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astron_ch_13b
astron_ch_13b

... are slightly higher in the atmosphere than the belts. Differences in temperature causes the differences in ...
Earth`s Motions
Earth`s Motions

... in motion is how planets were discovered. The retrograde motion of planets is more easily explained by the heliocentric model rather than the geocentric model. ...
Seasonal calendar lesson plan - Department of Environment and
Seasonal calendar lesson plan - Department of Environment and

... Understanding how the tilt of the Earth affects the seasons can be difficult to conceptualise. A lamp in the centre of a room with a terrestrial globe is a great way to show students how the tilt of the Earth affects the length of the day and seasonal change. To signify the beginning of the year, ma ...
Unit 1
Unit 1

... constellation, satellite, stars, moon, planets, sun, mass, matter, particles, solids, liquids, gas Essential Skills: Solar System Unit:  A solar system includes a star, planets, and other objects.  Planets revolve around a star in orbits of differing lengths.  The Earth is the 3rd planet from the ...
Revision sheet Q3
Revision sheet Q3

... 1-Multiple Choice: 1. Which tool measures wind direction? A. ...
ASTR 300 Stars and Stellar Systems Spring 2011
ASTR 300 Stars and Stellar Systems Spring 2011

... 1. If the Earth did not rotate, could you define the celestial poles and celestial equator? (Chapt. 2, Review Question 8) No, you could not define the celestial pole or equator. The direction to the pole is defined by the Earth’s rotational axis. 2. As the earth turns on its axis, an observer on the ...
Consulting the Planetary Expert: You
Consulting the Planetary Expert: You

... For thousands of years humans have looked up at the sky in wonder. As they observed they learned the sky was constant and predictable. They learned to tell the time of day, the date, the weather, their position and the occurrence of tides and eclipses. Many other events were thought to depend on the ...
Astronomy Directed Reading
Astronomy Directed Reading

... _________________________________________________________________________________ 18. How do the surfaces of the inner planets compare with that of Earth today? _________________ _________________________________________________________________________________ 19. How do the inner planets differ fro ...
Astronomy Content from Frameworks
Astronomy Content from Frameworks

... The Moon changes in position in the sky each day. It also changes in appearance from a full Moon to a thin crescent. These changes are called phases. The Moon's light comes from the Sun, and the sunlight is reflected off the Moon's surface. The phase of the Moon that we see depends on the orientatio ...
Size of Sun and Size of Planets
Size of Sun and Size of Planets

... Our Sun is the largest body in the Solar System but it is still considered an average-sized star. It is the only star in our solar system. The Sun is over 93 million miles away from the earth. It’s light takes about 8 minutes to reach the earth. Without its heat and light there would be no life on o ...
3-planets-of-the-solar-system
3-planets-of-the-solar-system

... Venus, Earth, and Mars. B) Hermes has a shorter period of revolution than Mercury, but a longer period of revolution than Venus, Earth, and Mars. C) Hermes has a longer period of revolution than all of the planets shown. D) Hermes has a shorter period of revolution than all of the planets shown. 2. ...
Planets and Small Objects in the Solar System Worksheet
Planets and Small Objects in the Solar System Worksheet

... 6. Asteroids and meteoroids are chunks of rocks left over from the formation of the early Solar System. Which of the following describes the difference between these? A) Asteroids are round and meteoroids are irregular shaped B) Asteroids are much larger than meteoroids C) Asteroids are located much ...
Exam Name___________________________________
Exam Name___________________________________

... A)  A theory can never be proved beyond all doubt; we can only hope to collect more and more  evidence that might support it.  B) A theory cannot be taken seriously by scientists if it contradicts other theories developed by  scientists over the past several hundred years.  C)  If even a single new  ...
View Presentation Slides
View Presentation Slides

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LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034
LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034

... 11. Describe the Equatorial coordinate system to fix the position of body in the celestial sphere. 12. Find the condition that twilight may last through out night. 13. Derive cassini’s formula for refraction, indicating the assumptions made. 14. If the moon’s horizontal parallax is 57’ and her angul ...
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... inner planets, the only one known to have current geological activity, and the only place where life is known to exist. Its liquid hydrosphere is unique among the terrestrial planets, and it is also the only planet where plate tectonics has been observed. Earth's atmosphere is radically different fr ...
The core of the Sun is
The core of the Sun is

... 1. measuring the orbital period and distance of Jupiter's orbit around the Sun. 2. measuring the orbital period and distance of one of Jupiter's moons. 3. measuring the orbital speed of one of Jupiter's moons. 4. knowing the Sun's mass and measuring how Jupiter's speed changes during its elliptical ...
SKYTRACK Glossary of Terms
SKYTRACK Glossary of Terms

... It happens twice each year, when the tilt of the Earth's axis is most inclined toward or away from the Sun, causing the Sun's apparent position in the sky to reach its northernmost or southernmost extreme. (b) Time of the year when the day is either shortest, or longest depending on where you are. S ...
Your guide to see five planets after sunset
Your guide to see five planets after sunset

... The planets are visible from across Australia for an hour or so after local sunset. Venus, Jupiter, Mars and Saturn are bright enough to be seen during twilight when the rays of the setting sun still brighten the sky. Mercury, the faintest of the planets, is the one that's most easily drowned out an ...
Coursework 1 File
Coursework 1 File

... Exercise class question - not to be handed in This question concerns the precession of the equinoxes, the phenomenon where the direction pointed to by the Earth’s rotation axis changes continuously. This effect arises because of the gravity of the Sun and the Moon acting on the spinning Earth. It on ...
The Sun
The Sun

... sideways to their motion, binding the gas to the field. • Sunspots are like “magnetic scabs” of gas unable to be recirculated to lower, hotter levels. They are bound to the magnetic fields in the photosphere, cooling as they radiate to the cold universe, and hence cool and darken. • Vertical structu ...
Study regarding the landscape arrangement of the green space
Study regarding the landscape arrangement of the green space

... the blue orbits (Moon, Sunday) gravitate around the Earth. The objects on the orange orbits (Mercury, Venus, Mars, Jupiter, Saturn) gravitate around the sun. In the arrangement, the sun, being the star which can be found in the center of our solar system with a diameter of 109 times larger than the ...
Solar System Test Review - Garnet Valley School District
Solar System Test Review - Garnet Valley School District

... going around the sun or the moon going around the earth. 11. The _________________________ states the sun, earth and other objects in the solar system formed from a rotating cloud of gas, called a nebula, about 4.5 billion years ago. 12. The _________________________ is the orbital point at which th ...
Professor Jonathan Fortney TA Kate Dallas Thursday, February 11
Professor Jonathan Fortney TA Kate Dallas Thursday, February 11

... 48) Which of the following best describes why the smaller terrestrial worlds have cooler interiors than the larger ones? A) They had more volcanic eruptions in the past, which released their internal heat. B) They have relatively more surface area compared to their volumes. C) The smaller ones are f ...
How long does it take light to travel from the Moon to the Earth, a L
How long does it take light to travel from the Moon to the Earth, a L

... ____  The  Greenhouse  effect  would  no  longer  act  to  heat  the  Earth’s  atmosphere   ____  At  sunset  the  Sun’s  apparent  color  would  be  no  different  than  the  noon"me  Sun   ...
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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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