The Solar System

The Solar System Early Astronomy Astronomy- the science that studies the universe It Investigates: properties of objects in space, and the laws under which they function. Geocentric Model Earth was a motionless sphere around which the rest of the universe revolved

The Solar System In A.D. 141, Ptolemy presented an advanced geocentric model of the universe that we now call the Ptolemaic System. The precision with which it predicted the motions of the planets, allowed it to go unchallenged for almost 13 centuries Epicycle- small circle each planet moved on Deferent- larger circle that the epicycle is centered on and moves around Earth

The Solar System The Catholic Church controlled scientific thought (if they controlled scientific thought, they had more power) during this time period and anyone not believing in a geocentric model of the universe was punished Biblical passages suggest the Sun is in constant motion while the Earth remains in one place It was thought that the creation of the planets occurred after the creation of Earth The development of modern astronomy was a break from previous philosophy and religious views. Scientists began to realize that the universe, and everything in it, was governed by natural laws.

The Solar System 1543 here comes Copernicus Heliocentric Model (sun at center) 1543 here comes Copernicus **actually Copernicus was not the first to suggest the heliocentric model but further developed and it eventually gained popularity Copernicus believed the sun was at the center of the solar system and was able to work out the arrangement of the known planets

The Solar System Johannes Kepler (late 1500’s) The path of each planet around the sun is an ellipse– oval shape When he used circular orbits his calculations did not fit observations More on this after Galileo 

The Solar System Galileo 1610 builds a telescope, discovers: Moons around Jupiter Proved not everything in the sky revolves around the Earth Venus goes through series of phases similar to the moon’s Not possible if both it and the Sun circled the Earth

The Solar System Now back to Johannes Kepler and ellipse… The path of each planet around the sun is an ellipse (oval-shape) with the sun at one focus and an imaginary point at the other Eccentricity- a measure of how round or flat (oval) a shape is Eccentricity = Distance between foci **has no units Length of the major axis    

The Solar System

The Solar System Why is eccentricity important? All planets revolve around the Sun (one foci) along an elliptical path called an orbit For all planets in our solar system, one of the two foci is always the sun Planets revolve around the sun at varying speeds. The closer the planet to the sun, the fast the speed

The Solar System Perihelion - the point in the orbit of a planet, at which it is closest to the sun Planets at perihelion travel faster here due to the greater gravitational attraction between the objects Aphelion – the point in the orbit of a planet at which it is farthest from the sun Planets at aphelion travel slower here due to less gravitational attraction   WHY IS THIS TRUE?

The Solar System

The Solar System The Solar System (SS)—Basic info Scientists think the SS formed about 4.6 billion years ago from a cloud of hydrogen, helium, rock ice and other materials pulled together by gravity Part of the milky way galaxy (galaxy = billions of starts held together by gravity) which is a spiral galaxy Consists of the sun, the planets, their moons, and a variety of smaller objects Sun is at the center Gravity holds the solar system together Distances in the SS Astronomical Unit (AU)- equal to the average distance between the sun and Earth About 150,000 km (93, 205 miles) SS extends more than 100,000 AU from the sun The Sun 99.85% of the mass of the solar system is contained within the sun Mid sized star-half way though its life cycle The Planets An object that orbits a star, is large enough to have become rounded due to its own gravity, and has cleared the area of its orbit Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, **Pluto Dwarf Planets An object that orbits the sun and is spherical but has not cleared the area of its orbit Pluto was considered the 9th planet of solar system but shares the area of its orbit with other objects so is now considered a dwarf planetS Satellites An object that orbits a planet, moons, except Mercury and Venus, every planet in the SS has at least natural satellite or moon Smaller Object Asteroids - small rock bodies that orbit the sun Comets- loose spheres of ice and rock that have very long narrow orbit

The Solar System In case you didn’t know….

The Solar System Terrestrial (Inner) Planets Small Dense Rocky surface In order from closest – farthest from sun Mercury Smallest Closest to sun Virtually no atmosphere Venus Thick atmosphere, always cloudy, greenhouse effect Hottest surface of any planet Unusual pattern of rotation, 8 months to rotate once and 7.5 months to revolve once Rotates from East to West

The Solar System Earth Mars The water planet- Liquid water covers about 70% of surface Suitable temperature range for most living things to survive Atmosphere rich in O2, N, CO2, greenhouse effect One moon Mars The red planet Too cold for liquid water now, had liquid water in the past Has water ice now Atmosphere is 95% CO2 Two moons

The Solar System ***Between mars and Jupiter there is an asteroid belt Gas or Jovian (Outer) Planets Called “gas giants” Large Less Dense Do not have solid surfaces Strong gravitational force which keeps gas from escaping Thick atmospheres Much of the material that makes up these planets is liquid because the pressure inside these planets is so high Have many moons Surrounded by rings- thin disk of small particles of ice and rock

The Solar System In order from closest – farthest from sun Jupiter Largest and most massive planet Thick atmosphere of hydrogen and helium At least 63 moons Saturn 2nd largest planet in SS Rings made up of chunks of ice and rock each traveling in its own orbit around Saturn At least 61

The Solar System Uranus Neptune Pluto– dwarf planet Very cold Methane in atmosphere (give it blue color) Surrounded by thin flat rings Axis of rotation is about 90o to vertical, rotates from top to bottom instead of from side to side At least 27 moons Neptune Cold, blue planet Atmosphere contains clouds At least 13 moons Pluto– dwarf planet Does not clear the neighborhood of its orbit Highly elliptical orbit Perihelion distance = 4440 million km from sun Aphelion distance = 7380 million km from sun