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September 2007 - East Valley Astronomy Club
September 2007 - East Valley Astronomy Club

... the sun, (solar wind) and other places, [3]. This is called the planet’s magnetosphere. A planetary magnetosphere can also be thought of as the region surrounding a planet within which its own magnetic field dominates the behavior of electrically charged particles. The solar wind is constantly emana ...
Life`s unity and flexibility: the ecological link
Life`s unity and flexibility: the ecological link

... ancient fossil data. On the contrary, the phylogenetic analysis of cytochrome oxidase sequences indicated that aerobic organisms belonging to very diverse bacterial and archaeal groups used a homologous cytochrome oxidase and, therefore, that aerobic metabolism must have had a single and ancient ori ...
TAKS objective 5 Earth and Space Systems
TAKS objective 5 Earth and Space Systems

... The most widely accepted theory for the formation of the universe. It states that all matter & energy were once packed into a tiny particles smaller than speck of dust. This particle was incredibly hot & dense which suddenly began to expand. Overtime universe cooled & continued to expand. Evidence s ...
“Here Comes the Sun” How the new
“Here Comes the Sun” How the new

... point Sungenis makes several elementary errors. For example he is wrong about the strength of the gravitational attraction of various celestial bodies at the Earth, and he confuses two different physical concepts – the centre of mass of a system of bodies and a point in space with zero gravity. A po ...
100 Characteristics of Earth Reasons for the
100 Characteristics of Earth Reasons for the

... Why do the Sun and Moon APPEAR to move across the sky from our point-of-view on Earth? ...
honors earth science - Grosse Pointe Public School System
honors earth science - Grosse Pointe Public School System

... 3. Recognize moon phases from photos and diagrams (earth-moon-sun). Predict moon phases from dates 4. Compare and contrast solar and lunar eclipses. 5. Explain the cause of tides. 6. Relate tides to moon phases (spring, neap, normal) 7. Explain why we do not see the “far side” of the moon from earth ...
How to Measure the Earth - Ramapo College of New Jersey
How to Measure the Earth - Ramapo College of New Jersey

... Ramapo College of New Jersey ...
The Sky This Month Mar Apr 2015
The Sky This Month Mar Apr 2015

... The New Horizons spacecraft is scheduled to fly through the Pluto-Charon system on July 14, 2015, travelling approx. 13.78 km per second (49,600 kph), then head out into the Kuiper Belt. The Pluto-and-moons system will be approximately face-on, so close attention will be payed up to the last days of ...
los angeles unified school district
los angeles unified school district

... HS-ESS1-1: Develop a model based on evidence to illustrate the life span of the sun and the role of nuclear fusion in the sun’s core to release energy in the form of radiation: Emphasize energy transfer mechanisms that allow energy from nuclear fusion in the sun’s core to reach Earth. HS-ESS1-2: Con ...
The astrobiological case for our cosmic ancestry
The astrobiological case for our cosmic ancestry

... which had remained a mystery for over four decades (Wickramasinghe 1967). These dust particles make up about 1 % of the mass of the entire galaxy and exist in the form of ...
S T A R S
S T A R S

... the brighter planets like Jupiter, Venus, Mars and Saturn but is a bit hard for the fainter planets.  The planets give off a more steady light and the stars give off a twinkling light. That is because the light from the stars travel a far greater distance and will be distorted and bent a little som ...
Solar System
Solar System

... The distance from Earth to the Sun is 1 astronomical unit Solar System. Object sizes use one scale, orbit distances (150,000,000 km), or AU. For comparison, the radius of use another. the Sun is 0.0047 AU (700,000 km). Thus, the Sun occupies 0.00001% (10−5 %) of the volume of a sphere with a radius ...
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DATA FROM CATALOGUES OF SOLAR SYSTEM OBJECTS IN

... it is not suitable to use them directly in the education process. Another option is to use data directly from NASA at neo.jpl.nasa.gov/orbits/. There is available online application displaying the current position of the minor planet in the solar system. This page has been an inspiration for me duri ...
Goals & Objectives - Sierra College Astronomy Home Page
Goals & Objectives - Sierra College Astronomy Home Page

... is not your Student ID#, nor is it your SSN, not is it the same as any other Astronomy ID# you may receive in another course.  This number should be used on all assignments and correspondence with the instructor ...
ISS Sighting Opportunities
ISS Sighting Opportunities

