HPS Atsonomy (Unit 9)

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44 Terms

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Hipparchus
First recorded start maps
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Ptolemy
Geocentric model of solar system
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Copernicus
First heliocentric model of solar system
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Brache
Incredible observations
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Kepler
Laws of planetary motion
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Galileo
First to utilize the refractive telescope
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Newton
First reflective telescope
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Hubble
Observed redshifts of galaxies (close or far)
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Penzias and Wilson
Discovered CMB (Cosmic Microwave Background)
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Hipparchus, Ptolemy, Copernicus, Brache, Kepler, Galileo, Newton, Hubble, and Penzias and Wilson
Order of old white male astronomers
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Sextant
Instrument that measures angle of stars
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Parallax
Apparent motion of star to observers position
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Retrograde Motion
When planets appear to move backwards in the sky compared to stars
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Reflector Telescope
Mirror based
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Refractor Telescope
Lense based telescope
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Spectroscope
Breaks down wavelengths of visible light
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Space Probes
Robotic spacecraft sent to explore space (no human)
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Declination
Celestial Latitude Coordinates (Northern star = 90 degrees)
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Right Ascension
Celestial Longitude Coordinates
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Ecliptic
The path the sun takes in the sky (rises in east/sets in west)
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Zenith
90 degrees above the observer’s head (north pole = north star)
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Altitude
How high the star is above the horizon (one first = 10 degrees)
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Azimuth
Direction the star is in (N=0 degrees, S = 180 degrees, etc)
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Paths of celestial bodies
Very ovally and not round!
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Constellations
Groups of stars which appear close together from Earth to form a recognizable shape
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S, M, V, E, M, AB, J, S, U, N, KB, and OC
Order of solar system
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Keplers Law
All orbits are ellipticsl, equal time = equal area, year is affected by distance from sun
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Semi-major Axis
The distance planets are from the sun
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Magnitude
how bright a star appears (related to brightness)
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Temperature
Average Kinetic Energy
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Brightness
Power per unit area (W/m^2)
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Luminocity
Power of a star
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Composition of a Star
Hydrogen and Helium
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Star Sequence
Nebula, Protostar, Main Sequence Star, Red Giant, Super Red Giants (split after that)
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Astronomical Distances (smallest to largest)
Astronomical Unit, Lightyear, Parsec, Megaparsec
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Steady State Theory
The universe looked the same the whole time and won’t change with time
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Hubble’s Constant
As things are farther away, the larger the shift in the color spectrum and faster they move
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Redshift
When a galaxy is far away and appears more red
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Cosmic Microwave Background
Leftover micro radiation left over from the big bang
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Closed Universe
“Big Crunch” and gravity wins
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Flat Universe
“Critical Density” and the universe never dies
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Open Universe
“Big Freeze” and gravity loses
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Inflationary Universe
“Big Rip” and gravity loses
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Critical Density
All the forces in the universe stay the perfect ratio and the universe continues forever