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Earth in Space - Learning Outcomes
Earth in Space - Learning Outcomes

... Which star is furthest from Earth and by how many times? ...
Astronomy 100—Exam 2
Astronomy 100—Exam 2

... A. red giant, white dwarf, planetary nebula, main sequence B. planetary nebula, main sequence, red giant, white dwarf C. main sequence, white dwarf, red giant, planetary nebula D. main sequence, red giant, planetary nebula, white dwarf E. white dwarf, main sequence, planetary nebula, red giant 42. W ...
Lecture 18: The Milky Way Galaxy
Lecture 18: The Milky Way Galaxy

... ~ once every 10 million yrs. the electron flips its spin ...
Astronomy, Chapter 1 Learning Target #1 Explain the motion of the
Astronomy, Chapter 1 Learning Target #1 Explain the motion of the

... reaction, like in a hydrogen bomb.  Even though it is constantly exploding in a nuclear reaction, the Sun and other stars are so large and have so much matter in them that it will take billions of years for the explosion to use all the "fuel" in the star. ...
What did ancient civilizations achieve in astronomy?
What did ancient civilizations achieve in astronomy?

... •  Kepler first tried to match Tycho s observations with circular orbits ...
WORD - UWL faculty websites
WORD - UWL faculty websites

...  The top panel shows two stars (Blue = “A”; red = “B”) orbiting one another. The green dot represents the Earth. This diagram is NOT TO SCALE.  The bottom panel shows the combined absorption-line spectrum of the stars (with the lines from each star labeled “A” and “B”). A thin "stationary" absorpt ...
Document
Document

lecture 2
lecture 2

... • A solar eclipse occurs when the Moon moves between the Earth and the Sun • A lunar eclipse occurs when the Earth moves between the Sun and the Moon and the Moon moves through the Earth’s shadow ...
FREE Sample Here
FREE Sample Here

... facing them. For different positions of the Moon, ask students how much of the surface of the Moon is lit, and how much of the lit surface can be seen from Earth. Emphasize that half the surface is always receiving light, but we just do not see it all. Before showing Figure 0.13, demonstrate and dis ...
Activity: Doppler Effect
Activity: Doppler Effect

... • The top panel shows two stars (Blue = “A”; red = “B”) orbiting one another. The green dot represents the Earth. This diagram is NOT TO SCALE. • The bottom panel shows the combined absorption-line spectrum of the stars (with the lines from each star labeled “A” and “B”). A thin "stationary" absorpt ...
005 Astrophysics problems
005 Astrophysics problems

... Which star is furthest from Earth and by how many times? ...
Lecture 3a
Lecture 3a

... was the Church’s defender). Spent last years of his under house arrest for stating that the Sun was at the center of the “universe” (solar system) CONTRARY to Scriptures 162 Lecture 3a ...
Our Sun, Sol - Hobbs High School
Our Sun, Sol - Hobbs High School

... is a highly magnetized, spinning neutron star with jets of particles moving almost at the speed of light streaming out above its magnetic poles. • These jets produce very powerful beams of light. • The precise periods of pulsars make them useful tools to astronomers. ...
Grade 5 CPSD Science Curriculum Guide
Grade 5 CPSD Science Curriculum Guide

... and night, and the seasonal appearance of some stars in the night sky. The Performance Expectations of this unit expect students to demonstrate grade-appropriate proficiency in supporting an argument that the gravitational force exerted by Earth on objects is directed down; Supporting an argument th ...
Part 1- The Basics
Part 1- The Basics

... temperature) to bottom-right (low luminosity and low surface temperature) – 90% stars in this band – The Sun is one of main sequence stars – Hydrogen burning as energy source ...
word document - FacStaff Home Page for CBU
word document - FacStaff Home Page for CBU

... _____ e) The sun will probably go supernova sometime, probably in about 5.5 billion years. _____ f) Vega is a star that has a stellar classification of A0 V. From this we can infer that Vega is more massive than the sun. _____ g) The heaviest elements (gold, lead, uranium, etc.) are thought to be ma ...
Reasons for the Seasons Webquest
Reasons for the Seasons Webquest

... THE SEASONAL EFFECTS ARE THE RESULT OF THE EARTH’S AXIS FLIPPING BACK AND FORTH: TRUTH: The Earth’s axis does slowly wobble like a top, completing one cycle in approximately 26,000 years. This motion is called precession, and it is responsible for a gradual change in the location of the position in ...
Time and Diurnal Motion 1a. The Earth Is Flat
Time and Diurnal Motion 1a. The Earth Is Flat

Sirius Astronomer - Orange County Astronomers
Sirius Astronomer - Orange County Astronomers

29 Jan: Maps of the Sky
29 Jan: Maps of the Sky

... for 2010: 221,600 miles or 356,600 km, 7 % less than its average distance. This will make the full Moon appear slightly larger than usual. “ ...
TRANSIT
TRANSIT

Scattering (and the blue sky)
Scattering (and the blue sky)

Distances and Sizes - University of Iowa Astrophysics
Distances and Sizes - University of Iowa Astrophysics

... The bright star Vega has a measured parallax of 0.1 arcsec (p = 0.1″) This means that Vega appears to move from +0.1″ to -0.1″ with respect to distant stars over a year’s observation D(pc) = 1/p(″) = 1/0.1 = 10 pc Vega is 10 pc (parsec) from Earth (remember: 1 pc = 3.26 light years) ...
chapter 17 measuring the stars
chapter 17 measuring the stars

...  Most stars are members of multiple-star systems – groups of two or more stars in orbit around one another  Binary-star systems: A system which consists of 2 stars in orbit around their common center of mass, held together by their mutual gravitational attraction.  Most stars are found in binary- ...
Part 1
Part 1

... 11. At the center of the Sun, fusion converts hydrogen into (A) water and carbon dioxide. (B) plasma and smoke. (C) radiation and elements like carbon and nitrogen. (D) radioactive elements like uranium and plutonium. (E) helium, energy, and neutrinos. 12. In order to start nuclear fusion, a high t ...
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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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