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... yourself. A simple backyard telescope can reveal many of them to your own eyes. Now that you understand our incredible solar system, think about what lies beyond. There must be many other wonders to be discovered. ...
... yourself. A simple backyard telescope can reveal many of them to your own eyes. Now that you understand our incredible solar system, think about what lies beyond. There must be many other wonders to be discovered. ...
Comets
... Some comets make many revolutions around the sun. The most famous returning comet is Halley's Comet. It revolves around the sun once every 76 years. It was named for Edmund Halley who discovered it in 1682. Its orbit of about 11 billion kilometers takes it just past Neptune. The tail of Halley's Com ...
... Some comets make many revolutions around the sun. The most famous returning comet is Halley's Comet. It revolves around the sun once every 76 years. It was named for Edmund Halley who discovered it in 1682. Its orbit of about 11 billion kilometers takes it just past Neptune. The tail of Halley's Com ...
LESSON PLAN: National Geographic Magazine Archive
... groups. Each group is assigned a planet and must tell the class all of the information about their planet as well as the interesting fact that they learned. ...
... groups. Each group is assigned a planet and must tell the class all of the information about their planet as well as the interesting fact that they learned. ...
Lesson 2 Power Notes Outline
... Today, we know that the orbits of the planets are only slightly elliptical, but the orbits of objects such as Pluto and comets are highly elliptical. ...
... Today, we know that the orbits of the planets are only slightly elliptical, but the orbits of objects such as Pluto and comets are highly elliptical. ...
Post-class version
... Findings on composition of atmosphere, counting by number of atoms • 90% hydrogen • 10% helium ...
... Findings on composition of atmosphere, counting by number of atoms • 90% hydrogen • 10% helium ...
Solar Magnetism in Little Ice Age, Orbits in Solar Ecliptic
... ^ When gravitons and photons transfer energy to each other, E=mc^2 (“Does the Inertia of a Body Depend Upon Its Energy Content?” by Albert Einstein "Annalen der Physik" - November 21, 1905) says the relation of mass to energy means they’re transferring mass, too. Another way to view their interactio ...
... ^ When gravitons and photons transfer energy to each other, E=mc^2 (“Does the Inertia of a Body Depend Upon Its Energy Content?” by Albert Einstein "Annalen der Physik" - November 21, 1905) says the relation of mass to energy means they’re transferring mass, too. Another way to view their interactio ...
music lessons (2) new
... I think we can hear it from here too. ALL PLANETS (CHORUS) We are the planets of the Solar System Different sizes for every one The music never ends We are such good friends And we all orbit the sun SUN ...
... I think we can hear it from here too. ALL PLANETS (CHORUS) We are the planets of the Solar System Different sizes for every one The music never ends We are such good friends And we all orbit the sun SUN ...
The ISM and Stellar Birth
... Reflection Nebulae: • Light reflected (scattered) by dust/gas much like the moon reflects the Sun’s light – so doesn’t generate its own light • Scatter light from cooler stars • Mostly scatters blue light (like our atmosphere) – so they appear blue. • Dust grains must have sizes ranging from 0.01mm ...
... Reflection Nebulae: • Light reflected (scattered) by dust/gas much like the moon reflects the Sun’s light – so doesn’t generate its own light • Scatter light from cooler stars • Mostly scatters blue light (like our atmosphere) – so they appear blue. • Dust grains must have sizes ranging from 0.01mm ...
Elements - Hofstra
... nuceleosynthesis (nuclear fusion) in all stars. Our sun is currently fusing Hydrogen atoms into Helium atoms, releasing heat as mass is converted to energy. When the Sun runs out of Hydrogen, it will begin to fuse Helium into Carbon. Our sun is too small to burn Carbon, so when it runs out of Helium ...
... nuceleosynthesis (nuclear fusion) in all stars. Our sun is currently fusing Hydrogen atoms into Helium atoms, releasing heat as mass is converted to energy. When the Sun runs out of Hydrogen, it will begin to fuse Helium into Carbon. Our sun is too small to burn Carbon, so when it runs out of Helium ...
