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SDO | solar dynamics observatory
SDO | solar dynamics observatory

... located. Remind them that Earth rotates counterclockwise and where they decided that the summer and winter solstices are located. Optional: Place signs for the months around the room in the correct spot. Add zodiac constellation signs as well. To conclude have students repeat the motions of a year o ...
THE HERTZSPRUNG-RUSSELL DIAGRAM (H
THE HERTZSPRUNG-RUSSELL DIAGRAM (H

... NOTE: Absolute Magnitude IS THE SAME THING AS LUMINOSITY ON THE GRAPH DEFINE: absolute magnitude (Pg. 372 if you don’t know) ...
ASTRONOMY
ASTRONOMY

... E. Fill in the blank. 1. There are about __________ stars you can see at night. 2. Latitudes on earth are like ____________ in space. 3. There are about ________ constellations. 4. The north-star has a magnitude of _____________. 5. The point directly overhead is called the ______________. 6. Polar ...
Week 3: Kepler`s Laws, Light and Matter
Week 3: Kepler`s Laws, Light and Matter

... • As we discussed last time, the apparent retrograde motion (a reversal in direction of motion) of the planets is caused by the fact the Earth and the other planets revolve around the Sun at different velocities. The Ptolemaic model of geocentric system, unsuccessfully tried to explain this motion b ...
Units
Units

... A process for understanding and predicting What about facts? will it rain tomorrow? what will be on the quiz? what will happen if…? ...
Supernovae: Heavy Elements
Supernovae: Heavy Elements

... A Different Kind of Big Bang • The pressure of these neutrinos causes part of the imploding core to rebound • This rebound comes in the form of a shockwave, which rips through the still collapsing outer core • The collapsing outer shell is met by the shockwave and then by a rarefaction wave and is ...
The Seven African Powers of Creation
The Seven African Powers of Creation

... of general relativity predicts that a sufficiently compact mass will deform spacetime to form a black hole. Around a black hole there is a mathematically defined surface called an event horizon that marks the point of no return. It is called "black" because it absorbs all the light that hits the hor ...
1. Heraclides of Pontus
1. Heraclides of Pontus

... explain retrograde motion. Epicycle: An orbit within an orbit. In order to explain retrograde motion, he said that planets orbit in small circles as they orbit around the solar system. Epicycles were used to explain retrograde motion. This model was very complicated, but could accurately predict the ...
DAY AND NIGHT, SEASONS
DAY AND NIGHT, SEASONS

... and day and night on two exoplanets. 1: An exoplanet that orbits with the same face to its star at all times. This type of planet is similar to the way in which we always see the same face of the Moon, and the exoplanet is described as ‘tidally locked’ to its star. Such planets rotate slowly. The t ...
how to precisely measure astronomic periods of time
how to precisely measure astronomic periods of time

... eclipses – which was of great importance for ancient societies – is also part of such considerations: A solar eclipse never happens at the times of lunar standstills. It rather occurs (like the lunar eclipses, Figure 11) in between the standstills. An adaption of Formula (1) holds in good approximat ...
Isaac Newton and the Laws of Motion and Gravitation 2
Isaac Newton and the Laws of Motion and Gravitation 2

... in the constellation Gemini, he saw a star appeared like a fuzzy disk rather than a point. – He initially thought it was a comet. But subsequent observation by him and others indicated that it was a planet, located beyond Saturn and not known until then. It was named Uranus. – Hershel became a promi ...
Coursework 6 File
Coursework 6 File

... star acting to tidally deform an orbiting planet can also act to limit the size of stable orbits for a satellite gravitationally bound to the planet. 1. A planet of mass Mp forms around a star with mass M∗ with separation r, and an orbiting satellite forms around the planet with semimajor axis asat ...
2.1.1 Study: The Big Bang Theory
2.1.1 Study: The Big Bang Theory

... Our sun formed about 5 billion years ago, and is about halfway through its life cycle. At the end of its cycle, it will expand to form a red giant, then collapse into a white dwarf. Stars larger than our sun will either supernova and then form a neutron star, or, if they are very large, supernova an ...
ppt
ppt

... • Observationally, one way to get a good “look” into the interior is using helioseismology  Vibrations on the surface result from sound waves propagating through the interior ...
Galaxy Notes Presentation
Galaxy Notes Presentation

... giant spiral galaxy including our Sun  The disk’s diameter is 100,000 light years  Mass is 1,000 to 2,000 billion times the mass of the Sun  The Sun lies a little more than 30,000 light years from the center  Cannot actually count the number of stars in the galaxy, can estimate as roughly 100 bi ...
Chapter 24 sun and light
Chapter 24 sun and light

... • The energy of an object is equal to its mass X the speed of light squared ...
L  ,sl = (10
L ,sl = (10

... STAR MAGNITUDES, LUMINOSITIES, AND FLUXES Distant Star Sol & Earth ...
Universe Standards - Harvard
Universe Standards - Harvard

Summer 2013, Vol. 2, No. 2 - CAAUL
Summer 2013, Vol. 2, No. 2 - CAAUL

... I would like to invite you to read the provocative and beautiful book The dimensional forms - and, behold dear reader, now you have my discovery in Sleepwalkers, by Arthur Koestler1. I shall not discuss Koestler's metaphor of your hands!...' The point is this. One can construct any number of regular ...
Unit 8 Chapter 29
Unit 8 Chapter 29

... E=mc2 Energy = mass x the speed of light squared Because the star is a place of intense heat and pressure, the atoms are torn apart into their component nuclei and electrons. By using Einstein's equation, astronomers were able to explain the huge quantities of energy produced by the sun. The sun cha ...
Introduction
Introduction

... Nearly all ancient civilisations practised astronomy at some level – Time of day or night – Seasons ...
Lecture 20: Formation of Planets, Exoplanets 3/30
Lecture 20: Formation of Planets, Exoplanets 3/30

... Jupiter would reduce Sun’s light by 1%; Earth reduces by .01% “easy” (done by 7th grader at NIU Science Fair) once spotted can also analyze Doppler shift and try and observe atmosphere PHYS 162 ...
Chapter 02
Chapter 02

... As a result of precession, the celestial north pole follows a circular pattern on the sky, once every 26,000 years. We are lucky to live at a time when a fairly bright star (Polaris, magnitude 2) is near the north celestial pole. It will be closest to Polaris ~ A.D. 2100. ...
Stellar Properties
Stellar Properties

... If too far for Parallax: Apparent brightness of the stars and inverse square law! ...
January 14 - Astronomy
January 14 - Astronomy

... during the course of a day. (Where does it rise, where does it cross the meridian, and where does it set.) ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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