Galaxies and Dark Matter

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Flashcards covering key concepts related to galaxies, dark matter, and methods for measuring distance in the universe.

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15 Terms

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Spiral Galaxy

A type of galaxy characterized by a flat disk and spiral arms, where stars orbit the center in the same direction.

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Elliptical Galaxy

A galaxy with an egg-shaped structure and stars that orbit in all directions.

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Irregular Galaxy

Galaxies that do not fit into spiral or elliptical classifications, often due to interactions with other galaxies.

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Milky Way Galaxy

A barred spiral galaxy approximately 100,000 light-years across, where our solar system is located about 27,000 light-years from its center.

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Distance Ladder

A series of methods used by astronomers to determine distances to celestial objects, building upon each other.

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Supermassive Black Hole

A massive black hole, often found at the center of galaxies, exhibiting significant gravitational influence.

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Active Galactic Nucleus (AGN)

A region at the center of a galaxy that is extremely bright due to gas accreting onto a supermassive black hole.

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Dark Matter

A type of matter that does not emit light and can only be detected by its gravitational effects on visible matter.

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Luminous Matter

Matter that emits or reflects light, making it detectable through observations.

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Gravitational Lensing

A phenomenon where the gravitational field of a massive object distorts the light from a distant object, making it appear brighter.

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MACHOs

Massive Compact Halo Objects, a category of potential dark matter candidates, including objects like black holes and neutron stars.

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WIMPs

Weakly Interacting Massive Particles, another category of hypothetical dark matter candidates.

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Rotation Curve

A plot of the rotation velocity of stars in a galaxy versus their distance from the galactic center.

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Standard Candles

Astronomical objects with known luminosities used to gauge distances in the universe.

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Globular Clusters

Spherical collections of stars which can be used to measure distances through variable stars.