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•TODAY •Chapter 5/10: The Sun Required: Sec. 1
•TODAY •Chapter 5/10: The Sun Required: Sec. 1

... The Sun is 150 million km (93,000,000 miles) away=1AU ! Distance found during the Transit of Venus, 1761 The Sun 109 times larger than Earth ! ...from its angular size It is 333,000 times more massive than Earth ! Newton’s Law of Gravity lets us measure mass Its surface temperature is 5,800 Kelvin ! ...
Astronomy 103: Midterm 2 Answers Correct answer in bold
Astronomy 103: Midterm 2 Answers Correct answer in bold

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Anomalous diffusion in generalised Ornstein
Anomalous diffusion in generalised Ornstein

... The objects which are produced by gravitational collapse will be termed juvenile planets. They must initially have a composition which is similar to that of the interstellar medium. They would have to undergo a radical transformation to become rocky or icy planets. We propose that such transformatio ...
Chapter 11
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... the MSW theory, the observed neutrino deficit could be the result of neutrino oscillations (neutrinos changing from one type to another during their flight from the Sun to Earth). 6. The SNO experiment uses the properties of heavy water to detect all three types of neutrinos. In 2002 it found that ...
Solar system - Wikimedia Commons
Solar system - Wikimedia Commons

... collided to form larger bodies (planetesimals) of roughly 5 km in size; then gradually increased by further collisions at roughly 15 cm per year over the course of the next few million years.[21] The inner Solar System was too warm for volatile molecules like water and methane to condense, and so th ...
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APSU_1000_35 Liberal Arts Univ. Life

... The Sun converts 600,000,000 tonnes of H into 596,000,000 tonnes of He every second! The difference in mass is the energy produced according to E = mc2. This is only a 0.67% efficient conversion! The Sun has enough hydrogen in its’ core to last another 5 billion years before it runs out Energy is on ...
Chapter 2 - AstroStop
Chapter 2 - AstroStop

... A) The time to complete one revolution of its orbit is dependent upon the size or radius of the planet. B) The smaller the radius of a planet, the more rapidly it rotates on its axis. C) The smaller the orbit, the longer it takes for the planet to complete one revolution. D) The larger the orbit, th ...
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... orbiting it. • Asteroids are rocky, and most orbit between orbits of Mars and Jupiter. • Comets are icy, and are believed to have formed early in the solar system’s life. • Major planets orbit Sun in same sense, and all but Venus rotate in that sense as well. • Planetary orbits lie almost in the sam ...
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... [v = distance/time = 584 million miles / ((24 hours/day)x(365 days/year)) = 66,700 mi/hr] Now, with the distance to the Sun and our velocity around the Sun known, we can use Newton’s equations, to calculate the mass of the Sun at 2.2 billion trillion tons! In fact, the Sun is 99.98% of the mass of t ...
The Sun - MsLeeClass
The Sun - MsLeeClass

... 3. When you are done you will discuss what you learned with a person with a different number than you 4. Working together you will answer the questions below. You may use your notes. You and your partner will turn in one answer sheet. One of you will write and one of you will read the question/check ...
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... Neutrinos are subatomic particles released as one of the products o f the fusion reactions in the centre of the Sun. They have spin, zero charge, probably a very tiny mass, and very high energy. They are so weakly interacting that most would easily pass through a light year o f solid lead. An unimag ...
Black Holes, Part 3, Dark Energy
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... A hydrogen sphere of the enormous size of UY Scuti is not possible to exist. The mass of such a gas sphere would be billions of times greater than it is. Its gravity would be so great that its atoms would be crushed long before the star became as big as it is. A gas sphere that's nearly 2.4 billion ...
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... distribution  of  weight  with  distance  from  the  axis.  Note  that  both  linear  momentum  and  angular  momentum are "conserved," that is, they do not change without some outside force changing them.   ...
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... thousand light-years. Most are actually within a few hundred light-years, with the exception of a few intrinsically brilliant stars that are many thousands of times more luminous than the Sun. For comparison, the Sun is about 26,000 light-years from the galactic center, orbiting on an outer spiral a ...
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... a) 4 hydrogen nuclei form 1 helium nucleus plus energy. b) 2 hydrogen nuclei form 1 helium nucleus plus energy. c) 6 hydrogen nuclei form 1 helium nucleus, 1 carbon nucleus plus energy. d) 3 hydrogen nuclei form 1 helium nucleus plus energy. e) 4 hydrogen nuclei form 1 helium nucleus, 1 carbon nucle ...
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... of such a tightly bound orbit requires a stellar encounter much closer than expected in the solar system’s current galactic environment. Only a small range of encounter geometries are capable of perturbing a scattered Kuiper belt-like orbit to this more Oort cloud-like orbit. As an example, an encou ...
`Daniel` – The Colonization of Tiamat
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... focused on the Hubble Space Telescope, concluding that its maximum range was a meager 357.14 light years. Recent upgrades, including digital imaging, may have increased that distance 10-fold, but even 3571.4 light years is still far short of ever being able to see galaxies that are millions or billi ...
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... around after the star forms gathers together into smaller clumps. They get caught in the gravitational field of the larger Sun, forming the “solar” system.  There are eight planets in our solar system: (and a few dwarf planetoids like Pluto).  Planets are divided into inner and outer. The inner pl ...
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... (another transit of Jupiter by Venus). In addition, as Mercury and Venus are frequent actors in these dramas, many of them take place unobservably near the Sun. In order to understand, and perhaps forecast, these celestial encounters one needs to appreciate that they involve physical bodies similar ...
Lecture 4 January 31 - Center for Astrophysics and Space
Lecture 4 January 31 - Center for Astrophysics and Space

... There is a VERY fast increase in nuclear energy production above 1,000,000K. At 15,000,000K in the core nuclear power generated finally balanced the luminosity from the surface. That’s the equilibrium we are still in. ...
The Motion of Celestial Bodies
The Motion of Celestial Bodies

... circle (deferent) which is in turn centered on a point slightly displaced from the Earth’s center. This geocentric world picture stood the ground for 1400 years until Nicolaus Copernicus on his death bed in 1543 introduced the heliocentric system with the Sun in the middle, but it took more than 100 ...
Geocentric vs. Heliocentric - Answering the Debate 2014
Geocentric vs. Heliocentric - Answering the Debate 2014

... long-held notion that the Earth was the center of the Solar system, but he did not question the assumption of uniform circular motion. Thus, in the Copernican model the Sun was at the center, but the planets still executed uniform circular motion about it.  As we shall see later, the orbits of the ...
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Solar System



The Solar System comprises the Sun and the planetary system that orbits it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets, with the remainder being significantly smaller objects, such as dwarf planets and small Solar System bodies such as comets and asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane. All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc, populations of trans-Neptunian objects composed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceres and the trans-Neptunian objects Pluto and Eris. In addition to these two regions, various other small-body populations, including comets, centaurs and interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed ""moons"" after the Moon. Each of the outer planets is encircled by planetary rings of dust and other small objects.The solar wind, a stream of charged particles flowing outwards from the Sun, creates a bubble-like region in the interstellar medium known as the heliosphere. The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
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