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Stars and Galaxies By: Ellen Wertz and Sarah Broge
Stars Stars appear as fixed luminous points in the sky at night. Stars first start out as a protostar. Next comes the Fusion Ignition stage. Then Main Stage. Next onto the Super giant/Red giant. Mostly referred to the Red Giant. The main stage is turned into the Red giant because it runs out of fuel. And lastly it will then turn into the white dwarf/Black Hole.
Red Dwarfs Can range from hundred times smaller than the sun, to only a little bit smaller. Because the Red Dwarfs are so small they burn fuel very slowly which allows them to live longer. They could live up to millions maybe even billions of years before the fuel burns out. Red Dwarfs are red because they burn only a little bit of fuel which makes them less hot. They are also the most common star in the outer space.
Yellow Star and Blue Stars Yellow Star: Medium stars like the Yellow Stars are yellow because they have a medium temperature. Their higher temperatures make the star burn more fuel faster. The gas from the Yellow Star creates a cloud called the Planetary Nebula. Blue Giant: Very large and compact. They burn fuel quickly which makes them have a very high temperature. The Blue Giant is a very bright star. Scientists can find new stars forming because the blue giants live for a short time.

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A meteoroid is a small rocky or metallic object traveling through space. Most meteoroids range in size from small grains to 1 meter and are fragments from comets or asteroids. When meteoroids enter the Earth's atmosphere, friction and compression cause them to heat up and glow - appearing as "shooting stars" or meteors. If they survive atmospheric entry and reach the ground, they are called meteorites.

Meteorites by James
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A meteorite hitting Earth could have major environmental consequences depending on where it lands. If it hits land, it could cause earthquakes, lower global temperatures by blocking the sun with dust for months, and disrupt power systems. If a meteorite hits the ocean it could trigger tsunamis across the ocean as well as hurricanes, again block the sun for months, cause earthquakes, and disrupt power. On average, 38,000 meteorites have hit Earth, with impacts concentrated at the poles. The meteorite that formed the Grand Canyon was around 30 meters wide and weighed 100,000 tons, entering the atmosphere at 20 km per second.

meteorspacemeteorites
Stars And Galaxies
Stars And GalaxiesStars And Galaxies
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1. Stars form from nebulae, which are dusty clouds in space. They begin as protostars and then become main sequence stars like our sun or massive stars. 2. After billions of years, main sequence stars become red giants as they run out of hydrogen fuel. Massive stars become red supergiants. 3. When stars die, red giants form planetary nebulae and red supergiants explode as supernovae. The remains of stars form neutron stars, black holes, white dwarfs or black dwarfs.

 
by asdf
Giant Star and Super Giant Star Giant Star: Many of the stars in the sky are Giant stars. They glow very brightly. When the sun becomes a giant star it will be seen farther away than it is now. Super Giant Star: It is the same thing as a Giant star, but bigger. If this kind of star were to replace the sun it would extend all the way to Uranus. As the star runs out of fuel then it will start to burn out.
Galaxies Galaxies: large systems of stars and interstellar matter typically containing several million to some trillion stars of masses between several million and several trillion times of our Sun of an extension of a few thousands to several 100,000 light years typically separated by millions light years distance.  They come in a variety of flavors: Spiral, lenticular, elliptical and irregular. Besides simple stars  they typically contain various types of star clusters and nebulae.
Spiral and Lenticular Spiral consist of two major components: a large flat disk usually containing interstellar matter, and young star clusters, and associations. The pattern that these galaxies make in the disk are most probably transient phenomena only cause by gravitational interaction with neighboring galaxies. The young stars are population I and the old bulge stars are population II.  Lenticular are basically spiral galaxies without spiral structure. Smooth disk galaxies where stellar formation has stopped long ago because interstellar matter was used up. They only consist of old bulge population II stars. Can hardly be distinguished from elliptical observantly.
Elliptical and Irregular Elliptical galaxies are actually of ellipsoidal shape and it is now quite safe from observation that they are usually triaxial or known as cosmic footballs refered to by Paul Murdin, David Allen, and David Malin.  Irregular is often due to distortion by the gravitation of their intergalactic neighbors these galaxies do not fit well into the scheme of disks and ellipsoids but exibit peculiar shapes. A subclass  of distorted disks is however frequently occurring.

