14 matter very cold

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intro to chapter 14, matter very cold, very hot

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kT is about how much energy

particles have at temperature T in

kelvin

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Worked example

• On a nice summer’s day (27 oC) how much energy would the particles have?

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Worked answer

JkT

KJKkTQ

JKk

KCT o

21

123

123

101.4

3001038.1

1038.1

30027

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Example questions

• Determine the amount of energy a particle would have if it were:

– In the centre of the Sun– In the centre of a supernova– In Mars’ northern polar cap– In interstellar space

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Location k / JK-1 T / K kT / J

Centre of the Sun 1.38 x 10-23

Centre of a supernova 1.38 x 10-23

Within magma 1.38 x 10-23

Within Mars' northern polar cap

1.38 x 10-23

In interstellar space 1.38 x 10-23

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Location k / JK-1 T / K kT / J

Centre of the Sun 1.38E-23 1.50E+07 2.07E-16

Centre of a supernova 1.38E-23 1.00E+11 1.38E-12

Within magma 1.38E-23 1.00E+03 1.38E-20

Within Mars' northern polar cap

1.38E-23 2.30E+02 3.17E-21

In interstellar space 1.38E-23 3.00E+00 4.14E-23

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If T = 10 000 K

eVkT 1

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The eV

• The energy gained by an electron as it moves through a potential difference of 1 V

JW

VCW

QVW

Q

WV

19

19

106.1

1106.1

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Show kT = 1eV (T = 10000K)

eVkT

JeV

JkT

KkT

KT

1

106.11

1038.1

100001038.1

10000

19

19

24

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Ideal gaskT

2

1

kT2

1

kT2

3 kT2

1

kT2

1

kT2

1

kT2

1

kT3

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Hotter and hotter

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Life at T = 300 K

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Fires and kilns, T = 1500 K

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White hot at the Sun’s surface, T = 6000 K

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Hotter still: inside the Sun, T = 6000000 K