W2 SOLAR SYSTEM Flashcards
ORBIT
Orbits result from a balance between gravity pulling inward and momentum of the object
KEPLER’S 1ST LAW
- planets move in ellipses with the sun at one focus
KEPLER’S 2ND LAW
- Speed of orbit varies in relation to distance from the sun
- Orbits are much faster closer too the sun, and much slower far from the sun.
KEPLER’S 3RD LAW
*Time period of orbit(how long a planet completes full orbit) is related to the distance from the sun
* Outer planets take longer to orbit vs inner planets are faster
ECCENTRICITY
*Eccentric orbits are long thin ellipses in which the largest diameter is very much greater than the smallest diameter
* The length of the long axis in relation to the length of the short axis of an ellipse; a measure of the difference between the ellipse and a perfect circle.
NUCLEAR FUSION
- The sun uses nuclear fusion for its continuous energy source
○ Releases 4hydrogen atoms to one helium atom, produces energy in the form or electromagnetic radiation
EARTH’S AVAILABLE ENERGY
1 solar enery 74tw
#2 geothermal energy 58w
#3 tides 3w
WHERE DOES SOLAR RADIATION GO?
- albedo 52tw
- re radiated as radiation
- water phase changes 40tw
- captured by living things 40tw
comets
what are they, composition
- Small bodies in highly eccentric elliptical orbits
- Compositions similar to Jovian planets
- May represent samples of early solar system
asteroids and meteors
composition
rock and iron
jovian planets
composition
hydrogen rich atmosphere and interior
-hydrogen under pressure becomes metallic liquid
-made of gas but are liquid and solid bc of temp and pressure
venus
- covered in non water dense clouds
- thick atmosphere
- no impact craters
- lots of volcanoes, still geologically active
- has motion in crust
mercury
- lots of craters
- made out of rock
- very dense, bigger core, part solid and liquid
mars
- once had water on it
similar to the moon
order of planets from sun
mercury, venus, earth, mars