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... Venus is the second planet from the Sun, orbiting it every 224.7 Earth days. It has the longest rotation period (245 days) of any planet in the Solar System, and, unusually, rotates in the opposite direction to most other planets. It has no natural satellite. It is named after the Roman goddess of l ...
9 Intro to the Solar System
9 Intro to the Solar System

... gravity and it basically runs the solar system. In fact, the term “solar” comes from the Latin word sol for son. We named the whole shebang after the Sun, so there you go. • The planets are smaller but still pretty huge compared to us tiny humans Earth in comparison to Jupiter ◦ At the big end we ha ...
The Copernican Model (1543)
The Copernican Model (1543)

... The Copernican Model (1543) The Copernican Model is Heliocentric and Geodynamic Heliocentric = “Sun Centered” Geodynamic = “Earth in motion” (The Ptolemaic Cosmology was Geocentric and Geostatic.) ...
Comets, Asteroids, and Meteors- Oh My!
Comets, Asteroids, and Meteors- Oh My!

... • Definition: objects that are too small and numerous to be considered planets • Rocky – 75% of all asteroids • Iron (metals) – 7% of all asteroids • Mixed (rock and iron blended) – 18% of all asteroids ...
Let us calculate planet`s orbit radii and its average orbital
Let us calculate planet`s orbit radii and its average orbital

... Other part of protomars moved in the direction of Jupiter. It was represented group of liquid and solid pieces. Large planets entrapped the small-sized parts. They can be observed by us as satellites of planets on high-altitude orbits, which one are move close to plane of ecliptic. Two large pieces ...
Earth
Earth

... -Explains high Earth rotation rate -Heat of impact melted any crust -magma ocean #2 ...
Time runs out for Herschel
Time runs out for Herschel

... system evolves may shed light on the mechanisms of terrestrial storms. Cassini is a joint project of NASA, ESA and the Italian Space Agency and has been observing Saturn since 2004. Scientists have not seen the north pole so clearly in the past because it is only now emerging from winter. Cassini’s ...
Exam Name___________________________________
Exam Name___________________________________

... 10) According to Copernicus, the retrograde motion for Mars must occur A) at quadrature, when Mars lies exactly 90 degrees east or west of the Sun. B) at greatest elongation, when Mars can get up to 47 degrees from the Sun. C) at opposition, when the Earth overtakes Mars and passes between Mars and ...
Everything from Velocity, Seasons, Tides
Everything from Velocity, Seasons, Tides

... Orbital velocity is the speed at which a planetary body moves in  its orbit around another body.  If orbits were circular, this velocity would be constant.   However, from discussion of Kepler’s Laws, we know that  planetary bodies orbit the sun (or their planet) in elliptical paths.  Therefore, whe ...
1 month - Otterbein
1 month - Otterbein

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Chapter 30 Notes
Chapter 30 Notes

...  The development of a calendar came from a need to be able to predict the seasons, annual floods, and other cyclical occurrences in communities’ lives.  The day and the year, as units of time, are based upon the motion of the earth.  Modern calendars also add one day every four years to account f ...
Guided notes part 1 - Duplin County Schools
Guided notes part 1 - Duplin County Schools

... June 21 or 22), the _________________________________________ comes up directly above the heel stone of Stonehenge Besides keeping this calendar, Stonehenge may also have provided a method of determining ________________________________ ...
Glossary - Sky Science
Glossary - Sky Science

... a huge ball of gas that emits radiation and light (or once did) because of nuclear reactions in its core. Sunspot: a dark, irregular patch on the sun's surface. Sunspots appear dark because they are about 2,000 degrees Celsius cooler than surrounding gases. Sunspots are areas with intense magnetic s ...
Introductory Astrophysics
Introductory Astrophysics

... – Earth is no different from the other planets and stars! ...
©JSR 2010 Seeing gravity 1/2 Gravitation – if the Earth could see
©JSR 2010 Seeing gravity 1/2 Gravitation – if the Earth could see

... It’s no surprise that the gravitationally brightest object in the sky is the Sun, for that holds us in our annual orbit. Different visual magnitudes in astronomy are represented on the logarithmic magnitude scale, where a factor of 100 in visual brightness converts to 5 on the magnitude scale. Hence ...
Big Bang Theory
Big Bang Theory

... Doppler Effect Song by Astrocapella ...
General Science Class: ______ Earth Science
General Science Class: ______ Earth Science

... 2. How do Earth, the other planets, and asteroids move in relation to the sun? 3. What direction does Earth rotate when viewed from above the North Pole? 4. Explain why Earth has night and day. 5. Infer as to which planets would take longer or shorter than Earth to orbit the sun. 6. During what seas ...
Chp. 3 The sun-earth
Chp. 3 The sun-earth

... object in the universe attracts every other object." That applies to celestial bodies in the solar system as well. While the Sun's mass exerts a much greater gravitational pull on Earth than Earth does on the Sun, both bodies attract one another. The Sun's great mass keeps its eight planets circling ...
Sept2 - University of Arizona
Sept2 - University of Arizona

... Galileo observed that Venus showed phases entirely like those of the moon from full to crescent, which it must do if the Copernican theory was correct. According to the Ptolemaic theory Venus would have to be a perpetual crescent. ...
Lec21_2D
Lec21_2D

... Heat and the Moons of Jupiter As a result of Jupiter’s tides …  Io is continually stressed by the tides of Jupiter. Its interior is kept entirely molten.  Europa feels some tidal stress as well. However, since it is further away, the stress is less. Europa’s interior is probably warm enough to me ...
Astronomy
Astronomy

... With the exception of the first two, the others are simply twice the value of the preceding number. Add 4 to each number: ...
Lecture
Lecture

... In this picture of the Earth rising, what is the predominant direction of the sun in relation to the observer? 1) above the observer 2) below the observer 3) behind the observer 4) behind the Earth ...
AST 1002 Fall 2014 Midterm Exam Version 1
AST 1002 Fall 2014 Midterm Exam Version 1

... 39) Which of the following best describes why we have seasons on Earth? A) The tilt of Earth's axis causes the northern hemisphere to be closer to the Sun than the southern hemisphere in summer, and visa versa in winter. B) Earth's elliptical orbit means we are closer to the Sun and therefore recei ...
Biblical Astrophysics - The Call of the Bride
Biblical Astrophysics - The Call of the Bride

... November 28th. If it survives without disintegrating, then it should be spectacular with a very long tail. Around mid-January, 2012 the comet's tail was already more than 40,000 miles long. According to NASA, the closest ISON will get to earth is 40 million miles on the day after Christmas. Word is, ...
2. Answer Key Practice Test, Topic 3
2. Answer Key Practice Test, Topic 3

... Jupiter, Saturn, Neptune, Uranus Uranus, Neptune, Saturn, Jupiter Jupiter, Saturn, Uranus, Neptune Neptune, Uranus, Saturn, Jupiter ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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