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File - We All Love Science
File - We All Love Science

... • Do now: Describe our Solar System by listing basic details: shape, structure of planets, relationship to the Sun, age. ...
1 UNIT 3 EARTH HISTORY - POSSIBLE TEST QUESTIONS OUR
1 UNIT 3 EARTH HISTORY - POSSIBLE TEST QUESTIONS OUR

... 2. What is the approximate age of the Universe? 3. Where is the center of our universe? Evidence for the Big Bang 4. What do we generally mean by the term “cosmic”? 5. Which is the most abundant element in the Universe (cosmic abundances of the original three)? 6. What does a cosmologic red shift im ...
Our Solar System
Our Solar System

... There are stream drainage patterns found on the planet from running water at some point long ago. ...
The Next Step: Exponential Life 1 — PB
The Next Step: Exponential Life 1 — PB

... that lies ahead—the post-human future where our remote descendants may transcend human limitations—here on Earth but (more probably) far beyond. This is my theme in the present chapter. The stupendous timespans of the evolutionary past are now part of common culture. But the even longer time-horizon ...
solar system form
solar system form

... Hydrogen, helium, and traces of lithium, the three lightest elements, were formed shortly after the creation of the universe. The heavier elements were produced much later by stars and are cast into space when stars die. By mass, 98% of the observed matter in the universe is hydrogen and helium. The ...
Astronomy Powerpoint
Astronomy Powerpoint

... • The future of the universe follows two possible paths: 1. The universe will expand forever. 2. The outward expansion will stop and gravitational contraction will follow. • The view currently favored by most scientists is an expanding universe with no ending point. • It should be noted, however, th ...
Solar System
Solar System

... • 1 AU = 150,000,000 kilometers away (Distance between Earth and Sun) • If distances are even farther, then astronomers use lightyears. A light-year is the distance light travels in one year. • Light travels at 300,000 km/sec • 1 light-year = 10 trillion km • The next closest star (Alpha Centauri) i ...
`Super Earths` Will Have Plate Tectonics, Scientists Predict
`Super Earths` Will Have Plate Tectonics, Scientists Predict

... Plate tectonics, the movement of the giant plates that make up Earth's solid outer shell, are responsible for earthquakes, volcanoes, and other major geological events. In essence, they have dominated Earth's geological history. Earth is the only known planet that has plate tectonics, and this “Our ...
PDF Version - OMICS International
PDF Version - OMICS International

... COMETS: are frozen balls of ice and dust that can resemble a “dirty snowball”.They orbit the Sun is highly elliptical orbits. Their orbital periods can range from a few years to several thousand years. Halleys Comet is famous due to the fact that everyone has a chance to see it in their lifetime (O ...
Star Dust By the Rev. Tom Garrison
Star Dust By the Rev. Tom Garrison

... Four to six pounds. 4-6 pounds of ash is all that is left of us when we die and are cremated. As it says in the burial service of the Book of Common Prayer: “Ashes to ashes. Dust to dust.” i Scientists tell us that approximately 40,000 tons of cosmic dust fall on earth every year from outer space.ii ...
Earth`s Motion and Seasons
Earth`s Motion and Seasons

... Flattened area containing the spiral arms that are pinwheeled shaped Contains lots of gas and dust with younger stars Our solar system is located on the Orion Arm 25,000 light-years away from the central bulge Open Clusters: vast cloud of dust & gas that forms a loose grouping of stars ...
The ISM
The ISM

... Dust obscuring Ha emission nebula ...
File
File

... 3. High (geosynchronous) orbit satellites are used for ____________ while low orbit satellites move over different regions and are used for _____________. A. B. C. D. ...
The Universe and Space Travel
The Universe and Space Travel

... spaceflights that will essentially transport people to Mars by 2025. He said he plans to travel to the International Space Station (ISS) on board one of his own SpaceX aircraft by 2020. The firm will also be focusing on exploring space travel to and beyond Mars and might make its plans public ...
ppt
ppt

... share the following common traits: ...
Slide 1
Slide 1

... gravitational collapse of a cloud (nebula) of dust and gas • As the nebula collapses, it forms a spinning disk (due to conservation of angular momentum) • The collapse releases gravitational energy, which heats the centre; this central hot portion forms a star • The outer, cooler particles suffer re ...
Planetary Diversity - MIT Computer Science and Artificial
Planetary Diversity - MIT Computer Science and Artificial