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Comets, asteroids & meteors
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Comets and asteroids are remnants from the formation of the solar system. Comets originate from the Kuiper Belt and Oort Cloud and are icy bodies, while asteroids originate from the Main Asteroid Belt and are rocky fragments. Both have irregular shapes and sizes ranging from 1-100 km. Comets have highly elliptical orbits with periods of 75 years to millions of years, while asteroids have more rounded orbits with periods of 1-100 years. When a meteoroid from space enters the atmosphere, it becomes a meteor or "shooting star"; any fragments that reach the ground are called meteorites.

meteoritecometsmeteors
Meteor, Meteorite, Meteoroids
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This lesson plan aims to teach students about meteoroids, meteors, and meteorites. It will begin with a motivation activity to familiarize students with related terms. Students will then learn about the differences between meteoroids, meteors, and meteorites - specifically what happens when a meteoroid enters Earth's atmosphere. The lesson emphasizes the importance of perseverance in achieving goals by relating shooting stars to making wishes come true through hard work. To evaluate learning, students will define and differentiate key terms and concepts in exercises.

semi-detailed lesson planmeteoroidmeteorites
Comets, meteors, and asteroids
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Comets, meteors, and asteroids

This document discusses comets, meteors, asteroids, and the moon. It provides details on their composition, sizes, orbits, and the potential effects of large impacts. A large comet impact would likely only injure humans, while the largest meteor ever could endanger humanity. The largest known asteroid impact 65 million years ago caused the extinction of dinosaurs. A second moon would result in bigger tides and more frequent solar eclipses.

Work Cited &quot;big star.&quot;  a1star.com . N.p., n.d. Web. 1 Jan. 2010. <a1star.com/images/big_stars.jpg>.  &quot;monocerotis.&quot;  blogspot.com . N.p., n.d. Web. 15 Jan. 2010. <2.bp.blogspot.com/_YjAa4cW4wmQ/SyZC6KMhyRI/AAAAAAAAAQY/cR_YrPfpa1E/s400/Light+Echoes+From+Red+Supergiant+Star+V838+Monocerotis+-+December+2002.jpg>.  &quot;red dwarf.&quot;  wolflodge.org . N.p., n.d. Web. 13 Jan. 2010. <www.wolflodge.org/bluestar/h_red &quot;red_super_star.&quot;  wikimedia . N.p., n.d. Web. 15 Jan. 2010. <upload.wikimedia.org/wikipedia/en/ &quot;space-7.&quot;  wordpress.com . N.p., n.d. Web. 13 Jan. 2010. <evidentfuture.files.wordpress.com/2009/10/space-7.jpg>.  &quot;stars and galaxies.&quot;  wordpress.com . N.p., n.d. Web. 13 Jan. 2010. <thenotscientist.files.wordpress.com/2008/03/stars-and-galaxies.jpg>. &quot;Stars.&quot;  physics.csbsju.edu . N.p., n.d. Web. 13 Jan. 2010. <www.physics.csbsju.edu/astro/C  &quot;yellow star.&quot;  blogspot.com . N.p., n.d. Web. 13 Jan. 2010. <4.bp.blogspot.com/_7wmnwYG9rgs
Work cited  http://hubblesite.org/gallery/album/galaxy/pr2007041a/large_web/ www.wikiwak.com/image/Antennae+galaxies+xl.jpg http://eponym327.blogspot.com/2008_05_01_archive.html http://www.nasa.gov/images/content/210307main_n1132_composite_665x639.jpg http://www.bcssa.org/newsroom/scholarships/great8sci/Photos/Space_Photos/Irregular_Galaxy.JPG Galaxies.&quot;  Students for the Exploration and Development of Space (SEDS) . N.p., n.d. Web. 15 Jan. 2010. <http://seds.org/MESSIER/galaxy.html

