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Phys 214. Planets and Life
Phys 214. Planets and Life

... Planetesimals grew to hundreds of km -a few million years (only 1/1000 the present age of the solar system). Dozens or even hundreds of planetesimals orbiting the Sun between the present day orbits or Mercury and Mars. Continued accreting - sometimes colliding violently. Computer simulations reprodu ...
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... Venus – rotates in a direction that is opposite to the sense of its nearly circular orbital motion. This retrograde rotation is not the result of tidal evolution. Thought to be due to the more dominating effects of an atmospheric thermal tide – the absorption of solar radiation couples with the mode ...
Our Universe SPA-4101
Our Universe SPA-4101

... -­‐  but  probably  with  massive  rocky  and  icy  cores  at  their  centres   Uranus  and  Neptune  are  normally  referred  to  as  ice  giants  –  they  are  composed   largely  of  rock  and  ice  with  only  ~  10  %  of ...
Evidence, Evolution & God`s Existence 4
Evidence, Evolution & God`s Existence 4

... If much slower, days and nights impossibly hot or cold ...
Unit 8 Chapter 28 Notes
Unit 8 Chapter 28 Notes

... because of the type of lava that was released. ...
Lecture3
Lecture3

... Last Time Earth’s Rotation (once per day) causes sun/ stars/etc. to rise, transit at their highest point at the meridian, and then set. Zenith is the point directly overhead. Stars you see depends on your latitude. Some stars are always up: they are circumpolar. Constellations: Just random grouping ...
Final Exam from 2004 - Onondaga Community College
Final Exam from 2004 - Onondaga Community College

... concedes that she does not know. The company President turns to you and remarks, “You took an astronomy course under the world famous luminary Dr. Jaquin. Explain to us how Saturn became so large.” Here is your opportunity to impress the President and get that raise or wilt into the crowd and be tra ...
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Light-years

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Lookback Time in Our Everyday Lives

... Novas and supernovas are astronomical events that have been recorded down through history. The remnants of some of these are now seen as glowing nebulae. Below is a list of some of these events, when they were seen on Earth, and when they actually occurred (taking into account the light time to get ...
Earth/Space Science ​FINAL​ Review/Study Guide: Gardana DUE
Earth/Space Science ​FINAL​ Review/Study Guide: Gardana DUE

... 34.) What are the characteristics of a constellation?  35.) What are the three main types of galaxies?  36.) How is a galaxy with a quasar in it different from a typical galaxy?  37.) How did Hubble’s discoveries lead to an understanding that the universe is expanding?  Chapter 2  38.) What are Eart ...
Space – Align the Stars - VUTechieTeacher
Space – Align the Stars - VUTechieTeacher

... 10. A group of billions of stars, dust and gas bound together by gravitational force is called a _____________. ...
Unit A: Trees and Forests
Unit A: Trees and Forests

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TAKS objective 5 Earth and Space Systems
TAKS objective 5 Earth and Space Systems

... dust) and ice crystals. When their orbits take them close to the sun, dust and ice heat up to produce a “tail” behind the comet. Larger comets may even become visible without the aid of a telescope. ...
AST301.Ch6.15.SolarSystems - University of Texas Astronomy
AST301.Ch6.15.SolarSystems - University of Texas Astronomy

... Comets: Iceballs, most in highly eccentric orbits which extend far beyond Pluto. Spend most of their time far from sun (in the “Oort cloud”; also the “Kuiper belt” comets outside of Neptune’s orbit). Comets and asteroids are “debris”, but very important because they represent the solar system when i ...
The Solar System (Ch. 6 in text) The solar system consists of the Sun
The Solar System (Ch. 6 in text) The solar system consists of the Sun

... Comets: Iceballs, most in highly eccentric orbits which extend far beyond Pluto. Spend most of their time far from sun (in the “Oort cloud”; also the “Kuiper belt” comets outside of Neptune’s orbit). Comets and asteroids are “debris”, but very important because they represent the solar system when i ...
Earth, Moon and Mars - International Space Science Institute
Earth, Moon and Mars - International Space Science Institute

... 4’600 million years ago the Sun and the planets formed out of an interstellar cloud? What were the external circumstances and specific processes that governed the origin of the Earth and determined its evolution to the present state? Is there – or was there – life in the past on another planet or on ...
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Goal: To understand how Galileo and Newton

... • He concluded that these stars had to be more distant that the stars you can see with your naked eye. • Also, this could mean that the distance to the known stars is probably much higher than expected, and therefore too large to be measurable with stellar parallax. ...
Celestial Equator
Celestial Equator

... The effect of the Sun being closer in the northern winter is reduced by the fact that the southern hemisphere has a higher percentage of oceans, which reflect heat and light back into space more efficiently than do forested land masses. If the Earth’s orbit were very elliptical (like Mercury), then ...
Chapter 9: Our Star, the Sun
Chapter 9: Our Star, the Sun

... Solar magnetic fields also create other atmospheric phenomena • prominences • solar flares – are large explosions in the Sun's atmosphere that can release large amounts of energy. ...
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04 Solar System

... is opposite to the Sun’s spin. c) the terrestrial planets have higher density and lower mass. d) comets do not necessarily orbit in the plane of the solar system. ...
The search of habitable Earth-like exoplanets
The search of habitable Earth-like exoplanets

... orbits of Sun-like G-type and some K-type stars, F-type where the originally defined habitable zone definition is valid → see Earth! ƒ Class II, III and IV habitats should also populate G-type and F, K, and M-type stars ƒ Lower mass stars should have less class I habitable planets but class II, clas ...
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astrocoursespring2012lec1-1-5

... the sky day after day due to our orbit and tilt. To understand this better watch this video that explains the sky at different points in its elliptical orbit … and at different times of year in its cyclical , tilting traversal around the sky…. see A Year on Earth… ...
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Motion of the Moon Phases of the Moon

... objects in the night sky (with the exception of the Moon) & they rise in the east and set in the west • “Planet” derived from Greek for “Wanderer” – The planets move slowly among the stars staying near the ecliptic – Different planets move at different speeds relative to the stars (of the visible pl ...
Designing Curriculum and Instruction in Elementary School
Designing Curriculum and Instruction in Elementary School

... the inner planets are made up almost entirely of rock and dust. This is also a result of the solar winds. As the outer planets grew larger, their gravity had time to accumulate massive amounts of gas, water, as well as dust. ...
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... • The Solar System refers to the Sun and the surrounding planets, asteroids, comets, etc. • The scale of things: – It takes light about 11 hours to travel across the Solar system. This is 0.001265 years. – It takes light about 4.3 years to travel from the Sun to the nearest star. – It takes light ab ...
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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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