Starshine Flashcards

Understand stellar properties

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1
Q

Name the various groups that stars are classified into.

A

Grouped based on stellar properties, they are red giants, white dwarfs and blue supergiants.

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2
Q

What is the only information we have from stars at enormous distances away from Earth?

A

The electromagnetic radiation we receive from them.

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3
Q

What can the EM emissions from stars tell us?

A

Temperature, chemical composition, speed of movement, approximate age, size and much more.

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4
Q

What does stellar mean?

A

“relating to a star”

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5
Q

What precise measure is used by astronomers to classify the brightness of stars?

A

Luminosity, it is defined as the rate at which energy of all types is radiated by an object in all directions.

This depends upon both it’s size and temperature.

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6
Q

What is a black body?

A

A perfect radiator, that will give off energy across the entire electromagnetic spectrum (a large range of wavelengths).

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7
Q

What is the “Stefan-Boltzman law?”

A

This tells us that the power output from a black body is proportional to its surface area and the fourth power of its temperature in Kelvin

L=(sigma)AT^4

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8
Q

What is a star’s spectrum?

A

The range of wavelengths of light given off by a star.

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9
Q

What is Wien’s law?

A

(lamda max)T=2.898*10^-3

Where lamda max is the peak wavelength at which the energy output is most. It’s evident from the SB law, that as the temperature of a black body increases, so does the energy emitted.

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10
Q

What can the temperature of a star tell us?

A

It determines the spectral output of the star, but it can also suggest chemical composition and age.

Because of this astronomers have classified stars into groups according to their temperature.

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11
Q

How are the spectral star classes labelled?

A

By letters, (O)h (B)e (A) (F)ine (G)irl, (K)iss (M)e.

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12
Q

What are the trends in hotter stars?

A

They tend to have more mass and are more luminous.

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13
Q

What happens due to the large gravitational pressure at the center of a massive star?

A

The nuclear fusion reactions within the star run very fast, producing a lot of energy and using the hydrogen fuel in the star at an incredible rate.

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14
Q

What are the characteristics of massive stars?

A

They are larger, and at high temperatures, the hotter stars are very luminous, giving off a great deal of energy.

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15
Q

What class of stars do blue supergiants belong to?

A

O class

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16
Q

What class of stars do red dwarf stars belong to?

A

M class

17
Q

What trend is seen in a graph plotted with luminosity against star temperature?

A

A general negative correlation, but when more data is added, the picture gets more complex.

18
Q

Why is it called a Hertzsprung- Russel diagram and not a graph?

A

The temperature measurements assume the star behaves as a black body.

Luminosity is not so accurate, because luminosity is a calculation that includes distance to the star, which is not so accurate.

19
Q

What is the ‘main sequence,’ in an H-R diagram?

A

The diagonal line across which most stars we observe fall. These stars exist in this state for the majority of their lifetime. They are stable stars.

20
Q

What are the main underlying features of the H-R diagram?

A

The plot is drawn with hotter temperatures on the left hand side.

There are places on the diagram which show other stages of a star’s evolution.

The top left area of the diagram is lightly populated.

21
Q

Why do we see such few blue supergiants in the H-R diagram?

A

Because they burn out in a few million years and most of them have already done so.