Chapter 12 Terms Flashcards

1
Q

Chromosphere

A

is the lower part of the Sun’s outer atmosphere that lies directly above the Sun’s visible surface

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2
Q

Convection Zone

A

is the region immediately below the Sun’s visible surface in which its heat is carried by convection

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3
Q

Corona

A

is the outer, hottest part of the Sun’s atmosphere

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4
Q

Coronal Hole

A

is a low-density region in the Sun’s corona

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5
Q

Cosmic Rays

A

are extremely energetic particles traveling at nearly the speed of light

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6
Q

Granulation

A

is the texture seen in the Sun’s photosphere

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7
Q

Hydrostatic Equilibrium

A

is the condition in which pressure and gravitational forces in a star or planet are in balance

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8
Q

Maunder Minimum

A

is the time period from about A.D. 1600 to 1740, during which the Sun was relatively inactive

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9
Q

Neutrino

A

are tiny neutral particles with little or no mass and immense penetrating power.
Nuclear Fusion is the binding of two light nuclei to form a heavier nucleus, with some nuclear mass converted to energy

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10
Q

Perfect Gas Law or Ideal Gas

A

is a law relating the pressure, density, and temperature of a gas

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11
Q

Photosphere

A

is the visible surface of the Sun

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12
Q

Pressure

A

is the force exerted by a substance such as gas on an area divided by that area

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13
Q

Prominences

A

is a cloud of hot gas in the Sun’s outer atmosphere

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14
Q

Proton-Proton Chain

A

is the nuclear fusion process that converts hydrogen into helium in stars like the Sun and thereby generates their energy

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15
Q

Radiate Zone

A

is the region inside a star where its energy is carried outward by radiation

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16
Q

Solar Cycle

A

is the cyclic change in solar activity

17
Q

Solar Flare

A

is a sudden increase in brightness of a small region on the Sun

18
Q

Solar Wind

A

is the outflow of low-density hot gas from the Sun’s upper atmosphere

19
Q

Spicule

A

is a hot, thin column of gas in the Sun’s chromosphere

20
Q

Strong Force

A

is the force that holds protons and neutrons together

21
Q

Sunspot

A

is a dark, cooler region on the Sun’s visible surface created by intense magnetic fields

22
Q

Zeeman Effect

A

is the splitting of a single spectrum line into two or three lines by a magnetic field