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Our Universe SPA-4101
Our Universe SPA-4101

... Star  and  planet  forma5on   Stars  form  from  the  gravita5onal  collapse   of  dense  interstellar  gas  clouds.  One  of  the     closest  star  forming  regions  to  the  Sun  is  the   Orion  nebula  –  which  glows  because ...
What`s Up - April 2016
What`s Up - April 2016

Scale Model of Solar System - Teaching Commons Guide for
Scale Model of Solar System - Teaching Commons Guide for

... momentum sends it far into space, although it slows down because of the Sun’s gravitational pull. Sometimes, comets come so close to the Sun, they just crash into it, instead of swinging around it. Well, they don’t really “crash,” because all the ice has evaporated long before they actually hit the ...
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File

... 21. This triangle was drawn as a triangulation to determine the distance to a tree across a river. The baseline was measured as 800 m and then angles carefully determined from each end to the tree. The scale drawing was made based on these measurements. The actual distance to the tree would be A. 7 ...
guide to orion 3-d flythrough
guide to orion 3-d flythrough

... The central area of the nebula is called the Trapezium cluster. It is dominated by four young, massive stars in a kite-like arrangement. The brightest of these stars, which has a luminosity 100,000 times that of the Sun, provides the energy that creates the nebula as we see it. It produces a flood o ...
OVERVIEW: Stars and space
OVERVIEW: Stars and space

... • to explain how stars are able to maintain their energy output for millions of years • to explain why the early Universe contained only hydrogen but now contains a large variety of different elements. Skills, knowledge and understanding of how science works set in the context of: • Our Sun is one o ...
Earth, Moon & Sun System
Earth, Moon & Sun System

... • The Earth is a sphere (ball shape). Because of this only half can be lit by the sun at any one time. ...
08Moon - NMSU Astronomy
08Moon - NMSU Astronomy

... Reflex motion of stars from Earth’s revolution • We talked about reflex motion of stars and Sun from Earth’s rotation (circles in the sky) • We talked about reflex motion of Sun from Earth’s revolution (different constellations at different times of year, seasons) • What about reflex motion of star ...
Nebulas & Stars
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... is PKS-2349 which is only about 1500 million light years away from Earth Quasars can live for a very long time scientists say that quasars that were discovered around 35 ...
Sections F and G
Sections F and G

... Most stars, such as the Sun, are only weak X-ray sources. But there are several hundred strong Xray emitting sources in the Galaxy. These are binaries which consist of a normal star filling its Roche lobe and a neutron star plus hot accretion disc. Near the neutron star, the strong magnetic field (~ ...
Brighter than the average star?
Brighter than the average star?

... Many popular astronomy books start by explaining how small and unimportant our Solar System is. The famous ‘Hitchhiker’s Guide to the Galaxy’ begins by describing our own star with the words “Far out in the uncharted backwaters of the unfashionable end of the Western Spiral arm of the galaxy lies a ...
gravity module homework - Temple University Sites
gravity module homework - Temple University Sites

... 1     Gravity is not just a force on planet Earth. Each planet has its own gravity, and each planet's gravity is different. Our moon has gravity too. So do the moons that circle other planets. The sun has gravity (lots of it). So do all of the other stars. In fact, everything has some gravity, but o ...
End of the line for a star like ours
End of the line for a star like ours

Powerpoint
Powerpoint

... • Interactive figure on “A more accurate model of the solar system” • The orbits and rotations of the planets will reappear in Chapter 7. • They are hard to display on a screen or projector • Today: Orbits of planets are very close to being in the same plane ...
Our Place in the Universe (Chapter 1) The Structure and Size of the
Our Place in the Universe (Chapter 1) The Structure and Size of the

... • Interactive figure on “A more accurate model of the solar system” • The orbits and rotations of the planets will reappear in Chapter 7. • They are hard to display on a screen or projector • Today: Orbits of planets are very close to being in the same plane ...
Lecture 19 The Milky Way Galaxy
Lecture 19 The Milky Way Galaxy

... •The Disk: - Contains most stars and dust - Contains most GMCs, so most star formation takes place in disk - Contains all open clusters, a few million to a billion years old - By proportion, the disk is thinner than a pizza crust (not deep dish!) ...
Our Planetary System 7.1 Multiple-Choice Questions 1) How does
Our Planetary System 7.1 Multiple-Choice Questions 1) How does

... A) Asteroids orbit the Sun while comets just float randomly around in the Oort cloud. B) Most asteroids are located much nearer to the Sun than most comets. C) It is thought that comets are far more numerous than asteroids. D) Asteroids are made mostly of rock and comets are made mostly of ice. Answ ...
Astronomy 100—Exam 1
Astronomy 100—Exam 1

... 9. Your friend, living on a planet 100 light-years away from the earth, has just sent to you a short message to inform you that she has just given birth to a baby. What is the age of the baby when you receive the message on the earth? A. The baby was just born. D. The baby is about 1 day old. B. The ...
Solar System
Solar System

... Ganymede is the largest moon of Jupiter and the largest moon in the entire solar system. It is composed of rock and water ice, and it has craters and possible earthquakes. Callisto is the most heavily cratered object in the solar system. It has a huge bull’s-eye crater called Valhalla, and its surfa ...
Elliptic Orbits
Elliptic Orbits

... Sun’s gravity causes it to deviate, it swings around the Sun, then recedes tending to another straight line path as it leaves the System. There is also the theoretical possibility of a parabolic orbit, going out to infinity but never approaching a straight line asymptote. However, this requires exac ...
The Milky Way
The Milky Way

... If an accreting White Dwarf exceeds the Chandrasekhar mass limit, it collapses, triggering a Type Ia Supernova. ...
titel - Maastricht University
titel - Maastricht University

... The line connecting a planet to the sun sweeps out equal areas in equal amounts of time. 3. Kepler's law of periods: The time required for a planet to orbit the sun, called its period, is proportional to the long axis of the ellipse raised to the 3/2 power. The constant of proportionality is the sam ...
Space Science Unit
Space Science Unit

... slide we will demonstrate the concept of parallax, which is the apparent change of a stars position in the sky. • The stars are not really moving, rather the Earth is and therefore we see ...
Carsten Denker - Center for Solar
Carsten Denker - Center for Solar

... Center for Solar–Terrestrial Research ...
Obliquity and precession of the equinoxes The angle ε between the
Obliquity and precession of the equinoxes The angle ε between the

... summer solar days. The Sun transits precisely at noon on local clocks on those days, but for many days after perihelion, the cumulative effect of consecutive short solar days causes the transit to occur earlier and earlier on the clock since the clock continues to measure out a constant 24 hour day. ...
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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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