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WIMPs versus MACHOS
WIMPs versus MACHOS

... “We see it as Columbus saw America from the shores of Spain. Its movements have been felt, trembling along the farreaching line of our analysis, with a certainty hardly inferior to that of ocular demonstration” Sir John Herschel (referring to evidence for Neptune, 150 years ago) ...
Astronomy Unit Notes - sciencepowerpoint.com
Astronomy Unit Notes - sciencepowerpoint.com

... Name:___________________ ...
Power Point Link
Power Point Link

... this requires oxygen in the air and water, and there wasn’t any until… • Cyanobateria created oxygen as a waste gas. • Apparently it took nearly three billion years to build up this level of oxygen…then BANG!--The Cambrian Explosion ...
The Speed of Sound and Doppler Effect
The Speed of Sound and Doppler Effect

... Does sound travel faster in steel or liquid water? ...
Chapter 14 - Heritage Christian School
Chapter 14 - Heritage Christian School

... However, the idea that the Earth is the center of the universe runs contrary to ancient religious thought. This is because hell was considered to be at the center of the Earth; therefore, if Earth was the center of the universe, then hell would in fact be at the center of the universe. Secularists l ...
dark - The Institute of Mathematical Sciences
dark - The Institute of Mathematical Sciences

... When the Universe was young, it was nearly smooth and featureless. As it grew older and developed, it became organised. We know that our solar system is organized into planets (including the Earth) orbiting around the Sun. On a scale much larger than the solar system (about 100 million times larger) ...
Doppler effect File
Doppler effect File

... • Sketch a graph of frequency v time for the observer as the car passes ...
a space smile - Physique chimie Dijon
a space smile - Physique chimie Dijon

AstroProjectDay3
AstroProjectDay3

Teacher`s Guide Understanding: The Universe
Teacher`s Guide Understanding: The Universe

... world's great observatories and prime stargazing sites reveal how scientists survey the sky and track supernovas and black holes. ...
form b - University of Iowa Astrophysics
form b - University of Iowa Astrophysics

... Questions 19+20: As a class project, you make observations of a unusual binary star. One of the components is a spectral class G2V star (a twin of the Sun) and it is clearly moving in an orbit. You cannot detect the light from the other component of the binary, but from your measurements you deduce ...
session iii - Problems of Practical Cosmology
session iii - Problems of Practical Cosmology

... near-Earth asteroids. Primordial quark nuggets have been predicted to contain most of the baryonic number of the Universe. It has been suggested by J.E.Horvath to search for these nuggets in the asteroidal-mass range. Since the strange quark matter is expected to have a plasma frequency as high as 2 ...
Life Cycle of the Stars
Life Cycle of the Stars

... • When the core of the matter becomes hot enough, thermonuclear fusion begins. • This means that there is enough heat to turn hydrogen to helium. • Once this has happened a true star has been born. • The star shines with its own light. • A solar wind then blows away the rest of the dust and gas. ...
2.1 Hubble Space Telescope
2.1 Hubble Space Telescope

... Astronomers were surprised to find that the galaxies’ estimated masses were so small, and the Spitzer Space Telescope was called upon to make precise ...
Answers
Answers

The University of Georgia Department of Physics and Astronomy
The University of Georgia Department of Physics and Astronomy

... Mach-Zender interferometer shown in the figure. Light from a infrared laser (λ = 1.00µm) is split into two waves that travel equal distances around the arms of the interferometer. One arm passes through an electro-optic crystal, a transparent material that can change its index of refraction in respo ...
"Star Tracks", Leaflet for Royal Society Summer Exhibition
"Star Tracks", Leaflet for Royal Society Summer Exhibition

... Our research group at the University of Oxford seeks to discover how the Milky Way works as a machine and how it was assembled. The Milky Way is not special. In fact, there are at least billions of galaxies in the Universe very similar to our own. However, we are in the fortunate position of being a ...
The Island Universe of Immanuel Kant - EU-HOU
The Island Universe of Immanuel Kant - EU-HOU

... much farther galaxies could be measured. As can be easily noticed in the previous slide (right panel), Hubble law works very well: velocity/distance ratio remains constant in a wide range of these two quantities, particularly for more distant galaxies where the proper motions velocities become negli ...
PH607lec11
PH607lec11

Physics worksheets- P1 Topic 3 The Universe
Physics worksheets- P1 Topic 3 The Universe

... The boxes show the names and diameters of some different objects that astronomers can see in the sky. Draw lines to match up the names with the diameters. (You do not need to remember the sizes!) ...
Poor Pluto - Leslie Looney
Poor Pluto - Leslie Looney

... •! Planets are now defined •! Stars – Nuclear burning machines, usually turning hydrogen into helium •! Colors (temperatures: cold/red to hot/blue), •! Sizes (Jupiter-sized to 1000x the Sun) •! Masses (80x Jupiter to 100x the Sun) •! Ages (Just born to nearly the age of the Universe) ...
Scale - Physics
Scale - Physics

Cosmic Hierarchy 9.5, 9.6
Cosmic Hierarchy 9.5, 9.6

... 1) How did the solar system form? The solar nebula theory says that the Sun and planets formed from a swirling cloud of gas and dust that was pulled together by gravity. a) As the cloud becomes smaller the material will orbit ...
Gravitational potential energy
Gravitational potential energy

Supernova’s
Supernova’s

... (sometimes visible) ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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