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Life in the Universe - abersychanastronomy
Life in the Universe - abersychanastronomy

... Nearly all of the original oxygen was released via photosynthesis from single-celled cyanobacteria some 3.5 billion years ago. For more than 1 billion years, this oxygen reacted with surface rocks and little stayed in the atmosphere. Eventually, some 2 billion years ago, the oxygen began to accumula ...
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... For the past 20 years, since the discovery of planets outside our solar system, we have been searching for Earth 2.0. In this talk we’ll explore what makes our own planet Earth such a haven for life and what this really means for the habitability of Earth 2.0. We’ll be talking about our solar syste ...
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... Characteristics of the Solar System support the solar nebula hypothesis The two types of planets can be understood with the condensation sequence caused by different conditions in the inner and the outer parts of the nebula The Solar System is different from the other planetary systems found so far: ...
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... Nucleus: The nucleus is the frozen center of a comet’s head. It is composed of ice, gas, and dust. Coma: The coma is a blob of gas that surrounds the nucleus of a comet; The coma is composed of water vapor, carbon dioxide gas, ammonia, and dust. Gas Tail: A tail of charged gases (ions) always faces ...
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... #10: Complete the following concept map by correctly adding the connecting phrases or terms provided to the appropriate locations. Some items may be used more than once; others may not be applicable to this diagram. ...
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... Nucleus: The nucleus is the frozen center of a comet’s head. It is composed of ice, gas, and dust. Coma: The coma is a blob of gas that surrounds the nucleus of a comet; The coma is composed of water vapor, carbon dioxide gas, ammonia, and dust. Gas Tail: A tail of charged gases (ions) always faces ...
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... The presence of the SiO gas, which can be formed by vaporizing rocks, and silica-rich glass have led to the collision interpretation. Although collisions seem to explain the current data, the probability of observing a collision is low. Current models of terrestrial planet formation give an approxim ...
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... just the right distance away to give us conditions that are suitable for life. All the other planets in the solar system are too hot or too cold. Astronomers believe that there are many stars that have solar systems, if not the majority. They cannot see the planets; they are too far away, but they c ...
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... characteristic rate, called its half-life, which can be measured in the laboratory • This is the key to a technique called radioactive age dating, which is used to determine the ages of rocks • The oldest rocks found anywhere in the solar system are meteorites, the bits of meteoroids that survive pa ...
Fulltext PDF
Fulltext PDF

... constituents are probably also present. ...
Search for Life in the Universe
Search for Life in the Universe

... • Terrestrial planets: – Migration of Jovian planets disrupts terrestrial planets in the habitable zone during the migration – Final elliptic orbits  long-term disruption ...
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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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