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... Gravity will pull galaxies together. ...
Content Clarification for Modeling the Universe: Earth and Space
Content Clarification for Modeling the Universe: Earth and Space

... history of the universe before stars formed. • Mathematical models and computer simulations are used in studying evidence from many sources in order to form a scientific account of the universe. ...
Public Lecture - Size of the Universe
Public Lecture - Size of the Universe

... Calculating Grains of Sand • One grain of dry sand measures approximately 0.5 mm – 20 mm of side-by-side sand would create 1 centimeter (< 0.5 in) ...
Search for Life in the Universe – What can we Learn from our own
Search for Life in the Universe – What can we Learn from our own

... decades are witnesses of these processes. The question arises, whether such rock or soil ejecta could also be the vehicle for life to leave its planet of origin, or, in other words, whether spreading of life in the solar system via natural transfer of viable microbes is a feasible process. Simulatio ...
Volume 2 (Issue 7), July 2013
Volume 2 (Issue 7), July 2013

... galaxies. Since we know very little about the evolutionary process of galaxies, it is possible that quasars, as old as they are, represent a very early stage in the formation of galaxies. The energy we see may be ejected from the cores of these very young and very active galaxies. Some scientists ev ...
Life in the Universe
Life in the Universe

... and survival of life as we know it. The GHZ was first proposed in 1991 by Guillermo Gonzalez of Iowa State University and Donald Brownlee and Peter Ward of Washington University, and has subsequently been endorsed by a number of other researchers, including Charles Lineweaver. Outside the galactic h ...
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

... ●   The sun’s structure consists of the corona, photosphere, chromosphere, transition zone, convection zone, radiation zone and the core, each with their own properties and characteristics. ●   Nuclear fusion occurs within the sun in which a reaction converts hydrogen into helium and releases energy ...
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

... ● The sun’s structure consists of the corona, photosphere, chromosphere, transition zone, convection zone, radiation zone and the core, each with their own properties and characteristics. ● Nuclear fusion occurs within the sun in which a reaction converts hydrogen into helium and releases energy, wh ...
Chpt4b
Chpt4b

... There are two basic types of meteoroids: random, shower The random kind which can be observed on any clear night (few per hour) are probably left over interplanetary debris. ...
Feb 2 Student Use
Feb 2 Student Use

... as best as you can, 2. then see what other groups you can link together to form recognizable shapes. (use your imagination and be creative) ...
origins of the Universe
origins of the Universe

... begin to contract and close in on itself eventually exploding again and starting the process all over again. ...
Slide 1
Slide 1

... (750°F), possible because of the large pressure Black smokers: mixed with volcanic chemicals ...
Meteors, Meteoroids, and Meteorites
Meteors, Meteoroids, and Meteorites

... Meteorites reach the Earth's surface because they are the right size to travel through the atmosphere. If they are too small, they will burn up in the atmosphere. If they are too large, they may explode before reaching the Earth's surface. One such meteorite exploded in Siberia in 1908. It left a 20 ...
CST Prep- 8th Grade Astronomy
CST Prep- 8th Grade Astronomy

... 62. When these bits enter our atmosphere they burn up as __________________ (also known as “shooting stars”). 63. Bits of outer space material that strike the Earth’s surface and can be found intact are now called __________________. 64. The “hole” left in the ground from an asteroid impact is calle ...
Why SETI will Fail
Why SETI will Fail

... origin of galaxies, stars, elements, planets => origin of life => chemical and biological evolution => technological intelligence ...
Witnesses to Local Cosmic History - Max-Planck
Witnesses to Local Cosmic History - Max-Planck

... far back as 1984, Wing Ip and a colleague, who were then working at the Max Planck Institute for Solar System Research, discovered that the large planets with their immense gravity must have hurled the small bits and pieces to and fro in the solar system. But even the planets themselves did not rema ...
Section 11: GRAPHIC STIMULUS
Section 11: GRAPHIC STIMULUS

... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
K-‐8 Earth and Space TEKS Cards
K-‐8 Earth and Space TEKS Cards

... Earth and space. The student knows there are recognizable patterns in the natural world and among objects in the sky. The student is expected to: (A) observe, measure, record, and compare day-to-day weather changes in different locations at the same time that include air temperature, wind direction, ...
Section 11: GRAPHIC STIMULUS
Section 11: GRAPHIC STIMULUS

... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
How mighty Jupiter could have changed Earth`s habitability
How mighty Jupiter could have changed Earth`s habitability

... how the Earth's orbit behaves over time." less likely to have planets with stable axes, which The model showed that most of Jupiter's locations makes them less likely to be habitable." resulted in little change in Earth's orbit and tilt, That said, he warns there are no "absolute rules" although the ...
2-IYA HighLights2009
2-IYA HighLights2009

... equipped with the latest instruments. In 2009, Servicing Mission 4 will overhaul Hubble, kitting it out with new gadgets and extending its life by at least five years. On the web: http://www.spacetelescope.org/about/history/servicing_mission_4.html ...
Survey of the Solar System - USU Department of Physics
Survey of the Solar System - USU Department of Physics

... This can be translated into a velocity of the star, which then tells us that the star is rotating around it’s system’s center-of-mass ...
is there life out there? - Bentonville Public Library
is there life out there? - Bentonville Public Library

... IO's surface is also dotted with more than 100 mountains that have been uplifted by extensive compression at the base of IO's silicate crust. Some of these peaks are taller than Mount Everest ...
Unit 3: Understanding the Universe
Unit 3: Understanding the Universe

... Science Science 8 January 6 weeks Published ...
Unit 5
Unit 5

... explain how stars can be different Be selective in choosing content from the textbook resource ...
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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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