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Skylog: Sky Safari

All About Stars

January 10 2010 23:45 UTC | Views: 632 | Comments: 0
Posted by: Kochava in Sky Safari Slideshow

[1]   The Sun - our closest star
Amateur Astronomy Picture of the Day for Oct 30, 2009
image credit: Giancarlo Calzetta (Pilolli)






[2]   Comparison of mass of hydrogen and helium atoms:

   Mass of a hydrogen atom:   1.007825 amu

 

   Mass of 4 hydrogen atoms:  4.0313 amu

 

   Mass of one helium atom:    4.00260 amu

 

   Missing mass:                      0.0287 amu

          (0.71% of the original mass of the 4 hydrogen atoms)



[3]   Comparison of Visual Magnitude and Absolute Magnitude


Star

 

Distance

 

Visual magnitude

 

Absolute magnitude

 

Luminosity

 

Class

 

Spectral

 

class

 

Sun

 

8 light minutes

 

-26.8

 

+4.83

 

V

 

G2

 

Sirius

 

8.6 LY

 

-1.44

 

+1.45

 

V

 

A1

 

Rigel

 

770 LY

 

+0.18

 

-6.69

 

Ia

 

B8

 

Aldebaran

 

65 LY

 

+1.0

 

-0.5

 

III

 

K5

 

Vega

 

25.3 LY

 

+0.03

 

+0.58

 

V

 

A0

 

Altair

 

16.8 LY

 

+0.76

 

+2.20

 

IV

 

A7

 

Deneb

 

3200 LY

 

+1.3

 

-8.7

 

Ia

 

A2

 




[4]    Spectral Class Mnemonics:


  Oven Baked Apples From Grandma’s Kitchen – Mmmm!

 


     “Oh Boy Another F’s Gonna Kill Me.”

 

     “Only Boring Astronomers Find Gratification Knowing Mnemonics!”

 

     “Oh Be A Fine Girl, Kiss Me!”

 

     “Only Boys Accepting Feminism Get Kissed Meaningfully!”



[5]   Spectral Classes and examples:



Spectral

 

class

 

Color

 

Surface Temperature

 

(K)

 

Examples –

 

main sequence

 

Examples –

 

giants

 

O

 

Blue

 

30,000 - 50,000

 

Theta-1C Orionis (in Trapezium, in Orion nebula)

 

Alnitak and Mintaka (in Orion’s belt)

 

B

 

Blue-white

 

10,000 - 30,000

 

Spica, Regulus, brighter Pleiades (Taygeta, Asterope)

 

Rigel, brighter Pleiades (Alcyone,  Electra, Maia)

 

A

 

White

 

7500 - 10,000

 

Vega, Sirius, Altair

 

Deneb

 

F

 

Yellow-white

 

6000 - 7500

 

Procyon

 

Canopus, Mirfak (Alpha Persei), Polaris

 

G

 

Yellow

 

5000 - 6000

 

Sun, Alpha Centauri A

 

Capella

 

K

 

Orange

 

3500 – 5000

 

Alsafi (Sigma Draconis), Keid (Omicron-2 Eridani)

 

Arcturus, Aldebaran

 

M

 

Red

 

2000 – 3500

 

Barnard’s star, Proxima Centauri

 

Betelgeuse, Antares

 




 [6]   The Hertzsprung-Russell Diagram
picture credit:  www.atlasoftheuniverse.com





[7]   Luminosity classes: 

  

 

          

                 Ia, bright supergiant

 

                 Ib, supergiant

 

                 II, bright giant

 

                 III, giant

 

                 IV, subgiant

 

                       V, main sequence or “dwarf”



[8]   Comparison of Spectral Classes
 

Type of Star

 

Spectral

 

class

 

Surface

 

Temp (K)

 

Radius

 

(Sun=1)

 

Mass

 

(Sun=1)

 

Luminosity

 

(Sun=1)

 

Lifetime

 

(millions

 

of years)

 

Abundance

 

Main Sequence

 

O

 

30,000–50,000

 

10

 

50

 

100,000

 

10

 

0.00001%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

B

 

10,000– 30,000

 

5

 

10

 

1000

 

100

 

0.1%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

A

 

7500-10,000

 

1.7

 

2.0

 

20

 

1000

 

0.7%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

F

 

6000-7500

 

1.3

 

1.5

 

4

 

3000

 

2%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

G

 

5000-6000

 

1.0

 

1.0

 

1.0

 

10,000

 

3.5%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

K

 

3500-5000

 

0.8

 

0.7

 

0.2

 

50,000

 

8%

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

M

 

2000-3500

 

0.3

 

0.2

 

0.01

 

200,000

 

80%

 

Giant Stars

 

(low mass stars at the end of their lives)

 

Mostly G, K, or M

 

3000-10,000

 

10-50

 

1-5

 

50-1000

 

1000

 

0.4%

 

Supergiant Stars (high mass stars at the end of their lives)

 

Can be O, B, A, F, G, K, or M

 

4000-40,000

 

30-500

 

10-70

 

30,000-1,000,000

 

10

 

0.0001%

 

White dwarfs (dying remnant

of a star)

 

D

 

Starts at around 100,000 K, then cools down

 

Under 0.01

 

Under 1.4

 

Under 0.01

 

<!--[if !supportEmptyParas]--> <!--[endif]-->

 

5%

 




[9]   The Orion Nebula - A Stellar Nursery

Amateur Astronomy Picture of the Day for Oct 29, 2009
image credit: Ricky Ford





 [10]   Gaseous Jets from Protostars
image credit:  www.hubblesite.org





[11]    Minimum Temperature Required to Ignite Fusion Reaction:

     Fusion of hydrogen to produce helium:                                  1 million K

 

     Fusion of helium to produce carbon, oxygen, and neon:         100 million K

 

     Fusion of carbon to produce sodium and magnesium:           600 million K

 

     Fusion of oxygen to produce silicon, phosphorus, and sulfur: 1 billion K



[12]   Carbon Star Mu Cephei - "Herschel's Garnet Star"

 

(wide field view of nebula IC 1396 - Mu Cephei at top left)
picture credit:  Slooh





[13]   Planetary Nebula M57 - The Ring Nebula
Amateur Astronomy Picture of the Day for Oct 13, 2009
image credit: Tony Farkas





[14]   Supernova Remnant M1 - The Crab Nebula
Amateur Astronomy Picture of the Day for Nov 9, 2009
image credit: Richie Jarvis



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