14 matter very cold
DESCRIPTION
intro to chapter 14, matter very cold, very hotTRANSCRIPT
What are these objects?
Order them from coldest to hottest
What are these objects?
Order them from coldest to hottest
kT is about how much energy
particles have at temperature T in
kelvin
Worked example
• On a nice summer’s day (27 oC) how much energy would the particles have?
Worked answer
JkT
KJKkTQ
JKk
KCT o
21
123
123
101.4
3001038.1
1038.1
30027
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
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
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
If T = 10 000 K
eVkT 1
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
Show kT = 1eV (T = 10000K)
eVkT
JeV
JkT
KkT
KT
1
106.11
1038.1
100001038.1
10000
19
19
24
Ideal gaskT
2
1
kT2
1
kT2
3 kT2
1
kT2
1
kT2
1
kT2
1
kT3
Hotter and hotter
Life at T = 300 K
Fires and kilns, T = 1500 K
White hot at the Sun’s surface, T = 6000 K
Hotter still: inside the Sun, T = 6000000 K