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You have an article to read after your You have an article to read after your

You have an article to read after your - PowerPoint Presentation

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Uploaded On 2017-04-11

You have an article to read after your - PPT Presentation

bellwork You have 9 minutes to do both Please read and answer the 3 following questions What is luminosity Where does our Sun rank among stars How are color and brightness ID: 536191

star magnitude object stars magnitude star stars object apparent brightness 000 system knowledge dimmer measure blue red brighter learning

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Slide1

You have an article to read after your bellwork. You have 9 minutes to do both.

Please

read

and

answer

the 3 following questions:

What is luminosity?

Where does our Sun rank among stars?

How are

color

and

brightness

related?

(think about it)Slide2

Learning Goals:How do stars differ from moons and planets, and from one another?How does the classification of stars help us understand how they evolve over their lifetimes?What are the different types of stars?

What happens when different types of stars die?

Why is it important for us to understand stars?

4.

Complex Knowledge

: demonstrations of learning that go

aboveand

above and beyond what was explicitly taught.

3.

Knowledge

: meeting the learning goals and expectations.

2.

Foundational knowledge

: simpler procedures, isolated details, vocabulary.

1.

Limited knowledge

: know very little details but working toward a higher level

.Slide3

No more late work from last week. It’s been more than 5 daysYou have already taken the testSorry, but welcome to growing up.Slide4

What main characteristic of stars are the “spectral classes” (O, B, A, F, G, K, M) based on?Slide5

Star sizes and colors

Are stars all the same size and color? Slide6

What is different about how these stars are drawn?What do you think that stands for?Slide7

Stellar Magnitude: Questions of the dayHow do we measure a star’s brightness? What characteristics about a star must we know to do this?

Inverse square law:

The amount of light an object receives from a source decreases by the square of the distance between the object and the source.Slide8

You’ve seen this before…Slide9

What happens to light as you recede from a star?Slide10

The Magnitude System - historicalSystem was originally devised by Hipparchus

(Greek Astronomer, 150 BC)

Brightest=1

Next brightest=2

Dimmest =6

(you can’t see anything dimmer than 6 with your naked eye)Slide11

The Magnitude System -currentWith the invention of the telescope and other observational aids the number of new objects soared and a modification was needed to the system in order to accurately categorize so many new objects. Slide12

The Magnitude System -currentIn 1856 Norman Robert Pogson formalized the magnitude scale by defining:a sixth magnitude object is an object that is 100 times dimmer than a first magnitude object

An eleventh magnitude object is 100 times dimmer than

a

sixth magnitude object and 10,000 times dimmer than a first

The scale is logarithmic, not linear

Vega is point zero.Slide13

Which star is going to seem brighter? A red star with a magnitude of 1 or a blue star with a magnitude of 4?Slide14

Which star is hotter? A red star with a magnitude of 1 or a blue star with a magnitude of 4?Slide15

Which star is bigger? A red star with a magnitude of 1 or a blue star with a magnitude of 4?Slide16

Apparent vs. AbsoluteApparent magnitude is dependent on 2 factors:

The

luminosity

of the star (

total energy per second radiated

)

The

distance

of the star from Earth

It is the

brightness of an object as perceived from earth. Slide17

Absolute magnitude is the measure of a celestial object's actual brightness.

Apparent vs.

AbsoluteSlide18
Slide19
Slide20

How do we measure this?

LOWER numbers are BRIGHTER than higher numbers!!!Slide21

*Hubble’s Sight: 30 (J.W.S.T.: 34) *Human Sight:6 *ISS: -5.9 *

Sirius: −1.46

*Venus: -4.89

*

Full Moon: -12.62

star

Distance (

ly

)

Apparent

magnitude

Absolute magnitude

Sun

.00001581

-26.72

4.8

Sirius

8.6

-1.46

1.4

Aldebaran

60

.85

-.3

Vega

25

.03

.6

Procyon

11.4

.38

2.6

Rigel

1400

.12

-8.1

Betelgeuse

1500

.5

-7.2Slide22

Visible to

typical

human eye

Apparent

magnitude

Brightness

relative

to Vega

Number of stars

brighter than

apparent magnitude

Yes

−1

250%

1

0

100%

4

1

40%

15

2

16%

48

3

6.3%

171

4

2.5%

513

5

1.0%

1 602

6

0.40%

4 800

No

7

0.16%

14 000

8

0.063%

42 000

9

0.025%

121 000

10

0.010%

340 000Slide23

Answer the questions of the dayHow do we measure a star’s brightness? What characteristics about a star must we know to do this?Slide24

Listen for and write down 2 things that he mentions that you did not know at the beginning of this class and 1 thing you did.https://www.youtube.com/watch?v=9P8Veb_AlJ0Slide25

Last Thing Google ClassroomDue Tomorrow!