The Solar System
... – only dwarf planet NOT in the Kuiper Belt • ERIS (Greek/Roman goddess of strife and discord) – Eris is larger than Pluto so logically either Eris had to be a "planet" or Pluto had to be reclassified. – largest dwarf planet, largest known member of the Kuiper Belt – orbits 10,128,000,000 km from the ...
... – only dwarf planet NOT in the Kuiper Belt • ERIS (Greek/Roman goddess of strife and discord) – Eris is larger than Pluto so logically either Eris had to be a "planet" or Pluto had to be reclassified. – largest dwarf planet, largest known member of the Kuiper Belt – orbits 10,128,000,000 km from the ...
The Solar System
... Sometime in the middle of the night, Holmes wakes Watson and says, “Watson, look up at the stars and tell me what you see.” Watson says, “I see millions of stars and even if a few of those have planets, it’s quite likely there are some planets like Earth, and if there are a few planets like Earth ou ...
... Sometime in the middle of the night, Holmes wakes Watson and says, “Watson, look up at the stars and tell me what you see.” Watson says, “I see millions of stars and even if a few of those have planets, it’s quite likely there are some planets like Earth, and if there are a few planets like Earth ou ...
Comets
... Some comets make many revolutions around the sun. The most famous returning comet is Halley's Comet. It revolves around the sun once every 76 years. It was named for Edmund Halley who discovered it in 1682. Its orbit of about 7 billion miles takes it just past Neptune. The tail of Halley's Comet has ...
... Some comets make many revolutions around the sun. The most famous returning comet is Halley's Comet. It revolves around the sun once every 76 years. It was named for Edmund Halley who discovered it in 1682. Its orbit of about 7 billion miles takes it just past Neptune. The tail of Halley's Comet has ...
solar system
... Now we’ll see some much smaller objects. In 2006, astronomers decided that Pluto would no longer be called a planet. It and other small planets would now be called dwarf planets. Dwarf planets are mostly like Pluto. For that reason, astronomers decided to call them plutoids. Plutoids orbit the Sun i ...
... Now we’ll see some much smaller objects. In 2006, astronomers decided that Pluto would no longer be called a planet. It and other small planets would now be called dwarf planets. Dwarf planets are mostly like Pluto. For that reason, astronomers decided to call them plutoids. Plutoids orbit the Sun i ...
Here
... • Aristotle was perhaps the most influential Greek philosopher. He favored a geocentric model for the Universe: The Earth is at the center of the Universe. The heavens are ordered, harmonious, and perfect. The perfect shape is a sphere, and the ...
... • Aristotle was perhaps the most influential Greek philosopher. He favored a geocentric model for the Universe: The Earth is at the center of the Universe. The heavens are ordered, harmonious, and perfect. The perfect shape is a sphere, and the ...
Commentary on the Liquid Metallic Hydrogen Model of the Sun
... through the orientation of its liquid metallic hydrogen lattice. When the Sun is quiet, much of its interior is constantly being degassed through the action of the fast solar winds exiting at the poles. During this time, degassing is restricted over equatorial regions. Eventually, the Sun becomes ac ...
... through the orientation of its liquid metallic hydrogen lattice. When the Sun is quiet, much of its interior is constantly being degassed through the action of the fast solar winds exiting at the poles. During this time, degassing is restricted over equatorial regions. Eventually, the Sun becomes ac ...
A Solar Polar Imager Concept - The National Academies of
... has shown the advantage of a second viewpoint for predicting the arrival time of Earth-directed CMEs. The proposed SPI coronagraph would be able to observe Earth-directed CMEs from the high-latitude perspective. For events that are “halos” as viewed from Earth, this would give far better speed estim ...
... has shown the advantage of a second viewpoint for predicting the arrival time of Earth-directed CMEs. The proposed SPI coronagraph would be able to observe Earth-directed CMEs from the high-latitude perspective. For events that are “halos” as viewed from Earth, this would give far better speed estim ...
Stellar Activity
... rest of the star assumed to have no field) – Model line profiles with thermal, turbulent, collisional, and rotational broadening ...
