almost circular and contained within a nearly-flat disc called the ecliptic plane. The four smaller inner planets; Mercury‚ Venus‚ Earth and Mars‚ also called the terrestrial planets‚ are primarily composed of rock and metal. The four outer planets‚ Jupiter‚ Saturn‚ Uranus and Neptune‚ also called the gas giants‚ are composed largely of hydrogen and helium and are far more massive than the terrestrials. 1.1 STATEMENT OF PROBLEM Simulation of solar system historically has been a major difficult terrain
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UNIT: Beyond the Solar System TOPIC: Planets A. Science Concept: Planets are the large celestial bodies which revolve around the sun in closed elliptical paths called orbits. Mercury‚ Venus‚ Earth and Mars are inner planets. Jupiter‚ Saturn‚ Uranus‚ and Neptune are outer planets. B. Science Processes: Communicating‚ Describing‚ Inferring C. Materials: Laptop‚ OHP‚ pictures‚ charts References: Science Web by Laarni S. Sta. Romana pages 426-432 III. Procedure:
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o quote the song “Drops of Jupiter” by the band Train‚ “Can you imagine no first dance‚ freeze dried romance‚ five-hour phone conversation‚ the best soy latte that you ever had… and me?” I first time I remember hearing this song was at the state dance team tournament in 2010. At the time I was a mere seventh grader‚ completely oblivious to my future and the events that were to come in the next few years. To say the least; I was innocent. That song changed my life. Somehow the words that Pat Monahan
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Solar disruption theory was one of several theories that emerged before the 18th century concerning the formation of the solar system. Solar disruption theory states that the collision of the sun with another stars caused debris to be ejected from its mass and these debris eventually became the planets. This theory was later discarded for the nebula theory of solar system formation. However there are some scientists that propose that it has some merit. The big question up until the 18th century
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understand how our own planet formed - How we came to be 2. 1st planet that was discovered (1995) - They track variations in the star’s spectrum (51 Pegasi) - Conclude that there is a companion orbiting the star • Min mass: 0.5 Mj (1mj= mass of Jupiter) • Orbiting at: 0.05 AU (1AU= distance from earth to sun) 3. Methods o Doppler Spectroscopy - Just like the star causes a planet to move in an orbit around it‚ the planet causes its host star to move - If a star is being orbited by a planet
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TELESCOPE VIEWING Planetarium show and Telescope viewing‚ is one of the best event I ever attended in our campus. Westconn hosted a planetarium show “A Closer look at Orion The Hunter” as well as telescope viewing of the Waxing gibbous Moon‚ Venus‚ Jupiter‚ Neptune‚ Uranus‚ autumn sky. The event was presented at the university’s Westside campus on Saturday‚ December 6th at 5pm. I chose this event to attend because I wanted to scrutinize about people’s behavior in communication manner. The presentation’s
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solar system; Pluto is the only planet that is smaller. Earth’s diameter is about 7‚200‚ while tiny Mercury has less than half of that size‚ about 3‚000 miles in diameter. Mercury‚ a planet‚ is smaller than Ganymede‚ a satellite revolving around Jupiter. One of the features of Mercury distinguishing it from other planets is that it has a different orbit loop. Whereas the orbit of most planets has the shape of a circle‚ the Mercury’s orbit has the shape of ellipse that looks like a stretched out
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there. In the end‚ it’s not very important how we classify the various objects in our solar system. What is important is to learn about their physical nature and their histories. Planet Order from the Sun The Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune |
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moons have orbits that are "backwards" (compared to their planet’s rotation) or highly inclined to their planet’s equator. Question 6 The region of our solar system between Mercury and Mars has very few asteroids‚ while the region between Mars and Jupiter has many asteroids. Based on what you have learned‚ what is the most likely explanation for the lack of asteroids between Mercury and Mars? There were very few planetary leftovers in this region‚ because most of the solid material was accreted
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The main difference between Planet Nine and Earth is the size‚Planet Nine is estimated at about ten times the size of earth‚but is not as big as some of the planets in our solar system like Jupiter and Neptune..Planet Nine is also a much colder and darker planet because it is so far from the sun that it gets no heat or
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