E treme Stars Caty Pilachowski Mini-University June 2012.

Slides:



Advertisements
Similar presentations
Notes 30.2 Stellar Evolution
Advertisements

Life Cycle of Stars.
Stellar Evolution Describe how a protostar becomes a star.
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,
Fill in the chart when you see a yellow star. Take notes on the stars and events as well.
Space Science = Astronomy
DO NOW QUESTION Yesterday we talked about the future of the universe. What do you think will happen to the universe?
Stellar Evolution: The Life Cycle of a Star. Stellar Nurseries All stars start out in a nebula (large cloud of dust and gas). All stars start out in a.
Stellar Deaths Novae ans Super Novae 16. Hydrostatic Equilibrium Internal heat and pressure from fusion pushes outward Gravity pulling mass inward Two.
Nebulas are made up of gas left behind by stars forming or exploding There are different classes of Nebulas The classes are: Reflection Nebulae, Emission.
Announcements Pick up graded homework (projects, tests still in progress) Turn in Homework 10 by 5:00 Vote tomorrow! Transit of Mercury (crossing in front.
Types of Stars Life Cycle of Stars Galaxies
+ Quick write What would happen if the sun disappeared?
Stars By: Mrs. Crisp.
Astronomy Unit Review. Topics Solar system(planets, asteroid belt, meteor, meteoroid, meteorite, comet etc) Measurement (AU and Light Years) Sun (structure;
TOPIC: Astronomy AIM: What are stars?
Key Ideas How are stars formed?
Copy everything in this colour into your notes!. Galaxies & Stars.
Star Properties. Star Distances Units of Distance for Space: Astronomical Units (AU): The distance from the earth to the sun (150,000,000 km) Light Years:
Star Properties. Where do stars come from? Stars form in a cloud of dust and gas in space called a nebula.
STARS By Bodin Lay. Types of Stars Main Sequence Stars - The main sequence is the point in a star's evolution during which it maintains a stable nuclear.
The UniverseSection 1 Question of the Day: Jackie used a portable electric drill to remove screws from a broken wooden table. He noticed that the screws.
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.
Astronomy Chapter Nineteen: Galaxies and the Universe 19.1 Tools of Astronomers 19.2 Stars 19.3 Galaxies and the Universe.
Stars Stars What are Stars?  Stars are large balls of hot gas.  They look small because they are a long way away, but in fact many are bigger and brighter.
Astronomy – Stellar Evolution What is a Star? Stars are hot bodies of glowing gas that start their life in Nebulae.(1) 2.
Stars The apparent twinkling of the stars is a product of the turbulence and motion of the Earth’s atmosphere Stars have different colors depending on.
The UniverseSection 1 Section 1: The Life and Death of Stars Preview Key Ideas Bellringer What Are Stars? Studying Stars The Life Cycle of Stars.
The Stars Chapter 14 Great Idea: The Sun and other stars use nuclear fusion reactions to convert mass into energy. Eventually, when a star’s nuclear fuel.
2005 K.Corbett Life Cycle of Stars K.Corbett 3 categories of stars  Sun-sized stars  (up to 6 times the size of the sun)  Huge stars  (
The UniverseSection 1 Key Ideas 〉 How are stars formed? 〉 How can we learn about stars if they are so far away? 〉 What natural cycles do stars go through?
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 Life Cycle of a Star The Horsehead Nebula – one of the most famous pictures in astronomy.
Warm up The sun is 4.6 billion years old – how can it continue to produce so much heat and light?
Studying the Lives of Stars  Stars don’t last forever  Each star is born, goes through its life cycle, and eventually die.
EARTH & SPACE SCIENCE Chapter 30 Stars, Galaxies, and the Universe 30.2 Stellar Evolution.
Megan Garmes Betsy Nichols
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: Space The Study of the Universe.  Mass governs a star’s temperature, luminosity, and diameter.  Mass Effects:  The more massive the star, the.
STARS.
Birth and Death of Stars. Astronomers learn about stars by observing the electromagnetic radiation the stars emit. The most common type of telescope collects.
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.
FORMATION OF STARS SES4U. OBJECTIVES 1. Name, describe, and give examples of several kinds of nebulae and explain the relationship between nebulae and.
Stars Goal: Compare star color to star temperature.
STARS A Life and Death Production. Nebula A very large diffuse mass of interstellar dust and gas (mostly Hydrogen). This material starts to collapse in.
STARS & their life cycles Like us, stars are born, grow older, become middle aged and eventually die!!! Unlike us, stars take billions of years to complete.
Study of the universe (Earth as a planet and beyond)
Stars Earth Science – Mr. Foster. Why do stars exist? Stars exist because of gravity Two opposing forces in a star are – Gravity – contracts – Thermal.
Unit 2 - Cosmology Part 1: Stars Part 2: Galaxies Part 3: Origin and Evolution of the Universe.
BEYOND OUR SOLAR SYSTEM CHAPTER 25 Part II. INTERSTELLAR MATTER NEBULA BRIGHT NEBULAE EMISSION NEBULA REFLECTION NEBULA SUPERNOVA REMANTS DARK NEBULAE.
Stars Huge spheres of very hot gas that emit light and other radiation. They are formed from clouds of dust and gas, or nebulas, and go through different.
STARS!. Gravity is a force that pulls objects with mass toward each other. Gravity increases as mass increases, so the Sun has stronger gravity than the.
Study of the universe (Earth as a planet and beyond)
Stellar Evolution Continued…. White Dwarfs Most of the fuel for fusion is used up Giant collapses because core can’t support weight of outer layers any.
Stars, Galaxies, and the Universe Section 2 Section 2: Stellar Evolution Preview Objectives Classifying Stars Star Formation The Main-Sequence Stage Leaving.
Stars and Galaxies Chapter 12. Stars Definition: a large ball of gas that emits energy produced by nuclear reactions in the star’s interior Planets, comets,
Stars change over their life cycles.
Stars: Old Age, Death, and New Life
Chapter 24 Stars and Galaxies.
Notes: 24.3 Evolution of Stars.
Stars Notes Ch. 28.
Life Cycle of Stars 2005 K.Corbett.
Stellar Evolution: Aim: The Life Cycle of a Star
A Life and Death Production
The Deaths of Stars.
The Life and Death of Stars
How are stars born, and how do they die?
STARS.
Stellar Evolution Chapter 30.2.
Stars and Galaxies.
Presentation transcript:

