Final Exam Flashcards
Copernicus
First modern astronomer who thought the sun was the center of the universe and the Earth revolved around it.
Galileo’s discoveries included:
features of the moon, planets aren’t disks, jupiters moons, supported the copernicus model
Aristotle
first astronomer who said the earth was a sphere
Composition percentages of the universe
74% dark energy, 22% dark matter, 3.6 intergalactic gas (nebula), .4% stars and planets.
Nebula:
large mass or
cloud of dust and gas
(~92% Hydrogen & 7%
Helium, trace others)
What material are stars and planets formed from
Nebulas
What’re the three types of nebulas
Reflection, Emission, Dark
Reflection Nebula:
Nebula that reflect(s) light
Emission Nebula:
When interstellar (between stars)Hydrogen is close to a hot star, the UVradiation from the nearby star ionizes the Hydrogen, which then emits light
Dark Nebula:
when dust particles block
radiation/light
Galaxies
Clusters of stars (“Globular clusters”) fall
into spherical distributions
How many galaxies are there in the universe
125 billion
What’re the three types of galaxies
Spiral, non-spiral, and elliptical
Spiral Galaxies
These galaxies are bright
What’re the 4 subcategories of spiral galaxies
Sa,Sb,Sc, and Barred Spiral Galaxies
Sa Galaxy
Large, dominant nucleus and tightly‐
wound spiral arms.
Sb Galaxy
Less prominent nucleus and more
open spiral arms (our Milky Way fall in this class)
Sc galaxies
Small nucleus and loosely‐wound
spiral arms.
Barred Spiral Galaxies:
Have a bar through theircentral region; are designated as SBa, SBb, and SBc
Elliptical Galaxies
More abundant than Spiral Galaxies • Older than Spiral Galaxies
Types of Elliptical galaxies
E0 Galaxies: spherical • E1: slightly flattened • ….. • E7: most flattened
Irregular Galaxy:
Those that do not fit into the other categories; no
obvious shape or structure.
S0 Galaxies:
Transition galaxies that are between spirals and
ellipticals.
Blue Stars
Very hot stars , with temps > 30,000 K, emit shorter wavelengths of radiation. These are also the brightest stars.
Yellow Stars
Stars with temps between 5,000 K and 6,000 K appear yellow (our Sun)
Red Stars
Cooler stars, with temps < 3,000 K. These are the dimmest stars.
Hertzsprung and Russell Diagram
Most: Main Sequence A few Blue Giants, Red Giants and Supergiants: Very bright
Dimmest:White and Red dwarfs
Stellar Lifecycle Details
Stars form from Nebula.
Gravitational Contraction: Because of gravity, the gas particles in thenebula cloud are attracted towards each other and contract Termed
self‐gravity.
This movement increases the kinetic energy which increases
Temperature.
The more massive the cloud, the more self‐gravity it has, and the more likely it is to contract .