Lecture 3 Flashcards

1
Q

1 AU (Astronomical Unit)

A

~150 million km

Distance between Sun and Earth

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2
Q

1 lyr (light year)

A

~10 trillion km

Distance light can travel in 1 year

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3
Q

Radar ranging

A

Bounce radio waves of other planets and measure the distance

Good for planets in solar system

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4
Q

Parallax

A

Uses hypotenuse

Good for nearby stars

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5
Q

Main-sequence fitting

A

Uses inverse square law

For things within milky way

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6
Q

Cephedes

A

So bright that they can be seen from other galaxies

Distance to nearby galaxies

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7
Q

Distant standards

A

Used supernova stars that explode to find galaxies

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8
Q

How many arcminutes in a degree?

A

60

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9
Q

Red-shift of galaxies

A

Uses Dopler Effect

Blue-shifter: Getting closer
Red-shifter: Going away

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10
Q

Hubble’s Law

v = H x D

A

Speed of galaxy’s recession is proportional to distance

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11
Q

What is the age of the Universe?

A

T = 1/H = 1/(13.7x10^9 yr)

or 4x10^17 secs

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12
Q

Big Bang nucleo-synthesis

A

1 sec after Big Bang, temp dropped to 10 billion K. Universe wad filled with electrons, protons, neutrons and photons but it was too hot to make atoms.
As it cooled, protons and neutrons fused to make light elements.
After 3 mins, too cold to make more fusion rxns.

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13
Q

What elements were created right after the Big Bang?

A

Hydrogen
Helium
Lithium
Beryllium

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14
Q

What produced heavy elements?

A

Stars

Hot enough for more fusion

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15
Q

What are the terrestrial planets?

A

Mercury
Venus
Earth
Mars

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16
Q

What are the giant planets?

A

Jupiter
Saturn
Uranus
Neptune

17
Q

How does a solar system form?

A

Gas-cloud collapses and forms a disk, spinning faster.

Central gas ball becomes dense and hot enough to start hydrogen fusion and create the Sun.

18
Q

Planetismals

A

Solid, forms very quickly (few Myr)

19
Q

Theory for moon formation

A

Planetismal crashed into young Earth.

Earth spins fast and becomes molten. A part of the crust broke off to form the moon.

20
Q

Hot Jupiters

A

Jupiter-like planet found close to the sun.

May have formed far out but orbital migration pulled it closer as it grew.

21
Q

2 theories of planet formation

A
  1. Slow - Grow by collisions and accretion

2. Fast - Spiral instability where proto-planet forms

22
Q

Igneous rock

A

Molten rock which solidifies

Types:
Basalt - Dense, iron and magnesium
Granite - Lighter, silicate admixtures

23
Q

Metamorphic rock

A

Existing rock formed by high pressure and heat

24
Q

Sedimentary

A

Gradual compression of sediments

Good for fossils

25
Q

Radiometric dating

A

Radioactivity decreases in deeper layers because of half-life
(e.g. All expected carbon at the top layer have decayed or turned into a different element in a deep layer)

26
Q

Age of sun and earth

A

Sun: 4.57 Gyr
Earth: 3.9-4.0 Gyr

27
Q

Eons

A

Hadean
Archean
Proterozoic
Phanerozoic

28
Q

Era

A

Subdivision of eon

29
Q

Periods and epochs

A

Subdivisions of era