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Notes: Sun-Earth-Moon System A. The Earth 1. ____Axis__ - imaginary vertical line around which Earth spins 2. _Rotation___– the spinning of Earth around its axis that causes day and night 3. _Revolution__– Earth’s yearly orbit around the Sun a. Earth’s orbit is an __ellipse___, or elongated, closed curve b. Because the Sun is not centered in the ellipse, the distance between Earth and the Sun changes during the year (video clip: Planetary Rotation and Revolution) 4. Earth’s __tilt____ causes seasons a. The hemisphere tilted toward the Sun receives more daylight hours and radiation than the hemisphere tilted away from the Sun b. The longer period of sunlight is one reason summer is warmer than winter Let’s Illustrate: Reason for the Seasons (video clip Earth’s Tilt on It’s Axis) B. The Moon 1. Motions of the Moon a. ___Rotation___ on its axis which takes about _29.5_ days, with the same side always facing Earth. (video clip: movement of the moon) b. Shines because it reflects sunlight (video clip: Why we always see the same side of the moon) 2. Phases of the Moon a. _New Moon____– the moon is between Earth and the Sun and cannot be seen b. __Waxing______– more and more of the lighted side of the moon can be seen each night (waxing crescent, first quarter, waxing gibbous) c. __Full Moon____– all of the moon’s lighted side is visible d. __Waning____– less and less of the lighted side of the moon can be seen each night (waning gibbous, third quarter, waning crescent) (video clip: phases of the moon) 3. Eclipses – when the Earth or the Moon casts a shadow on the other a. Solar Eclipse - the moon moves directly between Earth and the Sun, shadowing part of Earth; occurs during the day ; during a new moon (video clip: solar eclipse) (video clip: Sun’s corona during a solar eclipse) b. Lunar Eclipse - the Earth’s shadow falls on the moon; occurs at night ;during a full moon (video clip: lunar eclipse) 4. Tides - at any shoreline on Earth, the height of the water will rise and fall throughout the day. Gravity is responsible for these regular increases and decreases. a. The moon’s gravity pulls on Earth. 1.) This pull creates a bulge of water on the side of Earth facing the Moon. 2.) Earth’s rotation and inertia creates a bulge on the opposite side of Earth as well 3.) The two bulges create high tides and between the two bulges are low tides. (video clip: tides) b. The sun’s force on the tides is less than half of the effect of the Moon. 1.) It creates two additional bulges a.) Spring Tide - the sun, moon, and earth align during a new and full moon and high-tide waters are higher than normal b.) Neap Tide - when the moon is in the first or third quarter and high tides are lower than normal and low tides are higher than normal C. The Sun 1. Solstice - the day when the Sun reaches its greatest distance north or south of the equator a. Summer Solstice - occurs June 21 or 22 in the northern hemisphere b. Winter Solstice - occurs December 21 or 22 in the northern hemisphere 2. Equinox - the day when the Sun is directly over Earth’s equator a. Daylight and nighttime hours are equal all over the world b. Spring Equinox occurs on March 20 or 21 in the northern hemisphere c. Fall Equinox occurs on September 22 or 23 in the northern hemisphere Life Cycle of Stars • 1. Nebula – how a star begins as a large cloud of gas and dust; gravitational force causes the nebula to contract; it breaks into smaller pieces when gas and dust become so hot that nuclear fusion starts; A STAR IS BORN. Stars spend many years in a relatively constant state. The center shrinks, and the outer part of the star expands. Life of an Average Star • 2. All average stars, including our Sun, eventually becomes a Red Giant. • 3. Planetary Nebula – the outer part of the red giant grows larger until it eventually drifts into outer space. • 4. The hot outer core left behind is a White Dwarf. A white dwarf is about 1 million times as dense as the Sun. Most of its fuel is gone, so it not longer produces energy. It gives off enough leftover heat to glow faintly for perhaps a billion years. It continues to cool until it becomes cold and dark. It is then called a Black Dwarf. Life of a Massive Star • 2. If the star is a massive star, it becomes a Supergiant. • 3. The core eventually collapses violently, sending a shock wave outward through the star. The outer portion explodes producing a Supernova. This can be million of times brighter than the original star. • 4. Material left from a supernova is called a Neutron Star. These are about twice as massive as the Sun and very dense. • 5. If material left over from the supernova is more than three times as massive as the Sun, it becomes a Black Hole because the core collapses. The gravity from this mass is so strong that nothing can escape from it, not even light. • Stars take different lengths of time to go through their life cycle. The length of a star’s life depends on its mass. The most massive stars live the shortest lives because they use up their fuel more quickly than stars with less mass. The life cycle of a star is often compared with that of the Sun, which is an average star. In about 5 billion years, the Sun