Unit 2: Stars, Nebular Hypothesis and Impacts

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36 Terms

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Asteroid

A solid, rocklike mass that revolves around the sun. originate & typically orbit within region between Mars and Jupiter.

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Black Dwarf Star

The remains of a white dwarf star after it has expended all of its energy

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Black Hole

A point in space with a gravitational field so strong that not even light can escape. Created by the explosion of the most massive stars.

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Comet

a mass of rock, ice, dust, and gas traveling around the sun usually in a highly eccentric orbit. most originate from region beyond Neptune

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Conservation of Angular Momentum

The law of physics stating that the total amount of angular momentum in an isolated system remains constant. Cam=Mass x Width x velocity

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event horizon

the location around a black hole where the escape velovity equals the speed of light; the boundary of a black hole

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exoplanet

A planet outside of our Solar System.

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gas pressure

the outward pressure exerted by gas in a star as it is heated by fusion in the core

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Kuiper Belt

A region outside the orbit of Neptune where most short-period comets are thought to originate

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Light Year

The distance that light travels in a year, about 9.5 trillion kilometers

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Meteor

the light a meteoroid creates as it passes through Earth's atmosphere

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Meteorite

The part of a meteoroid that survives its trip through the atmosphere and strikes Earth's surface

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Meteoroid

Umbrella term for all fragments that travel through space and sometimes our atmosphere

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Milky Way Galaxy

the galaxy that contains our solar system. Spiral shaped with at least 3 arms, billions of stars in a disk 100,000 ly across and 10,000 ly thick at the galactic bulge center

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Nebula

A large cloud of dust and gas in space

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Neutron Star

The very small, very dense core of a massive star, left behind after a supernova.

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Planet

A celestial object that revolves around the sun, is a spheroid, and has cleared most of its orbit of large debris

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Planetary Accretion

The process by which planets grow through collisions and sticking due to gravity and chance. From planetary embreyos to planetessimals to protoplanets to true planets.

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Planetary Nebula

The expanding shell of gas that is escaping a dying, Sun-like (medium mass) star.

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Protostar

The piled up mass that has been pulled together by gravity at the center of a nebula. It has not yet undergone nuclear fusion.

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Red giant

The stage in the life cycle of a sun-like mass star during which the star increases in size and begins to fuse helium in its core.

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Red Supergiant

The stage in the life cycle of a massive star during which the star increases in size and begins to fuse helium in its core.

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Spagettification

The theory that you will become a long, thin stream of atoms, kilometers in length, but narrower than a hair wide when you get pulled into a blackhole

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Star

A mass of incandescent gas, where a balance exists between the nuclear reactions pushing outward from the interior and the gravitational forces pushing inward.

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Super Nova

Brilliant burst of light that follows the collapse of the core and explosion of a massive star

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Terrestrial Planet

Earth-like planets: Mercury, Venus, Earth, Mars

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Tunguska

Siberian site where an asteroid struck in 1908 with the power of 1000 atomic bombs

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Virgo Supercluster

The super cluster of galaxies of which our local group is a member. Contains roughly 2000 galaxies

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White Dwarf

a small, very dense star the size of earth that remains after a middle or low mass star runs out of fuel and is collapsed by gravity

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Walter Alvarez

A scientist who proposed that a large meteorite hit the earth in the Yucatan area of Mexico around 65 million years ago causing the extinction of the dinosaurs

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Iridium

An element that is rare on Earth but common in meteorites.

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Chixulub

Crater that is located in Yucatán peninsula from asteroid responsible for dinosaur extinction.

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Differentiation

The separation of material based on their density

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fusion

the process of two atoms coming together under tremendous pressure to form a new atom. 2 Hydrogen atoms fusing to make a Helium atom

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extinction

Definition: When 100% of a species dies, not even one member survives

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Mass Extinction

at least 66% of all species go extinct