ASTRONOMY 104 Study Guide Key Concepts and Equations

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A comprehensive set of flashcards covering key concepts and definitions in astronomy, suitable for exam preparation.

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34 Terms

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Astronomy

The science that studies celestial objects (stars, planets, galaxies) using physics and observations.

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Astrology

The non-science belief that celestial positions influence human behavior, using horoscopes without empirical evidence.

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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.

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Geocentrism

The model where Earth is the center of the universe, with all celestial bodies orbiting it.

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Heliocentrism

The model where the Sun is the center of the universe, with Earth and planets orbiting it.

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Nicolaus Copernicus

Proposed the heliocentric model in 1543, shifting the understanding from Earth-centered to Sun-centered orbits.

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Tycho Brahe

Made precise naked-eye observations of planetary positions, providing accurate data for Kepler.

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Johannes Kepler

Formulated the three laws of planetary motion using Brahe’s data.

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Galileo Galilei

Used telescopes to observe celestial bodies, providing evidence for heliocentrism.

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Isaac Newton

Developed the laws of motion and universal gravitation, explaining planetary orbits.

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Earth's Tilt

Earth's axis is tilted approximately 23.5 degrees, causing seasons.

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Ecliptic

The apparent path of the Sun across the celestial sphere as seen from Earth.

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Circumpolar Stars

Stars near the celestial poles that never set below the horizon.

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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.

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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.

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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.

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Centripetal Force

The force that keeps an object moving in a circular path, directed toward the center of the orbit.

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Escape Velocity

The minimum speed an object needs to escape a celestial body's gravitational pull without further propulsion.

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Orbital Velocity

The speed an object must maintain to stay in a stable orbit around a celestial body.

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Properties of an Ellipse

Includes shape, foci, semi-major axis, semi-minor axis, and eccentricity.

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Wave–Particle Duality of Light

Light behaves both as a wave and as a particle, depending on how it’s observed or measured.

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Electromagnetic Spectrum

The range of all possible wavelengths of electromagnetic radiation.

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Resolution of Telescopes

The ability to distinguish fine details, determined by aperture size, wavelength of light, and atmospheric conditions.

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Spectra

The distribution of light from a celestial object across different wavelengths, revealing its composition.

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Energy of a Photon

Determined by E = h * f, inversely proportional to wavelength and directly proportional to frequency.

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Luminosity

The total energy output of a star per unit time, measured in watts.

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Stefan–Boltzmann Law

The total energy radiated per unit surface area of a blackbody is proportional to the fourth power of its temperature.

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Wien’s Law

The wavelength at which a blackbody emits maximum radiation is inversely proportional to its temperature.

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Nebular Hypothesis

A model explaining solar system formation from a rotating cloud of gas and dust.

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Habitable Zone

The region around a star where conditions allow liquid water to exist on a planet's surface.

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Goldilocks Zone

Another term for the habitable zone.

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Radioactive Decay

The process contributing to heating Earth's core.

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Constants

Fundamental values such as G, h, and c necessary for astronomical calculations.

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Kepler's Third Law

P^2 = A^3, relating a planet's orbital period to its distance from the Sun.