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Opakování z minulého cvičení
Opakování z minulého cvičení

... renewed by 'new' comets picked up by the Solar System when it passes through giant molecular clouds. The Oort cloud may contain 100 billion comets. From time to time, the gravitational influence of a passing star will disturb the Oort cloud and send comets in towards the Sun, where the gravitational ...
Teacher Guide Lives of Stars
Teacher Guide Lives of Stars

Meet the Planets - Arbordale Publishing
Meet the Planets - Arbordale Publishing

... over two cards so that everyone can see. If the cards match, he or she keeps the pair and takes another turn. If they do not match, the player should turn the cards back over and it is another player’s turn. The player with the most pairs at the end of the game wins. Who Am I? Copy and cut out the c ...
Astronomy - Core Knowledge Foundation
Astronomy - Core Knowledge Foundation

... ● Explain that the sun is a source of energy, light, and heat  ● Classify the sun as a star  ● Identify Earth as a planet and our home  ● Identify the earth’s rotation, or spin, as the cause of day and night  ● Explain that other parts of the world experience nighttime while we have daytime  ● Expla ...
Einstein
Einstein

... the speed of light around magnetic fields. • Emission (mostly radio) is concentrated at the magnetic poles and focused into a beam. • Whether we see a pulsar depends on the geometry. – if the polar beam sweeps by Earth’s direction once each rotation, the neutron star appears to be a pulsar – if the ...
Activities, In the Footsteps of Galileo
Activities, In the Footsteps of Galileo

CH6.5.Ast1001.F13.EDS
CH6.5.Ast1001.F13.EDS

The Sun: Source of heat and light
The Sun: Source of heat and light

Search for Other Worlds - Science fiction 20 years
Search for Other Worlds - Science fiction 20 years

... of detecting of a very small mass. In 1992 Wolszczan and Frail used this method to discover the first exoplanet around the pulsar PSR 1257+12 (Wolszczan 1992). Unfortunately pulsars are pretty rare, so this method is not going produce a large number of exoplanet discoveries. Also, life it’s unlikely ...
The Resounding Universe
The Resounding Universe

... disciplines. Sight and hearing are complementary senses: eyes are made for looking at celestial bodies and ears to follow their harmonious motions. Aristotle (c. 384 BC – c. 322 BC) explains why mortals cannot hear these sounds. In fact, a sound or a noise can be perceived only when in contrast with ...
Lecture #33: Solar System Origin I The Main Point What is a
Lecture #33: Solar System Origin I The Main Point What is a

Astronomical Coordinates, Distances and Magnitudes
Astronomical Coordinates, Distances and Magnitudes

... direction as, for instance, the corner of the room or the tower of the church. The abstraction of this natural SR is named the Spherical Polar System. The position of a point is given by three coordinates: two angles (φ,θ) and a distance (r) as shown in the figure. The geographical (geographical lat ...
Chapter-by-Chapter Guide
Chapter-by-Chapter Guide

... Ecliptic plane: The two-dimensional plane in which Earth orbits around the Sun. Most of the other planets orbit nearly in this same plane. Axis tilt: The amount that a planet’s rotation axis is tipped relative to a line perpendicular to the ecliptic plane. The Milky Way Galaxy is a spiral galaxy, wh ...
Properties of Stars Name
Properties of Stars Name

... against its absolute magnitude. From such a diagram, other information about a star’s properties and life cycle can be determined. In this lab, you will construct an H-R diagram using data on the 20 stars that are nearest to our sun (Figure 21.1) and the 20 stars that appear brightest in our sky (Fi ...
Galaxies, stars and planets
Galaxies, stars and planets

... and contains materials with a range of properties that far exceeds anything that can be replicated in laboratories on the Earth. Temperatures range from close to absolute zero (−273.15 ºC) in dense clouds of gas and dust from which stars form, up to many millions of degrees in the interiors of stars ...
October 2011
October 2011

... The Sculptor Galaxy was too far south for Messier, it was swept up in 1783 by Caroline Herschel in one of her comet sweeps. Its tilted oval glow stands out even in binoculars. It’s 10 million light years away but it’s a starburst spiral with a high rate of radiant star formation. Strong gamma and X- ...
doc - Steve Kluge
doc - Steve Kluge

the orbit of venus
the orbit of venus

... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth?___________________ ________________________ ...
Which Constellation is Which?
Which Constellation is Which?

... You probably know some constellations. The Big Dipper looks like a giant pot with a long handle. Orion is named after a great hunter. You can see his belt, marked by three bright stars. Constellations are imaginary pictures in the sky. The stars look like they are all the same distance away. That’s ...
There He Goes Again - GeocentrismDebunked.org
There He Goes Again - GeocentrismDebunked.org

Astronomical Chronicle  for September, 2008
Astronomical Chronicle for September, 2008

The quick brown fox jumps over the lazy dog
The quick brown fox jumps over the lazy dog

... that wheel about the sun, had become very erratic. Ogilvy had already called attention to a suspected retardation in its velocity in December. Such a piece of news was scarcely calculated to interest a world the greater portion of whose inhabitants were unaware of the existence of the planet Neptun ...
The Sun and the Stars
The Sun and the Stars

... Thus, if we know the Earth’s radius, we can measure the distance to the sun, by measuring the solar parallax ...
Lecture 3
Lecture 3

Astro110-01 Lecture 7 The Copernican Revolution
Astro110-01 Lecture 7 The Copernican Revolution

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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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