E treme Stars Caty Pilachowski Mini-University June 2012

Brightest Star in the night sky SIRIUS Alpha Canis Majoris The Dog Star Sirius b – faint companion

Most Distant Star (that you can see!) Deneb Deneb = Alpha Cygni Distance: ~ 1500 LY Diameter: ~20 x Sun Mass: ~20 x Sun Luminosity: 60,000 x Sun 1 LY = 9,460,528,400,000 Km

The Closest Star Our Sun is a typical, middle-aged star Age: Distance: 150 million Km The Closest Star Diameter: 1.4 million Km = 100 x Earth Our Sun is a typical, middle-aged star Temperature: 6,000 C (outside) 15 million C (inside) Mass: 2 x 1030 kg = 300,000 x Earth Age: 4.6 billion years

A Range of Size and Mass 0.08 MSun ~200 MSun 0.1 MSun ~1000 MSun DIAMETER 0.1 MSun ~1000 MSun Only certain combinations of size and mass are stable Stars will shrink or expand to reach stability

Cool stars are reddish in color A Range of Temperature TEMPERATURE 200,000 C 2000 C The Sun is about 6000 C Hot stars are bluish in color Cool stars are reddish in color A star’s brightness depends on its temperature and radius

Allowed Temperature & Luminosity

The Sun formed 4.6 billion years ago A Range of Ages AGE ~13 Billion Years Brand New Stars The Sun formed 4.6 billion years ago Stars have been forming continuously since the Universe began 13.7 billion years ago Some old stars are still around; other stars are brand new

Birth of the Sun BIRTH

Middle Age BIRTH H The Sun Today

Inside the Sun: Energy and Motion The energy comes from nuclear fusion reactions in the Sun’s core Energy flows slowly from the inside to the surface

The Visible “Surface” of the Sun Sunspots cooler regions magnetic fields prominences originate from active regions

The Sun in Time The Sun is gradually growing brighter over time, as it converts hydrogen into helium Eventually…

As the Sun Grows Old He BIRTH H NOW

Future Sun The Sun as a red giant The Sun today The orbit of Venus Astronomers aren’t sure how big the Sun will grow when it becomes a red giant, Perhaps as large as the orbit of Venus, or even the orbit of the Earth The Sun today The Sun as a red giant The orbit of Venus

The Sun’s Final Glory He BIRTH H NOW

What’s Left? A White Dwarf Mass: 50% Sun Density: 1-2 tons per cc3 Composition: C & O, the “ashes” of nuclear fusion Cools & fades slowly 12,000 Km Sirius B

Sirius b Nearest White Dwarf Star Diameter: 1/100 Sun Mass: 98% Sun Distance: 8.6 LY Sirius b

BIGGEST VY Canis Majoris The The Sun A red “hypergiant” star Credit: NASA/ESA/R Humphreys/U Minnesota) A red “hypergiant” star Diameter: 2000 x Sun Mass: 30-40 x Sun Luminosity: 500,000 x Sun 5,000 light-years away VY Canis Majoris

