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15 Terms

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Spiral Galaxy

A type of galaxy with a flat, rotating disk that contains stars, gas, and dust, along with a central bulge and spiral arms.

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Elliptical Galaxy

A type of galaxy that ranges from nearly spherical to elongated shapes and contains very little gas and dust, dominated by older, redder stars.

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Irregular Galaxy

A type of galaxy with no definite shape or structure, often resulting from gravitational interactions or collisions.

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Hubble Tuning Fork Diagram

A classification system that categorizes galaxies into spirals, barred spirals, ellipticals, and irregulars.

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Milky Way Galaxy

A barred spiral galaxy containing 100-400 billion stars, about 100,000 light-years in diameter.

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Redshift

The phenomenon where light from a galaxy shifts to longer wavelengths as it moves away, indicating the expanding universe.

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Blueshift

Occurs when a galaxy moves closer, causing its light to shift to shorter wavelengths.

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Hubble’s Law

The law stating that the farther away a galaxy is, the faster it is moving away from us, expressed as Velocity = H₀ × Distance.

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Edwin Hubble

An astronomer who discovered that 'nebulae' were other galaxies and provided evidence for an expanding universe.

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Cosmic Microwave Background (CMB)

Faint radiation left over from the Big Bang, uniform across the sky, supporting the hot, dense early universe hypothesis.

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Dark Matter

Invisible matter that does not emit light or energy, detected through its gravitational effects and helps explain galaxy rotation curves.

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Dark Energy

A mysterious force causing the accelerated expansion of the universe, making up about 68% of it.

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Age of the Universe

Estimated to be approximately 13.8 billion years, determined using Hubble's Law and cosmic background radiation data.

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Dynamic Universe

The concept that the universe evolves over time, with galaxies forming, merging, and changing.

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Gravity’s Role

The force that pulls gas and dust together to form stars and galaxies, determining shapes and motion.