Astronomy Vocabulary Cheat Sheet

A Education › Astronomy cheat sheet in English by sayuri_3

Revision Sheet by Amber for 9H 2021, Unit 6.2-6.5 Astronomy Portfolio

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6.2 Galaxies - Vocabulary

Star
A giant ball of hot, glowing gases (usually hydrogen & helium)
Nuclear Fusion
A process where the nuclei of atoms join and emit energy as light, heat and other electr­oma­gnetic radiation.
Apparent Magnitude Scale
A measur­ement of a celestial object­'s brightness when viewed from Earth (the more positive the number the dimmer the star).
Absolute Magnitude Scale
A measur­ement of a celestial object­'s brightness if viewed from the same distance; a measure of a celestial object­'s actual brightness or luminosity.
Hertzs­pru­ng-­Russel Diagram (HR)
A graph that plots a star's temper­ature on the x-axis and absolute magnitude on the y-axis.
Main Sequence
A diagonal band most stars fall into when plotted on the HR Diagram..
Speed of Light
Light travels at 300,000 km/s.
Light-Year
The distance that light travels in a year (9,500­,00­0,0­00,000 km).
Parsec
Approx. 3.26 light-­years.
Parallax
The effect where an object appears to move when viewed from two different positions.
Galaxy
A group of stars held together by their gravity, galaxies form three shapes, ellipt­ical, spiral and irregular.
Conste­llation
An imaginary picture in the night sky made up of stars.

6.3 Life Cycle of a Star - Vocabulary

Nebula(e)
A cloud of gas and dust held together by the gravity of the hydrogen atoms within it.
Protostar
When the center of a nebula heats up and pressure increases.
Hydros­tatic Equili­brium
The balance of the forces of a star's gravity and energy output.
Red giant
Hydrogen decreases, gravity is stronger than energy output, a new type of nuclear fusion begins, releasing more energy, reaching a new hydros­tatic equili­brium and cooling to red.
Planetary Nebula
Helium supply decreases in a red giant and the outer region fades to a shell.
White Dwarf
The core of a planetary nebula continues nuclear fusion, increases energy rate and temper­ature to get a small, white hot star.
Black Dwarf
The result of a white dwarf cooling and fading away.
Red Supergiant
A contin­uation of the red giant until iron is formed, resulting in a much larger, red star.
Supernova
The event where a red supergiant runs out of energy and collapses, resulting in a large explosive death.
Neutron Star
The aftermath of a supernova with a mass of less than 3 solar masses, an incredibly dense star with a diameter of only tens of kilome­ters.
Black Hole
The result of a supernova with a mass greater than 3 solar masses, a region of space with an extrao­rdinary gravit­ational pull and density that even light cannot escape.

6.4 Moving Galaxies

Absorbtion Spectrum
A spectrum with lines missing from the pattern due to elements of the star absorbing their light wavele­ngths, therefore removing them from the spectrum.
Emission Spectrum
The pattern of wavele­ngths (or freque­ncies) that appear as coloured lines on a spectr­ascope; the light wavele­ngths that are emitted from certain gases when they return to a stable state.
Doppler Effect
The effect that occurs when an object is moving slower than the speed of sound; waves in front of the object compress while waves behind disperse.
Red Shift
An increase in wavelength of radiation emitted by a celestial body which shifts the absorption spectra in the red direction of the spectrum, indicating that the object is moving away from the Earth.
Blue Shift
A decrease in wavelength of radiation emitted by a celestial bosy which shifts the absorption spectra in the red direction of the spectrum, indicating that the object is moving towards the Earth.
Huibbl­e's Law
The further the galaxy, the higher the tendency to have a more red-sh­ifted spectra; the ffurther the galaxy, the faster it was moving away.
Big Bang Theory
the theory that the universe began from a hot dense state which has continued to expand and will continue to do so.

6.5 The Big Bang Theory

Singul­arity
A single, dense, hot point.
Cosmic Microwave Background Radiation
A form of electr­oma­gnetic radiation in the microwave spectrum left over from the formation of the Universe; evidence of the Bug Bang theory.

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