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Magic
Magic

... Meridian. A circle of longitude passing from the South point of the horizon, through the zenith to the North point of the horizon. It coincides with geographical longitude - a great circle crossing the equator and passing through the poles. Every point on the Earth's surface has its own meridian or ...
ppt
ppt

... Ch12: Cloud-covered Venus Ch13: Red Planet Mars Ch14: Jupiter and Saturn Ch15: Satellites of Jup. & Saturn Ch16: Outer World Ch17: Vagabonds of Solar System ...
Small Bodies of the Solar System Transcript
Small Bodies of the Solar System Transcript

... rocks barely tens of metres in diameter. As with so many natural distributions, there are fewer of the larger objects, and ever-increasing numbers at progressively smaller sizes. We expect that there are over a million objects larger than 1 km across, and many millions that are yet smaller. We can d ...
Habitability of planets around Red Dwarf Stars
Habitability of planets around Red Dwarf Stars

... to that the SSP will be given by the cosine of the angular distance from the SSP). On a tidally locked planet, we would expect zero obliquity; no diurnal insolation maxima and no summer growth season, or seasonal rains. Given a constant location of the sun in the sky, however, photosynthetic surface ...
The Formation of Planetary Systems
The Formation of Planetary Systems

... What about the exceptions (major ones listed here)? Mercury’s large metallic core Venus’ retrograde rotation Earth – Moon system Mars’s north–south asymmetry Uranus’s tilted axis Astronomy 1-1 ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... During a total lunar eclipse, the Moon moves passing in the Earth’s shadow. By observing the Moon during the eclipse, the ancient Greeks found that the diameter of the Earth’s shadow was about two-and-a-half times the Moon’s own diameter, at the distance of the Moon. The Greeks used this observation ...
File
File

... Reading Skills Read the passage below. Then, answer questions 9–10. The Chandler Wobble In 1891, an American astronomer named Seth Carlo Chandler, Jr., discovered that Earth “wobbles” as it spins on its axis. This change in the spin of Earth’s axis, known as the Chandler wobble, can be visualized if ...
Tackling the 5th Grade Science Test
Tackling the 5th Grade Science Test

... and/or debris that orbit them. Comets, asteroids and meteoroids orbit the sun. 2. Asteroids are metallic, rocky bodies that orbit the sun but are too small to be classified as a planet. 3. A meteor appears when a particle or chunk of metallic or stony matter called a meteoroid enters Earth’s atmosph ...
Session 1 - Museum of Natural Science and History
Session 1 - Museum of Natural Science and History

... Even faster – earth material would fly off into space, it would overcome the force of gravity. In this case it would never have formed a planet in the first place. Assumptions – earth is old, and thus to spin was greater in the distant past and these would be problems. Conclusion – assumptions are p ...
Lecture7_2014_v2
Lecture7_2014_v2

... – Doesn’t explain difference between earth-like planets, gas giants, ice giants ...
Chap. 2: Known the Heavens
Chap. 2: Known the Heavens

... are fixed on its surface • In the sphere, all stars are assumed in the same distance • The Earth is stationary and at the center of the sphere • Note that it is an imaginary object that has no basis in physical reality • However, it is a model that remains to be very useful for positional astronomy ...
The sun is a star.
The sun is a star.

... -Those who study the celestial bodies and their movements are called astronomers. -Aryabhatta was a famous astronomer of ancient India. -Sun provides the pulling force that binds the solar system. -The sun is about 150 million km away from the earth. -There are eight planets in our solar system. In ...
Earth Science Spring Break Packet 2016
Earth Science Spring Break Packet 2016

... there. Which reason explains this? A. The Moon has no wind or rain. B. Time passes much slower on the Moon. C. The dust on the Moon hardened into stone. D. The heavy astronauts left very deep footprints in the Moon's dust. 62. Each year, Earth moves once around A. Mars. B. Venus. C. the Sun. D. the ...
Ch 28-31
Ch 28-31

... 360 divided by 15 is 24 so there are 24 hours in a day! http://huntingtonastro.wikispaces.com/file/view/earth-rotation.png/199559520/earth-rotation.png ...
What`s Up, Earth?
What`s Up, Earth?

... Historically, the Earth's shape was discovered by studying the way ships disappear below the horizon as well as the shape of Earth's shadow on the Moon during an eclipse. Both of these methods rely on rather intricate reasoning. Fortunately, there is no need to pursue the historical route. We know ...
Basic Information about the Solar System Handout
Basic Information about the Solar System Handout

... planets, or exoplanets. As of early February 2011, astronomers have detected a total of 510 planets orbiting other stars. This number is up from the milestone of 100 exoplanets discovered as of January 2004. Most known exoplanets are gas giants, Jupiter-like planets, since current methods favor the ...
Solutions: Doppler Effect
Solutions: Doppler Effect

... At that time, Star B is moving directly away from Earth • Go to: http://www.howstuffworks.com/planet-hunting2.htm • Read the material and watch the animation. 7. How do we use the Doppler effect to help us detect the presence of planets around other stars? Because the planet tugs on the star (gravit ...
WORD - UWL faculty websites
WORD - UWL faculty websites

... At that time, Star B is moving directly away from Earth  Go to: http://www.howstuffworks.com/planet-hunting2.htm  Read the material and watch the animation. 7. How do we use the Doppler effect to help us detect the presence of planets around other stars? Because the planet tugs on the star (gravit ...
Chapter 17 - Department Of Computer Science
Chapter 17 - Department Of Computer Science

... The Moon revolves eastward around the Earth in an elliptical orbit  There are two different months – The period of the Moon with respect to the Sun is a little over 29.5 days – synodic month, or the month of the phases – The period of the Moon with respect to a star other than the Sun is approximat ...
Our solar system
Our solar system

... determines where various materials condense out; this determines where rocky planets and gas giants form. ...
L53 SNOWBALL PLANETS AS A POSSIBLE TYPE OF WATER
L53 SNOWBALL PLANETS AS A POSSIBLE TYPE OF WATER

... Terrestrial planets with abundant water have multiple climate modes, including an ice-free, a partially icecovered, and a globally ice-covered state. Recent geological studies have revealed that the Earth experienced global glaciations in its history (“snowball Earth” hypothesis). In the snowball gl ...
ASTRONOMY 113 Modern Astronomy
ASTRONOMY 113 Modern Astronomy

... with Powerpoint, Prezi, Google Sheets or similar, and add an audio narrative with free software like Jing, Screencast, etc., and post the final combined video to the blog as a single video on youtube or with other video software (like iMovie). From each lectures topic, pick a subject to ...
October 28, 2014
October 28, 2014

... binoculars to look a bit right of the Moon for Alpha Capricorni, a wide, lovely yellow double star. Look to Alpha's lower left for Beta Capricorni, a less wide, more difficult double for binoculars; the secondary star in this case is fainter. Mercury is now in its best dawn display for 2014. (The bl ...
Advanced AMG EOC Review 2014-2015
Advanced AMG EOC Review 2014-2015

... What are the three levels of cloud heights and what types of clouds are associated with them? What is the one type of cloud that spans all three heights? Describe the difference between water vapor and clouds, and clouds and precipitation. What precipitation process operates in cold clouds? What pre ...
ppt
ppt

... “By reason of the deviation of the Sun from the center of gravity, the centripetal force does not always tend to that immobile center, and hence the planets neither move exactly in ellipses nor revolve twice in the same orbit. There are as many orbits of a planet as it has revolutions, as in the mot ...
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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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