ast101h exam 1

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Last updated 5:56 PM on 12/8/25
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77 Terms

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Accretion

The process of material clumping together under gravity during planet formation.

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Absorption Lines

Dark lines in a spectrum created when atoms absorb specific wavelengths of light.

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Asteroid

A small rocky object orbiting the Sun that is not spherical and has not cleared its orbit.

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Asteroid Belt

Region between Mars and Jupiter containing rocky bodies; has gaps due to Jupiter’s resonances.

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Atmospheric Stripping

Removal of a planet’s atmosphere by the solar wind when no magnetic field is present.

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Atmospheric Escape

When atoms/molecules move faster than escape velocity and leave a planet permanently.

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Blackbody Radiation

Light emitted by an object depending only on its temperature.

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Carbon Cycle

Recycling of CO₂ between atmosphere, oceans, rocks, and volcanism on Earth.

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Centre of Mass

The point around which two orbiting bodies both orbit.

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Chemical Differentiation

Heavy materials sink, light materials rise inside a molten planet.

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Comet

A small, icy, dusty object that develops tails when near the Sun.

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Conduction

Heat transfer through solid material (crust).

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Convection

Heat transfer by moving fluid (mantle, gas layers).

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Corona

Sun’s outermost atmosphere; extremely hot.

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D/H Ratio

Ratio of deuterium to hydrogen; used to infer past water loss (e.g., Mars has high D/H).

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Differentiation Heat

Heat released when dense materials sink toward a planet’s center early in its life.

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Dirty Snowball

Common phrase describing comet composition.

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Doppler Shift

Change in wavelength due to motion of source; used to detect exoplanets by star wobble.

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Eccentric Orbit

An orbit shaped like a stretched ellipse.

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Edge-on Orientation

Viewing angle required for exoplanet transits.

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Electromagnetic Spectrum

Range of light wavelengths; includes gamma, X-ray, UV, visible, IR, radio.

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Emission

Object gives off light based on its temperature.

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Escape Velocity

Minimum speed required to leave a planet’s gravitational pull.

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Flyby Mission

A spacecraft that passes a target once without stopping or landing.

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Frost Line

Distance from the Sun where ices can form; divides rocky inner planets from icy outer planets.

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Galilean Moons

Jupiter’s four moons discovered by Galileo: Io, Europa, Ganymede, Callisto.

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Gas Giant

A large planet composed mostly of H & He (Jupiter, Saturn).

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Geological Activity

Surface change from volcanism, tectonics, erosion; requires internal heat.

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Greenhouse Effect

Infrared radiation emitted by a planet is trapped by atmospheric gases, warming the surface.

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Greenhouse Runaway

Extreme greenhouse warming where oceans evaporate (e.g., Venus).

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Habitable Zone

Region around a star where liquid water can exist.

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Half-life

Time for half of a radioactive sample to decay.

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Heavy Bombardment

Early Solar System period of intense asteroid/comet impacts.

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Hydrogen Compounds

Ices like water, ammonia, methane found in outer planets.

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Impact Cratering

Holes caused by collisions with space rocks; more craters = older surface.

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Infrared Light (IR)

Long-wavelength light useful for seeing through dust/molecular clouds.

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Interstellar Object

An object that is not gravitationally bound to the Sun (e.g., ’Oumuamua).

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Jovian Planets

The outer gas/ice giants: Jupiter, Saturn, Uranus, Neptune.

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Kepler’s First Law

Planets orbit in ellipses with the Sun at one focus.

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Kepler’s Second Law

Planets sweep equal areas in equal times (move faster when closer to Sun).

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Kepler’s Third Law

Orbital period squared ∝ distance cubed.

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Kirkwood Gaps

Empty regions in asteroid belt due to Jupiter’s resonances.

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Kuiper Belt

Region beyond Neptune containing icy bodies and dwarf planets.

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Light Curve

Graph of star brightness over time; dips show transits.

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Magnetic Field

Created by rotating, molten metal core; protects planet from solar wind.

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Mantle

Layer where convection transports heat upward.

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Meteorite

Rock from space found on Earth; used for radioactive dating.

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Microlensing

Exoplanet detection via gravitational focusing of light.

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Molecular Cloud

Cold gas/dust region where stars form; blocks visible light.

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Nebular Hypothesis

Theory describing Solar System formation from a rotating gas cloud.

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Nuclear Fusion

Process powering stars; not active in planets.

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Oort Cloud

Spherical cloud of very distant comets around the Solar System.

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Orbital Resonance

When two objects influence each other by orbiting at exact integer ratios (e.g., Io–Europa–Ganymede).

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Outgassing

Release of gases from a planet’s interior (mostly via volcanoes).

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Photosphere

Visible surface of the Sun.

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Planet Criteria - 1. Orbits the Sun 2. Spherical 3. Cleared its orbit

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P-waves

Seismic waves that pass through solids and liquids.

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Radioactive Dating

Measuring isotope ratios to determine ages of rocks/meteorites.

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Radial Velocity Method

Exoplanet detection via star’s spectral line wobbling from Doppler shift.

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Radiative Zone

Sun’s layer where energy moves via radiation.

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Recovery Mission

Mission where a spacecraft lands, returns samples, and comes back to Earth.

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Resonance Gap (Rings)

Gaps in planetary rings created by gravitational interactions with moons.

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Scattering

Light bouncing in many directions; why we can read a page or see blue sky.

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Slingshot Maneuver

A spacecraft accelerates using gravity during a close pass of a planet.

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Solar Wind

Charged particles from the Sun that strip atmospheres without magnetic protection.

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Spectrum

Range of light broken into wavelengths; reveals temperature, composition, motion.

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S-waves

Seismic waves that cannot pass through liquid → prove Earth’s outer core is liquid.

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Tectonics

Surface reshaping through plate motion.

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Transit Method

Exoplanet detection via dip in starlight when planet crosses star.

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Tidal Heating

Frictional heating caused by distortions in a moon’s orbit (e.g., Io, Europa).

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Umbra (speaking generally)

Full shadow; not central to AST101, but sometimes appears in lunar eclipse context.

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Volcanism

Eruption of molten rock from interior; reshapes surfaces, releases gases.

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Visible Light

Light humans see; blocked by dust in molecular clouds.

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Wobble (Stellar)

Motion of a star caused by orbiting planets; basis of the Doppler method.

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X-ray Astronomy

Must be done from space because Earth’s atmosphere blocks X-rays.

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Yellow Dwarf

Category of Sun; not heavily tested but sometimes mentioned.

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Zero-Age Main Sequence (ZAMS)

When a star first begins fusion; only indirectly relevant.