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... • Theory – a body of related hypotheses can be pieced together into a self consistent description of nature ...
2-The Earth in space
2-The Earth in space

... As Earth rotates, one side of Earth faces the sun. This side of Earth has daytime. The other side of Earth faces away from the sun. This side of Earth has night time. Axis [AK•sis] an imaginary line that runs through Earth’s center from the North Pole to the South pole Orbit [AWR•bit] the path that ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... circumference of the Earth. For a distance between the cities of 5000 stadia (about 804 km), we obtain the value of 6.4 × 108 cm for the radius of the Earth. Information on the Eratosthenes’ method is coming from a chapter on the winds of “The Architecture”, by Marcus Vitruvius Pollio [5]. He is wri ...
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two

... Example 7 : Consider the moon’s orbit around the earth. It’s tempting to draw it as a circle and use the same analysis we did with other earthorbiting satellites. The moon’s mass is quite large though, about 1/81 of the mass of the Earth, which is too large to ignore. The radial force the earth exe ...
stellarparameter1 - Physics and Astronomy
stellarparameter1 - Physics and Astronomy

... Luminosity (energy emitted per second; unit watts) Chemical composition (what stars are made of) Age Distance Velocity ...
maymester2
maymester2

... What’s important so far? continued • Without use of a telescope, Tycho Brahe made very accurate measurements of the positions of celestial objects. • Johannes Kepler inherited Brahe’s data and determined three empirical laws governing the motion of orbiting celestial objects. – 1st Law: Each planet ...
PHYS 390 Lectures 1/2 - The Big Picture 1/2
PHYS 390 Lectures 1/2 - The Big Picture 1/2

... Knowing the radius of the Earth’s orbit Res, distances to nearby stars can be found through parallax, the apparent motion of nearby stars caused by the motion of the Earth in its orbit around the Sun (first used in 1838 by Freidrich Wilhelm Bessel). Below, the Earth is shown in its orbit at two extr ...
SWFAS Apr 16 Newsletter - Southwest Florida Astronomical Society
SWFAS Apr 16 Newsletter - Southwest Florida Astronomical Society

... the lunar landing was aborted after an oxygen tank exploded two days later, crippling the Service Module upon which the Command Module (CM) depended. Despite great hardship caused by limited power, loss of cabin heat, shortage of potable water, and the critical need to jury-rig the carbon dioxide re ...
Unit 6 - LPS.org
Unit 6 - LPS.org

... 6.2 Newton’s Law of Gravitation Essential idea: The Newtonian idea of gravitational force acting between two spherical bodies and the laws of mechanics create a model that can be used to calculate the motion of planets. Nature of science: Laws: Newton’s law of gravitation and the laws of mechanics ...
1 History of Astronomy - Journigan-wiki
1 History of Astronomy - Journigan-wiki

... model of the solar system and heavenly sphere was a refinement of previous models developed by Greek astronomers. Ptolemy’s major contribution, however, was that his model could so accurately explain the motions of heavenly bodies, it became the model for understanding the structure of the solar sys ...
Aust Curriculum Connections 2012
Aust Curriculum Connections 2012

... the universe, including the formation of galaxies and stars, has continued since the Big Bang  gathering data to analyse everyday motions produced by forces, such as measurements of distance and time, speed, force, mass and acceleration  recognising that a stationary object, or a moving object wit ...
Force. - BotsRule
Force. - BotsRule

... jointly with Leibnitz, differential calculus. He also calculated a formula for finding the velocity of sound in a gas which was later corrected by Laplace. Newton made many contributions to astronomy. He defined the laws of motion and universal gravitation which he used to predict precisely the moti ...
Astronomy 100—Exam 1
Astronomy 100—Exam 1

... 11. For mapping purpose, the Earth is divided into two equal halves by an imaginary line called the equator. Likewise, the sky is divided into two equal halves by an imaginary line called the A. ecliptic. C. celestial equator. E. none of the above. B. line of nodes. D. zodiac. 12. Which of the follo ...
study-notes-for-2016-2017-1st-qtr-exam
study-notes-for-2016-2017-1st-qtr-exam

