The Sun (Earth, Moon and Sun) Flashcards

1
Q

What is it from Earth to the sun?

A

150 million km or 1 Astronomical unit.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What is the diameter of the Sun?

A

1.4 million km just over 100x diameter of the Earth.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

What gases make up the sun and how much?

A

Hydrogen (75%)

Helium (25%)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Why is the sun so important?

A

Provides all the heat, light and energy requirements for life on Earth.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What is the visible surface of the sun called?

A

The photosphere

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What is the temperature of the visible surface of the sun?

A

The photosphere’s temp is 5800K

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What the the relatively thin ‘sphere of colour’ above the photosphere?

A

The chromosphere

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

What is the extensive outline which is the glowing region of ionised gas making up the Sun’s atmosphere?

A

The corona

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

What is the thickness of the chromosphere?

A

2000km

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Why is the chromosphere not normally visible?

A

The light from the photosphere is too dominant. However it can be seen as a slender pink ring just before totality is reached during a solar eclipse.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

What is the temperature of the corona?

A

2 million K which is hot enough to emit X-rays.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

What is nuclear fusion?

A

The reactions that happen in the central core of the sun and is the sun’s source of energy. The heat of the core allows hydrogen nuclei (protons) to fuse to make helium nuclei in a series of reactions called the proton-proton chain.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

What is the temperature of the sun’s core?

A

15 million K

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

How many tonnes of of matter is lost each second by the sun?

A

4 million tonnes.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

What is the total mass of the sun in tonnes?

A

2.0 x 10(to the power of)27

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

What are sunspots?

A

Cooler areas of the photosphere that correspond to strong localised magnetic fields.

17
Q

How big are sunspots?

A

About the size of the earth.

18
Q

What is an umbra?

A

A central darker region, about 2000K cooler than the photosphere

19
Q

What is a penumbra?

A

A lighter (i.e. Less dark than umbra) surrounding area, with a temperature about 200K cooler than the photosphere.

20
Q

How does the sun rotate?

A

The sun does not rotate as a solid body. It’s rotation periods varies from 25 days at its equator to 36 days at its poles.

21
Q

How long is the solar cycle?

A

The regular pattern of 11 years for sunspots. During which number of sunspots increases to a maximum before falling again.

22
Q

What is a Butterfly diagram?

A

The chart which shows the general pattern of the positions of sunspots.

23
Q

What is the Maunder Minimum?

A

The period between the years of 1645 and 1715 when the sun was relatively inactive and very few sunspots were observed. This corresponds with a period of extremely cold winters in Europe.

24
Q

How can you find the rotation period of the sun?

A

You observe a group of sunspots, recording their position and timing how many days later the spots return to the same position. This would be the time of one rotation.

25
Q

What is the solar wind?

A

This is a steady stream of charged particles (mainly protons and electrons, but with trace of ions of helium and other elements) flowing outwards in all directions from the sun’s corona at speeds of typically 400km/s.

26
Q

What are coronal holes?

A

Cooler regions of the corona close to the sun’s magnetic poles where open magnetic field lines escape more easily at speeds as fast as 850 km/s. This is where fast solar wind is thought to have originated from.

27
Q

What are prominences?

A

Huge clouds of cooler gas in the Sun’s atmosphere.

28
Q

What are filaments?

A

Huge clouds of cooler gas in the Sun’s atmosphere that appear as dark silhouettes against the brighter photosphere.

29
Q

What are solar flares?

A

Sudden releases of energy

30
Q

What is a transit?

A

When a planet travels in front of the sun and it looked like a dark shadow.

31
Q

What type of radiation is emitted from exceptionally hot regions of the sun?

A

X-rays.