Solar System Flashcards
Explain the nebula hypothesis
Sates that the sun and the planets developed out of the same cloud of gas and dust
1) A nebula began to collapse under its own gravity- gravity increased assisted nearby supernova or other force
2) Spins faster- angular momentum (“ice skater effect”)
3) Flattens out into disk shape with most mass in center (“pizza dough effect”)
4) Energy from collisions and pressure from gravity- nebula become hotter from increase in density
5) When temp in core reaches 10 million degrees Celsius, thermonuclear fusion begins (converting hydrogen to helium)
What are the basic components of the solar system?
- The sun
- The planets
- Asteroids
- Kuiper Belt
- Oort Cloud
How were the planets created from dust and gas? (What is the origin of dust and gas)?
- Dust: produced in the cores of stars
- Gas: left over from Big Bang
- Planets form by the progressive collision of dust particles to form larger and larger objects
What is the order of the planets starting from the sun?
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune
How were the inner planets created?
- Formed closer to the sun
- These planets lost their dense gases because at the temperature of the gases, gravity was not strong enough to hold the gases
- Other lighter elements may have been blown or boiled away (from sun radiation)
- Denser material sank to center of planets, layers formed
- Less dense material stayed on outer part of planet
- Small/rocky, made of heavy elements (ex. iron, nickel)
How were the outer planets created?
- Formed farther from the sun (in cold region)
- Cold- did not lose their light elements (helium, hydrogen) or ices
- At first, thick layers of ice surrounded small cores of heavy elements
- However, due to intense heat/pressure in planets’ interiors, ices melted to form layers of liquids/gases
- Low density, huge planets, made mostly of gas
What are the 2 most common elements in the solar system, the universe, the sun, and the gas giants?
Hydrogen and helium
What is Kepler’s first law and what is its significance?
Law of ellipses- anything orbiting anything has an orbit which is the shape of an ellipse
The planets are not the same distance from the sun at every point in their orbit
What is Kepler’s second law and what is its significance?
Law of equal areas- objects move faster in their orbit when they are closer to the sun
A line between the sun and the planet sweeps equal areas in equal time
What is Kepler’s third law and what is its significance?
Law of harmonics- there is a mathematical relationship between a planet’s distance from the sun and how long it takes that planet to orbit the sun
Scientists can find out how far away the planets are from the sun by using this law
What is the age of the Earth? How do we know?*
- 6 billion years old
- Analyses of radioactive elements and daughter products in meteorites that were formed at the exact same time as Earth
- Radioactive decay: a method of determining the absolute age of an object by comparing the relative percentages of a radioactive (parent) isotope and a stable (daughter) isotope
As you look down onto the North Pole of the Earth, in what direction is the Earth :
- rotating
- revolving
- counterclockwise
2. counterclockwise
Perihelion (when is the Earth’s)
The point in the orbit of a planet at which the planet is closest to the sun
Earth’s perihelion: January 4
Aphelion (when is the Earth’s)
The point in the orbit of a planet at which the planet is furthest to the sun
Earth’s aphelion: July 4
Asteroid
- Rocky object orbiting the sun
- Most orbit between Mars and Jupiter (asteroid belt)
Comet
- Small body of ice, rock, and cosmic dust that follows a highly elliptical orbit around the sun
- Gives off gas/dust in the form of a tail as it passes close to the sun
Gas giant
- Composed mainly of gases
- Rocky cores which resemble a terrestrial planet
- Dozens of moons
- All have rings
Geocentric universe
The sun, the stars, and the planets revolve around Earth
Heliocentric universe
The planets revolve around the sun in the same direction but at different speeds and distances from the sun
Hurricane
A severe storm that develops over tropical oceans and whose strong winds of more than 120 km/h spiral in toward the intensely low-pressure storm center