Measuring the Stars. Chapter 10. Chapters 17, 19, 18

Similar documents
Chapter 8: The Family of Stars

Magnitudes. How Powerful Are the Stars? Luminosities of Different Stars

How does the Sun shine? What is the Sun s structure? Lifetime of the Sun. Luminosity of the Sun. Radiation Zone. Core 3/30/17

Stars. Properties of Stars

Light III The Atom & Spectra. February 12, 2012

a. Star A c. The two stars are the same distance b. Star B d. Not enough information

Photographs of a Star Cluster. Spectra of a Star Cluster. What can we learn directly by analyzing the spectrum of a star? 4/1/09

Chapter 11 Surveying the Stars

Spectra of a Star Cluster. Photographs of a Star Cluster. What can we learn directly by analyzing the spectrum of a star? 4/1/09

A1101, Lab 5: The Hertzsprung- Russell Diagram Laboratory Worksheet

15.1 Properties of Stars

Get ready for quiz # 5! Get out a ½ sheet and Calculator

Pr P ope p rti t es s of o f St S a t rs

Gaia Launched in Dec D map of the stars near Sun = 10% of Galaxy Measure the positions of a billion stars to brightness V=20 Precise to

5. A particular star has an angle of parallax of 0.2 arcsecond. What is the distance to this star? A) 50 pc B) 2 pc C) 5 pc D) 0.

Astronomical Measurements: Brightness-Luminosity-Distance-Radius- Temperature-Mass. Dr. Ugur GUVEN

Stars III The Hertzsprung-Russell Diagram

Mass-Luminosity and Stellar Lifetimes WS

Chapter 15: Surveying the Stars

ASTRONOMY QUIZ NUMBER 11

Lecture 26 The Hertzsprung- Russell Diagram January 13b, 2014

The Cosmic Perspective. Surveying the Properties of Stars. Surveying the Stars. How do we measure stellar luminosities?

Midterm Study Guide Astronomy 122

Review: HR Diagram. Label A, B, C respectively

Lecture 10: The Hertzsprung-Russell Diagram Reading: Sections

OPEN CLUSTER PRELAB The first place to look for answers is in the lab script!

The Sun (chapter 14) some of this is review from quiz 3, but you should

HOMEWORK - Chapter 17 The Stars

OPEN CLUSTERS LAB. I. Introduction: II. HR Diagram NAME:

Review Questions for the new topics that will be on the Final Exam

Chapter 15 Surveying the Stars Pearson Education, Inc.

Astronomy 1 Fall 2016

Announcement Test 2. is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar points, scantron, 1 hr.

Types of Spectra. How do spectrum lines form? 3/30/09. Electron cloud. Atom. Nucleus

PARALLAX AND PROPER MOTION

The Hertzsprung - Russell Diagram Laboratory 11

ClassAction: Stellar Properties Module Instructor s Manual

Book page cgrahamphysics.com Stellar Spectra

Extrasolar planets. Lecture 23, 4/22/14

Hydrogen Lines. What can we learn from light? Spectral Classification. Visible Hydrogen Spectrum Lines: Series. Actual Spectrum from SDSS

Properties of Stars & H-R Diagram

Chapter 10 Measuring the Stars

Distances to the stars Friedrich Bessel Cygni 10 light years. Just beat Struve and Henderson who measured Vega and α Centauri respectively.

Astronomy 141 Life in the Universe Professor Gaudi Homework #4 Solutions

Characterizing Stars

The Hertzprung-Russell (HR) Diagram

Organizing the Family of Stars:

Stars, Galaxies & the Universe Announcements. Stars, Galaxies & the Universe Observing Highlights. Stars, Galaxies & the Universe Lecture Outline

HR Diagram Student Guide

Agenda. LAB (Inst. Dickinson): Lab Constellation/Star Quiz Angular Measurement Lab

Lab 3: Stars, Stars, Stars!

Assignments for Monday Oct. 22. Read Ch Do Online Exercise 10 ("H-R Diagram" tutorial)

ASTR-1020: Astronomy II Course Lecture Notes Section III

Lecture Outlines. Chapter 17. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Astron 104 Laboratory #8 The H-R Diagram

Measuring stellar distances.

Hertzprung-Russel and colormagnitude. ASTR320 Wednesday January 31, 2018

Chapter 15 Surveying the Stars

Astro 1050 Mon. Apr. 3, 2017

Astronomy 150: Killer Skies. Lecture 20, March 7

Determining the Properties of the Stars

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. Dr. Joseph E. Pesce, Ph.D.

Astron 104 Laboratory #9 The H-R Diagram

Hertzsprung-Russel Diagrams and Distance to Stars

Gaia Launched in Dec D map of the stars near Sun = 10% of Galaxy Measure the positions of a billion stars to brightness V=20 Precise to

INSIDE LAB 8: Plotting Stars on the Hertzsprung- Russell Diagram

Stars I. Distance and Magnitude. How Does One Measure Distance? Distances. Stellar Parallax. Distance Equation some examples!

Reading and Announcements. Read Chapters 8.3, 11.5, 12.1 Quiz #5, Thursday, March 21 Homework #5 due Tuesday, March 19

( ) = 5log pc NAME: OPEN CLUSTER PRELAB

Convection causes granules. Photosphere isn t actually smooth! Granules Up-Close: like boiling water. Corona or of the Sun. Chromosphere: sphere of

Newton s Laws of Motion

Lab 8: Stellar Classification and the H-R Diagram

Parallax: Measuring the distance to Stars

Chapter 15 Lecture. The Cosmic Perspective Seventh Edition. Surveying the Stars Pearson Education, Inc.

