Astronomy Test Flashcards
Astronomer #1
Aristotle
Greek
Geocentric
Syllogism
Epicycles to explain retrograde motion
Astronomer #2
Ptolemy
Egyptian of Greek descent
Geocentric
Epicycles + eccentric Earth + equant to explain retrograde motion
Astronomer #3
Copernicus
Polish
Heliocentric
Epicycles w sun in the middle
Astronomer #4
Tycho Brahe
Danish
Geocentric
Sextant to measure light from planet or star
Astronomer #5
Galileo
Italian
Heliocentric
Jupiter’s 4 moons
Astronomer #6
Kepler
German
Heliocentric
3 laws based on Tycho’s data
Astronomer #7
Newton
British
Heliocentric
Newton’s Law of Universal Gravitation
Astronomer #8
Hubble
American
Heliocentric
Further galaxies recede faster than closer ones
Sun
99.8% of the mass of the solar system
solar wind is charged particles flying off the sun
Sun’s 1st Layer
Core
nuclear fusion - fuse hydrogen to make helium
Sun’s 2nd Layer
Radiative Zone
Sun’s 3rd Layer
Convective Zone
Sun’s 4th Layer
Photosphere
Sun’s 5th Layer
Chromosphere
transition zone
Sun’s 6th Layer
Corona
Mercury
Mariner 10
Venus
Venus Express Mission
Earth
Landsat Satellites
1 moon
Mars
Viking 1
2 moons
Jupiter
Voyager 2
Saturn
Voyager 2
Uranus
Voyager 2
Neptune
Voyager 2
Binary System
2 stars orbit center of mass
Dying Star
shrinks into white dwarf - electron degeneracy
under goes supernova
- neutron star - neutron degeneracy
- black hole - denser core
bigger star to live longer
Chandrasekher Limit
- 1.4x the mass of the sun
- determines the transformation a dying star will go through
Standard Candles
Measure brightness of objects to tell how far they are
Cephid Variable Stars
Brighten and dim periodically - can tell how far away they are
Type 1a Supernova
White dwarf is in binary system and takes mass from the other star - mass exceeds Chandrasekhar limit and can undergo a supernova
Better standard candle than Cephid Variables
Kepler’s First Law
Planets move in elliptical orbits around the sun
Kepler’s Second Law
Planets move equal areas in equal time
Kepler’s Third Law
Major axis in an elliptical orbit
Semimajor axis in an elliptical orbit
Minor axis in an elliptical orbit
Semimajor axis ^3 = period of an orbit ^2