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Astronomy Terms
Astronomy Terms

... explosion of concentrated matter and energy and has been expanding ever since Copernicus = Polish astronomer who first stated the theory that Earth and other planets revolve around the sun Light-year = the distance that light travels in one year Gravity = force of attraction between objects Orbits = ...
How many moons does Mercury have? (Update)
How many moons does Mercury have? (Update)

... Mercury's Size and Orbit: Given Mercury's small size (the smallest planet in the ) and its proximity to the sun, it's gravity is too weak (and it's Hill sphere too small) to retain a natural satellite. Basically, if a large object were to approach Mercury today, to the point that it actually entered ...
CHAPTER 2 - THE RISE OF ASTRONOMY
CHAPTER 2 - THE RISE OF ASTRONOMY

ppt
ppt

... Very few small planets found Remember, Earth’s mass is 318 times less than Jupiters; (Mj) ...
On a New Primary Planet of our Solar System, Long Suspected
On a New Primary Planet of our Solar System, Long Suspected

... between color shades of red and green, as e.g. Mars, and the double star in Andromeda, who’s light decreases and increases, and even competely disappears before our eagle eyes. Kant and Wünsch, in their cosmological papers, hold that this planet does not exist for them, but was incorporated into Jup ...
Observational Constraints The Nebular Hypothesis
Observational Constraints The Nebular Hypothesis

Lecture11 - UCSB Physics
Lecture11 - UCSB Physics

... • C) The gas in the nebular disk would have to be clumpy rather than smooth • D) The gas in the nebular disk would have to be mostly methane and ammonia rather than hydrogen and helium ...
MS Science - Kawameeh Middle School
MS Science - Kawameeh Middle School

Week 9
Week 9

Lecture11 - UCSB Physics
Lecture11 - UCSB Physics

... •C) The gas in the nebular disk would have to be clumpy rather than smooth •D) The gas in the nebular disk would have to be mostly methane and ammonia rather than hydrogen and helium ...
UNIT VIII/B: THE EARTH IN SPACE – STARS AND GALAXIES
UNIT VIII/B: THE EARTH IN SPACE – STARS AND GALAXIES

... d. Light from distant galaxies outside our Local Group is "red-shifted," indicating that they are moving away from us (and from each other). e. Actually, it is the space that is expanding, carrying the galaxies along with it! This phenomenon is called the "expansion of the universe." f. Spectral lin ...
Specific Word Instruction Possible Sentences
Specific Word Instruction Possible Sentences

... stronomy is the study of the planets, stars, and galaxies. People have been watching the movement of the sun, moon, planets, and stars since ancient times. So astronomy is a very, very old science. From early times, people tried to make models of the universe. For many years, no one wanted to believ ...
STAAR Science Vocabulary 2016
STAAR Science Vocabulary 2016

... Nebula—cloud of gas and dust in space; location of star formation Supernova—the death of a large star by explosion Electromagnetic Spectrum—grouping of electromagnetic radiation from radio waves to gamma rays; all can travel through space; do not need a medium to travel Light Year—unit of length; di ...
Document
Document

... Lynne has drawn a model of the lunar cycle. She tells her friend that it is complete except for the labels, which she will put on a key to the side. Lynne’s friend says that even with the key and labels, the model is not fully complete. Look at the picture provided of Lynne’s model. ...
Chapter 13 Exploring the final frontier
Chapter 13 Exploring the final frontier

... of interaction infinite. How are these same concepts viewed in the theory of relativity? 12. In one paragraph, describe what is meant by the ‘relativity of simultaneity’. 13. In terms of the energy required, accelerating a spacecraft to light speed is an impossibility. Explain why this is so. ...
Scales This is a 16 meter by 16 meter scene. A meter is close in size
Scales This is a 16 meter by 16 meter scene. A meter is close in size

... Next we zoom out and see a scene that is 1 mile square, and you start seeing a city. At 100 miles on a side, you see a landscape. It seems pretty big. You probably wouldn’t want to walk it. We can back up still further and see the diameter of Earth, 12, 756 km across. Which is big, until you compare ...
Naked-eye astronomy
Naked-eye astronomy

10_origin_life
10_origin_life

... effect to raise temp. above 0 C. Mars has since lost most of its atmosphere for unknown reasons, perhaps absorption in rocks. ...
~Crowfoot
~Crowfoot

Chapter 18 Notes - Valdosta State University
Chapter 18 Notes - Valdosta State University

... at the center. That would explain the high velocities of stars orbiting near the center, the tremendous energy generated by the core and the shape of most galaxies. The most distant objects detected in the universe are called quasars (quasi-stellar radio sources). The closest known quasar is 600 mil ...
powerpoint - Physics @ IUPUI
powerpoint - Physics @ IUPUI

... did not get along with) to find a model which based on the observations would make sense in order so “that it may not appear I have lived in vain.” ...
Document
Document

... A brown dwarf is a substellar object below the sustained hydrogenburning limit of about 7.5% to 8.0% solar masses, and forms in a manner similar to stars by fragmentation of collapsing gas clouds. An extra-solar giant planet is a giant planet like Jupiter in orbit around a star other than the sun, a ...
Extrasolar Planets - University of Maryland Astronomy
Extrasolar Planets - University of Maryland Astronomy

... That kind of speed is still undetectable around ordinary stars. However, the Sun’s motion in response to Jupiter is a hefty 4.5 meters per second, and that is measurable (albeit with a lot of cleverness in the observational setup!). However, this detection method means that it is a lot easier to dis ...
Stars
Stars

... When we look up into the night sky, it is easy to imagine, as did the ancient Greeks, that all the stars are the same distance, stuck to some sort of Celestial Sphere that rotates through the heavens as the Earth stands still. This conclusion would be very wrong, however. It has taken astronomers th ...
From Earth to the Galaxies
From Earth to the Galaxies

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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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