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Solar Eclipses
Solar Eclipses

... The gravitational attraction of the Moon varies as the square of the distance (Newton’s Law of Gravitation) - gravity stronger on side facing the Moon than on opposite side. The Moon pulls the ocean water towards it on facing side - creates tide - and pulls the Earth away from the ocean water on the ...
ASTR 111 Lab Manual - Ohio Wesleyan University
ASTR 111 Lab Manual - Ohio Wesleyan University

... longer than the sidereal day because the Sun moves from west to east along the ecliptic from day to day due to Earth’s revolution around the Sun, which is opposite to the eastto-west motion of the Sun due to Earth’s rotation on its axis. As a result, the Earth has to turn through a little more than ...
Unit 5
Unit 5

... establish calendars based on the length of time that earth takes to revolve around the sun. A calendar is a system of organizing time that defines the beginning, length, and divisions of the year. The ancient Egyptians created one of the first calendars. Egyptian astronomers counted the number of da ...
Chapter 2
Chapter 2

... good approximation to the orbits of the Sun and the Moon, but it could not account for the observed variations in planetary brightness or the retrograde motion of the planets. A more complex model was needed to describe these heavenly “wanderers.” In the first step toward this new model, each planet ...
Pictures in the Sky Teacher`s Guide
Pictures in the Sky Teacher`s Guide

... Have your students color the planets on page 7 as described below. You may have to read the descriptions to your students, then see if they can figure out which planet is which and color it. The Sun: The Sun is not a planet but a star. It seems bigger, brighter, and hotter than the stars we see at n ...
ReviewJeopardy
ReviewJeopardy

... “Sun” Stuff 100 ...
2012 Alston Publishing House Pte Ltd Science SMART Teacher`s
2012 Alston Publishing House Pte Ltd Science SMART Teacher`s

... Activity: Ask pupils to look out the classroom window and observe the sky. Ask pupils:  What can you see in the sky? (Answer: The Sun.)  Why can you see the Sun? (Answer: Because it is bright.)  Where does the Sun come from? (Answer: Accept all possible answers.) Then, ask pupils to imagine that ...
The Solar System - MrCrabtreesScience
The Solar System - MrCrabtreesScience

... • Found four of Jupiter’s Moons • Found objects outside of our solar system that did not revolve around either the sun or earth. • Was sentenced to house arrest for his beliefs by the Inquisition ...
Pata Picante Simon
Pata Picante Simon

... methane, nitrous oxide, and ozone). _____ Compare and contrast the major greenhouse gases (carbon dioxide, methane, nitrous oxide, fluorocarbons), their abundance and heat trapping capacity. _____ Describe how major volcanic eruptions, changes in sunlight received by the Earth, and meteorite impacts ...
Chapter 2 User`s Guide to the Sky: Patterns and Cycles
Chapter 2 User`s Guide to the Sky: Patterns and Cycles

... •  Three, although some stars emit large amounts of infrared or ultraviolet light, those types of radiation are invisible to human eyes. •  The subscript ‘V’ in mV is a reminder that you are counting only light that is visible. •  Other magnitudes systems have been invented to express the brightness ...
Young Astronomers Digest
Young Astronomers Digest

... amongst us, however, can relish more advanced topics like the (still hotly-debated) theories on why the moon looks bigger than the horizon than directly overhead, as well as the different contributing factors as to why our Earth will not be ripped into two when the next planetary alignments comes al ...
2nd sem eoypp w 3rd mp highlighted 2016-17 File
2nd sem eoypp w 3rd mp highlighted 2016-17 File

... methane, nitrous oxide, and ozone). _____ Compare and contrast the major greenhouse gases (carbon dioxide, methane, nitrous oxide, and fluorocarbons), their abundance and heat trapping capacity. _____ Describe how major volcanic eruptions, changes in sunlight received by the Earth, and meteorite imp ...
Here
Here

