1.3 The Sun Flashcards

1
Q

How can the sun be observed safely

A

Fitting the objective of a telescope with a h alpha filter or Mylar filter

The safest way is to use an indirect projection method in which a pinhole camera or a telescope focuses an enlarged image of the sun onto a screen which reduces the brightness level so that it is safe

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2
Q

What does 1 AU mean?

A

150 million KM and it’s the distance from Earth to the sun

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3
Q

What’s the Suns diameter?

A

1.4 million km

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4
Q

What’s the temperature of the Suns photosphere

A

5800k

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5
Q

What is the corona?

A

The outside glow of ionised gas - a faint luminous white ring

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6
Q

What temperature is the corona?

A

2 million kelvins

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7
Q

What’s the chromosphere

A

A gaseous layer above the photosphere

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8
Q

How hot is the chromosphere

A

4600k

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9
Q

What’s a sun spot?

A

Cooler areas on the photosphere that correspond to strong localised magnetic fields, these inhibit upward motion of convecting solar material and prevent it from reaching the top of photosphere resulting in lower temperatures

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10
Q

What’s the umbra of a sun spot?

A

A central darker and cool region of a sun spot, about 2000k cooler than photosphere

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11
Q

What’s the penumbra of a sun spot?

A

A less dark surround area of s sun spot with temperature of 200k cooler than photosphere

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12
Q

What’s the Suns rotation period

A

25 days at equator, 36 at the poles

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13
Q

How do we use sunspots to determine Suns rotation period

A

Observing a group of sunspots, recording there position and timing how many days it takes to return to the same position

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14
Q

What’s solar maximum

A

The most active time for sunspots - when there are most sunspots, last 5.5 years where often 100 sunspots visible at s time.

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15
Q

What’s solar minimum!

A

When it’s the calmest and least sunspots last first 5.5 years ones that are visible are short lived

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16
Q

Where do sun spots mainly appear

A

The cycle begins with sunspots 35 to 40 degrees north or south of solar equator, eventually progress to 5-10 degrees of the solar equator

17
Q

How do we predict sunspots?

A

The solar cycle, an 11 year Chloe of the general pattern has been knows as a butterfly diagram which shows us frequency of sun spots

18
Q

How does the sun shine? (What’s thermonuclear fusion)

A

It’s the source of the sun energy, in the core of sun the temperature of 15million k is so hot hydrogen nuclei fuse together to make helium nuclei and in each fusion energy is transferred and converted and radiates to the Suns photosphere where it then radiates outwards into space

E=mc^2

19
Q

What does sun look like at different wavelengths

A

Visible light

H Alpha is a visible spectral line that’s can observe solar prominences and filaments. allows a narrow range of wavelengths either side of 657 nm to pass through

X-Ray’s are emitted form corona and allow us to understand further about Suns temperature

20
Q

How does the sun look at different wave lengths

A

Visible - how we see it

H alpha - plane with crack and a few feature

X Ray - bursting out X Ray’s looks like a fireball

21
Q

What is solar wind and what’s it like/ made of

A

A steady stream of charged particles mainly protons and electrons flowing outwards in all directions from Suns corona at speeds of 400km/s typical

The fast solar wind travels at 850km/s as it is believe to originate from coronal holes (cooler regions of corona) which allow particles to escape more easily

22
Q

What’s the sun made of?

A

Hydrogen 75%

Helium 25%

23
Q

How thick is the chromosphere?

A

2000KM

24
Q

When can you observe the chromosphere

A

Can be observed a slender/ pink ring just before totality is reached during a solar eclipse

25
Q

When can the corona be observed

A

In a solar eclipse the glowing region of ionised gas emits X Ray’s too

26
Q

What’s the temperature of central core of the sun

A

15 million K

27
Q

How fast do the solar winds travel?

A

Typical - 400km/s

Fast- 850km/

28
Q

What’s a solar prominence

A

Huge clouds of cooler gas in the Suns atmosphere

29
Q

What’s a filament

A

Same as prominence but appearing as dark silhouettes against the brighter photosphere

30
Q

What’s a solar flares

A

Sudden releases of energy