... rest of the star assumed to have no field) – Model line profiles with thermal, turbulent, collisional, and rotational broadening ...
Scale Distances in the Solar System
... out other ‘large’ objects from its orbital zone, hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its elliptical orbit is much more eccentric than the eight planets. At times, Pluto is 49 AU from the Sun and at other times ...
... out other ‘large’ objects from its orbital zone, hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its elliptical orbit is much more eccentric than the eight planets. At times, Pluto is 49 AU from the Sun and at other times ...
Sorting the Solar System
... This is great! You are being real scientists. This is exactly what biologists, chemists, geologists, and astronomers do. And as new bacteria or birds or fossils are found, they use their knowledge of what has already been discovered to help them think about this new object. That's exactly what happe ...
... This is great! You are being real scientists. This is exactly what biologists, chemists, geologists, and astronomers do. And as new bacteria or birds or fossils are found, they use their knowledge of what has already been discovered to help them think about this new object. That's exactly what happe ...
Solar System Scale Activity
... other ‘large’ objects from its orbital zone; hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its ellipQcal orbit is much ...
... other ‘large’ objects from its orbital zone; hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its ellipQcal orbit is much ...
The Outer Solar System - Super Teacher Worksheets
... The first stop our tour of the outer solar system is the fifth planet, Jupiter. Next to the Sun, Jupiter is the second most massive object in our solar system. It’s bigger than three hundred Earths! Made up of hydrogen and helium and a few other gasses, there are violent wind storms that circle arou ...
... The first stop our tour of the outer solar system is the fifth planet, Jupiter. Next to the Sun, Jupiter is the second most massive object in our solar system. It’s bigger than three hundred Earths! Made up of hydrogen and helium and a few other gasses, there are violent wind storms that circle arou ...
Word format
... More Kuiper Belt objects may be discovered in future that rival Pluto in size and may even be considered for designation as dwarf planets. All of the planets revolve around the Sun in the same direction. If we were to look down on the solar system from above its north pole, all the planets would be ...
... More Kuiper Belt objects may be discovered in future that rival Pluto in size and may even be considered for designation as dwarf planets. All of the planets revolve around the Sun in the same direction. If we were to look down on the solar system from above its north pole, all the planets would be ...
pdf format
... More Kuiper Belt objects may be discovered in future that rival Pluto in size and may even be considered for designation as dwarf planets. All of the planets revolve around the Sun in the same direction. If we were to look down on the solar system from above its north pole, all the planets would be ...
... More Kuiper Belt objects may be discovered in future that rival Pluto in size and may even be considered for designation as dwarf planets. All of the planets revolve around the Sun in the same direction. If we were to look down on the solar system from above its north pole, all the planets would be ...
DO IT YOURSELF SIMPLE TEMPLATE FORMAT
... What shapes are planetary orbits? Our Solar System consists of many types of objects circling around the Sun, held in their orbits by gravity. Name all of the objects you can think of that orbit the Sun. Write down what you know about each one. This activity will look specifically at planets, which ...
... What shapes are planetary orbits? Our Solar System consists of many types of objects circling around the Sun, held in their orbits by gravity. Name all of the objects you can think of that orbit the Sun. Write down what you know about each one. This activity will look specifically at planets, which ...
ppt
... The excitation of turbulences decreases with shock velocity, while damping (by non-linear wave interactions and ion-neutral collisions) does not. ...
... The excitation of turbulences decreases with shock velocity, while damping (by non-linear wave interactions and ion-neutral collisions) does not. ...
Heliosphere
The heliosphere is the bubble-like region of space dominated by the Sun, which extends far beyond the orbit of Pluto. Plasma ""blown"" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates the Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical. The limited data available and unexplored nature of these structures have resulted in many theories.On September 12, 2013, NASA announced that Voyager 1 had exited the heliosphere on August 25, 2012, when it measured a sudden increase in plasma density of about forty times. Because the heliopause marks one boundary between the Sun's solar wind and the rest of the galaxy, a spacecraft such as Voyager 1 which has departed the heliosphere can be said to have reached interstellar space.