Chapter 1: A Modern View of the Universe Vocabulary

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Vocabulary practice flashcards generated from Chapter 1 of The Essential Cosmic Perspective Ninth Edition.

Last updated 11:23 PM on 9/24/26
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15 Terms

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<p>Cosmic Address</p>

Cosmic Address

The multi-tiered sequence specifying Earth's location in space: Earth, Solar System, Milky Way Galaxy, Local Group, Local Supercluster, Universe.

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<p>Star</p>

Star

A large, glowing ball of gas that generates heat and light through nuclear fusion.

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Planet

A moderately large object that orbits a star and shines by reflected light; it may be rocky, icy, or gaseous in composition.

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Moon (or Satellite)

An object that orbits a planet.

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<p>Asteroid</p>

Asteroid

A relatively small and rocky object that orbits a star.

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<p>Comet</p>

Comet

A relatively small and icy object that orbits a star.

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Solar (Star) System

A star and all the material that orbits it, including its planets and moons.

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<p>Nebula</p>

Nebula

An interstellar cloud of gas and/or dust.

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Galaxy

A great island of stars in space, all held together by gravity and orbiting a common center.

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Universe

The sum total of all matter and energy; that is, everything within and between all galaxies.

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Light-Year

The distance light can travel in 1 year1\text{ year}, which is about 10 trillion kilometers10\text{ trillion kilometers} (6 trillion miles6\text{ trillion miles}).

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Speed of Light

The finite speed at which light travels through space, equal to approximately 300,000 km/s300,000\text{ km/s}.

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<p>Cosmic Calendar</p>

Cosmic Calendar

A scale model on which the entire history of the universe is compressed into a single 1-year1\text{-year} calendar.

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<p>Ecliptic Plane</p>

Ecliptic Plane

The flat plane defined by Earth's orbital path around the Sun, relative to which Earth's rotational axis is tilted by 2312o23\frac{1}{2}^\text{o}.

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<p>Expansion of the Universe</p>

Expansion of the Universe

The cosmological process in which space expands uniformly, causing all galaxies outside our Local Group to move away from us at speeds proportional to their distance.