Unit 34 Flashcards
Elliptical galaxy
A galaxy with an elliptical shape and little dust or gas
Spiral galaxy
A galaxy flattened into a disk shape with a pattern of spiral arms wound about a central nucleus. Spiral galaxies usually include dust, gas, and active regions of star formation.
Dust lanes
The dark colored (brownish) squiggly line type structures visible in galaxies.
Irregular galaxy
A non-symmetrical galaxy that does not have a well defined shape like either the spiral or elliptical galaxies. Irregular galaxies include dust, gas, and active star-forming regions
Star cluster
A group of stars that formed from the same cloud of material and have been held together in a cluster by gravitational forces.
A small open cluster can consist of only a few dozen members while a large globular cluster can contain more than a million individual stars.
What plays the biggest role in determining which type of galaxy forms?
Angular momentum
Local group
A small group of about two dozen galaxies that is associated with our milky way (we’re in it)
Galaxy cluster
A group of galaxies that is gravitationally bound together into a cluster, which vary greatly in size. A small cluster may have just a few members, while a large cluster may have several thousand.
Supercluster
clusters of clusters of galaxies
Void
The space between galaxy superclusters
Cosmological red shift
(or just Red Shift)
The shifting of galaxy light to the red end of the spectrum caused by the expansion of the universe.
Doppler stuff. Think of the same affect of a police siren coming towards you, passing you, then moving away. The sound you hear at different points in this process will be different because of the wavelengths
What is the Hubble Law?
The proportionality between the observed recessional velocity of a galaxy and the distance to that galaxy.
Hubble constant
The constant of proportionality, H, in the Hubble Law. It gives the rate at which our Universe is expanding
Cosmic microwave background
A uniform radiant field with an apparent temperature of 2.725 K that is observable in every direction.
Microwaves from the big bang. The universe’ temperature.
What do the COBE and WMAP tell us?
That there are slight variations in the microwave temperature