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Flashcards in Chapter 2 Deck (31)
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1
Q

Number of galaxies in the universe

A

125

2
Q

Our galaxy

A

Milky way

3
Q

Location of our solar system

A

on the trailing edge of the milky way

4
Q

Light years in diameter?

A

100,000

5
Q

We are ______ light years from the center

A

30,000

6
Q

Milky Way

A

flattened disk shaped collection of stars, barrel shaped

7
Q

Whats at the very center of the milky way galaxy?

A

a black hole

8
Q

Formation of the solar system

A
  1. large rotating cloud of gas and dust
  2. nebula cloud flattened into a disk shape
  3. gravity pulled matter proportional to its mass together, forming a protosun
  4. the proto sun grew in mass, drawing more mass to it
  5. meanwhile, material accreted together creating protoplanets, which in turn drew more mass towards them to create planets
9
Q

Gravity

A

mutual force exerted by the mass of objects that are attracted one another and produced in an amount proportional to each object’s mass

10
Q

Planetesmal hypothesis

A

suggests a process by which early protoplanets formed from the condensing masses of a nebular cloud of dust, gas and icy comets

11
Q

Moons in our solar system

A

165 (around 6 planets)

12
Q

Planets in our solar system

A

8

13
Q

Speed of light

A

300,000 km per second

14
Q

How long does it take for light to travel the diameter of our solar system?

A

11 hours

15
Q

Earth orbits around the sun in a _______ (_____) path

A

elliptical (oval) path

16
Q

Perihelion

A

when the Sun and Earth are closest in distance (January 3)

17
Q

Aphelion

A

when Sun and Earth are farthest apart (July 4 )

18
Q

Plane of the Ecliptic

A

a plane touching all points of Earth’s orbit

19
Q

Cause of sun spots

A

Visible surface disturbances on the sun caused by magnetic storms

20
Q

What causes the auroras?

A

When solar wind reacts with the magnetosphere and is directed above the poles, where they interact with gases in the ionosphere

21
Q

Magnetosphere

A

Earth’s magnetic force field, which is generated by dynamo-like motions within the planet’s outer core; deflects the solar wind flow toward the upper atmosphere above each pole

22
Q

Aurora

A

Coronal mass ejections ( and solar flares and solar winds) interact with the magnetosphere and gases in the ionosphere to create a light display at the poles

23
Q

Frequency (

A

number of waves passing a fixed point per second

24
Q

Wein’s Displacement Law

A

all objects radiate energy in wavelengths related to their individual surface temperatures (the hotter the object, the more shortwave radiation emitted)

25
Q

Wavelength

A

The distance between two corresponding point on any two successive waves

26
Q

Stefan Boltzman Law

A

Objects that are efficient absorbers or radiation are good emitters too

27
Q

Solar minimum

A

period during which FEW sunspots are visible

28
Q

Solar maximum

A

period during which sunspots are numerous.

29
Q

Sun spot cycle

A

11 years between solar maximums, where magnetic activity (solar flares, CME’s, magnetic storms, prominence flares)

  • most of the flares are pulled back into the sun because of magnetic force, some are released in the form of solar wind
30
Q

Solar Wind

A

Clouds of electrically charged particles?

31
Q

Wavelength unit

A

Micrometers μm

1