... Our Sun is much larger than a planet and is composed of hot, glowing gases (mostly hydrogen & helium) that are continually undergoing nuclear fusion. The Sun does not have a solid surface. The sun is currently about 5 billion years old and has enough helium to “burn” for another 5 billion years. Bec ...
Chapter 3
Chapter 3

... Babylonians Knew length of the year to accuracy of about 4 minutes. Divided year into 12 equal months of 30 days each. Babylonian number system based on 60. Angular system based on 360 degrees, 60 minutes to 1 degree, and 60 seconds to 1 minute. They had a 24 hour day they believed in symmetry of 12 ...
Astro101 lecture from Aug 27
Astro101 lecture from Aug 27

... collecting rain in a bucket, you collect the most water if the rain is pouring straight down, and collect no water if the bucket is angled sideways (perpendicular to the incident rain). The same is true for receiving solar energy. ...
Extreme Tidal Waves in Binary Star Systems
Extreme Tidal Waves in Binary Star Systems

... so we only see the near side of the Moon. It will In binary star systems, tides can be much more volatile. Tidal take another few billion years to interactions are particularly intense in compact binary white dwarf synchronize the Earth with the systems. White dwarfs are the burnt out cores of stars ...
Astronomy - Core Knowledge UK
Astronomy - Core Knowledge UK

... Children’s University of Manchester website and animation about day and night, with quiz. Children’s University of Manchester website and activity about changing day length through the year. MET office animation and activities on day and night. TeacherTube video on seasons on Earth. ...
Rotation
Rotation

... the sun, moon and stars look as though they are moving from east to west. We say that the sun, moon, and stars rise in the east and set in the west. However…it is actually the Earth’s rotation that causes this apparent movement. ...
Sky Diary - Society for Popular Astronomy
Sky Diary - Society for Popular Astronomy

... above the eastern horizon. Climbing higher each morning, it reaches its greatest elongation to the west of the Sun on 28 September, when it will lead the Sun by 18 degrees. On that date Mercury will be obvious, due east, around 10 degrees above the horizon at 05:25 UT, some 35 minutes before sunrise ...
Slide 1
Slide 1

... Why did they have this idea?? When observing from the Earth, planets change their position each night relative to the stars…which made it seem like these were all moving around the Earth ...
Friday, Sep. 5
Friday, Sep. 5

... Apparent motion of Sun during the year The Earth orbits the Sun once a year. This makes the Sun appear to pass in front of different stars (the constellations of the zodiac) during a year. The zodiac does not lie on the celestial equator, but is on a circle tipped about 23o from the equator. This i ...
Chapter 1 slides
Chapter 1 slides

... constellation and their relative brightness within that constellation using the Greek alphabet Alpha Ursa Majoris for example is the brightest star in the constellation Ursa Major With the advent of powerful telescopes and the ability to resolve billions of stars and galaxies, the convention for ide ...
Astronomy 1001/1005 Midterm (200 points) Name:
Astronomy 1001/1005 Midterm (200 points) Name:

... The most important property of a telescope is its collecting area or the size of its objective lens. The only information we get in astronomy comes from light, so the more light we can collect the better, and a bigger lens allows us to collect more light. The second most important property is its an ...
Astronomy
Astronomy

... A light-year A millenium An astronomical unit A mile A kilometer* ...
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Lunar theory

Lunar theory attempts to account for the motions of the Moon. There are many irregularities (or perturbations) in the Moon's motion, and many attempts have been made to account for them. After centuries of being problematic, lunar motion is now modeled to a very high degree of accuracy (see section Modern developments).Lunar theory includes: the background of general theory; including mathematical techniques used to analyze the Moon's motion and to generate formulae and algorithms for predicting its movements; and also quantitative formulae, algorithms, and geometrical diagrams that may be used to compute the Moon's position for a given time; often by the help of tables based on the algorithms.Lunar theory has a history of over 2000 years of investigation. Its more modern developments have been used over the last three centuries for fundamental scientific and technological purposes, and are still being used in that way.
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