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PRS Questions (queestions after Midterm 2)
PRS Questions (queestions after Midterm 2)

... Conservation of energy Newton’s law of gravity Actually, all of these laws of physics are important factors ...
Northern and Southern Hemisphere Star Chart
Northern and Southern Hemisphere Star Chart

Our Universe - E Natural Health Center
Our Universe - E Natural Health Center

... Only the most massive stars—those of more than three solar masses—become black holes at the end of their lives. Stars with a smaller amount of mass evolve into less compressed bodies, either white dwarfs (白矮星) or neutron stars (中子星). Black holes are difficult to observe on account of both their smal ...
5-E Galaxy T - McDonald Observatory
5-E Galaxy T - McDonald Observatory

Digging Deeper - subfreshmanhomework2016-2017
Digging Deeper - subfreshmanhomework2016-2017

... Not all of the stars in the sky can be seen from a single location. A person viewing stars in the Northern Hemisphere cannot see all the stars visible in the Southern Hemisphere. Some are located below the horizon. The stars that can be observed from any given place also vary throughout the year. As ...
Jeopardy - Mr. Morrow`s Class
Jeopardy - Mr. Morrow`s Class

... Stars do not move, but because Earth is rotating it looks like they move across the night sky from east to west. ...
ASTRONOMY 161
ASTRONOMY 161

... Moon is surrounded by a ring of Sun. (3) Partial: Observer is in penumbra, to one side of umbra; Moon takes ‘bite’ out of Sun. ...
The Celestial Sphere Friday, September 22nd
The Celestial Sphere Friday, September 22nd

... Moon is surrounded by a ring of Sun. (3) Partial: Observer is in penumbra, to one side of umbra; Moon takes ‘bite’ out of Sun. ...
Advanced STARS - WordPress.com
Advanced STARS - WordPress.com

... It is the 2nd closest planet to the sun It is the closest planet to Earth Venus orbits the sun every 224.7 earth days It’s rotation is very slow. It takes 243 earth days to complete 1 rotation. So a year on Venus is shorter than a day on Venus Venus rotates in the opposite direction of other planets ...
Ch 28-31
Ch 28-31

... “atmosphere” of hydrogen gas from the inner planets. ...
Astronomy (stars, galaxies and the Universe)
Astronomy (stars, galaxies and the Universe)

... All stars are created from the gases in a nebula When the contracting gas and dust from a nebula become so dense and hot that nuclear fusion begins, the protostar begins to shine When a star begins to run out of fuel, its core shrinks and its outer portion expands The evolutionary path of a star dep ...
How a small scientific spark grew during the Renaissance
How a small scientific spark grew during the Renaissance

... From Ptolemaeus life we don’t know much. But he was more common as Ptolomy. However, he is known for three scholar works, they all have to do with Geography, Astronomy and Geometry. Ptolomy made the first steps in understanding our Universe. The model of the solar system developed by Ptolemy (87 - 1 ...
Study Guide for the Comprehensive Final Exam
Study Guide for the Comprehensive Final Exam

... Solve problems relating to the relative brightness or luminosity of two stars given their m or M values. Determine the hottest and coolest stars from a list of stars with their spectral types. State or identify a characteristic temperature for an O star, a G2 star and an M star. Solve problems with ...
Part A
Part A

... 7. Most of the mass in the universe is in stars. 8. The Big Bang theory is an explanation of the beginning of the universe. ...
Chapter One: Mapping the Earth`s Surface
Chapter One: Mapping the Earth`s Surface

... o Technically you wouldn’t fall off even if there was an edge – why not? Gravity pulls you towards Earth’s center.  Lunar eclipses – our shadow is round! Demo with balloons and projector  Pictures from outer space – BEST PROOF! ...
19 The Milky Way Galaxy
19 The Milky Way Galaxy

class 1,S11
class 1,S11

... • How did we come to be? —The matter in our bodies came from the Big Bang, which produced hydrogen and helium. —All other elements were constructed from H and He in stars and then recycled into new star systems, including our solar system. • How can we know what the universe was like in the past? • ...
- Schwab`s Writings
- Schwab`s Writings

... like the “fractals” of chaos theory. A newer theory 4 is an outgrowth of “string” theory and posits the perpetual repetition of “branes” in multidimensional space touching each other as starting points of new universes every time one of them cools off in infinite dissipation. The most commonly accep ...
BBC Stargazing Live Star and Moon Guide
BBC Stargazing Live Star and Moon Guide

... The Moon is the Earth’s only natural satellite. Apart from Mercury and Venus, all the other planets in the Solar System have their own moons. Jupiter has more than 60 but only four can be seen easily through a small telescope. These are known as the Galilean moons in honour of their discovery by Gal ...
Chapter 8 - TeacherWeb
Chapter 8 - TeacherWeb

... Large stars may explode and become supernovas, black holes, neutron stars, or pulsars. Supernovas: Massive stars use hydrogen faster than smaller stars. They don’t tend to have long lives when compared to other stars. When it explodes it may become a supernova—a gigantic explosion which throws the s ...
Astronomy (stars, galaxies and the Universe)
Astronomy (stars, galaxies and the Universe)

The Sun!!
The Sun!!

Lucas - WordPress.com
Lucas - WordPress.com

... Auriga is located north of the celestial equator. Its name is the Latin word for "charioteer", associating it with various mythological charioteers, including Erichthonius and Myrtilus. Auriga is most prominent in the northern Hemisphere winter sky, along with the five other constellations that have ...
How did the Solar System form?
How did the Solar System form?

... •  Solar system formation begins because of gravity - most stuff ends up in the sun •  A disk is formed because of rotation •  Planet cores form in the disk because rocks hit and/or gravitationally attract each other •  If there’s ice around (> 5 AU from the star, where it’s cold) the cores are bigg ...
Chapter 2 The Copernican Revolution
Chapter 2 The Copernican Revolution

... © 2011 Pearson Education, Inc. ...
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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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