Physics and Astronomy Lecture Notes Vocabulary Exam 1

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A set of vocabulary flashcards covering basic physics, radiation, Kepler's and Newton's laws, astronomical measurements, and cosmological bodies based on lecture notes.

Last updated 9:50 PM on 9/8/26
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47 Terms

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Electromagnetic radiation

A rapidly changing electric and magnetic field that propagates through space carrying momentum and energy.

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Wavelength

The distance between adjacent peaks of the field.

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Frequency

The rate at which the electric and magnetic fields change, describing how fast it oscillates.

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Visible light

The portion of the light spectrum with wavelengths between 400400 and 700700 that human eyes can see.

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Speed of light (cc)

A constant velocity equal to c=3×108 m/s=6.7×108 m/hc = 3 \times 10^8\text{ m/s} = 6.7 \times 10^8\text{ m/h}.

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Photons

Light particles with energy defined by E=hνE = h\nu or E=hcλE=\frac{hc}{{}\lambda}

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Plank's constant (hh)

A fundamental constant equal to h=6.67×1034 J sh = 6.67 \times 10^{-34}\text{ J s}.

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Spectrum

A band of colors, as seen in a rainbow, produced by a separation of the components of light according to wavelength.

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Albedo

The fraction of light that an object reflects, ranging from 00 to 11.

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Blackbody radiation

Radiation emitted by all dense objects, where an object's peak wavelength depends on its temperature.

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Wein's constant (bb)

A constant equal to b=2.96×106 nm Kb = 2.96 \times 10^6\text{ nm K} used to find peak wavelength via \frac{\frac{}{}{}}{\frac{}{}{}}.

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Continuous spectrum

Smooth light across a broad range of wavelengths, characteristic of blackbody radiation.

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Emission line spectrum

Bright lines at a specific wavelength on a dark background.

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Absorption line spectrum

Dark lines at specific wavelengths on a continuous background caused by an absorbing medium.

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Element

A substance defined by the number of protons in its atom's nucleus.

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Isotope

Atoms containing the same number of protons but a different number of neutrons.

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Ion

An atom with an unequal number of protons and electrons, resulting in a positive or negative charge.

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Lagrange points

Locations in space where satellites can orbit, such as L2L2 which is shadowed by the Earth.

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Kepler's first law

The law stating that the orbit of each planet about the sun is an ellipse with the sun at one focus.

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Eccentricity

The amount of flattening of an ellipse, where a perfect circular orbit is 00 and any orbital eccentricity must be less than 11.

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Semimajor axis

Half of the major axis of an ellipse (1 AU1\text{ AU}).

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Kepler's second law

The law stating that planets sweep out equal areas in equal times, moving faster closer to the star and slower farther away.

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Perihelion

The point in an orbit when the planet is closest to the star.

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Aphelion

The point in an orbit when the planet is furthest from the star.

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Kepler's third law

The law stating that more distant planets orbit the Sun at a slower average speed, expressed as P2=a3P^2 = a^3.

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Inertia (Newton's first law)

The principle that an object at rest remains at rest unless acted on by an unbalanced force.

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Newton's second law of motion

The law governing force, stating that force equals mass times acceleration (F=m×aF = m \times a).

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Newton's third law of motion

The law of action/reaction, stating that every action has an equal and opposite reaction.

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Zenith

The point in the sky directly above your head at any given time.

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Cosmology

The concept and study of the cosmos.

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Retrograde motion

The apparent backward movement of a planet across the sky relative to background stars.

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Prograde motion

The standard forward movement of a planet across the sky.

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Apparent magnitude

A star's brightness as measured from Earth.

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Absolute magnitude

A star's actual intrinsic brightness.

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Precession

The slow change in the direction in which Earth's rotational axis points over time.

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Stellar parallax

The apparent shift in the position of a star relative to its background when viewed from different positions.

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Parsec

Parallax arcsecond; the distance from the sun to an astronomical object that has a parallax angle of 11 arcsecond.

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Astronomy

The study of objects that lie beyond our planet Earth.

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Hypothesis

A potential educated explanation for an observation.

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Theory

A hypothesis that has been rigorously tested and consistently supported, providing a comprehensive framework for understanding.

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Comet

An icy, dusty body that often orbits the sun in a very elliptical path.

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Asteroid

A small, rocky body orbiting the sun between Mars and Jupiter.

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Galaxy

A group of many billions of stars orbiting around a central black hole.

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Star

A large ball of gas burning hydrogen into helium and other elements through nuclear fusion in its core.

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Exoplanets

Planets located outside of our solar system.

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Universe

The infinite collection of all known matter and space.

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Equation that givs peak wavelength

λpeak = b/T