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Chapter 24
Chapter 24

BLynchTalk3
BLynchTalk3

... Effects of CMEs September 1, 1859 More Recent CME effects Very Recent CME & Solar Flare effects October 29, 2003 ...
PHE-15 (2007
PHE-15 (2007

... Explain the atomic origin of emission and absorption spectra. ...
Forcing
Forcing

... “Forcing” is produced by an external process, e.g. ...
Solar-cycle variation of low density solar wind during
Solar-cycle variation of low density solar wind during

... from the Sun, or from low density source plasma extending from density-depleted prominence cavities. The plasma inside ejecta at 1 AU is not always low density however. Intrinsically higher density plasma, for example including prominence material, may be encountered, and plasma compression may also ...
Sterilization & Disinfection
Sterilization & Disinfection

neuroaesthetics, neurological disorders and creativity
neuroaesthetics, neurological disorders and creativity

Sterilization and disinfection
Sterilization and disinfection

... Radiations damage DNA in several ways: UV light induces cross-linking between adjacent pyrimidines ...
Slide 1
Slide 1

The Cosmos, the Solar System and the Primeval Earth
The Cosmos, the Solar System and the Primeval Earth

... or coming together of two stars. As early as 1745, the French scientist Count Buffon postulated that the Earth had been torn out of the sun by a passing comet. He estimated the age of the Earth to be 70,000 years, while theology proclaimed that the Earth was less than 6,000 years old. It is generall ...
Systems of classification
Systems of classification

... The classification of living organisms has been controversial throughout time, and these schemes are among those in use today. Top: Aristotle’s system distinguished only between plants and animals on the basis of movement, feeding mechanism, and growth patterns. This system groups prokaryotes, algae ...
02B-2 - El Camino College
02B-2 - El Camino College

... Eventually, a star runs out of its fuel: it is no longer hot enough to smash and fuse smaller atoms together. At this point, the star begins to collapse (gravity pulls the atoms closer and closer together). In large stars, the inward falling material collides and rebounds (like a “superball”) outwar ...
Bioleaching of nickel from olivine using chemoheterotrophic fungi
Bioleaching of nickel from olivine using chemoheterotrophic fungi

... beyond conventional sources. The importance of low-grade ores and waste residues as a source for raw materials is expected to increase in the near future. In particular, the escalating depletion of highgrade sulphidic ores make it necessary to obtain metals from the more abundant but lower grade sil ...
Introduction Strategies
Introduction Strategies

... Constellations are found within galaxies, which are huge groups of stars, dust, and gas. There are many galaxies in the Universe. Stars are groups of gasses that emit heat and light; but stars aren’t the only things that shine in the sky. Meteors, comets, meteorites, and asteroids also move through ...
Other Solar System Bodies
Other Solar System Bodies

... formed during meteor impacts in the past. These have recently been shown to form minimagnetospheres, which cause a small deflection in the solar wind near the surface. Note also that the moon spends part of its orbit inside the terrestrial magnetosphere, such that its interaction at these times is w ...
Lecture 21-Hot Big Bang
Lecture 21-Hot Big Bang

... the cosmic background radiation changed to microwave Wavelength and its temperature dropped to about 3K. ...
From meteorites to evolution and habitability of planets
From meteorites to evolution and habitability of planets

Lecture 9
Lecture 9

... In principle, you can find the age of a rock by measuring the ratio of potassium-40 to argon-40. 100 atoms of potassium-40, 11 atoms of argon-40: age equals 1.3 billion years. Higher potassium/argon ratio: younger. Lower potassium/argon ratio: older. In practice, it is more subtle: Argon is an inert ...
Poster - unist
Poster - unist

Where can we find bacteria?
Where can we find bacteria?

The Transport of Cosmic Rays
The Transport of Cosmic Rays

Lecture23-ASTA01 - University of Toronto
Lecture23-ASTA01 - University of Toronto

10.1
10.1

... compressed. They are shifted more toward the violet end of the spectrum. If the star is moving away from you, there is a red shift, which means its wavelengths get longer. They are stretched out and shifted toward the red end of the spectrum. This red-shifting of wavelengths has been observed with m ...
earth`s atmosphere sky watChÍng
earth`s atmosphere sky watChÍng

The Sun - SAASTA
The Sun - SAASTA

... nearly 150 million kilometres away. It is gigantic compared to the Earth. If you think of the Sun as a football, Earth would be the size of the head of a match. The Sun measures as much across as 109 Earths side by side and it could hold more than a million Earths inside its volume. Only because the ...
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EXPOSE



EXPOSE is a multi-user facility mounted outside the International Space Station dedicated to astrobiology. EXPOSE was developed by the European Space Agency (ESA) for long-term spaceflights and was designed to allow exposure of chemical and biological samples to outer space while recording data during exposure.The results will contribute to our understanding of photobiological processes in simulated radiation climates of planets (e.g. early Earth, early and present Mars, and the role of the ozone layer in protecting the biosphere from harmful UV-B radiation), as well as studies of the probabilities and limitations for life to be distributed beyond its planet of origin. EXPOSE data support long-term in situ studies of microbes in artificial meteorites, as well as of microbial communities from special ecological niches. Some EXPOSE experiments investigated to what extent particular terrestrial organisms are able to cope with extraterrestrial environmental conditions. Others tested how organic molecules react when subjected for a prolonged period of time to unfiltered solar light.
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