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THE DYNAMIC TRIO - Siemens Science Day
THE DYNAMIC TRIO - Siemens Science Day

... Solar System – The solar system includes the Sun and everything that orbits it. This includes eight planets and their natural satellites such as Earth’s Moon; dwarf planets such as Pluto and Ceres; asteroids; comets and meteoroids. Sun – a star made up of 92% hydrogen and 7.8% helium, which is at th ...
The Solar System: The Sun and the Planets
The Solar System: The Sun and the Planets

Space by Clare and Emma D.C.
Space by Clare and Emma D.C.

... planet in the solar system not to be named after a Greek or Roman deity. ...
1 - BYU Physics and Astronomy
1 - BYU Physics and Astronomy

... 56. The "Drake Equation" (a) expresses the amount of energy radiated by material falling into a black hole, (b) can be use to calculate the maximum possible size for an object of varying brightness, (c) is used to predict the occurrence of eclipses, (d) yields a crude estimate of the number of extra ...
molecular clouds
molecular clouds

... Protostar Becomes A Star • Once sufficient temperature (>= 10 million degrees K) and pressure is reached in the core of the protostar, nuclear fusion begins and the protostar has now officially become a star ...
Dating the Universe
Dating the Universe

... ! The outer planets were massive enough (especially Jupiter and Saturn) to accrete gases from the nebula ! But the inner planets were not! ! Jupiter may have prevented the formation of another terrestrial planet in the asteroid belt ...
Solar System Formation
Solar System Formation

... unstable, i.e., when Q ~ MstarH/(Mdr) < 1 where Md is disk mass within r (Kuiper 1949, Cameron 1978) This would form planets very quickly (orbital timescales, or few hundred years) with a characteristic scale H and so with a mass of around Mjupiter [=(H/r)3M* assuming H/r=0.1] It is not clear if a c ...
Conversations with the Earth
Conversations with the Earth

... • You need “metals” to make planets –Metals are elements heavier in mass than helium ...
Summary of week 1:
Summary of week 1:

... has insufficient mass to become a star (< 80 Jupiter masses) or a brown dwarf (< 13 Jupiter masses). Brown dwarf: A “failed star”, that is, an object more massive than a planet, but insufficient to become a star. These objects typically have fusion reactions involving deuterium early in their life c ...
Life Cycles of Stars
Life Cycles of Stars

Lesson 1 | Scientific Inquiry
Lesson 1 | Scientific Inquiry

... 1. The inner planets are those closest to the Sun. 2. The inner planets are made of rocky and metallic materials. a. Because of its small mass, Mercury’s gravity is not strong enough to hold gases to its surface. b. Venus is covered by a thick layer of clouds. c. The high temperatures on Venus are c ...
The Sun
The Sun

... Gravity and Pressure • Self-regulating… • Higher fusion rate would expand star, lowering core’s self-gravity and thence density, pressure, temperature and thus lowering fusion rate. And vice versa ...
General Proper es of the Terrestrial Planets
General Proper es of the Terrestrial Planets

... •  All  the  planets  revolve  around  the  Sun  in  a  counterclockwise   (prograde)  direcCon.  As  they  move  in  their  orbits,  they  also  change   their  poisCon  in  the  sky.   •  The  apparent  moCon  of  the  planets  in   ...
Secular Increase of the Astronomical Unit: a Possible Explanation in
Secular Increase of the Astronomical Unit: a Possible Explanation in

... now, several authors have discussed a redefinition of the system of astronomical units, e.g., Huang et al. (1995); Standish (2005); Klioner (2008); Capitaine and Guinot (2009). By using equations (1) and (24), we obtain GMSun in SI units, and so far GMSun is conventionally regarded as being a “fixed ...
Astronomy Study Guide
Astronomy Study Guide

... • Moon o orbits the Earth in about 27 days o The moon is currently thought to have formed when a Mars-size object collided with Earth. The material ejected from Earth’s atmosphere then came together under the force of gravity to form the moon. o The moon rotates on its axis at the same rate that it ...
Solar System Test Review - Garnet Valley School District
Solar System Test Review - Garnet Valley School District

... going around the sun or the moon going around the earth. 11. The _________________________ states the sun, earth and other objects in the solar system formed from a rotating cloud of gas, called a nebula, about 4.5 billion years ago. 12. The _________________________ is the orbital point at which th ...
The Sun, at a mean distance of 92.96 million miles, is the closest
The Sun, at a mean distance of 92.96 million miles, is the closest

... huge sphere of mostly ionized gas, supports all life on Earth. It powers photosynthesis in green plants, and is ultimately the source of all food and energy. In fact, the Sun produces in 1 second the U.S. energy needs for 90,000 years! The connection and interactions between the Sun and Earth drive ...
Rendezvous with Rosetta
Rendezvous with Rosetta

... Solar System, Kuiper belt & Oort cloud • Distance from Sun: 30 Trillion km! • Size: Completely surrounding Solar System! • Material & Shape: The Oort Cloud is not disk-shaped like the Kuiper Belt; it’s round like a ball,It completely envelops the sun and the rest of our solar system. Billions of ic ...
Sun
Sun

... Whereas Alpha Centauri is 4.3 light years distant, the Sun is only 8 light minutes away from us. Consequently, astronomers know far more about the properties of the Sun than about any of the other distant points of light in the universe. A good fraction of all our astronomical knowledge is based on ...
Session 5 – Evidence for a young earth
Session 5 – Evidence for a young earth

... University of California modeled the moon’s interior and found that it would have frozen in only 30 million years, which is less than one percent of the age assigned by the nebular theory. There are several answers they give to try to explain this, radioactive decay heating the planet, tidal forces ...
Our Solar System Exhibit Guide
Our Solar System Exhibit Guide

... solar panels, antennae. How do you think the rover is powered? It gets energy from ...
We especially need imagination in science. It is not all mathematics
We especially need imagination in science. It is not all mathematics

... Four dusty protoplanetary disks around young stars in the Orion nebula. The red glow in the center of each disk is a newly formed star, roughly a million years old. Each image is a composite of emission lines from ionized oxygen (blue), hydrogen ...
stars and planets
stars and planets

... 4.2 light years away.The Sun is part of a single star system but there are also binary and multiple stars where 2 or more stars orbit around each other. • Stars are born inside clouds of gas and dust known as nebulas which exist throughout the galaxy. Some nebulas form from the gravitational collaps ...
Uranus is considered to be the brightest planet in our solar
Uranus is considered to be the brightest planet in our solar

... planets live. In our neighborhood there are nine planets. All of which are very different, just like people. There are also thousands of comets and asteroids that come to visit us. Our solar system is a very elaborate place. So let’s ...
Properties of Earth (6.E.1.2)
Properties of Earth (6.E.1.2)

... last about 13 Earth days. The planet is in a region the scientists call The Goldilocks Zone. This zone is at a distance from Gliese 581 where temperatures on the planet range from 0 C and 40 C. These temperatures suggest that the planet has some conditions similar to those on Earth. ...
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History of Solar System formation and evolution hypotheses



Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.
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