Vocab Flashcards
standard unit
a fixed and reproducible reference value used for the purpose of taking accurate measurements
system of units
a group of standard units and their combinations. The two major systems of units used today are the metric system and the British system
metric system
the decimal system of units most used in the world; also called the mks system
British system
the system of units still often employed in the U.S. and is sometimes referred to as the fps system (foot-pound-second)
length
the measurement of space in any direction
meter
the standard unit of length in the mks system. Equal to 39.37 inches or 3.28 feet.
kilogram
the unit of mass in the mks system; 1 kg has an equivalent weight of 2.2 pounds
time
the continuous forward-flowing of events
second
the standard unit of time. It is now defined in the terms of the frequency of a certain transition in the cesium atom
SI (International System of Units)
a modernized version of the metric system that contains seven base units
derived units
combinations of fundamental units
conversion factor
an equivalence statement expressed as a ratio
significant figures
the method of estimating or expressing error in mathematical operations and measurements
physics
the most fundamental physical science, concerned with the basic principles and concepts that describe the workings of the unviverse
position
the location of an object with respect to another object
motion
the changing of position
scalar
a quantity that has magnitude but no direction
vector
a quantity that has both magnitude and direction
average speed (v)
the distance traveled divided by the change in time
distance (d)
the actual path length between two points
instantaneous speed
how fast an object is traveling at a particular moment or instant
average velocity
the change in position/displacement divided by the change in time
displacement
the directional straight-line between two points
instantaneous velocity
the velocity at a particular instant of time
acceleration
the change in velocity divided by the change in time
average acceleration (a)
the change in velocity divided by the time for the change to occur
acceleration due to gravity (g)
9.80 m/s^2 or 32 ft/s^2
free-fall
the state of motion solely under the influence of gravity
terminal velocity
the maximum velocity reached by a falling object because of air resistance
centripetal acceleration
the “center-seeking” acceleration necessary for circular motion; a=v^2/r
projectile motion
the motion of a projected or thrown object under the influence of gravity
force
any quantity capable of producing motion
unbalance, or net force
the sum of vector forces with a nonzero result. A force capable of producing motion
Newton’s first law of motion
an object will move at a constant velocity unless acted upon by an external unbalanced force
intertia
the natural tendency of an object to remain in a state of rest or in a uniform motion in a straight line
mass
the quantity of matter and a measurement of the amount of inertia that an object possesses
Newton’s second law of motion
the acceleration of an object is equal to the net force on the object divided by the mass of the object; a=F/m
newton
the unit of force in the mks system; 1 kg x m/s^2
weight
a measure of the force due to gravitational attraction (w=mg on the Earth’s surface)
friction
the ever-present resistance to relative motion that occurs whenever two materials are in constant with each other (solids, liquids, or gases)
Newton’s third law of motion
whenever one object exerts a force upon a second object, the second object exerts an equal and opposite force upon the first object
Newton’s law of universal gravitation
the gravitational force between two masses (m1 and m2) is directly proportional to the product of the masses and inversely proportional to the square of the distance r between their centers of mass; F=Gm1m2/r^2
G
the universal gravitational constant; G= 6.67 x 10^ -11 Nm^2/kg^2
buoyant force
the upward force resulting from an object being wholly or partially submerged in a fluid
Archimedes’ principle
an object immersed wholly or partially in a fluid experienced a buoyant force equal in magnitude to the weight of the volume of fluid that it displaced
linear momentum
the product of an object’s mass and its velocity
law of conservation of linear momentum
the total linear momentum of a system remains constant if there is no external unbalanced forces acting on the system
angular momentum
mvr for a mass m going at a speed v in a circle of radius r
torque
the force that tends to produce rotational motion
law of conservation of angular momentum
the angular momentum of a system remains constant unless acted upon by a net torque
work
the product of a force and the parallel distance through which it acts
joule (J)
a unit of energy equivalent to 1 N m or 1 kg m^2/s^2
foot-pound
the unit of work (and energy) in the British system
energy
the capacity to do work
kinetic energy
the energy of motion equal to 1/2 mv^2
potential energy
the energy a body possesses because of its position
gravitational potential energy
the potential energy resulting from an object’s position in a gravitational field; in other words, the stored energy that comes from doing work against gravity
conservation of total energy
the total energy of an isolated system remains constant
conservation of mechanical energy
in an ideal system, the sum of the kinetic and potential energies is constant; Ek + Ep = E (a constant)
power
work or energy per unit time
watt (W)
a unit of power equivalent to 1 kg m^2/s^3 or 1 J/s
horsepower (hp)
a unit of power equal to 550 ft lb/s (746 W)
kilowatt-hour (kWh)
a unit of energy (power x time); P = E/t and E = Pt
alternate energy sources
energy sources that are not based on the burning of fossil fuels and nuclear processes
renewable energy sources
energy sources that cannot be exhausted, such as wind and hydro power
waves
the propagation (spreading) of energy from a disturbance
longitudinal wave
a wave in which the particle motion and the wave velocity are parallel to each other
transverse wave
a wave in which the vibrations are perpendicular to the wave velocity
wavelength
