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Motions of the Night Sky
Motions of the Night Sky

... This change in the sun’s apparent behavior is due to the 23.5o tilt of the earth’s axis, and is also the cause of our seasonal weather changes. The hyperlink below illustrates further. http://deepimpact.jpl.nasa.gov/disczone/braintwist-comet1a.html ...
Chapter 3: Galileo, Newton, and Einstein
Chapter 3: Galileo, Newton, and Einstein

... parallax could mean one of two things: 1. Stars are so far away that stellar parallax is too small to notice with the naked eye 2. Earth does not orbit Sun; it is at the bottom of the universe With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they did ...
Brightness vs. Distance
Brightness vs. Distance

Dimensional Analysis Part I FA # 22
Dimensional Analysis Part I FA # 22

... (4) Fill in the missing blanks in the table below using the table on page 17 of your textbook. SI Prefixes GigaMega- ...
The Sky and its Motions
The Sky and its Motions

... Close to where it is now. ...
What, and Why, is the International Astronomical Union?
What, and Why, is the International Astronomical Union?

... The formal structure evolved in Brussels and signed into effect in Rome consisted of Standing Committees “for the study of various branches of astronomy, encouragement of collective investigations, and discussion of questions requiring international agreement or standardization.” The word in the Fre ...
Knows that Earth is the only body in our solar system that
Knows that Earth is the only body in our solar system that

... Earth. How are the four inner planets different from the five outer planets? ...
meteor
meteor

... NASA's Hubble Space Telescope took this photo of Comet ISON on Oct. 9, 2013, when the comet was inside Mars’ orbit and about 177 million miles from Earth. The nucleus of ISON appears to be intact. ...
class 4, S11 (ch. 2c and 3)Jan20
class 4, S11 (ch. 2c and 3)Jan20

... the Sun sweeps out equal areas in equal intervals of time. (the closer to the Sun, the faster it moves) ...
Astronomical Knowledge Questionnaire (Student
Astronomical Knowledge Questionnaire (Student

...  During winter clouds block the light coming from the Sun weakening it while in summer there are few clouds which means the light coming from the Sun is stronger.  The Earth’s tilted axis means that one hemisphere has more direct sunlight and longer days making it summer while the other hemisphere ...
v A v A
v A v A

... = 0.0093 x 1.496 x 108 km = 1.392 x 106 km or Rsun = 6.96 x 105 km Can we apply same principles to the stars? e.g.  Cen (like Sun) D = 1.3 pc = 2.7 x 105 AU; if Rcen = Rsun  = 2Rsun/D = 0.0093 AU/2.7 x 105 AU = 3.3 x 10-8 rad = 0.007 arcsec (angular diameter of a dime 150 km away!) Can we resolve ...
The Stars and the Solar System
The Stars and the Solar System

... You can also see Earth’s moon in the night sky. A MOON is a small, rounded body in orbit around a planet. A moon does not produce its own light. It reflects light from the sun. Most planets have at least one moon. ...
The Stars and the Solar System
The Stars and the Solar System

... You can also see Earth’s moon in the night sky. A MOON is a small, rounded body in orbit around a planet. A moon does not produce its own light. It reflects light from the sun. Most planets have at least one moon. ...
Adventurer Pathfinder
Adventurer Pathfinder

... tail. The comet is much like a large, dirty, space snowball. It consists of frozen gases, ice, and dust. Comets orbit the sun like planets. The best known comet, Halley’s Comet, is seen every 77 years. Meteors are often mistaken as “shooting stars.” They are really metallic or stony material. When c ...
Unit 1
Unit 1

... • The number of protons (atomic number) in a nucleus determines what element a substance is. • Each element has a number of electrons equal to the number of protons • The electron orbitals are different for each element, and the energy differences between the orbitals are unique as well. • This mean ...
Neptune and Beyond, Asteroids, Comets
Neptune and Beyond, Asteroids, Comets

... Hershel ‘asteroid’ (meaning star-like object) More than 300,000 asteroids have been identified and cataloged, over a million asteroids lager than 1km are estimated to be there and many millions smaller ones. ...
Stars - Denbigh Baptist Christian School
Stars - Denbigh Baptist Christian School

... Next closest star to Earth is Proxima Centauri. This is 270,000 times farther away than the distance from Sun to Earth. (4.3 light-years away) These types of distances cause us notation problems. The numbers are so large, that scientists introduced the new distance – light year. This is the distance ...
I. Structure of the Earth
I. Structure of the Earth

Our Solar System
Our Solar System

... tectonic “cracking” of Mars’ crust and is the longest known crevice in the solar system. • Although it is much colder on Mars than on Earth, the similar tilt of Earth’s and Mars’ axes means they have similar seasons. Like Earth's, Mars’ north and south polar caps shrink in the summer and grow in the ...
Powerpoint for today
Powerpoint for today

... Objects are dumb. They do not know the past and they are not good predictors of the future. They only know what forces act on them right now. Newton’s First Law of Motion Every object continues in a state of rest or a state of motion with a constant speed in a straight line unless acted on by an unb ...
Sun - rmwright
Sun - rmwright

... Temperature ranges from -235° C to -210° C because it is so far away from the Sun In 2006, Pluto was demoted to a dwarf planet Ninth planet from the Sun ...
Class 8 - ruf.rice.edu
Class 8 - ruf.rice.edu

... a = semi-major axis b = semi-minor axis c = distance from center to focus ...
HERE - physicsisphun.org
HERE - physicsisphun.org

But how to find Polaris?
But how to find Polaris?

... – This is because you are comparing the surface with yourself as a frame of reference (a scale to compare size) ...
Solar Noon
Solar Noon

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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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