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Today`s Powerpoint - Physics and Astronomy
Today`s Powerpoint - Physics and Astronomy

... a) stars don’t seem to show any parallax. b) we don’t feel as though Earth moves. c) objects fall toward Earth, not the Sun. d) we don’t see an enormous wind. e) All of the above were valid reasons. ...
Document
Document

... the top of Mt. Everest in a direction tangent to the ground. If the initial speed were high enough to cause the ball to travel in a circular trajectory around Earth Earth, the ball’s ball s acceleration would – a) be much less than g (because the ball doesn’t fall to the ground). Note: someone in a ...
The Small Objects. The Sun.
The Small Objects. The Sun.

... An average period is 11 years (from 7 to 15 years). The magnetic fields in sunspots reverse their direction when a cycle is over. No sunspots were observed in 16451715, when a Little Ice Age took place in Europe and America. ...
ASTR 1120H – Spring Semester 2010 Exam 1 – Answers The AU is
ASTR 1120H – Spring Semester 2010 Exam 1 – Answers The AU is

... PART II (30 points) – 6 mathematical problems (5 points each): 1. The angular size of the Moon as seen from the Earth is α = 1,867″ (about ½°). What was the angular size of the Earth as seen by the Apollo astronauts who walked on the Moon? (The Earth's diameter is 12,756 km. The Moon's diameter is ...
The Solar System Sections 16.1-16.8
The Solar System Sections 16.1-16.8

... Formation of the Solar System • Began with a large, swirling volume of cold gases and dust – a rotating solar nebula • Contracted under the influence of its own gravity – into a flattened, rotating disk • Further contraction produced the protosun and eventually accreted the planets • As particles m ...
Macmillan Natural and Social Science 1 [bold PB font]
Macmillan Natural and Social Science 1 [bold PB font]

... Additionally in this unit, your child will investigate the changing phases of the moon and consolidate reasons for day and night. They will say the Sun chant. This chant allows your child to review the key vocabulary of the unit in context. Encourage your child to listen to the chant while looking a ...
Class 1: From Astrology to Astronomy
Class 1: From Astrology to Astronomy

... (The “Starry Vault”) • The sun and moon moved across the sphere on similar path. ...
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Astronomy Timeline This is a timeline of important events

... TeideAstro - educación ambiental ...
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Science at a Glance

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AST 111 Lecture 7
AST 111 Lecture 7

... • Earth’s orbit around the Sun causes the Sun to move in the sky – Earth must rotate a little extra to bring the Sun to the Meridian ...
EARTHSKY Why Earth has 4 seasons Some assume our planet`s
EARTHSKY Why Earth has 4 seasons Some assume our planet`s

... amounts of land mass and ice sheets in the northern hemisphere make Earth top-heavy. An analogy for obliquity is imagining what would happen if you were to spin a ball with a piece of bubble gum stuck near the top. The extra weight would cause the ball to tilt when spun. Over long periods of geologi ...
Origin of the Solar System – Notes Rings encircle Jupiter, Saturn
Origin of the Solar System – Notes Rings encircle Jupiter, Saturn

... hydrogen, helium, ammonia, and methane, are gases under normal conditions on Earth. But in the interiors of these planets, pressures are so high that these substances are liquids, not gases. The Jovian planets might be better described as “liquid giants”! As you might expect, a planet’s surface temp ...
Planet Jupiter - Rocky View Schools
Planet Jupiter - Rocky View Schools

... 000K, compared to a temperature of only about 110K at its surface. Four spacecraft have visited Jupiter, two Pioneer fly-bys in 1974 and two Voyager probes in 1979. The probes obtained high-resolution images of Jupiter’s gaseous surface and gave scientists valuable information about the planet and i ...
SE 1.0 - Edquest
SE 1.0 - Edquest

... Solar winds pass the Earth at an average speed of 400 km/s. This protects us from the devastating effects of the solar winds … A. Earth’s atmosphere B. Earths gravity C. Earth’s magnetic field D. Earth’s ozone ...
About Neptune - COSTA VERDE production
About Neptune - COSTA VERDE production

... Average surface temperature: -214 °C ...
universal gravitation pdf
universal gravitation pdf

... • All planets affect each other, can cause perturbations (wobbles) in orbits • Neptune and Pluto were discovered because of perturbations in Uranus’ orbit. • Perturbations of distant stars have led to discoveries of planets, double stars ...
PHASES OF THE MOON
PHASES OF THE MOON

... Jupiter Saturn Uranus Neptune Pluto The Inner Planets are Mercury, Venus, Earth, Mars. They are called the Rocky planets. The outer planets are Jupiter, Saturn, Uranus, Neptune, Pluto. They are the Gas planets. The inner and outer planets are separated by the Asteroid Belt between Mars and Jupiter. ...
Terminology Used in Planetary Data
Terminology Used in Planetary Data

... can throw people into confusion. At times it can be like reading another language! So here is a brief summary of the commonly used terms and what they mean. The diagram will help you to better understand these descriptions! Orbits In our solar system, the planets orbit the Sun and each planet has mo ...
Which of the following statements is TRUE
Which of the following statements is TRUE

... Week 5 – Quiz #6 Star X has a surface temperature that is 3 times higher than that of the Sun. Both stars have exactly the same radius. Which of the following statements is TRUE? A. The luminosity of the Sun is 81 times that of the star X B. The typical photon emitted by star X has a lower energy t ...
Jeopardy Sun & Earth
Jeopardy Sun & Earth

... As the Earth revolves around the Sun it is tilted in space. At different times of the year, different parts of the Earth are tilted towards or away from the Sun. ...
Cycles - Needham.K12.ma.us
Cycles - Needham.K12.ma.us

...  Tides are caused by gravity pulling on the Earth’s bodies of water and upon the Earth itself.  There are 2 gravitational bodies that affect the tides: the sun and the moon.  The moon is much closer to the Earth than the sun is, so it has a much greater influence upon the tides. ...
AST 101 Lecture 15 Is Pluto a Planet?
AST 101 Lecture 15 Is Pluto a Planet?

... Maximum mass: 0.013 M, or 13 MJ Planets orbit stars (must they?) Planets dominate their orbit Planets are round. “It all depends on what the meaning of ‘is’ is” William Jefferson Clinton ...
AST 101 Lecture 17 Is Pluto a Planet?
AST 101 Lecture 17 Is Pluto a Planet?

... Titius-Bode Law A mathematical relation published by J.E. Bode in 1772 a = (2n x 3 + 4) / 10 •  a is the semimajor axis of the orbit in AU •  n is an index: –  Mercury: -1 (set 2-1 = 0) –  Venus: 0 –  Earth: 1 –  Mars: 2 –  Jupiter: 4 –  Saturn: 5 ...
Lecture #2 - Personal.psu.edu
Lecture #2 - Personal.psu.edu

... More Precisely 2-3: Weighing the Sun Newtonian mechanics tells us that the force keeping the planets in orbit around the Sun is the gravitational force due to the masses of the planet and Sun. This allows us to calculate the mass of the Sun, knowing the orbit of the Earth: ...
Venus - Mr. Nussbaum
Venus - Mr. Nussbaum

... and relative condition of its surface. It is easily observed with the naked eye and is sometimes called the “evening star” or “morning star.” Venus is covered by thick, noxious clouds of sulfuric acid that obscure its surface. The thick layers of cloud create an extreme insulating effect (like the g ...
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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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