the distance from any point on a wave to an identical point on the adjacent wave
amplitude
the maximum displacement of a wave from its equilibrium position
frequency
the number of oscillations of a wave during one second
hertz (Hz)
one cycle per second. The SI unit of frequency
period (T) (physics)
the time for a complete cycle of motion
electromagnetic waves
a transverse wave consisting of oscillating electric and magnetic fields
speed of light
c= 3.00 x 10^8 m/s
sound
a wave phenomenon caused by variations in pressure in a medium such as air; speed of sound= 340 m/s
intensity (I) of sound wave
the rate of energy transfer through a given area, with units of watts per square meter (W/m^2)
sound spectrum
an ordered arrangement of various frequencies or wavelengths of sound. The three main regions of the sound spectrum are the infrasonic, the audible, and the ultrasonic
decibel (dB)
a unit of sound intensity level; 0.1 bel
ultrasound
sound with frequency above 20 kHz
speed of sound
how fast sound travels in a medium; for example, speed of sound = 344 m/s in air at room temperature
Doppler effect
an apparent change in frequency resulting from the relative motion of the source and the observer
redshift
a Doppler effect caused when a light source, such as a galaxy, moves away from the observer and shifts the light frequency lower, or toward the red end of electromagnetic spectrum
standing waves
a stationary wave from arising from the interference of waves traveling in opposite directions
resonance
a wave effect that occurs when an object has a natural frequency that corresponds to an external frequency
reflection
the change in the direction of a wave when it strikes and rebounds from a surface or the boundary between two media
ray
a straight line that represents the path of light
law of reflection
the angle incidence equals the angle of reflection, as measured relative to the normal, a line perpendicular to the reflecting surface
specular reflection
the reflection from very smooth (mirror) surfaces
refraction
the bending of light waves caused by a seed change as light goes from one medium to another
index of refraction
the ration of the speed of light in a vacuum to the speed of light in a medium
total internal reflection
a phenomenon in which light is totally reflected in a medium because refraction is impossible
dispersion
different frequencies of light refracted at slightly different angles, giving rise to a spectrum
focal length
the distance from the vertex of a mirror or lens to the focal point
concave or converging mirror
a mirror shaped like the inside (concave side) of a small section of a sphere
convex or diverging mirror
a mirror shaped like the outside (convex side) of a spherical section
diffuse reflection
rays reflected from relatively rough surfaces that are not parallel
real image
an image from a mirror or lens that can be brought to focus on a screen
virtual image
an image from a lens or mirror that cannot be brought to focus on a screen
convex or converging lens
a lens that has a surface shape of the out of the outside (convex side) of a spherical section
concave or diverging lens
a lens that has the shape of the outside (concave side) of a spherical section
polarization
the preferential orientation of the electric vector of a light wave to one plane
linearly polarized light
the condition of transverse light waves that vibrate in only one plane
diffraction
the bending of waves when moving past an opening or obstacle that has a size smaller than or equal to the wavelength
principle of superposition (wave)
the combined waveform of two or more interfering waves is given by the sum of the displacements of the individual waves
constructive interference
a superposition of waves for which the combined waveform has a greater amplitude
destructive interference
a superposition of waves for which the combined waveform has a smaller amplitude
quantum
a discrete amount
photoelectric effect
an emission of electrons that occurs when certain metals are exposed to light
photon
a “particle” of electromagnetic energy
dual nature of light
light sometimes behaves as waves and sometimes as particles
line emission spetrum
a set of bright spectral lines of certain frequencies or wavelengths formed by dispersion of light from a gas discharge tube. Each element gives a different set of lines
line absorption spectrum
a set of dark spectral lines of certain frequencies or wavelengths, formed by dispersion of light that has come from an incandescent source source and has then passed through a sample of cool gas
principal quantum number
the numbers n = 1, 2, 3, … used to designate the various principal energy levels that an electron may occupy in an atom
ground state
the lowest energy level of an atom
excited states
the energy levels above the ground state in an atom
fluorescence
the property of a substance, such as the mineral fluorite, of producing visible light while it is being acted upon by ultraviolet light
phosphorescence
a glow of light that persists after the removal of the source of photons needed for excitation of the material’s electrons
x-rays
high-frequency, high-energy electromagnetic radiation formed when high-speed electrons strike a metallic target
laser
acronym for Light Amplification by Stimulated Emission of Radiation; it is coherent, monochramatic light
stimulated emission
process in which an excited atom is caused to emit a photon
universe
everything that is: all energy, matter, and space
celestial sphere
the apparent sphere of the sky on which all the stars seem to appear
ecliptic
the apparent annual path of the sun on the celestial sphere
celestial prime meridian
an imaginary half-circle running from the north celestial pole to the south celestial pole and crossing perpendicular to the celestial equator at the point of the vernal equinox
right ascension
a coordination for measuring the east-west positions of celestial objects. The angle is measured eastward from the vernal equinox in hours, minutes, and seconds
declination
the angular measure in degrees north or south of the celestial equator
parsec (pc)
the distance to a star when the star exhibits a parallax of one second of arc. This distance is equal to 3.26 light years.
