Term
|
Definition
|
|
Term
Sun's distance to Jupiter |
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
~ 3,000,000 Km/s or 1,080 X 10^6 Km/h |
|
|
Term
How long ago was the Big Bang? |
|
Definition
13.5-14 billion years ago |
|
|
Term
Ancient civilizations used astronomy for: |
|
Definition
-timekeeping -tracking seasons -calendar -monitoring planets and stars -predicting eclipses |
|
|
Term
Who thought up the first Geocentric idea? |
|
Definition
|
|
Term
Greek astronomers with geocentric idea |
|
Definition
|
|
Term
|
Definition
the loops the planets make in there orbit around the sun. -seemed to go forward and backwards |
|
|
Term
|
Definition
Circles around circles. -explained retrograde motion |
|
|
Term
|
Definition
proposed sun-centered model (heli-centric) |
|
|
Term
|
Definition
thought perfect circles weren't the answer and devised a set of 3 laws |
|
|
Term
|
Definition
1. Law of orbits 2. Law of areas 3. Law of period |
|
|
Term
|
Definition
The orbit of every planet is an ellipse with the Sun at one of the two foci. |
|
|
Term
|
Definition
A line joining a planet and the Sun sweeps out equal areas during equal intervals of time.[1] |
|
|
Term
|
Definition
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. |
|
|
Term
|
Definition
used telescope and discovered: -Jupiter's moons -phases of Venus -Saturn's rings -Milky way |
|
|
Term
|
Definition
Realized force that hold moon in orbit is gravity. |
|
|
Term
Newton's law of Universal Gravity |
|
Definition
centrally acting force stops planets from continuing in straight lines |
|
|
Term
|
Definition
Low earth orbit. requires 28,800 km/h |
|
|
Term
|
Definition
Geo-stationary earth orbit. require 36,000 Km/h |
|
|
Term
|
Definition
|
|
Term
what way does earth rotate? |
|
Definition
it rotates same direction of its orbit (counter clock wise when viewed from north pole) |
|
|
Term
Mass of planets and sun % |
|
Definition
Planets = ~0.15% Sun = 99.85% |
|
|
Term
Is our universe expanding? |
|
Definition
Yes. all planets and stars are moving farther apart. |
|
|
Term
Sun's Distance to Kuiper Belt |
|
Definition
|
|
Term
Sun's distance to oort cloud |
|
Definition
|
|
Term
which way do all the planets orbit? |
|
Definition
|
|
Term
what planets have a different axis tilt? |
|
Definition
|
|
Term
Characteristics of terrestrial planets |
|
Definition
rocky and small no or few moons no rings |
|
|
Term
characteristics of Jovian planets |
|
Definition
Gaseous and big rings many moons |
|
|
Term
|
Definition
large body of small objects orbiting the sun. (past Neptune) ~ 30-50 AU from sun |
|
|
Term
2 Hypothesis for formation of solar system |
|
Definition
1. Gravitational collapse of nebula. 2. Close encounter of sun with another star |
|
|
Term
gravitational collapse hypothesis |
|
Definition
huge cloud of material is disturbed (supernova?) |
|
|
Term
formation with gravitational collapse |
|
Definition
1. heating = protostar (dense materials collide) 2. Spinning = smoothing (making materials compact more) 3. flattening = protoplanetary disk (make chaotic motion into orderly movement) |
|
|
Term
what happens after protoplanetary disk cool? |
|
Definition
condenses into planetesimals -made of 98% helium and hydrogen |
|
|
Term
where is the frost line located? |
|
Definition
|
|
Term
where is the frost line located? |
|
Definition
|
|
Term
|
Definition
process where small "seeds" grew into planets |
|
|
Term
small planetesimals and large planetesimals shapes |
|
Definition
small = any kind of shape large = spherical due to gravity |
|
|
Term
why can't terrestrial planets capture gas? |
|
Definition
Their gravitation pull is too weak or gas was blown away by solar winds |
|
|
Term
|
Definition
comet tails always point away from sun and SOHO (solar and heliospheric observatory) |
|
|
Term
solar wind effects on planet formation? |
