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Lecture 1
Lecture 1

... position of Star A as seen in July and label it “Star A July”. Describe how Star A would appear to move among the distant stars as Earth orbits the Sun counterclockwise from January of one year, through July, to January of the following year. Consider two stars (C and D) that both exhibit parallax. ...
Lecture26_Future
Lecture26_Future

Dynamics of disks with planets
Dynamics of disks with planets

The Dynamics of the Galaxies in the Local Group
The Dynamics of the Galaxies in the Local Group

... Milky Way Future • The Milky Way will merge with the Andromeda galaxy to become an elliptical galaxy – Their collision does not need to be as direct a hit as shown in the movie – They do always approach each other close enough to make a merger inevitable ...
Earth Science Exams and answer keys 2015 Season
Earth Science Exams and answer keys 2015 Season

... D) new 62. This diagram represents the moon revolving around the Earth in an elliptical orbit. As the Moon makes one complete revolution around the Earth starting at the position shown, how will the gravitational attraction between the Moon and Earth vary? A) decrease, then increase B) increase, the ...
The Milky Way Galaxy is Heading for a Major Cosmic Collision
The Milky Way Galaxy is Heading for a Major Cosmic Collision

... Milky Way Future •  The Milky will merge with the Andromeda galaxy to become an elliptical galaxy –  Their collision does not need to be as direct a hit as shown in the movie –  They do always approach each other close enough to make a merger inevitable ...
PE-00-intro-course outline
PE-00-intro-course outline

... predict the behavior of all energy and of all matter in the universe except for that which is (or was) both very massive and very small.  The various physical, chemical and biological systems and cycles of Earth have made it a rare yet unlikely unique home for life.  The evolution of the universe ...
Is there life outside of Earth? Activity 2: Moving Stars and Their Planets
Is there life outside of Earth? Activity 2: Moving Stars and Their Planets

... and the “Rocky-planet” switch. A rocky planet is denser than a gaseous planet, so the mass of the rocky planet will be higher than a gaseous planet of the same size. The mass of the student-created planet is given in the upper right-hand corner of the model in multiples of Earth’s mass. Encourage yo ...
EarthScience_Topic 3
EarthScience_Topic 3

... – Meteor: a streak of light in the sky that occurs when a meteoroid enters Earth’s atmosphere “shooting star” ...
Sample Stellar Evolution TEST QUESTIONS
Sample Stellar Evolution TEST QUESTIONS

... 7. Nuclear fusion in stars is controlled by the dependence of density on mass. 8. The Sun has a core in which energy travels outward primarily by radiation. 9. Energy flows by radiation or convection inside stars but almost never by conduction. 10. Hydrostatic equilibrium refers to the balance betwe ...
Pluto
Pluto

...  Temperature: What is the temp. range your planet? How does this compare to the temperature on Earth?  Composition of Your Planet and its Appearance: What type of planet is it (is it rocky or a gas giant)? What is its internal composition? What does your planet look like?  Rings: If there are rin ...
Activity I: Plotting a Light Curve due to a Transit
Activity I: Plotting a Light Curve due to a Transit

... this dip in intensity repeated every 3.52 days. From the drop in intensity and the length of the period we can tell a number of things about the planet. The drop in intensity can lead us to tell the size of the planet and thus, if it is large enough to hold an atmosphere. The period of the planet wi ...
Chapter 19. Mapping the Universe from Herschel to Sloan
Chapter 19. Mapping the Universe from Herschel to Sloan

... (Andromeda Galaxy) and M33, but the star were too faint to obtain spectra which could be classified. Therefore, we did not know if these stars were ordinary main sequence objects in a rather nearby cluster of stars, within the boundaries of the Milky Way Galaxy or whether they were supergiants in a ...
transit observations of new planets
transit observations of new planets

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Slide 1

... Venus is the victim of a runaway greenhouse effect—just kept getting hotter and hotter as infrared radiation is reabsorbed ...
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15_Uranus Litho.indd

... Uranus was discovered in 1781 by astronomer William Herschel. The seventh planet from the Sun is so distant that it takes 84 years to complete one orbit. Uranus, with no solid surface, is one of the gas giant planets (the others are Jupiter, Saturn, and Neptune). ...
Class 28 (Jun 2) - Physics at Oregon State University
Class 28 (Jun 2) - Physics at Oregon State University

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Chapter 13 section 2
Chapter 13 section 2

... absolute magnitude is about average. The Sun shines with a yellow light. Although the Sun is an average star, it is much closer to Earth than other stars. Light from the Sun reaches Earth in about eight minutes. Light from other stars takes many years to reach Earth. The Sun is unusual in one way. I ...
Astronomy in 1936 The History of the Universe
Astronomy in 1936 The History of the Universe

... • Evidence showing density waves do occur. • Old, red stars show spiral density perturbation. • Molecular clouds form on inner edges of spiral arms. • HI gas flow shows discontinuity due to shocks at inner edges of spiral arms. • Bright young stars also in narrow arms. • Observed width ∆θ ~ t*(Ω - Ω ...
Debris Belts around Vega - Astronomical Society of the Pacific
Debris Belts around Vega - Astronomical Society of the Pacific

memphis astronomical society short course in astronomy 2015
memphis astronomical society short course in astronomy 2015

... particularly difficult test, but you are expected to know most of the important concepts in astronomy. You should not feel that the test is like a final exam in an astrophysics course, but if you pass it, you can rightly be called a “Knowledgeable Amateur Astronomer”. The various segments are listed ...
Dorn_projectF08 - Bowling Green State University
Dorn_projectF08 - Bowling Green State University

... changing appearance of its surface. The Moon orbits at roughly 380,000 km. distance with a diameter of 3475 km., compared to Earth it is 27% smaller with a reflection magnitude at opposition of -12.7. The best views through a telescope are between the crescent and quarter phases when angled light fr ...
Study Guide for Earth Science Final
Study Guide for Earth Science Final

... 109. What is the composition of the sun? 110. What are the characteristics of sunspots? 111. What is the source of the sun’s energy? 112. Describe the relationship of color and temperature of stars. 113. What do light-years measure? 114. What characteristic of a star does magnitude describe? 115. De ...
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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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