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First life in primordial-planet oceans: the
First life in primordial-planet oceans: the

... matter, and that possibly life began spontaneously on this planet in several ways since life has existed from its beginning 4.6 Gyr ago. However, all laboratory attempts to create life have consistently failed and all serious attempts to model probabilities suggest they will always fail. Life chemis ...
Advanced Environmental Biotechnology
Advanced Environmental Biotechnology

bacteria - MHS Biology Mrs. Gates
bacteria - MHS Biology Mrs. Gates

... 3. These protists are very important to the Earth because they produce a lot of oxygen. ...
O - Portland State University
O - Portland State University

... Kelly Scientific Resources has an opening for an Extractions Technician at an environmental company in Tigard, OR.   This position has the potential to become a temp to hire opportunity.  The successful candidate will perform sample preparation duties including solvent extractions, solid phase extra ...
Metabolic-pathway– directed targeted metabolomics
Metabolic-pathway– directed targeted metabolomics

... full-scan high-resolution LC-MS data set used for an initial non-targeted metabolomics workflow in a pathway-driven targeted fashion. • Using a target compound identified by a non-targeted strategy (trigonelline, N-methyl-nicotinic acid) the subsequent hypothesis-driven targeted ...
The Mariner Jupiter/Saturn 1977 Mission
The Mariner Jupiter/Saturn 1977 Mission

... The deep atmospheres of Jupiter and Saturn, which must consist mostly of hydrogen and helium, are rendered opaque by high cloud decks, apparently very complex in structure. Permanent banding and ephemeral disturbances or storms have been charted from Earth at low resolution, and Jupiter's longlived ...
The maximal runaway temperature of Earth-like planets
The maximal runaway temperature of Earth-like planets

... water vapor leading to a runaway. Komabayashi solved the problem by adopting the Eddington approximation in the gray approximation, and found a solution in which the water vapor did not prevent temperature divergence. Ingersoll (1969) discussed the possible runaway on Venus and considered only the I ...
Science: Single Award Unit 3 (Physics) Higher Tier
Science: Single Award Unit 3 (Physics) Higher Tier

... Use the information from both tables to answer the following questions. (ii) Name the telescope which could be used to observe very hot stars. ________________________________________________________ [1] (iii) Which source will be detected using the XMM Newton telescope? ______________ ...
The role of the sun in climate forcing
The role of the sun in climate forcing

... solar variability coluld be much larger. The analysis of cosmogenic nuclides stored in natural archives provides a means to extend our knowledge of solar variability over much longer time periods. The response of the climate system to solar forcing depends not only on the amount of radiation, but al ...
An Investigation of the Sterilization Effect of 385nm UVA-LED
An Investigation of the Sterilization Effect of 385nm UVA-LED

Read the report
Read the report

Masers (Microwave Amplification by Stimulated Electromagnetic
Masers (Microwave Amplification by Stimulated Electromagnetic

Absolute Motion and Quantum Gravity - Philsci
Absolute Motion and Quantum Gravity - Philsci

Latitudinal and radial gradients of galactic cosmic ray protons in the
Latitudinal and radial gradients of galactic cosmic ray protons in the

... distance. Three different phases in the trajectory have been marked by different colors: Red indicates the fast latitude scan, and green and blue the slow ascent and descent in the southern and northern hemisphere, respectively. The Earth is located between 0.98 and 1.02 AU and between −7◦ and 7◦ wi ...
highen_13_gravwaves - Mullard Space Science Laboratory
highen_13_gravwaves - Mullard Space Science Laboratory

EUROPEAN ACADEMIC RESEARCH, VOL
EUROPEAN ACADEMIC RESEARCH, VOL

Spontaneous Generation
Spontaneous Generation

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doc 1.5MB

Mars geodesy, rotation and gravity
Mars geodesy, rotation and gravity

... as the Mars Science Laboratory (MSL) in 2011, Phobos Grunt and Yinghuo-1 in 2011, or MAVEN (Mars Atmosphere and Volatile Evolution Mission) in 2013, and ExoMars (2016–2018), will further complement our knowledge of Mars. In addition to providing information on the geology of Mars (Rossi & van Gassel ...
MCB2010L Lab review Topics
MCB2010L Lab review Topics

... the growth curve, Spectrophotometer, O.D. and Transmission in Spectrophotometer. What is antibiotics? What is antiseptics? What is the zone of inhibition? How is it measured? What is being measured? Why is there such a zone, factors affecting the performance of the test. How is bacterial susceptibil ...
VSC - Science
VSC - Science

100 Pectin is a complex polysaccharide consisting mainly of
100 Pectin is a complex polysaccharide consisting mainly of

No Slide Title
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protostellar disks under the influence of winds and uv radiation
protostellar disks under the influence of winds and uv radiation

... Star formation and the creation of protostellar disks generally occur in a crowded environment. Nearby young stars and protostars can influence the disks of their closest neighbors by a combination of outflows and hard radiation. The central stars themselves can have a stellar wind and may produce s ...
The depth of maximum shower development and its fluctuations
The depth of maximum shower development and its fluctuations

... wit an energy above 1017 eV. These data were obtained using all four methods and reflect an alteration of xmax towards lower atmosphere depths with increasing energy. Figure 4 shows xmax values averaged over energy intervals together with the data from other experiments. Numerical values for Yakutsk ...
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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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