Chapter 2 Flashcards

1
Q

Nubula

A

A slowly rotating and collapsing cloud of susy and light gases.

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2
Q

Accretion Process

A

Collect and stick together gradually,
Grains
Bolders
Planetesimals
Planet

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3
Q

Sun mass

A

The sun comprises 99.8 of the mass of the entire solar system.

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4
Q

Inner/Terrestrial Planets

A

Small, dense, rocky, and rich in metals.
Ex: Mercury, Venus, Earth, and Mars

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5
Q

Outer/Jovian Planets

A

Large, low density, gas, and ice giants.
Sun swept volatile gases to cooler out disk.
Ex: Jupiter, Saturn, Uranus, and Neptune

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6
Q

What makes a planet?

A

Orbits sun
Spherical
Clears material in its orbit

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7
Q

Why Pluto is not a planet.

A

Pluto still has lots of asteroids and other space rocks along its flight path, rather than having absorbed them over time, like the larger planets have done.

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8
Q

Source of energy of the Sun comes from?

A

H atoms fuses with other H atoms - He
Multiple fusion reactions releasing energy.

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9
Q

High temperatures of the sun comes from?

A

Electrically-charged gas and particles
Moving particles create a magnetic field.

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10
Q

Dark spots on Sun’s surface

A

Increased in solar radiation caused by magnetic storms due to interaction of the suns surface and magnetic field.

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11
Q

Solar Flairs

A

Magnetic field lines near sunspots often tangle.

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12
Q

Solar Flairs can…

A

Affect radio communications.
Explosions of hot energy and gases.

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13
Q

Solar Wind

A

Charged particles from the sun.

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14
Q

Solar Wind facts…

A

H nuclei and free electrons
From outer atmosphere of sun (corona)
Three days to reach earth
Examined this experiment using foil.

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15
Q

Earths Magnetosphere

A

2 magnetic metals move over one another to create a magnetic field.

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16
Q

How Earths Magnetosphere works.

A

Flow of the outer core around the inner core creates this field.

17
Q

The Earths Magnetosphere protects….

A

Us from radiation poisoning.

18
Q

Aurora Borealis

A

Interaction of our atmosphere with solar wind.

19
Q

Electromagnetic Spectrum

A

Energy comes in different wavelengths and frequencies.

20
Q

Sun and Earths wavelengths.

A

Sun radiates shortwave energy.
Earth radiates long wave energy.

21
Q

Insolation

A

The total amount of solar radiation energy received on a given surface area during a given time.

22
Q

Tropic insolation

A

Receive more concentrated insolation due to Earth’s curvature.

23
Q

Seasonality

A

Refers to seasonal variations of suns position above horizon and changing day length during the year.

24
Q

Day length

A

Affected by the suns max altitude, which depends on,
The time of year
Latitude

Equator vs. Arctic

25
Q

Suns altitude

A

Angle above horizon.

26
Q

Altitude

A

The angel from Earths surface to the line connecting to you and the sun.

27
Q

Declination

A

Latitude that receives overhead insolation (subsolar point: sun directly above Earth).

28
Q

5 reasons for seasons

A

Revolution
Rotation
Tilt of Earths axis
Axial parallelism
Sphericity

29
Q

Revolution

A

Earth revolves around the sun for a year.
Voyage takes one year.

30
Q

Rotation

A

Earth rotates on axis once every 24 hours.

31
Q

Axial Parallelism

A

Earths tilt.
Axis maintains alignment during orbit around the sun.
North pole points toward the North Star (Polaris)

32
Q

Sphericity

A

Earth is an oblate spheroid.

33
Q

Energy Budget

A

Radiant energy that reaches Earth from the sun and flows from Earth back out to space.

34
Q

Fusion

A

Two light nuclei merge to form a heavier nucleus.
The process releases energy.
The leftover mass becomes energy.

35
Q

Nebular theory

A

The solar system developed from a nebula.

36
Q

Sunspot

A

Magnetic field is 2,500 times stronger than Earth’s.