... wavelengths? 13. What is a blackbody? What does it mean to say that a star appears almost like a black body? … 15. What is Wien’s Law? How could you use it to determine the temperature of a star’s surface? 16. What is the Stefan-Boltzmann law? How do Astronomers us it? ...
Planets Orbiting the Sun and Other Stars - Beck-Shop
Planets Orbiting the Sun and Other Stars - Beck-Shop

... passage near the Sun will heat the body of the comet and release volatile material restricted the time during which the volatiles are there. The end of their life is for them to move as a dead object with all their volatiles used up unless the gravitational attraction causes them to impact a planet ...
NATS1311_082108_bw - The University of Texas at Dallas
NATS1311_082108_bw - The University of Texas at Dallas

... 2. Measurement and Prediction - Explore the necessity for accurate and reliable data from measurements in order to make predictions. Measure the density of several objects. 3. Conservation of Energy/Momentum - Study laws of conservation of momentum and energy. Determine speed of a ball by 2 differen ...
A Human-Powered Orrery: Connecting Learners with the Night Sky*
A Human-Powered Orrery: Connecting Learners with the Night Sky*

... long as 45 minutes to set up, similar to the one in the YouTube video. We have used this only when we have extra time such as an overnight with lots of help. However, this model could also be the basis for a more permanent model on a playground, for example. The scale for this model is 1 m = 100,000 ...
Spring 2017 - Astronomers of Humboldt
Spring 2017 - Astronomers of Humboldt

... the following objects: Venus (crescent phase), Double Cluster in Perseus, Orion’s Nebula (including a view of the Trapezium), Andromeda Galaxy, Pinwheel Galaxy, M71 (globular cluster in Sagitta), M79 (globular cluster in Lepus), Cigar Galaxy (M82) and Bode’s Galaxy (M81) in Ursa Major, M35 (open clu ...
ASTRONOMY
ASTRONOMY

... believes aliens could already be listening to Earth and alien life may have landed in clumps of bacteria cells. One planet found near the centre of the Milky Way, is known as OGLE2005-BLG-390Lb, is 20,000 light years away, and it has a surface temperature estimated at no more than -173°C. It orbits ...
Preview Sample 3 - Test Bank, Manual Solution, Solution Manual
Preview Sample 3 - Test Bank, Manual Solution, Solution Manual

... is linked to distance from the Sun, ask how seasons differ between the two hemispheres. They should then see for themselves that it can’t be distance from the Sun, or seasons would be the same globally rather than opposite in the two hemispheres. As a follow-up on the above note: Some students get c ...
File earth, sun, and moon
File earth, sun, and moon

... New York Sun in 1835. This fanciful illustration is supposed to have shown what astronomers were seeing with new and more powerful telescopes. ...
Kohoutek Is Coming - Institute of Current World Affairs
Kohoutek Is Coming - Institute of Current World Affairs

... was a long hairy Comet seen, he did but deride at it and make a Joke of it,saying that it concerned the Part-hians that wore long hair and not him who was bald, but within a year Vespasian himself (and not the Parthian) dyed Let us then prepare for Trouble. We should onely expect it; but so expect i ...
Space Jeopardy
Space Jeopardy

... d)move closer and closer to the sun ...
Physics 55 Midterm Exam
Physics 55 Midterm Exam

... tidal forces from the Earth and Sun. Other planets such as Venus, Mars, and Jupiter have either too small a mass or are too far away to produce significant tides. Let’s consider the effects of the Earth and Sun in turn. Since the Earth is about 80 times more massive than the Moon, it will cause cons ...
Space Information Booklet
Space Information Booklet

... edge is about twice that diameter). Kuiper Belt Objects (KBOs) are, as their name implies, objects that originate from or orbit in the Kuiper Belt. Pluto is the only one KBO which was known for more than 60 years. Many KBOs have been discovered since 1992, however, and the current estimate is that t ...
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society

... planes of their orbits were tilted so the planets could not transit the host star as seen from Earth, or those that the TERRA software itself could have missed. Shedding (the right amount of) light The intensity of light energy bathing a planet depends on both the star’s luminosity and its distance ...
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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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