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A comprehensive set of flashcards covering key concepts and definitions in astronomy, suitable for exam preparation.
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Astronomy
The science that studies celestial objects (stars, planets, galaxies) using physics and observations.
Astrology
The non-science belief that celestial positions influence human behavior, using horoscopes without empirical evidence.
Celestial Sphere
An imaginary sphere surrounding Earth, used to map the positions of stars and celestial objects as if they were fixed on its surface.
Geocentrism
The model where Earth is the center of the universe, with all celestial bodies orbiting it.
Heliocentrism
The model where the Sun is the center of the universe, with Earth and planets orbiting it.
Nicolaus Copernicus
Proposed the heliocentric model in 1543, shifting the understanding from Earth-centered to Sun-centered orbits.
Tycho Brahe
Made precise naked-eye observations of planetary positions, providing accurate data for Kepler.
Johannes Kepler
Formulated the three laws of planetary motion using Brahe’s data.
Galileo Galilei
Used telescopes to observe celestial bodies, providing evidence for heliocentrism.
Isaac Newton
Developed the laws of motion and universal gravitation, explaining planetary orbits.
Earth's Tilt
Earth's axis is tilted approximately 23.5 degrees, causing seasons.
Ecliptic
The apparent path of the Sun across the celestial sphere as seen from Earth.
Circumpolar Stars
Stars near the celestial poles that never set below the horizon.
Kepler's Three Laws of Planetary Motion
(1) Planets orbit in elliptical paths, (2) A line from a planet to the Sun sweeps out equal areas in equal times, (3) The square of a planet's orbital period is proportional to the cube of its semi-major axis.
Newton's Three Laws of Motion
(1) An object remains at rest or in uniform motion unless acted upon, (2) F=ma, (3) For every action, there is an equal and opposite reaction.
Universal Law of Gravitation
Every mass attracts every other mass with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
Centripetal Force
The force that keeps an object moving in a circular path, directed toward the center of the orbit.
Escape Velocity
The minimum speed an object needs to escape a celestial body's gravitational pull without further propulsion.
Orbital Velocity
The speed an object must maintain to stay in a stable orbit around a celestial body.
Properties of an Ellipse
Includes shape, foci, semi-major axis, semi-minor axis, and eccentricity.
Wave–Particle Duality of Light
Light behaves both as a wave and as a particle, depending on how it’s observed or measured.
Electromagnetic Spectrum
The range of all possible wavelengths of electromagnetic radiation.
Resolution of Telescopes
The ability to distinguish fine details, determined by aperture size, wavelength of light, and atmospheric conditions.
Spectra
The distribution of light from a celestial object across different wavelengths, revealing its composition.
Energy of a Photon
Determined by E = h * f, inversely proportional to wavelength and directly proportional to frequency.
Luminosity
The total energy output of a star per unit time, measured in watts.
Stefan–Boltzmann Law
The total energy radiated per unit surface area of a blackbody is proportional to the fourth power of its temperature.
Wien’s Law
The wavelength at which a blackbody emits maximum radiation is inversely proportional to its temperature.
Nebular Hypothesis
A model explaining solar system formation from a rotating cloud of gas and dust.
Habitable Zone
The region around a star where conditions allow liquid water to exist on a planet's surface.
Goldilocks Zone
Another term for the habitable zone.
Radioactive Decay
The process contributing to heating Earth's core.
Constants
Fundamental values such as G, h, and c necessary for astronomical calculations.
Kepler's Third Law
P^2 = A^3, relating a planet's orbital period to its distance from the Sun.