Ask the Scientists Questions for Dr. Butner Star Formation 1/29/11.

Slides:



Advertisements
Similar presentations
Nebula to Protostar Giant molecular clouds within a nebula contract under the gravitational pressure, increasing its thermal energy. CO, NO, OH- Giant.
Advertisements

The Solar System and our Universe
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.
Star Life Cycle.
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,
Star Life Cycle.
Chapter 12 Space Exploration.
Life Cycle of Stars. Birth of a Star Born from interstellar matter (dust & gases) – Denser portions of the nebula Nebula begins to contract – Due to gravity.
Explore the Law of Gravity by demonstrating that gravity is a force that can be overcome.
Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe.
A History of the Universe Astronomy 315 Professor Lee Carkner Lecture 2.
© 2010 Pearson Education, Inc. Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe.
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.
The Formation of the Solar System How did it get to be this way?
Susan CartwrightOur Evolving Universe1 Star Birth n Most of the bright stars we see have lifetimes much less than the age of the Solar System l l star.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Goal: To understand how stars form. Objectives: 1)To learn about the properties for the initial gas cloud for 1 star. 2)To understand the collapse and.
Overview of Astronomy AST 200. Astronomy Nature designs the Experiment Nature designs the Experiment Tools Tools 1) Imaging 2) Spectroscopy 3) Computational.
Ch. 4 Sec. 5 The Expanding Universe Discover activity- How Does the Universe Expand pg What happens to the distances between galaxies that are.
Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe
Dark Matter, Dark Energy, How Come Some People Think We Need It and Others Don’t and the Fate of the Universe.
Star Formation. Introduction Star-Forming Regions The Formation of Stars Like the Sun Stars of Other Masses Observations of Brown Dwarfs Observations.
Star Formation Star = large balls of gas that produce energy and shine…. unless old. Nuclear Fusion = combines light elements to create heavy ones….
Stellar Brightness.  Apparent magnitude: brightness of a star as seen from Earth  The Ancient Greeks put the stars they could see into six groups. 
Chapter 12 Space Exploration. Section 12.1 page 428 Explaining the Early Universe GALAXY – collection of stars, planets, gas and dust held together by.
What causes day and night? (Please get this right…) What causes day and night? (Please get this right…) Do you see different stars at night here than you.
Quiz #6 Most stars form in the spiral arms of galaxies Stars form in clusters, with all types of stars forming. O,B,A,F,G,K,M Spiral arms barely move,
Astronomy: Life Cycle of A Star
Warm up The sun is 4.6 billion years old – how can it continue to produce so much heat and light?
Ch 26.2 & 3 Life Cycle of Average & Low Mass Stars 1.What are the stages of star low and average mass stars? 2.How does the star’s composition change as.
Life Cycle of a Star The changes that a star goes through is determined by how much mass the star has. Two Types of Life Cycles: Average Star- a star with.
Chapter 12 Space Exploration. Section 12.1 page 428 Explaining the Early Universe GALAXY – collection of stars, planets, gas and dust held together by.
What makes up the Solar System and what force is holding it in place? The Force of Gravity hold our Solar System in Place. Things that make up our Solar.
Chapter 12 Space Exploration. Section 12.1 page 428 Explaining the Early Universe GALAXY – collection of stars, planets, gas and dust held together by.
The Sun-Earth-Moon System. What is the moon? The moon is a natural satellite of Earth This means that the moon orbits Earth.
1) Name the planets in our solar system in order
Stars A star is a large, glowing ball of gas in space, which generates energy through nuclear fusion in its core. The closest start to Earth is the sun,
Exploring the Universe. Big Bang Theory The big bang theory is how the scientist say the universe began. How the Big Bang Started most people believe.
Study Notes for Chapter 30: Stars, Galaxies, and the Universe.
The Life Cycle of Stars.
Definition: A gigantic cloud of dust and gas in the universe that clumps together to form stars and planets. Facts: The gas is mostly the smallest atoms-
Study of the universe (Earth as a planet and beyond)
BEYOND OUR SOLAR SYSTEM CHAPTER 25 Part II. INTERSTELLAR MATTER NEBULA BRIGHT NEBULAE EMISSION NEBULA REFLECTION NEBULA SUPERNOVA REMANTS DARK NEBULAE.
The Beginnings … Of the Universe & Our Solar System.
Space Nebulae & Black Holes. Nebula Derived from the Latin word for "clouds". Nebulae are the basic building blocks of the universe They contain the elements.
The Big Bang.  Cosmology – The study of the structure and evolution of the universe.  Big Bang Theory – The universe was very hot and small. Billions.
Life of Stars. Star Birth – Nebular Model Huge clouds of gas and dust occur in space – may be exploded stars Most Nebulae (gas clouds) are invisible –
© 2010 Pearson Education, Inc. Chapter 14 Dark Matter and Dark Energy.
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,
Formation of Our Solar System
12-2 Notes How Stars Shine Chapter 12, Lesson 2.
Stellar Evolution Pressure vs. Gravity.
The Lives of Stars.
Interesting Stuff in Space
The Lives of Stars.
EARTH SCIENCE. WRITTEN WORK25% PERFORMANCE TASK50% QUARTERLY ASSESSMENT 25%
8 Space physics Topic overview
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
UNIT 10 PLANETS.
Composition of Stars Classify stars by their color, size, and brightness. Other properties of stars are chemical composition and mass. Color and Temperature.
Review: 1. How is the mass of stars determined?
The Life Cycle of Stars Starry, Starry Night.
FORMATION OF THE UNIVERSE
Bellwork 12/13 Thinking about our simulation last class…
3A Objectives Describe the nebular theory in detail.
Chapter 15 – Stars, Galaxies and the Universe
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Presentation transcript:

Ask the Scientists Questions for Dr. Butner Star Formation 1/29/11

How can you tell the difference between a star that is forming and a star that is about to collapse For massive stars, it might not be so easy as those stars seem to live very short lives. However, even for these stars, they seem to disperse their surrounding cloud material before they die. So as a starting point we might say that… New stars (forming stars) are surrounded by cold dust and gas Dying stars (stars about to collapse) might have shells of material (planetary nebulae or winds) that they have sent off into space signaling that their internal structure is becoming unstable

Examples Spectra are also different between the objects as well so you can use the derived properties (temperature, density, abundances) to help sort out which is which. Star Formation Note the extended gas/dark nebulae Planetary Nebulae Relatively Isolated Environment

What is the role of dark matter in the process of star formation Dark Matter – it is the material responsible for gravitational effects seen on very large scales Galaxies need dark matter (or something) to explain their rotation curves Clusters of galaxies need dark matter to explain the member velocities (i.e. if bound by gravity there is more material than we see). So what does that mean for star formation? Local star formation – probably not a big impact since the density of dark matter in our neck of the woods in the galaxy not great But…

Early Star Formation Dark Matter Can Be Important Recent results from the Herschel satellite suggest Early galaxies seem to have a burst of star formation when the associated amount of mass including dark matter is about 300,000,000,000 solar masses! See this story in Science Daily from 02/17/11 Early stars might be affected by dark matter Lots of models are being developed to explore HOW dark matter might change the mass of stars that are formed and hence the early production of heavier elements.

Are dark matter and dark energy related to star formation? Dark matter may influence early galaxy formation and the first stars. See recent results from Hubble Space Telescope and Herschel Telescope Check out Dark energy will affect star formation in the future as its influence grows. It will make star formation harder as even the galaxies are pulled apart.

Are the dark clouds collapsing, spreading or both? Both In some cases, they are collapsing as gravity wins over other forces In other cases, they are spreading (expanding) as other forces – such as stellar winds, radiation pressure, thermal pressure – overcome gravity Currently astronomers are trying to figure out what is going on with specific examples – and see what influences are important at what time in the process…

The sun will expand into a red giant before collapsing into a white dwarf, causing the earth to heat up to an uninhabitable climate. All planets should be similarly affected. When Mars warms up could it become a viable ``surrogate planet’’ for life since it has water? A definite maybe!

The Yes part If there is enough water underground… If we move a comet ``onto’’ Mars, we can add water The Maybe part Depends on the actual brightness of the sun. It might get more than 100 x its current brightness If it is too bright, even Mars might be too hot. Jupiter’s moon Europa might be a better choice…