... ; (seefigure 2). Gas refers primarily to hydrogen and helium, the most abundant elements in the universe. stars by a gravitational instability ofthe gas disk, provided These elements also happen to comprise molecules that do it is sufficiently cold and dense. No one knows whether not condense as sol ...
The Origin of the Solar System
The Origin of the Solar System

... grow by direct gas accretion without forming rocky ...
Homework October 24-28
Homework October 24-28

... 2. Which observed feature of the universe, discovered by Edward Hubble, is A) entropy B) expansion C) radiation D) redshift 3. Based on data collected from many different sources, such as the Hubble telescope and The Wilkinson Microwave Anisotropy Probe (WMAP), scientists have been able to show that ...
Take Home #1 Complete the following on your own paper. Do not
Take Home #1 Complete the following on your own paper. Do not

... 15) A prediction made in the Big Bang Theory is that the entire universe should be filled with left-over radiation. This radiation, referred to as Cosmic Microwave Background Radiation, was measured by the 1989 Cosmic Background Explorer (COBE) satellite. The success of this satellite prompted the d ...
Take Home #1 Complete the following on your own paper. Do not
Take Home #1 Complete the following on your own paper. Do not

... 15) A prediction made in the Big Bang Theory is that the entire universe should be filled with left-over radiation. This radiation, referred to as Cosmic Microwave Background Radiation, was measured by the 1989 Cosmic Background Explorer (COBE) satellite. The success of this satellite prompted the d ...
Introduction to the Universe
Introduction to the Universe

... 1 light sec = ________________________________ = _________ = _____________. Almost to ________ 1 light year = _______________________________ TRIVIA: 1 light year = ____________________. Nearest star to Sun = _______________ away. The Sun, all 8 planets are about _________ old. – How many years is t ...
SOFIA Science - Stratospheric Observatory for Infrared Astronomy
SOFIA Science - Stratospheric Observatory for Infrared Astronomy

... SOFIA can easily study: > IR: objects much cooler than normal stars like the Sun for example: stars and planets in the process of forming; > IR: objects embedded in, or behind, opaque ISM dust clouds; SOFIA’s instruments can see into and through those clouds > IR: organic molecules in space, which h ...
The Origin of the Solar System
The Origin of the Solar System

... The impact would vaporize low-melting-point materials (e.g., water) and disperse them explaining their lack in the Moon Only surface rock blasted out of Earth leaving Earth’s core intact and little iron in the Moon Easily explains composition similarities and differences with Earth The splashed- ...
Formation of Stars
Formation of Stars

... gravity and stop the compression. ...
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Panspermia



Panspermia (from Greek πᾶν (pan), meaning ""all"", and σπέρμα (sperma), meaning ""seed"") is the hypothesis that life exists throughout the Universe, distributed by meteoroids, asteroids, comets, planetoids and, also, by spacecraft in the form of unintended contamination by microorganisms.Panspermia is a hypothesis proposing that microscopic life forms that can survive the effects of space, such as extremophiles, become trapped in debris that is ejected into space after collisions between planets and small Solar System bodies that harbor life. Some organisms may travel dormant for an extended amount of time before colliding randomly with other planets or intermingling with protoplanetary disks. If met with ideal conditions on a new planet's surfaces, the organisms become active and the process of evolution begins. Panspermia is not meant to address how life began, just the method that may cause its distribution in the Universe.Pseudo-panspermia (sometimes called ""soft panspermia"" or ""molecular panspermia"") argues that the pre-biotic organic building blocks of life originated in space and were incorporated in the solar nebula from which the planets condensed and were further —and continuously— distributed to planetary surfaces where life then emerged (abiogenesis). From the early 1970s it was becoming evident that interstellar dust consisted of a large component of organic molecules. Interstellar molecules are formed by chemical reactions within very sparse interstellar or circumstellar clouds of dust and gas. The dust plays a critical role of shielding the molecules from the ionizing effect of ultraviolet radiation emitted by stars.Several simulations in laboratories and in low Earth orbit suggest that ejection, entry and impact is survivable for some simple organisms.
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