Lecture 3 Flashcards
1 AU (Astronomical Unit)
~150 million km
Distance between Sun and Earth
1 lyr (light year)
~10 trillion km
Distance light can travel in 1 year
Radar ranging
Bounce radio waves of other planets and measure the distance
Good for planets in solar system
Parallax
Uses hypotenuse
Good for nearby stars
Main-sequence fitting
Uses inverse square law
For things within milky way
Cephedes
So bright that they can be seen from other galaxies
Distance to nearby galaxies
Distant standards
Used supernova stars that explode to find galaxies
How many arcminutes in a degree?
60
Red-shift of galaxies
Uses Dopler Effect
Blue-shifter: Getting closer
Red-shifter: Going away
Hubble’s Law
v = H x D
Speed of galaxy’s recession is proportional to distance
What is the age of the Universe?
T = 1/H = 1/(13.7x10^9 yr)
or 4x10^17 secs
Big Bang nucleo-synthesis
1 sec after Big Bang, temp dropped to 10 billion K. Universe wad filled with electrons, protons, neutrons and photons but it was too hot to make atoms.
As it cooled, protons and neutrons fused to make light elements.
After 3 mins, too cold to make more fusion rxns.
What elements were created right after the Big Bang?
Hydrogen
Helium
Lithium
Beryllium
What produced heavy elements?
Stars
Hot enough for more fusion
What are the terrestrial planets?
Mercury
Venus
Earth
Mars