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Astro final
Astro final
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141 Terms
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Star these 141
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Star System
is a star ( or stars) and any object or plants that orbit around it
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Star
Is a large sphere of gas that generates heat and light through nuclear fusion in its core
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Planet
A spherical thing that orbit a star and has clear its orbit of smaller objects
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Dwarf Planet
basically like a planet but hasn't cleared its orbit
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Moons/Satellites
objects the orbit a planet
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Asteroid
a small rocky object that orbits a star
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Comet
small icy object that orbits a star
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Galaxy
a large collection of millions and billions of stars all orbiting the same center of gravity
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Cluster
group of galaxies
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Galaxy Cluster
is a collection of tens of thousand of galaxies all held together by gravity
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Galaxy Supercluster
is a large collection of tens of thousands of galaxy clusters held together by gravity
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The Universe
is everything that ever was, is, or will be
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Astronomical Unit (AU)
the average distance between the earth and the sun, 149,600,000
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Light Pollution
is scattered, manmade light which outshines dim light from celestial objects
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Asterism
is a pattern formed from brings stars
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Constellation
region of the night sky; every star inside the boundaries belong to the constellation; there are 88 constellation
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The Celestial Sphere
is the imaginary bubble surrounding the earth on which all celestial objects appear
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Ecliptic
is the apparent path of the sun around earth
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The Celestial Equator
the midway b/w the horizon and overhead point in the celestial sphere
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Altitude
is the degree above the horizon
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Direction
is the location in regards to north south east or west
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Zenith
is the point directly above the observer at an altitude of 90 degree
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North Celestial Pole
the path earth rotates around
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Circumpolar Star
stars that are always visible in the sky; they never set
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Right Ascension
Measure degrees east to west of the vernal equinox
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Declination
measures degrees north to south of the celestial equator
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Vernal Equinox
is the point where the path of the sun crosses the celestial equator
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Arcminute
is 1/60th of a degree on the sky
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Arcsecond
is 1/60th of an arcminute
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Solstice
when earth is tilted directly towards or away from the sun
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Equinox
hallway b/w solstices when the earth switches from pointing away to pointing towards the sun
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Speed
how far in a certain amount of time
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Velocity
both the speed and the direction
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Acceleration
change in velocity
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Vacuum Chamber
a chamber where there is no air resistance or friction
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Mass
how much stuff makes up an object
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Weight
the force of gravity pulling on an object
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Momentum
mass times velocity
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Net Force
overall force acting on an object
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Newtons Second Law of Motion
f=ma
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Momentum
can be exchanged b/w objects but the total amount stays the same
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Angular momentum
can be exchanged b/w objects , but the total amount stays the same if there are no net torques
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Perihelion
point in a planet's orbit that is closest to the sun
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Aphelion
point in a planet's orbit that is furthest from the sun
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Eccentricity
how squashed the elliptical orbit is, closer to 1 is unbound, closer to 0 is circle
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The Geocentric Model
earth centered model
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Model
is a conceptual representation
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Theory
is a testable explanation for many observations and experiments
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Retrograde Motion
earth is faster than mars in the orbit, when passing mars, it appears to slow down, move backwards then forward
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Epicycles
are circles on circles, the movement in a solar system
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Heliocentric Model
sun centered solar system, but not the center of the universe
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Astronomy
actual science
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Photons
particles of light
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Particle-wave duality of light
light behaves both as particle and a wave simultaneously
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Lens
curved material that refracts and focuses light
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CCDs
Sensitive detectors od photons
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Angular Resolution
measure of the sharpness and clarity of an image
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Spectrograph
disperses light and records it on a detector
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Spectral Resolution
the sharpness of detail that can be seen in a spectrum
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Light curve
a plot of brightness versus time
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Seeing
a measure of celestial objects blurring due to the atmosphere
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Adaptive optics
corrects the scrambles of incoming light waves
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Spring Tide
moon closest to the earth's orbit in alignment with the sun
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Neap Tide
moon closest to the earth's orbit but not in alignment with the sun
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Tidally locked
the time it takes for the moon to complete 1 full orbit around the earth is = the time it takes for the moon to rotate around itself
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Lunar eclipse
Moon passes into earth's shadow
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Umbra
full shadow
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Penumbra
partial shadow
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Solar Eclipse
moons casts a shadow onto the earth
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Seismology
is the study of seismic waves and how they change to learn about the earth's interior
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Mantle
medium density rock
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Crust
low density rock
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Lithosphere
solid lawyer of rock
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Conduction
heat flows from warm areas to cold areas
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Radiation
heat is released as light
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Erosion
gradual breakdown or transport of rock
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Scarp
crack caused by settling as a worm planetary body cools
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Regolith
fine powder of pulverized rock covering the moon's surface
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Subduction Zone
dense seafloor crust is shoved under lighter continental crust and recycled
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Ridge
seafloor spending pulls apart the crust , allowing material to rise up and cool to form new crust
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Hot spot
plume of hot mantle material
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Great Red Spot
located in Jupiter
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Orbital Resonance
recurring gravitational interaction usually due to orbits related by a ratio
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Shepherd Moons
a pair of moons that keep a ringlet sharp and narrow
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Nebular Theory
solar system is formed in a collapsing gas cloud
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Nebula
region of gas and dust
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Solar Nebula
region of gas and dust out of which the solar system formed
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Planetesimals
planet pieces
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Protoplanetary Disk
partially collapsed region of gas forming a stellar system
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Hydrostatic Equilibrium
the balance of the tow Maine forces of the sun, outward force of radiation, inward force of gravity
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Core
energy generated by photons buy fusing hydrogen atoms into helium
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The Radiation Zone
region where energy is transported by the radiative force of photons from the core
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The Convection Zone
region where energy is transported upward by convection
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The Photosphere
the visible surface of the sun
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The Chromosphere
beginning of the sun's atmosphere
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The Corona
outermost layer of the sun's atmosphere
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The Solar Wind
a flow of charged particle from the surface of the sun
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Fusion
nuclei combine to form a new atom
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Fission
the splitting of nuclei into smaller atoms
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Sunspots
are cooler areas on the sun's surface
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