Ch 2 Flashcards
(49 cards)
What is temperature?
It tells us how hot or cold something is relative to some standard reference point
Whats degrees Celsius?
In reference to water’s freezing point
Kelvin?
An absolute scale
Degrees Fahrenheit?
A scale of human experience
Celsius equation?
5/9 (F-32)
Kelvin equation?
C + 273
What is temperature a measure of?
Kinetic energy
The average speed (average motion) of atoms and molecules, where higher temperatures correspond to faster speeds
In what area would it be -20F?
Higher levitation, upper north
What’s energy?
The ability or capacity to do work on matter
It changes forms and transfers from one body to another, but cannot be created nor destroyed
Potential energy
When something has the potential to do the work (it is up in the air, it can be burned, etc.)
Kinetic energy
The energy of motion (the wind, a car)
Three ways for heat to be transferred
Conduction, convection, radiation
What’s the best conductor?
What’s the worst conductor?
Best: silver- 427W
Worst: still air- .023W
Conduction
Heat transfer from molecule to molecule within a substance
Convection
Heat transfer by a fluid (such as water or air)
What do we call vertical motions? How about horizontal motions?
Vertical- CONvection
Horizontal- ADvection
Radiation
Heat transfer that does not require the substances touching or a fluid between them: energy from the sun
How does radiation travel?
In the form of electromagnetic waves, which move at the speed of light in a vacuum (186,000 miles per second)
The shorter the wavelength, the more energy it carries!
What are the types of “light”?
Gamma ray, x-ray, ultraviolet, infrared, microwave, radio
What is basically earths surface?
A boiling pot of water
What do these have to do with the weather?
Conduction: only important very near the ground
Convection: many clouds form as a result of convection, as warm, moist air rises
Radiation: energy from the sun warms the planet; causes daily changes in temperature, and much more
Stefan- Boltzmann Law
The amount radiation emitted is proportional to the 4th power of T
Total radiation= temp x temp x temp x temp x constant
Wien’s Law
Hotter objects emit most of their energy at shorter wavelengths
Wavelength max= 2897/ T
Solar radiation name
Shortwave radiation