Constellations An group of stars the ancients originally named after mythical characters.

Slides:



Advertisements
Similar presentations
30.1 notes Characteristics of Stars
Advertisements

Introduction to Stars. Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs” By definition,
Chapter 11 Surveying the Stars. I.Parallax and distance. II.Luminosity and brightness Apparent Brightness (ignore “magnitude system” in book) Absolute.
Measuring Distance and Size of Stars Physics 113 Goderya Chapter(s): 9 Learning Outcomes:
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 10 Measuring the Stars.
Properties of Stars How do we measure stellar luminosities?
Constellations are groups of stars, sometimes in patterns of animals, or objects. Constellations are important because they can help define where in the.
Susan CartwrightOur Evolving Universe1 Introduction: The Night Sky n What do we see in the night sky? l l the Moon l l moving planets l l occasional comets.
Chapter 12: Surveying the Stars
CHAPTER 28 STARS AND GALAXIES
ASTR 1200 Announcements Website Second problem set due next Tuesday in class. Observatory Sessions.
Pages  Star color is an indication of temperature  Very hot stars (30,000 K) emit high-energy, low wavelength radiation. What color do they.
How Do Astronomers Measure the Brightness of a Star?  Stars vary greatly in brightness  Early peoples observed bright stars and grouped them into constellations.
Stars and galaxies. Constellations  Ancient Greeks, Romans and other cultures saw patterns of stars in the sky called constellations  They imagined.
Section #1: Properties of Stars.  Stars in the night sky display many characteristics and patterns.  Noticeable patterns seen among stars are called.
© 2010 Pearson Education, Inc. Chapter 15 Surveying the Stars.
Chapter 29 Notes Stars. The Sun: Solar Atmosphere Photoshere: visible surface, 5800 K Chromosphere: 30,000 K Corona: 1 to 2 million K, solar wind.
Stars.
Stars.
Astronomical Distances. Stars that seem to be close may actually be very far away from each other.
Stars!!!! Galaxies and the Universe too!. Stars are far away! The closest star to Earth is the sun. The next closest is Proxima Centauri If you can travel.
All stars form in clouds of dust and gas. Balance of pressure: outward from core and inward from gravity.
25.1 – Properties of Stars – Part I. Do Now  What does a star's color tell us about a star?
Prior Knowledge Questions (Do these BEFORE using the Gizmo.)
Chapter 22 Stars.
Cas Beta – 55ly Alpha- 230ly Gamma- 615ly Delta- 100ly Epsilon- 440ly.
Stars.
Ch. 12 Lesson 1 Stars. What are stars? A star is large ball of gas that emits (gives off) energy produced by nuclear reactions in the star’s interior.
Measuring the Stars Chapter Grouping of Stars Groups of stars named after animals, mythological characters, or everyday objects are called constellations.
Properties of Stars. Star Color – the color of a star is a clue to its temperature a.The coolest stars are red b.The medium stars are yellow c.The hottest.
Objectives Determine how distances between stars are measured. Distinguish between brightness and luminosity. Identify the properties used to classify.
EARTH & SPACE SCIENCE Chapter 30 Stars, Galaxies, and the Universe
The Sun Composed of hydrogen and helium. Very dense core, all gaseous because of the very high temperatures. The Sun is the largest object in terms of.
Characteristics of Stars. Distances and Size Magnitude Elements Mass and Temperature.
 Students will be able to determine how distances between stars are measured.  Students will be able to distinguish between brightness and luminosity.
Characteristics of Stars There are millions of stars in the universe, but they are very far apart. Because of this, distances between stars are measured.
Stellar Parallax Magnitude and H-R Diagram
Characteristics of Stars
Characteristics of Stars. What is a galaxy? It is a cluster of stars (hundreds of billions of stars) It is a cluster of stars (hundreds of billions of.
Stars Goal: Compare star color to star temperature.
“I always wanted to be somebody, but I should have been more specific.” Lilly Tomlin Any late HW2 are due before class on Wednesday. HW2 solutions posted.
Copyright © 2012 Pearson Education, Inc. Chapter 11 Surveying the Stars.
Characteristics of Stars. Distances and Size Magnitude Elements Mass and Temperature.
Measuring Stars. Visible Spectrum & Wavelengths Spectral Types Continuous spectrum: Produced when white light passes through a prism Emission spectra:
Stars and Their Characteristics Constellations Constellation- groups of stars that appear to form patterns –88 constellations can be seen from n.
Characteristics of Stars. What is a galaxy? (hundreds of billions of stars) (hundreds of billions of stars) Our solar system is located in the Our solar.
Study of the universe (Earth as a planet and beyond)
Chapter 25 Beyond Our Solar System
Study of the universe (Earth as a planet and beyond)
Astronomy Basic Properties of Stars. Kirchhoff’s Three Kinds of Spectra.
Study of the universe (Earth as a planet and beyond)
CHARACTERISTICS OF STARS 21-2 STARS Stars “twinkle” because our atmosphere causes them to shimmer and blur. A star is a very large ball of mostly hydrogen.
DO NOW: Write it down  1. Most of the galaxies in the universe are moving __________ from us. 2. Our evidence to support this is ___ ___________________________.
Distances in Space Characteristics of Stars
Stars Essential Questions:
28-1 A Closer Look at Light A. What is Light?
The Sun is the largest object in the solar system.
25.1 Properties of Stars Objectives:
Section 2: Measuring the Stars
Characteristics of Stars
Stars.
How Hot, Big, & Far?.
The Characteristics of Stars
Parallax and Measuring the universe notes
Stars.
Stars.
Section 2: Measuring the Stars
Basic Properties of Stars
What is a star? - body of gasses that give off “tons of” energy (light & heat) - clusters = those little specks in the sky that we see may really be more.
Stellar position, distance, and properties
Presentation transcript:

