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Exam2 Review Slides
Exam2 Review Slides

... Cooler, smaller red stars have been around for a long time Hot, blue stars are relatively young. ...
The early atmosphere
The early atmosphere

... 117 Ways to Pass the Earth Science Standards of Learning (SOL) Test 1. The same substance always has the same density ...
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... 1. Jupiter has a gigantic magnetic field called the magnetosphere. 2. Jupiter gives off more heat than it absorbs from the sun. 3. All four of the gas giants have a ring system. 4. All the planets orbit the sun in the same direction. 5. The orbits of all the planets lie in a flat plane except for th ...
PHYS178 2008 week 11 part-1
PHYS178 2008 week 11 part-1

... "If the candidate companion of 2M1207 is really a planet, this would be the first time that a gravitationally bound exoplanet has been imaged around a star or a brown dwarf" says Benjamin Zuckerman of UCLA, a member of the team and also of NASA's Astrobiology Institute. Using high-angular-resolution ...
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Planetary Cycles

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RIPL Radio Interferometric Planet Search

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... 2.7% nitrogen, 1.6% argon and less than 1% oxygen. Compare this to Earth’s 77% nitrogen, 21% oxygen and less than 1/10 of 1% carbon dioxide. Although Mars’ atmosphere is not poisonous, you could not breathe it to stay alive. The average temperature is cold, around –81°F, but varies from –274°F to 72 ...
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Robotics - UNL CSE

... where detailed analysis is performed. The data are then returned back to the Data Management Center to be filed away. This process usually takes four months. A planet at an earth-like distance from its star is in the stars habitable zone, where temperatures are just right for liquid water to not fre ...
HW8 - UCSB Physics
HW8 - UCSB Physics

... If there are about 3 supernovae per century in our Galaxy, there is 1 supernova per 33.3 years on average (100/3 = 33.3 years). For 1 supernova to occur in the sphere of 300 pc in radius, there will be 1/9.58 × 10−5 = 1.04 × 104 supernovae in the whole Galaxy. Time interval for 1 supernova to occur ...
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slides - quantware mips center

... systems, i.e., the systems with two or more planets (H.Rein, 2012, MNRAS, 427, L21). About ~600 multiplanet systems are known. Orbital resonances are ubiquitous in planetary systems, as confirmed in computations of the behaviour of resonant arguments. The occurrence of low-order resonances (such as ...
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... called these objects planets, or wandering stars. Old drawings and manuscripts by people from all over the world, including the Chinese, Greeks and Anasazi, attest to their interest in comets, solar eclipses and other celestial phenomena. And observations of planets surely date to well before the da ...
Dark Skies Above Downeast Maine
Dark Skies Above Downeast Maine

... During  the  month  of  December,  there  will  be  at  least  1  minor  body  that  will  make  a  near     approach  to  the  Earth  within  a  distance  of  10  lunar  distances.  This  closest  approach  will  be   from  the ...
The Family of Stars
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AST 301 Fall 2007 AST 301: Review for Exam 3 This exam covers

... Chapter 15: This chapter is continuous with Chapter 6 because it is concerned with developing a theoretical model that can explain most of the features of our solar system that we read about in Chapter 6. I suggest you try testing your understanding of the material by telling a friend (imaginary or ...
July - Westchester Amateur Astronomers
July - Westchester Amateur Astronomers

... Strange but true: When it comes to finding new extrasolar planets, or exoplanets, stars can be an incredible nuisance. It’s a matter of luminosity. Stars are bright, but their planets are not. Indeed, when an astronomer peers across light years to find a distant Earth-like world, what he often finds ...
Beyond Our Solar System
Beyond Our Solar System

... particularly apparent for Mercury. – Its orbit carries it as close to the sun as 0.307 AU and as far away as 0.467 AU. – You can see this variation in the distance from Mercury to the sun in the figure. – Earth’s orbit is more circular, and its distance from the sun varies by only a few percent. ...
Partial Solar Eclipse Watch Party
Partial Solar Eclipse Watch Party

... Solar eclipses are not rare events, in spite of what many people think. A minimum of two and a maximum of five solar eclipses occur every year. Total eclipses are more rare; zero to two total solar eclipses can happen in a year. Every eclipse can't be observed everywhere on Earth, as the Moon's tiny ...
Stars
Stars

... Supergiants and Supernovas • Stars that are about 8 times more massive than the sun have a more violent star evolution. • The core heats up to much higher temperatures. Heavier and heavier elements form by fusion and the star expands into a supergiant. • Iron forms in the core. Iron cannot release ...
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Rare Earth hypothesis



In planetary astronomy and astrobiology, the Rare Earth Hypothesis argues that the origin of life and the evolution of biological complexity such as sexually reproducing, multicellular organisms on Earth (and, subsequently, human intelligence) required an improbable combination of astrophysical and geological events and circumstances. The hypothesis argues that complex extraterrestrial life is a very improbable phenomenon and likely to be extremely rare. The term ""Rare Earth"" originates from Rare Earth: Why Complex Life Is Uncommon in the Universe (2000), a book by Peter Ward, a geologist and paleontologist, and Donald E. Brownlee, an astronomer and astrobiologist, both faculty members at the University of Washington.An alternative view point was argued by Carl Sagan and Frank Drake, among others. It holds that Earth is a typical rocky planet in a typical planetary system, located in a non-exceptional region of a common barred-spiral galaxy. Given the principle of mediocrity (also called the Copernican principle), it is probable that the universe teems with complex life. Ward and Brownlee argue to the contrary: that planets, planetary systems, and galactic regions that are as friendly to complex life as are the Earth, the Solar System, and our region of the Milky Way are very rare.
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