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Stars And Galaxies

  • 1. Stars and Galaxies By: Ellen Wertz and Sarah Broge
  • 2. Stars Stars appear as fixed luminous points in the sky at night. Stars first start out as a protostar. Next comes the Fusion Ignition stage. Then Main Stage. Next onto the Super giant/Red giant. Mostly referred to the Red Giant. The main stage is turned into the Red giant because it runs out of fuel. And lastly it will then turn into the white dwarf/Black Hole.
  • 3. Red Dwarfs Can range from hundred times smaller than the sun, to only a little bit smaller. Because the Red Dwarfs are so small they burn fuel very slowly which allows them to live longer. They could live up to millions maybe even billions of years before the fuel burns out. Red Dwarfs are red because they burn only a little bit of fuel which makes them less hot. They are also the most common star in the outer space.
  • 4. Yellow Star and Blue Stars Yellow Star: Medium stars like the Yellow Stars are yellow because they have a medium temperature. Their higher temperatures make the star burn more fuel faster. The gas from the Yellow Star creates a cloud called the Planetary Nebula. Blue Giant: Very large and compact. They burn fuel quickly which makes them have a very high temperature. The Blue Giant is a very bright star. Scientists can find new stars forming because the blue giants live for a short time.
  • 5. Giant Star and Super Giant Star Giant Star: Many of the stars in the sky are Giant stars. They glow very brightly. When the sun becomes a giant star it will be seen farther away than it is now. Super Giant Star: It is the same thing as a Giant star, but bigger. If this kind of star were to replace the sun it would extend all the way to Uranus. As the star runs out of fuel then it will start to burn out.
  • 6. Galaxies Galaxies: large systems of stars and interstellar matter typically containing several million to some trillion stars of masses between several million and several trillion times of our Sun of an extension of a few thousands to several 100,000 light years typically separated by millions light years distance. They come in a variety of flavors: Spiral, lenticular, elliptical and irregular. Besides simple stars they typically contain various types of star clusters and nebulae.
  • 7. Spiral and Lenticular Spiral consist of two major components: a large flat disk usually containing interstellar matter, and young star clusters, and associations. The pattern that these galaxies make in the disk are most probably transient phenomena only cause by gravitational interaction with neighboring galaxies. The young stars are population I and the old bulge stars are population II. Lenticular are basically spiral galaxies without spiral structure. Smooth disk galaxies where stellar formation has stopped long ago because interstellar matter was used up. They only consist of old bulge population II stars. Can hardly be distinguished from elliptical observantly.
  • 8. Elliptical and Irregular Elliptical galaxies are actually of ellipsoidal shape and it is now quite safe from observation that they are usually triaxial or known as cosmic footballs refered to by Paul Murdin, David Allen, and David Malin. Irregular is often due to distortion by the gravitation of their intergalactic neighbors these galaxies do not fit well into the scheme of disks and ellipsoids but exibit peculiar shapes. A subclass of distorted disks is however frequently occurring.
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  • 10. Work cited http://hubblesite.org/gallery/album/galaxy/pr2007041a/large_web/ www.wikiwak.com/image/Antennae+galaxies+xl.jpg http://eponym327.blogspot.com/2008_05_01_archive.html http://www.nasa.gov/images/content/210307main_n1132_composite_665x639.jpg http://www.bcssa.org/newsroom/scholarships/great8sci/Photos/Space_Photos/Irregular_Galaxy.JPG Galaxies.&quot; Students for the Exploration and Development of Space (SEDS) . N.p., n.d. Web. 15 Jan. 2010. <http://seds.org/MESSIER/galaxy.html