|
Definition
winds blow away gases in planetary nebula ending up with formation of planets. |
|
|
Term
|
Definition
take material from beyond frost line forming small accretion disk. abundant supply of gases create larger planets |
|
|
Term
why are planets farther from the sun bigger? |
|
Definition
larger amounts of gas available past frost line opposed to small amount of metal and rock within frost line. |
|
|
Term
|
Definition
-rocky leftovers from planetesimals. -concentrated in asteroid belt between Mars and Jupiter |
|
|
Term
|
Definition
Icy leftover planetesimals beyond orbit of Neptune |
|
|
Term
effects of impact and capture (asteroids comets) |
|
Definition
comet shoemakers with Jupiter -surface of the moon/mercury -tilt axis of planets (Venus, Uranus) -exchange of material -creates satellites -killed t-rex :( |
|
|
Term
|
Definition
may've been giant impact between earth and planetesimals -Phobos and Deimos (captured asteroids?) |
|
|
Term
|
Definition
potassium decays to argon relative amount of K^40 to Ar^40 dates rock. |
|
|
Term
how old is the solar system (approx) |
|
Definition
|
|
Term
|
Definition
1. energy for photosynthesis 2. green house effect keeping earth warm |
|
|
Term
|
Definition
Stellar nebula -> massive star -> red giant -> supernova ->neutron star/black hole OR stellar nebula -> average star -> red giant -> planetary nebula -> white dwarf |
|
|
Term
what kind of star do we have? |
|
Definition
main sequence star 1-10 Rsun |
|
|
Term
|
Definition
process of spitting atomic nucleus. power plants split big atoms like uranium to smaller ones |
|
|
Term
|
Definition
process of combining fusing) small atoms into larger ones |
|
|
Term
how does sun get its energy? |
|
Definition
Increased temp at center of sun due to gravitation contraction triggered Nuclear fusion |
|
|
Term
|
Definition
where fusion takes place (temp ~15 million K) |
|
|
Term
|
Definition
Energy transported outward traveling though this region (temp ~10 million k) |
|
|
Term
|
Definition
energy transported through convection (lava lamp) |
|
|
Term
|
Definition
if core temp drops, it contracts forcing it to heat up again heating of core causes fusino rate to rise forcing core to expand and cool again |
|
|
Term
|
Definition
visible layer of sun. radiation originates from here (temp ~5800K) |
|
|
Term
|
Definition
type of elementary particles with very low mass. produced during fusion reactions very difficult to detect |
|
|
Term
|
Definition
Chromosphere is 200Km above photosphere (temp ~5800-20,000 K) |
|
|
Term
|
Definition
light rays above atmosphere (temp 1-2 million K) can reach 8-10 million K) |
|
|
Term
|
Definition
cells on sun's surface. dark = cold spots. light = hot spots |
|
|
Term
|
Definition
Dark cooler features on sun (4000 K) strong magnetic field |
|
|
Term
|
Definition
magnetic activity causes flares send bursts of x rays and charged particles outwards |
|
|
Term
|
Definition
burst of energy charged particles outwards (related to flares) |
|
|
Term
Flare and Coronal Mass Ejections effects on earth |
|
Definition
bombard earth with high energy particles. aurora borealis knock out communications |
|
|
Term
|
Definition
50 year period (1650-1700) -average temp dropped by 1-2 degrees -result of sun spot number |
|
|
Term
how many planets reside in sun's orbital plane |
|
Definition
7 planets lie within 3 degrees of sun's equator |
|
|
Term
|
Definition
Venus and Earth Saturn and Jupiter Neptune and Uranus |
|
|
Term
How do we measure planet masses? |
|
Definition
using kepler and newton laws -measure gravitational pull |
|
|
Term
how do we measure their density? |
|
Definition
once mass and volume found we calculate D = Mass/volume |
|
|
Term
which planet is the most dense? |
|
Definition
|
|
Term
planets with magnetic field also have these 3 things |
|
Definition
