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SAP_Paper1_FutureOfUniverse
SAP_Paper1_FutureOfUniverse

... effects are very visible as the moon’s rotation is the same length as its orbit, causing the same face to be directed toward us at all times. In 50 billion years, if the sun has not engulfed the Earth-Moon system it will become tide locked, with each body showing one face to the other (Murray, C.D. ...
Test 1 Overview - Physics and Astronomy
Test 1 Overview - Physics and Astronomy

... • Draw simple sketches to help visualize problems • Solve numerical problems in the margin • Come up with your answer first, then look for it in the choices • If you can’t find the answer, try process of elimination • If you don’t know the answer, Go on to the next problem and come back to this one ...
Chapter 6 Physics
Chapter 6 Physics

... 13. Calculate the gravitational potential energy of the Sun-Earth system. 14. Determine the escape speeds from (a) Mercury (b) Earth’s Moon 15. A neutron star results from the death of a star about 10 times as massive as the Sun. Composed of tightly packed neutrons, it is small and extremely dense. ...
Solar System Crossword - Super Teacher Worksheets
Solar System Crossword - Super Teacher Worksheets

... 13. number of planets in our solar system 14. Neil Armstrong was the first person to walk on the... ...
The Night Sky
The Night Sky

... mercury and Venus as inferior planets, i.e. their orbits are interior to that of the Earth. • Provides a relationship between distance from Sun and orbital period. Planets farther from the Sun took longer to complete an orbit. ...
Pluto
Pluto

... • Most comets are NOT periodic. They visit the Sun once then zoom away (or hit Sun) • They come from the Kuiper belt and the “Oort cloud” (a sphere of perhaps 1012 comets, about 50,000 AU from the Sun) • Sometimes perturbed by a passing star and deflected into the Solar System • Made of primitive ma ...
Chapter 13
Chapter 13

... 4. Two identical stars are in orbit about their center of mass. The orbital period is 141 days and they are each moving at 29.6 km/s. Determine each star’s mass. Ans. 6.04 x 10 30 kg 5. A synchronous satellite has an orbital period that is equal to the length of the planet’s day. If we wish to place ...
Astronomy 1140 Quiz 3 Review
Astronomy 1140 Quiz 3 Review

... 1. The Moon’s density is 3.34 g/cm3 , much smaller than the value for the Earth, Mercury, and Venus, which is about 5.2-5.5 g/cm3 . It is similar to Mars, however, which is 3.93 g/cm3 . 2. Implies that the Moon (and by extension Mars) must not have a large iron core like these planets, or else it w ...
Size of Sun and Size of Planets
Size of Sun and Size of Planets

... Name ________________________ ...
Introduction to Space
Introduction to Space

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Discs and Planets

planetary configurations - Fort Thomas Independent Schools
planetary configurations - Fort Thomas Independent Schools

... Earth has less mass, less inertia, same gravitational force; thus, more easily accelerated ...
PPT - Mr.E Science
PPT - Mr.E Science

... Nebula – a huge gas cloud made up mainly of Hydrogen that collapse down on itself and compresses the gas down into a Protostar Star is “born” when the protostar has contracting tight enough for Hydrogen to fuse into Helium, this releases the light and energy we normally associate with a “normal” sta ...
ESRT Worksheet
ESRT Worksheet

... 6. What type of boundary is the East Pacific Ridge? ___________________________________________ 7. What is the size range for a particle to be classified as silt? ____________________________________ 8. What type of rock contains platy mica crystals? _____________________________________________ 9. ...
Friends of the Planetarium Newsletter September
Friends of the Planetarium Newsletter September

... NASA's Pluto-bound New Horizons spacecraft has traversed the orbit of Neptune. This is its last major crossing en route to becoming the first probe to make a close encounter with distant Pluto on July 14, 2015. The sophisticated piano-sized spacecraft, which launched in January 2006, reached Neptun ...
PowerPoint file - High Point University
PowerPoint file - High Point University

... life on Earth in the past ...
PowerPoint Presentation - AST121 Introduction to Astronomy
PowerPoint Presentation - AST121 Introduction to Astronomy

... life on Earth in the past ...
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the Powerpoint

The Solar System
The Solar System

... with the tradition of Roman gods and is appropriate—Pluto was the god of the underworld, and the planet is a dark and frozen place—but it was chosen because the first two letters are Percival Lowell's initials. ...
Orbits of the planets - University of Iowa Astrophysics
Orbits of the planets - University of Iowa Astrophysics

... far from the Sun. • In Ptolemy’s model, Venus and the Sun must move together with the epicycle of Venus centered on a line between the Earth and the Sun • Then, Venus can never be the opposite side of the Sun from the Earth, so it can never have gibbous phases – no “full Venus”. ...
Linking Asteroids and Meteorites through Reflectance
Linking Asteroids and Meteorites through Reflectance

... • His observations of the alignment of Jupiter and Saturn occurred two days later than when predicted by Copernicus • Tycho came up with a model where the planets orbit the Sun but the Sun orbits Earth ...
PPT - UBC
PPT - UBC

...  (f) Hertzsprung-Russell Diagram, dwarf, giant and supergiant stars, white dwarfs, first clues to stellar evolution. Pre-reading Chapter 8. ...
Space is Big…
Space is Big…

... It is 275,000-575,000 times as luminous as the Sun. The mass of the star is unknown. The mass estimated from its orbital motion is about 100 solar masses. On the other hand, the mass estimated from its luminosity is about 25-40 solar masses. ...
The Sun and Moon powerpoint.
The Sun and Moon powerpoint.

... ranges. Formed from igneous rock. • The Maria are similar to our oceans, but were formed by past lava ...
Pale Blue Dot - Pacific Science Center
Pale Blue Dot - Pacific Science Center

... and more than 1,700 have been confirmed. Of these confirmed exoplanets 1 is of the proper mass in the proper orbit to be considered Earthlike. This may seem like a discouraging figure to those interested in finding life beyond Earth. However we have only been looking for exoplanets since 1995 and ou ...
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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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