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Science

The concepts behind how the universe works — from subatomic particles to galactic structures, explained clearly.

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Total terms
10
Subcategories
2 min
Avg. read time
29 terms
A
Active Galactic Nucleus
An Active Galactic Nucleus (AGN) is a region at the center of a galaxy that emits a large amount of energy, often outshining the entire galaxy. This energy comes from a supermassive black hole that is actively consuming surrounding matter.
BeginnerAstronomy2 min
A
Asteroid
An asteroid is a small rocky body that orbits the Sun, primarily found in the asteroid belt between Mars and Jupiter. They vary in size and shape, and some can even be several hundred kilometers wide.
BeginnerAstronomy2 min
A
Astronomical Unit (AU)
An Astronomical Unit (AU) is a measurement of distance used in astronomy, defined as the average distance from the Earth to the Sun, approximately 93 million miles or 150 million kilometers. It helps astronomers describe distances within our solar system in a more manageable way.
BeginnerAstronomy2 min
B
Big Bang
The Big Bang is the leading scientific explanation for the origin of the universe. It describes how the universe expanded from an extremely hot and dense state about 13.8 billion years ago.
BeginnerAstronomy2 min
B
Blueshift
Blueshift refers to the phenomenon where light from an object is shifted towards the blue end of the spectrum. This occurs when the object is moving closer to the observer, indicating that the object is approaching.
BeginnerAstronomy2 min
C
Comet
A comet is a small celestial body made of ice, dust, and rocky material that orbits the Sun. When it gets close to the Sun, it heats up and releases gas and dust, forming a glowing coma and sometimes a tail.
BeginnerAstronomy2 min
C
Constellation
A constellation is a group of stars that form a recognizable pattern in the night sky. These patterns often represent animals, mythological figures, or objects and help astronomers navigate and identify stars.
BeginnerAstronomy1 min
C
Cosmic Microwave Background
The Cosmic Microwave Background (CMB) is the faint glow of radiation that fills the universe, a remnant from the Big Bang. It provides crucial evidence for the Big Bang theory and helps scientists understand the early universe's conditions.
BeginnerAstronomy2 min
C
Cosmic Web
The Cosmic Web is a large-scale structure of the universe, consisting of galaxies and galaxy clusters interconnected by filaments of dark matter and gas. It forms a web-like pattern that shapes the distribution of matter in the cosmos.
BeginnerAstronomy2 min
E
Event Horizon
An event horizon is the boundary around a black hole beyond which nothing can escape, not even light. It marks the point of no return for objects that venture too close to the black hole's gravitational pull.
BeginnerAstronomy2 min
E
Exoplanet
An exoplanet is a planet that orbits a star outside our solar system. These planets can vary greatly in size, composition, and distance from their stars.
BeginnerAstronomy2 min
G
Galaxy
A galaxy is a large system of stars, gas, dust, and dark matter, bound together by gravity. They come in various shapes and sizes and can contain billions to trillions of stars. Our solar system is located in the Milky Way galaxy.
BeginnerAstronomy2 min
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Galaxy Cluster
A galaxy cluster is a large group of galaxies held together by gravity. These clusters can contain hundreds or even thousands of galaxies, along with gas and dark matter.
BeginnerAstronomy2 min
G
Gravitational Wave
A gravitational wave is a ripple in spacetime caused by some of the universe's most violent and energetic processes, like merging black holes or neutron stars. These waves travel at the speed of light and were first detected in 2015, confirming a major prediction of Albert Einstein's theory of general relativity.
BeginnerAstronomy2 min
H
Habitable Zone
A habitable zone is the region around a star where conditions might be right for liquid water to exist on a planet's surface. This zone is crucial for the potential of life as we know it, as water is essential for living organisms.
BeginnerAstronomy2 min
H
Hubble Constant
The Hubble Constant is a number that describes how fast the universe is expanding. It measures the rate at which galaxies move away from us, indicating that the farther a galaxy is, the faster it is receding.
BeginnerAstronomy2 min
I
Interferometry
A technique used to measure the properties of waves, especially light, by combining signals from multiple sources. It helps in enhancing the resolution of images and understanding astronomical phenomena.
BeginnerAstronomy2 min
K
Kepler Mission
The Kepler Mission was a NASA space telescope project designed to discover Earth-like planets orbiting other stars. It used a technique called transit photometry to detect dips in brightness caused by planets passing in front of their host stars.
BeginnerAstronomy2 min
L
Light Year
A light year is a unit of distance that measures how far light travels in one year. It is commonly used in astronomy to express vast distances in space.
BeginnerAstronomy2 min
M
Main Sequence
The Main Sequence is a stage in a star's life cycle where it fuses hydrogen into helium in its core. This process generates energy that makes the star shine steadily for millions to billions of years, depending on its mass.
BeginnerAstronomy2 min
M
Meteorite
A meteorite is a solid fragment of a meteoroid that survives its passage through the Earth's atmosphere and lands on the surface. These objects can provide valuable information about the early solar system and the formation of planets.
BeginnerAstronomy2 min
M
Milky Way
The Milky Way is a large spiral galaxy that contains our solar system, along with billions of other stars and their planets. It is shaped like a flat disk with a central bulge and is part of the universe we observe.
BeginnerAstronomy2 min
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Moon
The Moon is Earth's only natural satellite, orbiting our planet and providing light at night. It plays a crucial role in influencing tides and has been a source of fascination for humans throughout history.
BeginnerAstronomy2 min
M
Multiverse
The Multiverse is a theoretical concept suggesting that our universe is just one of many universes that exist simultaneously. These universes may have different physical laws, dimensions, and properties, creating a vast and diverse reality beyond our own.
BeginnerAstronomy2 min
N
Nebula
A nebula is a large cloud of gas and dust in space, often serving as a nursery for new stars. They can also be remnants of dead stars, showcasing beautiful colors and shapes.
BeginnerAstronomy2 min
N
Neutron Star
A neutron star is a type of astronomical object that forms when a massive star collapses after a supernova explosion. It is incredibly dense, with a mass greater than that of the Sun packed into a sphere only about 20 kilometers wide.
BeginnerAstronomy2 min
P
Parallax
It is a method used to measure distances to objects in space by observing their apparent movement against a distant background. This effect occurs when an observer changes position, creating a shift in the perceived location of the object.
BeginnerAstronomy2 min
P
Parsec
A parsec is a unit of distance used in astronomy to measure how far away stars and galaxies are from Earth. One parsec is equivalent to about 3.26 light-years, which is the distance light travels in one year.
BeginnerAstronomy2 min
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Planet
A planet is a large celestial body that orbits a star, such as the Sun, and does not produce its own light. Planets are made up of various materials and can have different atmospheres, surfaces, and temperatures.
BeginnerAstronomy1 min