1. electrically conduction material within it 2. material is slowly circulating 3. has two internal layers composed of solid layer inside liquid one |
|
|
Term
internal structure of earth |
|
Definition
1. core - high density 2. mantle - medium density rocky material 3. crust - low density rocks |
|
|
Term
|
Definition
coolest most ridig layer of rock near planets surface |
|
|
Term
internal structure of Jovian planets |
|
Definition
magnetic fields indicate electrically-conducting material circulating. massive with low density |
|
|
Term
3 methods planets gain internal heat |
|
Definition
1. kinetic -movement 2. Gravitational - energy pulls material down impacting 3. radioactivity - releasing thermal energy |
|
|
Term
|
Definition
1. conduction -atoms vibrate slowly 2. convection - lava lamps 3. radiation - protons carry energy away from object |
|
|
Term
|
Definition
all small bodies: asteroids, comets, moons, mercury, modern mars |
|
|
Term
|
Definition
volcanism moving mantle pushes up molten material |
|
|
Term
solid convection causing no crustal break up |
|
Definition
|
|
Term
Solid convection causing crustal break up |
|
Definition
movement creates new material earth is only terrestrial body with this earthquakes and volcanoes |
|
|
Term
|
Definition
very dense no atmosphere. highlands and terrains. orbits quickly |
|
|
Term
|
Definition
covered in thick CO2 clouds Temp 480 C thick atmosphere volcanic features |
|
|
Term
|
Definition
surface temp 16 C atmosphere only place with life liquid water |
|
|
Term
|
Definition
more dense than water moonquakes Maria (dark lowlands) highlands, craters |
|
|
Term
|
Definition
CO2 atmosphere like earth's volcanoes and canyons water and methane moons Phobos and Deimos |
|
|
Term
|
Definition
giant red spot (cyclonic storm) many moons no solid surface. mostly H/He |
|
|
Term
|
Definition
rings (not solid orbiting like tiny moons) dynamic atmosphere many moons |
|
|
Term
|
Definition
|
|
Term
|
Definition
dynamic atmosphere (windiest) ice and volcanic activity 8 moons |
|
|
Term
|
Definition
has moon elongated orbit comet like composition |
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
rocky planetesimals that didn't accrete Jupiter gravity messed with orbit and prevented accretion |
|
|
Term
|
Definition
chunk of rock less than meter orbiting sun |
|
|
Term
|
Definition
rock that falls to earth through atmo to surface |
|
|
Term
|
Definition
bright tail left by meteorite |
|
|
Term
|
Definition
unchanged in composition since first formation -stony or carbon rich -stony: made of rocks with shiny metal -carbon: rock with dark carbon compounds + whiteish spheres |
|
|
Term
|
Definition
unchanged in composition since first formation -stony or carbon rich -stony: made of rocks with shiny metal -carbon: rock with dark carbon compounds + whiteish spheres |
|
|
Term
|
Definition
having experienced volcanism or differentialtion. Rocky or metal rich -rocky:resemble volcanic rocks -metal: made of iron. came from shattered asteroid |
|
|
Term
|
Definition
formed beyond frost line core dirty snowball have tails |
|
|
Term
|
Definition
coma - atmosphere that coes from comets heated nucleus plasma tail - gas escaping from coma dust tail - pushed by photons |
|
|
Term
what causes meteor showers? |
|
Definition
comets ejecting small particles that follow and come around earth orbit |
|
|
Term
consequence of large impact on earth |
|
Definition
bass surge (like volcanic river of gas) huge amounts of dust vaporize water hypercanes global tsunamis acid rain crop failure mass extinction |
|
|
Term
when was earth last impacted by comet/meteor |
|
Definition
65 million years ago. (dinosaurs) |
|
|
Term
|
Definition
~10 km across in Chicxulub Mexico |
|
|
Term
|
Definition
systematic survey to observe and track object that might approach earth. from 0-10 |
|
|