Announcements

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Announcements • Exam Grades Wednesday March 31 • Angel Grade update Friday April 2 • Star Assignment 6, due Wednesday March 31 Do Angel quiz,

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Announcements. Exam Grades Wednesday March 31 Angel Grade update Friday April 2 Star Assignment 6, due Wednesday March 31 Do Angel quiz,. Objectives. Plot an Hertzsprung-Russell Diagram Locate the regions of giant, main sequence and white dwarf stars. - PowerPoint PPT Presentation

Transcript of Announcements

Page 1: Announcements

Announcements• Exam Grades Wednesday March 31• Angel Grade update Friday April 2• Star Assignment 6,

due Wednesday March 31Do Angel quiz,

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Objectives

• Plot an Hertzsprung-Russell Diagram• Locate the regions of giant, main

sequence and white dwarf stars. • Describe the relations between

surface temperature, luminosity, mass and size for these types of stars.

• Describe the evolutionary state of the 16 brightest northern-hemisphere stars.

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What should we do with our information?

• Luminosities

• Surface Temperatures

• Masses

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Number of Stars vs Luminosity

LOWHIGH Luminosity1100 0.01 0.0001

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Stellar Masses

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What should we do with our information?

• Luminosities

• Surface Temperatures

• Masses

Look for Relationships

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No Relationship

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Luminosity - Mass Relation

L~M3.5

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HRDiagram:Luminosity

vs.Surface

Temperature

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Luminosity - Temperature

Relation: Hertzsprung-

Russell DiagramL

umin

osit

y ->

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Temperature

Lu

min

osi

tyRecall:

Hotter -> BrighterHotter ->

BluerBigger -> Brighter

Then cool+

Luminous-> Large

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Temperature

Lu

min

osi

tyRecall:

Hotter -> BrighterHotter ->

BluerBigger -> Brighter

Then small Luminosity

+ Hot -> small

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Stellar Size, Mass

& HR

Diagram

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Stars with low temperature and high luminosity must have large radius

Large radius

Small radius

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Stars with low temperature and high luminosity must have large radius

GIANTS

SUPERGIANTS

WHITEDWARFS

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Low-Mass Stars

High-Mass Stars Most Low Mass stars have

SmallLuminosity

Most Large Massstars have

LargeLuminosity

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Regions of the H-R Diagram

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Activity

• Answer the questions on your scantron sheet

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Temperature

Lu

min

osi

ty

1. Which star is the hottest?

A

BC

D

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Temperature

Lu

min

osi

ty

1. Which star is the hottest?

A

BC

AD

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Temperature

Lu

min

osi

ty

2. Which star is the most luminous?

A

BC

D

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Temperature

Lu

min

osi

ty

2. Which star is the most luminous?

A

BC

D C

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Temperature

Lu

min

osi

ty

3. Which star is a main-sequence star?

A

BC

D

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Temperature

Lu

min

osi

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3. Which star is a main-sequence star?

A

BC

D

D

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Temperature

Lu

min

osi

ty

4. Which star has the largest radius?

A

BC

D

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Temperature

Lu

min

osi

ty

4. Which star has the largest radius?

A

BC

DC

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Temperature

Lu

min

osi

ty

5. Which star is most like our Sun?

A

B

C

D

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Temperature

Lu

min

osi

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5. Which star is most like our Sun?

A

B

C

D

B

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HOT COOL

BRIGHT

FAINT

HRDiagram

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Astronomy Place Questions

6. Spica is a Main Sequence star, having a surface temperature of 26,000K. In order for a star with a surface temperature of only 6,000K to have the same Luminosity as Spica, its radius must be?

Luminosity = 4R2T4

If T ~ 4 x smaller, then R ~ 42 x larger = 16x

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7. The rate of fusion (number of He nuclei produced per second) in the core of the star Vega (a main-sequence star with a temperature of about 10,000K is roughly?

Lvega = 60 Lsun, so rate of energy generation

= rate of energy loss is 60 x larger than Sun’s

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8. A star having the same radius as the Sun, but a surface temperature 5 times higher than the Sun, would have a luminosity?

L ~ T4

54 = 625

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9. A main-sequence star that is twice as massive as the Sun will have a Luminosity?

L ~ M3. 5

23 = 8, 24 = 16, so 23.5 in between

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Lifetime on the Main Sequence

How long will it be before MS stars run out of fuel? i.e. Hydrogen?

How much fuel is there? M

How fast is it consumed? L M3.5

How long before it is used up?

M/L = M/M3.5 = M-2.5

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Main SequenceLifetimes

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Lifetime on the Main Sequence

• O & B Dwarfs burn fuel like a bus!

• M Dwarfs burn fuel like a compact car!

• Our Sun will last 1010 years on the Main Sequence

• MS Lifetime = 1010 yrs / M2.5

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Stars occur alone

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or in clusters

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another type of cluster

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Star Clusters

• Stars approximately the SAME AGE

• Stars approximately the SAME DISTANCE

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Cluster HR

Diagrams

Same DistanceSame Age

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Pleiades now has no stars with life expectancy less than around 100 million years

Main-sequenceturnoff

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Detailed modeling of the oldest globular clusters reveals that they are about 13 billion years old

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ClusterAges

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Activity

• Answer the questions on your scantron sheet

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Temperature

Lu

min

osi

ty

6. Which of these stars will have changed the least 10 billion years from now?

A

B

C

D

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Temperature

Lu

min

osi

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6. Which of these stars will have changed the least 10 billion years from now?

A

B

C

D

C

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Temperature

Lu

min

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7. Which of these stars can be no more than 10 million years old?

A

B

C

D

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Temperature

Lu

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7. Which of these stars can be no more than 10 million years old?

A

B

C

D

A

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A stars properties depend mostly on

1. Mass2. Age

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NEXT TIME

• Evolution of Stars

• READ chapter 17