Astro 7 Unit 3 Review Flashcards

1
Q

How do LOW mass stars live their lives?

A

longest lifetime (billions, trillions of years), fusion creates low mass elements, remnant is roughly earth sized

our sun is a low mass star

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2
Q

How do INTERMEDIATE mass stars live their lives?

A

tens - hundreds of millions of years lifetime, fusion creates elements between low and high mass, remnant is size of a large city, a few times bigger than our sun

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3
Q

How do HIGH mass stars live their lives?

A

couple million year life, fusion creates elements up to iron, remnant is immensely small hole, 30-40 times mass of sun

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4
Q

What is the end state of a LOW mass star?

A

becomes planetary nebulae, leaves behind a white dwarf

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5
Q

What is the end state of a INTERMEDIATE mass star?

A

becomes a type 2 supernova, leaves behind a neutron star

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6
Q

What is the end state of a HIGH mass star?

A

becomes type 2 supernova, leaves behind a black hole

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7
Q

What is the H-R Diagram and how is it used?

A

Horizontal Axis: left to right is hottest to coldest. spectral class is o - b - a - f - g - k - m which is determined using absorption lines

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8
Q

What is the main sequence?

A

main-sequence stars located on H-R diagram in a band from lower right across to upper left — around the slightly-wavy red line in the example H-R Diagram

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9
Q

How are different properties of stars related to stars on the main sequence?

A

when on the main-sequence stars are burning Hydrogen into Helium in their cores, higher temp = higher luminosity, more massive stars burn out faster

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10
Q

How are extrasolar planets detected?

A

found using ‘transit’ method, the brightness of the star decreases regularly due to the planet passing right in front of it

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11
Q

How does the habitable zone change depending on the mass of a star?

A

a less-massive star would have habitable zone closer to the star and a more-massive star would have habitable zone farther from the star

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12
Q

What is a habitable zone?

A

region around a star where liquid water could be present on a planet’s surface

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13
Q

What are black holes?

A

the end state of the highest-mass stars, left behind after supernova explosion, gravity is so great light cannot escape, infinite density and infinitely small

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14
Q

What is a type 2 supernova?

A

a violent explosion with the star’s core left behind

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15
Q

What is a neuron star?

A

if the remaining core is about 1.4 – 3 solar masses, about city sized

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16
Q

What types of stars are not on the main sequence?

A

red giants and super giants (most luminous) white dwarfs

17
Q

Nuclear Fusion

A

a long-lasting source of energy 4 protons combine to make helium-4 (2 protons and 2 neutrons) and release energy in gamma rays

18
Q

The Sun

A

mostly gas, hydrogen (73 %, by mass) and helium (25 %, by mass), 99.9% of all mass in solar system is sun

19
Q

Possibly layers of the sun?

A
20
Q

Parralax method

A

D = 1/p

ex: a star with measured parallax angle of 0.1 arcsec is 1 / 0.1 = 10 parsecs away
ex: a star with a parallax angle of 0.02 arcsec is 1 / 0.02 = 50 parsecs away

21
Q

Look at HR Diagram

A
22
Q

Drake equation - maybe the variables and their meaning?

A