Quiz 2 Flashcards
Exploration of Mercury
- 3 space craft
- boring dull
- political/ social reasons for not a lot of exploration
Exploration of Venus
- 40+ spacecrafts gone/ mostly Russia
- easy to get to
- cloud cover is/mysterious
- lander, orbiters, and balloons have been
- activity in 60s and 70s
- not a lot after collapse of USSR
Exploration of the Moon
- lots of activity when learning how to shoot rockets but became boring
- now wanting to be moon base, mining, for man
Exploration of Mars
- lots of activity in 60-70s
- lull in 80-90s
- lots of activity now
- many missions
Exploration of Asteroids
- none before 1989
- public does not care
- small with no gravity, hard to land on or explore
Exploration of Jupiter
- 7 all American missions
- could not use solar panels as power
- so they used nuclear reactors, small and expensive
Exploration of Saturn
- 4 all American missions
- far away and 1000x the size of earth
Exploration of Comets
-none before 1985 because the move faster with very little gravity
Accession Disc Theory
- solar nebula theory
- as gas/dust collapses, pieces “acret”
- bump into each other and stick and grow into planets
Evidence of accession disc theory
- other stars have discs around them
- we should see planets around other stars
- stars should wiggle from pull of planets
Astrometry
- track movement of stars relative to background
- we tracked stars for decades
- didn’t find any
“first” extra solar planet found
- found around dead exploded star
- but he found earth and was embaressed
actual first extra solar planet found
- we didn’t find it at first because awe assumed planets had orbits like those in our solar system
- found around another regular star
- assumed to be an error
- it has 4 day revolution
- found by mayor and Pegg
- called 51 Pegg
Lessons in Extra-solar Planet Discovery
1) theory must be validated by observation or experiment
2) Human bias is hard to overcome
3) verify results before publishing
4) your results build on other results
5) discoveries are often very unexpected
new technique to find planets
looking for light shifts due to sun passing in front of planets. vice versa
two types of planets
terrestrial, jovian
Terrestrial Planets
- small
- rocky/dense
- inner solar system
- few moons
- no rings
Jovian planets
- larger
- gaseous/low density
- outer solar system
- lots of moons
- all have rings
what things in space have craters on them
every hard surface
non planet objects
- asteroids
- meteors
- comets
Asteroids
small rocky orbit between mars and Jupiter
Comets
icy with elliptical orbits, tails near sun
Meteoroids
tiny rocks often burn up in earths atmosphere
accession disc theory implies that
everything is the same age
what is the best method to determine age
radioactive dating
what is radioactive dating
- looking at molecules because they emit a particle
- approximate time for decay is half-life
half-life
time for half of all particles to decay by measuring the percent that decay
what is often used to date objects younger that 50,000 years
C14
how old are moon rocks
4.5 billion years old
how old are meteorites
4.6 billion years old
how old is earth
3.9 billion years old
how old is mars
4.3 billion years old
how can accession disc theory be right if the things are all different ages
you have to account for the time it takes for things to cool
evidence to solar system formation
1) disc shape
2) orbits in same direction
3) two planetary types
4) rings around Jovian planets
5) craters everywhere
6) space debris
7) all things about same age
what is the sun made up of
73% hydrogen, 25% helium, 2% heavy elements
based on solar nebula theory what should planets be made of
98% hydrogen and helium
why is earth not made of 98% hydrogen and helium
- early earth was
- little planets could not hold it all due to weak gravity
- big planets lost some but still have lots of He, H
what does solar wind do
strips away upper layer of terrestrial atmosphere
accretion
- many small grains collide and stick
- speed dependent
condensation
gases collide with grains and condenses
Planetsimal
due to condensation and accretion, small rocks become bigger about centimeter in size
protoplanet
when rocks accret and become at least 100km in size
protoplanets grow slowly or quickly
quickly because they steal food from other planets
two tories about how protoplanets become planets
homogeneous accretion and heterogenous accretion
homogenous accretion
- similar type planetsimals merge
- heat makes them liquid
heterogeneous accretion
- iron planetesimals form first and merge to create a core
- then other types of planetismals collide to form outer layers
when does plant growth start to slow down?
when sun ignites and solar wind blows away remaining dust and gas and leaves behind rocks and planets
we observe craters on what kind of surfaces?
all solid ones and is strong evidence of accretion disc theory
what is the theory of how planets were created
planets developed from gas and dust via condensation into grains, growth by collision, then by gravity into planets
why are solid/ terrestrial planets in the inner solar system
because its warmer and only heavy elements condense into grains
why are jovians in the outer solar system
because icy lighter elements also condense far away
why should jovian be larger
because they have more “food” at larger distances
what can jovian do that terrestrials can not
trap H, He atmospheres