photosphere
the sun’s outer surface, visible to the eye
proton-proton chain
a series of stellar nuclear reactions in which four hydrogen nuclei (protons) combine to form one helium nucleus and release energy
apparent magnitude
the brightness of a star (or other celestial object) observed from earth
absolute magnitude
the brightness of a star it would have if it were placed 10 pc (32.6 ly) from earth
H-R diagram
the plot of the absolute magnitude versus the temperature of stars
main sequence
the narrow band on the H-R diagram on which most stars fall
red giants
a relatively cool, very bright star that has a diameter much larger than average
white dwarfs
a hot white star that has a much smaller diameter and much higher density than average. It is believed to be the final stage of a low-mass star
nebulae
vast clouds of interstellar gas and dust
nucleosynthesis
the creation of nuclei of elements inside stars
planetary nebula
a luminous shell of gas ejected from a old, low-mass star
brown dwarfs
low-mass objects that are larger than a typical planet but do not have enough mass to begin fusion in their cores. Also called “failed stars”
nova
a white dwarf star that suddenly increases dramatically in brightness for a brief period of time
supernova
an exploding star
neutron star
an extremely high-density star composed almost entirely of neutrons
black hole
an object whose gravity is so strong that the escape velocity is equal to or greater than the speed of light; thus no radiation can escape from the object
galaxy
a large-scale aggregate of stars (plus some gas and dust) held together by gravity. Galaxies have a spiral, elliptical, or irregular structure. Each contains, on average, 100 billion solar masses
globular clusters
a large, spherical group of gravitationally bound stars, usually found in the outlying regions of the galaxy
Local Group
the cluster of galaxies that includes our own Milky Way
dark matter
the as-yet-unidentified nonluminous matter in the universe
cosmology
the study of the structure and evolution of the universe
Hubble’s law
the recessional speed of a distant galaxy is directly proportional to its distance away
Big Bang
theory of the beginning of the universe that states that the known universe was smaller hotter, and denser in the past, and that is began rapidly expanding 13.7 billion years ago
cosmic microwave background
the microwave radiation that fills all space and is believed to be the redshifted glow from the Big Bang
astronomy
the scientific study of the universe, which is the totality of all matter, energy, space, and time
solar system
the sun, nine planets and their satellites, the asteroids, the comets, meteoroids, and interplanetary dust
geocentric model
the old false theory of the solar system, which placed the Earth at its center
heliocentric model
the model of the solar system that places the sun at its center
law of elliptical orbits
all planets move in elliptical orbits around the sun, with the sun at one focus of the ellipse
astronomical unit (AU)
the average distance between the earth and the sun, which is 93 million miles
law of equal areas
an imaginary line (radial vector) joining a planet to the sun sweeps out equal areas in equal periods of time
harmonic law (Kepler’s third law)
the square of the sidereal period of a planet is proportional to the cube of its semimajor axis (one-half the major axis
terrestrial planets
the four inner planets: Mercury, Venus, Earth, and Mars. All are similar to the Earth in general chemical and physical properties
Jovian planets
the four outer planets: Jupiter, Saturn, Uranus, and Neptune. All have characteristics resembling those of Jupiter
prograde motion
orbital or rotational motion in the forward direction. In the solar system, this is west-to-east, or counterclockwise, as viewed from above the Earth’s North Pole
retrograde rotation
orbital or rotational motion in the backward direction. In the solar system, this is east to west, or clockwise, as viewed from above the Earth’s North Pole
sidereal period
the orbital or rotational period of any object with respect to the stars
conjunction
when two planets are lined up with respect to the sun
opposition
the time at which a planet is on the opposite side of the Earth from the sun
albedo
the fraction of incident sunlight reflected by a body’s surface
rotation
the turning of an object about an axis passing through the mass
revolution
the movement of one mass around another
Foucault pendulum
a pendulum that is used to demonstrate the rotation of the Earth
parallax
the apparent motion, or shift, that occurs between two fixed objects when the observer changes position
aberration of starlight
the apparent displacement in the direction of light coming from a star that results from the orbital motion of the Earth
dwarf planets
a new class of planets, of which there are three: Pluto, Ceres, and Eris
solar nebula
a large, swirling volume of interstellar cold gas and dust that contracted under the influence of its own gravity and formed in the shape of flattened rotating disk
condensation theory
a process of solar system formation in which interstellar dust grains act as condensation nuclei
summer solstice
the farthest point of the sun’s latitude north of the equator (for the Northern Hemisphere), around June 21. The beginning of summer
winter solstice
the farthest point of the sun’s latitude south of the equator (for the Northern Hemisphere), around December 22. The beginning of winter