BRIGHTEST & MOST MASSIVE Mass = 265 Suns (probably 320 Suns at birth!) Luminosity = 8-9 million x Sun Diameter: 35 x Sun Distance: 165,000 LY Future hypernova? R136A* Located in the Large Magellanic Cloud

The HOTTEST STARS are tiny, dim, new white dwarfs T=200,000 C NGC 2440 (central star) Distance: 4500 LY NGC 6302 (central star) Distance: 3800 LY Hidden by central dust ring KPD 0005+5106 Distance: 2500 LY Only 2200 years “old”

COLDEST Stars The Brown Dwarfs! WISE 1828+2650 Temperature ~25 C About 27 LY Mass < 0.1 Suns Too small for nuclear fusion

The Oldest Stars! HE 1523-0901 13.2 billion years old Mass: 0.8 Suns Distance: ~7500 LY A red giant star Today 13.2 billion Years ago

The Youngest Stars Stars are forming today in the “empty” regions of interstellar space.

Stages of Star Formation

Stars on the Weird Side!

The Famous Pleiades Distance: 1300 LY Brightest Star Cluster Formed about 115 million years ago The blue glow is dust!

V838 Monocerotis – The Light Echo V838 is a “central star” of a planetary nebula Distance: 20,000 LY Mass: 5-10 Suns (originally much more massive) Outburst in 2002 - The “expanding shell” is actually an expanding light echo

V838 Monocerotis – The Light Echo To Earth Arrives first Arrives later

A Real Shooting Star! 13 LY tail 291,000 mph Mira = Omicron Ceti An unstable red giant Losing mass Distance: 400 LY Mass: 1.2 Suns 13 LY tail 291,000 mph GALEX GALEX As seen by Hubble

Epsilon Aurigae Dust Disk Binary star (6 + 8 Suns) 27 year period One star is invisible! An unseen blue star hides in a disk of dust that orbits a yellow supergiant When the blue star passes in front of the yellow star, the disk blocks the light of yellow star 8 AU Dust Disk

Stellar Cannibalism Binary stars that orbit close together often transfer mass between the stars Semi -Detached Binary Detached Binary Contact Binary Warning: Artist’s Conceptions

R Corona Borealis – The “Fade Out” Star Yellow supergiant star Distance: 6000 LY Mass: 0.8 Suns Sometimes fades by a factor of 1000 or more in brightness! Emits “puffs” of soot that block the light of the star This star smokes!

More R Corona Borealis Extreme helium star Very little hydrogen Lots of carbon Origin: merger of two white dwarfs?

Extreme Spots! Artist Conception HD 12545 holds the record for the largest “starspot” Warning: Artist’s Conception The rotation and revolution of close binary stars are locked together, forcing the stars to rotate as fast as they orbit. Fast rotation makes big spots.

Extreme Rotation! Rotates every 16 hrs! Other stars, too! Regulus Regulus = Alpha Leo Distance: 78 LY Mass: 3.8 Suns Radius: 3-5 Suns Altair Vega Rotates every 16 hrs! Other stars, too!

Crab Pulsar MORE EXTREME ROTATION Distance: 6500 LY Mass: ~ 1.4-2.0 Suns Remnant of 1054 Supernova Density: 100,000,000 tons per thimbleful Spins 30 times per second

Magnetars! Extreme Neutron Stars SGR 1900+14 Magnetars! Extreme Neutron Stars SGR 1900+14 Distance: 20,000 LY Mass: ~ 2 Suns Diameter: ~20 Km 7 LY Most intense magnetic fields in the Universe Hundreds of millions times stronger than the strongest human-made magnets Only 5 known Sources of intense gamma ray bursts Warning: Artist’s Conception

Supernova 1987a

Supernova 1987a Detected in 1987 Exploded 170,000 years ago Originally about 18 solar masses Where is the neutron star?

Black Holes Closest candidate: Best candidate: V616 Mon Distance: 3000 LY Star mass: ~0.5 Suns BH mass: ~6 Suns BH Diameter: ~40 km Orbit period: 7.75 hrs Best candidate: V404 Cyg Distance: 7,800 LY Star mass: ~0.7 Suns BH mass: ~12 Suns BH Diameter: ~75 km Orbital period: 6.5 days

The Universe is Full of Surprises! And that’s what makes astronomy so much fun!

Kirkwood Observatory Open Tonight, 10:30-11:30PM Weather permitting! Kirkwood Observatory is located at the west end of Dunn’s Woods, behind Bryan Hall

Happy Summer Solstice! On the handout: URL for this presentation on the Web Related websites Kirkwood Observatory open tonight