will become a giant. Now it is a main sequence star, between an average star and a red giant. The Sun has an expected lifetime of about 10 billion years. How are Stars Classified? • All stars are huge spheres of glowing gas. Made up mostly of hydrogen, stars produce energy through nuclear fusion. • Stars are classified according to color, temperature, size, composition, and brightness. • The brightness of a star is described in two ways: 1. apparent magnitude – is a star’s brightness as seen from Earth 2. absolute magnitude – is the brightness the star would have if it were a standard distance from Earth; actual brightness H-R Diagram • About 100 years ago, two scientists Ejnar Hertzsprung and Henry Norris Russell made a graph to find out if the temperature and brightness of stars are related. They plotted the surface temperatures of stars on the x-axis and their absolute brightness on the y-axis. The points formed a pattern. This graph is still used today, called the Hertzsprung-Russell diagram. Main Sequence- diagonal band on H-R diagram (about 90% of stars) * Upper Left – hot, blue, bright stars * Lower Right – cool, red, dim stars * Middle – average yellow stars like the Sun The other 10% are dwarfs, giants and super giants. The Solar System • The Solar System is made up of 8 planets, the Sun, many small objects, and a huge volume of space. • The sun is the center of our Solar system. • All objects in the solar system revolve around the sun. • Gravity holds the solar system together. About 99.85% of the mass of the entire solar system is contained within the sun. • Distances within the solar system are so large that they are measured using astronomical units. One astronomical unit (AU) equals the average distance between Earth and the sun, about 150,000,000 km. • A planet is round, orbits the sun, and has cleared out the region of the solar system along its orbit. All except Mercury and Venus have at least one natural satellite, or moon. • A dwarf planet is an object that orbits the sun and has enough gravity to be spherical, but has not cleared the area of its orbit. • The solar system also includes many smaller objects that orbit the sun, such as asteroids and comets. • Scientists think the solar system formed about 4.6 billion years ago from a cloud of hydrogen, helium, rock, ice, and other materials pulled together by gravity. • Planets began to form as gravity pulled rock, ice, and gas together. The rock and ice formed small bodies called planetesimals. • Over time, planetesimals collided and stuck together, eventually combining to form all the other objects in the solar system. • Close to the sun, the inner planets are small and rocky. • Farther from the sun, the outer planets are gas giants. • Beyond the gas giants, ice and other materials produced comets and dwarf planets. The Planets • Inner Planets (Terrestrial Planets) – Small, dense, rocky surface with iron cores – Includes: Mercury, Venus, Earth, Mars • Outer Planets (Gas Giants) – Large, lightweight, no solid surface, have many moons – Made up of liquid and gases – Includes: Jupiter, Saturn, Uranus and Neptune Inner Planets • Closest to the Sun; 36 million miles from the Sun • Smallest planet; 4,879 km in diameter (not much larger than Earth’s moon) • Revolution (Orbit) – 88 days Rotation – 58.9 days • No Moons • Thin atmosphere is constantly replenished by the solar wind • Surface is rocky and cratered • Temperatures range from 430⁰C to -170⁰C • Much of what we know about Mercury has come from space probes. • Second from the sun; 67 million miles from the Sun • Similar to Earth in size and mass, called “Earth’s twin”; 12,104 km in diameter • Revolution (Orbit) – 224.7 days Rotation – 244 days • No Moons • Brightest planet • Extremely dense atmosphere of clouds. The pressure of Venus’s atmosphere is 90 times greater than Earth’s • Has the hottest surface of any planet. Surface temperature of 450⁰C • Rocky surface with volcanic cracks • Third planet from the Sun • More than 70% of the surface is covered in water • Earth is “just right” for life as we know it. Earth is not too hot or too cold. • Earth is the only planet with an atmosphere that is rich in oxygen and it traps heat. The atmosphere protects the surface from most meteors and the Sun’s radiation. • One large Moon • Only planet where life is known to exist • Fourth planet from the Sun; 141.5 million miles from the Sun • Called the Red Planet because of iron-rich rocks, leaving a rusty dust behind • 6,794 km in diameter • Revolution (Orbit) – 2 years Rotation – 24 ½ hours • 2 small Moons: Phobos and Deimos • Scientists think that liquid water flowed on Mars’s surface in the distant past. • Has dust storms that cover the planet for days • Has largest volcano in the solar system – Olympus Mons • Thin atmosphere of mostly carbon dioxide • Tilted on its axis; which causes seasons Outer Planets • • • • 5th from the Sun; 483.3 million miles form Sun Largest planet; 142,984 km in diameter Revolution (Orbit) – 11.9 years Rotation – 9.9 hours At least 63 Moons; Galileo discovered the largest moons in 1610 – Io, Europa, Ganymede, and Callisto • Thick gas atmosphere of mostly hydrogen and helium • Storms swirl the planet; the largest being the Great Red Spot (larger than Earth!) • • • • 6th planet; 886 million miles form the Sun Second largest planet; 120,536 km in diameter Revolution (Orbit) – 29.5 years Rotation – 10.7 hours Has beautiful rings around it (thousands of them); made of chunks of ice and rock • At least 61 moons; the largest Titan is larger than Mercury • Thick gas atmosphere (hydrogen and helium); clouds and storms • • • • • • • • • • First seen in 1781 7th from the Sun; 1,778 million miles from Sun Twice as far from the sun as Saturn, so it is much colder. 