Week 1: Planets in the Solar System and Beyond Flashcards
What is the Copernican Principle?
Humans and Earth don’t hold a special place in the universe - we are fairly average and normal.
What defines a planet?
- orbiting around a sun
- large enough to have enough gravity to become round and clear its surrounding neighborhood
- too small to generate nuclear energy (significantly smaller than a star)
What was surprising about 51 Pegasi b when it was discovered?
01 first exoplanet orbiting a star discovered
02 really short orbit (4.4 days)
03 closer to its star than was previously thought possible
What’s notable about the Kepler satellite in relation to exoplanets?
01 responsible for a majority of later exoplanet discoveries (2009 and onwards)
02 allowed us to detect smaller exoplanets more similar to earth (not like the gas giant of 51 Pegasi b)
What is the Doppler technique?
a method of discovering exoplanets
look at the subtle gravitational effects of exoplanets on their parent stars
What is the Kepler method?
a method of discovering exoplanets
look at a star’s brightness to detect subtle dips, indicating a planet moving in front of the star periodically
What is eccentricity? (include actual numbers)
a measure of how much a planet’s orbit differs from a perfect circle
e=0 indicates a perfect circle orbit
e=1 highly eliptical
How does the eccentricity of planets in our solar system compare to the eccentricity of exoplanets?
Planets in the solar system have generally not very eccentric orbits, while exoplanets can get a lot more eccentric.
How does eccentricity contradict the Copernican principle?
planets in the solar system are so much less eccentric than lots of the exoplanets we have discovered so maybe we are special after all
What do stars form out of, and what are its properties?
molecular clouds
very dense and dusty gaseous clouds of atoms that are so cold that they stick together and become molecules such as H2, CO2, CH4
How is planet formation related to star formation?
It happens at the same time! As a star forms, planets form around it.
What starts star formation?
collapsing of a molecular cloud
can be motivated by a nearby supernova
What is the protoplanetary disc?
area of molecular cloud around a star that is left over from star formation
where planets eventually form
What happens to material in the protoplanetary disc not used up by planet formation?
driven away by the parent star’s radiation
What is the frost line? What can be found on either side of it?
the minimum distance from a star at which hydrogen compounds can form ice
inside of frost line is where rocky + metallic materials are (rocky planets)
outside of frost line is more icy/watery rocks (gas giants)
What is differentiation for rocky planets?
the process by which molten material in newly formed rocky planets separates itself into layers based on density
denser elements sink down to planet’s core
creates solid crust, molten mantle, and solid core like earth
How does differentiation happen in gas giants?
molten material separates itself into layers based on density
forms core of heavy molten materials (vs rocky planets’ solid core)
atmospheric layers - outer layer of cold gas, inner layer of super heavy pressure means matter exists simultaneously as solid, liquid, and gas
How many stars are in the milky way?
100-400 billion stars
What kind of star is most common in the milky way?
long-lived small red dwarfs (difficult for us to observe)
How many stars are estimated to have planets?
As few as 20% or as many as 90%
Describe the mass breakdown of a solar system (What percent of mass is certain materials?)
less than 1% metals + rocks
1.4% hydrogen compounds (H2O, CH4, NH3)
98% hydrogen + helium gases
What is the condensation curve?
describes what materials can be solid/liquid based on their distance from the host star
metals and rocks condense at high temperatures, so they exist close to the host star
hydrogen compounds condense at the second highest temperatures (exist further from star than rocks/metals)
gases condense at the lowest temperatures so they are most common the furthest from the host star
Vaporization temperature of a material is the closest it can get to its host star (when a material is vaporized, radiation pushes it away)
What is radiation pressure and what does it do?
pressure from stars that drives away gas and dust from the star’s immediate vicinity (leaves rocks and metals)
What are the characteristics of small rocky planets?
aren’t big enough to have atmospheres (not enough gravity)
don’t generally have geological activity
cratered surface - no atmosphere to protect from space objects