Lab 8 – The Distance to the Pleiades. Open or Galactic Cluster.

Slides:



Advertisements
Similar presentations
Copy and Answer in NB 1.What are the three layers of the suns atmosphere? 2.What produces auroras? 3.What are sunspots and why are they dark? 4.Describe.
Advertisements

Agenda Review magnitude scale and HR diagrams
Stars Mr. Skirbst Physical Science Topic 25. Stars Composition: - determined by spectral analysis - hydrogen (60 – 80%) - helium (20 – 30%) - other (O,
Measuring Distance and Size of Stars Physics 113 Goderya Chapter(s): 9 Learning Outcomes:
The HR Diagram Astronomy 315 Professor Lee Carkner Lecture 8.
Do NOT open CLEA until all the black boxes have finished loading.
The Universe  Viewing the Night Sky Clear view of the horizon ○ Stay away from ambient light, houses, & trees A good star chart Telescope or binoculars.
Clicker Question: The HR diagram is a plot of stellar A: mass vs diameter. B: luminosity vs temperature C: mass vs luminosity D: temperature vs diameter.
Building the Hertzsprung-Russell (H-R) Diagram Use the worksheets passed out in class.
Logarithms and The Distance Modulus. Logarithms and Exponents 10 2 = = 1000 Question asked: If you multiply a number by itself a number of times.
The Family of Stars Please press “1” to test your transmitter.
The Nature of the Stars Chapter 19. Parallax.
Another galaxy: NGC The Milky Way roughly resembles it.
PG. 127 Measuring the Stars. Groups of stars Long ago, people grouped bright stars and named them after animals, mythological characters or every day.
Red Stars, Blue Stars, Old Stars, New Stars Session 1 Julie Lutz University of Washington.
Measuring the Stars How big are stars? How far away are they?
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.
HR Diagram. Characteristics of Stars  Temperature/Color  Mass  Luminosity Absolute Magnitude Apparent Magnitude.
Chapter 19 Star Formation
Measuring Stellar Distances Stellar Parallax few hundred pc Absolute & Apparent Magnitudes distance Spectroscopic Parallax Cepheid variables.
PULSATING VARIABLE STARS Types of Intrinsic Variables:  Long-period variables  Cepheid variables  RR Lyrae variables  Flare stars Cepheid variables.
Stars. Astronomy The study of space How astronomers measure distance 1. Light years– The distance light travels in one year 9.461x km.
Announcements Project Medley Outlines due Tuesday! – 1 page typed and double-spaced – What do you plan to do for your project? On-Campus Observing Moved.
The Nature of the Stars Chapter 19. Parallax.
Stellar Characteristics. Temperature Temp. is measured in Kelvins Blue stars are hot, above 30,000 K Yellow stars are warm Red stars are cool, below 3,000.
Stars Classifying stars: H-R diagram Vogt-Russell theorem Mass-luminosity relation Evolution on the HR diagram.
 Stars can be classified in three ways:  Size – How massive the star is  Temperature – A stars color reveals its temperature. ▪ Red stars have a cooler.
Ch. 28 The Stars Properties of Stars ???
Classification of Stars – HR diagram Objectives: understand the differences between near and bright visible stars learn how to use the HR-diagram to classify.
Measuring the Stars Chapter Grouping of Stars Groups of stars named after animals, mythological characters, or everyday objects are called constellations.
Characteristics of Stars. Stars… Are hot balls of plasma that shine because nuclear fusion is happening at their cores… they create their own light Have.
Objectives Determine how distances between stars are measured. Distinguish between brightness and luminosity. Identify the properties used to classify.
Friday, February Turn in your Matter Storyboard and your Vocab Poster. Remember, your Study Guide is due Monday (at the BEGINNING of class). 2. Take.
Intro to Astrophysics Dr. Bill Pezzaglia 1 Updated: Nov 2007.
Star Properties (Chapter 8). Student Learning Objectives Classify stars Explain how star properties are related.
Stars.
Cluster. Star Clusters A nebula often results in a cluster of stars. A cluster of stars from the same molecular cloud: –were formed at about the same.
Stellar Clusters Homework Problems Chapter 13
 Students will be able to determine how distances between stars are measured.  Students will be able to distinguish between brightness and luminosity.
PHYS 206 Stars in General Only 6 of the 20 brightest stars in the sky are closer to us than 10pc  14 of the 20 brightest stars in the sky must have absolute.
Measuring the Stars What properties of stars might you want to determine?
Measuring the Stars How big are stars? How far away are they? How bright are they? How hot? How old, and how long do they live? What is their chemical.
Characteristics of Stars Basics Star = body of gas Gives off heat & light Vary in size, color, composition, temperature & brightness.
A105 Stars and Galaxies  Homework due today  Remote observing this weekend Today’s APODAPOD.
Properties of Stars: Brightness (37). Remember… We have learned how to determine a star’s: We have learned how to determine a star’s: –Chemical Composition.
David Randall.  What is a H-R Diagram?  What is an open cluster?  Why open clusters?  Procedure.
 Learning Target: Describe the properties of Stars  Kick off: What are three important things you learned last semester. Vocabulary: 1. magnitude 2.
Measuring Stars. Visible Spectrum & Wavelengths Spectral Types Continuous spectrum: Produced when white light passes through a prism Emission spectra:
Chapter 25 Beyond Our Solar System
Hertzsprung–Russell diagram review. Temperature Luminosity An H-R diagram plots the luminosities and temperatures of stars.
What is a Hertzsprung-Russell Diagram?
Stars.
Lab 7 – The HR Diagram.
The Hertzsprung-Russell Diagram (a.k.a. H-R Diagram)
Properties of Stars Apparent Magnitude: the brightness of a star as it appears from Earth. Size Temperature Distance Absolute Magnitude: how bright the.
The Characteristics of Stars
Stars.
Stars.
Unit 8: Star Light Star Bright Assessment Review
Astronomy 105 Laboratory Lab 09.
Characteristics of Stars Chapter 3 Section 4 ISN p. 33
Astronomy 105 Laboratory Lab 07.
Lab 9 – Ages and Distances to Clusters
Chapter 10 Star Cluster.
Basic Properties of Stars
The Lifecycle of Stars.
The Hertzsprung-Russell Diagram (a.k.a. H-R Diagram)
Stellar position, distance, and properties
Properties of Stars Apparent Magnitude: the brightness of a star as it appears from Earth. Size Temperature Distance Absolute Magnitude: how bright the.
The Hertzsprung-Russell Diagram (a.k.a. H-R Diagram)
Presentation transcript:

Lab 8 – The Distance to the Pleiades

Open or Galactic Cluster

M13 - Globular Cluster Distance-23,000 ly Size-150 ly

Stars in a Cluster Common Properties Distance Age Chemical composition Different Properties Spectral Types (temperature) Luminosity Class (size) Mass

D >10 pc 10 pc D <10 pc 10 pc Star Cluster D >10 pc D <10 pc O B A F G K M Main-sequence HR Diagram O B A F G K M Color-Magnitude Diagram Distance Modulus = m - M The difference between the absolute magnitude and the apparent magnitude can be used to find the distance to a star cluster. If m-M > 0 then the distance to the cluster is > 10 pc. If m-M = 0 then the distance to the cluster is = 10 pc. If m-M < 0 then the distance to the cluster is < 10 pc. DM { Distance Modulus

n Interstellar Dust –Reddens Light (makes stars appear cooler) –Dims Light (makes stars appear further away)

Pleiades - Open Cluster

The End.