Temperature

0.0(0)
studied byStudied by 0 people
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
Card Sorting

1/23

encourage image

There's no tags or description

Looks like no tags are added yet.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

24 Terms

1
New cards

What types of scales are celsius and fahrenheit?

Reference scales for measuring temperature, relative to two common reference points (freezing & boiling), can go above and below these

2
New cards

What type of scale is kelvin?

- Absolute scale

- Begins at absolute zero (-273.15°C)

- Theoretically no molecular activity, no energy, to radiation emitted

3
New cards

Convert celsius to fahrenheit

(°C x 9/5) + 32

4
New cards

Convert fahrenheit to celsius

(°F - 32) x 5/9

5
New cards

Convert celsius to kelvin

°C + 273.15

6
New cards

Convert fahrenheit to kelvin

((°F - 32) x 5/9) + 273.15

7
New cards

Why are freezing and boiling points for celsius and fahrenheit different?

- Different scientific method used to get the scale

- Celsius based on fresh water

- Fahrenheit based on salt water

8
New cards

What is temperature?

- Average amount of kinetic energy potential/molecular activity in a volume

- Hotter objects produce/emit more radiation absorbed into out own bodies increasing out kinetic energy

- Ability of a substance to transfer energy to another substance as radiation

9
New cards

What is heat?

Energy in the process of being transferred

10
New cards

What is radiation?

Energy emitted as electromagnetic waves (all substances emit this above absolute zero)

11
New cards

How does the molecular structure of an object relate to its temperature?

- Gas has more energy

- Fewer molecular bonds

- Moves more than a solid

- Molecules collide more

- It will be hotter

12
New cards

What is the Stefan Boltzmann law?

Intensity of energy radiated by a black body increases according to the fourth power of its absolute temperature (hotter the temperature, the more energy you emit, exponential increase)

13
New cards

What is Wein's law?

Radiating body, wavelength of peak emissions inversely proportional to absolute temperature (increased temperature, shorter wavelength, radiation type can change)

14
New cards

What are peak emissions?

Range of wavelength where most of the radiative emissions are found

15
New cards

What is a black body?

- Theoretical

- Perfect emitter

- 100% of radiative energy emitted at an absolute temperature

- Emissivity 1.0 or 100%

16
New cards

What is a grey body?

- All bodies in nature

- Imperfect emitter

- Gives a proportion of maximum output at a temperature

17
New cards

What is emissivity?

Proportion of substances theoretical black body emissions that is emitted (0.8 = 80% of black body ideal)

18
New cards

How do radiation emissions react to changes in a substance's temperature in relation to Stefan Boltzmann and Wein's law?

Difference temperatures change the amount and types of radiation emitted

19
New cards

How does the sun's radiation emissions relate to Stefan Boltzmann and Wein's law?

- Sun gives more energy

- 64 milllion Wm2

- Short peak wavelengths

- 4 different types of radiation (ultraviolet, visible light, near infrared, infrared

20
New cards

How does the earth's radiation emissions relate to Stefan Boltzmann and Wein's law?

- Less energy

- 390 Wm2

- Longer peak wavelengths

- Near infrared and infrared radiation

21
New cards

What is solar radiation?

Radiation emitted by the sun

22
New cards

What are the approximate wavelengths of solar radiation?

- Infrared (45%), 0.8 um to 1 mm

- Visible light (45%), 0.4 to 0.8 um

- UV (10%), <0.4 um

23
New cards

What is terrestrial radiation?

Radiation emitted by the earth

24
New cards

What is the approximate wavelength for terrestrial radiation?

3 to 100 um