Ch 9+10 Flashcards
Why is it hard to tell depth on the moon?
You expect to see shades of shadows on a gray scale, but in reality it’s only black and light.
Moon Composition
Highlands (83%), Mare/Maria – flat plains of basaltic lava (17%)
How do craters form?
Crater hits, “comes out”, and particles fall back into hole that was made
Cold Traps on Moon
Where the sun’s rays never shine (poles of moon) ice in crater is unmelted
Highlands on Moon
- Made of relatively low-density rock that solidified on the cooling Moon
- Extremely heavily cratered, bearing scars of billions of years of impacts
Maria
-dark colored basalt (volcanic lava) laid down in volcanic eruptions years ago
Moon’s Surface
- fine grained soil of tiny, shattered rock fragments
- upper layers are porous with loosely packed dust
Impact Craters
Regardless of size or angle of impact, they are roughly round & circular
Formation of Impact Craters
(1) Impact occurs
(2) Projectile vaporizes and a shock wave spreads through the lunar rock
(3) Ejecta are thrown out of the crater
(4) Most of the ejected materials fall back to fill the crater, forming an ejecta blanket
Fission Theory
Moon was once part of Earth, but somehow separated from it early in history
Sister Theory
The Moon formed together but independent of Earth
Capture Theory
The Moon formed elsewhere in the solar system and was captured by Earth (least likely theory)
Avg Distance of Mars from the Sun
227 million kilometers (1.52 AU)
Avg Distance of Venus from the Sun
108 million kilometers (0.72 AU)
Appearance of Venus
- Appears very bright, featureless white ball
- Goes through phases like Moon
- Planet’s surface not visible b/c of dense clouds that reflect 70% of sunlight