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10 Astronomy Things to Remember for 50 Years
10 Astronomy Things to Remember for 50 Years

... • Cold winter and warm summer is not because the earth is closer to the sun in summer. • Seasons are caused by the tilt of the earth relative to the sun. • The north pole of the earth always points toward the same position in the sky • As the earth orbits the sun’s light falls more directly on the n ...
Section 3.3
Section 3.3

... The rise has been relentless and shows a remarkably constant relationship with fossil-fuel burning, and can be well accounted for based on the simple premise that 57% of fossil-fuel emissions remain airborne. Here the number 57% was selected to fit the curve at the ends of the record, but what is si ...
Ch 22-2
Ch 22-2

... • Phases of the moon • Solar eclipse • Lunar eclipse ...
1. The planetary winds in Earth`s Northern Hemisphere generally
1. The planetary winds in Earth`s Northern Hemisphere generally

... 29. Which two stars have the most similar luminosity and temperature? (1) Betelgeuse and Barnard’s Star (2) Rigel and Betelgeuse (3) Alpha Centauri and the Sun (4) Sirius and Procyon B 30. The Big Bang Theory, describing the creation of the universe, is most directly supported by the (1) redshift of ...
Homes for life
Homes for life

... The habitable zone is the region around a star in which an Earth-like planet could have liquid water. The surface temperature of a planet is governed by the incident stellar radiation, its albedo and the greenhouse effect of the atmosphere. The concept of the habitable zone is problematic because th ...
About Uranus - COSTA VERDE production
About Uranus - COSTA VERDE production

... It mainly consists of 83% hydrogen (H), 15 % helium (He) and 1.9 % Methane (CH4) and is an ice giant, which is a subspecies of the gas giants, as it is mostly composed of ice and rock as well as gases. ...
Teacher: Mrs. Zimmerman Astronomy Part 2 Practice Test 1. In the
Teacher: Mrs. Zimmerman Astronomy Part 2 Practice Test 1. In the

... 38. [Refer to figure 8] A total solar eclipse sometimes occurs when the Moon is at position A. Explain why a total solar eclipse does not occur every time the Moon is at position A. --------------------------39. Base your answer to the question on the diagram below, which shows Earth as viewed from ...
From the Everett and Seattle Astronomical
From the Everett and Seattle Astronomical

... same direction as their planets rotate – tend to slowly move farther and farther away. The distance between the Earth and our own Moon is slowly increasing by this very mechanism. "Retrograde" moons – those that orbit counter to the direction their planets rotate – tend to be pulled in closer and cl ...
Earth from Space
Earth from Space

... Historically, solstices and equinoxes have meant a lot to mankind. • Vikings visited wells and made monetary sacrifices (money) during the summer solstice. • Wyoming’s Bighorn medicine wheel, an arrangement of stones built several hundred years ago by the Plains Indians, aligns with the solstice su ...
Chap. 4: Gravitation and the Waltz of the Planets
Chap. 4: Gravitation and the Waltz of the Planets

... • To explain why Venus is never seen very far from the Sun, the Ptolemaic model had to assume that the deferents of Venus and of the Sun move together in lockstep, with the epicycle of Venus centered on a straight line between the Earth and the Sun • In this model, Venus was never on the opposite si ...
Basic Astronomy Note - Mr. Dewey – Grade 7/8
Basic Astronomy Note - Mr. Dewey – Grade 7/8

... They are approximately 4 light years away. At the speed of light it would take 4 years to get there. One light year is 9.46 trillion kilometers. With current technology, travelling at approximately 50,000km/hr, it would take about 80,000 years to get there (our closest neighbouring solar system). ...
Comets - LWC Earth Science
Comets - LWC Earth Science

... - When a meteoroid strikes our atmosphere at high velocity, friction causes this chunk of space matter to heat up and create a streak of light known as a meteor (shooting star). ...
Chap 2 Lecture(1)
Chap 2 Lecture(1)

... At any distance from the subsolar point the radiation received is more diffuse. ...
2.1.1 Study: The Big Bang Theory
2.1.1 Study: The Big Bang Theory

... outward pressure and the inward force of gravity. Our sun formed about 5 billion years ago, and is about halfway through its life cycle. At the end of its cycle, it will expand to form a red giant, then collapse into a white dwarf. Stars larger than our sun will either supernova and then form a neut ...
STARS
STARS

... atmosphere cause the gases to give off light called Aurora • These Auroras are often seen from Earth’s polar regions. • Also known as Northern Lights (aurora borealis) • Link to Video ...
CENTRAL MICHIGAN UNIVERSITY
CENTRAL MICHIGAN UNIVERSITY

... Overview of the solar system: content, motions, origin of the solar system, unanswered questions ...
How to use custom background????
How to use custom background????

... Kepler’s 3 Laws 1) Planets move in elliptical orbits, with the sun at one focus of the ellipse 2) Planets do not move with constant speed. They move faster when nearer the sun, and slower when they are farther away 3) The amount of time it takes a planet to orbit the sun exactly once is related to t ...
CopernicanRev
CopernicanRev

... Explain Aristotle’s main argument against the heliocentric model. What was Aristotle’s other (and weaker) argument against the heliocentric model? Who gave the first evidence in favor of the heliocentric model? What was the evidence? Who added the mathematical calculations to the geocentric model? W ...
Motion in the Sky & Getting to know the Sky
Motion in the Sky & Getting to know the Sky

... The “why’s” of orbital motion (planets, moons) come from combining the idea of a generic force that causes accelerations with the specific force of gravity. ...
Day & Night
Day & Night

...  Jupiter rotates faster than any other planet. It takes 9 hours 56 minutes to spin around once on its axis, compared with 24 hours for Earth. Which means it has the shortest day. ...
Document
Document

... the stars in the sky should be different for observers at different latitudes • This is confirmed by additional observations – E.g. Canopus is visible in Egypt but not further north ...
Ellipses, Parallax, and Retrograde Motion – Study Guide
Ellipses, Parallax, and Retrograde Motion – Study Guide

... 4. Draw or describe a shape with an eccentricity of 0 (zero), 1 (one), 0.2 and 0.9. Include where the foci (or center) are. A perfect circle has an eccentricity of zero; a line has an eccentricity of 1 (one). This is eccentricity of 0.2: This is eccentricity of 0.9: 5. If the Earth still had a 23.5 ...
8th Grade Science Pre
8th Grade Science Pre

... living organisms to understand how they are related. The theory of evolution was developed before scientists discovered DNA; however, the theory supports these new data. What does this sequence of events tell us about the theory of evolution? A. It is a bad theory because it makes scientists biased. ...
Another New Year`s Day Celebration
Another New Year`s Day Celebration

... of Mare Crisium include Langrenus, Petavius and Funerius. January’s Lunar Cycle: The first day of 2014 January could be astronomically special for those who live by lunar calendars—a new moon occurs on this day! Therefore, a new lunar cycle commences with the new year of 2014! The last time a new mo ...
Hmwk2012 - science9atsouthcarletonhs
Hmwk2012 - science9atsouthcarletonhs

... Complete the following work in a separate homework folder. Organize the work by section. Clearly underline titles and defined words. You are responsible for the vocabulary in each section. However, you only need to define those terms not already completed in class. With the exception of starred (*) ...
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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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