features of the suns Flashcards

1
Q

The James Webb Space Telescope

A

(JWST)
observ es at infrared wav elengths

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2
Q

how many earths could fit inside the sun

A

About one million Earths could f it inside the Sun

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3
Q

The Sun

A

A large sphere of hot, dense,
mostly ionized gas (plasma),
bound together by grav ity.
Energy is produced in the Sun’s
core and makes its way to the
surf ace.

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4
Q

The Sun consists of dense gas

A

by mass: 70% H, 28% He, 2% other
(90% of all the atoms are Hydrogen)
* Density = Mass / Volume
* Average Density of the Sun = 1.4 g/cm3
(density of water is 1.0 g/cm 3

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5
Q

Most common elements in the Sun

A

H 90%
He 8.7%
O 0.08%
C 0.04%
N 0.01%
Si 0.004%
Mg 0.004%
Ne 0.004%
Fe 0.003%
S 0.002%

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6
Q

The Solar Atmosphere: Photosphere

A

visible surface of the Sun
* Temperature 5700K
* Density 10−9 kg/liter
* 400 km thick

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7
Q

tops of the cells on the Sun’s ‘surface’ (photosphere

A

graunualtion

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8
Q

The photosphere of the Sun is

A

an apparent surface: you would notice little change as you
go through it, like flying through a cloud

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9
Q

Sunspots are dark because

A

they are cooler (4000K
v s. 6000K) than the regions around them

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10
Q

The Sun rotates once

A

every 4 weeks
Differential rotation:
* 26 days at the equator
* 38 days at the poles

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11
Q

Sun’s Magnetic Field

A

produced by the flow of plasma in the interior

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12
Q

Sunspots occur when the

A

when the Sun’s
magnetic field bursts through the surface
* Magnetic field
lines prevent
hotter plasma
from rising into
the sunspot
* Sunspots come
in pairs, with
opposite
polarities

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13
Q

Sunspots vary in an

A

an 11-year sunspot cycle

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14
Q

The number of sunspots and solar activity in general peaks

A

every 11 years

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15
Q

The Solar Atmosphere: Chromosphere

A

lay er abov e the photosphere
* T ~ 15,000 K.
* 1,000 km thick

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16
Q

spicules

A

magnetic jets and loops

17
Q

The Solar Atmosphere: Corona

A

Outermost lay er,
v ery thin but hot,
T > 1 million K
* Visible during
a total
solar eclipse

18
Q

The corona is much hotter than layers below i

A

The Sun’s magnetic f ield acts like a pump
that accelerates the particles in the corona.

19
Q

Very hot gas can be seen in

A

x-rays

20
Q

Solar prominences

A

are created by plasma looping along
magnetic f ield lines

21
Q

Solar Flares

A

Two prominences short
out, releasing huge burst
of energy (million H
bombs)

22
Q

Solar Wind

A

The solar wind (charged particles) escapes
through coronal holes, seen in X-ray images.
The Sun is ev aporating! (but very slowly)

23
Q

solar wind what it is

A

electrons and
protons streaming away
f rom the corona

24
Q

Earth’s magnetic f ield
def lects

A

most of the solar
wind around the Earth,
collects the rest in the
Van Allen belts.

25
Q

Coronal Mass Ejection

A

Coronal Mass Ejection
A solar flare or coronal mass ejection (CME)
can trigger the aurora borealis

26
Q

Aurora

A

When the low-density gas
of the upper atmosphere is
heated, it emits an
emission-line spectrum.
Aurora Borealis