Constellations An group of stars the ancients originally named after mythical characters

Measuring the Stars Parallax Apparent shift in position of a star relative to other stars caused by the motion of the observer. The larger the effect of parallax the closer the star is. Parallax is used to estimate distances to nearby stars.

Parallax

Original Photo Photo taken 6 months later

Measuring the Stars Light-year The distance light travels in 1 year Speed = 3 × 10 8 m/s (300,000,000 m/s) Parsec Equal to 3.26 light years The distance at which an object has a parallax of one arc second.

Magnitude The brightness of a star The lower the magnitude, the brighter the object Each lower magnitude is 2.5 brighter than the next Magnitude 1 star is brighter than a magnitude 2 star Can have a zero magnitude and negative magnitude Examples A magnitude 1 star is 2.5 times brighter than a magnitude 2 star A magnitude 2 star is 2.5 times brighter than a magnitude 3 star

How many times brighter is a magnitude 1 star compared to a magnitude 3 star? How many times brighter is a magnitude 1 star compared to a magnitude 4 star?

How many times brighter is a magnitude 1 star compared to a magnitude 3 star? 2.5*2.5 = 6.25 How many times brighter is a magnitude 1 star compared to a magnitude 4 star? 2.5*2.5*2.5 = 15.6

Apparent magnitude How bright a star appears to be as observed from Earth. Depends on distance Absolute magnitude The brightness an object would have if it were placed at a distance of 10 parsecs (32.6 light years) from Earth. Does not depend on distance

Luminosity The amount of energy that a light source emits per second Does not depend on distance Depends on temperature & size Varies from (.0001 to 1 millions) times brighter than the sun

Luminosity For an analogy with which you are familiar, consider again the headlights of a car. When the car is far away, even if its high beams are on, the lights will not appear too bright. However, when the car passes you within 10 feet, its lights may appear blindingly bright. To think of this another way, given two light sources with the same luminosity, the closer light source will appear brighter. However, not all light bulbs are the same luminosity. If you put an automobile headlight 10 feet away and a flashlight 10 feet away, the flashlight will appear fainter because its luminosity is smaller

MASS of a STAR Mass of a star determines Temperature & Size Temperature & size determines L uminosity Greater original mass of star  shorter life span

More massive a star  greater gravity pressing inward Greater gravity  requires greater density inside the star in order to balance its own gravity. Greater density  higher temperature in the core Higher temperature  faster the rate of nuclear fusion Faster the rate of nuclear fusion  larger energy output Larger energy output  greater luminosity

Greater luminosity  More rapidly it burns hydrogen fuel  Shorter lifespan of the star Greater original mass of star  shorter life span

Alpha Centauri 4.3 light years away is the closest star to our solar system