51,118 km in diameter (much smaller than Jupiter and Saturn) Revolution (Orbit) – 83.8 years Rotation – 17.2 hours At least 27 Moons Ocean of water and ammonia It looks blue-green because of traces of methane in its atmosphere Thin rings Axis of rotation is tilted at an angle of 90⁰ from the vertical. Rotates from top to bottom instead of side to side. • • • • • • • • 8th planet: 2,793 million miles from Sun 49,528 km in diameter Revolution (Orbit) – 163.8 years Rotation – 16.1 hours Cold, Blue-green planet 2 main rings, 3 small rings At least 13 moons Poisonous thick gas atmosphere The Great Dark Spot was probably a giant storm. Images taken 5 years later showed that the spot was gone. • • • • • • • Last planet to be discovered (1930) 3,660 million miles form the Sun 2,000 miles in diameter Revolution (Orbit) – 248 years Rotation – 6 days 1 moon, Charon, half the size of the planet Small, rocky, made of methane ice In 2006 Pluto was demoted from being a planet and is now classified as a dwarf planet Notes: Sun-Earth-Moon System A. The Earth 1. __________– imaginary vertical line around which Earth spins 2. _________– the spinning of Earth around its axis that causes day and night 3. _________– Earth’s yearly orbit around the Sun a. Earth’s orbit is an __________, or elongated, closed curve b. Because the Sun is not centered in the ellipse, the distance between Earth and the Sun changes during the year 4. Earth’s _________ causes seasons a. The hemisphere tilted toward the Sun receives more daylight hours and radiation than the hemisphere tilted away from the Sun b. The longer period of sunlight is one reason summer is warmer than winter Let’s Illustrate: Reason for the Seasons B. The Moon 1. Motions of the Moon a. ____________on its axis which takes about _____ days, with the same side always facing Earth. b. Shines because it reflects sunlight 2. Phases of the Moon a. _____________– the moon is between Earth and the Sun and cannot be seen b. _____________– more and more of the lighted side of the moon can be seen each night (waxing crescent, first quarter, waxing gibbous) c. ____________– all of the moon’s lighted side is visible d. ____________– less and less of the lighted side of the moon can be seen each night (waning gibbous, third quarter, waning crescent) 3. _______________– when the Earth or the Moon casts a shadow on the other a. _____________- the moon moves directly between Earth and the Sun, shadowing part of Earth; occurs during the _____; during a ___________ b. _____________ - the Earth’s shadow falls on the moon; occurs at ________; during a _________ 4. ________– at any shoreline on Earth, the height of the water will rise and fall throughout the day. __________ is responsible for these regular increases and decreases. a. The moon’s gravity pulls on Earth. 1.) This pull creates a bulge of water on the side of Earth facing the Moon. 2.) Earth’s rotation and inertia creates a bulge on the opposite side of Earth as well 3.) The two bulges create high tides and between the two bulges are low tides. b. The sun’s force on the tides is less than half of the effect of the Moon. 1.) It creates two additional bulges a.) ______________– the sun, moon, and earth align during a new and full moon and high-tide waters are higher than normal b.) _____________– when the moon is in the first or third quarter and high tides are lower than normal and low tides are higher than normal C. The Sun 1. _____________– the day when the Sun reaches its greatest distance north or south of the equator a. ______________occurs June 21 or 22 in the northern hemisphere b. ______________occurs December 21 or 22 in the northern hemisphere 2. ____________– the day when the Sun is directly over Earth’s equator a. Daylight and nighttime hours are equal all over the world b. _______________occurs on March 20 or 21 in the northern hemisphere c. ________________ occurs on September 22 or 23 in the northern hemisphere The Solar System • The ________________is made up of _____________, the ________, many ___________________, and a huge ________________________. • The sun is the ________________of our Solar system. • All objects in the solar system ___________around the ____. • __________holds the solar system together. About ________ of the mass of the entire solar system is contained within the _________. • Distances within the solar system are so large that they are measured using ______________________. One astronomical unit (_____) equals the average distance between _________________, about __________________. • A ___________ is __________, ________________, and has __________________________ of the solar system along its orbit. All except Mercury and