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Avogadro`s Number
Avogadro`s Number

... Avogadro’s number is almost incomprehensibly large. For example if one mole of dollars was given away at the rate of a million dollars per second beginning when the Earth was first formed some 4.5 billion years ago, would any remain today? Surprisingly, about three fourths of the original mole of do ...
Exploring Space
Exploring Space

... The universe is everything in space—all matter and energy are part of it. Our Milky Way galaxy is just one of more than 125 billion known galaxies in the universe. A fundamental question in astronomy is: how did the universe form? In 1929, astronomer Edwin Hubble observed that all of the galaxies he ...
Space Jeopardy
Space Jeopardy

... Stars for 4 Question:Planets that are close to the sun…. a)move through the asteroid belt b)orbit faster than the outer planets c)orbit slower than the outer planets d)move closer and closer to the sun ...
Jupiter - Midland ISD
Jupiter - Midland ISD

...  Hydrogen and helium make up 92% of Jupiter  When Jupiter formed 4.6 billion years ago, it did not have enough mass to allow nuclear fusion to begin so it never became a star.  The alternating light and dark burst of its surface makes Jupiter unique in our solar system. ...
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society

... the constellation Cygnus, monitoring their brightness photometrically every 30 minutes for four years. It was searching for any minute decreases in brightness that might indicate one or more planets transiting (passing in front of) their host star as seen from Earth. (For comparison, if Earth transi ...
Science and the Universe - Wayne State University Physics and
Science and the Universe - Wayne State University Physics and

... From our location within the Galaxy, we cannot see through its far rim because the space between stars is not empty, but contains (an extremely sparse distribution of) interstellar dust or gas which absorbs visible light The interstellar gas and dust are believed to be the raw material for future fo ...
PLANETARY SCIENCE
PLANETARY SCIENCE

... the solar system. One AU is the average distance between Earth and the Sun, which is equal to about 150,000,000 km. For measuring distances outside the solar system, astronomers use a unit called a light-year. The symbol for light-year is ly. One light year is the distance light travels in a vacuum ...
document
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... g is the strength of the gravitational field at some point, then the gravitational force on an object of mass m at that point is Fgrav = mg.  If g is the gravitational field strength at some point (in N/kg), then the free fall acceleration at that point is also g (in m/s2). ...
Stefan-Boltzmann`s law Wien`s law
Stefan-Boltzmann`s law Wien`s law

... Cosmological background radiation / Cosmic microwave background radiation (CMB) is microwave radiation - left over from the Big Bang that fills the universe roughly uniformly in all directions. The Big Bang predicts an expanding universe that had a very high temperature at the beginning; during the ...
ISNS3371_020607_bw
ISNS3371_020607_bw

... diameter) crater Pwyll 1000 kilometers to the south. - a few small craters - less than 500 meters in diameter were probably formed at the same time as the blanketing occurred by large, intact, blocks of ice thrown up in the impact explosion that formed Pwyll. ...
New Light on the Solar System
New Light on the Solar System

A Brief guide to the night Skies for those who know nothing
A Brief guide to the night Skies for those who know nothing

... tenth planet outside the orbit of Pluto, but as yet this has not been proved to exist. ...
282 ways to pass Earth Science Answers
282 ways to pass Earth Science Answers

... Earth received mainly short wave ____ visible____ during the day and later reradiates this energy back into space as _____ infrared energy _________waves (heat energy). 108. Infrared heat energy is absorbed by two gases ____Carbon dioxide__ and ____ water vapor__ (green house gasses). 109. As the am ...
Earth Science
Earth Science

... Earth received mainly short wave ____ visible____ during the day and later reradiates this energy back into space as _____ infrared energy _________waves (heat energy). 108. Infrared heat energy is absorbed by two gases ____Carbon dioxide__ and ____ water vapor__ (green house gasses). 109. As the am ...
Name_________KEY 282 WAYS TO PASS THE EARTH SCIENCE
Name_________KEY 282 WAYS TO PASS THE EARTH SCIENCE

... Light from distant galaxies show a shift to the ___ red_______ end of the visible spectrum, which is evidence that the universe is ____ expanding ___________. Our Solar System ...
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... The apparent magnitude of stars was first recorded by the Greek astronomer Hipparchus about 160 B.C. Hipparchus grouped stars according to their brightness or magnitude. He called the twenty brightest stars first magnitude stars. Stars half that bright were second magnitude. Third magnitude stars we ...
EARTH SCIENCE REGENTS REVIEW
EARTH SCIENCE REGENTS REVIEW

... * The Milky Way galaxy is about 100,000 light years across and has a spiral shape. We are located towards the end of a spiral arm. * A light year is the distance light travels in one year (9.5 trillion kilometers) * The Sun is an average star (part of the Main Sequence) and is about half-way through ...
Universe Discovery Guides: January
Universe Discovery Guides: January

... nearing the end of its life and has expanded to become a red supergiant star. But it is still working hard to build the wealth needed to support future generations of stars within our galaxy. Imagine you could be deep inside Betelgeuse, near its core — the star’s storehouse. You could watch the star ...
Climate Change
Climate Change

... Celsius ...
ExTRaSOLaR pLaNeTS
ExTRaSOLaR pLaNeTS

... The Optical Gravitational Lensing Experiment (OGLE) located at Las Campanas, Chile, was used to find the first planet through ...
Is our solar system unique?
Is our solar system unique?

... Ways to Find Out • Look at our own solar system, and think about how it might have formed • Look at other solar systems while they form • Look for and study other solar systems • Create computer models and see if you can produce a solar system ...
How did the Solar System form?
How did the Solar System form?

... Ways to Find Out ...
Astronomy - Surfin` Through the Solar System
Astronomy - Surfin` Through the Solar System

... 3. Constellation- a group of stars that can be seen as a pattern from Earth 4. Comet- a bright body that orbits the sun in an oval shaped path 5. Meteor- chunks of rock or metal flying through space 6. Asteroid Belt- asteroids that orbit the sun between Mars and Jupiter Procedures/Activities 1. Read ...
planetary temperatures, albedos, and the greenhouse effect
planetary temperatures, albedos, and the greenhouse effect

... from the reflectivity of different portions of it. For example, the surface of the Moon has an albedo of 0.07 (on average, 7% of the incident sunlight is reflected, 93% is absorbed), even though there are bright and dark regions that have reflectivities different from the average. We can measure the ...
4th Unit
4th Unit

... the Soviet Union and the United States), as well as a later missions to space? What space spin-offs are used now by our society that were originally created for use in space? ...
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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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