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Unit 4 Space
Unit 4 Space

... would kill any life on Earth they struck. Luckily, our magnetic field deflects this solar wind. We can see these particles being deflected when we see the Northern Lights. Large outbursts of solar winds can wreak havoc with satellites as well as Earthbound energy supplies such as power plants. (c) M ...
Animated Science Space Revision
Animated Science Space Revision

... methane. Saturn was known to the ancients, including the Babylonians and Far Eastern observers. Saturn turns on its axis once every 10 hours and 34 minutes giving it the second-shortest day of any of the solar system’s planets. Fusion does not occur in Saturn as it is a gas giant. Animated Science ...
Slide 1
Slide 1

... A new study has evidence that Jupiter's moon Europa is full of salt water. Previous studies have indicated that the surface of Europa is ice. Scientists were wondering what was underneath this ice. With the help of the Galileo spacecraft, we may finally have the answer. It all started when Galileo f ...
Our Fun Sun - Environmental Science Institute
Our Fun Sun - Environmental Science Institute

... body has. A table is given with the known gravitational force for each planet, as well as its diameter. Consider the planet Uranus. Uranus has a larger diameter than Earth, but still has a much smaller gravitational force factor relative to Earth. Uranus has less mass since it is a gas planet. This ...
Answer key for Space study guide
Answer key for Space study guide

... Beginning of spring March 20th or 21st ***Autumnal Equinox: Beginning of fall September 22nd or 23rd ...
Sun - Blackboard
Sun - Blackboard

... The distance between two stars on the celestial sphere can only be given as the difference between the directions in which we see the stars. Therefore, distances on the celestial sphere are measured as angles, i.e., in ...
Lesson 7
Lesson 7

... There is much information to learn about the planets. It takes Earth one year, 365 days, to complete one orbit around the sun. The planet Mercury takes only 88 days to orbit the sun, since it is closest to the sun; but Pluto takes 248 years. Pluto and Neptune are the coldest planets with temperature ...
3 Habitable Zones in Extrasolar Planetary Systems
3 Habitable Zones in Extrasolar Planetary Systems

... Jovian-type planets do not have a solid or liquid surface, covered by an atmosphere, near which organisms may exist. Therefore, usually they are considered as inhabitable. But there is the possibility that moons of giant planets are within a habitable zone. The best candidate for producing a habitab ...
Introduction: - TrevorMander.com
Introduction: - TrevorMander.com

... The closer to the poles you get (the greater the latitude), the greater the seasonal temperature effect of the tilt of the Earth, and the lower the sun will appear in the sky. Day and night is 6 months long at the poles. “The sun at the North Pole is continuously above the horizon during the summer ...
Earth Science 24.3 The Sun
Earth Science 24.3 The Sun

... eat, has somehow come from solar energy. The sun is also important to astronomers, since until recently, it was the only star we could study the surface of. Even with the largest telescopes, most other stars appear only as points of light. ...
Seasons
Seasons

... 5) More about the moon phases, and what must be known for the class regarding phases? (several) 6) What is the celestial sphere, and how does it affect our view of the night sky? 7) Can retrograde motion be described a bit more? ...
Volume 1 (Issue 6), June 2012
Volume 1 (Issue 6), June 2012

... Mercury, accordingly are the planets for which we see transits. However, as seen from outer planets such as Mars, Jupiter etc, the Earth itself transits the Sun. While transits of Mercury are relatively common, occurring once or twice every decade, the transits of Venus are extremely rare, occurring ...
Click www.ondix.com to visit our student-to
Click www.ondix.com to visit our student-to

... toward proper place where will rest thus terrestrial motion always linear always comes halt heavens however move naturally endlessly complex circular motion heavens therefore must made fifth different element called aither superior element aither incapable change other than change circular movement ...
Chapter 2 PowerPoint
Chapter 2 PowerPoint

... • Diurnal motion requires at least one celestial sphere • Annual motion requires at least one additional sphere • Irregular motion requires at least two additional spheres ...
Earth, Moon & Sun System
Earth, Moon & Sun System

... Solar Motion • When the northern axis is leaning away from the sun, the northern hemisphere gets the least direct rays • Because of the position of earth in its revolution, days are shorter so the earth has less time to absorb energy from the sun so the days are cooler. ...
Apparent size (apparent diameter)
Apparent size (apparent diameter)

... 2. This matter exploded outward (hence: Big Bang) 10-20 billion years ago. 3. The explosion created hydrogen (the simplest element) 4. The universe began to evolve with clouds of hydrogen contracting to form new stars. 5. We can observe the expansion and evolution of the universe continuing today. W ...
The Local Sky The Local Sky
The Local Sky The Local Sky

... energy hitting one square metre per second –  Flux can then be used to calculate apparent visual magnitude –  Some stars are so bright they have negative magnitudes –  Faint stars detected by telescopes have magnitudes larger than 6 –  Apparent visual magnitude is based only on visible light. –  App ...
Grade 9 Applied
Grade 9 Applied

... If the answer is true write T. If the answer is false write F. 26. _____ A nebula is a cloud of dust and gas, the birthplace of stars. 27. _____ Distances between the planets are measured in astronomical units. 28. _____ There is a black hole very close to the Earth. 29. _____The Milky Way is an ell ...
Venus Transit and the Astronomical Unit
Venus Transit and the Astronomical Unit

... Since A and B differ 9 in latitude and the circumference of Earth is given by 2r, the distance AB is given by AB = (2r/360) × 9 where r is the radius of Earth. Similarly, since the distance CD is 1/5 the solar diameter and the Sun subtends an angle of 30' or 0.5 at Earth, the angle  is 0.1, wh ...
July - Magic Valley Astronomical Society
July - Magic Valley Astronomical Society

... times interrupted by Pluto, whose unusual elliptical orbit periodically causes it to cross into Neptune's path, making Neptune the farthest planet from the sun for a 20-year period once every 248 Earth years. Though massive, Neptune has the smallest diameter of the solar system's "gas giants," a gro ...
Great Galaxies 5 - School Performance Tours
Great Galaxies 5 - School Performance Tours

... These are huge numbers and each of the numbers in this list is larger than the one before it. Some of these mathematical terms you may not have heard before but these are the numbers that are needed when calculating the distances from earth to other objects in the universe. For instance there are hu ...
8L Earth and Space SoW
8L Earth and Space SoW

... them to describe relationships in the data. L4-6 – 4 Selecting the data, The AT spreadsheet Selecting the data provides data about the planets, dwarf planets and some moons in the Solar System. Students are asked to use the data to help them to work out which statements are true. L5 – 5 Ratios and p ...
Alone in the Universe - Let There Be Light : The Book
Alone in the Universe - Let There Be Light : The Book

... candidates (planets not yet completely confirmed) that orbit in less than 50 days, University of California at Berkeley astrophysicist Andrew Howard and his team analyzed the trends they represent, including the finding that smaller planets are more abundant. There ...
Celestial Sphere 2015
Celestial Sphere 2015

... annual path of Sun on the CS ...
Origin of the Earth and of the Solar System
Origin of the Earth and of the Solar System

... A Supernova is a gigantic explosion of a massive star after gravitational collapse (if no more energy can be gained by nuclear fusion). At maximum a Supernova can be brighter than a whole galaxy. The outer layers are expelled, while the center collapses to a Neutron Star or even to a Black Hole. All ...
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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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