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Ch 28-31 Lessons
Ch 28-31 Lessons

... 2. What causes the day and night cycle? ________________________________________________________________ How long is the day/night cycle? ___________________ 3. What is actually happening when the Sun rises at a particular location on Earth? __________________________________________________________ ...
File
File

... to determine the “age”. _____________________ Precession causes the equinox constellation to shift west. Early in the 21st Century the equinox will move west and begin the age of _______________________. What constellation is the sun in on June 21? ...
discover the wonders above
discover the wonders above

... LIGHTNING STORMS ...
Print this PDF
Print this PDF

... contain  silicate  materials  that  were  melted  in  space,  amino  acids,  and  other  presolar  grains,  particles   likely  formed  from  stellar  explosions.  Diamond  and  graphite  are  among  materials  found  to  be  present   in  these  grains.  Chondrites  are  thought  to  be  over  4.5 ...
cook - University of Glasgow
cook - University of Glasgow

... Sound method, but angle between Sun and Moon hard to measure precisely. Heliocentric model (Sun much larger than the Earth). Not widely accepted, because no parallax shift ...
Death by Black Hole Study Guide-Answers - crespiphysics
Death by Black Hole Study Guide-Answers - crespiphysics

... 3. What evidence did Galileo cite for a Sun centered universe? Venus has phases; Jupiter has 4 large moons that orbit it 4. Describe how Harlow Shapely used the distribution of globular clusters to determine we were not at the center of the Milky Way (or universe). He observed they were not evenly d ...
Jupiter
Jupiter

... Jupiter is the most stormiest planet in our solar system with wind that mostly reach 300 miles per hour and one of the strongest, biggest and the longest storm to last is the great red spot in southern hemisphere and it has lasted for more than 300 years and the wind speed over 500 miles per hour . ...
- ISP 205, sec 1 - Visions of the
- ISP 205, sec 1 - Visions of the

... 26. A It turned into carbon dioxide by reacting with nitrogen in Venus’s atmosphere. B It is frozen in craters near the poles. C Water was removed from the atmosphere by chemical reactions with surface rock. D Ultraviolet light split the water molecules, and the hyrdrogen then escaped to space. ...
pompton lakes high school - Pompton Lakes School District
pompton lakes high school - Pompton Lakes School District

... theory and testing in their study of the universe.  Explain the concept of the celestial sphere and how we use angular measurement to locate objects in the sky.  Describe how and why the Sun, Moon and stars appear to change their positions from night to night and from month to month.  Explain how ...
pompton lakes high school - Pompton Lakes School District
pompton lakes high school - Pompton Lakes School District

... theory and testing in their study of the universe.  Explain the concept of the celestial sphere and how we use angular measurement to locate objects in the sky.  Describe how and why the Sun, Moon and stars appear to change their positions from night to night and from month to month.  Explain how ...
Eyes to the Sky
Eyes to the Sky

... Our own galaxy seen edge-on; this faint band crossing the sky is the combined light of millions of stars. ...
Earth and Space Science
Earth and Space Science

...  Recognize and discuss the different properties of soil, including color, texture (size of particles), the ability to retain water, and the ability to support the growth of plants.  Explain how air temperature, moisture, wind speed and direction, and precipitation make up the weather in a particul ...
Habitability of the Goldilocks planet Gliese 581g: results from
Habitability of the Goldilocks planet Gliese 581g: results from

... Aims. In 2010, detailed observations have been published that seem to indicate another super-Earth planet in the system of Gliese 581, which is located in the midst of the stellar climatological habitable zone. The mass of the planet, known as Gl 581g, has been estimated to be between 3.1 and 4.3 M⊕ ...
Test Bank for Life in the Universe, Third Edition Chapter 2: The
Test Bank for Life in the Universe, Third Edition Chapter 2: The

... 37. What is the relationship between Newton's three laws and Kepler's three laws? A) Newton's laws can be derived from Kepler's laws B) Newton's laws and Kepler's laws are identical C) Kepler's laws are general and apply to any motion, while Newton's laws apply only to planetary motion in the solar ...
navigation - Claire Lambe Home
navigation - Claire Lambe Home

... lodestone, when floated on water, always pointed north. Pytheas, a Greek explorer in the 4th Century B.C. sailed far enough north to discover the legendary Thule which inspired Virgil to create the concept of Ultima Thule, the 'uttermost point attainable'. 'Farthest Thule', where day and night each ...
Conceptual Physics - Southwest High School
Conceptual Physics - Southwest High School

... towards the earth, measured by how far it falls below straight line motion in one second, is less than that of an apple here on earth by the ratio of five meters to 1.37 millimeters, which works out to be about 3,600. What can be the significance of this much smaller rate of fall? Newton’s answer wa ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... Tidal heating slows the bodies' rotation until it becomes tidally locked, and the tidal bulge does not change any more. Two (from many) examples of tidal heating: Moon’s rotation, originally faster than now (the Moon showed all sides earlier), has been tidally locked to the Earth since 3.5 bill. y. ...
Events: - Temecula Valley Astronomers
Events: - Temecula Valley Astronomers

... Earth is built like a layer-cake, with the less dense atmosphere, ocean, and crust floating atop the denser mantle, which in turn floats atop the outer and inner cores of our planet. An iceberg’s buoyancy is enough to lift only about one tenth of it above the sea, with the other nine tenths below th ...
Precession of the Equinox - Binary Research Institute
Precession of the Equinox - Binary Research Institute

... with its large fixed stones, is an ideal vantage point for observing this slow movement of the stars from year to year, and ancient cultures certainly had many of these “observation” structures. Nevertheless, it would have taken generations, and careful record keeping to notice a large enough moveme ...
Unit 11: Astronomy
Unit 11: Astronomy

... 2. Solar size units In this section, we will use the diameter of the sun to represent a unit of 1. We will call this unit the sun size unit. diameter of the sun = 1,392,000 km = 1 sun size unit = 1 SSU We can compare the size of other objects to the sun using the sun size unit. 1. How many sun size ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... Tidal heating slows the bodies' rotation until it becomes tidally locked, and the tidal bulge does not change any more (68). Two (from many) examples of tidal heating: Moon’s rotation, originally faster than now (the Moon showed all sides earlier), has been tidally locked to the Earth since 3.5 bill ...
meteor shower
meteor shower

... http://cometography.com/pcomets/109p.html • Meteorites ...
Here - ScienceA2Z.com
Here - ScienceA2Z.com

... Hubble image of protoplanetary disks in the Orion Nebula, a light-years-wide "stellar nursery" likely very similar to the primordial nebula from which our Sun formed. After 100 million years, the pressure and density of hydrogen in the centre of the collapsing nebula became great enough for the prot ...
The Constellation Lepus, the Hare
The Constellation Lepus, the Hare

... days. R Leporis is at a distance of 1500 light-years. The colour intensifies as the star brightens. It was named for John Russell Hind and has been reputed to be the most beautiful star in the sky. There is one Messier Object in Lepus, M79, discovered in 1780 by Pierre Méchain. It is a globular clus ...
How the Earth Moves Transcript
How the Earth Moves Transcript

... slightly detracted from the original simplicity of this new model. Fearing the reaction of the Catholic Church, who had declared as doctrine that the Earth occupied the centre of the Universe, Copernicus delayed the publication of his model until 1543, the year of his death. Unfortunately, the predi ...
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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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