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Cassini divide:
- 1. largest division between some of the rings
- 2. space caused by gravity of moon mimas
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Roche limit
1. minimum radius at which a satellite may orbit without being broken apart by tidal forces
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Uranus characteristics
- 1.small angual size
- 2. 4 times the diameter of earth
- 3. no core
- 4. methane in atmosphere makes planet blueish-green
- 5. 10 thin rings,
- 6.retrograde motion bc of its obliquity
- 7. orbital period of 84 yrs
- 8. voyager 2
- 9. shepard moon
- 10. somewhat larger denisty than uranus
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Triton
Neptune's largest moon; only major moon to revolve around a planet in a retrograde direction
Will crash onto Neptune in future
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who was pluto discovered by
clyde tombaugh in 1930
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what was used to discover pluto
blink comparator
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pluto
- 1. 17 degree tilt to ecliptic
- 2. methane atmosphere
- 3.moon-- Charon
- 4. pluto 1/5 our moon
- 5. small and ecentric orbit: thus maybe a former moon of Neptune
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Piazzi
Discorvered asteroids in 1801
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asteroids
- known as minor planets
- ceres is the largest asteroid
- Pallsa and Vesta have diameters greater than 300 km
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asteroid belt
asteroids that orbit the sun at distanc eof 2.2-3.3 aU
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apollo asteroids
50 asteroids with diameters lager than 1 km tat have eccentric orbits that cross the Earth's orbit
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Kirkwood Gap
gaps between asteroids in asteroid belt; due to synchronous tugs from Jupiter on the asteroids which used to be located there
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trojan asteroids
two groups of asteroids which are located at Jupiter's distance from the Sun
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The orgin of the asteroids
Asteroids are primordial material that never formed into a planet because of Jupiter's gravitational influence
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Edmund Halley
- Used Newton's methods to calculate orbits of many coments
- corrently predicted next return of what would become Comet Halley
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Parts of a comet
- 1. Head: consists of coma and nucleus
- 2. coma: part of comet's head made up of a diffuse cloud of gas and dust
- 3. Nucleus: comet is solid chunk of a comet, locatd in the head
- 4.tail: gas and/or dust that is swept away from comet's head.
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Ion tail v. Dust tail
- 1. Ion tail: is a straight tail
- 2. dust tail: curved tail
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what is the nucleus of a comet like
a dirty snowball (water, ice, frozen carbon dioxide, and small grains
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how comet "dies"
gradual evaporation of their nuclei
trhough evaporationof all volatile material
falling into the sun
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Jan Oort and the Oort cloud
jan: proposed comet cloud exists in a spherical shell
these billion of comet nuclei exist in Oort cloud
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Kuiper belt
band of comets and dwarf planets that exists closer to the solar system than the oort cloud
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scattered disk
third source of commets (beside kuiper belt, oort cloud) iwhich is larger than Kuiper belt and smaller than Oort cloud
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three different meteroid sizes
- 1. smallest meteoroids slowed down at top of Earth's atmoshpere---> micro meteorites
- 2. streak in sky from dust grain sized meteroid is heated up by passage through earth's atmoshpere--> meteor
- very brigh meteorr--> fireballs
- 3. Largest meteoroids: able to pass through Earth's atmosphere
meteorite: meteroid after it passes through atmosphere
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radiant
point in the sky from which the meteors of a shower appear to radiate
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three categories of meteorites
1. irons: iron meteorites that are made up of 80%-90% (with some nickel)
2. Stones: stony meteorites that can contain flakes of iron and nickel
3. Stony irons: meteorites that are half stone and half iron
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Sun characteristics
- 1. is a G2 star, that is the main sequence phase of its life
- 2. in 5 billion yrs will become red giant star
- 3. has differential rotation like outer planets
- 4.
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solar constant
1.solar energy striking earth at the rate of 1,380 watts
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solar luminosity
total rate at which sun releases energy into space in all directions
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solar limb
edge of solar disk
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limb darkening
how solar disks look dimmer near their edges,
proof that the temperature decreases with increasing height within the sun's photosphere
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granulation
divison of the sun's surface into small convection cells
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granules
areas where hot material is rising from below and then descending
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what is the chemical make up of the photosphere
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sun's core
must hold more helium than the photosphere since some of hydrogen that was there has already been converted into helium during lif eof the sun
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chromosphere
region of the solar atmoshpere 2,000-3,000 km thick
lies between photosphere and corona
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transition zone
directly above the chromophere, 200 km thick,
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spicules
narrow jets of gas which are part of the chromosphere but exted through the transition zone into the corona
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solar corona
portion of the solar atmoshpere only visible during a total solar eclipse
above the transition zone
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How is the chromosphere heated?
1. shockwaves: produced in solar interior and dump their energy in the corona
2. magnetic reconnection heating: changes in coronal magnetic field
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coronal holes
large dark area in the corona
are cooler than the surrounding corona
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solar wind
continous flow of nuclei and electrons from the sun
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thomas harriott
first person after Galileo to report sunspots
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sunspots
1500 degrees coller than surrounding photosphere
locations where sun's magnetic field passes from its interior through the photosphere into the atmoshpere
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Zeeman effect
measures the sun's magnetic field, by splitting spectral lines by a strong magnetic field
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solar maximum and minimum
maximum: tie when most sunsposets are visjible on solar surface
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