1/47
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced |
---|
No study sessions yet.
Kinetic energy
is the energy that an object possesses due to its motion. It is dependent on the mass and velocity of the object.
Radiative energy
is the energy carried by electromagnetic waves, such as light. It is a form of energy that can travel through space and is emitted by objects as they radiate heat.
potential energy
is the energy stored in an object due to its position or configuration. It can be converted to kinetic energy when the object is set in motion.
Gravitational potential energy
is the potential energy held by an object because of its vertical position or height in a gravitational field. It is calculated based on the object's height above a reference point and its mass.
Kepler’s first law of planetary motion
states that planets move in elliptical orbits around the Sun, with the Sun at one of the foci of the ellipse.
Keplers second law of planetary motion
states that a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time, meaning that planets move faster when they are closer to the Sun.
Kelpers third law of planetary motion
states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit, indicating a relationship between a planet's distance from the Sun and its orbital period.
Venus Phase
galileo’s observations of the phases of Venus proved that it orbits the sun and not Earth
Reflection Nebula
stellar light scattered by surrounding dust particles-these dust particles reflect light from the stars they surround
Intersteller extinction
the dimming of light from distant stars caused by interstellar dust and gas absorbing and scattering the light.
Ecliptic
the path the sun appears to take around the celestial sphere each year
Precession
The direction in which Earth’s axis points does indeed change slowly but regularly
Quasers
Brlliant centers of galaxies, glowing with the light of an extraordinarily energetic process
Newtons first law of motion
EVery object willc ontinue to be in a state of rest or move at a constant speed in a straight line unless compelled to change by an outside force
Newtons second law of motion
The change of motion in a body is proportional to and in the direction of the force acting on it
Newtons second law of motion
Every action has an equal and opposite reaction
Angular momentum
A measure of the rotation of a body as it revolves around some fixed point
Waves
A wave is a pattern of motion that can carry energy without carrying matter along with it
Particles of light
Photons; The higher the frequency the higher the energy
The electromagnetic spectrum
The range of all types of electromagnetic radiation
Universal law of gravitation
Gravitational attraction between two bodies must be proportional to their masses
Emission line spectrum
A thin or low-density cloud of gas emits light only at specific wavelengths that depend on its composition and temperature, producing a spectrum with bright emission lines. Jumping from higher energy to lower energy
Continuous spectrum
A cloud of gas between us and a light bulb can absorb light of a specific wavelength, leaving dark absorption lines in the spectrum. Photon jumps from lower to higher energy
Absorption line spectrum
a spectrum of (incandescent) light bulbs spans all wavelengths
The doppler effect
Things get louder the closer you are, and quieter the further they are
Waxing crescent phase
A thin crescent appears
Firat quarter phase
Half of the moon is visible; rises around noon and sets around midnight
Waxing Gibbous phase
When more than half of the moon is illuminated
Solar eclipse
The sun is at least partially covered by the moon
Lunar Eclipse
When the moon passes into the shadow of the Earth
Photon
A self contained packet of electromagnetic energy
Inverse square law
The apparent brightness of a source gets weaker with distance
Gamma rays
The shortest wavelength; 7.1 nanometers
X rays
the second shortest wavelength, able to penetrate body tissues.
Ultraviolet
Also called black light; blocked by the ozone layer and causes sunburns and cancer
Visible light
The waves that humans can visibly perceive
Infrared
Heat radiation: a continuous spectrum Absorbed by water and carbon dioxide molecules
Microwave
Short wave communication; Absorbed by water vapor
Radiowave
Waves that can travel long distances; ideal for wireless communication
Blackbody
AN object that does not scatter radiation but absorbs all the electromagnetic energy that falls onto it
Wien’s law
The wavelength of light emitted by an object is inversely proportional to the object's temperature
DIspersion
The separation of light colors or the variation of velocities among objects
Atomic mass number
Number of protons and neutrons
Upward jump
Electron gains energy
Downward jump
Electron loses energy
Ground state
An atom’s lowest point of possible energy
Excited state
Atom absorbs energy and is moved to a higher energy level
Ionization
If enough energy is absorbed, the electron can be completely removed from the atom