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Detection and Properties of Planetary Systems
Detection and Properties of Planetary Systems

DOCX
DOCX

... heavenly luminaries (sun, moon, and stars) rotate daily around Polaris. There is no "outer space". The centre of the earth plane is the north pole and the Rupes Nigra or Mount Meru; and outer edge is Antarctica and the ice wall. There is no south pole. The sun and moon are the same size, each about ...
Which exoEarths should we search for life
Which exoEarths should we search for life

Name: Notes – #45 The Diverse Sizes of Stars 1. A Hertzsprung
Name: Notes – #45 The Diverse Sizes of Stars 1. A Hertzsprung

... 6. Super giants tend to have surface temperatures cooler than the sun but emit 104 time or more energy than the Sun. Why is this true? 7. The size of the star Betelgeuse in the constellation Orion is approximately the same size as ____________’s orbit around the Sun. 8. What stars have the same temp ...
Skinner Chapter 2
Skinner Chapter 2

... 44. A supernova is the most likely source for the heavy elements present in the Sun and the rest of the solar system. [It is also possible that a supernova may have created the shock wave that initiated compression and collapse of the interstellar cloud of gas and dust, leading to the formation of t ...
The most accepted theory of the origin of the solar system is the
The most accepted theory of the origin of the solar system is the

... developing thick atmospheres, and with increasing depth and thus pressure, layers of liquid. However, since Uranus and Neptune reside in a region where apparently the solar nebula’s density was significantly less, the formation of their cores at their current distance from the Sun is highly implausi ...
Lecture7 - UCSB Physics
Lecture7 - UCSB Physics

... • The formation of terrestrial planets around a star is thought to have occurred by what process? •  A) Breakup of a large disk of matter which formed around the star •  B) Condensation of gas from the original star nebula •  C) Capture by the star of objects traversing the depths of space •  D) Acc ...
File
File

... material (mostly H and He) within a spiral arm of the milky way galaxy began to contract and flatten into a rotating disk Disk rotated and most of the mass concentrated in the center Surrounding the central disk, the turbulent rotating nebula of interstellar gases began to cool and condense, forming ...
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s*t*a*r chart - Ontario Science Centre
s*t*a*r chart - Ontario Science Centre

... past. This season's evening sky features Orion the Hunter. Connect three bright stars to form Orion’s belt. Betelgeuse, a red super-giant star, marks the left shoulder. Notice its reddish appearance in comparison with the ‘blue’ color of the belt stars. Betelgeuse is one of the largest and most lumi ...
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... 1. List four things included in the universe. 2. What force holds galaxies together? 3. List three different types of galaxies. Homework 4. What is the name of the galaxy in which we live? 5. In what type of galaxy do we live? The Sun Class Work 6. What type of celestial object is the sun? 7. When o ...
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THE STAR - physics.udel.edu
THE STAR - physics.udel.edu

... 1.6; it is currently approximately magnitude 2.2. Delta Cassiopeiae, also known as "Ruchbah" or "Rukbat," meaning "knee," is an Algol-type eclipsing variable star. It varies by 0.1 magnitudes around magnitude 2.7; its period is 2 years and 1 month. Ruchbah appears to have a blue-white hue and it is ...
Flat Earth FE / Scientists “don`t know” Anything about Creation
Flat Earth FE / Scientists “don`t know” Anything about Creation

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astronomy - Mr. Barnard

... ____5. The explosion of a massive star near the end of its life is known as a (1) nebula (3) nova (2) supernova (4) pulsar ____6. According to our present theories of stellar evolution, our sun will change next into (1) a white dwarf (3) a red giant (2) a black hole (4) a supernova ____7. When a sta ...
Chapter 6 The Archean Eon of Precambrian Time I. Introduction
Chapter 6 The Archean Eon of Precambrian Time I. Introduction

... graywackes, conglomerates, and by banded iron formations iii. entire sequence is often surrounded by granitic intrusive rocks b. granulite association: composed largely of gneisses derived from strongly heated and deformed tonalites, granodiorites, and granites, as well as layered intrusive gabbroic ...
How was the Solar System Formed?
How was the Solar System Formed?

... Planets of the Solar System Standards: 1b Students know the evidence from Earth and Moon rocks indicates that the Solar System was formed from a Nebula cloud of dust and gas approximately 4.6 billion years ago (bya). 1c Students know the evidence from geological studies of Earth and other planets su ...
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14 The Planets

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Slide 1 - Fort Bend ISD
Slide 1 - Fort Bend ISD

... standard distance from the Earth • Scientists study globular clusters to compare brightness of stars • All about same distance from Earth ...
Origin and Nature of Planetary Systems
Origin and Nature of Planetary Systems

... Introduction: While there is only one Solar System (the system of the star Sol), as of early April 2015, there are 1207 known extrasolar planetary systems with 1911 known planets (called extrasolar planets or exoplanets). Of these planetary systems 480 have two or more planets. In this activity, we ...
Name ______KEY Date Core ______ Study Guide Galaxies and the
Name ______KEY Date Core ______ Study Guide Galaxies and the

... Galaxy: a huge group of stars, gas and dust held together by gravity Quasar: a very bright center of a galaxy. Shortened for quasi-stellar “seeming like a star” ...
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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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