capstone Flashcards
Describe what is the relationship between a star’s luminosity and size. What about the relationship between color and temperature?
The brighter the star the bigger it will be and smaller the star the dimmer it will be. The bluer/whiter the star is the hotter it is and the redder/orangery the cooler it is.
How is it possible for white dwarfs to have a lower luminosity than the sun even though the sun is much cooler than the white dwarfs?
White dwarf can have a lower luminosity or brightness than the sun due to being smaller than the sun. The white dwarf is hotter than the sun due to its color but is dimmer due to its size.
The main fuel for red giants’ stars in their core is
Helium
This is the type of star is what stars are mainly in their life cycle
Main sequence
What process is happening in the core of a star
Nuclear Fusion
When a star’s core runs out of hydrogen, the core shrinks and does what….
Heats up
Kepler’s 1st Law:
All planetary orbits are elliptical or oval in shape.
What is the difference between the perihelion and the aphelion
The perihelion is when it’s closer to the sun and the aphelion is when it’s farther away.
Kepler’s 2nd Law (AKA Equal Areas Law)-
a line joining a planet to its sun sweeps out equal areas in equal times as the planets travel along its orbit.
explain how and why a planet’s speed changes as it travels around its sun. Think about when a planet travels faster/slower in its orbit.
As the planet travels closer to the sun, it travels faster.
This is due to the strong gravitational force of the sun.
The farther away from the sun the slower it will travel.
The planet will take the same amount of time to travel
Same area due to the changing of speeds.
What is eccentricity and how does it relate to the second law? Give examples to help explain.
Eccentricity is how oval shape a celestial object’s orbit is indicated by either 0 (circular) or 1 (elliptical). This connects to the second law of planetary motion because those celestial bodies that are moving faster nearer the sun and slower away from the sun depends on the type of orbit they have. Those that have more of an elliptical orbit will have a bigger difference between speeds as they travel near the sun versus away from the sun. those with more circular orbit will not have a great difference between speeds when far or near the sun.
3rd Law (AKA Harmonies Law):
The square of a planet’s period equals the cube of the semi-major axis (average distance between the planet and its sun).
Explain what this law means in your own words.
This means that that the farther a planet is from the Sun, the slower its orbital speed, and vice versa.
Sedimentary
Characteristics
How it is formed
Examples
Fossils, easily broken, layers
Broken down into sediments, Sediments are cemented and compacted
Sandstone Limestone
Metamorphic
Characteristics
How it is formed
Examples
Ribbon like layers, foliated (Banded),
Immense heat and pressure
Marble Slate
Igneous
Characteristics
How it is formed
Examples
Shiny, glassy surface, air holes
Cooled down magma, intrusive is cool from magma slowly buried beneath the surface, extrusive form from cool magma on
Granite Pumice Obsidian