Chapter 13 Flashcards

1
Q

What is the fundamental method of measuring the distance of nearby stars

A

Triangulation

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2
Q

How do we find the distance using triangulation

A

We use parallax. We see the location of a star in January for example and then it’s location in July and draw a triangle using earth and that star

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3
Q

What is the nearest star to the sun

A

The Proxima Centauri which is a member of a 3 star system called alpha centauri

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4
Q

What is luminosity

A

It is the absolute brightness of a star, and the measure of the total amount of energy radiated by a star each second

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5
Q

What is apparent brightness

A

It is how bright the star appears to be from earth, this depends on its luminosity and the distance of the star

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6
Q

What does a high magnitude mean in luminosity of a star

A

It means the star is dim, the higher the magnitude the dimmer it is and the lower the magnitude the brighter it is

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7
Q

What is absolute magnitude used for

A

Measuring a stars luminosity. It is the apparent magnitude the same star would have at 10 parsecs distance

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8
Q

What does a stars color mean

A

How hot it is, reds are relatively cool while blue ones are hotter

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9
Q

How do we measure their heat

A

Since they are black bodies, we only need to make observations of two wavelengths coming from them to determine their heat

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10
Q

What is a stars spectrum

A

It is how the energy it emits at each wavelength is shown. It can show a stars composition, temperature, luminosity, velocity, and rotation speed

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11
Q

How are star temperatures categorized

A

By letters going from highest to lowest; O B A F G K M, each type has 10 subdivisions from 0-9 the lower the number the hotter the star

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12
Q

Who demonstrated the physical connection between temperature and absorption lines

A

Cecelia Payne

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13
Q

How do we measure a stars motion

A

From the Doppler shift of its spectral lines

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14
Q

What does Steven Boltzmann’s law state

A

The hotter the star the greater it’s luminosity

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15
Q

How do stars differ in radius (dwarf stars, giant stars, supergiant stars)

A

Dwarf stars: equal to or less than the sun
Giant stars: between 10 and 100 times the sun
Supergiant stars: more than 100 times the sun

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16
Q

What is the hertzsprung-Russell diagram

A

It plots stellar luminosity against surface temperature

17
Q

What is the dark curve called on the plot

A

It is called the main sequence

18
Q

Where do 90% of stars lie

A

In the main sequence

19
Q

What are the three classifications of stars in the HR diagram

A

Main sequence, giants, white dwarfs

20
Q

How do astronomers measure distances in the universe

A

They use the method of standard candles also called the spectroscopic parallax

21
Q

What are binary stars

A

They are two stars that revolve around each other as a result of their mutual gravitational attraction

22
Q

How do we detect if a star is a binary pair

A

Many stars are, we can detect it by visual binaries, Doppler shift, or eclipsing binaries

23
Q

What does mass determine on the HR plot

A

Where it lies on the main sequence.

24
Q

Can the masses of stars in the binary sequence be measured

A

Yes