Origin of our Universe:

Slides:



Advertisements
Similar presentations
Life cycle of stars Nebulae to supernova.
Advertisements

A journey to the stars.
The Life of a Star (15.1) BLM 15.1b
Life Cycle of Stars. Omega / Swan Nebula (M17) Stars are born from great clouds of gas and dust called Stars are born from great clouds of gas and dust.
Stars & Galaxies.
A star is born… A star is made up of a large amount of gas, in a relatively small volume. A nebula, on the other hand, is a large amount of gas and dust,
The Life Cycle of a Star.
Stars, Life and Light.
The Sun. Sun A small star About 5 billion years old (should last 5 more) Composed of 75% hydrogen and 25% helium All elements in plasma phase ( hotter.
OUTCOME QUESTION(S): S1-4-08: What objects make up our solar system and Universe? Vocabulary and People CoreFusionNebulaSupernova Black holeGalaxyTerrestrial.
NOT THOSE TYPES OF STARS! LIFE CYCLE OF STARS WHAT IS A STAR? Star = ball of plasma undergoing nuclear fusion. Stars give off large amounts of energy.
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,
Life Cycles of Stars. Stars Stars are a large hot balls of plasma that shine The Sun is the Star in our solar system A group of stars that form a recognizable.
Stars start out as a Nebula –
Galaxies The Life and Death of the Stars. A galaxy is a cluster of stars, gas, and dust that are held together by gravity. There are three main types.
Stars, Life and Light. S1-4-05b Identify the parts of the Sun and its source of energy. S1-4-06b Explain the basic life cycle of a star. KEY WORDS FusionCorePhotosphere.
Stars and Galaxies.
The Universe Science 8.
Earth Science Notes Stars and Galaxies.
Lives of Stars Notes. The Lives of Stars A star is not organic, therefore it IS NOT alive. Astronomers typically talk about the life cycle of a star as.
Chapter 1: Stars and Galaxies When you look up at the sky on a clear night, you see billions of stars in the sky. Each star is actually a sun! A sun is.
Stars and the Sun a star is a ball of hot plasma (like a gas with an electrical charge) 90% of the matter in the universe is plasma it is not “on fire”
 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 
The Life and Death of a Star. Explain all life cycle of the stars. Explain EMR. KEY WORDS LuminosityMain sequence NebulaRed dwarfNeutron Star Red giantWhite.
Stars.
Life Cycle of a Star. Nebula(e) A Star Nursery! –Stars are born in nebulae. –Nebulae are huge clouds of dust and gas –Protostars (young stars) are formed.
The Universe… …is space and everything in it.
Life Cycle of Stars Birth Place of Stars:
The Life Cycle of Stars.
The Life History of Stars How stars form and die.
8.8 A and B Components the Universe and the Sun
Unit 2- Stars.
8.8 A and B Components the Universe and the Sun
Stars on and off the Main Sequence
12-2 Notes How Stars Shine Chapter 12, Lesson 2.
Chapter 30 Section 2- Stellar Evolution
Welcome to ASTRONOMY Jeopardy!.
The Sun is the largest object in the solar system.
Stars & Galaxies.
ORIGIN OF THE UNIVERSE UNIT 2 Big Bang.
Origin of our Universe:
8 Space physics Topic overview
Chapter 24 Stars and Galaxies.
Galaxies and Stars.
The Star Lifecycle.
It contains hundreds of billions of galaxies
The lifecycles of stars
Unit E – Space Exploration The Distribution of Matter in Space
Life Cycle of a Star.
Evolution of the Solar System
Stars and the Sun a star is a ball of hot plasma (like a gas with an electrical charge) 90% of the matter in the universe is plasma it is not “on fire”
19.3 Stars.
                                                                                 STARS.
Astronomy Star Notes.
Life Cycle of a Star.
The Life and Death of Stars
From protostars to supernovas
The Life Cycle of a Star.
Life-Cycle of Stars.
Galaxies and Stars.
Life of a Star.
Galaxies and Stars.
Stellar Evolution Chapter 30.2.
Life Cycle of a Star.
The Life Cycle of a Star.
04/07/2019 The Earth and Beyond.
The Universe… …is space and everything in it.
Stars and Galaxies.
Presentation transcript:

Origin of our Universe: Life of Stars

OUTCOME QUESTION(S): S1-4-08: Vocabulary & Concepts What objects make up our solar system and Universe? Vocabulary & Concepts  Core Fusion Nebula Supernova Black hole Galaxy

Our Sun 5 billion year old small star (should last 5 more) Composed of 75% hydrogen and 25% helium Elements in plasma phase (hotter state than gas) Energy comes from a Nuclear Fusion Reaction

Nuclear Fusion Reaction Joining two hydrogen to create helium Releases large amount of energy Fusion = join Fission = split Sun: joining (fusion) things to release energy Power Plants: splitting (fission) things to release energy

There is obviously more to the Sun then “burning ball of gas”

Core – centre and site of nuclear fusion Outside Layers of the Sun: Inside Core – centre and site of nuclear fusion Outside Photosphere – cooler surface (5500 oC) sunspots, surface storms – the part we “see” Chromosphere – inner atmosphere small solar explosions (flares), large (prominences) Corona – outer atmosphere (1 million oC) charged gas particles blow outward (solar winds)

“Life Cycle” of a Star Birth: Stars born out of Nebulae Nebula – huge clouds of dust and gas Youth – Middle Age: Gravity collapses material into a star that begins to release energy as a main sequence (MS) star Scientists categorize MS stars according to mass: Small - last longer (billions of years) Large - brighter but short-lived (few million yrs)

Attracted by gravity; matter clusters together Nebula 99% hydrogen and helium 1% iron, rock and ice Attracted by gravity; matter clusters together

Actually nebulae captured by NASA space telescopes

We can’t see most Red Dwarf stars – their light is too weak Small MS star – Red Dwarf Very cool temperatures of their outer gases Death: Forms a cool, dim star called a White Dwarf Fades out until it no longer emits light energy We can’t see most Red Dwarf stars – their light is too weak

Medium MS star – like the Sun Separated into small-med and large-med Death: Runs out of elements for fusion reaction Collapses then swells to produce a Red Giant small-med eventually fades out as white dwarf large-med explodes as a Supernova leaving behind a Neutron star “Pulsar” neutron star

Extreme energy produced for a short period Large MS star Extreme energy produced for a short period Fuses heavier elements (iron) after lighter ones Death: Collapses then swells to a Red Supergiant Gravity collapses the largest into a Black Hole Stars are in balance: nuclear fusion explodes outwards, large gravitational force collapses inwards When the reactor runs out of elements to fuse, gravity wins and the star collapses and (sometimes) explodes

There is still more to this puzzle, but…this is close enough Birth: Nebulae Smallest main sequence (MS) star Largest Medium Red Dwarf Red Giant Red Supergiant Supernova Death: White Dwarf Neutron star Black Hole There is still more to this puzzle, but…this is close enough

What do you notice?

Galaxies Huge collections of gas, dust and billions of stars and planets (collected by gravity) Constantly in motion Many shapes: spiral, elliptical, and irregular

Contains 400 billion stars Milky Way Galaxy Contains 400 billion stars Disc-shaped, with spiral arms – spiral galaxy We are on one of the arms Has a thicker Central Bulge Rotates around the bulge New evidence suggests the “central bulge” is actually a SUPER-MASSIVE BLACK HOLE!

CAN YOU ANSWER THESE QUESTIONS? S1-4-08: How do star create energy? What objects make up our solar system and Universe? Vocabulary & Concepts  Core Fusion Nebula Supernova Black hole Galaxy