life and death
Stellar Evolution.
Stars.
Made mostly of hydrogen
STARS Essential Questions.
Life cycle of a star 25.2.
The Life Cycle of a Star.
Stars.
Stars.
The Life Cycle of a Star.
The Life Cycle of a Star.
Section 2 The Life Cycle of Stars
Stars.
The Life Cycle Of Stars.
The Life and Death of Stars
EL: Be able to describe the evolution of stars.
Stars.
The Life Cycle of a Star.
Stars.
Stars.
STARS.
Life Cycle of a Star.
Stars.
Stars.
Stars.
Presentation transcript:

Astronomy 100 Are All Stars the Same?

Answer Now: Why does the Sun shine? Are all stars the same as our Sun? (How or how not?) Goal: – Be able to tell me how stars are born – Know what stars are made of – Know how stars shine – (if we have time) Know how stars die Vocabulary: Planck curve, luminosity, H-R Diagram, absolute magnitude, apparent magnitude, fusion, H, He, CNO Cycle, protostar, nebula, protostar, hydrostatic equilibrium, interstellar medium, compression wave,

Planck Curve - Temperature DIRECTLY related to peak wavelength.

Luminosity – Apparent magnitude – Absolute magnitude – Luminosity is the total brightness Temperature or Type – Can tell temp from color – Can tell type from spectrum, temp or color Types: O, B, A, F, G, K, M

star.html

It all starts with gas Interstellar medium Gas cloud (nebula) Compression wave Pockets of compacted gas Gravity further squeezes gas PROTOSTAR! Squished enough (enough energy) fusion begins STAR!

E=mc 2 H+H+H+H+H+H = He + H + H+ energy

Hydrostatic Equilibrium Energy from fusion

Compression Wave: &ei=c_iASe30OZ64qA PS-MSVDg&q=slinky+compression&hl=en &ei=c_iASe30OZ64qA PS-MSVDg&q=slinky+compression&hl=en

And in the end… < 4 Solar Mass – when finished fusing H, begins to fuse He Ffffffft (planetary nebula) White dwarf/black dwarf > 4 Solar Mass – when finished fusing H, begins to fuse He – when finished fusing He, begins to fuse C, N, O (shells) Kerblewie! (supernova) Black hole/neutron star

Review – define 3 of the terms at the beginning of this lecture. Quiz Review

High Mass Stars My candle burns at both ends; It will not last the night; But ah, my foes, and oh, my friends-- It gives a lovely light. Emily Dickinson

Brownian Motion: BKoqQxsM BKoqQxsM