Aubrie+Eaton


 * **Nebula**- Interstellar cloud of gas and dust || || [[image:http://ncse.com/files/images/607px-Eagle_nebula_pillars.jpg height="247" caption="external image 607px-Eagle_nebula_pillars.jpg"]] ||
 * external image 607px-Eagle_nebula_pillars.jpg || || The formation of a star, planets, etc. (a solar system) is thought to begin when gravity begins to pull together material from a nebula. ||
 * **Planetesimal**- Solid body reaching hundreds of kilometers in diameter


 * Planet**- A celestial body orbiting a star. ||  || Planetisimals formed as smaller particles collided and stuck together. Further growth continued through collisions and mergers of planetismals resulting in a smaller number of larger bodies: the planets.

Different elements and coumpounds were able to condense depending on their distance from the sun which impacted the compositions of the forming planets. ||
 * **Terrestrial planet**- The inner four planets of our solar system. || [[image:http://t3.gstatic.com/images?q=tbn:ANd9GcRCKSKR_br_d1wCEd2DlvizhTKDboXBW6c3NjSJO1j9CT1qQHtDAA width="341" height="148" caption="external image images?q=tbn:ANd9GcRCKSKR_br_d1wCEd2DlvizhTKDboXBW6c3NjSJO1j9CT1qQHtDAA"]] || The four inner planets are Mercury, Venus, Earth, and Mars. ||
 * **Gas giant**- A large planet that is not primarily composed of rock or other solid matter. ||  || As each gas giant acquired material from its surroundings, a disk formed in its equatorial plane, much like the disk of the early solar system. ||
 * **Satellite**- An object which has been placed into orbit such as the moon. ||  || Satellites formed from when matter coalesced in the disk. ||
 * **Asteroid**- A class of solar system bodies in orbit around the sun. ||  || Asteroids comprise the thousands of bodies that orbit the sun within the planetary orbits that are leftovers from the formation of the solar system. ||
 * **Asteroid belt**- A region in the solar system between the orbits of mars and Jupiter occupied by asteroids. || [[image:http://t3.gstatic.com/images?q=tbn:ANd9GcTIEflAYa_mx20k-z5c9vrlh01ZWc7l1EIlfqUNBumieKb-nrNXZQ width="300" height="168" caption="external image images?q=tbn:ANd9GcTIEflAYa_mx20k-z5c9vrlh01ZWc7l1EIlfqUNBumieKb-nrNXZQ"]] || As asteroids orbit they occasionally collide and break into fragments. ||
 * **Meteor**- A bright streak of light that appears briefly in the sky.


 * Meteoriod**- Boulder sized particle of debri. ||  || Meteors are produced when a meteoride burns up in Earth's atmosphere.

Meteorids are asteroid fragments or any other interplanetary material that falls toward Earth and enters Earth's atmosphere. ||
 * **Meteorite**- A natural object that impacts earth's surface. ||  || A meteorite is part of a meteoroid that does not completely burn up. ||
 * **Comet**- small icy bodies that have highly eccentric orbits around the sun and are remnants from solar system formation. || [[image:http://www.thunderbolts.info/tpod/2006/image06/060227comet.jpg width="298" height="157" caption="external image 060227comet.jpg"]] || Comets are made of ice and rock, and they range from 1-10 km in diameter. ||
 * **Nucleus**- Small solid core of a comet that releases gas and dust particles ||  || When heated, the nucleus forms the coma and tails. ||
 * **Coma**- An extended volume of glowing gas flowing from a comet's head. ||  || The coma is approximately 1 million km in length. ||
 * **Kuiper Belt-** A cluster of remnants from the solar system's formation. ||  || The kuiper belt extends from the orbit of Neptune to approx. 55 AU from the sun. ||
 * **Oort Cloud**- A spherical cloud of comets that is approximately 1 lightyear away from the sun. || [[image:http://t0.gstatic.com/images?q=tbn:ANd9GcQhlbp5NSFSsq1Vs5PVTGR4zRJsdDz3NO_K5UA-PVshhHC7vx4W2g width="240" height="227" caption="external image images?q=tbn:ANd9GcQhlbp5NSFSsq1Vs5PVTGR4zRJsdDz3NO_K5UA-PVshhHC7vx4W2g"]] || Astronomers believe that the matter comprising the Oort cloud formed closer to the Sun and was scattered far out into space by the gravitational effects of the giant planets early in the Solar System's Evolution. ||

Assignment 2: Obsidian is a type of igneous rock, which means it is formed from lava. When in contact with ocean water, it rapidly cools not allowing large crystals to form giving obsidian its smooth and glossy texture. Many different colors may be formed due to tiny air bubbles trapped within the rock as well as different trace elements. Silicon, iron, magnesium and sometimes cristobalite are examples of trace elements that change the color. Directions: Work with a partner to explain one example of an **interaction between 2** of the [|earth systems] we discussed in class. (Lithosphere, Hydrosphere, Atmosphere, Biosphere). The systems are described in your notes for unit 1. Your job is to **type one paragraph** explaining ** how they interact ** and to ** include at least 1 supporting image **. Don't forget to make sure that the completed assignment is copied onto both of your wikis for grading purposes along with the title: **ASSIGNMENT 1: Earth Systems Interactions**.
 * ASSIGNMENT 1: Earth Systems Interactions**

The Carbon Cycle: Carbon is released into the atmosphere by the burning of fossil fuels and respiration. Carbon is absorbed in the biosphere by the photosynthesis of plants, decay of dead organisms, and the buildup of rock overtime.
 * example: Biosphere and Atmosphere**
 * [[image:http://www.cgemc-carbonoffset.com/images/carbon_cycle_NASA.jpg width="400" height="318"]] ||
 * http://www.hawaii-lisa.com/uploaded_images/Lava-flows-downt-the-pali-to-the-ocean-USGS-773056.jpg ||