Chapter 5 : The formation of stars and planets Flashcards
star
a dense cloud of gas that produces energy in its core by fusing light atoms into heavier ones
Kelvin temperature scale
use this to measure temperature of stars and other objects
interstellar cloud
cloud of cool dust and gas in the space between stars, it has self-gravity
self-gravity
a gravitational attraction among all parts of the same object
hydrostatic equilibrium of a cloud
when the forces on a cloud are balanced
molecular clouds
- the densest, coolest, interstellar clouds
- composed of hydrogen, dust and other gases
Once a molecular-cloud core begins to collapse, what happens?
the innermost core becomes a star, the outer parts form planets
protostar
innermost part of a collapsing molecular-cloud core
Formation of a protostar
- Molecular cores continue to collapse under their own gravity
- As cloud collapses, force of gravity increases and the collapse accelerates
- Center shrinks fastest; outer layers later
- Produces a dense protostar
Star Formation: Growing Protostar at the Center
-Protostar heats up due to the conversion of gravitational energy into thermal energy: Particles collide as they are pulled towards the center, Raises the temperature of the core, Pressures and temperatures are not yet high enough for fusion to occur
Wien’s Law
Relationship between temperature of an object and peak wavelength the object emits
Flux
Energy emitted by one square meter of the object every second
Luminosity
Total energy emitted every second
Depends on temperature and size of the star
nebula
interstellar cloud of gas and dust
Protostars emit mainly what type of light? (due to their cool temperatures)
infrared