... · New Moon (exact at 7:09 a.m. EDT). Wednesday, Sept. 28 · In bright twilight just 15 minutes after sunset, a telescope may show Saturn less than 2° above much-brighter Venus extremely low in the west. A very thin crescent Moon is setting 12° to their left. Look for Spica twinkling between the plane ...
New Horizons Spacecraft `Stays the Course` for Pluto System
New Horizons Spacecraft `Stays the Course` for Pluto System

... · As Mercury fades and descends below Venus day by day, how long can you keep it in view? ...
IES AZ-ZAIT - Junta de Andalucía
IES AZ-ZAIT - Junta de Andalucía

... 3. Answer the following questions: a. What do we call the days when both hemispheres have equal sunlight? b. What do we call the days when the day or night is the longest? c. What is the name of the zone between the two meridians? d. What is the name of the phase of the moon if you can’t see the Moo ...
Shouting in the Jungle: the SETI Transmission Debate
Shouting in the Jungle: the SETI Transmission Debate

... For a single parabolic antenna, the receiver’s 3 dB beamwidth, in radians, equals roughly wavelength divided by diameter [with the two measured in like units]. Given a terrestrial microwave signal at, say, the neutral hydrogen line (wavelength equal to 21 cm), the required receive antenna diameter t ...
Correct!
Correct!

... Name the order of the universe from the smallest to the greatest. Click on the letter of the correct answer ...
chapter 13 cosmology
chapter 13 cosmology

... learn what the universe was like in the past. However, there is a limit to how far back in time we can do this. If the universe is expanding and its volume is increasing now, then, in the past, the universe was smaller and things must have been crowded closer together. In fact, this has been confirm ...
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FREE Sample Here

... Answers/Discussion Points for Think About It/See It For Yourself Questions The Think About It and See It For Yourself questions are not numbered in the book, so we list them in the order in which they appear, keyed by section number. ...
Earth Science: GEU Standardized Test Practice SE
Earth Science: GEU Standardized Test Practice SE

... The theory of plate tectonics is supported as a valid theory because it ...
The Solar Nebula Theory
The Solar Nebula Theory

... • final large-scale collisions • Earth–Moon system • Mercury core formation ...
`Magnificent Desolation` transcript
`Magnificent Desolation` transcript

... aren’t really seas, there is no liquid water on the moon, they’re huge craters that were  flooded by molten rock long ago, but they got their name because early astronomers  mistakenly thought that the moon was covered in water.  Water isn’t the only thing the moon lacks, it does not have an atmosph ...
Trading Cards
Trading Cards

...  Asteroids orbit our Sun, a star, in a region of space between the orbits of Mars and Jupiter known as the Asteroid Belt.  One day on asteroid Ida, for example, takes only 4.6 hours (the time it takes for this asteroid to rotate or spin once). Ida makes a complete orbit around the Sun (a year in t ...
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Astrobiology



Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe: extraterrestrial life and life on Earth. This interdisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System, the search for evidence of prebiotic chemistry, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in outer space. Astrobiology addresses the question of whether life exists beyond Earth, and how humans can detect it if it does. (The term exobiology is similar but more specific—it covers the search for life beyond Earth, and the effects of extraterrestrial environments on living things.)Astrobiology makes use of physics, chemistry, astronomy, biology, molecular biology, ecology, planetary science, geography, and geology to investigate the possibility of life on other worlds and help recognize biospheres that might be different from the biosphere on Earth. The origin and early evolution of life is an inseparable part of the discipline of astrobiology. Astrobiology concerns itself with interpretation of existing scientific data; given more detailed and reliable data from other parts of the universe, the roots of astrobiology itself—physics, chemistry and biology—may have their theoretical bases challenged. Although speculation is entertained to give context, astrobiology concerns itself primarily with hypotheses that fit firmly into existing scientific theories.The chemistry of life may have begun shortly after the Big Bang, 13.8 billion years ago, during a habitable epoch when the Universe was only 10–17 million years old. According to the panspermia hypothesis, microscopic life—distributed by meteoroids, asteroids and other small Solar System bodies—may exist throughout the universe. According to research published in August 2015, very large galaxies may be more favorable to the creation and development of habitable planets than smaller galaxies, like the Milky Way galaxy. Nonetheless, Earth is the only place in the universe known to harbor life. Estimates of habitable zones around other stars, along with the discovery of hundreds of extrasolar planets and new insights into the extreme habitats here on Earth, suggest that there may be many more habitable places in the universe than considered possible until very recently.Current studies on the planet Mars by the Curiosity and Opportunity rovers are now searching for evidence of ancient life as well as plains related to ancient rivers or lakes that may have been habitable. The search for evidence of habitability, taphonomy (related to fossils), and organic molecules on the planet Mars is now a primary NASA objective on Mars.
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