chapter 7 Flashcards
a system of planets and other smaller objects in orbit around a star
planetary system
- first plausible theory of the formation of the solar system by Immanuel Kant in 1755
- stated that the solar system formed from the collapse of an interstellar cloud of rotating gas
nebular hypothesis (2)
- a cloud of interstellar gas & dust illuminated by stars or seen in a silhouette against a brighter background
- if the outward force is less than self-gravity, the object contracts; if it is greater than self-gravity, the object expands
nebula (2)
a young stellar object that derives its luminosity from converting gravitational energy into thermal energy
protostar
the remains of the accretion disk around a young star from which a planetary system may form
protoplanetary disk
- a conserved property whose value depends on the velocity and distribution of the system’s mass in a rotating/revolving system
- L = m x v x r
angular momentum (2)
- mass
- rate of speed
- how the mass is distributed
3 aspects of angular momentum (3)
physical law that states the amount of angular momentum of an isolated system doesn’t change
conservation of angular momentum
a flat, rotating disk of gas & dust surrounding young stellar objects
accretion disk
- a primitive body of rock and ice that combines with others to form a planet
- particles that are ~1km in size
planetesimals (2)
- the stored energy in an object that is due solely to its position within a gravitational field
- material in the inner disk falls farther and picks up greater speed & higher temperature
- material in the outer disk moves slower
gravitational potential energy (3)
material that remains solid at high temperatures
refractory materials
material that remains gaseous/liquid at cooler temperatures (water, ice)
volatile materials
contains element carbon-hydrogen bonds
organic
behavior in complex systems in which a small change in the initial state of a system can lead to a large change in the final state of the system
chaotic