welcome to astronomy 210 life in the universe. “the search for life in the universe” 3 rd...
TRANSCRIPT
Astronomy 210 Website is up Pickup Powerpoint notes at the
beginning of class Powerpoint presentations online Possible field trip to MLO Frequent Astronomy 100
refreshers Reading list soon…
Terrestrial Characteristics: Metallic core Oxygen dominated (silicates)
Material % (by mass)Iron 35Oxygen 30Silicon 15Magnesium 13Nickel 2.4Sulfur 1.9
Terrestrial Characteristics:
Thin (or nonexistent) atmospheres Few (or no) natural satellites Closely spaced orbits
Jovian Characteristics: Solid metallic-rocky cores Hydrogen dominated
Material % (by mass)Hydrogen 74Helium 24Water 0.6Methane 0.4Ammonia 0.1Rock & Metals 0.3
Cosmic Distances
Astronomical units of distance:
Astronomical Unit: The distance between the Sun and the Earth
93 million miles
Light year: The distance light travels in a year
Speed of light: 186,282 miles/sec
Light year: 5.9 trillion miles
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Gmgal
How many stars are in the Milky Way?
How many stars are in the Milky Way?
Orbital periodsun ~ 240 million years
Orbital distancesun ~ 28,000 light years
Mgal 100 billion Msun
Does this represent the actual number of stars in our
galaxy?
Our Sun is an “average star” in mass and luminosity.
The galaxy has many more low mass stars compared to high mass stars
Adjusted estimate of stars in Milky Way: 300 – 400 billion stars
It all depends on HO
HO – The “Hubble Constant” It is a measure of the slope of the
line in the Hubble Diagram Represents the expansion rate of
the Universe
OHUniverseofAge
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