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Chapter 13 - USM People Pages
Chapter 13 - USM People Pages

... has mass M and asteroid 2 has mass 2M. The two asteroids are released from rest with distance 10R between their centers. What is the speed of each asteroid just before they collide? Hint: You will need to use two conservation laws. ||| Two Jupiter-size planets are released from rest 1.0 * 1011 m apa ...
Eppur Si Muove – Stellar Parallax?
Eppur Si Muove – Stellar Parallax?

... 61 Cygni has a huge proper motion – 5 arcseconds per year – making it a likely candidate for being nearby ...
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Document

... Estimate the intensity of the radiation emitted per unit area from a star if it’s effective surface Temp is 6000K Estimate the energy emitted from a star if its peak wavelength is 600nm. Total power radiated Power output = E x surface area of star Surface area of a star = 4  R 2 Where R is the rad ...
Types of Stars
Types of Stars

3/r -- this talks about the surface area vs the volume of a planet
3/r -- this talks about the surface area vs the volume of a planet

... mean solar time is defined so that noon occurs at the time which the sun would cross the meridian on average mean and solar times agree only 4 times a year - mean time can be as much as 17 min behind or 15 min ahead the sun. Both solar and mean times are LOCAL times, different in each city. (time zo ...
Week 10
Week 10

... Thought Question: On Earth, the parallax angle measured for the star Procyon is 0.29 arcseconds. If you were to measure Procyon’s parallax angle from Venus, what would the parallax angle be? (Note: Venus’ orbit is smaller than Earth’s orbit.) A. More than 0.29 arcseconds B. 0.29 arcseconds C. Less ...
oct8
oct8

... Suppose every human being on Earth turned on 1000, 100-watt light bulbs. With about 6 billion people this would only be 6  1014 watts. We would need 670 billion more Earth’s doing the same thing to equal the energy output of the Sun. ...
astrocoursespring2012lec1-1-5
astrocoursespring2012lec1-1-5

... -minor errata They point to the cross-over point of the analemma as the the equinox. This is not the case. The equinox occurs halfway between the most northern, and south excursion of the Sun ...
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... • A solar eclipse happens when the moon passes between the Sun and the Earth • The corona is a million times fainter than the surface of the Sun so the only time it can be seen is during a total exlipse • Ancient people often thought that eclipses were signs from angry gods or omens of doom ...
nicolaus copernicus the revolutions of the heavenly
nicolaus copernicus the revolutions of the heavenly

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Part 1

... 11. At the center of the Sun, fusion converts hydrogen into (A) water and carbon dioxide. (B) plasma and smoke. (C) radiation and elements like carbon and nitrogen. (D) radioactive elements like uranium and plutonium. (E) helium, energy, and neutrinos. 12. In order to start nuclear fusion, a high t ...
OUTSIDE THE SOLAR SYSTEM
OUTSIDE THE SOLAR SYSTEM

... A: Actually, they are not. White light is a combination of all the other colors in the visible light spectrum. When looking through a telescope, it’s evident that stars come in many colors. However, the unaided human eye tends to combine these colors into white light. Q: Should I be worried about th ...
Characteristics of Stars (Ph)
Characteristics of Stars (Ph)

... Apparent Magnitude A star’s apparent magnitude is its brightness as seen from Earth. Astronomers can measure apparent magnitude fairly easily using electronic devices. Astronomers cannot tell how much light a star gives off just from the star’s apparent magnitude. Just as a flashlight looks brighte ...
Notes 1 - cloudfront.net
Notes 1 - cloudfront.net

Merit Badge College 2017 Astronomy
Merit Badge College 2017 Astronomy

... b. Sketch the phase and the daily position of the Moon, at the same hour and place, for four days in a row. Include landmarks on the horizon such as hills, trees, and buildings. Explain the changes you observe. c. List the factors that keep the Moon in orbit around Earth. d. With the aid of ...
Astronomy Assignment #10 Solutions
Astronomy Assignment #10 Solutions

... expressed in parsecs and p is expressed in arcseconds. 2. What do you need to know in order to get the scale of interstellar space in terms of kilometers or meters? This is quite the question. I believe that Nick Strobel is asking about the theoretical basis of the stellar (trigonometric) parallax. ...
"Science, Mesopotamian" In: The Encyclopedia of Ancient History
"Science, Mesopotamian" In: The Encyclopedia of Ancient History

... phenomena for a future year using the GoalYear method, which is based on accurate periods after which the phenomena repeat at nearly the same celestial position and calendar date. GoalYear predictions are thus essentially observations excerpted from diaries preceding that year by the appropriate per ...
origin of the solar system - Breakthrough Science Society
origin of the solar system - Breakthrough Science Society

... from the sun. Jupiter, with its great mass, The initial ‘clues’ was found to carry about 60% of the enTycho Brahe, Kepler, and other as- tire angular momentum of the solar system. tronomers of the renaissance era had no- The four giant planets together contribute ticed the outstanding “orderliness” ...
Jupiter - Trimble County Schools
Jupiter - Trimble County Schools

... Interesting note…at least to me! ...
Dark Matter - Berkeley Center for Cosmological Physics
Dark Matter - Berkeley Center for Cosmological Physics

... a) Explain how this represents a planet’s motion and the forces that cause it. b) How can you make the planet (rubber stopper) go faster? Slower? c) State a hypothesis relating distance and speed. d) Test your hypothesis and record your data in the table. e) Turn your hypothesis into a statement des ...
28 The solar system object in the photograph below is 56 kilometers
28 The solar system object in the photograph below is 56 kilometers

... 52 Describe the change that takes place in the gravitational attraction between Earth and the Sun as Earth moves from perihelion to aphelion and back to perihelion during one year. [1] 53 Describe how the shape of Earth’s orbit would differ if the Sun and focus B were ...
James`s 5-Page Final Exam Review
James`s 5-Page Final Exam Review

... a. Asteroid. We’ve discovered an asteroid that orbits at a semimajor axis of 2 AU. i. What is this asteroid’s orbital period? ...
Chapter 11
Chapter 11

... In 2002 it found that the number of electron neutrinos is about a third of the total number of neutrinos reaching the detector, showing that neutrinos oscillate. The SNO results are in excellent agreement with the predictions of the standard solar model. 7. Support for the SNO results came in 2002 f ...
Denton ISD
Denton ISD

A-level Physics A Question paper Unit 05 - Section 2A
A-level Physics A Question paper Unit 05 - Section 2A

... Describe the physical processes that give rise to the shape of each graph. Go on to show how the information in the graphs can be used to determine properties, such as the speed and period, of the Menkalinan binary system. You should include appropriate calculations in your answer. The quality of yo ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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