Venus have at least one natural satellite, or moon. • A ___________________ is an object that orbits the sun and has enough gravity to be spherical, but has _______________ _______________________. • The solar system also includes many smaller objects that orbit the sun, such as ______________ and _______________. • Scientists think the solar system formed about _______billion years ago from a cloud of ___________, ____________, _____, ______, and other materials ____________________ _____________________. • Planets began to form as gravity pulled rock, ice, and gas together. The rock and ice formed ________________ called ________________________. • Over time, planetesimals collided and stuck together, eventually combining to form all the other objects in the solar system. • _________to the sun, the inner planets are _____________. • _________from the sun, the outer planets are ___________. • __________the gas giants, ice and other materials produced comets and dwarf planets. The Planets • Inner Planets (Terrestrial Planets) – __________, dense, ___________surface with __________________ – Includes: Mercury, Venus, Earth, Mars • Outer Planets (Gas Giants) – _______, ___________, no solid surface, have __________________ – Made up of liquid and gases – Includes: Jupiter, Saturn, Uranus and Neptune Inner Planets • ________________________; 36 million miles from the Sun • ________________ planet; 4,879 km in diameter (not much larger than Earth’s moon) • Revolution (Orbit) – 88 days Rotation – 58.9 days • _______________________ • _____atmosphere is constantly replenished by the solar wind • Surface is _________and _____________ • Temperatures range from 430⁰C to -170⁰C • Much of what we know about Mercury has come from space probes. • Second from the sun; 67 million miles from the Sun • __________________ in size and mass, called “Earth’s ________”; 12,104 km in diameter • Revolution (Orbit) – 224.7 days Rotation – 244 days • ____________________ • ______________ planet • Extremely _________________of clouds. The pressure of Venus’s atmosphere is 90 times greater than Earth’s • Has the ________________of any planet. Surface temperature of 450⁰C • Rocky surface with volcanic cracks • Third planet from the Sun • More than ____% of the surface is ____________________ • Earth is “just right” for life as we know it. Earth is _______ ______________________ • Earth is the only planet with an atmosphere that is rich in __________and it ___________. The atmosphere protects the surface from most meteors and the Sun’s radiation. • ______________________ • Only planet where ________ is known to exist • Fourth planet from the Sun; 141.5 million miles from the Sun • Called the __________________ because of iron-rich rocks, leaving a ____________________ behind • 6,794 km in diameter • Revolution (Orbit) – 2 years Rotation – 24 ½ hours • 2 small Moons: ____________and Deimos • Scientists think that ______________________flowed on Mars’s surface in the distant past. • Has dust storms that cover the planet for days • Has largest volcano in the solar system – ____________________________ • Thin atmosphere of mostly carbon dioxide • ____________on its axis; which causes seasons Outer Planets • • • • 5th from the Sun; 483.3 million miles form Sun _____________________; 142,984 km in diameter Revolution (Orbit) – 11.9 years Rotation – 9.9 hours At least _____Moons; ______________ discovered the largest moons in 1610 – Io, Europa, Ganymede, and Callisto • Thick gas atmosphere of mostly hydrogen and helium • Storms swirl the planet; the largest being the _____________________ (larger than Earth!) • • • • 6th planet; 886 million miles form the Sun ____________________________; 120,536 km in diameter Revolution (Orbit) – 29.5 years Rotation – 10.7 hours Has __________________________ around it (thousands of them); made of chunks of ice and rock • At least ___moons; the largest _______is larger than Mercury • Thick gas atmosphere (hydrogen and helium); clouds and storms • • • • • • • • • • First seen in 1781 7th from the Sun; 1,778 million miles from Sun _________as far from the sun as Saturn, so it is much _____. 51,118 km in diameter (much ___________than Jupiter and Saturn) Revolution (Orbit) – 83.8 years Rotation – 17.2 hours At least _____Moons Ocean of water and ammonia It looks blue-green because of traces of _______________in its atmosphere __________rings Axis of rotation is tilted at an angle of ____⁰ from the vertical. Rotates from ____________________instead of side to side. • • • • • • • • 8th planet: 2,793 million miles from Sun 49,528 km in diameter Revolution (Orbit) – 163.8 years Rotation – 16.1 hours _________, ________________ planet 2 main rings, 3 small rings At least _____moons ______________thick gas atmosphere The ________________was probably a giant storm. Images taken 5 years later showed that the spot was gone. • • • • • • • Last planet to be discovered (1930) 3,660 million miles form the Sun 2,000 miles in diameter Revolution (Orbit) – 248 years Rotation – 6 days 1 moon, Charon, half the size of the planet _________, ____________, made of ___________________ In _________Pluto was _______________from being a planet and is now classified as a ___________________