Atoms and Spectra October 8th, 2013

Galaxies and Cosmology

Intro to Astrophysics

The Problem. Until 1995, we only knew of one Solar System - our own

Attendance Quiz. Are you here today? (a) yes (b) no (c) Captain, the sensors indicate a class M planet orbiting this star. Here!

Test #2 results. Grades posted in UNM Learn. Along with current grade in the class

Parallax: Space Observatories. Stars, Galaxies & the Universe Announcements. Stars, Galaxies & Universe Lecture #7 Outline

The Life Histories of Stars I. Birth and Violent Lives

Chapter 15 Surveying the Stars Properties of Stars

A star is at a distance of 1.3 parsecs, what is its parallax?

Black Hole Binary System. Outline - Feb. 25, Constraining the Size of the Region that Contains the Invisible Mass

Stars: basic observations

Astronomy 210 Spring 2017: Quiz 5 Question Packet 1. can: 2. An electron moving between energy levels

Lecture 14: Studying the stars. Astronomy 111 Monday October 16, 2017

Lecture 12: Distances to stars. Astronomy 111

Temperature and Radiation. What can we learn from light? Temperature, Heat, or Thermal Energy? Kelvin Temperature Scale

Properties of Stars. For such huge objects, stars have comparatively simple properties when seen from a long way off

OTHER MOTIONS. Just so far away they appear to move very slowly

Remember from Stefan-Boltzmann that 4 2 4

Model of Stars 5 Oct

Lecture 21. Stellar Size

HR Diagram Lab. Area 1 Area 4. Area 5. Area 2. Area 6 Area 3

For instance, for a particular star cluster, these data were derived:

Star Magnitudes & Distances with Stellarium (Stellarium Exercise #2)

Guiding Questions. Measuring Stars

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003

Transcription:

Measuring the Stars Chapter 10 Chapters 17, 19, 18 1

2

3

Bessel Hipparcos 4

Lecture-Tutorial on Parallax and the Parsec p 37 6) Consider two stars (C and D) that both exhibit parallax. If C appears to move back and forth by a greater amount than D, which do you think is actually closer to you? C. Star C D. Star D 5

9) If the parallax angle for Star A (p A ) is 1 arcsecond, what is the distance from the Sun to Star A? (Hint: Use parsec as your unit of distance.) 10) Is a parsec a unit of length or a unit of angle? It can t be both. 12) Place a second star Star B on the dotted line, farther from the Sun than Star A. Which star, the closer one (Star A) or the farther one (Star B), has the larger parallax angle? 6

1) Which of the following stars is closest to us? a. Procyon (parallax angle = 0.29 ) b. Ross 780 (parallax = 0.21 ) c. Regulus (parallax = 0.04 ) d. Sirius (parallax = 0.38 ) 7

8

What do you do in a Lecture-Tutorial? Work with a partner (or group of 3)! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Take time to understand it now! Come to a consensus answer you all agree on. If you get stuck, or are not sure of your answer, ask another group. If you re still stuck, raise your hand, and I ll help. 9

5) The star Lee has an apparent magnitude of 0.1 and is located about 250 pc away from Earth. Which of the following is most likely the absolute magnitude for Lee? A. -6.9 B. 0.1 C. 7.1 10

Vega has an apparent magnitude of 0.03 and an absolute magnitude of 0.58. If it were moved twice as far from Earth as it is now, which of the following would occur? a) Apparent magnitude number would increase b) Apparent magnitude number would decrease c) Apparent magnitude number would stay the same d) Absolute magnitude number would increase e) Absolute magnitude number would decrease 11

12

13

14

15

16

17

18

http://wwnorton.com/college/astronomy/under standing-our-universe/ 19

The Harvard Computers, 1913 20

If you analyze the light from a low density object (such as a cloud of interstellar gas), which type of spectrum do you see? a. Dark line absorption spectrum b. Bright line emission spectrum c. Continuous spectrum 21

22

23

24

The two axes on the Hertzsprung- Russell (H-R) diagram can be a) luminosity and temperature. b) apparent magnitude and absolute magnitude. c) radius and main sequence. d) radius and luminosity. e) spectral type and temperature. 25

26

Lecture-Tutorial book page 55: Luminosity, Temp, and Size 27

If you have two hot plates of the same temperature, which will cook the large pot of spaghetti first? a. The smaller hot plate. b. The bigger hot plate. c. Both will cook at the same rate since the temperature is the same. If two stars have the same temperature, but Star Jack is more luminous than Star Jill, which of the following is true? a. Jack is bigger than Jill b. Jill is bigger than Jack c. Jack and Jill are the same size d. There is no way to tell which star is bigger. 28

If two stars have the same size, but Star Alpha has a higher surface temperature than Star Beta, which of the following is true? a. Alpha is more luminous than Beta. b. Beta is more luminous than Alpha. c. Alpha and Beta have the same luminosity. d. There is no way to tell which star is more luminous. Lecture-Tutorial book page 55: Luminosity, Temp, and Size 29

Look at the HR diagram. Which star is larger, X or Y? a. X is larger b. Y is larger c. Same size d. No way to tell Look at the HR diagram. Which star is larger, Y or V? a. Y is larger b. V is larger c. Same size d. No way to tell 30

Suppose a star gets more luminous but does not change its temperature. What is happening? A. The star is contracting. B. The star is expanding C. The star is getting more massive. D. The star is changing its spectral type. AstroTour Stellar Spectrum Click here to launch this AstroTour (Requires an active Internet connection.) 31

AstroTour Atomic Energy Levels and the Bohr Model Click here to launch this AstroTour (Requires an active Internet connection.) AstroTour Atomic Energy Levels and Light Emission and Absorption Click here to launch this AstroTour (Requires an active Internet connection.) 32

AstroTour H-R Diagram Click here to launch this AstroTour (Requires an active Internet connection.) 33