CP 15 Surveying the Stars Flashcards

1
Q

what does the brightness of a star depend on

A

distance and luminosity

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2
Q

what is luminocity

A

Amount of power a star
radiates

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3
Q

what is brightness

A

Amount of starlight that
reaches Earth

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4
Q

TF Hotter object = more light = less energy

A

F Hotter object = more light =more energy

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5
Q

what are the hottest and coldest temp of stars

A

Hottest stars= 50,000K
Coolest stars= 3000K

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6
Q

What are the Spectral types that reveal its temperature (abbreviation)

A

Hottest - OBAFGKM - Coolest

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7
Q

TF Most stars arent in binary systems

A

F, About half of all stars are in binary systems

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8
Q

what are the three types of binary star systems

A

Visual
Spectroscopic
Eclipsing

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9
Q

What is a visual binary star system

A

We can directly observe the orbital motions of these stars

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10
Q

what is a spectroscopic binary star system

A

We determine the orbit by measuring Doppler shifts

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11
Q

what is an eclipsing binary star system

A

We can measure periodic eclipses

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12
Q

what is a a hertzsprung-russell (HR) diagram

A

Depicts Temperature
Color
Spectral type
Luminosity
Radius

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13
Q

TF Most stars fall somewhere on the main sequence of the H-R diagram

A

T

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14
Q

What are giant and supergiant stars

A

Stars with lower Temperature and higher Luminosity than main-sequence stars (larger radii)

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15
Q

what are white dwarf stars

A

Stars with higher Temperature and lower Luminosity than main-sequence stars (smaller radii)

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16
Q

Why is there an upper and a lower end to the main sequnce

A

stars bigger than 150M will exlpode
stars smaller than 0.08M cannot sustain fusion

17
Q

Main sequence star summary:

A

High-Mass Star:
* High luminosity
* Short-lived
* Larger radius
* Blue
Low-Mass Star:
* Low luminosity
* Long-lived
* Small radius
* Red

18
Q

what is a variable star

A

Any star that varies significantly in brightness with time

19
Q

Why do the properties of some stars vary

A

Some stars fail to achieve balance between
power generated in the core and power
radiated from the surface