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Ellipses
Ellipses

... would create a circular orbit. If there’s more than one massive celestial body, the orbiting object will have have an eccentric or elliptical orbit. This has many consequences, not on how we observe space but also how navigate it. Other than the threat of running into random objects, gravity is one ...
The Sun
The Sun

...  The Earth rotates around its axis and the Sun. Does the Sun rotate, too ?  The Sun like the planets rotates around its axis in an anti-clockwise direction when viewed looking down from above its North Pole. For an observer at Earth the rotation is from left to right, i.e., features move from the ...
The Sun
The Sun

...  The Earth rotates around its axis and the Sun. Does the Sun rotate, too ?  The Sun like the planets rotates around its axis in an anti-clockwise direction when viewed looking down from above its North Pole. For an observer at Earth the rotation is from left to right, i.e., features move from the ...
NASA discovers Earth`s bigger, older cousin, Kepler 452b
NASA discovers Earth`s bigger, older cousin, Kepler 452b

... people have dreamt about for thousands of years — another Earth,” NASA said in a statement. On Thursday, NASA released the latest catalogue of exoplanet candidates, adding more than 500 new possible planets to the 4,175 already found by the space-based telescope. “This catalogue contains our first a ...
Actual Earth Motions
Actual Earth Motions

May 2016 - Newbury Astronomical Society
May 2016 - Newbury Astronomical Society

... There are two factors, external to the telescope that can have a major effect on the telescope and will cause The telescope itself can perturb the image, if it hasn’t deterioration of the image. Astronomers call these two reached ambient temperature, this will result in a “boiling annoying effects ‘ ...
Version A - Otterbein University
Version A - Otterbein University

... maximal possible altitude of the sun above the horizon at noon? a. 23.5 degrees b. 66.5 degrees. c. 73.5 degrees d. 90 degrees. e. None of the above. 30. To see a constellation at a particular position in the sky, you need to know date and time. As an example, say we are seeing Taurus in the south a ...
Version B - Otterbein University
Version B - Otterbein University

... 8) Use the backside of the computer form to record the answers to the last three questions, which are not multiple-choice but short answer questions. 9) You should be able to answer all questions without using a calculator, but if you wish, you can use a scientific calculator. ...
Document
Document

... 1 The Spirit of Enquiry - Sun Fun Where does the Sun get its energy from to shine for hundreds of millions of years? To answer this we need to know what is inside the Sun! ...
explaining the seasons and locating the north and south celestial
explaining the seasons and locating the north and south celestial

Constellations appear to move across the sky at night because
Constellations appear to move across the sky at night because

... a) stars don’t seem to show any parallax. ...
Rotation and Revolution of Earth
Rotation and Revolution of Earth

... stellar parallaxes were not easily observed because stars are much more distant than was expected – All stellar parallaxes are less than 1 arcsecond – The nearest star with the largest parallax is Alpha Centauri (0.76 arcsec) – Such small angles cannot be measured with naked eye ...
distant stars nearby star parallax angle The principle of geometrical
distant stars nearby star parallax angle The principle of geometrical

... months apart. You can assume that the patch of sky is near the plane of the ecliptic. (Note that these images are actually artificial constructions to make it possible to measure many stellar parallaxes in one image. In practice, stars that are close enough to us to have measurable parallaxes wouldn ...
Discussion Activity #9
Discussion Activity #9

... enough to allow gravitational contraction and nuclear fusion to occur. B. As the Sun was forming, nuclear fusion reactions in the shrinking clouds of gas slowly became stronger and stronger, until the Sun reached its current luminosity. C. The Sun initially began generating energy through nuclear fu ...
Mon Nov 18, 2013 THE MOON`S TIDAL LOCK The old gibbous
Mon Nov 18, 2013 THE MOON`S TIDAL LOCK The old gibbous

... sunlight; half of it always in shadow, just like on earth. And just as we experience daylit and dark periods on earth, so the moon has both day and night. But the moon spins more slowly; a lunar day lasts two weeks, followed by two weeks of lunar night. As the moon orbits the earth, we can’t always ...
Inverse Square Law, Blackbody Radiation y
Inverse Square Law, Blackbody Radiation y

... The Inverse Square Law for Radiation The amount of energy emitted in one second by a source of light is called its luminosity and is measured in watts. A source of light with a luminosity of 1 watt emits one joule of energy per second. The luminosity of the Sun is 3.86×1026 watts. As light travels a ...
JOHN FLAMSTEED 1646-1719
JOHN FLAMSTEED 1646-1719

astrofe –astronomy ofe
astrofe –astronomy ofe

Class Project Physics 1010-042, Physics 1010
Class Project Physics 1010-042, Physics 1010

... There may be a few possible resolutions to Fermi’s Paradox about alien life. First of all, maybe they haven’t advanced as fast as we have. Even though the life form may be much older than us, maybe they are very slow at advancing. Another reason may be is that there really aren’t any other intellige ...
The Celestial Sphere Friday, September 22nd
The Celestial Sphere Friday, September 22nd

... same direction as Sun. We see only a sliver of Moon’s sunlit side. We see crescent Moon close to Sun in sky. “Horns” of crescent point away from Sun. ...
ASTRONOMY 161
ASTRONOMY 161

... completely hides Sun. (2) Annular: Moon umbra falls short of Earth; Moon is surrounded by a ring of Sun. (3) Partial: Observer is in penumbra, to one side of umbra; Moon takes ‘bite’ out of Sun. ...
Your Birthday on Another Planet
Your Birthday on Another Planet

... the Sun. If we could live on another planet, our birthdays would occur more or less frequently depending on the planet’s revolution period (the time taken to complete one full trip around the Sun). On a few planets, we couldn’t even celebrate our first birthday because we wouldn’t live long enough t ...
black hole
black hole

... gravity, a map of the Earth was projected onto the star, and a map of the familiar night sky was projected above. From here one can either look down and see several duplicate images of the entire surface of the star, look up and see several duplicate images of the entire night sky, or look along the ...
Chapter 5 Gravitational fields - crypt
Chapter 5 Gravitational fields - crypt

Peter Martinson: Defeating the Oligarchical Principle
Peter Martinson: Defeating the Oligarchical Principle

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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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